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Presentation on Multichannel Nonlinear Scattering for Nonintegrable equations by A. Soffer and M. I. Weinstein Presenter : Chulkwang Kwak Facultad de Matem aticas Pontificia Universidad Cat olica de Chile 2017 Participating School, KAIST


  1. Presentation on Multichannel Nonlinear Scattering for Nonintegrable equations by A. Soffer and M. I. Weinstein Presenter : Chulkwang Kwak Facultad de Matem´ aticas Pontificia Universidad Cat´ olica de Chile 2017 Participating School, KAIST August 21–25, 2017 C. Kwak August 21–25, 2017 1 / 19

  2. Part I C. Kwak August 21–25, 2017 2 / 19

  3. Nonlinear Schr¨ odinger equation Consider the nonlinear Schr¨ odinger equation with a potential V � i Φ t = [ − ∆ + V ( x ) + | Φ | 2 ]Φ , ( t, x ) ∈ R × R 3 (1) Φ(0) = Φ 0 ∈ H 1 ( R 3 ) . Aim : Asymptotic stability Given initial conditions which lie in a neighborhood of a solitary wave e iγ 0 ψ E 0 , the solution � � t � Φ( t ) = e − i 0 E ( s ) ds − γ ( t ) ( ψ E ( t ) + φ ( t )) converges asymptotically to a solitary wave of nearby energy E ± and phase γ ± in L 4 , as t → ±∞ , i.e., � t Φ( t ) ∼ e − i 0 E ( s ) ds e iγ ± ψ E ± , t → ±∞ . C. Kwak August 21–25, 2017 3 / 19

  4. Hypotheses for a potential V Hypotheses Let V : R 3 → R be a smooth function satisfying (V1) V ∈ S ( R 3 ). (V2) − ∆ + V has exactly one negative eigenvalue E ∗ on L 2 ( R 3 ) with corresponding L 2 normalized eigenfunction ψ ∗ . (V3) V ( x ) = V ( | x | ). Nonresonance Condition (NR) V satisfies (NR) condition if 0 is neither an eigenvalue nor a resonance of − ∆ + V . C. Kwak August 21–25, 2017 4 / 19

  5. Nonlinear bound state Consider a time periodic and spatially localized solution to (1) of the form Φ( t, x ) = e − iEt ψ E ( x ) . ψ E satisfies H ( E ) ψ E ≡ [ − ∆ + V ( x ) + | ψ E | 2 ] ψ E = Eψ E (2) ψ E ∈ H 2 , ψ E > 0 An H 2 -solution ψ E is called a nonlinear bound state or solitary wave profile . Note that the solution e − iEt ψ E does not converge to e − iE 0 t ψ E 0 , since there is a family of solitary waves. C. Kwak August 21–25, 2017 5 / 19

  6. Nonlinear bound state Theorem-Existence of ψ E Let E ∈ ( E ∗ , 0). Then, there exists a solution ψ E > 0 to (2) such that (a) ψ E ∈ H 2 . (b) The function E �→ � ψ E � H 2 is smooth for E � = E ∗ , and E → E ∗ � ψ E � H 2 = 0 , lim i.e. ( E, ψ E ) bifurcates from the zero solution at ( E ∗ , 0) in H 2 (and therefore in L p , 2 ≤ p ≤ ∞ thanks to Sobolev embedding). (c) For all ε > 0, | ψ E ( x ) | ≤ C E,ε e − ( | E |− ε ) | x | . (d) As E → E ∗ , � E − E ∗ � 1 2 � ψ E = [ ψ ∗ + O ( E − E ∗ )] ψ 4 ∗ in H 2 . Here ψ ∗ is the normalized ground state of − ∆ + V with corresponding eigenvalue E ∗ . C. Kwak August 21–25, 2017 6 / 19

  7. Nonlinear bound state Corollary For all E ∈ Ω, any compact subinterval of ( E ∗ , 0), we have � ψ E � H 2 ≤ C Ω � ψ E � L 2 . Theorem-Weighted estimates Let E ∈ ( E ∗ , 0). Also, E lie in a sufficiently small neighborhood of E ∗ . Then, for k ∈ Z + and s ≥ 0, �� x � k ψ E � H s ≤ C k,s � ψ E � H s and �� x � k ∂ E ψ E � H s ≤ C ′ k,s | E − E ∗ | − 1 � ψ E � H s Remark : By above theorems and corollary, we can regard any weighted L p norm of ψ E and ∂ E ψ E as a constant, which tends to 0 as E → E ∗ , in various estimates appearing in the analysis. C. Kwak August 21–25, 2017 7 / 19

