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(b) s(.) c~((O, oo );c(x)). (c) For t > O, the range of S(t) is contained in T)(B). (d) For t > O, BS(k)(t) ¯ £(X); BS(~)(.) Cm((0, ec );£(X)). (e) For any fixed 0 (0 ~+~ - ~), there exists an analytic extension of Bt S(k)(.) to the sector [argz I _< 0. (f) sup~>ol[t~(~+")+kBtS(k)(t)l[e(X) (g) For Vo ¯ X, v(t) de__f S(t)Vo, t >_O, one has that v is a strict solution D~vt+Bv=O,
v(O)
=vo,
v,(O)=O,
t¯[O,T],
(21)
for any T > O, iff vo ¯ D(B) and Bvo ¯ D(B). (h) If v is a strict solution of (21), then v,vt,D~vt,Bv ¯ BC([0, oo);X). For the proof of Lemma3, see [3]. For the solutions of (11) we have the following regularity results. LEMMA 4 Let (i) and (ii) of Theorem 2 hold. Let Vo ~¯ D(B) and v(t_) ae=f S(t)vo. Then the following conclusions hold for each T > O: (a) iet 2/ ¯ (0, l+a], I’ ¢ 1. ThenBv(t_) ¯ C’~([O,T];X) iff Bvo ¯ D,( a-~-5, ). Moreover, in this case there is a constant M = M("/,c~, B), but independent of T, such that
[IBv(_t)[Ic. ([O,TI;X) MllBvollv.(,-~ ,oo).
(22)
242
Ch~ment et al. (b) Let 7 e (1 + a, 2). Then Bv(~_) C’~([O, T]; X)iff v(~_) = v( O)(iff .BVo (c) Let 7 e (0, 1]. Then my(t) C([0, T] ; X) O B([ 0, T]; D~(7~)) if f Bv (~) BVo e C([0, T]; X) ~ B([0, T]; DB(7, iff BVo e DB(7, ~). Moreover, in this case there is a constant M = M(7, a, B), but independent v~ T, such that I[Bv(!)ll~(t0,T];~.(~,~)) ~ MllBvo[].~<~,~). (23) (d) Let T ~ (0,1+~),7#1. Then Bv(t)_ ~ h*([O,T];X) iff Bvo ~ V~(~). ~ (e) Let 7 6 [1 + ~, 2). Then Bv(~) h~([0, T] ; X)iff v(~)= Vo (i ff Bvo = (f) Let 7 ~ (0,1). Then Sv(~) C([0, T] ;~s(7)) if f Bv (~) - Bvo ~ C([0, T];~,(7)) iff Zvo e V,(~).
Observe that in all cases of Lemma4, the hypotheses made and Lemma3 give that v(t) is a strict solution of D~vt + Bv = O, v(O) = Vo, vt(O) Except for some technicalities, the proof of Lemma4 parallels that of [1, Lemma12]. For the analysis of (12) and (15) we need the corresponding resolvent. We fory E X, 1 fr e’XtA-l+~(Al+(~I + B)-lydA’ t > 0, S~(t)y = ~ ,,o (24) $1 (0)y = where the integration path is as in (18). One then has the following result. LEMMA 5 Assume that (i) and (ii) of Theorem 2, and (19) hold. Define S~ by (24), and let k be a nonnegative integer. Then properties (a)-(e) of Lemma3 hold with S replaced by S~. Moreover, for I = O, 1,
sup~f(~+~)+a-~ B~S~) (t)lk(x) ~0
The .function w(t) ~f Sl
(t)Wl
i8
a
strict solution of
D~(w~ - u~) + Bw = iff
w(O) =
w~(O) = w~,
(25)
Wl ~
For the proof of Lemma5, see [3]. Concerningthe solutions w(t) of (25), we then have the following regularity state~nents. def
~ LEMMA 6 Let (i) and (ii) of Theorem Z hold, let ~~ ~ B(~) and w(t) S~(t)w~. Then the following statements hold for each T > ~ l ~+~ ~ ~). (a) Let 7 ~ (0,2), ~ ~ 1. Then Bw(t) Moreover, in this case there exists a constant M = M (% a, B), independent of T, such that
IIBwff)llc,([o,rl;x) < Mllmtllv.~,~+, ~,.
(26)
243
Regularityof Solutionsof FractionalEvolutionEquations Let 7 e (0,1]. Then Bw(t_) e C([O,T];X) nB([O,T];Z)B(%oo)) D(B~--~-a) and BrDawl E DB(7, oo). Moreover, in this case there is a stant M = M(3", ~, B), independent of T, such that IIBw(t_)lt~(t0,Tl;Z).(~;~)) <_ MllB~-~.wlllv.(.~,~).
(27)
(c) Let7 ~ (0,2), 7 ¢ 1. ). Then Bw(t_) e hT([O,T];X) ifJwl e DB2(~(--(iT~ if fwl e :D(Br~z) an (d) Let 7 ~ (0,1). Then Bw(t_) C([O,T];gs(7)) B’-~w~ ~ In all cases of Lemma6, the assumptions made and Lemma5 imply that w(t) is a strict solution of (25). For the proof of Lemma6, see [3].
3
METHOD OF SUMS
AND NONHOMOGENEOUS
RESULTS
To analyze
D~z~+ Bz = h, z~(0) = 40) = o,
(28)
with h ~ 0, we use the method of sums of Da Prato and Grisvard [4]. The following Lemma[1, Theorem8] reformulates [4, Theorem 3.11]. LEMMA 7 Assume that f( is a complex Banach space and that ft, ~ are resolvent commutingpositive operators in f( with spectral angles CAand ¢~, respectively, such that ¢,i + ¢~ < ~r. I]? is one of the spaces T)~i(7,p), T),~(3’), Dh(7,p) or Dh(7), where3’ e (0, 1] and p ~ [1, oc], and if y ~ ?, then there is a unique x such that fix + ~x = y. Moreover, fix and ~x e ~ and there exists a constant C
such thatIlfixll~÷II*)xll~
To apply this Lemma,we write 2 d__e¢ Co([O, TI;X) ae=f {u C([0, T] ;X)lu(0) = 0 } and define/) in 2 by
v([~)= Co([O, TI;V(B)),(,?u)(_t) = B~(t),u e Then/) is a positive operator in ~’~" with spectral angle ¢~) = CB. For the interpolation spaces of/) one has, 3’ ~ (0, 1],
Weconsider the fractional
derivative
as an operator ~+~ in 3~ by
Z)(fi~+~) = { u ~ 21u, ~ 2,g~_~ * u, ~ C~([O,T]i X),(DTu,)(O) = 0}, (2~+,u)(t) de___f D~ut(t), u ~ Z)(ft,+,),
a e (0,1).
The equation (28) can then be written fil+az +/)z = h. In addition, define fi~
244
Cli~ment et al.
and ,z]~ for a e (0, 1) 73(~i.a) dej { u efi [gl-~ *u e CI([O,T];X),(D~u)(O) 0},
Concerning the operators ~1+~, a ¯ [0, 1), one has LEMMA 8 (a) ¢il+a is a positive,
densely defined operator with spectral angle
~(1 + a) and~i1+~= (A~)~+~. (b) For ~/¯ (0, 1) and (1 + c~)~/¯ (0, onehas
v~,÷o(~, ~) = { f l Y¯ c(1+~)’([0, T]; X),y(0) For ~),z~i~_ ~ ~1 ¯ (0, 1) and (1 + c~)~/¯ (1, onehas (~, (X)) ~--* { f [ f ¯ C(1+°~)0([0, T]; X); f(O) = if(0) = (c) For ~? ¯ (0, 1) and (1 + c~)r/¯ (0, 1) U (1, onehas [~ hO+~)"([ 0, T]; X). ~)al+o (O) = ~D.z~1+ o (~’ (~)) The corresponding statements for ~, 0 < a < 1, were given in [1, Lemma11]. Proof of Lemma8. (a) By [1, Theorem 10(b) and Lemma11],
~1+c~
= ~v~l
-----
(.~)~ = (.~l)l+a. To see that ¢A1+o-< ~(l+a) one applies [10, Prop. 4]. that ¢~i~+o < {(1 + a). By [13, Proposition 2.3.2], and as .~1+~ = (.41) ~+~, one then has ¢~i~ < {. By this contradiction, CA~+.= {(1 (b) and (c) follow by [1, Theorem 10(c) and Lemma11] and by the Reiteration Theorem. [] A combination of Lemma7 and Lemma8 immediately implies (b) and (d) Of following Lemma and also (a), (c), if 7 ¯ (0, 1 + a), To prove (a), (c), if ~, ¯ [1 + a, 2), apply ~ to (28), with e ¯ (7 - 1 - a, use [1, Theorem10(c)], and thus reduce the problem to a case already known. LEMMA 9 Let (i) and (ii)
of Theorem 2 hold. Then the following is true:
(a) Let h ¯ C’¢([0, T];X) with 7 ¯ (0,2), 7 ~t 1. /f7 ¯ (0, 1), assume h(O) := If 7 ¯ (1,2), assume h(O) = h~(O) = O. Then there exists a unique strict solution z of (28) such that Bz(t_) CT([0, T] ;X). Moreover, in thi s cas e there exists a constant M = M(7, c~, B, T) such that
(b) Let h ¯ .(" ~I3([O,T];i~B(7,~x~)), 3’ ¯ (0, 1]. Then thereexists a unique strict solution z of (28) such that Bz(t) ¯ .~C~/3([0, T]; ~z(3’, co)). Moreover, in this case there is a constant M= M(7, a, B, T) such that IlBz(t)ll~([o,T];v,(.r,~))
Regularityof Solutionsof FractionalEvolutionEquations
245
(c) Let h ¯ hT([O,T];X) with 7 (0,2), 7 ~ 1. /f7 ¯ (0 ,1 assume h(O) = ff-~ ¯ (1, 2), assume h(O) = At(O) = O. Then there exists a unique solution z of (28) such that Bz(t_) ¯ h~r([O,T];X). (d) Let h ¯ Co([0, T];7:)~(7)), with 7 ¯ (0, 1). Then there exists a unique solution z of (28) such that Bz(t) ¯ Co([O,T];I)B(7)).
4
AN INTERPOLATION
LEMMA
For the analysis of necessary conditions for solutions of (1) to exhibit a specific behavior one needs the following version of earlier interpolation results [2, Lemma 3], [9, Prop. 2.2.12]. Below, CI (I, X) denotes Lipschitz-continuous functions defined on I with values in X and C2 1. denotes functions having the first derivative in C LEMMA 10 Let X and Y be Banach spaces that are continuously injected in a Hausdorff locally convex topological vector space. Let I be a closed, bounded interval and let f ¯ Cc~(I,X) N C$(I,Y), where &,~ (0 ,2]. Then f ¯ C(1-°)5+°~(I, (X, Y)o,~) for each (0, 1) and
fl c,,-o)~,+o~(z.(x,Y)o,~) 2(llfllc~(~;x) + 2allIa-asup~e~llf’(t)llx,i/&> l,~
246
Cb~ment et al.
Then, by (a) of Lemma6, Bw E {: 1+o-~. By the relation Bu = Bv + Bwone has Bv E ~; 1+~-~. Thus, by (a) of Lemma4, we arrive at BUoE "DR((I+~_.~)(I+~)
REFERENCES 1. 2.
3.
4. 5.
6. 7. 8. 9. 10. 11. 12. 13. 14.
Ph. Clement, G. Gripenberg and S-O. Londen, Schauder estimates for equations with fractional derivatives, Trans. A.M.S. (to appear). Ph. Clement, G. Gripenberg and S-O. Londen, H6Ider regularity for a linear fractional evolution equation. In Topics in Nonlinear Analysis, The Herbert AmannAnniversary Volume (1998), Birkh~iuser, Basel, 69-82. Ph. Clement, G. Gripenberg and S-O. Londen, Regularity results for some fractional evolution equations, Helsinki University of Technology, Institute of Mathematics, Research Report A 413 (1999). G. Da Prato and P. Grisvard, Sommesd’op~rateurs lindaires et dquations diffdrentielles opdrationnelles, J. Math. Pures Appl. 54 (1975), 305-387. G. Da Prato, M. Iannelli and E. Sinestrari, Regularity of solutions of a class of linear integrodifferential equations in Banachspaces, J. Integral Eqs. 8 (1985), 27-4O. G. Da Prato and E. Sinestrari, Differential operators with non dense domain, Ann. Scuola Norm. Sup. Pisa C1. Sci. (4) 14 (1987), 285-344. P. Grisvard, Commutativit~ de deux foncteurs d’interpolation et applications, J. Math. Pures Appl. 45 (1966), 143-206. P. Grisvard, t~quations diff~rentielles abstraites, Ann. Sci. l~cole Norm.Sup.(4) 2 (1969), 311-395. A. Lunardi, Analytic Semigroups and Optimal Regularity in Parabolic Problems, Birkh~user, Basel, 1995. S. Monniaux and J. Pr/iss, A theorem of the Dore-Venni type for noncommuting operators, Trans. A.M.S. 349 (1997), 4787-4814. J. Priiss, Evolutionary Integral Equations and Applications, Birkh~iuser, Basel, 1993. E. Sinestrari, On the abstract Cauchy problem of parabolic type in spaces of continuous functions, J. Math. Anal. Appl. 107 (1985), 16-66. H. Tanabe, Equations of Evolution, Pitman, London, 1979. H. Triebel, Interpolation Theory, Function Spaces, Differential Operators, North-Holland, Amsterdam, 1978.
Infinite Horizon Riccati in Nonreflexive Spaces
Operators
WOLFGANG DESCH and WILHELMSCHAPPACHERUniversitgt tut fiir Mathematik, Heinrichstrasse 36, A-8010 Graz, Austria
Graz,
Insti-
EVA FA~ANGOV~ and JAROSLAV MILOTA Department of Mathematical Analysis, Charles University, Sokolovska 83, 18675 Praha 8, Czech Republic
ABSTRACT For the least square control problem with an unbounded controller and a bounded observer we prove that the optimal control is of feedback type also for infinite time horizon and a non-reflexive state space. This feedback is given by a Riccati operator which is a unique positive and symmetric solution of the algebraic Riccati equation.
1
INTRODUCTION
We consider the infinite
horizon control problem
Minimize J(u; xo) = []Cx(s)] 2 ~- lu(s)121 ds.
Partially supported by Spezialforschungsbereich F 003 "Optimierung und Kontrolle" Karl-Franzens-Universitgt Graz, grant GAUK 19/1997, and Aktion ~sterreich-Tschechische blik".
247
(1.1) at the Repu-
248
Deschet al.
over all u E L2(0, oc; U), subject ~ = Ax + Bu , z(O) = xo
(1.2)
Here A is the generator of an exponentially stable Co-semigroupin a non-reflexive Banach space X, and B is a bounded linear operator from a Hilbert space U into the extrapolated Favard class F-1. C is a bounded linear operator from the state space X into a Hilbert space Y. Since the range of B is not contained in X, this is a problem of unbounded control. The theory of the least squares regulator with unboundedcontrol in Hilbert spaces is well developed, see e.g. [1], [2] and references therein. It turns out that the formalism of the Riccati equation can be adapted to unbounded control and observation. The value function of the optimal control problem is a quadratic form (Pxo,xo), where P is a bounded, positive definite symmetric linear operator on X. In many cases the optimal feedback is synthesized by a feedback law u*(t) -B*Px(t), but there are intricate situations whenthis expression is not well-defined and the optimal control is not givenby a bounded state feedback. Such problems are likely to occur if the range of the control operator B is relatively large, or if an unbounded input B is combined with an unbounded observation C. Roughly speaking, bounded state feedback is a matter of comparing the range of P with the domain of B*. Our intention is to carry over the Riccati formalism to the case of nonreflexivc Banach spaces with the smoothest kind of unbounded control, namely control taking values in the extrapolated Favard class. This is only a very restricted class of unbounded control (it would be bounded in any reflexive space), but it appears frequently in semigroup settings for delay equations, integrodifferential equations, and age dependent population dynamics ([3]-[7]). Notice that existence and uniquehess of the optimal control is clear by quadratic opti~nizatiou in the Hilbert space L~(0, oo, U). The nonreflexive state space enters the scene only when we consider the relation between the optimal solution x and the optimal feedback. The Riccati equation is originally a Hilbert spaceconcept, but it can be rewritten in terms of the duality between X and X*. In nonreflexive spaces this duality is loaded with technical difficulties since the adjoint semigroupis usually only strongly continuous on a closed subspace of X*, called X~. Nevertheless, in a recent paper [4] we have shownthat the finite horizon control problem 7’
Minimizeg(u; x0, T) =/o [ICx(s)()" + lu(s)12] ds.
(1.3)
admits a Riccati operator P(t) which takes values in Xa), so that B*P(t) is well defined and the optimal control is giveu by bounded state feedback. In this note we derive a similar result for the infinite horizon problem. We~ni~nic an approach well-knownfrom the Hilbert space theory: Given the Riccati operator for the finite horizon problem, we perform a limiting procedure for T ~ oo, which leads to the Riccati operator for infinite horizon and the algebraic Riccati equation. In the next section we give a short overviewover the technical tools required, i.e. the concept of the extrapolated Favard class, and the Riccati equation for the fi~ite horizon control problem. In the subsequent section we state and prove the existence and uniqueness of the Riccati operator for the infinite horizon problem.
Infinite HorizonRiccati Operatorsin NonreflexiveSpaces 2
249
PRELIMINARIES
Let X be a Banach space with norm I I. Let A be the infinitesimal generator of a semigroup S(t) on X and let its growth rate be negative, i.e. S(t) is exponentially stable. Let X-x be the completion of X with respect to the norm Ixl_l :: IA-lx[,x E X. The Banach space X_I is said to be the extrapolated space with respect to the generator A (or the semigroup S(t)), see e.g. [7],[8] and references given there. Evidently, A can be extended from X1 (the domain of with the graph norm) to A_x : D(A_I) = X -~ X_~. Then p(A) = p(A-1) and (A - A_~)-1 is the continuous extension of (A - A)-x. Moreover, the semigroup S(t) has also a continuous extension to the C0-semigroup S_l(t) on X_~ and the generator of S_l(t) is A-1. The growth rate of S_l(t) is the saIne as for S(t), in particular it is negative. Wedefine the Favard class F of the semigroup S(t) by F := {x ~ X;limsupl S(t)x-x I < cx)} t t~o+ (see e.g. [8],[9]) and similarly the Favard class F_~ of S_~. Weintroduce the norm IzlF := supl S(t)x - x t I t>o on F and similarly IXlF_, on F_~. Obviously, A_a maps F isometrically onto F-t. If X is reflexive then E = D(A) ([8],[9]). For a non-reflexive space the adjoint semigroup S*(t) is not strongly continuous in general. As usual, X(v denotes the maximal closed subspace of X* where S*(t) is strongly continuous. By Theorem 3.2.6 in [8], F-1 can be imbedded into X(~*, and F_~ = X~:-)* whenever X is sunreflexive with respect to the semigroup S(t). The following well-known proposition is crucial for our formulation of control problems.See also [3],[41,[7],[8]. PROPOSITION 2.1 map
Let S(t) be a C0-semigroup on a Banach space X. Then the f~S-l*f:=
S_~(t- s)f(s)ds
is continuous from L~(O,T;F_~) into C([O,T];X) for all finite exists a constant c(T) such that
IIS-~*fllc([o,rl;x)
T > 0 and there
_< c(T)
On the basis of this proposition we define the mild solution of the equation (1.2) for B ~ £(U,F_I) and xo ~ X as follows t
x(t)
= S(t)xo
j~0
+ S-a(t
- s)Bu(s)ds
(2.1)
]l)eschet al.
250
Nowwe state the main result of [4] on the existence and properties of the differential Riccati operators. THEOREM 2.2 For each 0 < t < T < c~ there exists a unique operator P(T, t) £(X, °) satisfying t he f ollowing properties : (1) P(T, t) is symmetric in the sense that (P(T, t)x, z) = (P(T, t)z, for all x, zEX. (2) P(T, t) is positive in the sense that (P(T,t)x,x I >_ 0 for all x ~ X. (3) For each x ~ X, P(T, t)x depends continuously on t. (4) P(T, .) satisfies the following version of the Riccati equation: For each x, z ~ X, T
(P(T, t)z,
x) = ~ (CS(s - t)z,
CS(s
T
- f (B*P(T, s)S(s - t)z,
B*P(T, s)S(s -
Moreover, if P(T, t) is given as above, then the optimal control is determined by the feedback law ~t(t) = - B*P(T,t)2(t) and the value function of the optimal control problem is determined by P(T, .): (P(T,t)xo,x0)
= minJ(u;xo,
T-t),
where the minimumis taken over all u ~ L2(0,T - t; U).
3
ALGEBRAIC
RICCATI
EQUATION
The main result is the following theore~n. THEOREM 3.1 Let the following hypotheses be satisfied (HI) A is a generator of an exponentially stable Co-semigroup S(t) on a Banach space X; (H2) B E £(U,F_I) , U is a Hilbert space; (H3) C E £(X, Y), Y is a Hilbert space. Then there exists a unique P ~ £(X, @) satisfying t he f ollowing p roperties : (i) (Px, x)x.×.x" >_ 0 for all x e X ; (ii) (Px, y) = (Py, for allx , yGX; (iii) The following weak version o.f the algebraic Riccati equation holds for any x, y ~ F for which there are u, v ~ U such that A_ ~ x + Bu ~ X, A_ ~ y + Bv ~ X: (A_lx, PY)xe. ×xo + (A_iy, Px)xo. ×xo (Cx, Cy)~. - (B*Pz, B*Py)u
(13.1)
Infinite HorizonRiccati Operatorsin NonreflexiveSpaces
251
Moreover, the optimal control fi for ti~e problem (1.1),(1.2) is given by the feedback law ~t(t) = -B*P~(t) , (3.2) where ~ is the mild solution of ~=Ax-BB*Px
,
x(O)
=
(3.3)
For the value function the equality min J(u;
Xo)
=
(Pxo, Xo)
uEL2(R+;U)
holds for any z0 ¯ X. Proof: The proof is given in three steps. 1) Construction of P, Since the differential Riccati operator P(T, t) is symmetric and non-negative, the Cauchy type inequality [(P(T,t)x,y)l
2 <_ (P(T,t)x,x).(P(T,t)y,y)
holds for any x,y ¯ X. Because of the assumption (H1) we have T-t
(P(T,t)x,x)
= (P(T - t,O)x,x)
~, ICS(s)xl2ds<_cllxl j~O
where c~ is independent on t,T. Moreover, if T1 > T2 and u ¯ L2(O, Tr;U), then J(u; x, T2) ~_ g(u; x, TI). Consequently, (P(T2, O)x, x) <_ (P(TI, O)x, Therefore there exists lira (P(T, t)x, =: T--~oo
for all x ¯ X independently on t ¯ I~+. By symmetry we have 4(P(T, t)x, y) = (P(T, t)(x + y), x + y) - (P(T, y), ( x - y) so that we infer the existence of lira
(P(T,t)x,y)
=: a(x,y)
for any x, y ¯ X. The bilinear form a(x, y) is symmetric, non-negative and bounded. This means that there exists P ¯ £(X,X*) such that (Px,y) = a(x,y). We have shown that P(T,O) -~ in the weakopera tor topol ogy. By sy mmetry and monotonicity we get again a Cauchy inequality ](y,Px-
P(T,O)x)] ~ <_ (y, Py- P(T,O)y).(x, Px- P(T,O)x) 2. _< Cllyl (x, Px- P(T,O)x).
From this we deduce that P(T, O)x converges to Px in the strong topology, and as a consequence Px ¯ X~. Evidently the operator P satisfies (i),(ii).
252
Deschet al.
2) P solves (3.1). In (4, ibrmula (3.8)] we proved the following formula
(P(T, t)4, 4) = [ICx(s)l2 ÷ lu(s)l 2 -[~4,~) ÷ B*P(T, s)x(s)l’2]ds,
(13.4)
where x(.) is the mild solution of the problem &(s) = Ax(s) + Bu(s) , x(t) on the interval It,T]. Choose u E L~(I~+;U). Then the corresponding mild solution x E L2 Iq C(]~+;X), and P(T,s)x(s) -+ Px(s) pointwise in the norm of X® for T -+ oe. As B ~ £(U, F_~) and F_~ is continuously imbedded into °*, B*P(T, s)x(s) -~ B*Px(s). Because of the uniform boundedness of B*P(T, s), the dominated convergence theorem yields [ICx(s)l 2 + lu(s)l 2 -lu(s) + U*Px(s)12]ds
(Px(t), x(t))
(3.5)
Suppose now that Xo e X is such that there is Uo E U for which A_~xo + Buo ~. X. If u ~ W~’~(ll~+, U),u(O) = Uo, then the corresponding mild solution x is a classical one (Proposition 4.3 in [4]). Therefore, we have (using the symmetry of P (3.5))
~
(Px(t),x(t))
= 2(Px(t),A_~x(t) -= -ICx(t)l ~ - lu(t)l ~ + lu(t) + B*Px(t)]~ ¯
Especially, for t = O, 2(Pxo, A-~xo + Buo) = -ICxo] ~ - luol 2 + ]uo + B*Pxo]2 .
(3.6)
Evaluating (3.6) for x + y instead of x0 and subtracting (3.6) for x and y, we
(Px, A_~y + By) + (Py, A_~x + Bu) -(Cx, Cy) + (B*Px, v) (B*Py, u) (B*Px, B*Py) for any x,y ~ F,u,v ~ U such that A_~x + Bu ~ X,A_~y+ Bv ~ X. Further, (Px, A_~y + Bv)xex.~: = (A_~y, Px).,~.x.~
+ (Bv, Px).~.xX~
and (By, Px)xe. x.~e = (B*Px, v)u and (iii) follows. 3) Uniqueness. The equation (3.3) has a mild solution as the linear operator F : C([v, v + T]; C([T, "r + T]; X) defined by Fx(t)=
S_~(t-s)BB*Px(s)ds,
te[r,r+T],
(~.7)
253
Infinite HorizonRiccati Operatorsin NonreflexiveSpaces
has the norm [IFII < 1 for sufficiently small T independently on 7 E ll~ +. From (3.5) we infer immediatelythat IPxo, xo) is the value function of the infinite horizon problem, and that the optimal control is obtained by the feedback ~t(t) = -B* P~(t). Nowlet Q ¯ £(X, (~) s atisfy ( i)-(iii). I f x is a c lassical sol ution to (1. 2) for u E W1’2, then we obtain after a simple computation
: 2(Qx(t),A_x(t) + Bu(t)) : -tCx(t)l- lu(t)l + lu(t) + B*Qx(t)l Taking into account the exponential stability of S_1, we get limt-~c~ (Qx(t), x(t)) 0, and by integration,
+ B*Qx(t)12]dt
(3.8)
The validity of (3.8) can be easily extended to any x0 ¯ X and u E L2(I~+;U). This shows again that (Qx, ~:) is the value function, so that (Qx, x) = (Px, for all x E X. Since P and Q are symmetric, we obtain Q = P. COROLLARY 3.2 Let P be as in Theorem 3.1.
Then
(i) there exists a continuous extension P_~ of P, P-1 : F_I ~ X* (ii) P maps:D(A) into :D(A*) (iii) for x ~ T)(A) the algebraic Riccati equation PAx + A*Px + C*Cx - P_~BB*Px = 0
(3.9)
is satisfied. Proof : (i) Since F_~ is continuously is a linear continuous form on X and that (x, Py}xe.×x~ = {P-~x,y}x.×x £(F-1, X*) and (P-~Bu,y)x. xx (ii) and (iii)
imbedded into °*, t he map y~ (Py, x) therefore there exists P_~x ~ X* such for y ¯ X,x ~ F_~. Moreover, P_~ ~ = (u,B*Py}[~
x,y ¯ ~) (A),u = v = 0.From(3.7)and
(3.10)
(a.10)we have
(Px, Ay) = (P_IBB*Px, y) - (C*Cx, y) - (PAx,y) i.e. Px e 7?(A*) and (3.9) follows. ACKNOWLEDGMENT The authors thank to L.Maniar for pointing in the previous version of this contribution.
out the error
REFERENCES 1.
B.van Keulen. H~-Control for Distributed Systems : A State Approach, Systems & Control : Foundations & Applications, Birkh/iuser, 1993.
254 2.
3.
4. 5. 6. 7.
8. 9.
Deschet al. I.Lasiecka, R.Triggiani. Differential and Algebraic Riccati Equations with Applications to Boundary/Point Control Problems: Continuous Theory and Approximation Theory, Lecture Notes in Control and Information Sciences 164, Springer Verlag, 1991. W.Desch, W.Schappacher. Somegeneration results for perturbed semigroups. In: P.Clement, S.Invernizzi, E.Mitidieri, I.Vrabie, eds. SemigroupTheory and Applications. Lecture Notes in Pure and Applied Mathematics 116, M.Dekker, 1989, pp. 125-152. W.Desch, J.Milota, W.Schappacher. Least square control problems in nonreflexive spaces, to appear in Semigroup Forum. O.Diekmann, S.A.van Gils, S.M. Verduyn Lunel, H.-O. Walther. Delay Equations. Functional-, Complex-, and Nonlinear Analysis. Springer Verlag, 1995. G.Greiner. Perturbing the boundary conditions of a generator. Houston J. Math. 15: 527-552, 1987. R.Nagel, E.Sinestrari. InhomogenousVolterra integrodifferential equations for Hille-Yosida operators. In:Lecture Notes in Pure and Applied Mathematics 150, M.Dekker, 1994, pp. 51-70. J.van Neerven. The Adjoint of a Semigroup of Linear Operators. Lecture Notes in Mathematics 1529, Springer Verlag, 1992. P.L.Butzer, H.Berens. Semi-Groups of Operators and Approximation. Springer Verlag, 1967.
A Hyperbolic Variant Simon’s Convergence
of Theorem
Alain HarauxCNRS Laboratoire d’Analyse Num6rique,Universit6 P. et M. Curie, Paris, France
The main object of this report is convergence to an equilibrium of weak global energy-bounded solutions of the wave equation utt + cut - Au + f(x,u) where ~2 is a bounded smooth domain of ~v, c > 0 and
is a function analytic in s satisfying some relevant growth conditions. Such a result has been obtained recently in a joint work with M.Jendoubi [8] as a culminating point of our attempts to understand in depth the fundamental theorem of L. Simon [17] on convergence of bounded trajectories of semilinear parabolic systems with analytic nonlinearities. The convergence problem for gradient or gradient-like systems has already a rather long history starting around 1960 with some investigations of S. Lojasiewicz on the steepest descent problem in differential geo~netry. Even in finite dimensions the question is more complicated that it maylook at first sight. S. Lojasiewicz [12, 13] was led to the idea that analyticity of the potential is the key to convergence and, under this condition, established a topological property of stationary points which allows to derive convergence via a simple differential inequality. Muchlater, in 1982, J. Palls and W. de Melo [15] somehowconfirmed the necessity 6f the Lojasiewicz condition which may fail even for C~ gradient systems. Very soon after, in 1983, L. Simon achieved his remarkable work on parabolic problems. In tile mean time, Tile convergence property had been established for various gradient and quasi-gradient flows by B.Aulbach [1], H. Matuno[14] and T.J. Zelenyak [18]. The dimension condition used in the proofs of Aulbach and Matano has been later exploited in a quite general context by Hale-Raugel [3] and allows convergence proofs under standard regularity assumptions, in particular analyticity is not needed. However, apart from the case of thin domains, in higher space dimensions 255
256
Haraux
this hypothesis is not very natural. Also the counterexalnple of [15] suggests that we have to be careful even when dealing with the heat equation. And maybe there is something really deep hidden behind this strange-looking Lojasiewicz Lemma. The hyperbolic case studied below as well as a recent result of E. Feireisl and F. Simondon [2] for degenerate parabolic equations seem to confirm once more the interest of this simple intuitive idea: analyticity of the potential has a tendancy to kill small oscillations, even if the solution itself is not analytic!
1
FINITE
DIMENSIONAL
GRADIENT
SYSTEMS
In this section we consider the finite dimensional Euclidian space X = l~ N with usual norm denoted as I.I and a potential field F : tt: N ~ l~. For simplicity we assume F N) E C201~ and we denote by VFthe gradient of F. Weconsider the first governed by the equation u’+VF(u)=0,
order gradient system
tk0
(1.1)
First we recall a simple well-knownfact on bounded solutions of (1.1) PROPOSITION 1.1 If u is any 91obal bounded solution
of (1.1),
we have
lim dist(u(t),g) with £={aeX,
VF(a)=0}
PROOF First we notice that F is a Liapunov function of (1.1). Moreprecisely for any solution u of (1.1) we have
-lu’(t)l~ <_ ~F(u(t)) =
0
(1.2)
Since u, and therefore F(u) is bounded, (1.2) implies (1.3)
u’ E. L~(O, +e~; X) Then by differentiating
the equation u" = -V~F(u)u ’ ~ L~(O, +oo; X)
(1.4)
and therefore
- lu’(t)l
(1.5)
e
By (1.5) the function p(t) I¢(t)l ~ te nds to a l imit as nonnegative and p ~ L~ (0, +oc; X), we conclude that lim (u’(t))
t--~+~x)
t
Since p is
HyperbolicVariant of Simon’sConvergenceTheorem
257
This last property implies the result sihce then by the equation, any limiting point of u(t) as t -~ +e~ belongs to g = (a E X, ~7F(a) 0}. REMARK 1.2. It is natural
to wander whether in fact we have
lim u(t) = a £ The situation is as follows 1) If N > 1, the answer is negative in general. More precisely, if N = 2 the omega-limit set of a bounded trajectory can be a full circle even for F ~ C°°, of. Palls-De Melo [15 ]. 2) If N = 1 we have convergence since any non constant trajectory is monotone. If N > 1 we have convergence assuming that F is (real) analytic. THEOREM 1.3 (Losjasiewicz) Let F : l~ N -~ ]~ be real analytic and let u be any boundedglobal solution o[ (1. I). There exists a ~ ~ such that lim lu(t) - aI = 0
(1.6)
The proof of theorem 1.3 relies on the following deep lemmadue to Lojasiewicz [12, 13 1. LEMMA 1.4 (Losjasiewicz) Let F : NN _.+ ~ be real analytic and let a ~ g. There are two real numbers (depending on a in general)
oe(o,1/2); such that
Vue X,lu - al _
(1.7)
The proof of Lemma1.4 is quite involved and is based on the theory of real analytic manifolds. On the other hand, it is very easy to understand why (1.7) not satisfied in Palls-De Melo’s counterexample, and the proof of Theorem1.3 is a simple consequence of Lemma1.4. Part of the depth of Lemma1.4 is contained in the quite non-trivial and essentially global information that any critical point of F close enough to a has to be at the same energy level as a. Indeed when VF(u) = and lu - a t _< r], (1.7) gives F(u) = F(a). On the other hand there is apparently no way of globalizing (1.7) completely. It would be very useful, especially in view infinite dimensional generalizations, to find either a non-constructive elementary proof by contradiction or (even if it is very complicated) a constructive method allowing to determine 0 in terms of F and a. PROOFof Theorem 1.4 (admitting Lemma1.3) Let a be any limiting point u(t) as t -~ +oo. As a consequence of Proposition 1.1, we have a ~ £. Introducing v = u - a and C(v) = F(u + a) -
258
Haraux
we may assume that in fact a=0 After this reduction,
F(0)=0
(VF)(0)=0
since F(u(t)) is nonincreasing and a = lim U(tn) for some
sequence tn tending to infinity,
we have Vt > 0, F(u(0) >_
(L8)
Also by (1.2) we have also , since ~ =-VF(u)
= -I-’(t)llVF(-(t))l In addition, either F(u(T)) for someT fin it e, in wh ichcase F(u(t) ) = 0 for all t k T and as a consequence of (1.2) we conclude that u(t) ~ a. Or F(u(t)) > 0 for all t > 0. In this last case ~(-[F(u(t) °) : -O[F(u(t) )] °-’ ~ F(u(t) ) 0 IVF(u(t ) ~-° )llu’ [F(u(t))] and by (1.7) this implies
°) >Olu’(t)l ~(-[F(u(t))]
(1.9)
on any interval of (0, +oc) on ~vhich the condition
lu(t)l_< is fulfilled. Inequality (1.9), implying an ~ bound on u ~, i s q uite s uggestive o f convergence. To complete the proof we select s > 0 such that
1 sup[F(s)l° < ~
and
~ Isl<~
~
(1.10)
Then let tl > 0 be such that lu(h)l <_
(1.11)
aud T := sup{t~ > t,,
[u(t)l
~, Vt E ( t, ,t~)}
By using (1.8) for t = te we find, integrating (1.9)
’¢t.~z (t,,T),
t~ 9~t
1 r/ lu’(t)ldt < ~[F(t,)]° < ~
If we assume combining(1.10), (1.11) and (1.12) , we obtain by letting t2
N(T)I
(1.12)
259
HyperbolicVariant of Simon’sConvergenceTheorem a contradiction
with the definition
of T. Hence T = +~ and lu’(t)ldt <
In particular a(t u’ ~, E +~) L and ’a(t) is convergent as t
2
A RESULT
OF L.SIMON
L. Simon[17] cousidered in particular the semilinear heat equation ut-Au+f(x,u)--O u=0 where ~ is a bounded smooth domain of
inR+ onl~ + ×Ogt l~ N,
C
×~
(2.1)
> 0 and
f : f~ x IR ---+ I~ is analytic in u, uniformly with respect to x ~ f~ He obtained THEOREM 2.1 (L. Simon) Let u be any bounded global solution on [0, +co) × ~. There exists ~ ~ g such that lim Ilu(t)
- vlI~ = 0
of (2.1) bounded
(2.2)
with
$ = e C( )n HI(a)/ - zs f( x,o) ina} The proof of Theorem2.1 is quite subtle and we shall not indicate its details. It relies essentially on the Lojasiewicz Lemmaand most of the difficulty consists in extending this Lemmaon an infinite dimensional setting. Although Lemma1.4 has an essentially global character since it involves the nonlinear energy functional, Simon has used the linearized equation around an equilibrium ~o ~ g. Fredholm’s alternative for the linearized stationary operator allowed him to apply Lemma1.4 to an auxiliary finite-dimensional nonlinear potential. Then he was able to come back to the concrete energy functional modulo a translation procedure replacing ~ by 0. The end of proof is parallel to the proof of Theorem 1.3, replacing the potential F(u) by the energy functional
= 1/~lVul2 with
dx + /~F(x,u)dx
(2.3)
It
j~0
F(x, u) := f(z,
s)ds
(2.4)
260
Haraux
Here note that even if f does not depend on x in the original equation (2.1), fact it does after the translation procedure since f(u) is replaced by g(x,u) f(u ÷ ~(x)) - f(u) REMARK 2.2 1) The original proof of Theorem 2.1 [17] seemed to use quite strong regularity properties of the solutions. Someprecise remarks on the natural functional setting will be given in Section 4. 2) The same result is no longer true if f is Ck with respect to u, cf. P. Polacik and K.P. Rybakowski[16] for a counterexample with f depending on x and k arbitrarily large. However their technique depends essentially on the x-dependence and they cannot handle the C~ case.
3
SECOND ORDER GRADIENT-LIKE
SYSTEMS
In this section we consider the second order differential system governed by the equation u" + c~’u’ + ~F(u) 0, t _ > 0 (3 .1) For simplicity we assume N) F e Cz(I~ and we denote by VF the gradient of F. First we have a simple general result whoseproof is essentially identical to the proof of Propositon 3.1 PROPOSITION 3.1 If u is any global bounded solution
of (1.1),
we have
lim dist(u(t),£) with ~ = {a ~ X, VF(a) = 0} PROOF First we notice by the equation, boundedness of implies that u’ and u" are also bounded. In addition for any solution u of (1.1) we have d~{ lu’(t)] 2 + F(u(t))} = -lu’(t)l 2 < 0
(3.2)
Since u, and therefore F(u) is bounded, (3.2) implies u’ ~ L~(0, +~c;X) Then by differentiating
the equation
u’" + au" = -V~F(u)u ’ e L~(0, +~c; X) Multipying by u" and integrating on [0, t) we deduce that u"e L~(0, +~x);
(3.3)
HyperbolicVariant of Simon’s ConvergenceTheorem
261
Therefore ~-~]ud’(t)l s = 2(u’, u") E t (0, +ec; X) The rest of the proof is identical to that of Proposition 1.1. REMARK 3.2. It is natural
to wander whether in fact we have lim u(t) = a E
If N = 1 we have convergence (cf. e.g. [4, 5]). If N > 1, the answer is probably negative in general. In [7] the following result w~ obtained THEOREM 3.3 Le¢ F : ~N ~ ~ be real analytic solution of (1.1). There exists a ~ ~ such that
and let u be any bounded global
lim ~u(~) - a~ =
To prove this result,
(3.4)
we had to consider the modified Liapunov function
H(t) = ~lu’(t)l ~ + F(u(t)) + e(VF(u(t)), For e > 0 small enough, using Lemma1.4, it can be shown that for t large ~t {(H(t)) °} _< -O-~(lu’(t)l + IVF(u(t))l)
(3.5)
Then the proof parallels the first order case.
4
THE MAIN RESULT
Wenow consider the second order evolution problem utt+cut-Au+f(x,u) u=0
=0 inlR + x~ on~ + )
(4.1)
where Ft is a bounded smooth domain of ll~ ~v, c > 0 and f:Ft
x~--~
In Ill] M.A. Jendoubi adapted to equation (4.1) the method of L. Simon [17] for infinite dimensional systems of parabolic type (cf. also [10] for an abstract reformulation of Simon’s results under natural regularity conditions). He proved the following result.
