On the Spatial Asymptotics of Solutions of the Toda Lattice
We investigate the spatial asymptotics of decaying solutions of the Toda hierarchy and show that the asymptotic behaviour is preserved by the time evolution. In particular, we show that the leading asymptotic term is time independent. Moreover, we es…
Authors: Gerald Teschl
ON THE SP A TIAL ASYMPTOTICS OF SOLUTIONS OF THE TOD A LA TTICE GERALD TESCHL Abstract. W e inv estigate the spatial asymptotics of decaying solutions of the T oda lattice and s ho w that the asymptotic b eha vior is preserve d by the time ev olution. In particular, we sho w that the leading asymptotic term is time independent . M oreo ver, w e establish infinite propagation sp eed for the T o da lattice. All r esults are extended to the en tire T o da as we ll as the Kac–v an Mo erbeke hierarch y . 1. Introduction Since the seminal work of Ga rdner et al. [9 ] in 1 967 it is k nown that c o mpletely int egra ble wa ve equations ca n b e solved b y vir tue of the inv erse sca ttering tra ns - form. In pa rticular, this implies that short-rang e perturba tions of the free solution remain short-rang e during the tim e evolution. This raise s the q uestion to what extend spatial as ymptotical prop erties are pr eserved during time ev olution. In [1], [2] (see also [1 3]) Bondar ev a and Shubin considered the initial v alue problem for the Korteweg–de V ries (KdV) equation in the c lass of initial conditions which ha ve a prescrib ed asymptotic expansion in terms o f pow ers of the spatial v ariable. As part of their a nalysis they o btained that the leading term o f this asymptotic expansion is time independent. Inspired by this in triguing fact, the a im of the present paper is to prov e a general res ult for the T o da equation which co ntains the ana log of this result plus the known res ults for short-r ange p er turbation alluded to b efor e a s a sp ecial case. More sp ecifically , recall the T o da lattice [2 3] (in Flaschk a’s v ar iables [8]) d dt a ( n, t ) = a ( n, t ) b ( n + 1 , t ) − b ( n, t ) , d dt b ( n, t ) = 2 a ( n, t ) 2 − a ( n − 1 , t ) 2 , n ∈ Z . (1.1) It is a well studied physical mo del and the prototypical discrete in tegra ble wa ve equation. W e refer to the monog raphs [7], [10], [21], [23] o r the revie w articles [14], [22] for further informa tion. Then our main re s ult, Theorem 2.5 b elow, implies for example tha t (1.2) a ( n, t ) = 1 2 + α n δ + O ( 1 n δ + ε ) , b ( n, t ) = β n δ + O ( 1 n δ + ε ) , n → ∞ , 2000 Mathematics Subje ct Classific ation. Primary 37K40, 37K15; Secondary 35Q53, 37K10. Key wor ds and phr ases. T o da lattice, spatial asymptotics, T o da hierarc hy , Kac–v an Mo erb ek e hierarch y . W or k supported by the Austrian Science F und (FWF) under Gran t No. Y330. Discrete Con tin. Dyn. Syst. 2 7:3 , 1233–12 39 (201 0). 