THE UNIVERSITY OF CHICAGO UNIFORM ESTIMATES FOR THE ZAKHAROV SYSTEM AND THE INITIAL-BOUNDARY VALUE PROBLEM FOR THE KORTEWEG-DE VRIES

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THE UNIVERSITY OF CHICAGO UNIFORM ESTIMATES FOR THE ZAKHAROV SYSTEM AND THE INITIAL-BOUNDARY VALUE PROBLEM FOR THE KORTEWEG-DE VRIES AND NONLINEAR SCHRÖDINGER EQUATIONS ADISSERTATIONSUBMITTEDTO THE FACULTY OF THE DIVISION OF THE PHYSICAL SCIENCES IN CANDIDACY FOR THE DEGREE OF DOCTOR OF PHILOSOPHY DEPARTMENT OF MATHEMATICS BY JUSTIN HOLMER CHICAGO, ILLINOIS JUNE 2004

CHAPTER 1 INTRODUCTION InChapter 1, we derive estimates for the 1D Zakharov system, a PDE system consisting of a nonlinear Schrödinger (NLS) equation and a nonlinear wave equation, that are uniform as the wave speed approaches. Letu 0 : R C, andn 0,n 1 : R R be giveninitial data. The 1D Zakharov system (1D ZS ɛ )is: t u ɛ = i u 2 ɛ in ɛ u ɛ (1.1) ɛ 2 t 2 n ɛ n 2 ɛ = u 2 ɛ 2 (1.2) 1D ZS ɛ = u ɛ t=0 = u 0 n ɛ t=0 = n 0 t n ɛ t=0 = n 1 where u ɛ : R [0,T] C, andn ɛ : R [0,T] R. The modernmethod of applying the contractionprinciple insuitably defined Bourgainspaces has beenused to prove local wellposedness of 1D ZS ɛ by [BC96], [GTV97] ona time interval [0,T ɛ ] whose length depends on ɛ. As a formal eercise, if we send ɛ 0in1DZS ɛ, and assume that u ɛ v for some v, thenby setting ɛ = 0 in(1.2), we epect that v solves the cubic nonlinear Schrödinger equation t v = i v 2 ± iv v 2 1D NLS = v (1.3) t=0 = u 0 In order to prove rigorous results concerning the convergence u ɛ v as ɛ 0, uniform in ɛ bounds on u ɛ onsome fied time interval [0,T] are needed. Some such uniform estimates were obtained by [AA88] from energy identities, and were applied by [AA88] and [OT92] to obtain results on the aforementioned convergence. Our 1

objective is to obtain improved uniform bounds in order to enhance the convergence results of [OT92]. The method eamined eploits local smoothing properties for the Schrödinger group e it 2 and uniform estimates for the inverse reduced wave operators P ±, defined so that (ɛ t ± )P ± z(, t) =z(, t), P ± z(, 0) = 0. By applying these estimates directly and employing a contraction argument in a suitable Banach space, [KPV95] obtained uniform estimates under a smallness assumption u 0 L 2 1 10.Themain result of this chapter removes the smallness assumption of [KPV95] by employing a different technique, previously developed by [Chi96], [KPV98] to treat NLS equations having an order 1 nonlinearity. We introduce a pseudodifferential operator B with symbol b(, ξ) S 0 depending on a constant M and satisfying e M b(, ξ) e M 2 and apply it to the k-th derivative of (1.1) inthe form t u = i 2 u ± 1 2 iup ± (uū) ifu (1.4) where + t f(, t) = 1 2 n 0( + ɛ t )+1 2 n 0( ɛ t ɛ )+1 2 ɛ ɛ t n 1 (y) dy The commutator [B,i ] 2 generates a first order term that is negative and whose size can be controlled by the constant M. Infact, by selecting M = c u 0 L 2,thiscommutator is sufficiently negative to absorb the first order terms B (± k 1 2 iup ± (uū)). The key obstacle inshowing this is that [B,P ± ] is not of lower order in (nor can it be made small by any other device). It would instead suffice if the composition BP ± B 1 were bounded independently of M; however, this turns out to be false as well. This problem is resolved by observing that BP ± B 1 is in fact bounded independently of M if we restrict to certain spatial frequency ranges, and that BP± B 1 is bounded independently of M on the complementary spatial frequency ranges. The error terms obtained by replacing P ± by P± are handled using positivity proper-