262
Haraux
THEOREM 4.1 Assume that f is analytic in s, uniformly with respect to x Of (x,s) and 02f ~ and f(x,s), ~s2 (X,S) are bounded in ~ × (-/~,/~) Vfl > O. Let a solution of (1.1) and assume that there exists p >_ 2 such that t3 {u(t, .),ut(t, t_>l
.)} is precompact in W2’P(Ft) W"P(~)
(4.2)
with p >N-~ if N<_6, and p > N if N>6. Then setting $ = {V E H’~(~) there exists ~ E S such that lim {l[utllw,.,(~) Il u(t, .) ~(. )l lw~.,(n)} = 0. This result is interesting because no growth condition on f is required, on the other hand it is only applicable to strong solutions and the condition of boundedness in W~,~(~) × WLP(~)is restrictive and not always easy to check in practice. hypothesis was motivated by the necessity of using an infinite dimensional extension of the classical Lojasiewicz inequality. In fact when trying to extend the method of 3, in a first approach it is natural to .consider, after replacement of u by u - ~, the functional
=dx ¯ (t)=~ I~1
+ E(~)+~ f~ [-/~u+ f(x, ~)].~
with E(u) = l ~¢ lVulU dx + L F(x, u)dx as a possible Liapunov functional. ¯ ’(t)
~( -c~+~f’(x,u))[ut[~-dx+~
= ~(-~+~]’(x,u)),ut,~dx-~
Howeverthe computation gives jf ~[-Au + f( x,u)]uttdx+~/~ ,V
ut,~dx
,-Au+f(x,u),2dx-a~[-Au+f(x,u)]utdx
The three firs~ terms fi~ just OK,bu~ the las~ one is of higher order wi~h ~he bad sign.In order to overcome~his di~culty, Jendoubi considered ~he modified functional H(t) = ~(t) + 6 ~ IVutl2 dx + ~ ~1- Au + f(x,u),:
dx + ~ ~ f’(x,u),ut,
By using (4.2), he proved that for ~ small enough and t > H’(t)
~ -¢
f (iw,,i +1-+ f(x,u)l2} dx
~ dx.
263
HyperbolicVariant of Simon’s ConvergenceTheorem To conclude the proof of Theorem4.1, Jendoubi used the following result
LEMMA 4.2 Under the hypotheses of Theorem 4.1, let ~ E S, then there exist 9 ~ (0, ½) and a > 0 such that Vu ~ W2’P(12) n H~(~), []u- ~l]2,p < a implies
II - ~xu+ f(x,u)lb:(m> 1-a 6lE(u)- E(~o)l
(4.3)
for some ~ > O. Actually (4.3) does not look too natural since when f = 0, the energy is comparable to the square of the norm of -Au in H-l(f~) rather than L2(f2). As a matter of fact, in [8] we established LEMMA 4.3 Assume that f is analytic in s, uniformly with respect to x ~ 12 and either N = i and f(x,s), and ~-~/(x,s) are bounded in ~ × (-~,~3) for all l~ > or N >_ 2, f(x,O) ~ L~(~t)
I-~(~,s)l < c(1 + Isl~) a.~.on~ × (-~,~)
(4.4)
for some C >_ 0 and c~ >_ 0, (N - 2)~ < 2. Given ¢: ~ S, then there exist ~ e (0, ½) and a > 0 such that Vue H~(f~), Ilu - ~llH~(a) < a implies
II- ~Xu+f(x,u)llH-,(~) 61E (u) (~ -~-° E
(4.5)
for some ~ > O. From Lemma4.3, following the strategy of the previous proofs, we obtained the following final result THEOREM 4.4 Assume that f is analytic in s, uniformly with respect to x ~ f~ and either N = 1 and f(x, s), and °o~s(x, s) are boundedin 12 x (-l?, 17) for all/? O, or N >_ 2, f(x,O) ~ L~(~) ]-~(x,s)l
_< C(1 + Isl ~) a.e.on f~ x (-oe,c~)
(4.4)
/or some C >_ 0 and a >_ O, (N - 2)a < 2. Let u be a solution of (1.1) such that ~ {u(t, .),ut(t, t>_o
.)} is boundedin go~ (~t) x L2(12).
Then there is a solution qo of
such that lim {[[Ut[IL:(~)flu(t, .) -- qO(.)[[So~(~)} = O
(4.6)
264
Haraux
REFERENCES 1. 2. 3. 4. 5. 6.
7.
8. 9.
10. 11.
12. 13.
14. 15. 16. 17. 18.
B. Aulba.ch, Approach to hyperbolic manifolds of stationary solutions, Springer-Verlag Lecture Notes in Math. 1017 (1983), 56-66. E. Feireisl ~z F. Simondon, Convergence for semilinear degenerate parabolic equations in several space dimensions, to appear (1999). J. Hale & G. Raugel, Convergence in gradient-like systems with applications to PDE, Z. Angew. Math. Phys. 43 (1992) 63-124. A. Haraux, Syst~.mes DynamiquesDissipatifs et Applications, R.M.A. vol 17 (Masson, Paris, 1991). A. Haraux, Asymptotics for some nonlinear O.D.E. of the second order, Nonlinear Anal. TMA10 (1986) 1347-1355. A. Haraux, "Semilinear hyperbolic problems in bounded domains", Mathematical Reports, vol.3, Part.1 (Edited by J.DIEUDONN15,).Harwood Academic Publishers, NewYork (1987). A. Haraux & M.A. Jendoubi, Convergence of solutions of second-order gradient-like systems with analytic nonlinearities. Journal Diff. Eq 144 (1998), 313-320. A. Haraux & M.A. Jendoubi, Convergence of solutions of the wave equation with analytic nonlinearities. Calculus of variations and PDE,to appear (1999) A. Haraux & P. Polacik, Convergence to a positive equilibrium for some nonlinear evolution equations in a ball, Acta Math. Univ. Comeniane, 2 (1992) 129-141. M.A. Jendoubi, A simple unified approcb to some convergence theorems of L. Simon. Journal Funct. Anal. 153 (1998), 187-202. M.A. Jendoubi, Convergence of global and bounded solutions of the wave equation with linear dissipation and analytic nonlinearity, Journal Diff. Eq. 144 (1998), 302-312. S. Lojasiewicz, "Ensembles semi-analytiques", I.H.E.S. notes (1965). S. Lojasiewicz, Une propri~t6 topologique des sous ensembles analytiques r6els. Colloques internationaux du C.NIR.S #117. Les dquations aux d6riv6es partielles (1963). H.Matano, Convergence of solutions of one-dimensional semilinear heat equation, J. Math. Kyoto Univ. 18 (1978) 221-227. J. Palis, W. de Melo, Geometric theory of dynamical systems: An introduction Springer-Verlag, New-York(1982). P. Polacik, K.P. Rybakowski, Nonconvergent bounded trajectories in semilinear heat equations, J. Diff. Equa. 124 (1996), 472-494. L. Simon, Asymptotics for a class of non-linear evolution equations,with applications to geometric problems, Ann. of Math., 118 (1983), 525-571. T.J. Zelenyak, Stabilization of solutions of boundaryvalue problems for a second order parabolic equation with one space variable, Differentsial’nye Uravneniya 4 (1968) 17-22.
Solution of a Quasilinear Parabolic-Elliptic Boundary Value Problem V. PLUSCHKEDepartment of Mathematics Luther-University, Halle, Germany
1
and Computer Science,
Martin-
INTRODUCTION
In this paper we consider the following parabolic-elliptic interface problem: Let f~ E ll~ N, 1, N _> 2, be a simply connected, bounded domain with boundary 0~ E C and I = [0,T]. For given nonnegative g = g(x,t,u) : ~ × I × R -~ II~ we define f~e = fl \ suppzee g(x, t, u) ,
f~p = fl \ f~e ,
F = Of~e n Of~v
and assume that £te, tip are independent of t and u. Then we look for a weak solution of
in Q/,:= f~ × I, on rT:= r × I, on BT:: 0~ × I, x e f~p,
g(x, t, u) u, + A(t)u = f(x,
u(x,t) = u(z,O)= Vo(~)
(1) (2) (3) (4)
N where up =u[~,u~ utah, and A(t)u =-~,~__, = (~(x,~)~) +~0(~,~)~. Since g = 0 for x ~ ft~ the problem is elliptic on ~t¢ × I and parabolic on tip × I. Parabolic-elliptic interface problemsdescribe eddy currents in applications to electromagnetic field theory (cf. MacCamy and Suri [5]). The linear parabolic-elliptic problem of type (1)-(4) is investigated by a number of authors (cf. l, [21, [3 ]) who derived existence and uniqueness under rather general assumptions for g. A parabolic-elliptic interface problem with special nonlinear monotoneoperator A is solved by Zlmal [10]. Wenow investigate the problem with nonlinear dependence of f and g on u. Unlike in [10] even on f~p × I the coefficient g must not be bounded below by a positive constant. Since supp.~e~ g(x, t, u) maycontain sets of zero measure where g = 0 the parabolic problem on f’tp × I may degenerate. The decrease to 265
266
Pluschke
zero ofg is restricted by a condition on 1/g belonging to L~(flp) for all t E I,u E I~. Moreover, our technique is not restricted to Hilbert spaces. Hence we can prove stronger regularity results, e.g. almost everywhere boundedness with respect to t of ut on fp × I and even continuity of the solution u in QT for nonsmooth data. To construct the solution we use se~nidiscretization in time (Rothe’s method) that approximates the quasilinear degenerate problem by a set of linear nondegenerate uniformly elliptic problems. This method was also used by Ka~ur [3, Chapter 6.2] to solve the linear problem in somewhatlarger spaces. For f¢ = q} our problem also includes degenerate parabolic equations. However, in that case we refer to [6] for stronger results. In the present paper we do not suppose most general assumptions on the data in the parabolic region. Finally, note that our degeneration in equation (1) differs essentially from the degeneration b(u), considered by manyauthors (cf. e.g. [1]). Although for smooth b we can write b(u)~ = b’(u)u,, the set where b’ vanishes depends on u, whereas in our case the set of degeneration is supposed to be fixed for all u.
2
PRELIMINARIES
In the following [l’ lip := I[’ [Ip,~ denotes the normin Lp(f) and (., .) the duality between Lp(gt) and Lp, (~), lip + liP ~ = 1. L~,o(f) is the weighted Lebesgue space with weight 0 = O(x) and finite norm [[ullp, ~ = (f~ o(x)[?t(x)[ p dx)1/p. By [[. [[o and [[. [[o,~ we denote the norm in C(~) and HSlder space C~(~), respectively. wpl(f), l)dp~ (f) are the usual Sobolevspaces where l)dp~ (fl)is normedIlull,, :- IIVul] p. For functions restricted to tip we write l)dp~(flp) if the trace vanishes on 0fl~ ~ Off. For fixed t ~ I the operator A(t) generates a bilinear form I/~(fl) x ~,(~) denoted by A(~)(.,.). Moreover, we use the standard evolution spaces C(I,V), C°’~(I,V), and L,(I, 1/’). By c we denote a generic nonnegative constant being independent of the subdivision. Next we formulate the assumptions which are supposed to hold throughout the paper. Note that for every N there are p and r fulfilling the following restrictions. ASSUMPTIONS Suppose tip being simply connected with boundary °’~ Oi~p ~ C and meas~c_~(0~p Cl Of) > 0. Let g and f be Carath~odory functions defined ~×(I×IR). Let further be r > N, a > 1,p >_ max{2, Nr/(N+r)},p > N(a+l)/2a, and 2r(p- 2)/(r - 2) Np/(N- 2) Then we suppose for arbitrary t, t ~ ~ I and u, u~ ~ C(~) (i) U0e b~/~(llv); (ii) g(., t,u) :I x C(~) -~ Loo(~)is uniformly bounded in Loo(~) and fulfils Lipschitz condition IIg(., ~,~) - g(., ~’, u’)ll~ _<e, (1~ - ~’l ~ - u’ll ~). Furthermore, g(x, t, u) >_ for al l (x , t, u) ~ f × I × I~an 1/g(.,t,u) :I × C(fi---~) -> L~(fip) is boundedin L~(fp). (iii) a~ ~ C°’~(I,C(~)), ao ~ C°’~(I,L~(~)) ellipticity condition
with ao >_ 0, and it,
holds the
QuasilinearParabolic-Elliptic Boundary ValueProblem ~i,k aik (x, t) ~k >_ a
267
f6r all (x, t) E Q--~ and ~ E ~v, a >
: I x C(~) ~ Lp(~) is bounded in L,(~) and fulfils (iv) f(.,t,u) condition Ilf(’, ~,u) f(.,t’ ~’~" (v) Compatibility condition: ¢ ~ L.,~(.,o,~o)(~) such
the Lipschitz
There exist an extension ~0 ~ ~ (~) of Uo and
(g(., 0, Uo)¢, v) + A(0)(~o,v) = (f(.,
(C)
for all v ~ W~,(~) ~ L~(~p) holds. Welook for a weak solution in the following sense: DEFINITION Wecall u a weak solution of problem (1)-(4) u e L~(I , I}V~ (~)) has a derivative ut ~ L~(I, Lp,g(~)) and fulfils the relation ~(g(.,t,u)
ut,v)dt
+ ~ A(o(u,v) dt= f1(f(’,t,u),v)dt
(R)
for all v ~ LI(I,I~V 1 (t)¢~ L~(~p)) and initial condition (4). Wecall u a local weak solution if there is a time ~, 0 < ~ _< T such that u is a a weak solution in ~ := [0, ~]. Due to assumption (ii) a weak solution has a time derivative with ~ = pa/(a + 1) since the estimate
I1 11., <1/g .
~/(~+l)~
in L~(I, L~(~,))
=cllull,
(5)
holds. Moreover,the boundarycondition (3) and the first condition of (2) is fulfilled by the choosen function space for u, while the second condition in (2) is included the relation (R) in the sense that any smooth weak solution by the Gauss formula fulfils the equation (1) as well as transmission condition (2). Wediscuss the compatibility assumption (v). For v e I)V),(~) we see Oo must fulfil the elliptic equation A(0)/)o = f(., 0, ~ro) on f~g. Moreover, ~ro E I)dr ~ (ft), the boundary values of the extension on O~care given by the traces of Uo on F and ~0 = 0 on 0~ \ F. Hence, the extension of Uo into tic is fixed by an elliptic Dirichlet problem on tic. However, relation (C) also includes a transmission condition 0.~ Do,~ = 0~, Uo,v on F in weak sense. There is no freedom to fulfil it. Thus condition (v) is overdetermined: One cannot prescribe an arbitrary even very smooth initial function (4), but it is possible to ’bend’ it somewhatin neighbourhoodof F in order to fulfil (v). This compatibility condition is not supposed e.g. in [2], [3], [7], [10]. But these authors do not prove L~-boundedness with respect to time of the derivatives of u. In our case condition (v) is necessary: LEMMA 1 Let u be a weak solution of problem (1)-(~) with data fulfilling tions (i)-(iv). Thencompatibility condition (v) is satisfied.
assump-
268
Pluschke
PROOF Weprove the assertion for the more general case that ut ¯ Leo(I, L1 (fiTs)), p > 1, and no assumption is madeon 1/g. Of course, this is fulfilled by (i)-(iv) to the estimate (5). Owingto the choosen function spaces there is a sequence {t.n}, t,~ -~ 0, and a constant C such that II.a(.,tn)Nl,r <_.C, Nut(.,tn)Np,~(.,t.,,4.,t.)) < c and (g(.,t,~,u(.,t,d)ut(.,t,
d, v) + A(to)(u(.,t,d,
v) = (f(’,t,.,U(’,tn)),
(6)
for every v ¯ I~, (fl) r-i Loo(fly) holds. Thenthere is a subsequence{t,~. } such u(.,t,~.)~w
inl~l(fl),
w~,:=g(.,t,~,u)~/’ut(.,t,~)~w
inLp(flv).
By our assumptions we have u ¯ C°’l(I, Ll(flp)), hence winv = Uo and thus ’W -~’~ 00. The compact embedding 1~ (fl) C C(fi) even yields uniform convergence lz(’,tn~) --+ ~o as t,~ -~ 0. Moreover, let g~ := g(.,t,~,u(.,t,~)), := g(. ,O, Uo) we have g~ut(.,t.~)
gllp’ 11: w~ ~ _lip’ = ~ w~(^lip’ = y~, lolP’ -g ) w~ +go Yo ~ .
in L~(~tp)
since gk ~ go in Lc~(flT~). Wenowdefine ¢ := g~l/Pw in lip, ¢ = 0 in fl\ flT~, then ¢ ¯ Lpmo(fl) and g~ut(.,tn~) -~ g0¢ in Lp(flT~). Finally, a limit process t.,~ -~ 0 in (6) yields the compatibility conditon (C). In order to solve the problem (1)-(4) by semidiscretization in tilne (Rothe’s method) we subdivide the time interval I by points tj = jh (h > 0,j = 0,... ,n) and look for a solution uj ¯ 1~:,! (fl) of the discretized problem (gjSui,v)
+ Ay(uj,v) = (fj,v)
Yv¯ l~l,(fl)
(Ri)
uo = 0o,
(40)
j = 1,... ,n, where 5uj := (uj - uj_~)/h, gy := g(x, tj,uj_~), ]~ := f(x,t~,u~_~), and Ay(., .) := A(t~)(., .). This is a set of linear non-degenerated elliptic boundary value problems to determine the approximation uj if uj_~ is already known. Since fj, g~uj_~ ~ Lp(~) C (W~, (~)) holds for p ~ Nr/( N + r) and g j ~ 0, ao~ 0 the existence and uniqueness of a solution follows from [8, Theorems7.3 and 5.4]. Observe that the assumption r > N implies uj ~ C(~). Weconclude this section with some inequalities which we need for the a prioriestimates. Anessential tool in our investigations is the interpolation inequality (see [4, pp. 62-681)
Ilwll _
where g < ~ and ~,i~+i/N
< 0 ~ 1 , (7)
which is applied to power type functions w := iui(P-~U~’u defined on ~. Since w = 0 on a part of 09~ (cf. assumptions) IIwlN,~,a~ is an equivalent norm in ~)~ (~). Using Youngs inequality and ~he estimate (5) we obtain ~
c,
u n,
Vue W~(av)nL~(a~),
(8)
with p/2 < s < Np/(N - 2) where ~ = 1 for a = 1 and fl = 3(a,0) > 1 ~v-~(N-~) 1 < a < 1 + s(~s-v) . The last condition on a arises from the fact that we need
269
QuasilinearParabolic-Elliptic Boundary ValueProblem
a0 < 1 in order to derive (8) from (7). If 0 = 1 we obtain from (7) the Friedrichs inequality Vu e 1)¢~1(a) c~ L~(a),
(9)
where kF = kF(s, f~).
3
A PRIORI
ESTIMATES
FOR THE APPROXIMATIONS
In this section we derive estimates for the derivatives of uj with respect to x and for the discrete time derivative. The first estimate follows from the second one since uj can be regarded as a weak solution of the elliptic Dirichlet problem Ajuj = fj-gjSuj in [2, u~lon = O. Then from [8, Theorem6.3] and the positivity of Aj follows
Ilujlll,~
(10)
for all j = 1,... , n and all subdivisions since fj and gj are uniformly bounded in L~(ft) and Lc~(f~), respectively. Hencethe following estimate of (fuj is the crucial result of this section. However, due to the dependence of g on u we only obtain a local estimate. LEMMA 2 For small Lipschitz constant l~ fulfilling interval/~ = [0, ~], :~ < T, and ho > 0 such that
115uyllp,~_< M~Vtj
condition (12) there is a time < ~ 7
holds independent of the subdivision if h < ho. PROOFWetake the difference (Rj) - (Rj-1), j --- 2,... ,n, and test it v = ISujlP-’~6ui. By the use of the notation wj := I(~ujl(P-e)/:5uj and assumption (iii) we estimate (gjSuj, lSujl~-25uj } - (gj_~5uj_~, lSujl~-:Suj ) + klh [lwjll~,~ + kneh llSujllp~n ~
~ h ~(~, ~-~ )~ + l(&_~ - &)(~, where k~ = 4(p-1)/p ~ > 0 and ka e := infnextao(x,t) ~ 0. Note that Vv (p- 1)I~uj[p--2VUj = 2(p- 1)/plSujl (~-~)/~ Vwj. Then we continue by replacing the weight gj-1 by gj on the left side and estimating the right side by means of HSlders inequality, Youngsinequality, and Lipschitz conditions (iv) and (v), I}Sujll~,g~ - (gj~uj-1, ~ l:h
I~ujIp-2~Uj}
+
k~h Ilwill~,~ + ~ kn~hIlSuj[l~,n
1lSujll;-1 + lph 1tSuj-~llp,n~ 115u~ll~,~ + leh IlSuj-xllp,n, 1lSuyll~,~l~
-2)/~-a + ~hII~u~ll~ IIw~ll~,~ II~u~ll~ +~hIlu~ll~ll~u~ll~ p-~dx + /_ IgJ-~- gJl ISuj-xlI~u~l
270
Pluschke
where sz = 2r(p - 2)/(r
- 2) Np/(N - 2). Fu rthermore we hav 1
1
and
These estimates and inequality
(10) then imply
1
+hh[J~p I~uj-llelduylV-~dx+llh f~ Iduy_llP+’dx.
(11)
Observe that the total powerof ~u, in the last two integrals is p + 1 while on the left-hand side we have only the power p. This comes from the dependence of g on u. Wewill manage it below by application of a nonlinear Gronwall lemma, however we have to ensure that no item [l~ujll ~p with ~ > 1 appears on the right-hand side. Otherwise one cannot expect to obtain boundedness of [16ujl[ from the above inequality since it will be fulfilled for every fixed h’just if ~l~uj[I will be sufficiently large. This is not happen if ~lJuj_ll[ ap appears instead of [16uj[[ ~. In order to handle it by means of formula (8) however we have to take care that a > 1 and s > p do not exceed the given bounds. This can only be realized by using (5). Thus we apply HSlders inequality Z, : ( I~u~-ll"
’dx I~j-~l" I~1’-’ dx a~d z~ : [ I~u~-,l" I~u~-,I
with Pl = ~ = ~P/(a + 1), P2 = s2, P3 = 82/(2 -- 1) and p~ = ,~, pe = s3/p, respectively. In both cases we have se = s~ = ap~/(ap - a - 1) < Np/(N - 2) by our assumptions on p. Then we obtain with (5) and Youngs inequMity
where ~ > 1 is sufficiently close to 1 and B = ~(p, ~) >i 1. Applyingnow (8) to norms acting on ~p and Friedrichs inequality (9) to II~u~ll~and II~uyllLwe obtain fi’om (11)
- II~uy_l IIp~,g~_, + k,phIIw~ll?,~ + k~ph Ilau~ll~,., II~uyll~,g~ <
Quasilinear Parabolic-Elliptic
BoundaryValue Problem
Summingup these inequalities
for j = 2,...
271
, ~ yields
i
i
j=2
j=2 i j=2
i-1
i j=2
for every i = 2,... ,n. The critical item is the last If le ~ kas it can be canceled by the corresponding Otherwise we apply Friedrichs HSujH~. If the condition (le is fulfilled
inequality
sum on the right-hand sum on the left-hand
side. side.
(9) to the rest of the sum over ]~Suj]l~,ne
- inf ao) kF(p,~) ~e xI
(12)
< 4(p- 1~ p2
there is an e > 0 such that max{0, le - kae }pkv + e
I1~1~,~, + ~0h~ llwjll~,~ j=2 i
i-1
for every i = 2,... ,n. It remains to estimate II~u~ II~,g, +chIIw~ ~1~,2, We use the compatibility condition (v) and test the difference (R~)-(C) with I~UllP-a~u~. This yield s simil ar to our manipulations at the beginning of the proof
ll~u~lI~,~ + k~hHWlH~,~ + ~ h ll~utll~,~ + (Ao - A1)(Uo,
lSu~lP-~Sul)
~ [~¢[[~,~o [[5u1[[~,~ + -1 lachl[SUl[[~ + ch [[OoH~[[w~ [[~,2 []Su~ [[~v-:)/: + ch [[Oo[[v[[Su~[[~-1 where owing to f~ = f(., t~, ~o), fo = f(’, 0, ~o) no Lipschitz condition with respect to u is used. By the same reason we have
Applying again Youngs inequality,
(8),
and (9) we obtain
We fix now e < min{1/2, k~} and choose then h~ > 0 with h~C~ < 1/2. obtain uniform boundedness of ~l~u~H~ + ch Ilw~ll~,~for all h ~ h~.
Then we
272
Pluschke
The result of these comprehensivemanipulations is the discrete Gronwall inequality i
i
j=l
j=l
II ullp,g , (14) j=l
i = 1,... , n, obtained from (13) and the last calculations. It is essential that the second sum on the right side only runs up to i - 1 since fl > 1 while the first sum also mayrun up to i - 1 if h _< h2 is small enough such that the coefficient c2h is less than 1. Wewrite ck again instead of c~/(1 -c~h~), k = 1,2,3. Omitting the sum on the left-hand side a nonlinear discrete Gronwall lemmaderived by Willett and Wong[9, Theorem 4] yields the bound e~ [[~u,’[~, _ < [c: (~-’)-
- 1)c~ ~ he~(~-’)J (~
fori= 1 ....
j=l
where ei = (1 + c~h)-~ and ~ ~ n is choosen sm~ll enough such that the expression in the brackets remains positive. Since ih = t~ we have e~ ~ e -c~ih = e-c~. This implies
Then there is a ~ ~ T independent of the subdivision such that the expression in brackets is positive and bounded for all ti e [0,~]. This proves the lemmawith h0 = min{h~,h~}. From (10), (14); and the embedding inequalities
(5), (9) we immediatly
COROLLARY 1 Let the assumptions of Lemma 2 be fulfilled. i
Ilull ,r ~ M2,
-< Ma,
Then
p
h
M4
j=l with ~ = ap/(a + 1) and s = Np/(N - 2) hold independent of the subdivision
if
At the end of this section we add an example that illustrates the behaviour of 115ujllp,a if the compatibility condition (C) is violated. Since (C) is imposedto for t = 0 the first difference quotient is of special interest. EXAMPLE 1 For 12 = (0, 2) G I~ we consider the equation .q(x)
u~-uz.~
=0 in (0,2)
×I with
g(x)=
01 for x ~ (1,2) (0,1) forx~
(15)
and conditions (2)_--(4). If we prescribe Uo(x) = 2 - x on f~ = (1, 2) we mayex~end this function by Uo(x) = into f~ e = (0, 1) as a s ol ution of equation (15 ) ful filling
273
QuasilinearParabolic-Elliptic Boundary ValueProblem
~’o,e(1- 0) = [~o,v(1 + 0). However,compatibility condition (C) is not fulfilled O~,e(1- 0) #/)’~,~,(1 + It is an easy exercise to compute ux as a solution of the discretized problem X(1,2) Ul(X) - hut’(x ) = X0,2) (2 - x), u~(0) = u~(2) = 0. Thenwe -e (2-z)/v~ -( + 2-’*)/v~ e
2
2 e(l_z)/v~)
as h ~ 0. This shows: although 5ul converges pointwise for every fixed x E flp we see that 116ulll~,9 = ll6ulll~,n~, = (9(1 e-1/f-~)lh (p-~)/2) is unbounded forp > 1. It is interesting to see that [[Suiiip,9 remains boundedif p = 1. This is no contradiction to Lemma 1 since the reflexivity of Lp(l’l?p) for p > 1 is an essential tool in the proof of Lemma1. Indeed, if p = 1 it would be possible to prove Lemma2 under suitable assumptions on the data without compatiblity condition (C) since in this case there is used an regularized characteristic function as a test function in order to obtain the estimates.
4
RESULT
In this section we prove convergence of the Rothe approximations to a weak solution of problem (1)-(4). Therefore we introduce the Rothe approximations obtained from uj by piecewise constant and piecewise linear interpolation w.r.t, time t, respectively, ~t,~(x,t ) = ~uj(x) ift E (tj_,,tj] [~o(~)if < o
’
(tn(x,t)
= ~uj_,(x)
ift
~ (tj-l,tj]
[~o(z) i~, <_
’
and (tn(x, t) - tj h ui_~(x)
t - tj-1 + ----h---ui(x),
t ~ [tj_~,tj]. ., If wewrite f’~ = f(., ~n, g,~), g,~ = g(., ~,~, fi,~), and .) = A([~)(., .) wi th ~n = if t~_~ < t ~ ty, piecewise constant interpolation of (Ry) over ~ yields ~( ~g u~ , v) dt + ~ A’~(~ ’~, v)dt = ~(f~,
v) dt
~) (R
~ L~(~v)). The results of Lemma2 and Corollary 1 for all v ~ L~(], W~,(~) ~~ the following a priori estimates for the Rothe approximations, II t (’,t)ll,,a"
~ M1,
II t (’,t)ll~,".
II~%,t)-~(.,t’)ll~,.~Mzlt-t’l,
< M~,
II t (’,t)ll~dt
II~(.,t)-~"(.,t)ll~,~
~
(16)
5Mzh~, (17)
It ~ - ~"IIL.(Z,L~(.)) ~ MAh~/O,II~ - ~ IL,(ZL.(.)) ~ MA h~/~, II~(’,t)ll~,~ ~ M~,IW~(.,t)ll~,~ ~ Mu,II~(.,t)lla,~
(18) (19)
274
Pluschke
for all t, t’ E ~f, where the estimates (17) and (18) are an easy consequence of construction of fi’~, fin, and ~in, respectively. These estimates are the basis for convergence assertions for the Rothe approximates which yield our existence result by passing to the limit n -~ cc in relation (Rn). In order to obtain more regularity of the weak solution we need another interpolation inequality. For our r > N and 0 < A ~ 1 - N/r we have the continuous embedding ~/](~) C CX(fi) and it holds for allue~)(flp) (l~r)
Ilullo,- < Ilull , II ll -° with 1/,- 1/p1/r+
A/N + 1IN ~ 0 ~ 1.
(20)
Especially we obtain by means of (17) and (19)
~[~"(.,t).- ~"(.,t’)l[o,~~ clt (1-°) - t’[
Vt, t’ e i
for some0 6 (0, 1), hence there is a ~ > 0 such that
Nowwe are ready to prove the final result. THEOREM 1 Let assumptions (i)-(v) and condition (12) be fulfilled. Then there a local weak solution u of problem(1)-(4) with additional regularity u ~ C~(f~v for some c~ > 0 and ut ~ Lp(~,Ls(f~)), s = Np/(N 2) A subsequence of the Rothe approximations converges to the solution u in the following sense,
as nk -~ ~ where q ~ [1,~),
A < 1 - N/r, u = ap/(a + 1).
PROOFThe compact embedding CZ(f~, × ]) C C~’(~, x/~) for 0 < a and the weak compactness of a bounded sequence in L~(~,~V~(f~)) imply from (21) and (19) the existence of a subsequence {~’~} (we write {fi’~} again choose subsubsequences below) with convergence properties (22~) and (23). standard arguments we see that the limits coincide. Convergenceproperty (23) for the sequence {~n~} follows from (19) with same limit u due to (18~). To prove the second part of convergence assertion (22) observe that {fi’~} bounded in W.~(Q$) due to (163) and (19~). By the.Rellich theorem there subsequence with fi~
--~ u in L~(Q~)
as n~ ~ ~. Let now be A < 1 - N/r. Then there is a 0x such that (20) holds with /~ = 2 for ~1 < 0 < 1. For fixed q > 2/(1 - 01) we then obtain ’![ II~,"~ (., t)- u(.,t)l[oq, a dt <_cshpess []~n~- uH~°,~f/lift ’’~- u[[~’-°)q d~,
275
QuasilinearParabolic-Elliptic Boundary ValueProblem
which yields convergence (22) if 0 is chbosen such that (1 O)q = 2. Theremaining convergence properties (24) and (25) follow from (16) under consideration of In order to prove that u is a weak solution we have to investigate the behaviour of g’~ and fro. as nk ~ c~. From (22) and (18) we obtain ~n~ -4 u in Lv(~, Ls(ft)) as nk -~ ~. Since s > p assumption (iv) yields fn~ ~ f(.,
",u)
in L~(Q~).
(26)
By application of the interpolation inequality (20) we obtain frown (172) and (193)
II~(.,t) - ~(’,t)ll0,~,~. ch,, ,
1-0
hence we have convergence of {~n~} to u in L~(], C(~)). Thus assmnption yields g.n~ ._+ g(., , u) in L~(Q~)which owing to (24) implies g’~ft~ ~ --~ g(., .,u)u,
in L~(],L~(~t))
(27)
Moreover, by an analogue argument like in the proof of Lemma1 we see from (16~) that u e Loo(i, Lp,~(.,t,,,)(~)). Finally, passing to the limit n = nk --~ c~ in relation (Rn) we obtain relation (R) due to convergence properties (23), (26), and (27), assuming first a more regular test function v. Initial condition (4) is fulfilled by construction and the uniform convergence on ~p × ~f. The usual density argument for the test functions concludes the proof. [] REMARK 1 Friedman and Schuss [2] prove uniqueness of a weak solution belonging to L~(QT) for the linear parabolic-elliptic problem. For our nonlinear problem (1)-(4) fulfilling assumption (i)-(v) we can prove uniqueness, too. Assume were two solutions u and u~, we define z := u- u~ and obtain from (R) with v = [z[P-~z for every fixed to ~ ~ (g(.,t,u)ut-g(’,t,u’)u’t,
IzlP-~z}dt
A(t)(z, Iz l’-~’z)dt
Then we consider
and insert (28) into the lastitem. The resulting inequality we estimate similarly as in the proof of Lemma2. Note that the nonlinear Gronwall inequMity used in that proof is no suitable tool to prove uniqueness since c~ > 0 in (14) is essential for its application. However,for given solutions ~ and u’ we mayreplace Ilu~ll and
276
Pluschke
[1~ g(’,t,u(’,t))ll.,m,
by constants, hence differently from Lemma2 now we have the total power p of z on the right-hand side and may use the well-known linear Gronwall lemma. Since the weak solution is unique the convergence assertions for the Rothe approximations in Theorem1 hold for the whole sequence. REMARK 2 The global assumptions (ii) for g w.r.t, u may be replaced by local assumptions supposed for all u E C(12p) with Ilu - U011o,n. _< R for some R :> 0. Then a truncation method yields a weak solution which is a solution of the original problem for small t since u is continuous on f~p x [0, 7~]. This generalization is not possible for f on f~e since we have no information whether Ilu(., t) -/)ollo,as witl small for small t. Weonly knowfi’om (23) that Ilu(., t)llo,n e is uniformly bounded, however the bound depends on the choosen R and may be much bigger than R even if the time intervall is small.
REFERENCES 1.
H.W. Alt and S. Luckhaus, Quasilinear Elliptic-Parabolic Differential Equations, Math. Z., 183:311-341 (1983). 2. A. Frie&nan and Z. Schuss, Degenerate evolution equations in Hilbert space, Transact. of the AMS, 161:401-427 (1971). 3. J. Ka~ur, Method of Rothe in Evolution Equations, B.G. Tcubner, Leipzig (1985). 4. O.A. Lady~enskaja, V. A. Solonnikov, and N. N. Ural’ceva, Linear and Quasilinear Equations o] Parabolic Type, AMS,Transl. Math. Monographs, Providence, R. I. (1968). 5. R. MacCamyand M. Suri, A time-dependent interface problem for twodimensional eddy currents, Quart. Appl. Math., ~: 675-690 (1987). 6. V. Pluschke, Rothe’s method for degenerate quasilinear parabolic equations, In: Z. Dogla, J. Kuben, and J. Vosmansk); (eds.), Equadiff 9 CD-ROM,pp. 247-254, Masaryk Univ., Brno (1998). 7. R.E. Showalter, Degenerate E~:olution Equations and Applications, Ind. Univ. Math. J., 23:655-677 (1974). 8. C. G. Simader, On Dirichlet’s Boundary Value Problem, Lecture Notes in Math. 268, Springer, Berlin--Heidelberg-New York (1972). 9. D. Willett and J. Wong,On the discrete analogues of some generalizations of Gronwall’s inequality. Monatsh. fiir Math., 69:362-367 (1965). 10. M. Zlfimal, Finite element solution of quasistationary nonlinear magnetic field, R.A.LR.O. Anal. Num., 16:161-191 (1982).
Singular Cluster Interactions in Few-Body Problems S. ALBEVERIO Institut fiir Angewandte Mathematik, Universit’~t Bonn, D-53115 Bonn; SFB 256; SFB 237; BiBoS; CERFIM(Locarno); Ace.Arch., USI (Mendrisio); Fakult/it fiir Mathematik, Ruhr-UniversitS~t Bochum,D-44780 Bochu~n. P. KURASOV Dept. of Math., Stockholm University, 10691 Stockholm, Sweden; Dept. of Math., Lule£ University, S-97187 Lule£, Sweden;St. Petersburg University, 198904 St. Petersburg, Russia.
1
INTRODUCTION
The present paper is devoted to the study of the few-body quantum mechanical problem with singular finite rank cluster interactions. The corresponding Hamiltonians play" an important role in mathematical physics, since few--body Hamiltonians with more regular interactions present considerable difficulties which make impossible a detailed analytic study [13]. Also a numerical study of such Hamiltonians using Faddeev equations present very hard problems, since the interaction between the particles does not vanish at large distances. On the other hand few-body problems with singular cluster interaction are useful and intensively studied in statistical physics, since the corresponding Hamiltonians can be analyzed in detail even if the number of particles is very large. Models describing one dimensional particles are of particular interest, since the eigenfunctions of the manybody Hamiltonians can often be calculated using Bethe Ansatz [14]. In fact the well-known YangBaxter equation was first written in connection with the study of system of several one-dimensional particles with pairwise delta interactions. Similar methods were used in atomic physics to study collisions of several part!cles [12] (in three dimensions). Few-body systems in applications are usually investigated by combining the classical description of the dynamics of heavy atoms with the quantum description of the dynamics of electrons and other light particles. The first attempt ~ to construct a three body Hamiltonian describing three quantum particles in R interacting through pairwise delta fnnctional potentials is due to G.V.Skorniakov and K.A.Ter-Martirosian [29]. R.A.Minlos and L.D.Faddcev proved that the corresponding Hamiltonian is not bounded from below and therefore cannot be used in ~7
278
Albever|o and Kurasov
the originally intended physical applications [24, 25]. The operator was defined using the method of self-adjoint perturbations used by F.A.Berezin and L.D.Faddeev for investigating Schbdinger operators with delta potential in R3 [10]. Almost three decades later semibounded three-body operators in dimension three with ge:aeralized two-body interactions were constructed by extending the standard Hilbert space of square integrable functions in R9 [17, 18, 19, 27,.30]. The most interesting model considered used the theory of generalized extensions suggested by B.Pavlov [7, 26]. Different aspects of these models were analyzed recently [8, 23, 20]. A general approach to these operators is described in [7, 22]. Let us mention that a realization of a many-bodylower bounded Hamiltonian with point interactions for particles in R3 has been obtained in the original Hilbert space by using the theory of Dirichlet forms [2]. The few-body systems of two dimensional particles with twobody interactions was studied in [11], where it was proven that the corresponding Hamiltonian is semibounded. It is stressed particularly in [7] that few-bodyHamiltonianswith delta interactions can be efficiently studied by using the theory of finite rank perturbations. Hamiltonians describing point interactions created at manycenters, e.g. of importance in solid state physics, have been discussed in [1]. Rank one for~n bounded interactions were analyzed in detail in an abstract setting by B.Simon and F.Gesztesy [15, 28]. Perturbations in terms of quadratic form were studied in [3]. In [16] rank one form unbounded interactions are defined following the paper by F.A.Berezin and L.D.Faddeev [10] and introducing a renormalization of the coupling constant. See also [4, 5], where these interactions are defined without renormalization of the coupling constant using a certain regularization procedure. It is not hard to extend this technique to obtain few-body operators with form bounded cluster interactions (see e.g. [7]), but operators with more singular interactions need a more detailed investigation. The present paper is devoted to the study of the few-body operator with one singular cluster interaction having finite rank. It is proven that this interaction in general is described by unbounded boundary operators. This operator can serve as an elementary brick in the construction of the few-body Hamiltonian with several singular cluster interactions. The paper is organized as follows. In Section 2 the few-body operator witb finite rank cluster interaction is heuristically defined. A precise definition of this operator is given in Section 3 by separating the center of mass motion and using the extension theory of operators with finite deficiency indices. To describe the analytic properties of these operators a study of rational transformations of Stieltjes functions is given in Section 4. The resolvent of the few-body operator is calculated in Section 5. The few-bodyoperator is described in Section 6 without separation of the center of mass motion. Then the extension theory for symmetric operators with infinite deficiency indices is used. The extension is described by certain bom.~daryconditions involving unbounded operators.
2
FEW-BODY OPERATOR WITH FINITE CLUSTER INTERACTION
RANK
The Schr6dinger operator describing several quantum mechanical particles is characterized by the following property: the original Hilbert space 7-/and the operator
279
Singular Cluster Interactions in Few-Body Problems possess several tensor decompositions n = l,2,...,N
7/ = K,~ ® Hn,
(1) A
= Bn ® IH,, + IK,, ® An;
where B,, and .4,, are positive self-adjoint operators acting in the Hilbert spaces Kn and H,~ respectively. The index n parameterizes the cluster decompositions and the number N of such decompositions is in general different from the number of particles. The operator An describes the motion of the particles forlning the corresponding cluster in the coordinate system associated with the center of mass of the cluster. The operator Bn describes the motion of all other particles in the same coordinate system. Each pair of operators (An, B~) appearing in the tensor decomposition determines the unperturbed operator ,4 uniquely, since it is essentially self-adjoint on the algebraic tensor product of the domains of the operators An and B,~. The few-body operator with singular finite rank interactions can heuristically be defined by N
.4°
:
d.
.4 n=l
+
(2)
j=l
where ~,~j are singular vectors defining the cluster interactions. In what follows we suppose that these vectors belong to the Hilbert spaces 7~-2(An) associated with the corresponding operators A,~ ~2~j E 7/-2(A,~), j = 1,2,...,dr,
n = 1,2,...,N.
The numbers dn E N determine the rank of the cluster interaction. The coupling constants anak form dn x dn Hermitian matrices. Then the perturbation term is formally symmetric. If the vectors ~2,,j do not belong to the spaces 7/-1(A,,) then the perturbation term is not form bounded with respect to the unperturbed operator. To determine the few-body operator in this case it is necessary to carry out a special analysis i.ncluding the extension theory for symmetric operators. The aim of the current paper is to describe few-body Hamiltonians with one cluster interaction. This is the first step towards the definition of general few-body Hamiltonian with finite rank cluster interactions. Let us consider the Hilbert space 7/ and the operator ,4 possessing the tensor decomposition 7/ = K ® H,
(3)
‘4 = B ® IH + IK ® A where B and A are positive self-adjoint operators in the Hilbert spaces K and H respectively. Consider d singular vectors from the Hilbert space 7/-2(A). The the few-body operator with single cluster interaction is heuristically described by d
‘4°=
(4) j,k=l
280
Albeverio and Kurasov
where the coupling constants ajk form an Hennitian matrix. If the vectors ~j are from the Hilbert space H, then the perturbation term is a bounded operator. The perturbed operator in this case has the same domain as the original operator A. The problem of defining the operator with cluster interactions is trivial in this case. Therefore we are going to concentrate our attention on the case of so-called H-independent vectors. d C DEFINITION2.1 The set of vectors (~J }j=l if and only if any nontrivial linear combination d
d
j=l
j=l
~-{-2
(,4)
is called H-independent
does not belong to the Hilbert space H. In what follows without loss of generality we suppose that the vectors form an orthonormal sct in 7-/_2(A), i.e.