1 2 G. TESCHL for all t ∈ R provided this holds for the initial condition t = 0. Here α, β ∈ R and δ ≥ 0, 0 < ε ≤ 1. A few re ma rks a re in order : First of all, it is imp o rtant to point out that the error terms will in genera l grow with t (see the discussion after Theorem 2.5 for a rough time dependent b ound on the error). An analogous result holds for n → −∞ . Moreov er, there is nothing sp ecial a b o ut the p ow ers n − δ , which can b e replaced by any bounded sequence whic h, roughly sp eaking , do es decay at most expo nent ially and whose difference is asymptotica lly o f lower o rder. Finally , similar r esults hold for the Ablowit z–La dik equation. How ever, s inc e the Ablowitz–Ladik system doe s not have the s ame difference structur e s ome mo difications are neccessa r y and will be given in Michor [17]. 2. The Ca uchy problem for the Toda la ttice T o se t the stage let us re c all some basic facts for the T o da lattice. W e will o nly consider b o unded solutions a nd hence require Hyp othesi s H. 2.1. Supp ose a ( t ) , b ( t ) satisfy a ( t ) ∈ ℓ ∞ ( Z , R ) , b ( t ) ∈ ℓ ∞ ( Z , R ) , a ( n, t ) 6 = 0 , ( n, t ) ∈ Z × R , and let t 7→ ( a ( t ) , b ( t )) b e differ entiable in ℓ ∞ ( Z ) ⊕ ℓ ∞ ( Z ) . First of all, to see co mplete integrability it suffices to find a s o -called Lax pair [16], that is, tw o op erato rs H ( t ) , P ( t ) in ℓ 2 ( Z ) such that the Lax equation (2.1) d dt H ( t ) = P ( t ) H ( t ) − H ( t ) P ( t ) is eq uiv alent to (1.1). Here ℓ 2 ( Z ) deno tes the Hilber t space of squa re summable (complex-v alued) sequences over Z . One can easily convince oneself that the right choice is H ( t ) = a ( t ) S + + a − ( t ) S − + b ( t ) , P ( t ) = a ( t ) S + − a − ( t ) S − , (2.2) where ( S ± f )( n ) = f ± ( n ) = f ( n ± 1) are the usual shift op er ators. Now the Lax equation (2.1) implies that the op erator s H ( t ) for different t ∈ R are unitarily equiv a lent (cf. [21, Thm. 12.4]): Theorem 2 .2. L et P ( t ) b e a family of b ounde d skew-adjoint op er ators, such that t 7→ P ( t ) is differ entiable. Th en t her e exists a family of u nitary pr op agators U ( t, s ) for P ( t ) , that is, (2.3) d dt U ( t, s ) = P ( t ) U ( t, s ) , U ( s, s ) = 1 l . Mor e over, the L ax e quation (2.1) implies (2.4) H ( t ) = U ( t, s ) H ( s ) U ( t, s ) − 1 . As p ointed out in [19], this r esult immediately implies globa l existence of b ounded solutions of the T o da lattice as follows: Considering the Banach space of a ll b ounded real-v alued co efficients ( a ( n ) , b ( n )) (with the sup norm), lo cal exis tence is a conse- quence o f sta nda rd res ults for differential equations in Banach spaces. Moreov er, ON THE SP A TIAL ASYMPTOTICS OF SOLUTIONS OF THE TOD A LA TTICE 3 Theorem 2.2 implies that the norm k H ( t ) k is constant, which in turn pro vides a uniform bo und on the co efficie n ts o f H ( t ), (2.5) k a ( t ) k ∞ + k b ( t ) k ∞ ≤ 2 k H ( t ) k = 2 k H (0) k . Hence s olutions o f the T o da la ttice ca nnot blow up and are globa l in time (see [21, Sect. 12.2 ] for details): Theorem 2.3. Supp ose ( a 0 , b 0 ) ∈ M = ℓ ∞ ( Z , R ) ⊕ ℓ ∞ ( Z , R ) . Then ther e exists a unique int e gr al curve t 7→ ( a ( t ) , b ( t )) in C ∞ ( R , M ) of the T o da lattic e (1.1) s u ch that ( a (0) , b (0 )) = ( a 0 , b 0 ) . How ev er, more can b e shown. In fact, when consider ing the inv erse sca ttering transform for the T o da lattice it is desirable to e s tablish existence of solutions within the Marchenko class, that is, solutions satisfying (2.6) X n ∈ Z (1 + | n | ) | a ( n, t ) − 1 2 | + | b ( n, t ) | < ∞ for all t ∈ R . That this is indeed true was