3 ties of the operators U ± = P ± + P±, and using once again that u solves (1.4). Theorem 1. Let k 4, (u 0,n 0,n 1 ) H k H 1 ( 2 d) H k 1 2 H k 3 2,andset M u 0 H 1.Then T>0with ( T e 2M + u 0 H k + n 0 H k 1 2 + n 1 H k 3 2 ) N (independent of ɛ) andasolution(u, n) to 1D ZS ɛ on [0,T] such that ɛ, 0 <ɛ 1, u L T H k + 1 D 1/2 k u L 2 L 2 T ce 2M u 0 H k (1.5) with c independent of ɛ. We remark that the proof of this result canprobably be adapted to yield a bound for any given time T>0, provided 0 <ɛ ɛ 0,where ɛ 0 = ɛ 0 (T, u 0 H k, u 0 H 1, n H k 1 2, n 1 H k 3 2 By enhancing the argument of [OT92] in places, and using in the uniform bounds furnished by Theorem 1 in place of the energy estimates of [AA88], we obtain Theorem 2. For given initial data (u 0,n 0,n 1 ),letu ɛ be the solution to 1D ZS ɛ on a time interval [0,T], andletv be the solution to 1D NLS with initial data u 0. In the noncompatible case (n 0 + u 0 ū 0 ) 0,if ) (u 0,n 0,n 1 ) (H k+1 H 1 ( 2 d)) (H k+ 1 2 L 1 ) (H k 1 2 L 1 ) (1.6) then u ɛ v L T H k cɛ where c depends on the norms of the spaces in (1.6). In the compatible case (n 0 + u 0 ū 0 )=0,if (u 0,n 0,n 1 ) (H k+2 H 1 ( 2 d)) (H k+ 3 2 L 1 ) (H k+ 1 2 Ḣ 1 L 1 ) (1.7)

4 then u ɛ v L T H k cɛ2 where c depends on the norms of the spaces in (1.7). In Chapter 2, we consider the initial-boundary value problem (IBVP) for the Korteweg de-vries (KdV) equation on the half-line and line-segment. Let S(t)φ = e iξ e itξ3 ˆφ(ξ) dξ (1.8) so that ( t + 3 )S(t)φ =0andS(0)φ = φ, andthusu(, t) =S(t)φ() solvesthe initial-value problem for the linear KdV equation. By a change of variable in the definition (1.8), one obtains the sharp smoothing properties S(t)φ() L s+1 H 3 t S(t)φ() L H s/3 t c φ H s c φ H s s+1 Therefore, time traces of solutions canbe takeninh 3 t and derivative time traces canbe takeninh s/3 t. Thus it makes sense to consider the following formulation of IBVP for KdV onthe right half-line: For f(t) H s+1 3 (R + t ), φ() Hs (R + ), find u solving t u + u 3 + u u =0 for(, t) (0, + ) (0,T) u(0,t)=f(t) for t (0,T) (1.9) u(, 0) = φ() for (0, + ) One can similarly formulate IBVP for KdV on the left-half line: For f(t) H s+1 3 (R + t ),

5 g(t) H s/3 (R + t ), φ() Hs (R ), find u solving t u + u 3 + u u =0 for(, t) (, 0) (0,T) u(0,t)=f(t) for t (0,T) u(0,t)=g(t) for t (0,T) u(, 0) = φ() for (, 0) (1.10) [CK02] introduce a new versatile method for treating problems of this type. In one section of their paper, they prove eistence and uniqueness of a solution u to problem (1.9) inthe case s = 0. Their method is to introduce a Duhamel forcing operator s+1 3 L(h)(, t), for h(t) H0 (R t ), with the properties ( t + 3 )L(h)(, t) =0 for 0 L(h)(0,t)= 1 3 h(t) L(h)(, 0) = 0 Thus, u(, t) =S(t)φ() +3L(f S(t)φ =0 )(, t) solves the linear homogeneous problem t u + u 3 =0 for 0 u(0,t)=f(t) (1.11) u(, 0) = φ() [CK02] prove suitable estimates on u solving (1.11) in terms of f(t) andφ(t), and a solutionto (1.9) for s = 0 is obtained by the contraction principle. The goal of this chapter is to adapt the techniques of [CK02] to address (1.9) for 3 4 < s < 3 2 (some estimates in[ck02] fail outside 1 2 < s < 1 2 ), and to address (1.10), where an additional boundary condition appears, for 3 4 <s<3 2.To accomplish this, we introduce analytic families of operators L λ (h)(, t), Lλ + (h)(, t),