=
(5)
H
Any set of independent vectors can be orthonormalized and the new set is independent also. In particular
e The Hermitian coupling matrix can be diagonalized using a certain orthogonal transformation. Therefore it is enough to consider only diagonal coupling matrices. Thus the following heuristic operator will be studied in this paper d
(6) j=l
where the vectors ~?j form an orthonormal subset of H_.~ and tim real coupling constants are different from zero,
(7)
% ~R, %¢0, j=l,2,...,d.
3
CLUSTER INTERACTION OF MASS MOTION
VIA
SEPARATION
OF THE CENTER
The operator ~l~ can be defined using the following formed decomposition d
B ® I~ + IK ® A + E ay((pj,
.)E~j
j----1
(8) =
B ® IH + IK ® A -1-
O~j((~Oj,
.)H(~j
Singular Cluster Interactions in Few-Body Problems
281
The operator d
As = ,4 + E aj(~j,
’}n~j
(9)
is a finite rank perturbation of the operator ,4 and it can easily be defined following [6]. To define the operator As we restrict first the operator A to the domain Dom(g °) = {¢ E Dom(A): (¢pj,¢)H = 0,j = 1,2,...,d}.
(10)
The restricted operator A° is symmetric and densely defined. The deficiency elements at point i are given by 1 A - i ~j’j = 1, 2,...
,d,
and form an orthonormal subset of the Hilbert space H. The intersection the deficiency subspace and the domainof the original operator is trivial
between
Ker (A°* :E i) ~ Dom(A) = {0}. Therefore the restricted operator is densely defined and has deficiency indices (d, d). The vectors W:-7~J form a basis in the deficiency subspace Ker (,4 0* - i) denoted by M, i.e. M= Ker (A°* - i). All self-adjoint extensions of the operator A° can be described using von Neumann formulas. But we prefer to define the extension using Krein’s resolvent formula. Essentially all extensions of the operator A° can be parameterized by an Hermitian operators ~/ acting in M in such a way that the resolvent of the corresponding self-adjoint operator A"~ is given by ~ 1 A+i 1 A-i - 1 .__, A’~ - z A - z A - z "~ + q(z) P~4 A where "Krein’s Q-operator" q can be chosen as follows q(z) = PM’-’~-~_ l+zA z M. q is a d x d ~natrix Nevanlinnafunction, i.e. its imaginary part is positive in the upper half plane "~z > 0. Our choice of q is determined by the normalization condition q(i) = JIM.
(12)
If all vectors ~,~- are from the space 7/_~ (A) then the relation betweenthe coupling parameters al, a~, ¯ ¯ ¯, ad and the Hermitian operator ~, is given by ")’
:
O~(-1)
+
PMAIM,
(13)
~The self-adjoint extensions that would not be described by this formula would have the following property: the operator A° is not the largest common symmetric restriction of the perturbed and unperturbed operators. But this implies that at least one of the coupling constants is equal to zero, which is impossible due to our assumption (7).
282
Albeverio and Kurasov
where a is the following coupling operator defined in M d j=l
The second term in (11) is well defined. In fact using the orthonormat basis in $4 we have APM
(14) H
II
since the deficiency subspace/14 is a subset of 7-/-1 (A). (Weremark that the scalar pr°ducts/ l,,Tf~-i~j, A,-4~-i~kl)H =---(~J’A--~°kl Hare welldefined.) In the case where some of the ~oj are not from 74_1(A) the operator 3‘ cannot be calculated from the coupling parameters without using additional assumptions. Only some partial information concerning the operator 3’ can be recovered. The formal expression (9) does not define a unique operator in this case, but a certain family of self-adjoint operators described by several parameters. The number of free real parameters can be different from d~ (the number of real parameters in yon Neumannformulas), since the operator 3‘ should satisfy some admissibility conditions if the vectors ~oj are not 74_l-independent. Supposethat a certain linear combination of the vectors ~oj belongs to the space 7/-1
¢
d
=
e
then the scalar product ¢, ~-V-~¢
aj
~C
is well defined. Therefore the operator H
necessarily satisfies the admissibility condition
aj~j, A~ + 1 j=l
’ k:l
H j,k=l
where 3‘i~¢ are the coefficients of the operator 3’ in the chosen orthonormal basis
The operators satisfying all admissibility conditions are called admissible. The family of admissible operators 3‘ was described in [6]. Ii~ in addition the operator A and all vectors ~j are homogeneouswith respect to a certain group of unitary transformations, then the operator "), could be determined uniquely by requiring additional natural homogeneity properties of the perturbed operator. This approach has been developed in [4, 5] for perturbations of rank one. In what follows we suppose that the extension of the operator A° is determined by a certain admissible Hermitian operator % which is compatible with the heuristic expression (9). This extension will be denoted by ~. In what f ollows t he operator
283
SingularCluster Interactions in Few-Body Problems
A~ will be substituted for the operator A~. The corresponding few-body operator with single cluster interaction is defined by A"~ ~. = B®IH +I~ ®A
(15)
The last formula determines the operator A~ uniquely, since ~ B ® Itl + IK ® A is essentially self-adjoint on the algebraic tensor product of the domains of the operators B and A~. Hence Dom(,4 7) : Dom(B) x Dom(A~).
(16)
In order to simplify our presentation let us restrict ourselves to the case of perturbations of rank one (d = 1). Weare going to drop the lower index of the coupling constant and singular vector
To calculate the resolvent of the operator A~ we need to study the properties of the Nevanlinna functions describing the interaction.
4
RATIONAL
TRANSFORMATIONS
OF STIELTJES
FUNCTIONS
Let us prove first some facts concerning Nevanlinna functions F which belong to the Stieltjes class, i.e. possess the representation F(z) =/; 1A_ + ZAdP(A)’
(17)
where the real measure p is finite f~ dp(A) LEMMA 4.1 Let F be a Stieltjes function. Then for any real y and any positive e > 0 there exists a certain b = b(y, e) > 0 such that the following estimate holds If(z ÷ iy)l < ~lxl
b
(18)
for all x < A. PROOFConsider the real and imaginary parts of the function F(x + iy) = /; l +~-Z-x--_-~y (z + iY))~ apta). .... The imaginary part ~F(x + iy) = y ; (A - A~+I x) 2 + y2 d0(A) is uniformly boundedfor all x < A. The real part is given by the sum of two integrals as follows: ~¢ f~ ~(1 - y~) -, i~)
L
284 The first follows
Albeverio and Kurasov integral
is uniformly bounded. The second integral
can be estimated as
( )2 for all x < A - 1. To estitnate J’~ dp(A) < e/2 and we get
the latter
f? %x-I_lap(a)
integral
f?ap(a)+l=l
<_ \-~:-~_x A~dp(A) C For all x function therefore lemma is
we choose C > ,4 such that
+
’x’.
_< Xo = C(1 - 71 f~ dp(A)) the last expression is estimated e[xI. The F(x + iy) is continuous on the bounded interval z0 < x < A and is uniformly bounded on this interval (which is empty if x0 > A). The proven. []
The following lemmadescribes rational transformations of Stieltjes LEMMA 4.2 Let F be a Stieltjes
functions.
function. Let a, b, c, d be real numbers such that ad - bc = 1.
(19)
Then there exists a real numberAt, such that for any real y and any positive e > 0 there exists b~ = b~(y, e.) such that the function G(z) aF(z) + b cF(z) +
(20)
possesses the representation a(z)=~z+g(z),
~
(21)
where
Ig(x+iY)I
(22)
for all x < A~. PROOFCondition (19) guarantees that the function G is a Nevanlinna fl~nction and possesses the representation ~ l+Az G(z) = (~ + ,Sz + ~ -A----~ dp~(A),
f_
where f-~o~ dpt(A) < ~, ~,/3 ~ R, /3 > 0. The support of the measure p~ coincides with the set of real points z where the boundary values G(z + iO) are not real or do not exist. The function G is real on the interval (-c~, A) outside the points where cF(z) + d = 0. The derivative ~ ~ + 1 dF(z) ~zz - (~---)~ 2 dp’ (A)
Singular Cluster Interactions in Few-Body Problems
285
is positive for all z < A. It follows that there exists at most one point where F(z) = - ~. Therefore the support of the measure p~ is bounded from below. Lemma 4.1 implies then estimate (22). The lemmais proven. Weremark that the constant/~ appearing in (22) is different fi’om zero only if the function F has a finite limit F(~) at infinity and F(oc)
5
KREIN’S
RESOLVENT
FORMULA
To calculate the resolvent of the operator A~ we will need the following corollary of the two previous Lemmas. LEMMA5.1 /unction
Let y be an arbitrary positive real number. Consider the Nevanlinna
=
1
1
-
I/~ E ~t-1 (A), then the/unction satisfies
~]H A-.~
A +1
¯
the estimate
IG(x + iy)[ <_ Cl(y)(1 + Izl)
(23)
/or all negative x < 0 and a certain C~(y) > O. I] ~ e 7t_~(A) \ ~t_~(A), then /unction can be estimated by
IG(x+i )l < .for all negative x < 0 and a certain positive C2(y) > PROOFThe function q is a Stieltjes function, since the operator A is positive. Lemma4.1 implies that the estimate (23) holds for all ~ ~ 7-/_:(A). Consider the case ~ ~ 7-/_~(A) \ 7/_~ (A). Weare going to prove that the real of q(x + iy) tends to minus infinity when x -~ -~c. In fact the function q can be presented by the following integral
where the measure p is finite, i.e. f~¢ alp(#) < oc, but the integral ~ diverges. The real part of q(x + iy) is given by ~q(x + iy) =~ (#--~:~,2x) - #Y
fo~ x#(p__-_ x_)_ d ,p ).
The first integral in the last formula is boundedfor negative values of x : c~ # -- X ~0o~ py2
~0
(25)
286
Albeverio and Kurasov
The second integral in (25) is negative and can be estimated x 2 /o ~ ,x,# dp(#) ~ ¯~o(~ x#(p_ x)2 +x)y’2 dp(#) >_ x 2 + y~ # - x _ > x ~ + y~ 2 ao #dp(#). The last integral tends to infinity when x -~ -~. It follows that lim G(x+iy)
1
li m
,~-~-~
.~-~-~~ - q(~+ i~)
-0.
Therefore the continuous function G(x + iy) is uniformly bounded on the interval x < 0, i.e. the estimate (24) holds. The lemmais proven. Weremark that if y = 0 then the esti~nates (23) and (24) hold for x ~ (-co, where .4~ is a certain real constant. THEOREM 5.1 The resolvent of the operator A~ = B ® IH + I~ ® A~ at a cert~ain point A, ~A ~ O, is given by the formula 1 _ 1 (A-A A~-A where
q(A-
1 A-
~ A +q(A
B) =(~,I+(A-B)@A A-A
The function
1 "l’--q(xTiy)
(26)
1 l~)h" A:+
COMMENT Let us discuss formula (26) first. f ~ 74 the following inclusion holds 1 (’-’~’~v,f)h
_ B)
Let ~ ~
74-1(a).
Then for any
1 V/~+ 1~ = ( ~V, -’~. -~ Jib 741(B).
satisfies the estimate (23) and it follows that the operator 1
-~ _ q(~ maps 741 (B) onto 74_~ (B). This implies
3’ - q(A - B)
¢P’f
®~ ~ 74_2(A).
(27)
This means that formula (26) defines a bounded operator in the Hilbert space
for ~ Consider now the case ~ ~ 74-2(A) \ 74_~(A). For any f ~ 74 the vector 1 1 The function (’-~L~,f)h (" A-TTtp,(A + i) ~_xf)H belongs to the spac e K. 1 "~-q(.~+iu)l is bounded fornegative x(see(24)) andtheoperator "r-q(a-B) is bounded in K. This implies that condition (27) holds. Therefore formula (26) defines boundedoperator acting in the Hilbert space for any q9 fi 74_~(A).
Singular Cluster Interactions in Few-Body Problems
287
PROOFof Theorem 5.1 Let us denote by YB the operator of spectrM transformation for B - the linear operator which maps the operator B into the operator of multiplication by the independent real variable x. Then the resolvent on a dense set can easily be calculated as follows 1
£
~ f = (W-~)¢ ~ (.TBf)(x)
=~¢
-
1 A--~
f
= (x "r - A)(~ ’stb)(x)
1(~ A-A \[7+q()~-B)
"
Wehave supposed that ¢ E £~, where £~ is an algebraic tensor product of Dora (B) and Dora (a~). The operator ~ i s e ssentially s elf-adjoint o n t his d omain and t his completes the proof of the theore~n. []
6
CLUSTER INTERACTION WITHOUT SEPARATION OF THE CENTER OF MASS MOTION
The resolvent of the operator .4 ~ has been calculated using the tensor decomposition. The operator A~ is a self-adjoint extension of the symmetric operator A° = B®I~ +I~:
°®A
with infinite deficiency indices. Consider the annulating set (I’~eg of regular functionals for the operator A° defined as follows: ¯
if
~ E
qr~_I(A) then
v~ = {~: ¯ = ~(~) ®v, ~(~) e ~_~(B)}, ¯
if ~ ~ ?/_~(A) \7/_~(A)
Let us consider the corresponding subspace of regular elements from the domain °~. of the adjoint operator .4
288
Albeverio and Kurasov
* if ~a E 7/_~(,4) then °*) = {’~b: $ ---’~ + A.A--~+~p(~b)®W,~ e Don,(A), p(~b) ~ ~h!_, Domreg(A
The boundary form of the adjoint operator calculated on the regular elements is given by 0.) =~ U, V ~ Domreg(A
(u, A°*v)- (‘4°*u,v) : (p(U)®~, 9) - (0, p(v)
(28)
A symmetric extension of the operator .40 can be defined in ter~ns of any symmetric operator F by restricting the operator .40, to the domain of flmctions from °*) satisfying the boundary condition Domreg(A
-(¢, ~2): rp(U).
(29)
In order to obtain the perturbed operator possessing the tensor decomposition (8) let us consider the symmetric operator .4r determined by the following boundary operator F=3,-B
%(.42+1)(A
~+1)~o
.
(30)
H
The operator (~o,(.A~+I)(A~+I)AA-1 V-’! ~u is a boundedself-adjoint operator in K commuting with the operator B. The norm of this operator is less than or equal to 1. Therefore the operator F is essentially self-adjoint on the domain Dom(B) the operator B. Weare going to keep the same notation F for the corresponding self-adjoint operator. Let us find an expression for the resolvent of the operator .4r. Consider an arbil trary f ~ 7/and suppose that .~b = ~ + ~f+a P0P) ® ~ = ~-v-~f. Then the fimction ’(,, satisfies the fbllowingequation + ~.4 (.4 - ~)V5 ~ A~ + ~ (P(~) ® ~) and the boundary conditions (29). Applying the resolvent of the original operator ‘4 to the previous equation we get ~_
I+AA 1 ‘4-A .42+1
p(¢)
1 ®~°- A-A f
I+AA 1 ~)~ p(¢) f)’" =-(~’)--251 ~ r+(~, 3i--~ ‘4~:~ )
(31)
This equation can be solved and tile function p(¢) can be calculated if the operator F+ (~o, ~ A 1---~+~ ~o)y is invertible. The operator can be simplified as follows taking
SingularCluster Interactions in Few-Body Problems
289
into account equality (30) hI+AA 1 19~)
r + (~, ~1:~ A" =’r-B
~,(A~+I)(A2+I)~
-
~,~--~A2-+~
h
=’r+
~,
t+(~-B)®A
(32) H
1 A2+l ~° H’
A-A
which holds on functions from DomB. Since ~ E ~_~(A) and the operators and B are positive the following inclusion holds (~,A~--~_~f)H ~ K. The comment after Theorem5.1 shows that the operator F + (~o, L+-~1--A--,~\,, is invertible A-A A2+I K. Therefore there exists p(’¢’) Dom (r) C K which sa tisfies eq uation (3 The component ~ of the function ¢ can be calculated using the formula 1
I+AA
A- >, A2 + i p(¢) ® Thus the function ¢ is given by
The resolvent of the operator operator A"r. This implies that been first defined only on the Thus the following theorem
Ar coincides with the resolvent of the self-adjoint the operator Mr is in fact self-adjoint even if it has regular elements. has been proven.
THEOREM 6.1 The operator .A r which is the restriction the set of regular elements
of the operator A°* to
A~ + 1 (P(¢) ® °*) ~o) ~ Dom~eg(A
(33)
satisfying the boundary condition
(~, ~)H= rp(¢)
(34)
is self-adjoint and its resolvent is given by
(35) for any A; 9A ~ O. COMMENT In the course of the proof of the previous theorem we have shown that the density p(¢) is an element from the domain of the operator F. It is possible prove that the restriction of the operator Ar to the domain of functions possessing
290
Albeverio and Kurasov
the representation (33), boundary conditions (34) and having p(¢) E Dom essentially self-adjoint. Suppose that ~o E 7/-1 (,4). Then the boundary conditions (34) can be simplified as follows. Consider the scalar product (~, C/H, where ¢ is any function fi’om the domain of the operator Ar. Then the following equalities hold
= -~/p(~b)+
=
+
~o,\(A~-i-~.~-SUF1
) +A2+---- ~ p®~o ~,
(36)
p(¢) h
=
+ c) p(¢),
where we have used the fact that the function ¢ satisfies boundary condition (34). Taking into account (13) the latter condition can be written
= p(¢). One can define the operator .Ar using this boundary condition, but this condition cannot be generalized to the case of 7-/-2 interactions, since the scalar product ~ does not necessarily define function from K in this case. (fl’ A’--~A+~ P ®(ill REFERENCES 1.
2. 3.
4. 5. 6. 7.
S.Albeverio, F.Gesztesy, R.Hoegh-Krohn, and H.Holden, Solvable pwblems in quantum mechanics, Springer, Berlin, 1988 (Russian edition, Mir, Moscow, 1990). S.Albeverio, R.Hoegh-Krohn: and L.Streit, Energy forms, Hamiltonians, and distorted Brownian paths, J. Math. Phys., 18:907-917, (1977). S.Albeverio and V.Koshmanenko,Singular rank one perturbations of selfadjoint operators and Krein theory of selfadjoint extensions, to appear in Potential Analysis. S.Albeverio and P.Kurasov, Rank one perturbations, approximations, and selfadjoint extensions, J.Funct.Anal., 148:152-169 (1997). S.Albeverio and P.Kurasov, Rank one perturbations of not semibonnded operators, Int. Eq. Oper. Theory, 27:379-400 (1997). S.Albeverio and P.Kurasov, Finite rank perturbations and distribution theory, Proc. Amer. Math. Soc., 127:1151-1161 (1999). S.Albeverio and P.Kurasov, ;~ingular perturbations of differential operators and exactly solvable SchrSdinger type operators, CambridgeUniv. Press, to appear in 1999.
Singular Cluster Interactions in Few-Body Problems 8. 9. 10. 11.
12. 13. 14. 15. 16. 17.
18.
19.
20. 21.
22. 23.
24. 25. 26. 27.
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S.Albeverio and K.Makarov, Attractors in a model related to the three body quantum problem, C.R.Acad. Sci. Paris Set. I Math., 323:693-698 (1996). S.Albeverio and K.Makarov, Nontrivia| attractors in a model related to the three-body quantum problem, Acta Appl. Math., 48:113--184 (1997). F.A.Berezin and L.D.Faddeev, Remark on the SchrSdinger equation with sin~ular potential, Dokl. Akad. NAUKSSSR, 137:1011-1014 (1961). G.F. Dell’Antonio, R.Figari and A.Teta, Hamiltonians for systems of N particles interacting through point interactions, Ann. Inst. H.Poincard, Phys. Theor., 60:253-290 (1994). Yu.N.Demkovand V.N.Ostrovsky, Zero-range Potentials and their Applications in Atomic Physics, Plenum, NewYork, 1988. L.D.Faddeev and S.P.Merkuriev, QuantumScattering theory for Several Particle Systems, Kluwer, Dordrecht, 1993. M.Gaudin, La Fonction d’onde de Bethe, Masson, 1983. F.Gesztesy and B.Simon, Rankone perturbations at infinite coupling, J.Funct. Anal., 128:245-252 (1995). A.Kiselev and B.Simon, Rank one perturbations with infinitesimal coupling, J. Funct. Anal., 130:345-356 (1995). Yu.A.Kuperin, K.A.Makarov, S.P.Merkuriev, A.K.Motovilov, and BoS.Pavlov, The quantumproblem of several particles with internal structure. I. The two-body problem, Theor. Mat. Fiz., 75:431-444, 1988. Yu.A.Kuperin, K.A.Makarov, S.P.Merkuriev, A.K.Motovilov, and B.S.Pavlov, The quantum problem of several particles with internal structure. II. The three-body problem, Theor. Mat. Fiz., 76:242-260, 1988. Yu.A.Kuperin, K.A.Makarov, S.P.Merkuriev, A.K.Motovilov, and B.S.Pavlov, Extended Hilbert space approach to few-body problems, J. Math. Phys., 31:1681-1690, 1990. P.Kurasov, Energy dependent boundary conditions and the few-body scattering problem, Rev. Math. Phys., 9:853-906 (1997). P.Kurasov and J.Boman, Finite rank singular perturbations and distributions with discontinuous test functions, Proc. Amer. Math. Soc., 126:1673-1683 (1998). P.Kurasov and B.Pavlov, Few-body Krein’s formula, to be published in Proc. of Krein’s conference, Birkhauser. K.Makarov, Semiboundedness of the energy operator of a system of three particles with paired interactions of (~-function type, Algebra i Analiz, 4:155171 (1992). R.A.Minlos and L.D.Faddeev, Commenton the problem of three particles with point interactions, Soviet Physics JEPT, 14:1315-1316 (1962). R.A.Minlos and L.D.Faddeev, On the point interaction for a three-particle system in quantum mechanics, Soviet Physics DokL, 6:1072-1074 (1962). B.S.Pavlov, The theory of extensions and explicitly solvable models, Uspekhi Mat. Nauk, 136:99-131 (1987). B.S.Pavlov, Boundary conditions on thin manifolds and the semiboundedness of the three-body SchrSdinger operator with point interactions, Mat. Sb. (N.S.), 136:163--177 (1988).
292 28.
29.
30.
Aibeverio and Kurasov B.Simon, Spectral analysis of rank one perturbations and applic.~tions, in Mathematical Quantum Theory. H. SchrSdinger Operators (Vancouver, BC, 1993), volume 8 of CRMProc. Lecture Notes, Pages 109-149, Amer. Math. Soc., Providence, RI, 1995. G.V.Skorniakov and K.A.Ter-Martirosian, Three body problem for short range forces. I. Scattering of low energy neutrons by deutrons, Soviet Phys. JEPT, 4:648-661 (1957). L.E.Thomas, Multiparticle Schr6dinger Hamiltonians with point interactions, Phys. Rev. D, 30:1233-1237 (1984).
Feynman and Wiener Path Integrals Representations of the Liouville Evolution I. ANTONIOU International Solvay Institutes for Physics and Chemistry, Brussels, Belgium / Department of Mathematics and Mechanics, MoscowState University, Moscow,Russia O. G. SMOLYANOV International Solvay Institutes for Physics and Chemistry, Brussels, Belgium / Department of Mathematics and Mechanics, MoscowState University, Moscow,Russia
Weshow that the Liouville equation for any Hamiltonian system can be identified with the SchrSdinger equation obtained by the SchrSdinger-Dirac quantization of some "extended" Hamiltonian system whose phase space is the product of two copies of the initial phase space and hence whose configuration space coincides with the initial phase space. This identification allows us to represent somesolutions of the Cauchy problem for the Liouville equation by Feynmanpath integrals [1] over trajectories in the phase space of the extended Hamiltonian systems. In turn such a representation gives a frame to investigate some models which allow us -- under suitable assumptions -- to develop the Fokker-Planck equation (= forward Kolmogorov’s equation) and the backward Kolmogorov equation and hence the Langevin’s equation (= stochastic Ito’s equation) describing physical Brownian motion as the Ornstein-Uhlenbeck process (see [2-5]). The Feynmanmeasure over a space of trajectories in the phase space (it is called also Hatniltonian, or symplectic, Feynmanmeasure) is defined to be a distribution having a given Fourier transform; the Feynmanintegral of a function is defined to be the value of the distribution on the function, assumed belonging to the domain of the distribution. In the paper the Feynmanintegrals are calculated as limits of suitable sequences of finite dimensional integrals. Besides we represent the Feynman integrals by integrals over the usual Wiener measure on the same space of trajectories. This new representation is used to obtain the representation of Feynman integrals by limits of sequences of finite dimensional integrals. Besides the representation by Wiener measure allows us to justify some limiting procedures which 293
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arise in the process of investigation of some models of nonequilibrium statistical mechanics. Any vector space is assumed to be a space over the field of real numbers, and any topological spaces are assumed to be Hausdorff ones. The terminology and notations of the theory of topological vector spaces are used without cornments. For any locally convex space (LCS) E the symbol E x denotes the space of all continuous linear functionals on E equipped with the topology for which (Ex) x coincides with E as a vector space. A map ~ ofa LCS Et into a LCS E2 is called smooth if it is continuous and Ghteau differentiable infinitely manytimes and if for any n ~ N and for any compact K C E~ the mapping (x, h~,..., hn) ~ f(n}(x)h~ ... K x E~ x .’. x E~ -~ E2 is continuous.
1
FEYNMAN INTEGRALS
OVER TRAJECTORIES
After some definitions which are used in a rigorous approach to the Feynmanmeasure, we will present a quite new result: a representation of a Feynmanintegral over trajectories in the phase space byan integral over Wiener measure. The assumptions, under which this result is obtained, are rather restrictive; nevertheless, they are satisfied just in the case of the integrals whicharise in the representation of the solutions of the Liouville equations. Let E be a LCSand, for x e E, g ~ E×, ~o~(x) = ig(’~’), If ~ -~ i s a LCS of some complex valued functions on E containing the functions {~ : g ~ Ex} ghen the Fourier transform of ’0 ~ ()c/~)x (the elements of ($c~)x will be (:ailed distributions on E) is defined by (~’~)(g) = r/(~oa). If the span of ~o~ x is dense in 3c~ then any Y/~-distribution can be reconstructed by its Fourier transform. Belowwe need not explicit definition of ~rE; so we usually will not rnention ~’E. If b is a quadratic functional on Ex, a ~ E and a ~ C, a ~ 0 then the Feynman a-measure on E with the correlation functional b and with the mean value a (or, shortly, with parameters (b,a,~)) is the distribution ~,~,~ on E, whose Fourier transform is defined by (reb,,~,o)(9) = exp((a/2)b(g) \ / REMARK 1 If a = -1 and b is positively definite then the Feynman measure gSb,a,a can be identified with the Gaussian (cylindrical) measure. REMARK 2 Let E = C[0,1]; then E× is the space of all Borel measures on [0,1]. Let further a = 0, a = i and b : E× --> 1R~ be defined by: b(~z) f rain(s, t)t/(ds)u(dt). Then Cb,~,~ is the "classical" Feymnanmeasure. Let
nowQbeaLCS,
P=Q× andE=QxP.
DEFINITION 1 [6) Hamiltonian Feynman measure on E, with the mean value a ~ Q, is the Feynmanmeasure on E with parameters (b, (a, 0), i), where b is defined by b((q, p)) = 2p(q). Nowwe start to define the most important for the paper example of the Feynman measure -- a sequential Feynmanmeasure. Let S be a finite-dimensional Euclidean space. A (Bochner) locally integrable function g on S taking values in a Banach
295
PathIntegrals Representations of Liouville Evolution space, is called integrable (over S) if for any ~o E 79(s) there exists f g( s)~o(ss)ds, s s -~ 0; then the limit depends only on ~(0) and, by the definition, f g(s)ds s lira f g(s)~(-cs)ds, where c2 E D(S), ~(0) = 1. If T is a Banachspace then for .---~0 S
t ~ (0, oc) the symbolCp([0, t], T) denotes the vector space of all right continuous functions on [0, t], taking values in T, whose distributional derivatives are Radon vector measures. We will define the sequential Feynman measure on the space 8~ = C~([0, t], E) (t > 0) assuming that E (= Q × P) is finite-dimensional. For any z ~ Q and for any finite family a of elements of [0, t], a = {0 = to < tl < ... < t,~(~)+~ t} , le t ~( z,a) be a s et of a ll functions ~ ~ & suchthat the projection of ~(t) onto Q is equal to z and, if k ~ {0, 1,..., re(a)}, the restriction ~ onto [t~, t~+~) is constant; let also d(a) max{(t~+~ - t~) :k = 0, 1,. .. ,re (a)}. DEFINITION2 For any z E Q the sequential Feynman measure ~ on $~ is the functional on the vector space of functions f on 3t for which the following limit exists: m(o’)
f...fexp (i k=o lim ~ E
d(o-)-~o
m(~) ~ Pk(q~:+~-- q~:)) dpdq f/~ ,.,J’~ exp(i k=0 where f~ is the function on the product of re(a) copies of E which is defined f~((q,,p~),...,(q~(~),p,~(~)))= f(g~), g~ e ~(z,~), 9~(t~) = (%,p~), dql dp~ ...dqm(~)dpm(~). For such functions f the entity ~z(f) is defined to equal to this limit and is denoted by f f(q,p)~(dqdp). PROPOSITION1 For any z ~ Q the sequential Hamiltonian Feymnan measure.
Feynman measure (I)z
Proof: Let us define the duality between £t and itself
=
is the
by
+
here ({q,{~), (r~q,rlp) e ~ = Q, x P~., where Q~ Cp([O,t],q), P~ = C~( [O,t],P) and integrals f{p(r)rfq(T)dr, f ~?p(r)~’q(r)dr are integrals, resp., of integrands and r~p with respect to the measures, which are distributional derivatives, resp., of rlq and {q. The latter integrals are defined in a natural way: the only difference with the usual definition is that the product of number-valued functions is now substituted by the paring of elements of P and Q (one can use also the so called Kolmogorov’s integral). Then the doruain of ~: contaius the set and direct calculations showthat the Fourier transform F ~2: of (I)-" is defined (F qh~)(~q, ~) = (~.b (~q, ~p)+i({p( t) -~(0) which just provesthat (~ is a Hamiltonian Feynman measure. The following theorem describes some connections between the sequential man measure and the Wiener measure.
Feyn-
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Let again dime < ec and let w be the standard Wiener measure on Cp([0, t],E x E). Let moreover gC be an analytical function on the complexification of ExE and g be its restriction to ExE; we assume also that Vx E E the function z ~ g(x,z) is linear and hence 9(x,z) = go(z)z [= (go(x))(z)] where, for any x ~ E, 9o(x) is a linear continuous functional on E. THEOREM 1 Let g~ be the analytical extension of g0 on the complexilication of E, let %be the complex-valued function on (£t x £t, w ~ w) which is defined by:
) where ~ is an entire function and f denotes the stochastic integral, and let % be integrable w.r.t, any z-shift (z ~ E) of the Wiener measure w. Then ¢~ belongs the domain of the sequential Feynmanmeasure 0~, for any z ~ E, and
0
P~OOF The la~er dhnen~ion~l ~nte~r~I~; under~ome~ufl,~ble clmn~eof v~r~ble~ ~heyc~ube transformed~ntoin~e~r~l~ which~reu~ed~n ~he de~ni~on of ~he ~eq~en~i~l Feynmm~ inCe~r~l. ~EMA~ 8 A ~infil~rs~emen~ c~n be form~l~edfor hffiui~e-dimen~on~l spaces E.
2
HAMILTONIAN SYSTEMS (A COORDINATE-FREE APPROACH)
Webriefly review soIne elements of infinite-ditnensional Hamiltonian mechanics. Our considerations do not depend on the dimension of the corresponding phase space. DEFINITION3 [7,8] A symplectic LCS is a pail" (E,I) where E is a LCS and I e L(Ex , E), + =-I . A hamiltonian sy stem is a c ol lection (E, I, 7 /) where (E, is a symplectic space and 7/ is a complex valued function on E which is called a Hamiltonian flmction. (7-/is usually assumed to be a smooth function; the space is called a phase space of the system.(E, I, 7/)). DEFINITION 4 If (E, I, 74) is a Hamiltonian system then Hamilton’s equation for
(E,~, 74) :’(t) = I(74’(f(t))) with respect to a function f of a real variable t, taking values in the phase space E. The equation for the observables g is the Liouville equation:
~’(t) = -{7/,~(t)}
(2)
PathIntegrals Representations of Liouville Evolution
297
where g is a fnnction, of the real parameter t, taking values in a space of complex valued functions defined on E and {., .} is the Poisson bracket which is defined for any two (Gfiteau differentiable) functions ~, ¢ onE, by {%¢}(x) ~o’(x)(I(¢’(x))); one can also define Poisson brackets for vector valued functions on E and hence one can define equations for vector valued first integrals. Let now E be a Hilbert space. For some distributions u on E one can define Poisson bracket {~,u} and {u,~2} by: {~,u} = -{u,(p}, {u,(p} being the distribution on E which is the derivative of u along the Hamiltonian vector field he : z ~ I((p’(x)), E -~ Thederi vative of a dis tr ibution u alo ngany vector field k is the distribution denoted by dku which is defined by the assumption that for any test function ~ one has, in natural notations, (u, dk~) = (dku, ~) where dk¢p is the derivative of ~ aloug the vector field k, defined by (dk(p)(x) = ~p’(x)k(x); of course in order to make this definition correct one need to assume that dkT belongs to the space of test functions. If moreoverdku = ~3"k" u, where ~"k is a multiplicator in the space of distributions then/3 ~ is called the logarithmic derivative of u along k (el. [9]). In particular if k is a constant vector field, k(x) = ko for any x E E and if both u and dkou are the usual (a-additive) measures on E then/3~o is r-almost everywhere defined function on E which is called the logarithmic derivative of u along k0. If kl, k2 E E and u has logarithmic derivatives along kl and along k~, then u has also a logarithmic derivative along any linear combination of kl and k~, and moreover the mapping [span{k1, k~} ~ k ~ fl" k e £~(u)] is linear. Let again u be a probability measure on E, let u have logarithmic derivative along any vector from a vector subspace E~ of E, E~ being in turn a Hilbert space w.r.t. its ownnorm and let k be a vector field on E (k : E ~ E) whose range is contained in El. Then, if tr k’(x) = for an y x ~ E,where U(x) is thederi vative of k "al ong E~" and the trace is calculated w.r.t. E~, then ~3~exists iff the trace of the random linear operator k ® .B.~ (in E~) exists (a randomlinear operator in E~ is defined be a linear mappingof E~ into the space of E~- valued randomvariables on (E, u)); ~ in this case ~3~ k = tr k ®/3. (see [9]). If the vector field k is Hamiltonianttien tr k’ = 0 (if it exists). Underall these assumptions {u, ~o} =/37~, ¯ u = tr ((I~’) ® ~3")u. The Liouville equation with respect to distributions, is adjoint of (2): ¯ ’(t) = {7-/, ~(t)}
(3)
where ~ is a function of the real variable, taking values in a space of distributions on E and {., .} is the Poisson bracket of 7-/and ~(t). EXAMPLE 1 The system of equations (2) and (3) is the Ha~nilton equation the Hamiltonian systern (~, I~, 7-/e). Here £ is the product of a LCSE(E) consisting of some complex functions on E, and a LCS S(E) of some distributions on E, Ig is the multiplication on i (=v/-L~) and 7{g(~, u) = -iu({7-/, ~}). The statement this exampleis also a corollary to the followiug observation. THEOREM 2 The equation for first integrals Liouville equation for any Hamiltonian system is the Schrbdinger equation which is obtained by the SchrbdingerDirac quantization of the Hamiltonian system (EL, IL,’tlL) where EL = QL × PL , QL = E, PL = E’, IL(p,q) = (q,--p), 7-tL(q,p) = -’H’(q)Ip.
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Antoniouand Smolyanov
PROOFThe SchrSdinger equation obtained by the quantization nian system (EL, IL, 7/n), has the following form
of the Hamilto-
.Of z-~-[ = iT/’(.)I(f(t)’(.) = i(~t,f(t)} but this is just the equation for first integrals for the Hamiltonian system.
3
FEYNMAN PATH
INTEGRAL
REPRESENTATIONS
In this section we formulate two theorems -- theorems 3 and 4 --- about such representations. Theorem3 gives the representation by integrals over the Wiener measure; Theorem 4 gives the representation by (Feynman) integrals over the Hamiltonian Fcynman measure. The proof of the Theorem 3 is based on Ito’s formula; the Theorem 4 can be deduced from the Theorem3 taking in account Theorem1. But actually the method to guess these theorems was quite opposite. On euristical level Theorem4 is implied by Theorem2 if one uses an euristical representation of solutions fbr SchrSdinger equations by Feynmanpath integrals over the phase space; after that one need to recognize in this representation just the sequential Feynmanintegral and after that one can use Theorem1 in order to get the (formal) statement of Theorem 3; after all that one need only to prove Theorem3 (using Ito’s formula). THEOREM 3 Let (E, I, 7/) be a Hamiltonian system with the finite dimensional phase space and let 74 and also ~? be restriction to E of some analytical fllnction defined on the complexification of E. Let, for any t ~ [0, to] and any z ~ E the function (Vl ,’b’2)~’--)’
¯
~(~Vl(~) ~ 1
I(d
1
exp {for 7/’ (z 1 l --~-~v,(r) -~v ~v~(r)))}~
~(r)).
~vl(t)(Z~
1
1
~V2(~))
be w-integrable. Then the Cauchy problem for the equation (2) with the initial data (0, ~) has a solution f on the segment [0, to] which is defined by l
.~ z + ~v~(t) PROOF
- ~v~(t)
l
__5~V~(T)).
)
i o(dv
It is quite similar to the proof of Ito-Feynman--Kacformula. Let
299
PathIntegrals Representations of Liouville Evolution ¯ I d(--~-~,iv,(T)
+ g’~v.2(~-))
Theu, due to Ito’s formula,
..)) --~( ~ --~v~ (t) + ~ v~v~( t) ) 1 v~(t) __~2x/~v;(t)).i ¢~(t)
+
47
+i)dt
l_~_d(v~(t ) + v/~v,~(t)).
’
47
similarly, 1
1
1 1
Proceeding similarly to [10] (see also [11], [12]) one can deduce from the latter identity that function f satisfies equation (2) and initial data (0,r/). THEOREM 4 Let assumption of Theorem 3 be satisfied and let f be the solution of the Cauchyproblem for the equation (2) with the initial data (0, ~).
l(t)(z)=f
--
~(q(t) )O"(dq
PROOFThis is the corollary to the theorems 3 and 1. REMARK 4 Some similar results to distributions.
4
ADDITIONAL
are. valid for Liouville
equations with respect
REMARKS
One can expect that the representations of the Liouville evolution by functional integrals can be as useful as well knownrepresentations of solutions for Schr6dinger equations, which now belong to the main tools in the quantum theory. Wewill list here ouly a couple of possible applications. One of them is of a pure methodological character: it allows us to obtain, for the Liouville evolution, the already known diagrmn technique. Somepossible applications to problems of nonequilibfium statistical mechanics are potentially more interesting. One of ideas in this direction can be formulated as follows. Using the functional integral representation for the Liouville evolution of a finite dimensional classical (sub)system and an (may be infinite dimensional) reservoir can integrate over degrees of freedom of the reservoir and pass to a limit under the functional integral. Then one can get just a functional integral representation for a solution of the (forward) Kolmogorov’s equation giving a Markovian approximation
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for the evolution of the subsystem. The Liouville equation itself is a nonstochastic forward Kolmogorov’s equation. Moreover, any Schr6dinger equation is the Hamiltonian e:quation for an appropriate classical Hamiltonian system (describing an infinite dimensional harmonic oscillator whosephase space is just the Hilbert space of the pure states of the quanturn system). On the other hand any mixed state of a quantum system ca~ be described by a probability on the Hilbert space of pure states of the system and the evolution of probability is precisely a Liouville evolution. Hence a Markovian approximation of the evolution of an open quantum system can be described by the Kolmogorov’s equations with respect to the functions or measures on the Hilbert space of states and these equations can be obtained from the equations for Liouville evolution by the above described method. Wemay extend this discussion to the quantum Liouville-von Neumannequation. Wethank Professor I. Prigogine for his interest and support. The financial support of the European Commission (DG XIII ESPRIT Project NTGONGS) and the Interuniversity Attraction Poles is gratefully acknowledged.
REFERENCES 1. O.G. Smolyanov, E.T. Shavgulidze. Functional integrals. MoscowUniv. Press, 1990. 2. I. Prigogine. Non-Equilibrium Statistical Mechanics. New-York--London.., Interscience Publishers, a Division of John Wiley and Sons, 1964. 3. R.J. Rubin. Momentum autocorrelation functions and energy transport in :harmoniccrystals with isotopic defects. Phys.Rev., V. 131, N’- 3, 1963, pp. 964---989. 4. H. Nakazawa. A statistical mechanical model of Brownian motion. Supplement of Progr.of Theoretical Physics, ~’-" 36, 1966, pp. 172-192. 5. E.L. Chang, R.M. Mazo and J.T. Hynes On the Fokker-Planck equation for the nonlinear chain. Molecular Physics, V. 28, 5’-~ 4, 1974, pp. 997-1004. 6. O.G. Smolyanov, M.O. Smolyanova. Transformations of Feynmanintegral under non-linear transformations of phase space. Theor.&Math.Phys,v.100, ~’-" 1, 1994, pp.3-12. 7. O.G. Smolyanov. Infinite dimensional pseudo-differential operators and Schroedinger quantization./Doklady Math., v. 263, N-* 3, 1982, pp. 558-562. 8. P. Chernofl’, J. Marsden. Infinite-dimensional Hamiltonian systems. Lect.Notes Math, V. 425, 1974. 9.. O.G. Smolyanov,H.v. Weizsaecker. Differential properties of measures. Infinite Dimensional Analysis, QuantumProbability and Related Topics, v. 2, B’-" 1, 1999. 10. B. Simon. Functional integrals in quantumphysics. Prinston University Press, 1979. 11. O.G. Smolyanov. Stochastic Schroedinger-Belavkin equation and corresponding Kobnogorovand Lindblad equations. Vestnik h’IGU, Moscow,.~’-0 4, set. 1, 1998, pp. 19-24. 12. S. Albeverio, V.N. Kolokol’tsov, O.G. Smolyanov. Continious quantum measurements: local and global approasches. Rev. in Math. Physics, vo].. 9, J~’-" 8, 1997, pp. 907-920.