  8. Decay estimates Decay estimate Let K = − ∆ + V acting on L 2 ( R 3 ), and assume Hypotheses on V . Also, V satisfies (NR). Let P c ( K ) denote the projection onto the continuous spectral part of K . If 1 /p + 1 /q = 1, 2 ≤ q ≤ ∞ , then � e itK P c ( K ) ψ � L q ≤ C q | t | − (3 / 2 − 3 /q ) � ψ � L p . If ψ is more regular ( ψ ∈ H 1 ), then � e itK P c ( K ) ψ � L q ≤ C q � t � − (3 / 2 − 3 /q ) ( � ψ � L p + � ψ � H 1 ) . A simple consequence is the following local decay estimate Local decay estimate Under the same assumption as in the above theorem, let σ > 3 / 2 − 3 /q . Then �� x � − σ e itK P c ( K ) ψ � L 2 ≤ C q | t | − (3 / 2 − 3 /q ) � ψ � L p . C. Kwak August 21–25, 2017 8 / 19

  9. Decomposition of the solution Φ We decompose the solution to (1) as Φ( t ) = e − i Θ ( ψ E ( t ) + φ ( t )) where Φ(0) = Φ 0 = e iγ 0 ( ψ E 0 + φ 0 ) � t Θ = E ( s ) ds − γ ( t ) 0 E (0) = E 0 , γ (0) = γ 0 Orthogonality Condition d � ψ E 0 , φ 0 � = 0 and dt � ψ E 0 , φ ( t ) � = 0 The orthogonality condition ensures that φ ( t ) lies in the Range of P c ( H ( E 0 )). C. Kwak August 21–25, 2017 9 / 19

  10. Decomposition of the solution Φ � iφ t = [ H ( E 0 ) − E 0 ] φ + [ E 0 − E ( t ) + ˙ γ ( t )] φ + F , (3) φ (0) = φ 0 where F = F 1 + F 2 , γψ E − i ˙ F 1 = ˙ E∂ E ψ E , F 2 = F 2 , lin + F 2 , nl . Here F 2 , lin is a linear term in φ of the form F 2 , lin = (2 ψ 2 E − ψ 2 E 0 ) φ + ψ 2 E φ and F 2 , nl is a nonlinear term in φ of the form F 2 , nl = 2 ψ E | φ | 2 + ψ E φ 2 + | φ | 2 φ. C. Kwak August 21–25, 2017 10 / 19

  11. Decomposition of the solution Φ The Orthogonality condition says φ (0) = φ 0 = P c ( H ( E 0 )) φ 0 , which implies F = P c ( H ( E 0 )) F . Moreover, we know ˙ E ( t ) = � ∂ E ψ E , ψ E 0 � − 1 Im � F 2 , ψ E 0 � and γ ( t ) = −� ψ E , ψ E 0 � − 1 Re � F 2 , ψ E 0 � . ˙ C. Kwak August 21–25, 2017 11 / 19

  12. Linear propagator of dispersive part φ Consider the homogeneous linear equation � iu t = ( H ( E 0 ) − E 0 ) u + ( E 0 − E ( t ) + ˙ γ ( t )) u, (4) u ( s ) = f. Let U ( t, s ) be the propagator associated to (4), i.e. u ( t ) = U ( t, s ) f, U ( s, s ) = Id. Using the gauge transform � t u ( t ) = e − i s [ E 0 − E ( τ )] dτ − i ( γ ( t ) − γ ( s )) v ( t ) , (4) is equivalent to the equation iv t = ( H ( E 0 ) − E 0 ) v with the initial data v ( s ) = f . The solution v is of the form v ( t ) = e − i ( H ( E 0 ) − E 0 )( t − s ) f. Hence � t U ( t, s ) = e − i s [ E 0 − E ( τ )] dτ − i ( γ ( t ) − γ ( s )) e − i ( H ( E 0 ) − E 0 )( t − s ) . (5) C. Kwak August 21–25, 2017 12 / 19

  13. Linear propagator of dispersive part φ Now (3) can be rewritten as the integral equation, in addition to the Orthogonality condition, � t φ ( t ) = U ( t, 0) P c ( H ( E 0 )) φ 0 − i U ( t, s ) P c ( H ( E 0 )) F ( s ) ds. 0 We remark that the gauge transform (5) preserves L p or weighted L 2 norms, i.e., � U ( t, s ) g � X = � e − i ( H ( E 0 ) − E 0 )( t − s ) g � X where X = L p or a weighted L 2 . C. Kwak August 21–25, 2017 13 / 19