firs t established in [20] and rediscovered in [11] using a different metho d. F urthermo re, the w eight 1 + | n | ca n b e replaced by an (almost) arbitrary w eight function w ( n ). Lemma 2 .4. Su pp ose a ( n, t ) , b ( n, t ) is some b ounde d solution of the T o da lattic e (1.1) satisfyi ng (2.7) for one t 0 ∈ R . Then (2.7) X n ∈ Z w ( n ) | a ( n, t ) − 1 2 | + | b ( n, t ) | < ∞ , holds for al l t ∈ R , wher e w ( n ) ≥ 1 is some weight with sup n ( | w ( n +1) w ( n ) | + | w ( n ) w ( n +1) | ) < ∞ . Moreov er, as was demonstr ated in [5 ] (see also [6]), o ne can ev en replace | a ( n, t ) − 1 2 | + | b ( n, t ) | by | a ( n, t ) − ¯ a ( n, t ) | + | b ( n, t ) − ¯ b ( n, t ) | , where ¯ a ( n, t ), ¯ b ( n, t ) is some other b ounded so lutio n of the T o da lattice. See also [12], where similar res ults a re shown. This result shows that the asy mptotic b ehavior as n → ± ∞ is preserved to leading o rder by the T o da lattice. The purp ose of this pap er is to show that even the leading term is preserved (i.e., time indep endent) by the time evolution. Set (2.8) k ( a, b ) k w, p = P n ∈ Z w ( n ) | a ( n ) | p + | b ( n ) | p 1 /p , 1 ≤ p < ∞ sup n ∈ Z w ( n ) | a ( n ) | + | b ( n ) | , p = ∞ . Then one has the fo llowing result: Theorem 2.5. Le t w ( n ) ≥ 1 b e some weight with sup n ( | w ( n +1) w ( n ) | + | w ( n ) w ( n +1) | ) < ∞ and fix some 1 ≤ p ≤ ∞ . Supp ose a 0 , b 0 and ˜ a 0 , ˜ b 0 ar e b oun de d se quenc es such that (2.9) k ( a + 0 − a 0 , b + 0 − b 0 ) k w, p < ∞ and k ( ˜ a 0 , ˜ b 0 ) k w, p < ∞ . Supp ose a ( t ) , b ( t ) is the unique solution of the T o da lattic e (1.1) c orr esp onding t o the initial c onditions (2.10) a (0) = a 0 + ˜ a 0 6 = 0 , b (0) = b 0 + ˜ b 0 . 4 G. TESCHL Then this solution is of the form (2.11) a ( t ) = a 0 + ˜ a ( t ) , b ( t ) = b 0 + ˜ b ( t ) , wher e k (˜ a ( t ) , ˜ b ( t )) k w, p < ∞ for al l t ∈ R . Pr o of. The T o da e q uation (1.1) implies the differen tial equation d dt ˜ a ( n, t ) = a ( n, t ) ˜ b ( n + 1 , t ) − ˜ b ( n, t ) + b 0 ( n + 1 ) − b 0 ( n ) , d dt ˜ b ( n, t ) =2 a ( n, t ) + a 0 ( n ) ˜ a ( n, t ) − a ( n − 1 , t ) + a 0 ( n − 1) ˜ a ( n − 1 , t ) + ( a 0 ( n ) + a 0 ( n − 1))( a 0 ( n ) − a 0 ( n − 1)) , n ∈ Z (2.12) for ( ˜ a, ˜ b ). Since our requirement for w ( n ) implies that the shift ope r ators a re con- tin uous with resp ect to the norm k . k w, p and the same is true for the multiplication op erator with a b ounded seq uence, this is a n inhomogeneous linear differential equation in o ur Banach spa ce which has a unique global solution in this Banach space (e.g., [4, Sect. 1.4]). Moreover, since w ( n ) ≥ 1 this solution is b ounded and the corresp onding co efficients ( a, b ) coincide with the solution of the T o da equation from Theorem 2.3. Note that using Gr onw all’s inequalit y one can ea sily obtain an explic it bound (2.13) k (˜ a ( t ) , ˜ b ( t )) k w, p ≤ k (˜ a 0 ( t ) , ˜ b 0 ( t )) k w, p e C t + k ( a + 0 − a 0 , b + 0 − b 0 ) k w, p 1 C (e C t − 1) , where C = 4( k H k + k a 0 k ∞ ) (since k a ( t ) k ∞ ≤ k H k by (2.5)). T o se e the claim (1.2) from the in tro duction, let (2.14) a 0 ( n ) = 1 2 + α n δ , b 0 ( n ) = β n δ , α, β ∈ R , δ > 0 , for n > 0 and a 0 ( n ) = b 