Spectral Characterization of Mixing Evolutions in Classical Statistical Physics I. ANTONIOU International Solvay Institute for Physics and Chemistry, CP 231, ULBCampus Plaine, Bd. du Triomphe, 1050 Brussels, Belgium / Theoretische Natuurkunde, Free University of Brussels Z. SUCHANECKI International Solvay Institute for Physics and Chemistry, CP 231, ULBCampusPlaine, Bd. du Triomphe, 1050 Brussels, Belgium / Hugo Steinhaus Center and Institute of Mathematics, Wroclaw Technical University
1
INTRODUCTION
The decay of correlation functions, which is equivalent to mixing, qualifies physical systems approaching equilibrium and includes all types of chaotic behaviour. Although all ergodic properties have an equivalent description in terms of the spectra of the evolution operators in Hilbert space there is no necessary and sufficient spectral condition for mixing. The only sufficient condition knownis that of absolutely continuous spectrum which guarantees mixing from the Riemann-Lebesgue Theorem. The purpose of this work is to give the complete spectral characterization of mixing based on a recent characterization of decaying measures [1]. After a description of the ergodic hierarchy (in Section 2), we describe the ergodic properties in terms of the evolution operators (Section 3) and review their spectral manifestation (Section 4). The spectral characterization of mixing is obtained (Section 5) from identification of the decaying singular spectrum resulting from the decaying singular measures [1].
2
THE ERGODIC
HIERARCHY
OF DYNAMICAL
SYSTEMS
A classical dynamical system on the phase space f~ is described by the evolution group {St}, with t real for flows and integer for cascades. The phase space is 301
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Antoniouand Suchanecki
endowed with a a-algebra ~ of measurable subsets of ~ and a probabilit:¢ p. Usually p is the equilibrium measure, i.e. 5’, preserve the measure #: #(S;-:(A))
measure
= #(A), for all A @.
The evolution of dynamical systems can be classified according to different ergodic properties which correspond to various degrees of irregular behaviom. Let, us recall the most significant ergodic properties [2, 3, 4, 5]: (I) Ergodicity expresses the existence of only one equilibrium measure, which meansthat for any t there is no nontrivial St-invariant subset of l’l, i.e. if for some t and A ~ ~ S[-~(A) = A, #-a.e., then either p(A) = orp(A) = 1 . Ergodicity is equivalent to the condition lim T 1 j~0 T-~+oo~ #(S~-~(A)
t3B)dt=p(A)#(B),
for all
A,B 6 ~.
(II) Weakmixing is a stronger ergodic property and is expressed for cascades by the fact that for each A, B ~ ~ l,i~moo #(A th S-’~(B) ) = p(A)#(B) where J is a set of density zero, which may vary for different choices of A and B. Recall that a set J C IN has density zero if lira card[J~ {1,...,n)]
: O.
Weakmixing is equivalent to absolute Cesaro convergence, for discrete and continuous time t: T-~oolim ~1 ~r (III)
[#(S~~ (A) f~ B) - #(A)p(B)[dt Mixing is stronger and means that lim #(A t3 S~-~(u)) = #(A)#(B) for all A, B ~ ~ It is easy to show that weak mixing implies ergodicity and obviously mixing implies weak mixing. Fully chaotic systems are qualified by the even stronger Kolmogorovproperty. (IV) Kolmogorovsystems are qualified by the existence of a sub-a-algebra ~0 of ~, called K-subalgebr’a, such that for ~. = St(~o) we have (i)
~ C i~i~ , for s < t.
(ii)
o-(U ~) = @.
(iii)
O~ I~t = ~-~, the trivial
a-algebra.
MixingEvolutionsin ClassicalStatistical Physics 3
THE EVOLUTION
OPERATORS
303 AND ERGODIC
PROPERTIES
The ergodic properties of classical dynamical systems can be conveniently studied in the Hilbert space formulation of dynamics due to Koopman[6]. Weconsider the Hilbert space L2 = L2(f~,~,#) of square integrable functions on ft. The transformations St induce the Koopmanevolution operators Vt acting on the functions f ¯ L2 as follows: Vtf(w) = f(Stw), w¯ As St preserve the measure # the operators Vt are unitary. In the case of flows the selfadjoint generator of Vt is knownas the Liouville operator Vt
iL .= te
(1)
In the case of Hamiltonian flows the Liouville operator is given by the Poisson bracket associated with the Hamiltonian function H Lf = i{H,f}. The Liouville operator is the starting point of equilibriuln and non-equilibrium statistical physics [7, 8, 9]. The ergodic properties (I-IV) of classical dynamical systems can be described as properties of the corresponding Koopmanevolution operators Vt or as properties of the selfadjoint Liouville operator L in the case of continuous time. This approach allows us to study and classify in a unified way dynamical systems in terms of operator theory and functional analysis. The description of evolution in terms of the Koopmanoperators Vt over L2 does not imply any loss of information about the underlying dynamics St. This was established by the converse to Koopman’s Lemma[10] which is an extension of the Banach-Lamperti theory of implementation of isometrics. In fact a positivity preserving group of evolution operators Vt on L~, Vtf >_ O, if f >_ 0, is implmnented by a unique measure preserving point transformations St of f~, i.e. Vtf(w) can be written as f(Stw). The ergodic properties (I-IV) can be expressed as properties of the corresponding evolution operators as follows: (I)
{St} is ergodic if and only if {I~f} is Cesaro convergent, i.e. r
lim 1 T--~c~ (II)
j£0 ~ fi4(g)
{St} is weakmixing if and only if {Vtf} is absolute Cesaro convergent, i.e. lim lf0r
(III)
dt = 0
IfVt(g)ldt =
{St} is mixing if and only if {Vtf} converges weakly in L2, i.e. lim (f, Vtg) =
for any two functions f, g ¯ L2 such that fn f d# = Ji~ g d# = 0.
304 (IV)
Antoniouand iSuchanecki The K-property can be described in terms of 1,~ in a similar way as for transformations St. Putting 74t d--fL2(a,~t,#)
O {1} and 7-/a=~L2(f~,~,#)
we have the analog of conditions (i)-(iii) (i’) (ii’)
characterizing K-flows
1/~(7/0) D Vt(7/0), for s lin( U 7/t) = 7-/(--denotes the closure) tEIR
(iii’)
N 7/t = {0}.
tEIR
Can we express the ergodic properties in terms of the spectra of Kooptnan operators?
4
SPECTRAL
MANIFESTATION
OF ERGODIC
PROPERTIES
The spectrum of the evolution group Vt, t ~ IR, corresponding to a flow is the spectrum of the selfadjoint generator L (1). The spectrum of the evolution group 1/’~, n ~ ~, is the spectrum of the unitary Koopmanoperator V = V:~ . The Caley transform relates naturally the spectra of unitary and selfadjoint operators [11]. The spectrum of an arbitrary dynmnical system may contain, like the spectrum of an arbitrary selfadjoint or unitary operator, any of the three components, namely discrete, absolutely continuous and singular spectrum [12]. Weassume below the knownfacts from the spectral theory of dynamical systems in the Hilbert space of square integrable functions [3]. (I) Ergodicity of a dynamical system amounts to imposing additional conditions on the discrete part of the spectrum. Namely a dynamical system with continuous time is ergodic if and only if 0 is a simple eigenvalue of L. In the case of discrete time ergodicity means that 1 is a si~nple eigenvalue of V. Ergodic dynamical systems may have, of course, eigeni~alues other than 1. However, as we shall see soon, the spectral characterization of properties stronger than ergodicity involves only the continuous part of the spectrum of a dynamical system. (II) It is therefore interesting to knowwhat are the dynamical systems which not have, apart fi’om 1, other eigenvalues. In other words, what ergodic property characterizes the dynamical systems which restricted to the Hilbert space 7/= have continuous spectrum. It turns out that the class of dynamical systems with continuous spectra coincides with the weakly mixing systems [2, 3]. (III) Since mixing systems are weakly mixing, a necessary condition for mixing is that the dynamical group {Vt} has purely continuous spectrum on 7/. This condition is, however, not sufficient. There are exa~nples of weakly mixing systems which are not mixing [4]. On the other hand, if the group {V~} has absolutely continuous spectrum then, applying the Riernann-Lebesgue lemma, it is easy to see that the’dynamical system corresponding to {Vt} is mixing. Therefore the class of dynamical syste~ns with absolutely continuous spectrum is a proper subclass of mixing systems. For an examplethat the converse inclusion is not true see [13]. (IV) The class of K-systems is in turn a proper subclass of dynamical systems with absolutely continuous spectrum. This is a consequence of the Weyl - von
MixingEvolutionsin ClassicalStatistical Physics
305
Neumanntheorem on the canonical commutation relations [5] group {V~.} of unitary operators satisfies properties (i’)--(iii’) has a homogeneous Lebesgue spectrum [5]. Weremark here homogeneousLebesgue spectrum are equivalently characterized a time operator canonically conjugate to Vt [14, 15]:
which says that a if and only if that systems with by the existence of
I/~tTV~ T + tI. On the basis of time operators Misra, Prigogine and Courbage [14, 15] elaborated a rigorous theory of irreversibility. In order to complete the spectral characterization of dynamical systems we must identify the necessary and sufficient conditions for mixing.
5
SPECTRAL
CHARACTERIZATION
OF MIXING
A necessary and sufficient condition for mixing is that the autocorrelation functions decay [4, 5].
/
nfV~fd#~O
for
eachfET/=L
2@1,
(2)
It follows from the above considerations that amongthe above mentioned ergodic properties only mixing does not have a satisfactory spectral characterization as we don’t knowthe necessary and sufficient spectral properties of the evolution operators for mixing. On the other hand, the property of mixing is very i~nportant in physics because not only mixing systems approach equilibrium in classical and quantum systems, but also because the decay of unstable quantum systems is a property of mixing systems. As there exist dynamical systems with continuous spectrum which are not mixing and as all dynamical systems with absolutely continuous spectrum are mixing the natural questions arises: Which property of continuous spectrurn characterizes precisely 1nixing systems? What is the spectrum of mixing systems? Consider, an abstract unitary group Vt = e itL acting on a Hilbert space 74, generated by the selfadjoint operator L with spectral family {Ex}: L =
)~dEx.
Denoteby 74p the closed linear hull of all eigenvectors of L. The continuous subspace of L is the orthocomplement of 74p: 74c = 74 ~ 74,. Recall that the singular continuous subspace 74sc of 74c consists of all f E 74c for which there exists a Borel set Bo of Lebesgue measure zero such that f~o dE)~f = f. By 74a¢ = Hc O 74sc we shall denote the absolutely continuous subspace of 74c. Recall also that 74p, 74¢, 74~ and 74~¢ are closed linear subspaces of 74 which reduce the operator L and that 74 = 74, @74a¢ @74sc. The spectra of the corresponding reductions of L will be called respectively point, continuous, singular continuous and absolutely continuous spectrum of L, and will be denoted by a,(L), ae(L), a~¢(L) and a~¢(L) correspondingly [16]. Let # = #t, denotes, for a given h ~ 74, the spectral measure on a(L) determined by the nondecreasing function Fh(A)=(h,
Exh),
for
AeIR.
306
Antoniouand Suchanecki
Let h = hp + hac + hsc be the decomposition of h correspouding to the direct sum 7/p c~ 7/ac ® 7/sc. Putting lip = Php, ~ac : ~th,¢ and #so = tths¢ we obtain the Jordan decomposition of # # = #p + #so + #ac (3) onto the point, singular continuous and absolutely continuous component. Conversely, given any three finite Borel measuresI~p,/-tac and l-tsc, where p, is concentrated on a countable set of points, and the other two measures are respectively singular and absolutely continuous, one can always construct a Hilbert space 7/and a selfadjoint operator L such that these measures are spectral measures associated with some h ~ 7/. Moreover, the point, singular and absolutely continuous spectrum of L coincides with #p, #so and #ac respectively. This can be proved by taking as 7/the direct sum L2(IR, #p) @L2(]R,/Zac) (~ L2(]R,/Zsc) and as L the operator multiplication by A [16]. It has been shownrecently [1] by S. Shkarin and one of us (I.A.) that the Jordan decomposition (3) of a a-additive measure can be further refined. Nmnely the Banach space Mof a-additive finite complex-valued measures on the real line IR is the direct sum of two linear closed subspaces MD and j~ND, where MD is the set ND of measures p ~ 3/I whose Fourier transform converges to 0 at infinity and 3d is the set of measures # ~ M such that t, ¢ MD for any v ~ ~ \ {0} absolutely continuous with respect, to the variation I#l of #. The corresponding decomposition /.t
= /~D -Jr pND
concerns in fact the singular continuous component in the Jordan decomposition since, obviously, each absolutely continuous componentdecays and the discrete does not. This result can be applied directly to obtain analogous refinement of the spectral decomposition of L or, equivalently, the group {Vt}. Let us call, following the property (2), decaying elements those elements h ~ 7/which satisfy (h,t~h)~0,
ast~.
and denote by 7/~ the set of all decaying ele~nents in the singular continuous subspace 7/~. The space 7/~ consists of all vectors tt ~ 7/~ such that the corresponding measure # = #h is singular with respect to the Lebesgue measure and its Fourier transform is 0 in infinity. 7/sDc is a closed linear subspace of 7/s¢.. Indeed, it is obvious that multiplication by scalars does not lead outside 7/~. Let h~,h~ ~ 7/~ and denote by #l and #2 the corresponding spectral measures. It follows from the inequality: Fh(A) = (E~,(h~ h2), hi + h~) ~ = IJE~hl -4-E)~h2[I
2 +~ NIIExh~+ E.xh~ll [IE~h~- E~h.~ll = 2 (llE~,h,II2 e) + liE,,hell = 2(Fh,(~) Fh=(~))
307
MixingEvolutionsin ClassicalStatistical Physics
that the measure #h is absolutely continuous with respect to both pl and tt2. There¯fore applying [1] Lemma 2 (see also [17] XII, Th. 10.9), we see that h e ~sDc The space 7{sDcis also closed. For, if {hn} E 7{s~, h~ ~ h in the n-norm, then for each Borel set A C ~
:
~,~(.4)
Therefore ~ converges weakly to ~ ([11] IV 9.3, Th.5). Since M~¢is a closed subspace of the Banach space ~ [1] it is also weakly closed. Therefore p ~ ~. Weshall show now that L does not lead out of the space H~ [16], i.e.:
where D(L) is the domain of L. Indeed, if h ~ D(L) then 2 = ~Lh]~ < On the other hand, the spectral me~ure ~Lh is determined by the function fLh(l)
= (Lh, ExLh)
A’2d(h, Ex, h).
Therefore eitXdFLh(A)
ei~A~dFh(A)
and applying [1], Lemma2, once again we see that Lh e ~. Following the notation of [1] let ~ be the space of all h e Hsc such that any measure u ¢ 0 which is absolutely continuous with respect to ~h does not decay. The space H~D will be called the space of non decaying singular elements. Weshall show that H~~ is also L invariant. Let h ~ ~c~ be in the domain of L and let Ph be the corresponding spectral measure. If Lh ~ ~):D then there is a component u of the measure ~Lh sucH that its Fourier transform ~(t) tends to 0 if t ~ ~. By [1] Th.1 u is just the restriction of ~ch to some Borel set A = A(h). Thus ~(t)
eitXlA(t)A~dph(t).
Note that the function ~-~ is integrable with respect to the measure u since A-~ du(A) =
A-~IA(5)a ~ dph(a) = ph(A).
Therefore ([1] Lemma2) ’[’~eita~
-~du(~)~0,
as
t~.
This leads to contradiction because the latter integral is the Fourier transform of the measure Ph restricted to the set A and, by the assumption on h, any measure which is absolutely continuous with respect to ~h cannot decay.
308
Antoniouand Suchanecki
It can also be shown[lS] that both spaces 71sDc and 71sNcD reduce the operator L [16] and that we have the direct sum decomposition 7-/sc = 71~ @7/~cD. This leads to the following direct sum deco~nposition of the whole space 71: 71 = 71. ¯ ~ ¯ 71~ ¯ ~.
(4)
Therefore denoting the corresponding spectra of reduced operators by a~,, and tisNc D respectively we obtain a new decomposition of the spectrum a of any selfadjoint operator which is the missing necessary fact to describe mixing and decay: ti = tip U O’ac U ti~.
U ti~O.
Weare therefore led to the following definitions: "HD = 7-/a¢ ~ 71sDcthe space of decaying ele~nents with respect to "]_/ND
~__. ~.~p
~ "~./sNc D the
space of non-decayingelementswith respect to Vt
o’D : tiac U O’sDcthe decay spectrum of L or Vt O"ND : tip
U
ti~D the non-decay spectrum of L or 1~
and to the following spectral characterization of mixing: THEOREM 1 A dynamical system is mixing if and only if the evolution {Vt}tem on 7t = L~ ~ {1} has purely decaying spectrum, i.e. a(L) :
tiD = .O.ac U tisDc
g~vup
(5)
Proof: As we mentioned in the beginning of this section the necessary and sufficient condition for mixing is that for each h ~ 7{ equality (2) holds. This however means that in the decomposition (4) of 71 consist only of the component71D 71ac This is equivalent that the spectrum of the dynamical system is of the form (5).
6
CONCLUDING
REMARKS
1. Weprovide here the complete spectral characterization I
of dynamical systems
Ergodicity: a(L) ap(L) U ac(L), 0 ~ ti p(L), 0 has multiplicity 1,
~.
II
Weakmixing: a(L) = ap(L) U ac(L), ap(L) = {0}, 0 has multiplicity a(L) = ac(L) on 7/.
III
Mixing: ti(L) = ap(n) U aD(L) = ap(L) a~(L) U aa~(L), ti p(L) = {0 has multiplicity 1 or ti(L) ti P(L) on7-/ Absolutely continuous spectrum: a(L) = tip(L)U ate(L), multiplicity 1 or ~r(L) = aac(L) on
IV
ap(L) = {0}, 0 has
K-systems: ti(L) = tip(L)UO’ac(L), tip(L) = {0}, 0 has mnltiplicity 1, tiac(L) has uniform multiplicity or a(L) = tiac(L) with unifbrm multiplicity on "H.
309
MixingEvolutionsin ClassicalStatistical Physics
2. Although the spectra of the Koopmanoperators in Hilbert space characterize the different ergodic properties mathematically, they do not give any information about the decay rates of autocorrelation functions, i.e. how fast a mixing system goes to equilibrium. This information is however essential for physical and engineering problems. The Brussels-Austin groups have shownrecently [19, 20, 21] that the rates of approach to equilibrium appear as resonance eigenvalues in extended spectral decomposition of the Koopmanoperator in rigged Hilbert spaces beyond the Hilbert space of square integrable phase functions. In fact these resonances determine the natural physical equivalence of dynamical systems [22, 23]. 3. The result of Section 4 allows to provide a spectral characterization of quantum mixing states which decay. The wave functions ¢ are elements of a separable Hilbert space 7{ evolving under the unitary solution Ut, t E lR, of the Schroedinger equation Ot¢=-iH¢,
t~=
l,
Vt = e -iHt ¯ If {E~} is the spectral family of H we have H = f wdE~ Ja (H) I"
e-~’~ dE,~. Ut = [ J~ (H) The survival amplitude of the pure state ¢ evolving under the unitary group Ut is : I~,Ut%b) : ~ H e-iWtd{%b,E~%b ( Therefore ~p is decaying if and only if ¢ is in the decaying subspace ~D of the Hmniltonian H
A more genera] discussion involving the spectra of the L]ouvflle-von Neumann erator Lf : [H, f] in the Hilbert-Schmidt space [24, 25] will be presented elsewhere 4. The distribution of the support of the spectral measures of the evolution operators provide another characterization of mixing and decay. This result will be presented elsewhere. ACKNOWLEDGMENTS We thank Professor I. Prigogine for his interest and support and S. Shkarin for discussions. This work enjoyed the financial support of the European Commission through the ESPRIT PROJECT NTCONGSDG XIII and the Belgian Governmentthrough the Interuniversity Attraction Poles.
310
Antoniouand Suchanecki
REFERENCES 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. 11. 12. 13.
14. 15. 16. 17. 18. 19. 20.
21.
22. 23. 24. 25.
I. Antoniou and S.A. Shkarin, Decaying measures Math. Docl. (accepted). P.R. Hahnos Lectures on Ergodic Theory, Chelsea Publishing Company, New York 1956. V.I. Arnold and A. Avez Ergodic Problems of Classical Mechanics, Benjanfin, NewYork 1968. W. Parry Topics in Ergodic Theory, Cambridge University Press 1981. I. Cornfeld, S. Fomin and Ya. Sinai Ergodic Theory, Springer-Verlag, Berlin 1982. B. Koopman, Hamiltonian systems and transformations in Hilbert spaces, Proc. Nat. Acad. Sci. USA 17 315-318 (1931). R. Balescu Equilibrium and Non-equilibrium Statistical Mechanics, Wiley, New York 1975. I. Prigogine Non-Equilibrium Statistical Mechanics, Wiley, NewYork 1962. I. Prigogine From Being to Becoming, Freeman, NewYork 1980. K. Goodrich, K. Gustafson and B. Misra, On converse to Koopman’s lemma, Physica 102A 379-388 (1980). N. Dunford and J. Schwartz Linear Operators I : General Theory, Wiley, New York 1988. N.I. Akhiezer and I.M. GlazmanTheory of Linear Operators in Hilbert Space, Vol. I and II, Pitman Publishing Limited 1981. N. Wiener and E.J. Akutowicz, The definition and ergodic properties of the stochastic adjoint of a unitary transformation, Re’ud. Circ. Mat. Palermo (2) 6 205-217 (1957). B. Misra, I. Prigogine and M. Courbage, From deterministic dynamics to probabilistic descriptions, Physica 98 A 1-26 (1979). S. Goldstein, B. Misra and M. Courbage, On intrinsic randomness of dynamical systems, J. Star. Phys. 25 111-126 (1981). H. WeidmannLinear Operators in’Hilbert space, Springer Verlag 1980. A. Zygmund,Trigonometric Series Vol. I,II, Cambridge, University Press 1968. I. Antoniou, S. Shkarin and Z. Suchanecki, Decay spectrum and decaying subspaces, (to appear). I. Antoniou and S. Tasaki, Generalized spectral decomposition of mixing dynamical systems, Int. J. QuantumChemistry 46 425-474 (1993). I. Antoniou, L. Dmitrieva, Yu. Kuperin and Yu. Melnikov, Resonances and the extension of dynamics to rigged Hilbert spaces, Computers Math. Applic. 34 399-425 (1997). I. Antoniou and Z. Suchanecki, Extension of the dynamics of unstable systems, Infinite Dimensional Analysis, QuantumProbability and Rel. Topics 1 127-165 (1998). I. Antoniou and Bi Qiao, Spectral decomposition of the tent maps attd the isomorphism of dynamical systems, Physics Letters A 215 280-290 (1996). I. Antoniou, V. Sadovnichii and S. Schkarin, Newextended spectral decomposition of the Renyi map, Phys. Left. A (1999) (submitted). I. Antoniou, M. Gadella and Z. Suchanecki, General properties of the Liouville operator, Int. J. Theor. Phys. 37 1641-1654 (1998). I. Antoniou, S. Shkarin and Z. Suchanecki, The spectrum of the Liouville-von Neumannoperator in the Hilbert space J. Math. Phys. (in press).
On Stochastic SchrSdinger Equation as a Dirac Boundary-Value Problem, and an Inductive Stochastic Limit V. P. BELAVKIN School of Mathematics, Nottingham University, E-mail address: vpb©maths, nott. ac. uk
NG7 2RD, UK,
Dedicated to Sergio Albeverio.
ABSTRACT ~Ve prove that a single-jump quantum stochastic unitary evolution is equivalent to a Dirac boundary value problem on the half line in one extra dimension. It is shownthat this exactly solvable modelcan be obtained from a Schr6dinger boundaryvalue problemfor a positive relativistic Hamiltonianin the half-line as the inductive ultrarelativistic limit, correspondent to the input flow of Dirac particles with asymptotically infinite momenta. Thus the problem of stochastic approximation is reduced to the to the quantum-mechanical boundary value problem in the extra dimension. The question of microscopic time reversibility is also studied for this paper.
1
INTRODUCTION
The stochastic evolution models in a Hilbert space have recently found interesting applications in quantum measurementtheory, see for example the review paper [1]. In this paper we are going to show on a simple example that classical discontinuous stochastics can be derived fi’om a quantum continuous deterministic conscrvative dynamics starting from a pure quantum state. It has been already proved in [2] that the piecewise continuous stochastic unitary evolution driven by a quantum This work was supported by Royal Society research grant GR/M66196.
grant
311
for UK-Japan collaboration
and EPSRC
312
Belavkin
Poisson process is equivalent to a tilne-dependent singular Hamiltonian SchrSdinger problem, and the continuous stochastic unitary evolution driven by a quantum Wiener process can be obtained as the solution of this problem at a central limit. Here we want to start form a non-singular time-independent dynamics. There exits a broad literature on the stochastic limit in quantumphysics in which quantumstochastics is derived from a nonsingular interaction representation of the Schr6dinger initial value problem for a quantum field by rcscaling the time and space as suggested in [3]. Our intention is rather different: instead of rescaling the interaction potentials we treat the singular interactions rigorously as the boundary conditions, and obtain the stochastic limit as an ultrarelativistic limit of the corresponding Schr6dinger boundary value problem in a Hilbert space of infinite number of particles. Weshall prove that the discontinuous and continuous quantum stochastic evolutions can be obtain in this way from a physically meaningful time continuous (in strong sense) unitary evolution by solving a boundary value problem with an initial pure state in the extended Hilbert space. First we shall describe the boundary value problem corresponding to the singlepoint discontinuous stochastic evolution and demonstrate the ultrarelativistic li~nit in this case. Then the piece-wise continuous stochastic evolution and the continuous diffusive and quantumstochastic evolution can be obtained as in [2, 4]. But before to perform this program, let us describe the unitary toy model giving an "unphysical" solution of this problem corresponding to the free hamiltonian h (p) = -p. This toy model in the second quantization framework was suggested for the derivation of quantum time-continuous measurement process in [5]. Recently Chebotarev [6] has shown that the secondary quantized time-continuous toy Hamiltonian model in Fock space with a discontinuity condition is equivalent to the Hudson-Parthasarathy (HP) quantum stochastic evolution model [7] in the case of commuting operatorvalued coefficients of the HP-equation. Our approach is free from the commutativity restriction for the coefficients, and we deal with time-reversible Dirac Hamiltonian and the boundary rather than physically meaningless discontimfity condition and time irreversible -p. Moreover, we shall prove that the stochastic model can be obtained from a positive relativistic Hamiltonian as an inductive ultra relativistic limit on a union of Hardy class Hilbert spaces. Wecall this limit the inductive stochastic approximation.
2
A TOY HAMILTONIAN
MODEL
Here we demonstrate on a toy model howthe time-dependent single-point stochastic Hamiltonian problem can be treated as an interaction representation of a self-adjoint boundary-value Schr6dinger problem for a strongly-continuous unitary group evolution. Let 7/be a Hilbert space, H be a bounded from below selfadjoint operator, and S be a unitary operator in 74, not necessarily commuting with H. The operator H called Hamiltonian, is the generator for the conservative evolution of a quantum system, described by the Schr6dinger equation ihOt~I = H~h and the operator S (:ailed scattering, describes the unitary quantuna .jump r/~-~ S’q of the state vectors r/ff 7/caused by a singular potential interaction in the system, with the continuous unitary evolution r/~-~ e-~;t~’r~ whenthere is no jump. As for an exaluple of such
Stochastic Equationas a Dirac Boundary-Value Problem
313
junlp we carl refer to the vou Neumannsingular Halniltonian model for indirect instantaneous measurement of a quantum particle position x E I~ via tile registration of an apparatus pointer position y E II{. It can be described [2, 4] by the x-pointwise shift S of y as the multiplication ~ by a (x) = ~°, i n t he Hilbert s pace Lz (II~ 2) of square-integrable functions ~ (x,y), and it does not commutewith the free I-Iamiltonian operator H = 7 (Y~" - 0~) say, of the system "quantum particle plus apparatus pointer". It is usually assumed that the quantum jump occurs at a random instant of time + t , = s with a given probability density p (s) > 0 on the positive half of line 11~ f~ p (s) ds = 1. If H and S commute,the single-point discontinuous in t stochastic evolution can formally be described by the time-dependent Schr6dinger equation ihOtx (t) = Ha (t) X withthe s ingular stoch astic Hamil tonian H~(t) = H + itt6~ (t) In S, where 6~(t) = 6(t-s) = dr(s) is the Dirac &function of z = s-t. Indeed, integrating the time-dependent Ha~niltonian H,. (s) over r from 0 to t for a fixed s ~ N, one can obtain V (t,s) = e-~ f~/%(r)d,r = e-~,tHS&~o(S) = e~,{s-t.)nSA~o(s)e-~,sH ’ where A~ (.s) = f~ 6~ (s)dr is identified with the indicator function 1[o,0 of interval [0, t) for at > 0 (at t_< 0it is zero ifs > 0). The right hand side is for~n of the unitary stochastic evolution V (t, s) which should remain valid even the operators H and S do not commute. First the evolution is conservative and continuous, V (t, s) = e-~ ~ for t ~ [0, s), then the quantum jump S is applied at t = s, and at t > s the evolution is again continuous, described by the Hamiltonian H. As it was noted in [2], the rigorous form of the stochastic SchrSdinger equation which gives such solution even for noncommutingH and S in the positive direction of t, is the Ito differential equation dtV(t,s)+~HV(t,s)dt=(S-I)V(t,s)dlt(s),
t>0,
V(0,
Here dtV (t, s) = V (~ + dr, s) - V s) i s t he forward diff erential corr esponding to an infinitesimal increment dt > 0 at t, and dl~ (s) = t (s - t) is theindi cator function Atd~ (s) = l[t,~+dt} (S), the forward increment of the Heaviside function t ~ 1~ (s) = 10 (s - t), where lo = 1{-o~,0/. The equation (2.2) simply means that t ~ V (t) for a fixed s = z satisfies the usual SchrSdinger equation ihO~V (t) HV(t) if t ¢ s as dlt (s) = 0 for a sufficiently small dt (dr < s - t if t < s, and dt > 0 if t > s), while it jumps, dtV -- (S - I) V at t = s as dlt (s) It=s -- 1 >> Integrating d~)~ (z) = d~V (z) ~ on the domain of the operator H first from z = s with an initial condition X (0) = rh and then from s to t with the initial condition X (s+) := limz-,~, (z) = S:~ (s) one can easily obtain the solution form X (t, s) = V(t, s) r~, where V (t,z)
= e-~Hs (z) ll°’°(z)
-~ zH , S(z) e~ZHSe
without the commutativity condition for H and S.
314
Belavkin
Nowwe shall prove that the stochstic single-jump discontinuous evolution V (t) can be treated as the interaction representation V (t)X ° = e~th(:)Xt for a deterministic strongly-continuous Schrbdinger evolution xo ~ Xt in one extra dimension z E IR with the initial conditions X° (z) = ~ (z)~/E H localized at z > ° (z) = 0 at z _< 0. Here h (/~) = -~fi is the free Hamiltonian, where [~ = -ihO: is the. momentum in one extra dimension of z ~ l~. PROPOSITION 1 The described stochastic Hamiltonian problem (2.2) is unitary equivalent to the self-adjoint boundary-value Schriidinger problem ihO, Xt (z) = (H + il~Oz) t ( z) , Xt (O_) =Sxt(O)
(2.4)
in the Hilbert space 7l ® L2 (~) in the sense that the stochastic evolution V (t) t > 0 coincides with the unitary cocycle V (t, z)X ° (z) = ~ ( z- t ) r esolving t boundary value problem (2.~) with respect to the plane propagation t°~ along z as Xt = e tO" V (t) °, YX° ~~-I ® L2(~) Proof. The boundary value problem (2.4) is well defined on the space of smooth square-integrable ~-valued functions X, and is symmetric as H is self-adjoint, and due to the unitary boundary condition 0= (IIX(-0)II~-IIX(0)II
~) =2 Re{~(z) lx’(z)}dz=
In fact, this problemis selfadjoint as it has apparently unitary solution
x~ (z) = e¼~’"~ (z + t), ~ (s) = S~(~)~o
(2.5)
where Xo (s) = e-~Hzx.° (8). Indeed, substituting Xt (z) = e~zUx~ (z) into the equation {2.4} we obtain the transport equation OtXto (z) = OzX~O(z) with the same boundary condition X~ (-0) SXto (0) an d th e in itial co ndition X] = X0 cor responding to a X° ~ N ® Le (IR). This simple initial boundary-value problmn has the obvious solution X~(z) = X*(z + t) with Xt given in (2.5) ~ (s) = Sq°")(t-~)X° (s), t > 0, X* (s) = S-~I-’.°)(~),~ ° (s), t <
(2.6)
(s} in 7{ and of shift eta’ in L~ (II~) i~nplies the unitarity The unitarity of S~X~ t the resolving map V : Xo ~ Xt in N @L~ (~),
I1211 : = : Moreover, the map t ~ Vt has the multiplicative representation property 17r~ ft : 1,’~+t of the group R ~ r, t because the tnap t ~ Saa(*} is a multiplicative shiftcocycle, S~(*)et°’S ~(*} = et°’S a~+’(s), Vr, t E ~ by virtue of the additive cocycle property for the commutingA~(s) = It (s) - lo [A~+ e"°" A~](s) = 1~ (s) - lo (s) + It (s + t) - lo (s et°’A~+" (s).
Stochastic Equationas a Dirac Boundary-Value Problem
315
The subtraction X (t, z) e~thX* (z ) offree evolution wit h the generator ~X ( z) ihO~X(z) obviously gives
x (t,
s) = x - t) = ° ( s),
= e~(S-t)gsa~o[S)e-~SltX° = V (t,s) Thus the single-point discontinuous unitary e-~,th-cocycle V(t,
8)
:e ~t~V ~(=es-t)H~A~o(s
o
)
-~ e sH
,
tEll~
with /X~ (s) = l[0,t ) (s) for a positive t and s E II~+, solves indeed the single-jumpIto equation (2.2). It describes the interaction representation for the strongly continuous unitary group evolution Vt resolving the boundary value problem (2.4) with initially constant functions X° (s) = ~ at s > 0. REMARK 1 The toy SchrSdinger boundary value problem (2.~) is unphysical three aspects. First, the equation (2.~) is not invariant under the reversion time arrow, i.e. under an isometric complex conjugation ~7 ~-~ ~ and the reflection t ~-~ -t, even if ~ = S-~ and ImH = 0 as the Hamiltonian ~ = i~iOz is not real, hn ~ = lion.. Second, a physical wave function et (z) should have a continuous propagation in both directions of z, and at the boundary must have a jump not in the coordinate but in momentumrepresentation. The momentumcan change its direction but not the magnitude (conservation of momentum)in the result of the singular interaction with the boundary. And third, the free Hamiltonian ~ must be bounded from below which is not so in the case of hamiltonian function h (z, p) = corresponding to the equation (2.~). Nowwe showhowto rectify the first two failures of the toy model, but the third, which is a moreserious failure, will be sorted out in the next sections by considering the toy model as a dressed limiting case. Instead of the single wavefunction X~ (z) on I~ let us considering the pair (¢, of input and output wave functions with
¢’(z) = x’(z), > 0,
= x"
<0
on the half of line II~ +, having the scalar product
They satisfy the system of equations i~Ot~ t(z)=(H +ihO~)¢t(z), f12 ° e~®L~(~+) ~ ( II~ ihO~(~~ (z) = (H - ih0~)~ (z), ~0 e ~R ® +) for a quantmnsystem interacting with a massless Dirac particle in 1~+ through the boundary condition ~t (0) = S¢t (0), where ~t (0) ~ (0_). One can showthat this is indeed the diagonal form of the Dirac equation in one dimension in the eigenrepreseutation of the Dirac velocity c = -az along z ~ ll~ +, with the electric and
316
Belavkin
magnetic field componentsu~:, given by the symmetric and atisymmetric parts u + fi of u on I~ in the case In, u = 0. The componentsof (¢, ~) propagate independently at z > 0 as plane waves in the opposite directions with a spin (or polarization) oriented in the direction of z, and in the scalar case H = C are connected by the Dirac type boundary condition (1 + i#) ~t (0) = (1 ) Ct (0) c orre spondent to a point mass h# at z = 0. The input wave function Ct (z)
e-~tg¢ ° (z + t) _-~t(h+H~
(2.7)
is the solution to the equation (2.4) at z ~ ll~+with X°[~>0 = ¢o which does not need the boundary condition at z = 0 when solving the Cauchy problem in t :> 0. The output wave function satisfies the reflected equation at z > 0 and the unitary boundary condition at z = 0: ihOt~t (z) = (H - il~O,) ~b’ (z), ~’ (0) =
(2.s)
It has the solution ~’ (z) = -{’~ [ ~o (z - t) z (z) + S (t - z)¢o(,_ z )1, where 1~ (z) = 1 - l~ (z). This can be written in the similar way as
° (z - t) = ~-~"(~’+~)6 ° (z) 6~(z) =~-~’~V3
(12.9)
with ]~ = -ih8~ if 0o (z) is extended into the domain z < 0
S (Z) Ct (Z) = ~7 (--Z), S (Z) ~.-H,~ -~H
(2.10)
at t = 0. Note that reflection condition (2.10) remains valid for all t > 0 if ¢t extended into tile region z < 0 by (2.7) for all t ~ l~+: ~bt (-z)= e-~tH s (t + z)¢O (t + z) = S (z)e-~’tH¢O (z + t) = S (z)¢t Extending also the output wave ~t by (2.9) into the region z < 0 we obtain the continuous propagation of ¢, ~ through the boundary in the opposite directions, with the unitary reflection holonome connection (2.10) for all z ~ N. If/~ = where/~r/ = H---~ with respect to a complex conjugation in 7/, then the system of Sc}lrgdinger equations for the pair (¢, ~) remains invariant under tile time relicttion with complex conjugation up to exchange ~-t ~_ #)t. Indeed, in this case the complex conjflgated hamiltonian ~ = -ittO, coinsides with the operator [~ corresponding to h (z,p) = p = f~ (z, p). The boundary value problem is invariant under time reversion if 3 = S-1 as the reflection condition (2.10) is extended to the negative t by the exchange due to S (z) -t = o~ (-z). Thus the reversion of time arrow is equivalent to the exchange of the input and output wave functions which is an involute isomorphism due to
=dz = Ilxll== I1¢(~)11
(z) dz.
Stochastic Equationas a Dirac Boundary-Value Problem 3
A UNITARY
REFLECTION
317
MODEL
As we have seen in the end of the previous section, a unitary quantumstate jump at a randominstant of time s _> 0 is a result of solving of the toy SchrSdinger boundary value problem in the interaction representation for a strongly continuous unitary evolution of a Dirac particle with zero mass. The input particle, an "instanton" with the state vectors defining the input probabilities for s = z, has the unboundedfrom below kinetic energy e (p) = -p corresponding to the constant negative velocity v = e’ (p) = -1 aloug the intrinsic time coordinate z which does not coincide with the direction of the momentum if p > 0. One can interpret such strange particle as a trigger for instantaneous measurement in a quantum system at the time z E ~+, and rnight like to consider it as a normal particle, like a "bubble" in a cloud chamber on the boundary of lI~ d x R+ as it w~ assumed in [2], with positive kinetic energy and a non-zero mass. Our aim is to obtain the instanton as an ultrarelativistic limit of a quantum particle with a positive kinetic energy corresponding to a m~s m0 ~ 0. Here we shall treat the kinetic energy separately for input and output instantons as a function of the momentump ~ ~- and p ~ ~+ respectively along a coordinate z ~ ~+ with the same self-adjoint operator values e (p) ~ 0 in a Hilbert space b its spin or other degrees of freedom. For exampleone can take the relativistic mass operator-function e(p) = (pe + h:~) ~/2, ~ ~
= p~- V
(3.1)
in the Hilbert space ~ = L: (~) which defines the velocities v (p) = pie (p) e~ (p) with the same signature as p. At the boundary z = 0 the incoming particle with the negative momentump < 0 is reflected into the outgoing one with the opposite momentmn-p. The singular interaction with the boundary causes also a quantum jump in other degrees of freedom. It is described by the unitary operator a in ~ which is assumed to commute~ith e (p) for each p as it is in the quantum measurement’model [2] when a = e ~oy with V = 0y in (3.1}. Let ~ be a Hilbert space with isometric complex conjugation ~ ~ ~ ~ ~ ~ b, and L~ (~-) = ~ ~ ~ (~-) b e t he s pace of s quare-integrable v ector-functions f (k) ~ on the half-line ~- ~ k. Wedenote by ~- the isomorphic space of Fourier integrals :(z)=
~1 f~eiazf(k)
dk,
f ~L~(~-).
which is the Hardy class of ~-valued functions T ~ L~ (~) having the analytical continuation into the complex domain Im z < O. One can interpret L~ (~-) as the Hilbert space of quantum input states with negative momentap~ = hk, k < 0 along z ~ ~ and spin states ~ 6 ~. The generalized eigen-functions ~ (z) = exp [ikz]
~, k < O, e (hk) ~ = ~
corresponding to spectral values ~ ~ ~+ of ¢ harmonic waves moving from infinity towards ~./[k I along z. The amplitudes ~ are arbitrary to the identity operator 1 in ~, ~ (k) = sal, as
~=~.
(3.2)
(k) h-~e (h k), ar e gi ven as the z = 0 with the phase speed ¢~ = in ~ if all e (p) are proportional it was in the previous section where
318
Belavkin
The singular interaction creates the output states in the sa~ne region z > 0 of observation where the input field is, by the momentum inversiou p = -Pk ~-~/5 = P~,, reflecting the input wave functions ~ ~ ~- isometrically onto 1
~(~) = ~/ff ~ e-ik~](k)dk
= a~(-s) ’ s
by ](k) = af(k), k < 0. The space $+ = {~:~ e ~-} is the conjugated Hardy subspace $+ = {~ : ~ ~ ~- } of analytical functions ~ (z) = ~ (5) in Im z > 0. reflected wave function satisfies the boundary condition ~ (0) = a~ (0) corresponding to the zero probability current j (z) = ~(z)~~ ~ - ~[~(z)~[ at z : 0, and togetber with the input wave function ~ (8), s ~ 0 represents the Hilbert square norms (total probability) in $- and $+ by the sum of the integrals over the halSregion ~:
]l~(8)ll~ + ll~(s)~] 2 ds =
II~(z)ll~dz
~l@(z)~12dz.