  14. Well-posedness theory Contraction mapping principle ⇒ Local well-posedness The equation (1) admits the following mass and energy conservation laws: � R 3 | Φ( x ) | 2 dx = N [Φ 0 ] N [Φ( t )] ≡ � � � H [Φ( t )] ≡ 1 R 3 |∇ Φ( x ) | 2 dx + 1 R 3 V ( x ) | Φ( x ) | 2 dx + 1 R 3 | Φ( x ) | 4 dx 2 2 4 = H [Φ 0 ] For C 0 > 0 such that | V ( x ) | ≤ C 0 , � Φ( t ) � 2 H 1 ≤ 2 H [Φ 0 ] + ( C 0 + 1) N [Φ 0 ] ≤ C ( � Φ 0 � 2 H 1 + � Φ 0 � 4 H 1 ) Local well-posedness implies Global well-posedness C. Kwak August 21–25, 2017 14 / 19

  15. Main Theorem Theorem-Asymptotic stability Let Ω η = ( E ∗ , E ∗ + η ), where η is positive and sufficiently small. Then for all E 0 ∈ Ω η and γ 0 ∈ [0 , 2 π ), there exists a positive number ǫ = ǫ ( E 0 , η ) such that if Φ(0) = e iγ 0 ( ψ E 0 + φ 0 ) where � φ 0 � L 1 ( R 3 x ) + � φ 0 � H 1 ( R 3 x ) < ǫ then � t Φ( t ) = e − i 0 E ( s ) ds + iγ ( t ) ( ψ E ( t )+ φ ( t ) ) with ˙ γ ( t ) ∈ L 1 ( R t ) E ( t ) , ˙ ( ⇒ ∃ lim t →±∞ ( E ( t ) , γ ( t )) = ( E ± , γ ± )) C. Kwak August 21–25, 2017 15 / 19

  16. Main Theorem Theorem A. - Asymptotic stability and φ ( t ) is purely dispersive in the sense that �� x � − σ φ ( t ) � L 2 ( R 3 ) = O ( � t � − 3 2 ) for σ > 2, and � φ ( t ) � L 4 ( R 3 ) = O ( � t � − 3 4 ) as | t | → ∞ . C. Kwak August 21–25, 2017 16 / 19

  17. Decomposition of initial data Let � E ∈ ( E ∗ , 0) and � γ ∈ [0 , 2 π ) be given. Consider the initial data Φ 0 , which is nearby a nonlinear bound state: Φ 0 = e i � γ ψ � E + δ Φ . In general, � ψ � E , δ Φ � � = 0, so we can find E 0 and γ 0 such that � e − iγ 0 Φ 0 − ψ E 0 , ψ E 0 � = 0 , i.e. Φ 0 := e iγ 0 ( ψ E 0 + φ 0 ) = e iγ 0 ψ E 0 + [ e i � γ ψ � E − e iγ 0 ψ E 0 + δ Φ] . Indeed, let F [ E, γ, δ Φ] := � ψ E , φ 0 � = � e iγ ψ E , e i � γ ψ � E − e iγ ψ E + δ Φ � . Then F [ � E, � γ, 0] = 0. C. Kwak August 21–25, 2017 17 / 19

  18. Decomposition of initial data We write F [ E, γ, δ Φ] = F 1 [ E, γ, δ Φ] + iF 2 [ E, γ, δ Φ] . The Jacobian matrix of ( E, γ, δ Φ) �→ ( F 1 , F 2 ) is given by | ψ E | 2 �   � �  − 1 d 0 � 2 dE | ψ E | 2 � E = �  E � � 0 � E = � E at ( � γ, 0). Since the curve E �→ � ψ E � 2 E, � L 2 has no critical point for E ∈ ( E ∗ , 0), the determinant of the Jacobian matrix at ( � E, � γ, 0) is nonzero. By the implicit function theorem, for any δ Φ near 0, there uniquely exists ( E 0 , γ 0 ) near ( � E, � γ ) such that F [ E 0 , γ 0 , δ Φ] = 0, i.e. the decomposition Φ 0 = e iγ 0 ( ψ E 0 + φ 0 ) with � ψ E 0 , φ 0 � = 0 holds. C. Kwak August 21–25, 2017 18 / 19

  19. Thank You for Your Attention!! C. Kwak August 21–25, 2017 19 / 19

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