0 ( n ) = 0 for n ≤ 0. Now cho ose p = ∞ with (2.15) w ( n ) = ( (1 + | n | ) δ + ε , n > 0 , 1 , n ≤ 0 . and a pply the previo us theo rem. T o see Lemma 2.4, just c ho ose a 0 ( n ) = 1 2 , b 0 ( n ) = 0 and p = 1. Finally , let us remark tha t the requirement that w ( n ) do es not grow faster than exp onentially is imp o rtant. If it w ere no t present, our r esult would imply that a compact p erturbation of the free s olution a ( n, t ) = 1 2 , b ( n, t ) = 0 remains compact for all time if and only if it is equal to the free solution. This is well-known for the KdV equation [24], but we are not aware of a refer e nc e for the T o da equa tion. Theorem 2 .6. L et a ( n, t ) , b ( n, t ) b e a b ounde d solution of the T o da lattic e (1 .1 ) . If the se quenc es a ( n, t ) − 1 2 , b ( n, t ) ar e zer o for al l exc ept for a finite numb er of n ∈ Z for two differ ent times t 0 6 = t 1 , then t hey vanish identic al ly. Pr o of. Without loss we can choose t 0 = 0 and supp ose that the s equences a ( n, 0) − 1 2 , b ( n, 0) are zer o for a ll except for a finite num b er o f n . Then the ass o ciated reflection co efficients R ± ( k , 0) (see [21] Chapter 10) are rational functions with resp ect to k and by the in verse sc a ttering tra nsform ([21] Theorem 13.8 ) we hav e R ± ( k , t ) = R ± ( k , 0) exp( ± ( k − k − 1 ) t ), which is not ra tional for any t 6 = 0 unles s R ± ( k , t ) ≡ 0 . Hence it must be a pure N so liton solution, which has compa ct suppo rt if and o nly if it is trivial, N = 0. ON THE SP A TIAL ASYMPTOTICS OF SOLUTIONS OF THE TOD A LA TTICE 5 F or related unique contin uation results for the T o da eq uation s ee Kr¨ ug e r and T eschl [15]. 3. Extension to the Toda and Kac–v an Moerbeke hierarchy In this section w e show that our main res ult extends to the en tire T o da hierar- ch y (which w ill co ver the Kac–v an Mo erb eke hier arch y as well). T o this end, we int ro duce the T o da hierar ch y using the standar d Lax forma lis m following [3] (see also [10], [21]). Cho ose constants c 0 = 1 , c j , 1 ≤ j ≤ r , c r +1 = 0, and set g j ( n, t ) = j X ℓ =0 c j − ℓ h δ n , H ( t ) ℓ δ n i , h j ( n, t ) = 2 a ( n, t ) j X ℓ =0 c j − ℓ h δ n +1 , H ( t ) ℓ δ n i + c j +1 . (3.1) The sequences g j , h j satisfy the recur sion relations g 0 = 1 , h 0 = c 1 , 2 g j +1 − h j − h − j − 2 bg j = 0 , 0 ≤ j ≤ r , h j +1 − h − j +1 − 2( a 2 g + j − ( a − ) 2 g − j ) − b ( h j − h − j ) = 0 , 0 ≤ j < r . (3.2) Int ro ducing (3.3) P 2 r + 2 ( t ) = − H ( t ) r +1 + r X j =0 (2 a ( t ) g j ( t ) S + − h j ( t )) H ( t ) r − j + g r +1 ( t ) , a straightforward computation shows that the Lax equation (3.4) d dt H ( t ) − [ P 2 r + 2 ( t ) , H ( t )] = 0 , t ∈ R , is equiv ale nt to (3.5) TL r ( a ( t ) , b ( t )) = ˙ a ( t ) − a ( t ) g + r +1 ( t ) − g r +1 ( t ) ˙ b ( t ) − h r +1 ( t ) − h − r +1 ( t ) = 0 , where the dot denotes a deriv a tive with respect to t . V ary ing r ∈ N 0 yields the T o da hier arch y TL r ( a, b ) = 0 . All res ults men tioned in the pr evious section, Theorem 2.2, Theo rem 2.3, and Lemma 2 .4 rema in v alid for the en tire T o da hierarch y (see [21]) a nd so do es o ur main result: Theorem 3.1. Le t w ( n ) ≥ 1 b e some weight with sup n ( | w ( n +1) w ( n ) | + | w ( n ) w ( n +1) | ) < ∞ and fix some 1 ≤ p ≤ ∞ . Supp ose a 0 , b 0 and ˜ a 0 , ˜ b 0 ar e b oun de d se quenc es such that (3.6) k ( a + 0 − a 0 , b + 0 − b 0 ) k w, p < ∞ and k ( ˜ a 0 , ˜ b 0 ) k w, p < ∞ . Supp ose a ( t ) , b ( t ) is the unique solution of some e quation of the T o da hi er ar chy, TL r ( a, b ) = 0 , c orr esp onding to the initial c onditions (3.7) a (0) = a 0 + ˜ a 0 > 0 , b (0) = b 0 + ˜ b 0 . Then this solution is of the form (3.8) a ( t ) = a 0 + ˜ a ( t ) , b ( t ) = b 0 + ˜ b ( t ) , wher e k (˜ a ( t ) , ˜ b ( t )) k w, p < ∞ 6 G. TESCHL for al l t ∈ R . Pr o of. The pro of is almost identical to the one of Theorem 2.5. F rom TL r ( a, b ) = 0 one obtains an inhomog eneous differential equa tion for (˜ a, ˜ b ). The homo genous part is a finite sum ov er shifts of (˜ a, ˜ b ) a nd the inhomogeneo us part is a 0 ( g + 0 ,r +1 − g 0 ,r +1 ( t )) , h 0 ,r +1 − h − 0 ,r +1 , where g 0 ,r +1 , h 0 ,r +1 are formed from ( a 0 , b 0 ). Finally , it is stra ightf or ward to show that the k . k w, p norm of the inhomogeneo us pa rt is finite by induction using the recursive definition of g r +1 ( t ) and h r +1 ( t ). Similarly we also obtain Theorem 3.2. L et a ( n, t ) , b ( n, t ) b e a b ounde d solution of the of some e quation of the T o da hier ar chy, TL r ( a, b ) = 0 . If t he se qu enc es a ( n, t ) − 1 2 , b ( n, t ) ar e zer o for al l exc ept for a finite numb er of n ∈ Z fo r two differ ent times t 0 6 = t 1 , then they vanish identic al ly. Finally since the Kac – v an Mo erb eke hier arch y can b e obtained by setting b = 0 in the o dd equations of the T o da hierarchy , KM r ( a ) = TL 2 r + 1 ( a, 0) (see [18]), this last result also coveres the Kac –v a n Mo erb eke hierarch y . Ackno wledgments I w ant to thank Ira Ego rov a, F ritz Gesztesy , Thomas Kapp eler, and Helge Kr ¨ uger for discussions on this topic. References [1] I. N. B ondarev a, The Kortewe g–de V ries e quation in classes of incr e asing functions with pr escribe d asymptotic b ehavior as | x | → ∞ , M at. USSR Sb. 5 0:1 , 125–13 5 (1985). [2] I. Bondarev a and M. Sh ubin, Incr e asing asymptotic solutions o f the Kortewe g–de V ries e quation and i t s higher analo gues , So v. Math. Dokl. 2 6:3 , 716–71 9 (1982 ). [3] W. Bulla, F. Geszt esy , H. Holden, and G. T eschl, Algebr o-Ge ometric Quasi-Perio dic Finite- Gap Solutions o f the T o da and Kac-van Mo erb eke Hier ar chies , Mem. Amer. Math. So c. 135-641 , (1998 ). [4] K. 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T eschl, A lmost everything you always wante d to know ab out the T o da equa tion , Jahresb er. Deutsc h. Math.-V erein. 103 , no. 4, 149–162 (2001). [23] M. T o da, The ory of Nonline ar L attic es , 2 nd enl. edition, Springer, Berlin, 1989. [24] B. Zhang, Unique c ontinuation for the Korteweg– de V ries e quation , SIAM J. Math. A nal. 23 , 55–7 1 (1992). F acul ty of M a thema tics, University of Vienna, Nordber gstrasse 15, 1090 Wien, Aus - tria, and Interna tional Er win Schr ¨ odinger Institute for Ma thema tical Physics, Bol tz- manngasse 9, 1090 Wien, Austria E-mail addr ess : Gerald.Tesch l@univie.ac.at URL : http://w ww.mat.univi e.ac.at/ ~ gerald/
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