The free dynamics of the input and output wave functions can be described ~ the unitary propagation 1
~ (~) = ~ ff
eik(t¢(k)+z)f
1/2
~ (z) = ~ ei~’(~(~’)-~If(k)
(k) dk = [e-i’e~] (z), dk = [e-i’g~]
(3.3)
(z),
of a supe~osition of the ha~onic eigen-~nctions (3.2) in the negative and positive direction of z E N respectively with the same phase speeds Ck > 1 which are the eigen-values of the positive operators g (k) Ikl -~ e (k). The ge nerating se lfadjoint operators g, g are the restrictions g = e (iOn) I’D-, g = e (iOn) of t he kinetic energy operator given by the sym~netric function e (p) ou its symmetric dense domain ~ ~ L~ (N), to the dense domains ~ = ~ ~ g* in the invarim~t subspaces g~ ~ L~ (N). Instead of dealing with the free propagation of the input-output pair (~,~) the region z > 0 with the boundary condition ~ (0) = ~ (0), it is convenient to introduce just one wave Nnction
¢~(z) = ~ (z), Re0,¢~(z)= ~(-z), Re z < 0(~; considering the reflected wave as propagating in the negative direction into ~he region z < 0. Each ¢(-z) is aHardy class function a~ at z > 0, as wellasit is Hardy class function ~ (-z) at z > 0, but the continuity of the analytical wave functions ~ (z) at Re z = 0 corresponds to the left discontinuity ¢ (0_) = ¢¢ (0)
¢ (z)=~o(-z) ~ (z) + ~o(~) ~ (z), ~o(z)
z~o,
where¢ (0_) is defined as the left lower sectorial limit of¢ (z) at Re z ~ 0, Im z fi~ Obviously the Hilbert subspace ai°g - C L~ (N) of such wave functions is isomorphic
Stochastic Equationas a Dirac Boundary-Value Problem
319
to ~- by the unitary operator a1° = I + 5o (a - I), where 5o is the multiplication operator of ~ (z) by 1 if z < 0, and by 0 if z >_ 0. The unitary evolution group v t : ai°e-n~a-i°,t E ~ for ¢~ (z) = ~pt (z) + 10 (z) (a - 1) ~ (z) t (z),
(3.~)
is unitary equivalent but different from the free propagation e -ire of ~t in R. Each harmonic eigen-function (3.2) having the plane wave propagation
~o[.(z) = e-*~"~ (z) = ~ (z + for the negative k E II~-, is nowtruncated, ¢~ (z) ei kzcr~o(z)O~, and pr opagates in the negative direction as
¢[. (z) = ~o(~(z + ~t) = e-~’~t¢~ (z) # ¢~,(z keeping the truncation at z = 0. Therefore the subtraction Ct (z) = eite¢ t (z) of the free propagation of qot fi’om Ct does not return it to the initial ¢0 = ~rioqo0 but to Ct = a~-qa ° =vt¢o, where ~t = eit~ioe-it~, vt = a~a-i°, ~nd ¢0 ¢0. Thus we have proved the following proposition for the particular case >c = 0 of an operator >¢ ~ ~, defined in the Proposition 1 of previous section as Let ~ be a selfajoint operator in b, and ~, (z) --= e-i~z be the correspondent oneparameter unitary group in I}. Belowwe shall denote by ~,~ and ~,~ the operators of pointwise multiplication by the functions e,, : z ~-~ e× (z) and ~ : z ~ e,, (-z) z ~ II~ respectively. Both these operators are unitary in the Hilbert space L~ (ll~). If h~ = ]z is an operator in L~ (tl 0 which is given as a pseudo-differential operator h (z, ~~0 ~) = lit (z,iOz), the operator-function ~/ (z, ~ +~c)=~*~+~ (z) ^~
(z, iOz)~+~(z) =_"~+~
(3.6)
defines the symbol7~ (z, ~) = (z , ~c ÷ ~) of theoperator
It is defined on the exponential functions e~ (z) = -i~-" as t he pseudo-differential operator
PROPOSITION2 Let ~ = ~- be the Hardy class of L~ (~), the Hilbertspaceof functionsqo=~*~owith~oe g~,and~ ~ = ~+. Let the initial boundary-value Schrddinger problem iOt~t (z) = e~ (iO~)~t (z), ~0 ~ $;,z >
~, C L~ (~) =e,go’*"+,where (3.7)
ia~~ (z) = ~ (iaz) ~’ (z) , ~ (o) = be defined by the generators g~, ~ given by the symbols ~ (~) = ~ (~ + ~), ~ (~) ~ (~ - ~) respectively, where ~ (~) is the symmetric.function o] ~, ~ ~, corresponding to the kinetic energy e (p) = ~ (h-~p) > O. Then it is sel]adjoint if the initial output waves ~o are defined in ~ by ~o (-z) = a~ (z) ~o (z), z < O, where a~ =
320
Belavkin
by analytical continuation of each 99~ = ~99o into the domain~-. The solutions to (3.7) can be written
~ (z) = ~ (z),z > 0, ~ (-z) = ~ (z_),z < 0 where ¢~= e-i~¢t, a,~ (z), and
(~.s)
c~t= 99 0 +-a~)7r,~99 (1 ~ ~ , 5~ is pointwise multiplication ^t
eit~z~
~o~-itg,,
by
t (z,iO..)
~_ ff>~
is given by the symbol 7r~ (z, ~) of the orthoprojector #t = en~ioe-ite as in (3.6). Proof. Separating the variable t ~ I~ by 99t = consider the stationary Schrhdinger problem
e-i~.~t99k,
~t =. e-i~.~t~k,
~,, (z, iOz) 99~ (z) = ~k99k(z), ~k (--z) = a~ (z)
let us (3.9)
corresponding to the given initial and boundary conditions in (3.7). Here 99k extended to the domain ~- through the analytical continuation of e~k in Im z < 0, which are the generalized eigen-functions (3.2) of g = (i On) in $~ iff k < 0. Due to the selhadjointness of g in $-, the eigenfunctions ~ = e~+~ of g~ for (3.9) with negative k form an orthocomplete set for the Hilbert sp~e 8~, and the output ~ --1/2 1/2 cigen-functions ~ (z) = ~+~ (z) ~k, where aoOkwith ao = Po apo , form an orthocomplete set for the Hilbert space ~. The solutions to (3.7) can be written in the form (3.3)
~’ (~) = ~
e-~(~’)’~;+,~ (z) y (k)
(z),
~ (~) =
e-i~(~’~t~ (z) ] (~)
(z),
where fo (k) = efo (k) are defined as the Fourier transforms
f (~) =
./i~+~(z) ~o(z) dz, ] (k) =
,~+~(z)
by the initial conditions, analytically extended on the whole line ~. Due to the commutativity of a and g they satisfy the connection ~t (-z) = a~ (z) ~t (z) for t, not only for t = 0. The time invariance of this connection and the unitarity of the time transformation group in the Hilbert space $~ ~ S~, which follows from the unitarity of (3.3) in $~ C L~ (~), means the self-adjointness of the problem (3.7) for the pairs ~ ~ L~ (~, p) in the domain of the generator gz ¯ g~ with connection ~+ (-z) = a~ (z) ~- (z). Introducing
¢~(~)= ~t(z) +~o(z) (~(z) ~)~’ (z)= ~.(z~°(~)~ (~) as in (3.5), and taking into account that
¢~(z_) =a~(~)~o(~-~ ~ (~) =~-~°~-~~ (z) =a~ -~ ( °(-~ ~ (-~), we obtain the representation (3.8) as ~t (z) coincides with ¢~ (z) at z ~ ~t (-z) with St (-z) = ~t (z_) at z ~ 0.
Stochastic Equationas a Dirac Boundary-Value Problem
321
REMARK 2 The SchrSdinger boundary value problem (3.7) is physical in all three aspects. First, the equation (3.7) is invariant under the reversion of time arrow, i.e. under the reflection t ~ -t and an isometric complex conjugation ~ ~-~ ~ together with the input-output exchange ~ ~ ~ if d = a-1 and ~ = ~, where ~ (z) = ~ (-z). Second, the wave functions ~, ~t have continuous propagation in both directions of the momentum along z, and at the boundary z = 0 the momentum changes its direction but not the magnitude (conservation of momentum)as the result of the the boundarycondition ~ (0) ~-~ ~ (0). And third, the kinetic energy operator g,,@g,~ is boundedfrom below as the result of unitary transformation of ~ ~_ ~. (2.4). Indeed, from ~ (~) = e (~) = g (a) it follows that the symbol g,~ (z, a) of the complex conjugated operator ~ is given by g-~ (z) e*~ (z) e (i On) e_~ (z) = e*_~ (z) e (i On) e_~ (z if ,~ = &, as ~ (z) = e-r~ (z) and e_~ (z) = ~ (z). Therefore f~ (z, a) = where g~, (z, a) = ~ (z) is the symbol for the kinetic energy operator g~ = g,, the output wave qS. Thus the time reversion with complex conjugation in (3.7) equivalent to the input-output interchange (~t, ~St) ~ (~St,cpt) which preserves connection between ~ot and ~5t as
=
(z) = (z)
(z) = (z),
where ~ (z) = a,~ (-z) due to ~ -t .
4
THE ULTRARELATIVISTIC
LIMIT
Weshall assume here that the symmetric positive kinetic energy e (p) has the relativistic form IPl, or more generally, e (p) = v/p2 + h2#~" as it was suggested in (3.1). It corresponds to the finite bounds v:~ = ~:1 of the velocity v (p) = e~ (p) p ---~ ~c. Note that the phase speed % = ~(~)/a for the momentap = :t:hn,
= V/1 + ~/~ = v (h~) -~ ,
~ > 0 of the harmonic eigen-waves
e-i~’te~. (z) = e-in(~t+z), " e-ie~t~n (z) = -in(~t-z) has also the limit ~ = 1 at ~ --~ oc. Therefore one should expect that the rapidly oscillating input and output waves ~0t (Z) = e-i~(t+z)~bt (z) , ~t (z) = e-i~clt-z)~ t (z) in the ultrarelativistic
(4.1)
limit p ~ :l:~c will propagate as the plane waves with
¢t(z)=~(z+t)=et°’¢,
~bt(z)=(~(z-t)=e~
(4.2)
if the initial conditions are prepared in this form with slowly changing amplitudes ¢,~ ~ L~ (II~). This propagation will reproduce the boundary-reflection dynamics
322
Belavkin
~t (0) = a¢ (0) on the half line + 9 z = s if theinit ial wave amplitudes are connected by ~b (-z) = a¢ (z) for all z E IR. In particular, the solutions Ct (s)
¢ (s +t), ~ (s) =0, t ~ (s) : ,~-~(o) =,~¢’-~(o) : ,~¢(t - s), to this Hamiltonian boundary vahm problem with the input, wave functions
¢(z) = v~,s > 0, ¢(~) =0,z for the initinl state-vectors ~ ~ ~ will correspond to the single-jump stochastic dynamicsin the positive direction of t with respect to the probability density p > O, f~ p (s) ds = Belowwe give a precise formulation and proof of this conjecture in a more general framework which is needed for the derivation of quantum stochastic evolution as the boundary value problem in second quantization. But first let us introduce the notations and illustrate this limit in this simple case. In the following we shall use the notion of the inductive limit of an increasing family (~)~>0 of Hilbert subspaces ~ ~ $~,,~ < ~’. It is defined as the union ~ = U$~ equipped with the inductive convergence which coinsides with the unitbrm convergence in one of the subspaces $~, and therefore is stronger titan the convergence in the uniform completion ~ = ~. The dual inductive convergence is weaker then the convergence in K, and the iuductive operator convergence in g is defined as the operator convergence on each g~ into one of g~, ~ ~. Let 6- = Ug2, ~+ = Ug~ be the inductive limits for the increasing family + (g~- ,g~)~>o of Hardy classes $2 = ~g- D ~o, ~ = ~.$+ D ~o, ~,o < ~ in the notations of the previous section. Both ~-,~+ are dense in L~ (N), consist of the square-intergable 0-valued functions ¢ ~ 6-, ~ ~ ~+ having zero Fourier amplitudes
g (k)
e-~’~(z) dz, ~ (k)
(z)
for all k R ~ with sufficiently large ~ > 0. If ~ e g2 and ~ e g~, then ~ = e~0 e g-, ~ = ~ ~ g+, and the free propagation (a.3)can be written in the form (.4.1) with ¢~ = ei"ti~.~
t = i;e-i(i-~)ti~
@t = ei~t{~@ t = ~.z*°-i(g-~l)tz~w
"~ ~ ~.
These unitary transformations in g2 and in g+~, written as e~ (z) = ~-"~(~°=)W (z), ~ (z) = ~-,:,,~,~o=)~ are generated by the selfadjoint
(4.a)
operators
w~ (iOn) = ~ (e ( iOn) - ~)-~: = e ( ~ + ion) - ~,
~ (i&)= -~"(e (i&) -~)~"= e (~- i&)-
(4.4)
323
Stochastic Equationas a Dirac Boundary-Value Problem
They leave all subspaces ~7~ and ~+~ invariant respectively, however their generators da~,ga~ are not positive definite for a sufficiently large ~, and are not unitary equivalent for different ~ as ~,~w~e,~ = ~ - ~1 = w~ - ~1, e~w~.e~ = ~ - ~1 = w~ - ~1, where ~ = ~ - ~. Thus we have to prove that the propagation (4.4) has the inductive limit form of plane propagation (4.2) at ~ ~ ~ corresponding to the Dirac form of the limits lira w~. (iOz) = iO:, li~n ~. (iOz) = -iOz for the Schr6dinger generators (4.4). Another thing which we are going to prove for obtaining the single-jump stochastic limit is that the truncated wave
representing the pair (4.4) on the half-line ~+ 9 z as in (3.8), has the discontinuous limit X~(z)=x,(z+t),
X~=¢+(~-~)L¢.
(4.5)
Here ~ = e -it°’~oeit°= is pointwise multiplication by the characteristic function It of the interval -m < z < t which we shall obtain as the inductive limit of the orthoprojector ~t eite(s+io=)ioe-ite(s+io.)
eU~ ioe-i~
(4.6)
at a + ~. This results are formulated in the following proposition in full generality and notation of the proposition PROPOSITION 3 Let ~- be the Hilbert inductive limit of Hardy classes ~[ = ~ 6~ C L~ (R,p) be the Hilbert space of functions 6~, and 6~ = g~6+, where 6 + = U~ ~ 6~. Let the initial boundary-value SchrSdinger problem i0,¢~ (z) = ~,, (z,iO~)¢~ (z),
¢] = ¢ e 6;,z >
io~(z) = ~,~(z,iO=)~i (z) ,~ > o, ~ (o) be defined by the generators
with the symbols w~, &~given in (4.6), (3.1), and the initial as ~ (-z) = a~ (z) ~ (z), z < 0 by analytical continuation of each = ~in to the domain ~-. Then the solutions to (4.7) inductively converge
¢’ (z) ~ (~), z ~ 0, where Xt (z) = e~ (t) X~ (z + t),
(4.7)
324
Belavkin
Proo]. First let us note that the generators in (4.7) have the formal limits lira [~,~¢] (z) : ~:~ (z)i0~ [~¢] (z) = (~ + ~:0:)¢
with ~z = -0~. This follows from (4.6) and iOze~ = ~e~, Oz~ = i&~ as ~ (z) e:~ (z). Thus we have to prove that the solutions to (4.7) have the limits ¢ = lira ~ = lira ,~ in 6~ coinciding with the solutions to the Dirac boundary value problem
~ (z) = (- + ~0~)¢~(z), ¢0= ¢ ~ 6;,z ~0~¢ (~) = (,+ ~) ¢~ (z),z
> 0, ¢~(0)
with the initial ~o analytically deaned as ~o(-z) = ~ (z) ~o(z) in order to keep the solution ~t also in ~Xfor all t. Let us do this using ~he isomorphisms ~ ~ of ~he dense subspaces ~ and ~ C L~ (~). Due this the boundary value problem (~.7) is equivalem
=
~ , o,~ = ¢o ~ 6~,z > 0 ~o,~(~) ,~ > 0, ~o,~. (0) = (0)
with ~ (-k) = ¢ (n- k) - n = ~ (k), and ~,~ (-z) = a~0 (z) as a. for any scalar n. Thus we are to find the ultrarelativistic limit of the solutions 1
e-i(~(-k~-k~ 9 (k) dk,
(4.9)
with ~ (k) = e9 (k) at ~ ~ ~. Here the Fourier amplitudes
g (k)
/7 e-i~¢0(z) dz, ~ (k)
(z)
are defined by analytical continuation of the initial conditions e,.o ~ for a ~o < ~ such that the integration in (4.9) can be restricted to k < no dne to g (k) = 0 = ~ (k) for all k ~ no. Therefore the proof that the unitary evolution (4.9) inductively converges to the plane propagation et°~¢0,et°~o resolving this problem at ~ ~ ~ can be reduced to finding an estimate of the integral
It gives the value ~o ~hemeansquaredistances ¢
~O,n
O,n --
of~,~(~- t) from ~0~ ~.:~C a.do~4~,~(~ +t) from ~o
Stochastic Equationas a Dirac Boundary-Value Problem
325
To this end we shall use the inequality (~f2
~_
1 #2 /A2)l/2 -~<2~’ ---
w > II~1
for the monotonously increasing function k+w~(-k) < n°+w~ (-n °) of k < n°. We shall treat separately the three cases in (3.1): the scalar massless case #0 = 0 when ~ (k) =Ikl, the boundedness case [#1 <- ra when ~ (k) <_ V~ + 2 asin thescal ar case with # = po > 0, and the general vector case when ~ (k) = 2 + p]- V2)~/’2 In the first casek+w~(-k) =k-n+[n-k I=0foraltn>_0andk<~. Thus the plane wave propagation
~o,.(~)=¢o(z + , ¢o,~(z) = ~o(z is extended by ultrarelativistic limit n ---+ ~ from the orthogonal Hardy classes £o:F onto the inductive spaces ~o:F. By continuity they are uniquely defined as the opposite plane propagations on the whole Hilbert space L~ (IR) where they satisfy the connection ~o (-z) = a¢o (z). In the second casek+w~(-k) <m2/2~for all ~<=n-n ° °. > I#l andk < n Using the inequality le z - 1[ < 2Ix[ for any x e C with Ix] _< 1 we obtain the estimate 2rn III(~°,n)ll<_e -i(k+w~(-k))t 1[< 2[t llIk+w~(-k)[[ < Itl-~for the integral I (n°, n) with [[g[[~ = ~ f [[g (k)[[ ~ dk < 1. Hencefor any n° > 0, e > 0 and each t ~ IR there exists an’ < oc such that [[/(n°,n)[[ < e for all n > n’. Namely, one can take ~’ = ~:° +,nax {m, Itt m~/~} such that >c = n-~° > n’-n > m and It I m’~/~<< ~. Thus the plane wave propagation is indeed the ultrarelativistic limit of (4.9) in the inductive uniform sense. In the third case one should replace I) = ~ (I~d) by t he i nductive l imit ~° =Ul~, of Hilbert subspaces I~ of functions in L2 (~d) having the localized Fourier amplitudes h (k) = 0, k ~ (-n, n) for a d. Then #~ - V~ < #o~+ n2 i n each O~, an d []I ( n°, n)[I < It[ (#o2 + n2)/~< if [Ig[I < 1 for the Fourier amplitudesof ~bo e l)~ ®~-o and of~o6 ~ ® £~o, + where ~ are Hardy classes in L~ (I~). Hence for any ° >0, ~z, n EIR ~ > 0 and each t E IR there exists an’ < cx) such that [[I (n°, n)[[ < ~ for all ~ > n’, namely n’ }. = ~° + max{V/~0~+ n2, [t[ (#0~ + ~e)/e Howeverthe estimate It[ (#~ + ~) / (n °) depends now on ndefin ing the c hoice of g (k) in ~}° for each k < °. This p roves t hat t he plane wave propagation i s t he ultrarelativistic limit of (4.9) also in the general vector case, although not in the uniform but in the strong inductive convergence sense. Thus the boundary value problem (4.7) in the ultrarelativistic limit is unitary equivalen_t to the plane propagations (4.2) of opposite waves ’~bo, ’~0 with the connection ¢o (-z) = a¢o (z) for all z ~ R. In the half space z + this obviously can be written as
¢~(z) : 4 (z) ,z >_o, ~ (-~) =Z’o(z_)
326
Belavkin
where X~(z) = X0,t (z + t) is the truucated input wave(4.5) with ¢0 in the capacity ~t v, -t of ~p. Returning back to’~t= e~b ^, o tand=e,~b weshall obtain the representation o (4.8) with
:g’(z)=~;,(z)~o,~,~(~):g~(z)=~,~(t) ~, due to continuity of e,, (t), where:g~ = ~,X0,~is given in (4.8). REMARK 3 The truncated wave Xt = io¢ t + io~b t in the interaction representation X (t) = ei~’txt with respect to the shift group generatedby ~/ = i0,~ satisfies the stochastic single-jump equation d:g (t, z) + i~:g (t, z) dt = (a 1)X (t, z) dlt (z), t > 0
(4.10)
Indeed, the dynamical group e,~ (t) e- i×t is unitary in I}. Tileone-para~netric group e w: is apparently generated by the self-adjoint operator "~(iO,) = iO: in L2 (ll~) which is the symbol of the generator "~ for the shift group evolution e-u#. It is a unitary group in L~ (IR) due to the shift-invariance of the Lebesgue measure on ll~. Hence the truncated wave in the interaction representation is given by
x (t, z)=~(~ -t)= ,~~(t) x~ ( =~;,(z- t) ~,~(z):g~(z)=d(~’-~)’~:g0,t where ?(.o.t = Xo+ (a - 1) (lt - lo) :go with :go = io¢o + ib~o. Taking into account that dtdl, (z) = 0 in the Hilbert space sense as it is zero almost everywhere due dlt (z) = 1 >> dt # 0 only for the single point z = t having zero measure, we obtain d:g (t, z) ei (~-t)’¢ [(a - 1)dlt(z) = [(a - 1) dlt (z) i~dt] = [(a - 1) dlt (z) ixdt]
:go (z) - i.~:go,~(z) dt] ei(Z-O~Xo,t (z)
~(t,z).
Here we used that dlt (z) = dlo (z- t) = 0 if z ¢ t such dlt (z) ei(Z-’)×:go,t (z) = dlt (z) :g0.t (z) = dl,. (z) :go,z due to :go,t (z)It=~ = X0 (z) as It (z) - 10 (z) = 0 for any z > t > 0. Thus we proved that :g (t, z) indeed satisfies the stochastic single jumpequation (4.10) in Hilbert space L~ (II{, p) of the initial conditions :g = ~0¢ + ]0-L~ with respect to the unitary group evolution etO; . Returning to the notations ~ = h-~H, a = S of the Sec. 1 in tile Hilbert space ~ = 7-/ we obtain the stochastic equation (2.2) for the unitary cocycle V (t, s) e-t°" Vt, where Vt = ,~i°et(O~-ih-~ H) s-i°, as a quantum-~nechanical stochastic approximation. Namely, the toy Hamiltonian model for the interpretation of discontinuous stochastic evolution in terms of the strongly continuous unitary group resolving the Dirac boundary value problem in extra dimension, is indeed the ultrarelativistic inductive limit of a SchrSdinger boundary-value problem with bounded from below Hamiltonian g~ (p) = hw~,× (-h-~p).
Stochastic Equationas a Dirac Boundary-Value Problem
327
REFERENCES 1.
2.
3.
4.
5. 6.
7.
S. Albeverio, V. N. Kolokoltsov, O. G. Smolyanov, "Continuous Quantum Measureinent: Local and Global Approaches," Reviews in Mathematical Physics, 9, No. 8, 907-920 (1997) V.P. Belavkin, "A Dynamical Theory of Quantum Measurement and Spontaneous Localization," Russian Journal of Mathematical Physics, 3, No. 1, 3-23 (1995) L., Accardi, R., Alicki, A. Frigerio, and Y. G. Lu, "An invitation to the weak coupling and low density limits," QuantumProbability and Related Topics VI, 3-61 (1991) V.P. Belavkin, "A stochastic Hamiltonian approach for quantum jumps, spontaneous localizations, and continuous trajectories," QuantumSemicalss. Opt. 8, 167-187 (1996) V.P. Belavkin, "Nondemolition Principle of Quantum Measurement Theory," Foundations o] Physics, 24, No. 5, 685-714 (1994) A.M. Chebotarev, "The quantum stochastic equation is equivalent to a symmetric boundary value problem for the SchrSdinger Equation," Mathematical Notes, 61, No. 4, 510-518 (1997) R.L. Hudson, and K. R. Parthasarathy, "QuantumIto’s formula and stochastic evolutions," Comm.Math. Phys. 93, No. 3,301-323 (1984)
A MaximumPrinciple Parabolic Equations
for Fully Nonlinear with Time Degeneracy
JOACHIMVONBELOWLMPAJoseph Liouville, EA 2597, Universit6 du Littoral CSte d’Opale, 50, rue F. Buisson, B.P. 699, F-62228 Calais C6dex (France)
1
INTRODUCTION
AND MAIN
RESULTS
In the present contribution we derive somea priori bounds for classical solutions of fully nonlinear parabolic equations that include possible time degeneracies. Moreover we show that, in general, a comparison principle for such equations cannot hold. The boundary conditions are of mixed type, a Dirichlet boundary condition on one part of the time lateral boundary and a possibly dynamical one on the complementary part. The latter includes as a special case the Neumannboundary condition. Suppose 12 C_ Ii¢ ’~ is a bounded domain whose boundary is decomposed into two disjoint parts 0fl = 01~ e) 02fl, where 0212 is of class C2 and relatively open in 0~. Let v : Of/ -~ It ’~ denote the outer normal unit vector field on 02~ and 0~ the outer normal derivative. For T > 0 we set QT = ~ × [0,T] and introduce the parabolic interior QT and the parabolic boundary qT as QT= (fl tJ c9:~-l) × (0, T] and aT = Q’r \ Q"r. Weconsider fully non linear parabolic equations of the form b(u)t = F (x, t, u, Vu, D2u) =: F[u] and inequalities associated to them, where parabolicity means that F : ~T × It( × ll~ n x I~’’~ ---~ I~ is increasing with respect to q = D~u and b : I~ ---~ t~ is increasing with respect to u outside a compact interval in ll~. 329
(1)
(2)
yon Below
330
Here the order A _< B between symmetric matrices means that the matrix B - A is positive semidefinite. Note that we do not require strict monotonicity. Thus, degeneracies of the principal spatial part as e.g. the porous mediumequation are admitted. Throughout, Condition (2) will be assumed to hold. On 01~ × (0, T] we prescribe an inho~nogeneous DMchlet condition, while on 0~ × (0,T] we consider a possibly dynamical boundary condition/30(u) = 0 with
Go(u) :=~(x,t)O~+ c(x,t)O~u. Throughout we will assume the dissipativity c > 0, a _> 0
condition on 0~ x (0, T].
(3)
Without condition (3) blow up and nonuniqueness phenomena can occur already the case b(u) = u, see [2] and [3]. The investigation of differential equations of the form (1) is motivated by several applications, as e.g. models of hysteresis phenomenain physics, but also of theoretical interest, see [1], [4] and [5], as well as the dynamicalboundaryconditions, see [2] and [3] and the references given there. If b’ vanishes at some value of u, Equation (1) undergoes ti me degeneracy at that val ue. In thi s way, equ ations of the form (1) can display a change of type between parabolic and elliptic problems. The following results present some elements of a qualitative parabolic theory for classical solutions, i.e. solutions in C(-~T ) f’lC 2’1 (QT), as it is well established in the nondegeneratecase b(u) = u, see e.g. [2], [6] and [7]. It is clear that, if b is strictly decreasing in some noneInpty interval, then no classical maximumor comparison principle is possible, since in this case (1) can take locally the form of a backward heat equation. But one can control the solutions outside a compact part of the range, if the r.h.s, in (1) is governed by a generalized Osgoodsign condition. THEOREM 1 Suppose that b ~ C2(I~) and there are constants ~ >_ 0 and Zo i> 1 such that
~ +Z)~’(z)Io,. Izl >zo, ~(., ., z, 0, 0) <(Zz b’(z)
>0 for
Izl>z0,
b(-zo)=
rain
b and b(zo)
(4) max b. (5)
Then any ,solution u ~ C(-~T) ~ 2’~ ( QT) of t he B
~(~)~= F (~, t,,~, W,D~,,)i~
{
on0~x (0, T]
~o(U)=
satisfies m_axlul <_ e2~~r tnax ~maxlul,zo} . QT
[
qT
Note that here b was not assumedto be increasing on the whole real line. If b bears that property, then we can state the following positivity result. Conceivably, the critical values of b play a crucial r61e in separating techniques.
331
Fully NonlinearParabolicEquationswith TimeDegeneracy THEOREM 2
Let u E C(’~T) ~ ~’~ (QT) fulfill t he i nequalities b(u)t >_F(x,t,u,
Vu, D2u)
inQT,
02~× (o, TI
/~o(u) >_
on
u >_0
on qT,
under the conditions
F(.,., z, o, o) > 0 ]orz < o, b E ¢~(~),b(0)= 0, > 0in~, b’(z) =o ~ >o.
(6) (7) (8)
Then u >_ 0 in QT. Can one compare solutions of (1)? The best answer would be a comparison principle with respect to qT: b(u)t- F[u] <_ b(v)t - F[v] in QT, I3o(u) <_ Bo(v) on 0~ × (0, T] and u < v on qT imply that u _< v in QT. It turns out that, in general, this conclusion is false. COUNTEREXAMPLE A comparison principle with respect uniqueness of solutions in C(-~T) C~ ~,~ ( QT) of t he I BVP
to qT would imply
b(u)t = r (x, t, u, Vu, D2u) in QT,
13o(U) =
on c%Q× (0, T],
Ulqr = ~b ~ C(qT). For 1 _< k C N, choose b(u) = ~-~’+1and for a e [0, oc ) se Ya(x,t)
fort>a, for t < a.
(t-a) = 0
Then each y, belongs to C(-~T) ¢~ C2’1
(QT)
and is a solution of
b(u)t Au+ 3(2 k + 1 )u2~+~
in QT,
O,u = 0
on cgf~ × (0, T],
u(., O) =
in
Note that F is of class C~. Thus, even under a one-sided local Lipschitz condition with respect to u on F and even if b is strictly increasing in If{, a comparisonprinciple with respect to the parabolic boundary does not hold for equations (1) with proper time degeneracy. Without degeneracy, i.e. b(u) = u, such a principle holds under canonical conditions, see [2]. But, we can at least carry over a Nagumo-Westphal type conclusion [7,§24] with respect to qT.
332 THEOREM 3 Let
yon Below u,
v E C(-~T)
~l C2’1
(QT)
satisfy
13o(U) = Bo(v) = 0 02f~ x ( 0, T] and the inequality b(u)t - F[u] < b(v)t under the conditions b E C1 (l~) and b’ >_0 in
in
Then u < v on qT implies u < v
in QT.
Finally, we state the following weak maximumprinciple in the case where b has at most one critical value. THEOREM 4 Let u
~ C("~T )
ClC2’I(QT) satisfy
Bo(u) <_
on 02ft x (0, T],
(Bo(U)>_
Suppose that b E Ce(~), b’ > 0 in II~\{0} and F(.,.,.,0,0) Then maXuqT ~ maxu.~T
_< 0 (F(.,.,.,0,0)
_>
\(minUqT "-~ minU.)~T
Wenote in passing the Theorems1-4 apply especially
to equations of the form
(u~k+~), = F (x, t, u, Vu, D~u).
(k ~ N)
Moreover, Theorem1 applies e.g. to cubic l.h.s, b(u) = u(u-a)(u-b) with a < 0 < b that display a backwardparabolic equation in a nontrivial interval containing the origin.
2
PROOFS
Let us recall the basic comparison technique stemming from [7,§24] for Dirichlet boundary conditions and for dynamical ones from [2] or [3]. LEMMA 1 ([2,Lemma
2.1]) Let ~,~ e C(-QT)V~C’2’I(QT) B0(~o) _30(¢)
satisfy
on 02~ x (0, T],
and the following test point implication: If qo = ¢, V~ = V¢, D2tp <_ D2¢ at some point (x, t) e QT, then Otto < Ore at (x, t). Then qo < ¢ on qT implies ~ < ¢ in QT.
(9)
333
Fully NonlinearParabolicEquationswith TimeDegeneracy PROOFOF THEOREM 1 For ~ > 0, we first
set 99 = b(u) and ¢ = b(’~),
where
"~, qr "7 = (l + ~)e2~tmax~max[ul’z°} Then B0(99) = b’(u)Bo(U) = 0 and, by (3), 2a/3"7 b’(’7) >_ O. Moreo ver , ’7 > Zo _> 1 in ~T and, due to (5), b’(’7) > 0. Thus, as b is strictly increasing Izl _~ zo, 99 < ~b on qT. At a testpoint (x, t) E QTas in (9) we conclude 99=¢ ~ u=7>z0
and b’(u)
>0,
V99 = ~¢ ~ ~99 = b’(u)~u = 0 ~ ~u 0, D299 = b’(u)D~u <_ D~¢ = 0 ~ D~u <_ and using (4), 0~¢ - 0t99 = b’(’7)2/37 F(x,t,u,O, D~ u) _> b’(7)2/37 F(x,t,’7,0,O) >_ b’( 7)/3~f (1 - 7 -~) > 0. Now, Lemma1 yields 99 < ¢ in QT, which implies u < 7 _~ 7(T) in QT, since b is strictly increasing for Izl > zo. In order to show u > -7(T) we apply Lemma1 to ¢ b(u) and 99 = b(- 3’). Usi here that, b’(-’7) > 0 and F(x,t,-’7,0, O) >_ -(/37+/?’7-’)b’(-’7), we proceed similarly and conclude that 99 < ~/~ in QT, which again implies that u > in QT"As ¢ > 0 was arbitrary, the assertion of Theorem1 is shown.
PROOF OF THEOREM 2 For ¢ > 0, we apply Lemma 1 to 99 := 0 and ~p := b(u) ~(1 + t) . Note fi rst th at Bo(¢) >_ 0 by (3) and 99
and b’(u)
>
0 = V99 = ~ = b’(u)Vu =~ Vu = 0, 0 = D~99 <_ D~¢ = b’(u)D~u =~ Deu >_ 0, and using the differential inequality and (6), 0~¢-0t99 = b(u)i + e >_ F(z,t,u,O,O)
+e
Thus b(u) >_ in QT.Thispermits to co nclude that u _> 0 in QTdueto (7).
PROOFOF THEOREM 3 We can apply Lemma 1 di’rectly to 99 = u and ¢ = v: At a testpoint (x, t) ~ QTas in (9) the differential inequality yields due to 0 <_F(x, t, ~, V99,D’~¢)- F(x, t, 99, Vqa, D~’~)< b’(~)Ot¢ - b’(99)Ot99. Thus, necessarily, b’(99) > 0, which showsOre > 0t99 at the point (x, t). This shows Theorem 3. ~
von Below
334
PROOF OF THEOREM4 Fore>0, weapplyLemmalto~=b(u) and¢= b (et + a + maxqr u) in the maximumcase and to ~ = b (~ninq. r u - ~ - et) and ¢ = b(u) in the minimmncase. In both cases, at a testpoint (x,t) E QT as in (9), we can follow the proof of Theorem 1 in order to obtain b~(u) > 0 and cOt¢-cOt~ > br(u)e > 0 at (x,t) and conclude ~o < ¢ in Q~.. As b is strictly increasing, the assertion is shown. ~
ACKNOWLEDGEMENT The author thanks the anonymous referee for helpful comments, as well as M. Cuesta and C. De Coster for stimulating discussions.
REFERENCES 1. 2.
3. 4. 5. 6. 7.
H.W. Alt and S. Luckhaus. Quasi-linear elliptic-parabolic differential equations. Math. Z., lS3: 311-341, (1983). J. yon Below and C. De Coster. A qualitative theory for parabolic problems under dynamical boundary conditions, to appear in J. Inequalities and Applications. J. yon Belowand S. Nicaise. Dynamical interface transition in ramified media with diffusion. Comm.Partial Differential Equations, 21: 255-279, (1996). Ph. B~nilan, J. Carrillo and P. Wittbold. Renormalized entropy solutions of scalar conservation laws, preprint, (1999). Ph. Bfinilan and P. Wittbold. On mild and weak solutions of elliptic-parabolic problems. Advances in Differential Equations, 1: 1053-1073, (1996). O.A. Lady~enskaja, V. A. Solonnikov, and N. N. Ural’ccva. Linear and quasilinear equations of parabolic type. Amer. Math. Soc. Providence RI, (1968). W. Walter. Differential and integral inequalities. Springer Verlag, Berlin, 1970.
Dirac Algebra
and Foldy-Wouthuysen
H. O. CORDES Department of Mathematics, University Calitbrnia
Transform
of California,
Berkeley,
ABSTRACT Weoffer further results and a matured physical interpretation, concerning our invariant algebra P for the Dirac equation discussed in 1983 [1] and 1996 [2]. Especially, P may be fully described either with simple spectral theOry of the Hamiltouian or with a decoupling modulo order -c~ of the positive and negative energy parts of the Dirac equation, similar to the Foldy-Wouthuysentransform. There seems to be evidence indicating that only operators in P qualify as observables--i.e., can be measured with arbitrary precision--a feature comparable to the Heisenberg uncertainty relation.
0
INTRODUCTION
Wewill discuss properties of the Dirac equation O¢/Ot + iH¢ = O, (t,x) with Hamiltonian H = h(x,D),
= (t,x~,x.~,x3)
~
(0.1)
D = (D1,D2,D3), D1= -~0i ~1, where 3
h(x,~)
= Eaj(~j
-Aj(x))
+~+V(x),
with certain constant complexself-adjoint 4 × 4-matrices a j, ]~, and electromagnetic potentials (V(x),Aj(x)). Physical constants li, c,m,e are set = 1. Note, (0.1) represents a first order sym~netric hyperbolic syste~n of 4 PDE’s in 4 unknown functions ~ = (¢~,..., ¢4)T. The differential operator H is self-adjoint with respect to the inner product of H = Le(K~,C~). The symbol h(x,~) is a self-adjoint 4 × 4matrix with two real eigenvalues A~: of constant multiplicity 2 each: £±(x,~) = V(x) :t: V/1 + (~ - :. 335
(0.3)
336
Cordes
With proper assumptions on smoothness and growth of the potentials (0.1) will a semi-strictly hyperbolic system of pseudodifferential equations of type e’ = (1,0), in the sense of [1], [2], since the eigenvalues (0.3) satisfy ~+ - A__> c(1 + I~]), c for large Ix[ + For such systems we discussed the existence of an invariant algebra P of global pseudodifferential operators. Invariance means that the algebra remains unchanged under conjugation A ~ E*AE with the time propagator E = e -itt4 of equation (0.1). Details in Theorem1.1. Weare used to the following Dirac matrices aj, a
= -ia {71-----
0 -i
0
’ /3 = ’ ~ =
0 -1 1 0 ’
(0.4) ~r 3 ~
0 -1
.
In all of this paper we employ global pseudodifferential operators (0do’s) A a(x,D) ~ OpOcm, m = (m~,m~) ~ of "st rictly cla ssical" typ e: A s ymbol a(x, ~) e ~Pcmis O((x) m~(~)’~), (p) = v/~ ’2, its d eriv atives -(~) ~O:~a are O((x),~ {~)m),/~ = mr- ]¢~1,/~ = m~_-1/31, for all multi-indices a,/3. m= (m~, is the "order" of a and A. Assumptions are rigged such that h(x, e~ = (1,0). Wealso use ~ =(0,1), e = (1,1) fo r sp ecial or ders. Op erators in Op~bc= UOp~bCm obey a global "calculus of Cdo’s". Especially there are Leibniz formulas "with integral remainder" and "asymptotic Leibniz formulas" for products and adjoints. Details in [2], I. Our main results are formulated in section 1 and proven in section 2. [Theorem’s 1.1 and 1.2 were discussed in [1] and [3], dating back to 1983.] Here let us attach some physical comments. Equation (0.1), as relativistic wave equation of an electron or positron moving an electromagnetic field with potentials (V, A) was in the center of physical interest during the early 1930’s and later. It is likely that, at that time, the existence of an invariant algebra like P was not known. A Cdo .4 = a(x, D) Op¢c,~ may be regarded as bounded operator H -~ H-m (with the "polynomially weighted" ~Sobolevspace Hs---with normII(x) ’~ (D)s~ ’allL2 ). If mr, m.2 _> 0, then also A defines an unbounded operator of H with domain H.,n C H. Assuming that A* = A, with the formal Hilbert space adjoint ..... of H, one may show easily that every "rodelliptic" such operator is a self-adjoint operator of H. Moreover,every formally selfadjoint such operator of order e or e~ or e 2 admits a unique self-adjoint extension-its closure. [Not true for higher orders!] With this preparation we can state that our algebra P--or at least its formally self-adjoint operators of order e, e1, e2, (or of order 0 or of arbitrary order if rodelliptic) classif~ as physical observables. [In particular, location--the multiplication operators by x~, x.2, xa, momentums-thedifferential operators -ihO~,,..., angular momentum,energy, all are represented by differential operators, belonging to Op$c.] Also, conjugation with e -iHt of mr Observable A amounts to the "Heisenberg transform"--it defines the same observable A at time t, assuming that the physical states (the unit vectors of H) remain fixed. In other words, the self-adjoint elements of our algebra P have the property that they remain ¢do’s for all times.