6 for 2 < Re λ<1, with the properties ( t + 3 )Lλ (h)(, t) =0 for<0 L λ (h)(0,t)= 2 3 sin(π 3 λ + π 6 )h(t) L λ (h)(, 0) = 0 and ( t + 3 )Lλ + (h)(, t) =0 for>0 L λ + (h)(0,t)= 1 3 eπiλ h(t) L λ +(h)(, 0) = 0 The operator used by [CK02] is L = L 0 + = L0. (1.9) is solved by appropriately selecting an operator from the class L λ +, while (1.10) is solved by appropriately selecting two operators from the family L λ. Constraints on the eligible values of λ come from the required estimates. Theorem 3. Suppose 3 4 < s < 1 2. Then we have local wellposedness of (1.9) ) and local wellposedness of (1.10) for (φ, f, g) for (φ, f) H s (R + ) H s+1 3 (R + t H s (R ) H s+1 3 (R + t ) Hs/3 (R + t ). Suppose 1 2 <s<3 2. Then we have local well- ),providedφ(0) = f(0) and local posedness of (1.9) for (φ, f) H s (R + ) H s+1 3 (R + t wellposedness of (1.10) for (φ, f, g) H s (R ) H s+1 3 (R + t ) Hs/3 (R + t ),provided φ(0) = f(0). Finally, we consider the finite-length interval 0 <<1problem: t u + u 3 + u u =0 for(, t) (0, 1) (0,T) u(0,t)=g 3 (t) on (0,T) u(1,t)=g 1 (t) on (0,T) (1.12) u(1,t)=g 2 (t) on (0,T) u(, 0) = φ on(0, 1) with φ() H s ((0, 1)), g 1 (t) H s+1 3 (R + ), g 2 H 3 s (R + ), g 3 (t) H s+1 3 (R + ). This is accomplished by making use of two operators of type L λ positioned at the right

endpoint = 1 and one operator of type L λ + positioned at the left endpoint. The equation relating the desired boundary functions to the needed input functions for the forcing operators is a Fredholm equation. Theorem 4. (1.12) is locally wellposeded for 3 4 <s<3 2, s 1 2,for(φ, g 3,g 1,g 2 ) H s ((0, 1)) H s+1 3 (R + ) H s+1 3 (R + ) H 3 s (R + ), with the compatibility conditions g 3 (0) = φ(0) and g 1 (0) = φ(1) for 1 2 <s<3 2. In Chapter 3, we treat the initial-boundary value problem (IBVP) for the nonlinear Schrödinger (NLS) equation on the half-line. We introduce an operator analogous to the one used by [CK02], defined in terms of the Schrödinger group e it 2,toobtaina solutionto IBVP for NLS inthe cases s =0,s = 1. This problem, for the right-half line, takes the form: Given f H 2s+1 4 (R + t ), φ Hs (R + ), find u solving i t u + u 2 + λu u α 1 =0 u(0,t)=f(t) u(, 0) = φ() for(, t) (0, + ) (0,T) for t (0,T) for (0, + ) 7 (1.13) The left half-line problem is actually the same problem since u(, t) solvesthe left-hand problem for φ() andf(t) iffu(, t) solves the right-hand problem for φ( ) andf(t). The technique is a synthesis of the techniques in [CK02] with the standard proof of local wellposedness for NLS on the line R using the Strichartz estimates. We take the space traces and mied norm estimates for the group e it 2 and the Duhamel inhomogeneous solution operator used in the standard proof and add to them local smoothing or time traces estimates. We also need to introduce a Duhamel forcing operator L(h)(, t), satisfying (i t + 2 u)l(h)(, t) =0 L(h)(0,t)=h(t) L(h)(, 0) = 0 for 0

8 eamine its continuity and decay properties for h C0 (R), and prove space traces estimates, time traces estimates, and mied norm estimates for it. We thenpresent a solutionto the problem (1.13) by the contractionmethod for s =0,1<α<5and s =1,1<α<+. The L 2 -critical case s =0andα = 5 is also treated using the method of [CW89]. Theorem 5. There is local wellposedness of (1.13) for (φ, f) L 2 (R + ) H1/4 (R + t ) and 1 <α<5 and for (φ, f) H 1 (R + ) H3/4 (R + t ) and 1 <α<+. The primary new feature of the results obtained here, in comparison with earlier work onthe problem [SB01], [Fok02], is the limited regularity required onthe boundary data f(t).

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