Dirac Algebra and Foldy-Wouthuysen Transform
337
It is trivial that the energy observable--the operator H, commutingwith e belongs to our algebra P. Tile same is true for the total angular momentum,if the potentials are rotationally symmetric (because that operator com~nutes with H). But uone of the other above standard observables have this property--although "corrections" for them may be found, using Theorem1.1. Now,ibr these "other" observables a feature called "Zitterbewegung" was discovered, already in early Dirac theory--just this fact; their time propagation seems "unphysical". An electron moving with vanishing fields is calculated to execute a rapid oscillatory motion. For the case V = A = 0 several corrected observables were proposed, not exhibiting this oscillation feature, but none of these corrections proved entirely satisfactory ([4], Chapter 1). Our corrections ([1], p. 90) for more general potentials have similar features or are identical. But if we are allowed an opinion, in this context: Wesuggest to allow only the self-adjoint operators of P as true observables. They can be observed since they are stable in time. Measuring another observable--such ~ the space coordinate x~, for example, should amount to finding an element of P which is "close" to x~. Such elements exist, but are not unique. For example, for x = (Xl, x2, x3) we might propose
Xcorr= ¯ - ~c(x, D),
with
the
matrices
~ = e 0 ’ p = 0 e
the physical constants B,m, e, c. Only the first correction was added~there are countably many others, of lower and lower order. Still, an inspection seems to indicate that the correction is of order of magnitude ~the Compton-wavelength of the electron. It is knownfrom experiments [5], [6], [7] that this is the lower limit of accuracy for measuring the position .of an electron. Generally, this see~ns to be a matter similar to the Heisenberg uncertainty relation, which says that position and momentumcannot be measured simultaneously without a definite uncertainty. Here we are suggesting that only observables within P can be measured with arbitrary precision. Location x is not in P, but may be approximated by elements of P with accuracy about h hence it only Can be measured with that accuracy. In [1], [2] we madesimilar reflection with other observables. Here let us point to the following: Assume A(x) ~ 0, and V invariant under rotations: V = V(r), r = ]x~. would like to choose V = ~ = Coulombpotential, with a constant c ~ 0, but then must ’cap’ the singularity at r = 0 to create a C~-function, which then satisfies our general assumptions of section 1. With this V we set up equation (0.1). But also, the potential V should be observable. P does not contain V, but Theorem 1.1 will give V¢orr = V(txl) - E(x). ~c(x, (0.6) with E = grad V = electrical field strength, Ac, of (0.5). Here one finds that the correction symbol E(x)Ac(x,~) tends to get large near x = 0 for not too large [~[ if our cap is applied very close to 0. An interpretation of this: The potential V can only be measured if the electron is not too close to the point 0.
338
Cordes
One then might ask for the physical meaning of Vcorr. Especially: ]is this an expression for the fact that ’other’ forces are acting if the electron gets very close to the nucleus? In particular, since gauge theory suggests a vaguely related theory for a unification of electrical and weakforces ([8], [9]), does the present approach have any meaning, in that context? The author feels very indebted to A. Unterberger and G. Lumer for providing a challenge and encouragementfor continuing the present work (cf. also [10], [11]).
1
INVARIANT ALGEBRA FOLDY-WOUTHUYSEN
Wesummarize some results,
AND TRANSFORM
partly published earlier.
General assumptions: For a(x) = V, Aj require a(a)(x) = O.~a(x) = O((x)-I"l), I~3, for a ll ~ .
(1.1)
Then the (4 x 4-matrix-valued) symbol h(x, ~) and the eigenvalues )~±(x, ~) all belong to ¢c~. Note: No singularities allowed. THEOREM 1.1 Define a class P,~ C Op~PCmof ~Pdo - s A with 4 × 4-symbols a such that (i) At e~Hta(x, D) -ilit ~ Op¢cm, for all t (ii) At ~ C~(I~, Op~bc,n); (iii) O~A~ ~ C(I~, Op¢c,~_ke~), k = O, 1, 2,.... Assertion: (1) For = a(x, D)~ Pm the symbol allo ws a de composition a=q+z, with z Egmm-~, [h,q]
a. :0, x,~ 6 I~
(].2)
(2) Vice versa, if a symbol q ~ ¢c,~ commuteswith h for all x,~ ~ ]~a, there exists z ~ ¢cm-~ with A = a(x,D) E P,~, for a = q + z. Here the "correction symbo|" is an asymptotic stun z = Zz) (rood O(-c~)), with solutions z~ of order commutator equations, recursively, where zj_~ must be adjusted to insure solvability for z~. (3) Suppose A~, A: ~ Pm(both must have a decomposition (1.2)) have the q. Then b = z~ -z~ is symbol of b(x, D) Pm-~; it all ows (1. 2) wit h m- e i nstead of PROOFCf. [1],
Theorem 2.1.
THEOREM 1.2 Under our general assumptions on V,A, there exists operator U of H which is a Cdo : U = u(x, D) Opec0, su ch th at
= 0
H_
a unitary
= r 0 ’ (1.3)
where H± ~ Op~bc~, while F E O(-~x)) is of order -~c. (H± and F are 2 matrices of¢do-s.) The symbols u, h± of U, H±are asymptotic sums, u =
Dirac Algebra and Foldy-Wouthuysen Transform
339
h± = )~+ + Ehj. ; uj and hj:~ are obtained recursively, solving certain cmnmutator equations. Here A+of (0.3) and u0 of (1.4) relate to the diagonalization h(x, ~):
uo=
1+
0
1+1+(.---7 ’’=
u~u0 = 1, x,~ e ]R3, while H±= )~±(x, D)(mod(Op¢c_e~)),
0) {1.4)
with the eigenvalues A+of (0.3). PROOFCf. [3],
Theorem 1.1.
Note: The unitary operator U "decouples" the Dirac equation modulo O(-oo) into a pair of 2 x 2-hyperbolic systems of ~pde’s. An "approximate decoupling" was done in different setting by Foldy and Wouthuysen[12], with similar first few terms. There is work on more precise decoupling under special assumptions([4], p. a09,[13],[14],[15]). For Theorems 1.3, 1.4 below we add the general assumption that the potentials V and A assume a limit as Ix[ + oo. We then may assume (V°,A°) = lim]:rl_~(V(x), A(x)) = 0, since a conjugation of 0t +iH with expi(A°x carries (0.1) into that equation with potentials (V-V°, A-A°) while a Cdo a(x, D) is carried into a(x, A°-D). Moreoverthen, we require that V(a) (x) for all a. Under these assumptions Theorem 1.1 and Theorem 1.2 are related as follows: THEOREM 1.3 The class P,~ of Theorem 1.1 precisely A ~ Op¢cm with
U*AU = D E . ( B C ) whereB,
consists
E~Op¢cm,
of all operators C,D~O(-oo).
Theorem1.3 was indicated in [2], 10. A detailed proof is ibund below. THEOREM 1.4 Let 0 ~ Sp(H), let P± be the spectral projections and (0, oo). Then P,,~ precisely consists of A ~ Op¢cmwith
of H to (-co, 0)
P+AP_,P_AP+ ~ 0(-oo).
(1.5)
THEOREM 1.5 Let the potentials vanish. Then the graded algebra P = i0Pm is invariant (covariant?) under a proper Lorentz transform: Passing from coordinates (t, x) to coordinates (t’, x’) a physical state at t = 0 is turned into a physical state at t’ = 0 by a unitary map R : L2(t = 0) ~ :(t’ =0)--we fo llow th e so lution of (0.1) from t = 0 to t’ = 0 and use a transform of dependent variable, a relativistic contraction. This R also relates P and P’ : P’ = RPR*. PROOF For Theorem 1.5 cf. [16]; for Theorems 1.3, 1.4 see section 2, below.
340 2
Cordes PROOFS AND LINK
TO THE SPECTRAL
RESOLUTION
OF H
Somecomme,~tson spectral theory of Dirac operators with our kind of potentials: H = Ho + Z(x), with matrix-valued Z(x) = V(x) - ~A(x), and H± of (1.4} eI -md-elliptic (cf. [2], II): For large Ixl+l~l we have lh(x,()l > p(~), Isytnb(S±)I > p(~), with p > 0. The same for H - z, H± - z, if Re z it 0, or Izl < 1 [even for sz 2Ax)/ = 0, ((~ +z )+ < (~ 1 -A)) for H±]. We get A+ = (~)+{V+(A where the brackets give a bounded Cdo, while :t:(~) gives H~ = :t:(D), unbounded self-adjoint in He~, diagonalized by the Fourier transform. Hence H±also is selfadjoint in He~ = dora H±. The same argument works for H0 and H : u0 of (1.4) (with A = 0) diagonalizes h0; Ho then is unitarily equivalent to multiplication the diagonal matrix diag((~), (~),-(~),-(~)), with ess.Spectrum = L_ U ess Sp(H°~) = L±, with the half-lines L± ={1 < :t:z < ~c}. For H,H±and Ho,H°~ the difference of resolvents is compact--for example (H0 - i) -~ - (H - i) -4 = (H - i)-~Z(x)(Ho -~ is a product of Z( x)A(D) ~ K(H), A(~) = 1/(~) bounded operators using that a(x)b(D) is compact whenever a(cx3) = b(co) Hence H,H°~ also have essential spectra L+ U L_, and L±, respectively. Their resolvents are meromorphic flmctions in the complement sets. That is also where we found these operators e~ - rod-elliptic. By [2], III, Theorem4.1, H - z, H±- z have a Green-inverse for z ~ C\L+\L_ (z ~ C\L± ), their eigenvectors to eigenvalues in these complementsof their essential spectrum are rapidly decreasing (belong to
S).
Wealso need the resolvent (J- z) -~ of a ¢doJ ~ O(-~). Then J- z, 0 ~ z ~ always is 0 - md-elliptic, hence admits a Green inverse. All eigenvectors of J to z it 0 belong to S. Note, for J = H, H+, or J ~ O(-oc), even the eigenvectors of J : ~ - + S~ belong to S, for eigenvalues z ~ C\ess.Sp. ([2], III, Theorem4.1--for a more general theory of this "spectral invariance" cf. [17], [18]). In particular, the eigenspaces of J as (unbounded) map between any pair of Sobolev spaces Hs, H~ are independent Also, the resolvent (J - z) -~ is a ¢do[~ Op¢c_e~for H, H±~ Op¢co for O(vc)], and even the special Fredholm inverse Iz, defined at an eigenvalue z as inverse of (J - z) [ Ira(J* - ~) : Ira(J* - z) -+ Im(g - z), and 0 in ker(g - z) = (Ira(J* ±, belongs to Op¢cm, m = -e ~ for H, H±, m = 0 for O(-oc). Weneed the following result: LEMMA 2.1 For some s ~ ll~ ~ let A ~ Op¢c,,~ be Fredhohn in L(Hs, H.~_,~). Then there exists a Fredholm inverse B ~ Op¢c-mwhich also is a Green inverse, and A is rod-elliptic. Specifically, if A is invertible then A-t (the only Fredhohninw~rse) belongs to Op¢c_,~. PROOFWeremind of the fact that fl~ = ~r,.(x,D) = (x)"~(D) ’’~, with ~r~(x,~) (x) ~ (~)"~ defines an isomorphismH~ -+ Hs-,., for every s, r, and that II,. ~ Op¢cr has the property that II~-lAIIr
- A ~ Op¢c_~ C K(Hs), for A ~ Opec0, all s,r,
(2.1)
with the compact ideal K(Hs) ([2], III, 5). For Letnma 2.1 we may set m = 0 [nsing II_,~A instead of A], and then s = 0 [using H-~AIIs instead of A].
341
Dirac Algebra and Foldy-Wouthuysen Transform
Thus we now are looking at a Fredholm operator A E Op¢co. Such an operator must be 0 - rod-elliptic, by [2], V, Theorem 10.3. Indeed, A belongs to the C*algebra closure of Op~bco, hence is Fredholm in L(Ho) if and only if its algebra symbol does not vanish. That is, we have Isymb(A)l >_ p > 0, as Ix[ + I~1 large--i.e., A is 0 - md-elliptic. Using [2], III, Theorem4.3 again, conclude that ker.4, ker A* C S. Nowconsider the operator C = A* A + Pker A, with the orthogonal projection Px onto the closed subspace X C H. Clearly PkerA E O(--CK3), and thus C ~ OpCcois invertible in L(H). PROPOSITION2.2 For .4 ~ L(H) consider
the function
Az,~ : e-izDei~Zde-~xe -izD, z,~ ~ ~3.
(2.2)
Then A belongs to Opec0 if and only if Az,; ~ C~(ll~ 6, L(H)), ((x)l#l(o~O~Ao,o)(D)l~l)..,(
C~(IR6,L(H)), for al l c~ ,/3.
(2.3)
PROOFIt was shown in [2], VIII, Theorem 2.1, that the first condition holds if and only if A = a(x, D) with a(x, ~) CB~(]~ 6) = {C~-functions wi th bo unded derivatives}. For such a(x, ~) and A = a(x, D) we get Az,; = a(x + z, D + ~), hence O~O~Az,~= ^(~)’- + z, D + ~).
(2.4)
But we note that
= e
e C"for all
(Z.5)
If in addition to A:,; ~ C~ we have (2.3), then the operator at left (which symbol(x)I~l (f~,,,l~l~,~) a(~) ~, ~)) belongs to Op¢c0--i.e., its symbolsatisfies (2.5), firming the proposition. [For a virtually identical criterion cf. Beals [19].] REMARK 2.3 The condition A~,¢ E C~(II~,L(H)) reduces to "existence 0za 0~A0,0in L(H) for all a,/3", since 0]0~Az,~ = (O]OgAo,o)z,¢, and using that the condition is imposedfor all c~,/3. For the above operator C, it is clear then that C-~ ~ Opec0, and, moreover, that (C - A)-1 ~ Op¢co for every A e C\SpC where SpC C [e,I/e], some e 0. Indeed the condition of Proposition 2.2 applies to A-~ whenever it applies to A, assuming that A-~ ~ L(H). Moreover, we get the positive square root B = C~/2 = ~ ifr(C - A)-~v/~dA E Op¢co: The contour F above will be in Re A > 0, surrounding Sp(C); we get Bz,¢ : ~ 1fr(Cz,; - A)-~ v~dA. Differentiating this for z, ~ we get other well defined complex integrals, converging in L(H): For example O~,(C~,; - A)-~ = -(C~,¢ - A)-~(0~C~,¢)(C~,¢_~) -~, etc., .... Note, we get [(x/, (C- -~] = (C- A) -~[C, (x )](C- A)-~, where IV , (x /] e Op¢c_¢, et c. As a consequence, the operator B will satisfy the conditions of Proposition 2.2, so that B ~ Op¢co. Returning to the proof of Lemma2.1, the polar decomposition A -- QB, where Q = AB-~ ~ Op¢co, then takes place entirely within Op¢co. Note here that
342
Cordes
Q*Q= 1 - PkerA, QQ*= 1 - PkerA*. The first is trivial; for the second, let QQ*u = A(A*A + Pker.~)-lA*u = w. Clearly Q*Qu = 0 if u E kerA*. Let u e (kerA*) ± = hn A. Then u = Av, w = A(A*A + PkerA)-IA*Av = A(1 - Pke~.A)V. Wemay choose v _1_ ker A, then w = Av = u. So, QQ*= 1 in Im A = (Pker ’~)±, but QQ*= 0 in ker A*, confirming that QQ*= 1 - PkerA*. To construct a Green inverse of A, set G = B-1Q* ~ Opec0. Then GA = B-~(1 - Pke-~)B = 1 - Pke~, trivially, while AG = QQ* = 1 - PkerA’, also trivially, q.e.d. In fact we can state COROLLARY 2.4 Under the assumptions of Lemma 2.1 the special (uniquely characterized) Fredholm inverse F with FA = 1 - P~,erA, AF = 1 - Pker A*, with orthogonal projections with respect to the inner products of H.~ and Ht, respectively, are Green inverses. COROLLARY 2.5 For the operators J = H,H+ the resolvent (J - z) -1, z ~ C\Sp(J) as welt as the special Fredholm inverse of J - z, at an eigenvalue z in z = 0, Izl < 1, belong to Op¢c_~. Indeed, for real z the operator V = J- z is self-adjoint; the operator V + Pk,;~ ~. = W: H~ -~ H0 is invertible, hence W-~ ~ Op¢c_~. The desired special Fredholm inverse is given as G = (1 - Pkert,’)W-1; it clearly belongs to Opec_e,. For the resolvent we may directly apply Lemma2.1 to (J - z),k(D) (which is invertible in L(H)). Q.E.D. Next we want to focus on certain spectral projections of H, H+. These operators are self-adjoint, and we knowtheir essential spectra to be L+ U L_, L±, respectively. Consider the integral I,~ = ~ (J - ,~)-ld,k,
J = H,H~=., F = {Re ,~ = ~}, directed upwards, (2.6)
where we assume that ~ is not an eigenvalue of J. For the calculation assuine ~ == 0. The integral is assumed to be a Cauchy principal value at +ee, it then exists in norm-convergence of H. Write =
+
, and set A = ip, for
(2.7) Io = Io(J) = -~r
J(J~ + #’))-~d# = - sgn(J),
where we used the spectral resolution J = f vdE(v), and that .f~’~ v-~dv = ~sgn(v). This is important because we get E(t~) = ½ + I~, while it can be shc,wn that I~ is also meaningful in L(H~), for all s, so that E(n) e Op¢co, due completeness of Opec0 under the Frechet topology induced by all H.,-norms ([2], VIII). Indeed, we know that, for J as map H~ -~ H~, ker(J - ,~) is independent o:[ hence (J - 30-1 exists in L(H~) for all ,k ~ F. Moreover, using the isomorphism l-Is : Hs -~ H of Lemma 2.1, get II~(J- A)II~ -~ = J- A + Z~, where Z~ = II~JH; "1 -J e Op¢c_e~ e L(H). It follows that II~(J-A)-~II; -~ = (J-,~+ Z~)-~ =
343
Dirac Algebra and Foldy-Wouthuysen Transform
((J - A)(1 + (J - A)-1Zs)) -~ = (1 + Ws)~)-l(,] ,~ )-1, where Wsx = (J - A)- ~Zs is small as IA[ gets large. Similarly for (j2 + #2)-1. Thus indeed, the integrals (or the principal value) converge also in L(Hs), for all s. Wehave proven: PROPOSITION2.6 The spectral projections E(A) of each of the operators H, H’x, H+ of Theorem 1.2 all belong to Op~co, as long as A E ll~ belongs to the resolvent set of the corresponding operator. Focusing first on the proof of Theorem1.3 use the Cdo U of (1.3). (0.1) substitute ~b = Uw, and left-multiply by U* for
=
0
H_
’
=
r
0
’
In equation
(2.8)
Wehave decoupled the Dirac equation (modulo O(-~)) into a O¢/Ot + iH+¢ = 0
(2.9)
of2 x 2-systems, using ¢ for w again. Each system (2.9) is symmetric (semistrictly) hyperbolic (of type e~)--with the additional property that H+= A+(x, (mod Op~bc_e~): There is only one eigenvalue of the symbol, modulo order -e 2 = e ~ - e. Theorem5.1 of [1] maybe applied, together with the following corollary: PROPOSITION 2.7 Under the assumptions of [1], Theorem 5.1, if there is only one eigenvalue A(x,~) (of multiplicity n) (where n = 2 here) then the algebra coincides with Opec: It contains all strictly classical Cdo’s. PROOF Wediscuss only our special case with b of [1], (5.1) equal H = ,~(x, D) hi(x, D), h~ 6 ~ee~ - e, ,~ a multiple of 1. Clearly every symbol q E Ce.m commutes with ~, and we thus may construct a z of order m - e such that Op(q + z) ~ Again -z commuteswith ,~, hence an s of order m - 2e exists with Op(-z + s) ~ hence Op(q + s) 6 P. Iterating this we find that a correction w of any finite order may be fouud to bring Op(q + w) into P. It follows that q(x, D) itself belongs to P, as stated. Returning to 4 × 4-matrices we note that both the system (2.8) and the (fully decoupled) system O¢/Ot +iHA¢ = 0 (2.10) are semi-strictly hyperbolic of type e~, and thus must have their invariant algebra P~’ and Q, respectively. Clearly, e",(H" +ra)~’ = U¯ e",HtU, hence also pzX = U*PU. On the other hand, we claim that the algebra pa and Q are identical. look at Zt = ei(g’~+r~)~e-~H~t. Weget OtZt = ei(Ha+ra)tFAe--iHat ~ C°°(N, O(-eo)).
(2.11) Indeed,
(2.12)
344
Cordes
[Note, especially, the families e i Jr, .] : H, HZ~,H/x+ FA are of order 0, theiir derivatives are of order ke~, k = order of derivative, since e i:~ is evolution operator of a symmetric hyperbolic system ([2~, VI, Theorem3.1).] Integrating (2.12) we e i(Ha+ra)~
= (1 + O(t))e ~ = (1 + P(t))e iHa~, O,P e C~(~,O(-~)).
(2.13)
This indeed implies P~ = Q and, of course, P,,~ = Qm, m ~ ~. After Proposition 2.7 we expect Q,~ =
where A,D ~ Op¢c,~, C D B, C ~ O(-~). This will complete the proof of Theorem 1.2: LEMMA 2.8 For A ~ Op¢c~, ifeiH+tAe -i~-t Op¢c,~_je~, for all t, then A ~ O(-~).
= Qt ~ Op¢cm, and if also OjQt
PROOFNote Qt : Rll.~, Rt : eiH+tAe-iH+t ~ Opec,n, ~. : eittt+e-it~-t. Sim~ ilarly, OtQt = cht(A)t’~, with chl(X) = eiH+~(H+X- XH_)e-iH+~ e Op¢c,,.+~, as X ~ Op¢cm. By induction define ch2+~ = H+chJ - chill_, and chj(X) -iH-t. ei~+tchJ(X)e Then ch~(X) e Op¢cm+je~, as X ~ Op~c,~, and by our assu~nption. Nowwe claim that chj ). (A) = 2J Y~ d(mod Op¢Cm+(j_l)e~_e~
(2.15)
Indeed, this may be proven for t = 0 only, using Proposition 2.7. For j =: 1 get ch~(A) ch Y(A) = H+A- AH _ = H+A- A( 9_~ H+) = 2H+A + [A,H+] + ~_~ = 2H+A + ~_~, where ~ generally denotes some operator of O~cr. We used the special assumption on V(x) and (1.4) for H_ = 2V(x)(mod Op~,c_e~), i.e., H_ = ~-e~ -H+, since V ~ ~c-e~. By induction assume that chJ(A) = 2JH~A + ~m+(j-~)~-~. Then ch j+l (A) H+(2:iH~A + ~,n+tj-~)e~-e:) - (2JH~A ~m+(j_~)~_e~)(9_e~ H+). We H~AH+= H?~A + ~m+je’-~,
so, chJ+~(A) = 2J+~H?~A ~, ,+2~,_~:, pr
oving
Nowwe combine (2.14) and (2.15). Note that A = 0 belongs to the complement of ess.sp(H+), so that 0 at most is an eigenvalue of finite multiplicity. By Corollary 2.5 the special Fredholm inverse (for simplicity called H~~) inverting H+ in (ker H+)x =Im H+, and defined 0 in kerH+ belongs to Opy)c_e~. So we get .4~ = 2-JY~Ych~(A) + ¯ .... e = 9,,,-e
+ ~,,~-j~l~ -~, J = 1,2,....
(2.16)
Weclai~n that (2.16) implies that At ~ Op¢cm-~, hence A e Op¢cm_e~. Indeed, the unitary operator Vt-~ is O(0), since the exponentials exp(iH&t) are evolution operators of symmetric hyperbolic systems. Hence Wj = 9m-j~-~ e O(m -- je). For large j the distribution kernel of ~Vj becomes s~noother and its derivatives will decay faster. We may write Wj ~ formal Cdo ~ith symbol w~ wj = O(((x)(~))-l), as j > j(1). Note (2.16) implies equality of symbols symb(At) must satisfy the first few estimates for ¢c,n-~, as j gets large, he:ace symb(At) ~ ¢cm-~, since (2.16) holds for all j. Thus A 60p¢c,,~-~. Iterating A ~ Op~c,,~-ke, k = 2,3,... ~ A e O(-~), q.e.d. With the proof of Lemma2.8 the proof of Theorem1.3 is complete. Then Theorem 1.4 will follow if we look at the spectral projections P = E(0) and p/X = Ez,(0}
Dirac Algebra and Foldy-Wouthuysen Transform
345
H and HA + FA, respectively. (Assume 0 is not an eigenvalue of H and A +FA= U*HUor else take P = E(e) and pa = EA(e) for suitable small e.) We pA = U*PUas well. Let Q = 1 - P, QA = 1 - pA. Then p,Q, pA,QA E OpOco. Let P’, Q’ be the corresponding projections for the operator HA. Then Pa - P’ may be expressed by a difference of resolvent integrals (2.6), with a - z) -~ (HA + F~ - z)- ~ = (Ha - z)- t x a ( a + FA- z )- ~ e O (- ~). I ntegrals conve rge in L(Hs) for all s, as for Proposition 2.6. Hence Pa - P’, Qa _ Q, e O(-~).
Thec°nditi°ns°fThe°rem 00) m°dO(-~)" 1.~ may thus be formulated as P~AQ~, Q~AP~ ~ O(-~). Since P~ U*PU, ~ = U*QU,it is then clear that they equivalently may be fomnulated as (1.5). Q.E.D. als°P~=
( 00 0)i
, Q~= (10
REFERENCES 1. 2. 3. 4. 5. 6. 7. 8. 9. 10.
11.
12. 13. 14. 15.
HOCordes. A pseudo-algebra of observables for the Dirac equation. Manuscripta Math 45:77-105, 1983. HOCordes. The technique of pseudodifferential operators. London Math Soc Lecture Notes 202; Cambridge University Press, 1995. HOCordes. A pseudodifferential Foldy-Wouthuysen transform. Commin Partial Differential Equations 1983;8(13):1475-1485. B Thaller. The Dirac Equation. Berlin-Heidelberg-New York: Springer Verlag, 1992. WHeisenberg. Gesammelte Werke. Berlin-New York: Springer, 1984. A Sommerfeld. Atombau und Spektrallinien 1,2.5th ed. Braunschweig: Viehweg and Sons, 1931. E Wichmann. Quantenphysik. Braunschweig: Viehweg und Sohn, 1985. D Shirkov, N Bogoliubov. Quantum Fields. Reading, MA:Benjamin, 1982. A Pais, M Jacob, D Olive, M Atiyah. Paul Dirac. Cambridge: Cambridge University Press, 1998. A Unterberger. A calculus of observables on a Dirac particle. Preprint 96.02, Dept Math Univ de Reims, URA1870, 1996. To appear Ann Inst H Poincare (Phys Theor). A Unterberger. Quantization, symmetries and relativity. Preprint 96.09, Dept Math Univ de Reigns, URA1870. Perspectives on Quantization, Contemporary Math, AMS214:169-187, 1998. L Foldy, S Wouthuysen. On the Dirac theory of spin -7 particles. Phys Rev 78:20-36, 1950. E deVries. Foldy-Wouthuysen transformations and related problems. Fortschr d Physik 18:149-182, 1970. DRGrigore, G Nenciu, R Purice. On the nonrelativistic limit of the Dirac Hamiltonian. Ann Inst Henri Poincare - Phys Theor 51:231-263, 1989. B Thaller. Normal forms of an abstract Dirac operator and applications to scattering theory. J Math Phys 29:249-157, 1988.
346 16.
Cordes
HOCordes. Lorentz transform of the invariant Dirac algebra. Integr Equ Oper Theory 34:9-27, 1999. 17. B Gramsch. Relative inversionin dcr Stoerungstheorie von Operatoren und ¢-algebren. Math Ann 269:27-71, 1983. 18. E Schrohe. Spaces of weighted symbols and weighted Sobolev spaces on manifolds. Springer LNMVol 1256:378, 1987. 19. R Beals. Characterization of pseudodifferential operators and applications. Duke Math J 44:45-57, 1977.
On Perturbations for the Continuous Spectra of Semigroup Generators MICHAELDEMUTH Institute of Mathematics, Clausthal- Zeller feld, Germany
1
TU Clausthal,
Erzstr.
1, 38678
INTRODUCTION
In mathematical scattering theory the completeness of wave operators implies the stability of the absolutely continuous and can be used to discuss the behaviour of the singularly continuous spectra. Using the invariance principle the completeness problem can be shifted to the theory of semigroups. The absolutely continuous spectra are invariant if sandwichedsemigroupdifferences are trace class. The singularly continuous spectrum remains empty if semigroup differences decrease sufficiently fast. In stochastic spectral analysis this implies the stability for the spectra of generators of Markovprocesses. In the case of singular perturbations sets of finite capacity have no influence on the absolutely continuous spectrmn. There are sufficient conditions in terms of the equilibrium potential such that the singularly continuous spectrum remains empty.
2
SPECTRAL
INVARIANCE
AND SCATTERING
THEORY
The ~nathematical scattering theory has its origin in quantum mechanics where the dynamics of two quantum systems is compared asymptotically in large time scales. From the mathematical point of view it is a tool in the perturbation theory for the continuous spectra of self-adjoint operators. Let A,B be operators in different Hilbert spaces 7/~, 7-/2, respectively. Assume A, B to be self-adjoint and bounded below. Let J be a bounded identification operator mapping741 to 7/2. Let Pac(A) be the projection operator onto the absolutely continuous subspace of A. Waveoperators are defined by 347
348
Demuth Ft+ (B, J, .4) := s). - lime~tBJe-itApac(A
(Details in two-space scattering theory are given by Kato [8]). Introducing the polar decomposition ~+ = sgn (f~+) the wave operator g/+ is called complete if [sgn (f~+)]* sgn (D+)
(2)
sgn (Ft+)[sgn (f~+)]* Pac(B).
(3)
and For f~_ we have the corresponding definition. The operator sgn (D+) yields a unitary equivalence between A/p,~(A)7~, and B/poc(B)n~ such that the absolutely continuous spectrum remains invariant, i. e., aac(A) = a~(B).
(4)
The completeness problem was combined with the study of the singularly continuous part of the spectrum by results of Enss [6], [7]. The interested reader may find a smnmarizing and extended presentation of the Enss-method in the book by Perry [9]. If the waveoperator f~+(B, J, A) is complete and if its range satisfies ran[~+(B, J, A)] Pc(B)7-t.~,
(5)
it follows that there is no associated singularly continuous subspace, i.e., Psc(B)7-t~ {0}, im plying th e si ngularly co ntinuous sp ectrum tobe empty, i.e .,
(6) Here Pc(B), P~¢(B) are the projection operators onto the continuous and singularly continuous subspace of B.
3
STABILITY
CRITERIA
FOR
The Kato-Rosenblum-Birman-Pearson Lemmacombined with the invariance principle tells us that the wave operator fl+(B, J, A) exists if e-~J -.Je -A is a trace class operator (see e.g. Reed, Simon[10]). This can be generalized to sandwiched semigroup differences. CRITERION 1 Let A, B be two operators self-adjoint, Hilbert spaces 7-/~ and ~/.~. Assumethat 1) e-U(e-t~J - Je,A)e -A is a trace class operator,
bounded below, acting in
Perturbationsfor ContinuousSpectraof Semigroup Generators
349
2) (e-SJ - Je-A)e -A is a compact operator, 3) (J*J - l~tl)e -A is a compact operator, (J J* - ln2)e -B is a compact operator. Then the wave operator fl+(B, J, A) (and also fl_(B, J, A) exists and is complete implying O~c(B) = ~oc(A). ¯ (7) A proof of Criterion 1 is given by van Casteren, Demuth[1]. In the abstract theory of 2-summing operators the trace class property of a product of three operators can be investigated. This can be used for our situation when the Hilbert spaces are L2-spaces. THEOREM 2 Let 7-{~ = L~(#), ~2 = L~(~) be two different be self-adjoint, bounded below in these L2-spaces, such that
L2-spaces. A,B
e -A E B(L2(#), L°~(#))
(s)
e-~ e B(L~(~), L2(~))
(9) (10)
e-uj _ Je-A ~ 13(L°°(t~),
L~(~)).
Then the following assertions are proved by Eder, Demuth[5]: a) The sandwiched semigroup difference operator. Its norm can be estimated by
e-B(e-sJ-
Je-A)e -A is a trace class
(11)
eI[e-t~(e-t~ J - Je-’A)e-A[Itrac
where ke is the complex Grothendieck constant known to be smaller than ~r/2. I]’ I]~,~ denotes the normfrom L~ to ’~. L b) The operator (e-t~J - Je-~)e -A is. compact. Its operator norm can be estimated by ~. ]](e-s J - Je-A)e-A]] _< [[e-Al[~,oo
(12)
II(e-BJ - Je-A)e-Al[2, ~ [le-BJ-
je-Alloo,~ ¯
Note that in both estimates above the L~ - L°° smoothing of the semigroup difference e-BJ -- Je-A plays the crucial role. This seems to be a characteristic feature in manyspectral theoretical considerations. The last theorem is nowapplied to integral operators
in
Demuth
350
COROLLARY 3 Let A, B be self-adjoint, bounded below in 7-/1 = 742 :: L"(~.d). Set J = 1. Assume that A and B generate ultracontractive semigroups. Suppose for their integral kernels: supl(e-A)(x,y)l
< c, supl(e-U)(x,y)]
(13)
X,y
and sup~ /
I(e-d)(x,y)ldy
sup /I(e-’)(x,y)ldy
< c,
(14)
Set D := e-B - e -A. This is an integral operator, too. Denote its kernel by D(,., .). Then ao.c(A) a~c(B) if
f dx
j dy
(15)
ID(z,y)l
For additional information see also Demuth[2].
4
STABILITY
CRITERIA FOR asc
For time dependent completeness criteria one needs more information about the free evolution eirA. Hence we restrict our consideration to A = -A =: Ho in L’z($~d). In case of potential scattering with B = Ho + My, the standard assumption is
f
llMv(Ho + 1)-lM~(l.,ikr)lldr
< oo
(,16)
0
with the multiplication operators (U~f)(x) := ~(z).f(z).
(:17)
The condition in (16) is satisfied IV(:OI <_-’-~ c(1 + Ixl) for some ¢ > 0 and all [z I > R0, R0 large a~c(Ho + My) = ~ follows.
(18) enough. For such potentials
However,the condition in (16) is not applicable for singular perturbations, where B arises by imposing Dirichlet boundary conditions on a closed set F, called obstacle or singularity region. One possible way to include such singular perturbations consists in proving the existence and co~npleteness of ~t+(e-B, e-tt°) and show!rag ran[l~+(e -u, e-"O)] = P~(e-B)N = P~(B)T{,
19)
Perturbationsfor ContinuousSpectraof Semigroup Generators
351
with 7-I = L~(l~d). The following theorem is proved by Demuth,Sinha [3]: THEOREM 4 Using the notation from above assume that the wave operators f~=k(e-B,e -tt°) exist. Assume that we have two projection operators P+,P_ decomposing the Hilbert space and satisfying. P+ + P_ = 1,
(20)
s - lim P+e -it(exp(-H°)) = 0,
(21)
s - lira P_ eit(exp(-H°)) = 0,
(22)
(f~+(e-u,e -u°) --1) ¢(H0) P- is compact,,
(23)
(f~_(e-B,e -H°) - 1) ~b(Ho) P+ is compact,
(24)
(In (23), (24) ¢(.) is a special smooth function with compact support.) Then ran (a+(e -B, e-H°)) = Pc(B)7t and
The strategy of the proof is similar to that of Enss. He used a decomposition by defining P+, P_ via a transformation to the momentumspace. For the result here we defined the decomposition in terms of the spectral representation where ln(Ho) is diagonal. This possibility was studied by Perry [9], too. Howeverwe translated it to functions of H0. For an interested reader let me give the definition of P+, P_: DEFINITION 5 Let F be the Fourier transformation fl’om L2(~:~d,dx) to L2(~’t, dk). Let U be the transformation from L2(IRd, dk) to Le(~, db; L~(Su-~)) such that for smooth functions ~o (UF~(Ho)f)~(w) = ~(e~)(UF ~3 ~ b~t.
S d-1 ,
f
~ LZ(1Rd,dx). Let G be the Fourier transformation
(25) with respect to
Then we introduce P+f := F*U*G*Mx(~>o)GUFf,
(26)
P_ f := F* U’G* Mx(,~
(27)
Clearly, P+ +P_ = 1. The other conditions in (21) - (24) can be verified -xBe -xg° is compact for all A > 0 and if the extension of (e -s -e-H°)e-~°M(z)~+e a bounded operator. Weuse the abbreviation (x) := (1 + Ixl 2 1_
De~uth
352 Hence we can formulate the following theorem. THEOREM 6 Let H0 be the Laplacian in L2(~d). Let B be a sclf-adjoint ator, bounded below, acting in L-~(_~d). Assumethat e -’xB -- e -’xH°,
fl > 0, is
compact.
oper-
(28)
2 1_ Denote (x) := (1 + I )~. Le t th e ex tension of (e -B --
(29)
e-H°)e-H°M(~)l+~
be a bounded operator in L~(~d). Then B has no singularly
continuous subspace, or asc(B) =
¯
This theorem can be applied easily to the case where e -~B forms an ultracontractive sernigroup with a Gaussian estimate. COROLLARY 7 Let e-’xB be an integral (e-AB)(x,y), A > 0. Assume
operator
with the kernel
le-~’(x,y)l _< e A-~_1~_~ e
e~
¯
(30)
Denote the semigroup differences by D~ := e -:~" - e -~H°, A > 0.
(31)
Let dx / dy D:~(x,y)l(1
[y]:)~+~ < ~
(32)
for all A > 0. Then Theorem6 is applicable,
5
i.e. asc(B) =
APPLICATIONS
Werestrict ourselves here to singular perturbations. The Laplace operator Ho is associated with the Wiener process. Denote by E.~ {.} the expectation with respect to the Wiener measure, such that (e-~H°f)(x) -- E::{f(X(X))}
(33)
holds for all f ~ L~(~d). Denote the singularity region by F, where F is a closed set in ~d. Let its complement be denoted by Z = K/d \ F. The first hitting time of F for the Wiener trajectory X(.) (34) Sr := inf{s, s > 0, X(s) F}.
Perturbations for ContinuousSpectra of SemigroupGenerators
353
The family E.~{f(X(~)); Sr >_ A} restricted to L2(E) generates a strongly continuous semigroup in this space. Its generator is denoted by H~. e -’~H~ is an integral operator, the kernel of which is smaller than (e-~g°)(x,y). Dx = e -’xg° - e-~Hn has the kernel
The semigroup difference
Dx(x,y)= E~A{I}- E~’~{Sr>_ A} = E~A{Sr< A},
(35)
hereE.~"x{.} is theconditional Wienerexpectation. Moreover we have
/
IDx(x,y)[dx
< A}.
=
(36)
Thisis thepointwherewe canapplyCorollary 3 andCorollary 7. COROLLARY 8
LetH0,HE be givenas described above.
a) If Ez{Sr < A}dx < ~,
(37)
we get
b) If
aac(He) = aac(Ho) = [0,
(38)
f E~{Sr< ~}(1 I~l~)° <
(39)
+
for some a > 1 and all A > 0, we get
(4o) REMARKS The last results are related to the capacity of the singularity region F. The one-equilibrium potential of F is defined as vr(x) := E~{e-Sr,Sr
< co}
(41)
mapping ~d _+ [0, 1]. Clearly one has E~{Sr < A} _< e~vr(x).
(42)
On the other hand in this context the capacity of F satisfies
cap(I’) =f vr(x)dz.
(43)
354
Demuth
Hence a,.c(Hn) = aac(Ho) if cap(F) is finite. capacity is finite and if additionally vr(x)(1
Moreover, asc(He) is empty if the
(44)
for some 7 > 1. In both cases unboundedsingularity regions F are allowed. They can consist of a union of infinitely manyballs, if the dimension d is large enoughand if the radii of the balls are sufficiently decreasing.
REFERENCES J. van Casteren and M. Demuth, Completeness of scattering systems with obstacles of finite capacity, Operator Theory: Advances and Applications, 102:39 - 50 (1998). 2. M. Demuth, Integral conditions for the asymptotic completeness of two-space scattering systems, Helv. Phys. Acta, 71:117 - 132 (1998). 3. M. Demuth and K. B. Sinha, SchrSdinger operators with empty singularly continuous spectra, Preprint TU Clausthal, 1999. 4. M. Demuth, P. Stollmann, G. Stolz and J. van Casteren, Trace norm estimates for products of integral operators and diffusion semigroups, Integr. Equat. Oper. Theory, 23:146 - 153 (1995). 5. S. Eder and M. Demuth, A trace class estimate for two-space wave operators, Preprint TU Clausthal, 1999. 6. V. Enss, Asymptotic completeness for quantum-mechanical potential scattering, I. Short-range potentials, Comm.Math. Phys. 52:233 - 258 (1977). 7. V. Enss, Asymptotic completenes’s for quantnm-mechanical potential scattering, II. Singular and long-range potentials, Ann. Phys. 119:117 - 132 (1979). 8. T. Kato, Scattering theory with two Hilbert spaces, J. Funct. Anal. 1:342 369 (1967). 9. P.A. Perry, Scattering Theory by the Enss method, Mathematical Reports Vol. 1. Harwoodacademic publishers, Chur (1983). 10. M. Reed and B. Simon, Methods of modern mathematical physics, Vol. III: Scattering theory. Academic Press, NewYork (1979). 1.
Mathematical Study of a Coupled System Arising in Magnetohydrodynamics J.-F. GERBEAU and C. LE BRIS Cermics, Ecole Nationale des Ponts et Chauss~es, 6-8 av. Blaise Pascal, Champs-sur-Marne77455 Marne-La-Vall~e, France
1
INTRODUCTION
This work deals with the mathematical study of a system of partial differential equations related to a magnetohydrodynamic (MHD)problem. The MHDequations we consider govern the behaviour of an homogeneous incompressible conducting viscous fluid subjected to a Lorentz force due to the presence of a magnetic field. More precisely, we study a coupling between the transient Navier-Stokes equations and the stationary Maxwell equations. This model can be considered for example in industrial situations when the magnetic phenomenaare knownto reach their steady state "infinitely" faster than the hydrodynamics phenomena. Many mathematical works have been devoted to the study of MHDproblems. Weonly present here some of them briefly and we refer to [5] and A.J. Melt, P.G. Schmidt [10] for some more detailed overviews. The coupling between the transient Navier-Stokes equations and the transient Maxwell equations (without displacement current) has been studied in G. Duvaut, J.-L. Lions [3] and in M. Sermange, R. Temam[12]. Numerical methods conserving the dissipative properties of the continuumsystem in 2D are presented in F. Armero, J.C. Simo [1]. Less numerous works have been devoted to the fully stationnary MHD equations, namely a coupling between two elliptic partial differential equations (see for example M.D. Gunzburger, A.J. Melt, J.S. Peterson [7], J.-M. Domingez de la Rasilla [2]). Finally, let us mention an interesting alternative viewpoint which consists in considering the electrical current rather than the magnetic field as the main electromagnetic unknown(see A.J. Meir, P.G. Schmidt [9,10]). In the present work, the equations related to the velocity field are the transient Navier-Stokes equations whereas those related to the magnetic field are elliptic (see (2.1)-(2.8)). The difficulty is that the ellipticity of the equation for B depends 355
356
Gerbeauand Le Bris
the velocity field u. Briefly speaking, if the velocity becomestoo large, the system may become ill-posed. Under restrictive assumptions upon the physical data, we can however prove ~hat a strong solution exists and is unique at least on a time interval [0, T*] for sometime T* depending on the data (see Section 4, Theorem1, the result we prove here has been announcedin [6]). For this purpose, we give in Section 2 a presentation of the equations and the functional spaces, and we establish in Section 3 some preliminary existence and regularity results upon~ the magnetic equation. As soon as the magnetic operator is no longer invertible --- which may occur if the velocity becomes too large - we show in Section 5 that we can construct two distinct solutions to the system. This latter observation shows that the model we study here should be used only with great care in numerical simulations.
2 2.1
EQUATIONS
AND FUNCTION
The Transient/Stationary
SPACES
Model
Let fl be a sitnply-coImected, fixed boundeddomainin I1~3 enclosed in a (7°° boundary F. Weshall denote by n the outward-pointing normal to Ft. The transient/stationary problem we shall consider is the following : find two vector-valued functions, the velocity u and the magnetic field b, and a scalar function p, defined on flx [0, T], such that 0,u+u.Vu-r/Au divu 1 -curl (curlb) divb with the following initial
f-Vp+curlbxb
= =
0
= . curl (u x b) =
0
in ~,
in ~t,
(2.1) (2.2) (2.3) (2.4)
and bouudaryconditions : u b.n curlb×n
= = =
ult=o =
2.2
inQ,
in fl,
0 q k×n Uo
on F, on F, onF, in Ft.
(2.5) (2.6) (2.7) (2.8)
Functional Setting
For m _> 0, we denote as usual by Hm(Ft) the Sobolev space H"~(~)) = {u ~ L’~(Ft); D’ru ¯ L~(~),VT,I~l < ,,z}, where ~/= (3’~, 7~, ~/3) is a multi-index and 171 = 7~ + 72 + 7a. The norm associated with H"(~) that we will use is
357
CoupledSystemArising in Magnetohydrodynamlcs 7)7,
"~ ID I
= I1~’11-o.~)
I ~ The subspace of H (~) consisting of functions vanishing on 0f~ is denoted as usual by H~ (~) We shall denote respectively (LP(~)) 3 and (Hm(fl)) 3 by ~(~) and ~(~) when there is no ambiguity, by ~ and ~. Weshall use the Sobolev inequality : for 2 ~ p ~ 6,
II/ll~,
(2.9) Let T > 0 and let X be a Banachspace. The space L~(0, T; X), 1 ~ p ~ ~ is ~he space of classes of Lp functions from [0, T] into X. Werecall that this is a Banach space for the norm
II~(t)ll~ dt
if ~ ~ p < ~, ess supII~(t)llx if
p = ~.
The following trace spaces and norms will also be needed : H~/~(F) {v]r,v ~ H~(fl)},
’, H-t/~(r)= (H~/~(P))
][q[[Y~/~(r) -
inf
..,
:
[[k[]~-,/~(r
) =
inf
sup
Wedenote by C~(~) (resp. C~(fl)) the space of real functions infinitely differentiable with compact support in ~ (resp. ~). Weintroduce the spaces W= {C e (C~(g)) ~, di~ C : 0, C.nloa = 0}, V : {~ e (C~(a)) ~, div~ = 0}, V = {v ~ ~(a),divv
= 0},
W : {C ~ a ~(a),divC
: 0, C.n[o~ = 0},
H= {v e ~ (~), divv = 0, v.’~lo~= 0}. The space V (resp. W)is the closure of ~ (resp. W)in ~ (~) (resp. 1 ( ~)). H the closure of Y (and ~) in ~ (fl). L et u s r ecall t hat u.n makes s ense i n H-~/~(O~) as soon as u ~ L~(~) satisfies divu = 0. For v ~ V and C ~ Wwe denote
One can establish that [I,IIr (resp. I~.11~)defines a norm (resp. W) which equivalent to that induced by Hl(~) on V (resp. W) (cf. G. Duvaut and J.-L. Lions [4]). Thus we have Nr B e W For 2 ~ p ~ 6, this inequality that, for B ~ W
together with the Sobolev imbedding (2.9) imply
As well, Poincarfi inequality and (2.9) imply that, for u ¢
IlullL.¢m _
358
Gerbeauand Le Bris
2.3 Regularity
of the Data
Weshall suppose in the sequel that UoE H~(fl)~q tHI2 (fl), with divuo q ~ C(O,T;H3/2(F)),
(2.10) (2.11)
with frq=O,
k ~ C(O,T; 1/2 (F)),
(2.12)
f ~ L~(0, T; ~ (f~)).
(2.13)
From a. physical viewpoint, it is natural to assume that k is the trace on F of the gradient of the electrical potential : k = aV¢lr.
3
PRELIMINARY
(2.14)
RESULTS
First of all, we notice that we can split the magnetic field b(t) fi IHI~ (~) satisfying (2.6) and (2.4) into the sum of a function Bd(t) that satisfies (2.6) and a function B(t) ~ W. Indeed, we have : LEMMA 1 Let q ~ C(0, T;H~’-I/2(f~)) for k = 1 or k = 2, there exist C ( O, T; Hk ( f~ ) ) anda constantd4 such
JlB’qJc(o,T;~(m)<_&[lqJlc(O,T;H~-’/~(m)’
Bd.n = q on [0,T] × F and Moreover, we can impose that divBd(t)
= 0 and curIBd(t)
= 0 for
[O ,T ].~
PROOF It suffices to define Bd as follows : Bd(t) = V¢(t) where ¢(t) is a solution of the Nemnannproblem -A¢
=
0¢
= q(t)
On Let B(t) = b(t)following one :
Bd(t).
O~u + u.Vu - yA u div u 1 -curl (curl/3)
0
onr.~
Wereplace the original problem (2.1)-(2.8)
= =
din[) f-Vp+curlBxB+curlB
=
curl(u x B) + curl (u Bd)
div B =
0 in
0
xB
(3.1) (3.2)
f~,
in f~,
with
in ~,
(3.3) (3.4)
359
CoupledSystem Arising in Magnetohydrodynamics with the following initial
and boundary conditions u B.n curlBxn
= = =
ult=o
0 0 kxn
on F, on F,
(3.5) (3.6)
onF, in ~2,
= uo
(3.7) (3.8)
Wenow proceed to establish a preliminary existence and uniqueness result for the magnetic problem and two estimates which will be needed in the next section. Wedefine the (non-empty) convex set I~M = {V E L2(O,T; V),
supte[0,T] IIv(t)llv<_ IIOtvIIL=(O,T;L=Ia)) < M}.
The values of the constant Mand T will be fixed later.
Weonly suppose here that
1 M
(3.9)
Let us note that v E /CM implies v ~ C(0, T;V). For v following problem : find B 6 C(0,T; W) 1-curl (curl B) = curl (v x B) + curl (v ~)in f
]~ M, we
consider the
l x [0, T],
(3.10)
divB = 0 in f~ x [O,T],
(3.11)
with the following boundary conditions : B.n = 0
on F × [0, T],
curlB x n = k x n
(3.12)
on F x [0,T].
(3.13)
PROPOSITION1 For v ~ ICM and M satisfying hypothesis (3.9), the problem (3.10)-(3.13) has a unique solution C(0, T; W). Moreover, we ha ve the f ollo wing estimate :
sup[IB(t)llw_< ~ ÷ ~llvll~(O,T;V),
(3.14)
where a~, ~ and 71 are some constants defined below. ~ PROOFExistence
and uniqueness.
We define on W × W the bilinear
a~(C~, C2):_ol £curlCl.CU,’l C~ ax
form
- f.((tl×Cl).CurlC:~dz
and h~(t) ~ W’ such that, for C ~ W, < h~,(t),C
>= ~v(t)
Be(t).curlCdx +
-
xn, C>r
360
Gerbeauand Le Bris
First, let us prove that problem (3.10)-(3.131) is equivalent to find B E C(0, such that av(B(t), =< hv( t), C > (3 .1 5) for all C E W. Let B ~ C(0,T; W)which satisfies /f~ ~curl(curlB)-curl(v(t)
(3.15). Integrating by part, we have
× (B + Bd)).Cdx =< ~(k × n-curlB
for all C 6 W. First we deduce that < curlB x n,C >r=< k(t) yields (3.13). Moreover, since divC = 0, there exists p such that
x n,C >r which
lcurl (curl B) - curl (v(t) × (B + Bd)) The function p satisfies : -/kp Op On
= _
0 in Ft 1 curl (curl B).n - curl (v(t) x (B + Bd)).n a
It is straightforward to check that the normal component of curl (v x (B + Bd)) contains only tangential derivatives of v. Thus, using vie = 0, curl(v x (B Bd)).n = 0. Moreover,(curl curl B).n = -0~, ((curl B n).t~) - 0~((curl B x n).t ~), where 0t, and 0t= denote the tangential derivatives. Then, hypothesis (2.14) yields (curlcurlB).n
Op
= 0. Therefore ~nn = 0, which proves p
C~ ~
and (3.10). ~oonversely, we easily check that a solution of (3.10)- (3.13) satisfies (3.15). Moreover, a.,(., .) is continuous and coercive on Wx W. Indeed
_< ~llcurlC~llc~(n) llcurl (1_ w +d~d.~M)llC~llwIIC.,.ll < and ~7
> (l__d~dallvllv)llCll~,v O" > (~-d2d3M)llCIl~ Therefore, the Lax-MilgramTheorem implies that the variational problem (3.15) has a unique solution B(t) ~ W. The continuity in time of Bd and v implies that
Be c(o, T;W). Estimate in L~(0, T; W). Taking C B(t) in (3. 15), we hav -l £ ]curlB[~ dx =
/.v x (B + B~).curlBdxl-
~) IIBIIw+ ~ Ilvl~ (llBIl~ + IIB¢~ll~
CoupledSystemArising in Magnetohydrodynamics
361
Thus IlBllw _< d,~d.~llvllvllBiIw +e,~llvl]vllqllH,.-+dl IlklIH-,/~.Wededuce the estimate : sup liB(t)llw t~[0,Tl
(1 -- d~d3a~lVllL~(O,T;y))
For simplicity, we introduce the constants ~ = d~ [lk][L~(O,r;a-~/~ ) , ~ = C~ a~Iq][L~(O,T;H~/~), 7~ = d2daa, which gives (3.14). In the next section, the vector field B defined above will appear on the right hand side of the Navier-Stokes equation in the Lorentz force curlB x B. Wesee that we need an estimate on u in L~(0, T; IHI1 (~)) in order to prove the coercivity problem(3.10)-(3.13). Such a control on u is typically obtained with strong solutions of Navier-Stokes equations. To define strong solutions, the force term in NavierStokes equations has to belong to L°°(0, T; L:(fl)) (see R. Temam[13]). In scope, the estimate on B in L~(0, T; W)is not sufficient. That is why we establish now a "better" estimate on B. First, we need the following proposition which is a straightforward extension (in the non-ho~nogeneous case) of Proposition 2.1 Saramito [11] (see also Lemma2.1 and Remark2.3 of [11]). PROPOSITION 2 Letm be a nonegative integer and 1 < p < oo. Let g ~ W"~’~ (f~), with divg = 0 and g.n = 0 on F, k ~ Wm+~-WP’P(F),q ~ Wm+2-~/P’P(F). ~+~’p(f~) such that Then, there exists a unique B ~ W curl(curlB) div B B.n curlB x n
= = = .=
g in f~, in f~, 0 q on F, k x n onE,
PROPOSITION 3 Under hypothesis (3.9), the solution of problem (3.10)-(3.13) given by Proposition 1 satisfies -
1 -
where a,~_, 30. and 7"~ are some constants defined below. PROOFLet g be defined
by
g = acurl (v x (B + Bd)) = a(B.Vv - v.VB + Bd.Vv -- v.VBd). Wehave div g = 0, g.n = 0 on F (because v = 0 on F and the normal component of curl (v x B) contains only tangential derivatives of v, as said above). Moreover
_
362
Gerbeauand Le Bris
Thus, Proposition 2 with m = 0,p = 3/2 yields
IIBtlw~,3/=l~ _
Finally, we use (3.14) and the Sobolev inequality
and we introduce someconstants for ease of notation : c~2 = C2dh(llql[L,,o(O,T;W4/a.a/~) +[[k[ILoo(O,T;W,/~.~/=)), f12 : C4dha[lq[lLoo(O,T;H,/=),72 : c4dhoUq[lLoo(O,T;H,/2), which gives (3.16).
4
AN EXISTENCE
AND UNIQUENESS
RESULT
Let M > 0, we define
where ~o = IlfllL=(O,T;~=(n)) and the constants c~i, ~i and 3’i are defined in the previous section. Wealso define the fimctions lq, 1.~ and p:~ by p~(M)~ = 4max (,,UoU~.,
.=(M)= = Iluoll~.
~O(M)~)
3 + 2To,M)2 + pi(M)
,~(M) = e(M)+ c~(M)+ ~,o#,(M)#2(M).
(4.1)
(4.2) (4.3)
The constants Ch,...,cm ~ppear in the following proof ~nd do not dependon the physical data. THEOREM 1 As soon as the physical data Uo, l/q, a, f, q, k, are "small enough" (in a sense madeprecise below), there exists a time T* > 0 such that the MHD problem(~.1)-(~.8) has a unique solution [0, T*]. This solution satis fies u ~
L~(0,T*;~(a))n L=(0,~*;~(a)) .rid b ~ C(0,T*;a’ (a)) PROOF Existence. In the previous Theorem,"small enough" meansthat the data are suchthat the following property holds : There exists 0 < M < 1/7~ such that pi(M) ~ M, i = 1, 2,
(’.4.4)
CoupledSystemArising in Magnetohydrodynamics
363
Note that it is indeed possible to choose the physical data such that (4.4) satisfied : a straightforward calculus showsthat ®’(0) = c5(1 +
0~1)(0~1"~2
+ ~2) -[-
c50~2(0q~/1
+
thus, q, k and ~ can be set small enough such that 0 < O’(0) < 1 and therefore one can choose M > 0 small enough such that O(M) < M. In view of definitions (4.1)-(4.3) of ~i, i = 1, 2, 3, it is a simple matter to check by an analogous calculus that (4.4) holds as soon as Uo, f, 1/~ are small enough too. We define the time T* by T* = min(T, 3/(4c6~(M))), we choose M> that (4.4) holds and we define ~M KM= {v e L~(O,T*;V), suPte[0,T. ]
~ M,
[IV(t)IIV
Ilvll~(O,T*~(m) ~
The set ~Mis clearly convex. Moreover, in view of a classical compactness result (see for instance R. Temam[13], Theorem2.1), ~Mis a compact set of the Banach space L:(O,T*;V). For ~ ~ ~M, we use Proposition 1 to define B as the unique solution of al-curl(curlB) divB B.n curlB xn
= = =
= cm’l(gxB)+curl(gxB in ~, 0 0 on F, kxn onF.
d) ing, (4.5)
According to the estimates (3.14) and (3.16), we [Icurl B ) × BllL~(O,T.;L2
and IlcurlB x BallL~o(o,r,;~2)
Therefore, the force term F = f + (curlB) x (B + d) i s i n L~(0, T *; L 2 ( f~)) a sup ~(~[o,r] +¢~ (O~2 + ~’2/~/’~11 -t- ]~IM_ ~/1/~// -t- ]~2/~1) (1
"t- O~1+ ]~IM’~
_< Then, it is proved in R. Temam[13,14] that there exists a unique solution u G L2(0, T*; ~ (~)) ~q L~(0, T*; ~ (f~)) to the Navier-Stokes equations c9tu+u.Vu-~l/ku+Vp = F infl, divu = 0 inf’, (4.6) u : 0 on F,
I
364
Gerbeau andL~eBris
satisfying
moreover sup Ilu(t)[l~ < #I(M)2 ~, _< M te[o,T*] 2
3) [IF(t)ll2 dt + it, (M)
< p~(a,l)~ < ~. .,’14 Wethen deduce from the Navier-Stokes equations that
We deduce that u e /CM. Let us check the continuity iu L"-(O,T;V) of ~ --~ u. Let ~n be a sequence that goes to ~ in L~(O,T;V), it defines a sequence Bn, solution of (4.5). The force term corresponding to Bn in the Navier-Stokes equations has the required regularity to define a sequence u, bounded in L:(0,T;I~(~)) and such that Otun is bounded in L2(0, T;L~(It)). The sequence Un is therefore compact in L~(0, T; IE~ (~)). The uniqueness of the solution yields that u= goes u corresponding to g. Thus the application i7 ---~ u maps continuously the convex compact set /Ca4 into hi~nself. Therefore, the Schauder theorem ensures that the existence of a fixed point. This yields the existence result. Regularity of b. We have just proved that B ~ C(O,T*;W). We show as in Proposition 3 that B ~ C(0,T*;W~’a(~)) and therefore we have in particular B ~ L~(O,T*;Lq(~)),Vq > O. Using for example that B e Lc~(0, T*;LS(!~)), we easily check that the right-hand side of (4.5) belongs to ~¢ (0, T*; Ls/5 (it)). U lug Proposition 2, we deduce that B ~ L°°(0, T*; W~,S/5(Ft)), which implies B ~ L~(0,T*;L~(it)). The right-hand side of (4.5) is then in Lc~(0, T;L2(~)). Applying one more time the regularity result of Proposition 2, we finally condude that B ~ LC~(0, T*; lI-ll~ (it)). In view of the regularity d, we deduce that b e L°"(O,T*;IHI~(Ft). Uniqueness. Let (u~, p~, B~) and (u2, p2, B2) two solutions of problem(3.1)Wedefine u = u~ - u~, B = B~ - B~.. Combiningthe equations satisfied by (u~, 13~) and (u2, B2), we have Otu + u.Vu, + u~.Vu - rlA u + Vp = curl B x B~ + curl B~ x B, -1curl (curl B) = curl (u x B~) + curl (u~_ x B) + curl (u
(4.7) (4.8)
with u = 0, B.n = 0 and curlB x n = 0 on the boundary. Multiplying (4.7) by u, (4.8) by B and integrating we obtain
2dr
&
~ j~ a
- J2
(4.9)
365
CoupledSystemArising in Ma~net0hydrodynamics Weestimate the right-hand side of this inequality as follows :
where Ce and e are some constant, with e arbitrarily
small.
lcurlBz x )B.uldx ~ [IcurlB~llg~(n)llBllLqn)llull~(n
_
(n~llull~¢n~ + ellcurl~ll[~(n~,
~ x Ba.curlBldz ~ C~ lIB~ II~ll’~ll~(n~ + ~ll~ur~l~(n~, fnb~
In this last inequality, weestimatecur] B with equation(4.8)
~ + d~d~llu~ll~ L~£ ~cu~]~1~dx~ (11~11~ + II~all~)llc~r]~ll~llull~ Using sup~[0,T. ] ~[u~H~ ~ M and the coercivity 7x = d2daa, we deduce that 1
-
")’1M(II~IlIL~÷
assumption 0 < M < 1/~ with
IIBdIIL~)IlUlIL’Z"
(4.10)
Thus, [ue x B.curlB I dx <_ C~ 1 -~IM (IIB~II~ +
IIBall~’)elluell~ IMI[~+
d
(4.9) yields ~11-11~. ~ ¢(t)ll-li~.~ with¢ . I1~(~) (~)(ll~lll~+ll~ll,.~)=llu=ll~ta)) C~(llu, ll~(m+llB2lla~(a)II Oathering th~se inequalities,
estimate
Note that ¢ ~ LI(0, T*). Therefore, by GronwaHlemma~u = 0, and using again (4.10)~ B = 0. This provesthe uniqueness of a sgro~g solugion (lt~ b) of (2.1)-(2.8).
5
REMARK ON THE NON-UNIQUENESS
It has been proven in the previous section that the MHD problem (3.1)-(3.8) has unique solution for small data, at least on an interval [0, T*], T* > 0. The idea of the proof has been to ensure the coercivity Of equation (3.3) by controlling the normofu on [0, T*]. Weexhibit in this section an example(due to P.-L. Lions [8]) non-uniqueness in the case when the operator Tu : B ~ curl (curl B) - curl (u x is not invertible. From now on, we assume for simplicity that k = 0, q = 0, thus we deal with the homogeneous boundary conditions on F : u B.n curlBxn
= 0, = O, = 0.
366
Gerbeauand Le Bris
Let us assume that for so~ne to and some fi = ft(to,x) the opera.tot T,~ : B -~ curl (curlB) - curl (u x B) is not invertible. There exists a divergence-free field /) ~ 0 satisfying curl (curl/)) = curl (fix/)). Note that such a ~i is necessarilly "large enough", otherwise, Ta would be coercive. If we consider the force ] = ~.V/~ - r/A fi - curl/) x/), then (~i,/)) is a (stationary) solution to Otu+u.Vu-~lAu+Vp = ]+curlBxB, divu = 0, (5.1) curl(curlB) = curl(u x B), div B = 0. Next, we define u’ as the solution of
{
Otu+u.Vu-~Au+Vp divu
= ], = 0.
with the "initial" condition u’(t0, .)= fi(t0, Wefinally observe that (’C~, B) and (u’, 0) are different (since /) ~ 0) while both satist}" (5.1) on [to, +ec). Thus, we have two different solutions of the problem with homogeneous boundary conditions.
6
CONCLUSION
We have proved that the MHDsystem (2.1)-(2.8) has a unique solution on interval [0, T*] as soon as the physical data are regular and stnall enough, with T* > 0 depending on the data. Note that the proof may probably be extended to the case of muttifluid equations in two dimensions with constant viscosity and conductivity. Moreover, we have shown that a solution is not unique if the operator B --+ curl (curl B) - curl (u x B) is not invertible. This mayoccur as soon as the velocity becomes too large, but it is an open question to show that the operator do indeed becomenot invertible. The practical conclusion of this study is the following : even if the modelpresented here seems well-suited in some physical situations and even if it is mathematicaly well-posed under restrictive assumptions, it should be very carefuly used in numerical si~nulations since it could be ill-posed as soon as the velocity beco~nes too large.
REFERENCES 1.
2.
F. Armero and J.C. Simo. Long-time dissipativity of time-stepping algorithms for an abstract evolution equation with applications to the incompressible MHDand Navier-Stokes equations. Comp. Methods Appl. Mech. Engrg., 131:41-90, 1996. J.-M. Dominguezde la Rasilla. Etude des dquations de la magndtohydrodynamique stationnaires et de leur approximation par dIdments finis. Thb~se, Paris VI, 1982.
CoupledSystem Arising in Magnetohydrodynamics 3. 4. 5.
6. 7.
8. 9. 10.
11. 12. 13. 14.
367
G. Duvaut and J.-L. Lions. In~quations en thermo61asticit~ et magn~tohydrodynamique. Arch. Rat. Mech. Anal., 46:241--279, 1972. G. Duvaut and J.-L. Lions. Les indquations en mdcanique et en physique. Dunod, 1972. J.-F. Gerbeau and C. Le Bris. Existence of solution for a density-dependent ~nagnetohydrodynamic equation. Advances in Differential Equations, 2(3):427-452, 1997. J.-F. Gerbeau and C. Le Bris. On a coupled system arising in magnetohydrodynamics. Appl. Math. Letters, 1998. M.D. Gunzburger, A.J. Meir, and J.S. Peterson. On the existence, uniqueness, and finite element approximation of solutions of the equations of stationary, incompressible magnetohydrodynamics. Mathematics of Computation, 56(194):523-563, April 1991. P.-L. Lions. Private communication. A.J. Meir and P.G. Schmidt. A velocity-current formulation for stationary MHDflow. Appl. Math. Comp., 65:95-109, 1994. A.J. Meir and P.G. Schmidt. Variational methods Ibr stationary MHDflow under natural interface conditions. Nonl. Anal., Theo. Meth. Appl., 26(4):659689, 1996. B. Saramito. Stabilitd d’un plasma : moddlisation mathdmatique et simulation numdrique. Masson, 1994. M. Sermange and R. Temam. Some mathematical questions related to the MHDequations. Comm. Pure Appl. Math., XXXVI:635-664, 1983. R. Temam.Navier-Stokes Equations, Theory and Numerical Analysis. NorthHolland, 1979. R. Temam. Navier-Stokes Equations and Nonlinear Functional Analysis. CBMS-NSFRegional Conference Series in Applied Mathematics, SIAM, 2d edition, 1995.
A Disease
Transport
Model*
K.P. HADELER Universit~t Tfibingen, Biomathematik, Auf der Morgenstelle D-72076 Tfibingen, Germany ([email protected]) R. ILLNERDepartment of Mathematics and Statistics, University Victoria, British Columbia, Canada V8W3P4 ([email protected])
10,
of Victoria,
P. VANDENDRIESSCHE Department of Mathematics and Statistics, University of Victoria, Victoria, British Columbia, Canada V8W3P4 ([email protected])
ABSTRACT The Kermack-McKendrick model for the spread of disease in a homogeneous population is combined with a transport equation to yield a new model for the spatial spread of disease. This system provides a more detailed description of the migration and contact processes than the standard reaction diffusion model, which however, is a limiting case. For the epidemic transport model, global existence of solutions is shownby a Kaniel-Shinbrot iteration scheme. It is proved that the population of infectives eventually .disappears and also, using an energy integral approach, that the susceptible population approaches a constant. Key words: epidemic model, transport equation, monotone iteration, tional AMSsubject classifications:
1
energy func-
92D30, 82C70
INTRODUCTION
Transport equations are an established modeling tool in diverse areas such as neutron physics, the theory of dilute gases (and Boltzmann equations), and extended thermodynamics. In mathematical biology they have been used, sometimes under *Research of the first author supported by Deutsche Forschungsgemeinschaft; research of the second and third authors partially supported by the Natural Sciences and Engineering Research Council of Canada. 369
370
Hadele~ et al.
the name of velocity jump processes, in modeling the motion of bacteria aud of slime mold amoebae, aiming at a better understanding of chemotaxis and pattern formation [21], [13]. Transport equations have two advantages over the traditional reaction diffusion approach. They do not showthe unwantedeffect of infinitely fast propagation and they allow a more detailed description of the transport processes. In Brownianmotion particles are characterized by their position in space, they do not have an individual velocity or direction. As a consequence, diffusion equations show the phenomenonof infinitely fast propagation, as do similar systems with integrals over space modeling long range interaction [12]. To our knowledge, transport equations have not so far been applied in epidemic modelling. The goal of the present paper is to show that transport syste~ns can be formulated as realistic models for the spread of disease. They are generalizations of diffusion models; the latter occur as limiting cases for high particle speeds and large turning rates. An epidemic model based on the diffusion approach depends, with repect to the transport processes, only on the diffusion rates of susceptibles and of infecteds. These rates measure the overall mobility of the two populations. The epidemic transport models presented here depend on two transport kernels for the migration patterns of the susceptible and the infected populations, and a contact kernel, which measures, by comparing velocities, the duration of a contact and thus takes into account that transmission rates depend strongly on the duration of exposition. In this sense transport models are intermediates between diffusion models for overall behavior, and models based on individual behavior. Weunderline that transport systems, being hyperbolic partial differential equations as opposed to parabolic diffusion equations, require different mathematical methods, e.g. the method of characteristics. While parabolic systems have strong s~noothing properties, solutions of hyperbolic systems do not become smooth and therefore a concept of mild solution.is needed. Weshall show that some tools that were originally developed for the Boltzmann equation, work well for epidemic models, due to the product structure of the infection term. This applies, in particular, to monotoneiteration schemes of the Kaniel-Shinbrot type [17]. Weshow global existence of mild solutions to the initial value problem, and show that the class of infecteds goes to zero in the L~ norm, independent of the parameter values and the initial data. Finally we show that the susceptibles approach a spatially constant solution. So far an epidemic threshold theorem has not been proved, nor the final size of the susceptible class determined. Next we describe the modelling approach in some detail. We start from the simplest SI model in the form of ordinary differential equations, for susceptibles u and infecteds w
~ = -~u~ ~b = fluw - aw,
(1.~)
usually attributed to Kermackand McKendrick[19] (actually a special case of their more general model), see also [7]. Here ~ > 0 is the transmission rate and a > 0 is the recovery rate. The basic reproduction number is Ro = ~/a. If this modelis applied to a population structured by so~ne feature such as position in space, age, gender, social group, then the transmission pattern and the motion of individuals in feature space can and must be modeled. First we define, for a given individual an individual susceptibility, and then, for this individual, the infectivity
371
Disease TransportModel
to which it is exposed. The infectivity is a weighted integral over the infected population. Second, we describe how individuals move between classes defined by the structure variables. With respect to position in space we can have a variety of migration and diffusion models. Wecan either model the infectivity as an integral over space, or the movementsof individuals in space (or both). Both approaches involve integrals over the space variable. The first approach yields, in the simplest form, a system ut = -~u / k(x - y)w(t, y)dy
(1.2)
where k(x - y) is the infectivity an infected at position y exerts upon an individual at position x. The kernel function k is even and non-negative. In the second approach we keep a simple local transmission law and let individuals moveaccording to an integral equation,
u~= -Zu~o + 9(/g(x- y)u(t,~)du- ~(t, (1.3)
~t = Zu,~- ~w+/)(1/~(~- ~)~(t,~)dy- ~(t, where the kernels are even, nonnegative and normalized to have integral equal to 1. The number D is the rate at which susceptibles change position, and then K(x - y) is the density with repect to y of susceptibles arriving at x, and similarly for b,/~ and infecteds. While the kernel k in (1.2) describes contacts between individuals distant locations, the kernels in (1.3) describe movementsof individuals. Each system (1.2) and (1.3) can be reduced to a system of reaction diffusion equations, using the standard Taylor .expansion approximation and keeping three moments. Following the ideas of [18], (1.2) can be reduced
ut =-flu(koW+k~w.~.~) wt = flu(kow+ k,,w.~:,) where ko = f k(y)dy and k~ = f k(y)y2dy/2. obtain a standard reaction diffusion system
(1.4)
On the other hand, from (1.3)
ut = -~3uw + D~u~.~
(1.5)
Of course, mathematically, the two systems (1.2), (1.~) and also (1.4), (1.5) rather different structures. Modelsof the form (1.2) have been studied in [1], [2], [6]. In [3] a system with diffusion and contact distribution incorporating features of (1.3) and (1.5) was considered, and in [20] a system with a contact kernel and a diffusion kernel that includes both (1.2) and (1.3) as special cases has been studied. In [16] system (1.5) with D~ = 0 has been applied to the spread of rabies. Several authors, e.g., [8] and [23], have studied the joint effects of diffusion and age structure.
372
Hadeler et al.
Before studying equations of the form (1.3) with transport operators, we introduce a linear transport equation (without disease) in one space dimension. Lef, u(t, x, be the density of particles at position x with velocity s at time t. The free stream equation gives ut(t, x, s) + su.~(t, s) : O . (1. To incorporate particles turning (i.e., changing velocity), let # > 0 bc the rate constant of turning events, i.e., let turning be governed by a Poisson process with parameter #. Velocities are restricted to lie in the boundedset Y = {s: [s[ _< a}
(:1.7)
for some a ¯ (0, oo). At a turning event the particle chooses a new velocity s from ~) according to someprobability distribution that contains the previous velocity .~ as a parameter. Thus the transport equation becomes, see [4], ut(t,x,s)
+ sux(t,x,s)
where K/# is the probability
= fv K(s,$)u(t,x,$)d~
- #u(t,x,s),
(1.8)
kernel with K(s, ~) nonnegative, bounded and
fv
K(s,$)ds
= p.
(1.9)
If the set Y is replaced by a set of only two velocities, ~,’ = {+7}, with "7 > 0, then the transport equation becomes a correlated random walk in the sense of Goldstein and Kac [15]. In fact, if we write u+(t,x) = u(t,x,"7), u-(t,x) = u(t,x,-’y), then the system reads
ut+ + ~’u~= (#/2)(u- - +) u
+-
-
(1.10)
Then the function u = u+ 2u.~, + u- ~, satisfies the telegrapher’s equation uu + #ut = 7 from which the diffusion approximation can be obtained for large "7 and # [11], 1112]. To study the equation (1.8) on a bounded interval x ¯ I0, £] we need to impose boundary conditions. For a hyperbolic system data can be given along ingoing characteristics; thus at x = 0 data can be given for u(t, O, s) with s > 0, similarly at x = t7 data can be given for u(t,£,s) with s < 0. Wetreat here the case of periodic boundary conditious, which amounts to studying the problem on a circle S1. This is the simplest situation although not very realistic from a biological point of view. However,the proof carries over to the biologically realistic case of reflective (Neumann) boundary conditions, as shown in Section Nowwe formulate our model system by combining the disease transmission and the transport processes. We keep # and K as defined above for the density of susceptibles u(t, x, s) at time t, position x and velocity s, and take #7 and/-(" defined in a similar wayfor the density of infectives w(t, x, s). Thus, for infectives,/~7/#~ is the probability kernel where/5 is the rate constant of turning events, with /’((s, ~) >_ and [((s, ~) = D. (1. 11)
Sv
Disease TransportModel
373
To account for different velocities of infectives, we introduce into the transmission term the contact distribution L(s, ~), which is nonnegative, bounded and satisfies
f
(1.12)
v L(S, ~) ds = 1.
Combiningsystem (1.1) and (1.8) leads to the following system: ut(t,x,s)
+ suz(t,x,s)
= fv K(s,g) u(t,x,g)d~-
#u(t,x,s)
- flu(t, x, s) Iv L(s, ~) w(t, x,
wt(t,x,s)
+ swx(t,x,s)
=/, [f(s,$)w(t,x,$)d$-
ftw(t,x,s)
+flu(t, x, s) f, L(s, ~) w(t, x, ~) d$ - c~w(t,
(1.13) In contrast to equation (1.3), the integral is taken over velocity. Note that a system of the form (1.13) based on the correlated random walk (1.10), i.e., an epidemic model with only two velocities, has been investigated in [9], [10]. As described earlier, the parameters # and/t and the kernels K and/~ describe the dynamic behavior of the migrating populations of susceptibles and of infecteds. Here we can think of a time scale of hours or days. On the other hand, the kernel L measures transmission rates between individuals with different speeds. Wereasonably assume that infected individuals passing through a location at high velocity contribute little to total infectivity as opposed to sedentary individuals. For some proofs we need the assumption that the kernel K is symmetric (this assmnption may be technical). Symmetryin this context says that individuals switch from low velocities to high velocities at the same rate as from high to low velocities. Assume, on the contrary, that individuals choose higher velocities at a faster rate. Then either all individuals would have higher speeds or there would be transitions via intermediate speeds back to lower speeds. In the first case we could perhaps choose another set of velocities from the beginning. In the second case we would need more detailed information about cyclic changes in velocity. This argument amounts to saying that the symmetry assumption is the most natural and simple assumption next to the assumption of a constant kernel producing the uniform distribution. Wehave to specify initial and boundary conditions. Initially the densities, given by u(O,x,s) =_ uo(x,s) and w(O,x,s) -- Wo(X,S), are assumed to be continuous, nonnegative and bounded. For s > 0, the ingoing density at x = 0 is defined by the values of the outgoing density at x = g, and similarly for s < 0 with g and 0 interchanged; thus for all s, u(t, e, s) = u(t, O, s), w(t, e, s) = w(t,
(1.14)
This amounts to the earlier mentioned assumption of periodic boundary conditions. Note that we work on I~ x S~ x V, where V is given by (1.7), and the space variable is taken rood g.
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Welook for mild solutions to the initial boundary value problem formulated above for u and w. Wedefine mild solutions of (1.13.) as a pair of functions u(t, x, s) and w(t, x, s) that satisfy the system ~[u(t,x
+ts, s)] = fv K(s,~)u(t,x
+ts,$)d~
- uu(t,x +ts, s) - S7u(t,z +ts, s) f, L(s,
¯ +ts,
~dt [w(t, x + ts, s)] = fv R(s, $)w(t, x +ts, $) - fi w(t, x + ts, s) + Z u(t, x + ts, s) fv L(s, ~) w(t, ts, $) d~ - a w(t, x + ts, s). This type of solution concept is well-known in the theory of transport equations, see [5] or [17]; one of its main advantages is that it allows solutions of (1.13) for initial data that are not smooth. Indeed, with respect to the space variable, the solution is as smoothas the initial data, i.e., continuous in the present case (or just measurable, if initial data are measurable). Weremark that this concept of mild solution is stronger than the concept of weaksolution in the sense of distributions.
2
MONOTONE
APPROXIMATIONS
Weuse a Kaniel-Shinbrot [17] iteration scheme (see also [5, pp.136-137]) to show that the IVP formulated in the Introduction has a unique Inild solution for all t > 0. Firstly, for u, w, let lower sequences be denoted by {u(J)}, {w(J)}, (j) }, respectively, for j = 0, 1,.... Note upper sequences be denoted by {U(j) }, {W that the independent variables are dropped where no confusion arises, e.g., U(°) = U(°)(t,x, s). All equations are written in the classical form, but solved in the mild sense defined above. The iterative schemeis defined so that each equation is linear in the current variable. For j = 0, take u(°) = w(°) = 0,
with initial condition U(°)(0, m, s) = Uo(~, and periodic boundarycondition as in (1.14), U(°)(t, ~, s) = U(°)(t, With U(°) now given as a solution of the above, W(°) solves (°) +s W~ °) + (f~ + ~)W (°) = .f, /~ W(°) d~ + f~ U(°) iv LW(°) d~, W~ with initial condition W(°)(0, x, s) -- wo( x, s), and periodic boundary condition as in (1.14), W(°)(t, g,s) = W(°)(t,O,
(2.1)
Disease TransportModel For n = 0, 1,..., u(,~+l)
375
take the following iteration scheme
.(,~+~,
÷ (#+~/vLW(n,d~)
) /vKu(n)d~,
"+’) (D+~)w ~"+~) t + sw~ +
=
/v ~ w(~) d~ + ~ u(~) /~ L w(n)
(2.2)
w:
+
+ (b + w
withinitial conditions u(~)(0,x,s)= (j)(0, ,x s ) u( = O, x, s)~ U o( and w(J)(O,x,s)=W(J)(O,x,s)=w(O,x,s)~Wo(X,S) for j=1,2,..., andperiodic boundary conditions ~ in (l.14) foreachtermin ~hesequences. To prove results on this iterative scheme, we make use of the following theorem, which can be proved by use of an integrating factor. THEOREM 2.1
Consider the linear first order equations
dyi(t_____~)+ hi(t)yi(t) = gi(t), i dt where hi(t), gi(t) are nonnegativeand continuous on [0, c~), subject to th e i niti al conditions yi(O) = Yo > O. Then (i) I] h,(t) = h2(t), gl(t ) >_ g2(t). (res p. g,(t ) <_ g2(t)) for [O, oc),then y~(t) >_y2(t) (resp. y~(t) <_y~(t)) for [O, oc). (ii) If g,(t) = g2(t) and h~(t) h2(t) (resp. h~( t) <_ h2(t)) for all t ~ [0,~ ), then y,(t) <_y2(t) (resp. y,(t) >_y~(t)) for [O, oc). Monotonicity of the sequences defined by (2.1) and (2.2) is proved by induction in the following lemmas. LEMMA 2.2 Each starting term in the upper sequences defined above in (2.1) is nonnegative, namely U(°) > 0 and W(°) > O. Proof. Considerthe equation for = u(O, x, s), written as U0, sequence, denoted by {V(1)}, V(°) = O,
U(°) (t, x, s) in (2.1) with initial values (°) (0, x, s nonnegative and bounded. Construct an approximating to U(°) from the scheme
Vt(n+t) + s V.~n+~) +/z V(n+l) =/v K V(r0 d$, with v(J)(O,x,8)
-~- 0
for j = 1, 2, .. ..
(2.3)
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Hadeleret al.
For n = 0, d dt
(v¢’)(t,
x + +, x + st,
Thus V(1)(t, x + st, 8) : Uoe-*tt (°) >_V giving where
Co: IIUoll~. To proceed by induction, suppose that, for a fixed n,
IIV(’~)(t,’)ll~ < co \p=O
-"~, ~j e
where Then from (2.3) d (V(n+l)(t,
x + st,
8)) + tt
V(n+l)(t,x
dt (Clt)P
<_ C~Co
\~,=o
P!
Solving gives V(n+l)(t,x + st, 8) < I~-~ (Clt)P~_
p=O-t~. e-lit,
showing that
IIV(’~+~)(t, ")ll~< CoeC’te for all n, and t _> 0. Also Theorem2.10) showsthat for
v(~+’)(t,.) ~v~")(t,.). Thus {V(j)} is a nonnegative, nondecreasing sequence that is bounded above, and so on any arbitrary but bounded time interval [0, T], lim V(n)(t, .) = V(t, exists, is nonnegative and finite. Integrating (2.3) and letting n -~ oo, it foll[ows that V(t, .) is a mild solution of the first equation of (2.1). To showuniqueness this solution, suppose that V1(t, .) and V2(t, .) are both mild solutions of (2.1), and consider their difference
~’(t,.) =~q(t,.) - v.~(t,
Disease TransportModel
377
By linearity, this satisfies an estimate
e_
x +st, 8))+.e(t, x +st, s)-
dt
with !~(0, ") = 0. Integrating gives t
f0
Ilk(t, ’)11~_
Yt(n+~) + sy~(n+~) + (# + a) Y(~+l) = /v[~Y(n)dg + flU(°) , with Y(J)(O,x,s)=w(O,x,s)
for j=1,2,
....
(°) is well-defined for Proceeding as in the proof for U(°), it can be proved that W (°) t E [0, oo) and that >_ 0 . | LEMMA 2.3 For the iteration scheme (2.1) and (2.2) all the iterates defined/or t e [0, oc) by (2.1) and (2.2), and
are well-
0 = u(°) <_ u(~) <_ u(2) <_ ... <_ U(2) <_ U(1) (°), =U 0 --~
W(0)
< W(1)
< W(2)
’<
"’"
< W(2)
= W(1)
(0 = ). W
Proof. Consider first the equation for u(1) given by (2.2). An elementary argument shows that u(1) _> 0 = u(°). The same argument on the equation for w(~) in (2.2), shows that w(1) _> 0 = w(°). Comparing the equations for U(°) and U(t) from (2.1) and (2.2), gives (~) =U(°); si milarly, W (1) = W(°). Since U( °) _>u(° and W(°) >_ w(°), Theorem 2.1(i), (ii) shows that (1)
u (n),
limits
w= lim
w(n),
U= lim
U(n),
W= lim
nW
/or the sequences defined in (2.1), (2.2) exist, and u = U and w = W are global mild nonnegative unique solutions of (1.13) assuming uo(x, s) and wo(x, s) as inital ’values and satisfying the periodic boundaryconditions (1.14).
378
Hadeler et al.
Proof. By monotone convergence of (2.2) (theorem of Beppo Levi, applied to finite time interval [0, T]), u, w, U and Wexist and are at least measurable. They satisfy in the mild sense
(2.4)
where u(O,x,s)=U(O,x,s)
and w(O,x,s)=~V(O,x,s).
Define g = U - u and h = W- w, then their initial (in the mild sense)
values are zero and they satisfy
gt + s g* + #g = /v K g dg - ~g ]~ Lw d$ + ~U ffv Lh dg, ht + s h, + (£ + a)h
--£ if
£
£
h da + ~U Lhda + l~g Lwd~.
(.,.6)
Since g and h are nonnegative, we can obtain an L1 estimate. Weintegrate (2.5), (2.6) over s 6 P and a period in x. Then the terms containing K and /~ cancel with the # and/2 terms because of the assumptions on the kernels, and the second to the last term of (2.5) is nonpositive. The three remaining terms containing/~ can be estimated as in
and similarly for the other terms. Then we obtain d
(llgll ÷Ilhll) a(llgll +Ilhlll)
with c = 2a~3[ln[[~ ([[’u[[~ + [IU[[~ + [[w[[~). Since [Ig(0, ")[[1 = [[h(0, ")[l~ = 0, the above implies that g = h = 0, and so U W= w. Thus the equations (2.4) reduce to the pair of equations (1.13), and u w = Ware global mild solutions of the original problem (1.13). By construction, u and w are nonnegative. A standard argument based on Gronwall’s inequality shows uniqueness. Since the initial data are continuous, u and w are continuous with respect to the space variable and differentiable along characteristics. |
Disease TransportModel 3
ASYMPTOTIC
379
BEHAVIOUR
THEOREM 3.1 For system (1.13),
Ilu(t,’)lll
has a limit and
IIw(t,.)lll o a8 Proof. Integrating equations (1.13) with respect to s (thus cancelling the it and terms), then with respect to x, and adding, gives
d-~
(u + w)(t,s,x)dsdx
w(t,x,s)dsdx,
(3.1)
which is ~ 0. Define A =
(u +w)(t, x, s) ds
which exists and is nonnegative by monotonicity, (3.1) and u ~ 0, w ~ 0. Integrating (3.1) from t to ~ gives (u+w)(t,x,s)dsdx
a+~ ~ fvW(r,x,s)dsdsdr=
(3.2)
for all t > 0. Thus JO J~
for~ su~dently large. Usin~theequRtion forw from(1.13), integrating withrespect to~, ¯ and~ gives w(t, x, s) ds dx
=~
w(O,x, s) ds
~ Lw(r, z, ~) d~ ds d~ dr -
The first integral on the left is bounded(because
w(r, ~, s) ds dx dr.
(a.1) shows tha~
is bounded)and the second integral on the left is given by the initial condition. ~he second integral on the right is boundedas a function of t, see (a.2), hence d~ds ~vU d~ ; dr Lw(r,x,g) is bounded(as a function of t), and as it is monotoneincre~ing in t, it h~ a limit as t ~ ~. Nowintegrate the u equation si~nilarly, giving ~(t,~,s)
dsdz
u(O,~,s)
dsdz-
~ Lw(r,z,g)
dgdsd~dr
380
Hadeler et al.
thus the left side has a limit A~L>_ 0. Likewise
j~oe fv w(t, x, s)ds has a limit, namely A,, = A - A~ _> 0. But, because of (3.3) A,, must be z.ero. Thus liT(t, ’)111 -+ 0 as t -~ co, and Ilu(t, ")[11 has a limit as t -+ ~. With additional assumptions on the probability kernel K(s,g), we are able to prove that the density of susceptibles, u(t, x, s), tends to a constant in L~ as t -~ o~. The proof uses an energy functional (c]. the constant of motion for the o.d.e, system (1.1)), as suggested by Hartmut Schwetlick [22]. Firstly, we observe that u satisfies a maximumprinciple if the kernel K(s, ~) is symmetric. THEOREM 3.2 Assume that K(s, ~) = K(~, s) for all s, g ~ Y. Then the solution u of (1.13) constructed in Section 2 satisfies
Ilu(t,’)11~ _
(3.4)
Proo]. Suppose that at time t, So and ~o are chosen such that u(t, Xo + tso, So) = sup u(t, x, s). Then by (1.15) and the nonnegativity of u and
ddt [u(t, xo + tso, so)] <_ Iv I((so,~)u(t,
+tso, so)d~ - # u(t, xo + tsoso)
= (f -~ 0,
where the symmetry and normalization of K have been used. For any e > 0, set u¢(t,x,s) = u(t,x,s) - Thenclear ly d u~(t" xo + tso, So) dt ’ It follows as in [14, Lemma 1] that for all e > 0 and all x, s
As e is arbitrary,
the assertion follows. |
THEOREM 3.3 Assume that the kernel K(s, ~) is symmetric and strictly positive on "~ × Y, and that sup~ ILL(., ~)[[~ is finite. Then [or system (1.13), as t u(t, x, s) converges to a constant and w(t, x, s) converges to 0 ~.
Disease TransportModel
381
Proof. The last assertion is already p~oved in Theorem3.1. Define the positive number fi* by/3" = ~sup~ ILL(., g)lll and the (convex) energy functional E(u, w) = C 4: w + u - ln (u + 5)
(3.5)
where 5 > 1 and the constant C = C(a, ~*, 5) is chosen so that E(u, w) >_ for u,w _> 0. Setting b(u) = ln(u ÷ 5), th e fi rst eq uation of (1. 13) giv (bt(t,z,s)
+ sb.~(t,x,s))
ds = (u(t,z,s)
+5)
(3.6)
x (-;K(s,~)u(t,x,~)d$+#u(t,x,s)+~u(t,x,s)fvL(S,$)w(t,x,$)d$)ds. Using the assumption that the kernel is symmetric,
#= Iv K(s,~)ds
= Iv K(s,~)d~.
Thus the first two terms of the right side of (3.6) can be written
/v/v
K(s,,~)
(u( t, x, s ) - u( t,x, -(u-~,x~-~) d$
(3.7)
Because of the symmetryassumption, the integral in (3.7) is equal to the integral obtained by interchanging s aud $, namely ~/vK(s,~)
(u(t’x,~) - u(t,x,s)) (u(t, x, ~) + 5) d$
(3.8)
Taking the average value, each of (3.7). and (3.8) is equal 1 u(t’x’s) u- (t’x’~)u-~,x-~-~-~ -~/v/vK(s’~) _ u(t,x,s) - u(t,x,~) "~~((~,_x_(_~_~ ] ~ which simplifies to 1
(~(t,~,~)- ~(t,~, (u(t,x, s) +5)(u(t,x, ~)
d$ ds.
(3.9)
The last ter~n on the right of (3.6)
(u(t, x, s) + 5) L(s, ~) w(t, x, ~)
<-Z£ (fvL(s,~)ds) w(t,x,~)d~ <_ ~* [ w(t,x,$)dg,
(3.10)
382
Hadeleret al.
by the definition of 3*. Returning to the energy functional given in (3.5), C + w + u - ~;- ln(u
d-~ [[E[[~ = ~ =,
w~+ut+~jb~
ds dx
dsdx.
Usiug (1.13), (3.9) and (3.10), this
d~llEll~N
-s(w~ va 1?vf 4~*
+ u~) - aw - ~sbz ds (u(t’x’s)-u(t’x’$))~ g(s,~) (u(t,x,s) + ~) (u(t,z,$)
+ ~ =
+
w(~,~,~)~
(a~ll)
-s E~ ds dx - ~
4B*
x, s) + 5) (u(t, x, ~) + 5) f?fuK(s, ~) (u(t,(u(t’x’s)-u(t’x’$))~
The first integral on the right vanishes for periodic boundaryconditions, thus d
d~]SEth~ 0. Integrating (3.11) gives E(T)
+
Ilwll~ + ~
K(s,.~)(u(t,x,s)+~)(u(t,x,~)+~)d,~dsdx
~ g(o) ~ 2aeC+ H~o~+ ~o~, whereE(t) = [[g(u(t, .), .))][ Nownote that as E(T) ~ for al l T, thelast estimate impli es ( u( t, x, s ) - u( t, x, ~)
K(s,~)(u(t, x, s) + 5) (u(t, z, ~)+ ~)ds d~~.
f Tvfv
As u is bounded by I[Uoll~ (Theorem3.2), and K(s, ~) > 0 for all s, g, it follows that in the sense of measure u becomes asymptotically (~s t ~ ~) independent s. Specifically, consider time intervals IN, N + 1), then for all e > lira 14 {(t,x,s,g)
N~
~ [N,N 1)x [ 0, g) x V xF;[u(t ,x, s) - u(t,x ,g )l > e} =
Disease TransportModel
383
i.e., u(t, x, s) ~ u(t, x) in this four-dirn6nsional Lebesguemeasure sense. Using boundedness of u again, we see from (1.15) that u will then vary very slowly along most characteristics, and it follows that u(t, x) must asymptotically be independent of t and x as well (with the exception of sets of arbitrary small measure in IN, N 1) x [0, ~)). As boundedness and convergence in measure imply convergence in 1, the assertion follows. | Note that the density of infectives tending asymptotically to zero and the density of susceptibles tending aymptotically to a constant agrees with the result in [8]. For their diffusion modelthey are able to showthat if the initial susceptible density is positive (on a set of positive Lebesgue measure), then the density of susceptibles tends to a positive constant as t tends to ~ ; see [8, Theorem2.5].
4
REFLECTIVE
BOUNDARY
CONDITIONS
Our monotone approximation scheme, the resulting existence and uniqueness theorem for periodic boundary conditions (Theorem 2.4), and the asymptotic behaviour of Theorem 3.1 readily generalize to the case of reflective (Neumann) boundary conditions under an additional symmetry assumption on the kernels. The Neumannboundary conditions read u(t,x,s)
= u(t,x,-s)
Weconsider initial
and w(t,x,s)
= w(t,x,-s),
x = 0,
(4.1)
data satisfying the boundary conditions,
Uo(X,S) = Uo(X,-S)
and Wo(X,S) = Wo(X,-S),
x = 0, e. (4.2)
As is done for the Neumannproblem of the heat equation, we apply a reflection. Extend the initial data to [-~, ~] by uo(x, s) = Uo(-X, -s) and Wo(X, s) = Wo(-X, -s),
-g <_ x < O.
In view of (4.2) the extension is continuous at x = 0. Then we extend the data 2g-periodic functions on the real line. THEOREM 4.1 Consider system (1.13) under the assuznption that the kernel K satisfies K(s, ~) = K(-s, -~) and similar assumptions for [( and L. With 2~periodic boundary conditions as described above, the solution satisfies the symmetry conditions u(t,x,s)
= u(t,-x,-s)
and w(t,x,s)
=w(t,-x,-s).
Proof. If u(t, x, s), w(t, x, s) is a mild solution of this initial boundaryvalue problem, then u(t,-x,-s), w(t,-x,-s) is also a solution. This is checked by considering (1.15) and by using the assumptions on the kernel. As by construction, the initial values satisfy uo(x,s)
= Uo(-X,-S)
and wo(x,s)
= Wo(-x,-s),
384
Hadeleret al.
it follows that u(t,x, s) and u(t,-x,-s) are both solutions for the same initial values. So by uniqueness, the result is proved. | COROLLARY 4.2 Under the assumptions of Theorem 4.1, mann) boundary conditions (4.1) are satisfied.
the reflecting
(Neu-
Proof. Let x = 0 and x = t~ in Theorem 4.1. I If, in addition to the assumption on K in Theorem 4.1, K(s,g) = K(g,s) as imposed in Theorem 3.3, the convergence result of that theorem holds also for Neumannboundary conditions, since the convex functional E is nonnegative, see [5, Th. 8.5.1]. Based on similar results for the Boltzmannequation (see [5]), we expect that existence and uniqueness results based on our monotoneapproximation scheme can also be proved for moregeneral reflection laws (e.g., diffusive reflection) at the boundaries, and also for higher spatial dimensions. However, the elegant reduction to the periodic boundary conditions, as shownabove, is then not possible. Instead, use must be made of a solution procedure that tracks characteristics until they hit the boundary, and then continues solutions by using the boundary conditions. In conclusion, we have formulated a new spatially dependent SIR disease transmission model that allows for infection distance via motion. Our model is related to the diffusive spread models, but leads to finite speeds of propagation because of the bounds on the velocity domain. Wehave addressed certain analytical questions about our model, but others remain. For example, fbr periodic and zero Neumann boundary conditions it is plausible that Ro = ~/a plays the same role as in the ordinary differential equations case. But so far we have not proved a threshold theoreIn for the space-dependent problem. ACKNOWLEDGEMENTS We thank Hartmut Schwetlick for suggesting the energy functional used in Theorem3.3, and Dick Phan for constructive discussions. REFERENCES 1.
2. 3. 4. 5.
6. 7.
D.G. ARONSON, The asymptotic speed of propagation of a simple epidemic. In: W.E. Fitzgibbon, H.F. Walker (eds), Nonlinear Diffusion, p. 1-23, Pitman Research Notes in Mathematics 14, 1977. C. ATKINSON ANDG.E.H. REUTER,Deterministic epidemic waves, Math. Proc. Cambridge Philos. Soc. 80, (~976), 315-330. V. CAPASSO, Global solution for a diffusive nonlinear deterministic epidemic model, SIAMJ. Appl. Math. 35, (1978), 274-294. K.M. CASEANDP.F. ZWEWE~, Linear Transport Theory, Addison-Wesley, Massachusetts 1967. C. CERCIGNANI, R. ILLNER, AND M. PULVIRENTI, The Mathematical Theory of Dilute Gases, Springer Verlag 1994. O. DIEKMANN, Thresholds and travelling waves for the geographical spread of infection. J. Math. Biol. 6, (1978), 109-130. O. DIEKMANN, J.A.P. H~nsTE~tnE~z, ANDJ.A.J. ME,Z, The legacy of Kermack and McKendrick. In (D. Mollison, ed.) Epidemic Models: Their Structure and Relation to Data, p. 95-115, Cambridge University Press 1995.
Disease TransportModel 8.
9.
10.
11.
12.
13. 14. 15. 16. 17. 18.
19. 20.
21. 22. 23.
385
W. FITZGIBBON, M. PARROT,G. WEBB, Diffusive epidemic models with spatial and age dependent heteorogeneity, Discrete and Continuous Dynamical Systems 1, (1995), 35-57. K.P. HADELER, Travelling epidemic waves and correlated random walks. In: M. Martelli et al. (eds) Differential Equations and Applications to Biology and Industry. Proc. Conf. Claremont 1994, p. 145-156, World Scientific 1995. K.P. HADELER, Spatial epidemic spread by correlated random walk, the case of slow infectives. In: R.A. Jarvis et al. (eds) Ordinary and Partial Differential Equations, p. 18-32, Pitman Research Notes in Mathematics 370, 1997. K.P. HADELER, Reaction telegraph equations and random walk systems. In: S. van Strien, S. Verduyn Lunel (eds), Stochastic and spatial structures dynamical systems. Roy. Acad. of the Netherlands, p. 133-161, North Holland, Amsterdam 1996. K.P. HADELER, Reaction transport systems in biological modelling. In: V. Capasso, O. Diekmann (eds) Mathematics inspired by Biology. CIMELectures 1997, Lecture Notes in Mathematics, Springer Verlag 1999. T. HILLENAND A. STEVENS, Hyperbolic models for chemotaxis in l-D, Nonlinear Analysis, to appear. R. ILLNER,Global existence for two-velocity models of the Boltzmann equation, Math. Meth. Appl. Sci. 1, (1979), 187-193. M. KAC,A stochastic model related to the telegrapher’s equation, (1956), reprinted in Rocky Mtn. Math. J. 4 (1974) 497-509. A. KXLLI~N, Thresholds and travelling waves in an epidemic model for rabies, Nonlinear Analysis TMA8, (1984), 851-856. S. KANIELANDM. SHINBROT, The Boltzmann equation. L Uniqueness and local existence, Commun.Math. Phys. 58, (1978), 65-84. D.G. KENDALL, Mathematical models of the spread of infection, Mathematics and Computer Science in Biology and Medicine, p. 213-225, Medical Research Council HMSO,London, 1965. W.O. KERMACK ANDA.G. MCKENDRICK, A contribution to the mathematical theory of epidemics, Proc. Roy. Soc., Al15, (1927), 700-721. P. DE MOTTONI,E. ORLANDI,ANDA. TESEI, Asymptotic behavior for a system describing epidemics with migration and spatial spread of infection, Nonl. Anal. TMA3, (1979), 663-675. H.G. OTHMER, S.R. DUNBAR, W. ALT, Models of dispersal in biological systems, J. Math. Biol. 26, (1988), 263-298. H. SCHWETLICK, Reaktionstransportgleichungen, Dissertation University of Tiibingen 1998. G.F. WEBB,An age-dependent epidemic model with spatial diffusion, Arch. Rat. Mech. Anal. 75, (1980), 91-102.
Blow Up and Hovering in Parabolic with Singular Interactions : Can We "See" a Hyperfunction ?
Systems
GONTERLUMERInstitut de Math~natique et Intbrmatique, UniversitY. de Mons-Hainaut, Mons, Belgium / Solvay Institutes for Physics and Chemistry, Brussels, Belgium.
INTRODUCTION Briefly said and anticipating a little on terminology clarified later (1), the purpose of this paper is to investigate the relation(s) between "signals" and "responses" parabolic systems with interactions represented by distributions or hyperfunctions. First for the momentlet us recall (from [3]) that in the setting of a general Banach space X a system as mentioned above, and in the title, is considered to be governed by an equation of the form (more details in section 1)
(P)
u’ = ~u+ F(t) .(0_) = (si .)(0) B.(t) = ~(t) t
where a is a distribution or hyperfunction with support 0 and values in H C X (see section 1). The crucial ingredients in (P) -- setting F = f = T = 0(~) -- are which we call "signal" (see section 1 and [5]) and the corresponding solution u (P), defined for t > 0, called "response" (to a). Henceforth we thus assume in paper F=f=~=0. For such problems (P), when a is a "true" hyperfunction (meaning "it does reduce to a distribution") there can exist a # 0 with response identically 0; such ~Using the terminology of [3] and [2] or what is recalled of it here below in sections (} and 1, and otherwise explained in these sections. 2(P) is linear and hence by superposition F(t), f, ~o(t), play a well-known standard role.
387
388
Lumer
a are called nondetectable signals (in short nds), see [5].(3). Hence for a given response u the set of a giving rise to that u, which we shall denote E(u) and call "signal set" of u, maycontain in general infinitely manyelements. Of course is of the form {go + n : n any ads, or 0}. As said at the beginning we study the relations between u and E(u) in particular what can we say about E(u) knowing u (for t > 0) It follows already from a result in [3], that if E(u) contains a distribution the latter is uniquely determined and it is not difficult to see that it can indeed be computed from u, so that it is clear what is ~neant by the statements : "u co~nes from (uniquely determined) distribution" or "u does not come from a distribution". In this paper we mainly obtain the following : (a) In section 2 we show that if u comes from a distribution and is not identically 0 there must be blow up, i.e. Ilu(t)ll ~ oc as t --~ 0+. As a consequence, since we also show that there exist responses u ¢ 0 which stay bounded ("hovering responses"), we establish the existence of phenomenapermitting in principle to verify "visually" (film) an event that can only be caused by a true hyperfunction (detecting the latter without going through any analytic conditions difficult to verify). There is indeed a large class of such phenomena. (b) An essential general question is answered in section 3 : can one always recognize from knowing u, whether it comes from a distribution or not. Wegive such a characterization (howevernot of the "directly verifiable" kind of the results in section 2). In section 4, spectral expansions of u(t) are used to exhibit situations with blow much"steeper" than what distributions can produce suchas Ilu(t)ll = ON/’/z (while it is easily seen that distributions lead at worst to O(1/t~), integer _>0). up
1
ASSUMPTIONS. TERMINOLOGY
RECALLING
KNOWN FACTS,
NOTATIONS,
First we clarify assumptions, recall knownfacts, about (P). ~ is the "free operator" associated to A generator of a bounded irregular analytic semigroupQ(t) on X, [31, [4], [11, via: D(ft)=D(A)®H
.4 :H~0 ,
(1)
Ac J,.
H c X is the space of "harmonic elements" used as "boundary~ values" (the intuitive image is : for X = C(~), associate to C(O~) via harmonic (A-harmonic’ extension H C C(fl) = X)i the connection with the boundary operator B is B~ = B : X onto H, ker B = D(A). (here D(A) ~ X except trivial Also :
(2)
situations.) A-1 is compact.
3Unlike [5], here and henceforth, unless we specify "classical nds".
we shall
not insist
(3) on an nds occuring
"in classical
A context"
Blow-Upand Hoveringin Parabolic Systems
389
For the (asymptotic) definition and construction of solutions u of (P) we refer [3], [2]. Werecall that we can alwayswrite [3],. [5]:
j----l
j----1
and that (P) (as here with F = f = ~ = 0) has always a unique solution given
u(t)=-~Q(J)(t)c~
for
t>0.
(5)
The assumptions above are sometimes a little stronger than in [3], for a more efficient development, since they remain fully realistic, in line with what is really satisfied in the classical contexts. Werefer to [3], [2], [5], for all that is not indicated explicitely above or elsewhere in this paper.
2
BLOW UP AND HOVERING
THEOREM 1 If u # 0 comes from a distribution
then [[u(t)[]
-~ cx) as t -+
PROOF If u comes from a distribution then it is given by (5) with all cj = 0 for j > some N integer >_ 1. Weshall show that under these circumstances if Ilu(t)ll does not tend to oc as t ~ 0 all cj = 0 thus reaching a contradiction (with u ~ 0). Werecall (see [3], [1]) that since Q(t) is boundedirregular analytic the following holds: Vt > 0 Q(t) : X -+ D(A); Q(t) -~ 1 (strongly)
on D(A) as t -~ 0,
(6)
and that in view of (2) we have D(A) N H = 0.
(7)
Weproceed nowin several steps : (i) First suppose there exists a sequence (in of positive numbers t~ tending to 0 such that A-Nu(tk) -+ some limit g. Then N
-A-~Vu(tk)
N
= E A-~VQ(J)(tk)cj j=l
= E A-~VAJQ(t~)cJ j:l
N
N-1
= e(t~)~A-(X-J)ci
= Q(t~) E A-(N-~)cJ
j=l
+ Q(tk)c~v.
(8)
j=l
In view of (6) the first of the just preceding 2 summandshas by itself a limit, hence Q(tk)cN -~ some limit gN. And again by (6) we have eN ~ D(A). But then A-~t?N = limA-~Q(tk)cg (since A-~CNe D(A)), so
= limQ(ta)A-~cN
(9) = A-leg again using (6)
eN = CN ~ HN D(A) = 0 (by (7)).
390
Lnmer
If (in case N >_ 2) we then also knowthat A-(N-~)U(tk) has a limit we can conclude that CN-1 = 0, and so on, up to c~. (ii) Supposethat for tk as in (i) Ilu(tk)ll remains bounded. Then A-s being compact (by (3)) for j = 1, 2,..., N, we can assume that A-Ju(t~) has a limit, so that from (i) abovefollows cj = 0 (all j _> 1, i.e. all j). (iii) If Ilu(t)l[ does not tend to co as t ~ 0, then there exists a sequence k) t k as mentionedin (ii) above and we get cj = 0 for all j. This concludes the proof. ¯ COROLLARY 2 If a response u is non zero and remains bouuded for t > 0 it can not come fi’om a distribution. Notice that it can be shown (using amongother things (3)) that always u(t) -~ as t -~ 0c, and "bounded for t > 0" is equivalent to "bounded near 0". Now, are there (many) responses u as mentioned in Corollary 2 ? The answer yes. Indeed, if we examine the construction of large classes of nds a in [5] (these being classical nds in RN for all N), we see that it is based on obtaining entire oo functions f(z) = ~ 7jz j ~ -~(~) of finite order p, 0 < p < 1, whose set of zeros j--1
contains the eignevalues of A (or rather of its selfadjoint extension A in that. A context - see [5] and (10) below), combined with finding appropriate corresponding g ~ H, such that setting w = ~ 7i(f(J),
the a in question are w ®g. Going fl~rther
into details recalled fi’om [5] (details not only needed in the present discussion but also in the next section), we recall that in the context of [5] spectral computations can be made adding to the assumptions in section 1, the following : X ~ 7-/a Hilber space, .4 C A in 7/selfadjoint <_ 0, A-~ compact. The eigengalues of .~ are denoted 0 > At _> :~ _> ... >_ ~, _> ..., the corresponding eigenvectors being e~, e2,..., e,,.... See [5] section 1, (4), (5) of [5]. Withthis, can be computedin 7/, see [5] section 3, (8) of [5], for a = w ® g as mentioned few lines above u(t)
= E f(~)e~t/J"e"’
(:11)
where f(z) is as mentioned before ~ 7jz j, g = ~ /~ne~.. j=l
n=l
Nowconsider one such classical nds a = w ® g as constructed in [5] and considered above, its corresponding f and, say, A~. Then f is of the form f(A) 0(3
with f*(£l) # O, and .f* also of order p, hence (see [5]) xw’iting .f*(A) and w* = k 7~5(j), j=l
we obtain a* = w* ® g where the latter
~; ,~ J j=l
is an admissible signal
Blow-Upand Hoveringin Parabolic Systems
391
(see in [5] the last 2 lines on p.735) for (P) bu~ not longer ands. Indeed applying now (11) with f* instead of f, we get for tile new response
(12) just one example belonging to the obviously very large class of bounded non zero responses (hovering responses) of which Corollary 2 speaks. Hence we can state THEOREM 3 There exist infinitely many responses u to which Corollary 2 applies, already in the classical A, R~v, contexts, for all N, hence permitting "visually" to verify that they can only come from true hyperfunctions.
CAN WE ALWAYS "SEE" FROM u WHETHER IT A DISTRIBUTION OR NOT ?
3
COMES FROM
For orientation see (b) of Section THEOREM 4 A continuous u :]0, cc[~ X is a solution distribution iff : ~N integer >_ 1, c* E X, such that : (i)
A-Nu is bounded and exponentially for all Re z > 0;(s).
(ii)
[A(1 - B)]Jc* is defined for j = 1,..., belongs to H.
of (P) (4) coming frown
decaying, and (A-Nu)~(z) = -R(z, A)c* N - 1 and for the latter
value, N - 1,
PROOF That tile condition is necessary follows starting along lines similar to the proof of theorem 1 above; N being as defined there, we have as in (8) -A-Nu(t) = Q(t)c*; c* = A-(N-1)cl + ...
A-lcN_I + ClV,
(13)
the exponential decay follows from (3), and we take Laplace transform (see [3]). Finally, using the equality on the second line of (13), applying repeatedly the operators B and A (recalling that all cj ~ H, while by (2) B D(A) -~ O, H -~ H,)and computinga little, we find the formulas of (15) below, fi’om which the necessity (ii) results. Succinctly, this goes as follows
A(c* - Bc*) = A-!N-2)C1 +... B[A(1 - B)]c* CN-~, et c.
+ c/v-l,
For the converse, (i) tells of course at once by uniqueness of Laplace transform that
--A-Nu(t) = Q(t)c* for t > 4werecall that here (P) is with F = f = ~ = 5"~"denotes "Laplacetransformof", R(., A) denotesthe resolvent.
(14)
392
Lumer
and now by (ii)
we can define cj E H, j = N - k,k = 0,...,N*EH fork=0,...,N-2, = B[A(1-B)]kc = [A(1- B)]N-~c * ~ g
cg-k cL Somelittle
1, via :
(15)
algebraic manipulations will then show that :
A-(N-I)Cl
h- A-(N-2)c2
+ "" CN =
A-(N-1)[A(1 _ B)]N-tc * + A-(N-2)B[A(1 _ B)]N-2c * +...
(16)
A-~B[A(1 - B)]c* Bc* = c* To obtain (16), start by replacing the first summandvia
A-(N-~)[A(1 A-(N-~)[A(1
B)]N-~c* = A-IN-~)(1 - B)[A(1 _ B)]N-:c* - A-(N-~)B[A(1 - *,
B)]N-~c * =
(17)
which added to the second summandof (16) leaves A(N-e)[A(1 - B)]N-’~c *, and then do again as in (17) now with N - 2 instead of N - 1,..., (16) reducing finally to A-~[A(1 - B)]c* + Bc* = c*. Hence (14) tells that with the c~ ~ H defined in (15),
-A-N -N : A
N
N j:l
proving (see (4), (5), above) that u is indeed a solution of (P) coming N
(H-valued) distribution
4
a
A SIMPLE EXAMPLE OF SPECTRAL COMPUTATION OF BLOW UP AT RATE HIGHER THAN POLYNOMIAL IN
For orientation see the final paragraph of the introduction. The exampleis spectral estimation based on (11) above ((10) being satisfied). Wetake for the classical A, R~, context, f~ =]0, lf, X = C(~), as described in detail 4 of [5]. Here ~, = -Tr~n2; en = en(x) = x/~sinTrnx,, x ~ ~, g =
typical of simplicity in section g(x) =
Ifl,,I = v/’~/7rn. Wetake (with the notations of section 2, around (10) and (11)) w defined as follows :
393
Blow-Upand Hoveringin Parabolic Systems -’: ~r ’~2t n ~’~e
(19)
Moreovere -~2n~t >_ 1/2 iff n~u2 S ~, and the largest n (~ 1) satisfying the latter condition is of the form
n=-
1
V~
-0,0-<0<1, Y.
fort_<
rr--
in 2
(20)
Using (20) in (19), and using (11), we conclude that in sup-norm and 7~-norm L~(f~)-norm) we have for appropriate M, and 0 < t _< some to > 0,
Ilu(t)ll_>Ilu(t)llc,¢m
(21)
This illustrates a typical sort of blow up of a response u which alternatively to Corollary 2 exhibits a phenomenum that also cannot come from a distribution, this time because the blow up is too steep 6. (It is of course well knownthat for Q(t) boundedanalytic -- irregular or not -- [1], [4], [7], ItQ(~l(t)[I = O(1/tj) so for a distribution we have the (1/t)-polynomial growth mentioned in the introduction.)
REFERENCES 1. 2. 3.
4.
5.
6.
7.
G Da Prato and E Sinestrari, Differential operators with non dense domain, Ann. Scuola Normle Pisa, 14, 285-344, (1987). G Lumer, Transitions singuli~res gouvern~es par des ~quations de type parabolique, C.R. Acad. Sci. Paris, 322, sfirie I, 735-740, (1996). G Lumer, Singular interaction problems of parabolic type with distribution and hyperfunction data, in "Evolution equations...", Mathematical Topics vol.16, (Advances in PDEs,) 11-36, Wiley-VCH,Berlin, (1999). G Lumer, Semi-groupes irrfiguliers et semi-groupes int~grfis: application l’identification de semi-groupes irrfiguliers analytiques et r5sultats de gfin~ration, C.R. Acad. Sci. Paris, 314, stifle I, 1033-1038,(1992). G5GLumer and F. Neubrander, Signaux non-d~tectables en dimension N dans des syst~mes gouvern~s par des ~quati0ns de type parabolique, C.R. Acad. Sci. Paris, 325, s~rie I, 731-736, (1997). S Ouchi, On abstract Cauchy problems.in the sense of hyperfunction, in Hyperfunctions and pseudo-differential equations, Lect. Notes in Math. 287, SpringerVerlag, 135-152, (1973). A Pazy, Semigroupsof linear operators and applications to partial differential equations, Springer-Verlag, (1983).
SThelatter however doesnot lend itself to easyaccurate"visual"verification.
Some Asymptotic
Problems in Fluid
NADERMASMOUDI CEREMADE(UMR 7534), Universite Place de Lattre de Tassigny, F-75775 Paris cedex 16
1
Mechanics de Paris-Dauphine,
INTRODUCTION
In this note, we summarize some results concerning some asymptotic problems coming from fluid mechanics. These asymptotic problems arise when a dimensionless parameter ~ goes to zero in an equation describing the motion of some type of fluid (or any other physical system). Physically, this allows a better knowledgeof the prevailing phenomenonwhen this parameter is small. This small parameter usually describes a physical reality. For instance, a slightly compressible fluid is characterized by a low Machnumber, whereas a slightly viscous fluid is characterized by a high Reynolds number (which means a low viscosity). In manycases, we have different small parameters (we can be in presence of a slightly compressible and slightly viscous fluid in the same time). Depending on the way these small parameters go to zero, we can recover different systems at the limit. For instance, if ~, ~i, ~,, ~ << 1, the limit system can depend on the magnitude of the ratio of ~/(f .... These asymptotic problems allow us to get simpler models at the limit, due to the fact that we usually have fewer variables or (and) fewer unknowns. This simplifies the numerical simulations, in fact, instead of solving the initial system, we can solve the limit system and then add a corrector. Whenwe try to pass to the limit, we: encounter many mathematical problems due to the change of the type of the equations, the presence of manyspatial and temporal scales, the presence of boundary layers (we can no longer impose the same boundary conditions for the initial system and the limit one), the presence of oscillations in time at high frequency .... In the array of examples, we are going to consider we will try to answer different type of questions: 1) Whatdo the solutions of the initial system (S~) converge to ? Is the convergence strong or weak ? 2) In the case of weakconvergence, can we give a more detailed description of the sequences of solutions ? (can we describe the time oscillations for instance ?) 395
396 2
Masmoudi THE NAVIERoSTOKES
EULER LIMIT
The zero-viscosity limit for the incompressible Navier-Stokes equation in a, bounded domain, with Dirichlet boundary conditions is a challenging open problem due to the formation of a boundary layer satisfying the Prandtl equations, which seem to be ill-posed. The whole space case was performed by several authors, we can refer for instance to Swarm[30] and Kato [17]. In an other work, Bardos treats the ,case of a bounded domain with a boundary condition on the vorticity, which does not engender any boundarylayer [3]. In the sequel, we will study this limit in the case we consider different vertical and horizontal viscosities. Weconsider the following system of equations (NS,,,) Otu’~ + V(un ® un) - ~,O~zu n - ~A~,yU~ = -Up in gt V.u n =0 in
(1)
~t
(2)
ua = 0, in 0gt
(3)
with V.u~~ = 0 (4) 2, 2, where 9 = w x [0, hi, or gt = w × [0, co[, and w = V or ]R ~, = ~,~, r/= y,~. When ~, ~, go to 0, we expect that u’~ converges to the solution of the Euler system
~-(0)~o ~’~
Otw + V(w ®w) = -Vp V.w = 0 in w.n=±wa=O on O~,
(5)
w(t =O)=°.
It turns out that we are able to justify this formal derivation under an additional condition on the ratio of the vertical and horizontal viscosities. THEOREM 2.1
Let s > 5/2, and w°~Hs(l~)~,
V.w °=0,
w°.n=O
on 0~.
We assume that U"(O) converges in L2(~), ° and ~,~?,~/~? go t o O, t henany sequence of global weak solutions ( la Leray) ~ of ( 1- ~ ) s atisfying t he e ne~yy inequality satisfies u’~ - w -~ O in L~°(O,T*,L2(~2)), n -~’ 0 in L2(0, T*, v/-~Vx.~un, V~OzU where w is the unique solution of (5) in ~) L~°(0,T*; HS(~) Wegive here a sketch of the proof and refer to [26] for a complete proof. The existence of global weak solutions for (NS~,,), satisfying the energy inequality is due to J. Leray n 2
n 2
(6)
AsymptoticProblemsin Fluid Mechanics
397
This estimate does not show that un is bounded in L2(0,T; 1) and h ence i f we extract a subsequence still denoted un converging weakly to u in L’~(O,T;L2), we can not deduce that un ® un converges weakly to w ® w. If we try to use energy estimates to show that un - w remains small we see that the integrations by parts introduce terms that we cannot control, since u~ - w does not vanish at the boundary. Hence, we must construct a boundary layer which allows us to recover the Dirichlet boundary conditions : /3 will be a corrector of small L2 norm, and localized near 0f~
{/3~(z= O)+ ~(z= O) div(13 n)=O,
Bn-~0
~(z = c~) = in
2) L~(O,T*;L
a possible choice is to take B of the form
~ = -~,(z = o)e-~Z~, .. . where ~ is a free parameter to be chosen later. Wewant to explain now the idea of the proof. In stead of using energy estimates on un - w, we will work with v n = un - (w + B~). Next we write the following equation satisfied by w~ = w + ~ O~wu + wU.Vw~ _ ~O~w~ - ~A~,~wu = 0~ + ~.Vw ~ + w.VB - ,O~w~ - ~A~,~w ~ - Wp
(7)
which yields the following energy equality
[[w~(0)l[~ w~.[Ot~ + w.vB - ~O~] ~w~ - nA~,~w Next, using the weakformulation of (1), we get for all
Then adding up (6),(8)
and subtracting (9),
Finally, using that f(u.Uq)q 0, we get
(8)
398
Masmoudi
Now, we want to use a Gronwall lemma to deduce that Ilv(t)ll~ remains s~nall. By studying two terms amongthose occurring in the left hand side of the energy estimate (10), we want to show why we need the condition v/rl -~ 0. In fact
2
where, we have used the divergence-free condition O~va = -O~v~ - O~vz. Wesee from this term that we need the following condition to absorb the first term by the viscosity in (10) cCllwll~~ ~, On the other hand, the second term can be treated as Nllows
Iv f O~Bv /~
2 _<~llO~,~ll~ + ,,llO~ll~
< ~lla~llz~+~11,~11~,~ The second term of the left hand side must go to zero, this is the case if we have u/¢ ~ O. Finally, we see that If v- ~ 0 then is a possible choice.
3
COMPRESSIBLE-INCOMPRESSIBLE OF A VISCOUS FLUID
LIMIT
The general set up for such asymptotic problems, is a straightforward adaptation of the one introduced by S. Klainerman and A. Majda [18], [19] in the inviscid case (Euler equations). Werecall the compressible Navier-Stokes equations in ~he so-called isentropic regime (even though Our results are trivially adapted to the case of general barotropic flows i.e. whenthe pressure is a function of the density only). The unknowns(/5, v) are respectively the density and the velocity of the fluid (gaz). From a Physics view-point, a compressible fluid should behave (asymptotically) like an incompressible one when the density is almost consta!~t, the velocity is small and we look at large time scales. More precisely, we scale p and v (and thus p) in the following way
# =o(x,et), v =eu(x,
(]1)
and we assume that the viscosity coefficients p, ( are also small and scale like/5 e~, ~ = e( where e e (0, 1) is a "small parameter" which is called the Math number.
399
AsymptoticProblemsin Fluid Mechanics
Wealso assume that we have # > 0 and # + ~ :~ 0. With the preceding scalings, the compressible system reads
{
-~+div(pu):0,
p>_0, (12)
Opu ~ + div(pu
®u) - #Au- ~Vdivu
a + ~Vp ~ 0.
The domain ~ can be the whole space ~N, the torus TN or an open domain of ~N (with different possible boundary conditions). In fact the proof, we are going to sketch is a local one and only uses the local energy estimates. Wealso recall the incompressible Navier-Stokes system 0~ + div(u
@ u) - ~Au + Vr = 0 div(u)
= 0
Wethen consider a solution (p~, u~) of the compressible Navier-Stokes equations (12) and we assume that L:(O,T;H ~) for all T L~/(~+~)~ i.e. is continuous with respect to t > 0 with values in L:~/(~+~)endowed with the weak topology. Werequire (12) to hold in the sense of distributions. Finally, we prescribe initial conditions :p~ , p~u~
:m~°
(14)
~ ~, ~L o e L~/(~+~), m~o : 0 &.e. on{p~: 0} andp~lu~[ where p~ ~ O, p~ ~ L~, m~ o = 0 on {p~ 0}. m~on {p~ > 0}, u~ denoting by ou~=p~ = Furthermore, we assume that
2 ° ~ u~o converges weakly in L to some u and that we have p~l~l P~ =
+~ (P~)’-70~(~)’-’+(7-1)(~)"
(2.)-" f p~0
(15)
1,
where, here and below, C denotes various positive constants independent of e. Let us notice that (15) implies in particular that, roughly speaking, : indeed, we just need to rewrite (P~)~- 7P~ (~)~-~ and recall that (t ~ ~) i s c onvex on [ 0, ~ ) s ince 7~ 1. Our last requirement on (p~, u~) concerns the total energy : we assume that we have E~(t)+
D~(s)ds~E~
~hereE~(t) =
n~l~l~(~)
(divu~)~(~)andE~= i 1 o
a.e.t,
+D~0
in
~’(0,~)
.f +
U(nT)
(16)
400
Masmoudi
Wenow wish to emphasize the fact that we assume the existence of a solution with the above properties, and we shall also assume that 3’ > N ~-. Andwe recall, the
’N
results in [22] which yield the existence of such a solution precisely when 3" > -2 9 3 and N _>4, 3’_> ~ and N=3, 3’_> ~ and N=2.
THEOREM 3.1 (with P-L.Lions) In addition to the above notations and condiN tions, we assume that 3" > -~. Then, p~ converges to 1 in C([0, T]; L~) and u~ is boundedin L2(O, T; H1) for all T e (0, oc). In addition, for any subsequence of (still denoted by u~) weakly converging in L2(O, T; l) (VT e(0, cx 3)) to some u, is a solution of the incompressible Navier-Stokes equation (13) (as defined above) corresponding to the initial condition u° °. = Pu For the proof of this theorem in the periodic case, we refer to [23]. The argurnent presented there uses the group method introduced by Shochet [29] (see also [].4]). However, we want to point out that the group method does not apply to all type of boundary conditions. Wegive here a sketch of proof based on a local method