Growth of Sobolev norms for the cubic NLS Benoit Pausader N. - - PowerPoint PPT Presentation

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Growth of Sobolev norms for the cubic NLS Benoit Pausader N. - - PowerPoint PPT Presentation

NLS on R T 2 Growth of Sobolev norms for the cubic NLS Benoit Pausader N. Tzvetkov. Brown U. Spectral theory and mathematical physics, Cergy, June 2016 NLS on R T 2 Introduction We consider the cubic nonlinear Schr odinger


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NLS on R × T2

Growth of Sobolev norms for the cubic NLS

Benoit Pausader

  • N. Tzvetkov.

Brown U.

“Spectral theory and mathematical physics”, Cergy, June 2016

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NLS on R × T2

Introduction

We consider the cubic nonlinear Schr¨

  • dinger equation

(i∂t + ∆) u = |u|2u This is a model for dispersive evolution with nonlinear

  • perturbation. We want to understand the following questions:

What is the influence of the domain? What kind of asymptotic behavior is possible? Creation of energy at small scales/ Growth of Sobolev norms

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SLIDE 3

NLS on R × T2

Introduction

We consider the cubic nonlinear Schr¨

  • dinger equation

(i∂t + ∆) u = |u|2u This is a model for dispersive evolution with nonlinear

  • perturbation. We want to understand the following questions:

What is the influence of the domain? What kind of asymptotic behavior is possible? Creation of energy at small scales/ Growth of Sobolev norms

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NLS on R × T2

NLS as a Hamiltonian system

Hamiltonian equation H(u) =

  • X

1 2|∇gu|2 + 1 4|u|4

  • dνg,

Ω(u, v) = ℑ

  • X

uv dνg, In general, only one more conservation law M(u) =

  • X

|u|2dνg. Natural to study the equation in H1(X).

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SLIDE 5

NLS on R × T2

NLS as a Hamiltonian system

Hamiltonian equation H(u) =

  • X

1 2|∇gu|2 + 1 4|u|4

  • dνg,

Ω(u, v) = ℑ

  • X

uv dνg, In general, only one more conservation law M(u) =

  • X

|u|2dνg. Natural to study the equation in H1(X).

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SLIDE 6

NLS on R × T2

NLS as a Hamiltonian system

Hamiltonian equation H(u) =

  • X

1 2|∇gu|2 + 1 4|u|4

  • dνg,

Ω(u, v) = ℑ

  • X

uv dνg, In general, only one more conservation law M(u) =

  • X

|u|2dνg. Natural to study the equation in H1(X).

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SLIDE 7

NLS on R × T2

NLS on Rd

On Rd, the equation is reasonably well understood: GWP when d ≤ 4 and ill-posed when d ≥ 5 [Ginibre-V´ elo, Bourgain, Grillakis, CKSTT, Killip-Visan, Kenig-Merle] 2 ≤ d ≤ 4: Solutions scatters , d = 1, small Solutions modified-scattering (cubic NLS completely integrable) , solutions scatter for quintic nonlinearity. In particular, smooth solutions satisfy u(t)Hs ≤ C(u(0)H1)u(0)Hs uniformly in time. These results can be extended to some cases of domain with “large volume” (e.g.H3: Banica, Ionescu-P.-Staffilani).

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SLIDE 8

NLS on R × T2

NLS on Rd

On Rd, the equation is reasonably well understood: GWP when d ≤ 4 and ill-posed when d ≥ 5 2 ≤ d ≤ 4: Solutions scatters [. . . ,Dodson], d = 1, small Solutions modified-scattering (cubic NLS completely integrable) , solutions scatter for quintic nonlinearity. In particular, smooth solutions satisfy u(t)Hs ≤ C(u(0)H1)u(0)Hs uniformly in time. These results can be extended to some cases of domain with “large volume” (e.g.H3: Banica, Ionescu-P.-Staffilani).

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SLIDE 9

NLS on R × T2

NLS on Rd

On Rd, the equation is reasonably well understood: GWP when d ≤ 4 and ill-posed when d ≥ 5 2 ≤ d ≤ 4: Solutions scatters , d = 1, small Solutions modified-scattering (cubic NLS completely integrable) [Zakharov-Shabat, Deift-Zhou, Hayashi-Naumkin, Kato-Pusateri], solutions scatter for quintic nonlinearity. In particular, smooth solutions satisfy u(t)Hs ≤ C(u(0)H1)u(0)Hs uniformly in time. These results can be extended to some cases of domain with “large volume” (e.g.H3: Banica, Ionescu-P.-Staffilani).

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SLIDE 10

NLS on R × T2

NLS on Rd

On Rd, the equation is reasonably well understood: GWP when d ≤ 4 and ill-posed when d ≥ 5 2 ≤ d ≤ 4: Solutions scatters , d = 1, small Solutions modified-scattering (cubic NLS completely integrable) , solutions scatter for quintic nonlinearity. In particular, smooth solutions satisfy u(t)Hs ≤ C(u(0)H1)u(0)Hs uniformly in time. These results can be extended to some cases of domain with “large volume” (e.g.H3: Banica, Ionescu-P.-Staffilani).

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SLIDE 11

NLS on R × T2

NLS on Rd

On Rd, the equation is reasonably well understood: GWP when d ≤ 4 and ill-posed when d ≥ 5 2 ≤ d ≤ 4: Solutions scatters , d = 1, small Solutions modified-scattering (cubic NLS completely integrable) , solutions scatter for quintic nonlinearity. In particular, smooth solutions satisfy u(t)Hs ≤ C(u(0)H1)u(0)Hs uniformly in time. These results can be extended to some cases of domain with “large volume” (e.g.H3: Banica, Ionescu-P.-Staffilani).

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NLS on R × T2

(modified) Scattering

A solution scatters if it eventually follows the linear flow: u(t) = eit∆ {f + o(1)} , t → ∞. On R, solutions sometimes have a “modified scattering”

  • u(ξ, t) = eit∂xxF−1

ei|

f (ξ)|2 log t

f (ξ) + o(1)

  • ,

t → ∞ with a logarithmic correction.

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SLIDE 13

NLS on R × T2

(modified) Scattering

A solution scatters if it eventually follows the linear flow: u(t) = eit∆ {f + o(1)} , t → ∞. On R, solutions sometimes have a “modified scattering”

  • u(ξ, t) = eit∂xxF−1

ei|

f (ξ)|2 log t

f (ξ) + o(1)

  • ,

t → ∞ with a logarithmic correction.

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NLS on R × T2

NLS on small domains

For domains with “smaller volume”: weaker dispersion, one expects the linear flow to play a less important role. This is what we want to explore.

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NLS on R × T2

Global existence

For GWP: only need control locally in time. Expect same theory as in Rd. Verified in lower dimensions (Td: Bourgain, d = 2 or Sd: Burq-G´ erard-Tzvetkov). Even true in critical cases, e.g. T4 (Herr-Tataru-Tzvetkov, Ionescu-P.). Idea: Appropriate functional spaces to obtain small data theory. Large data, only obstruction is infinite concentration of energy at a point in space-time → blow-up analysis + concentration compactness → back to situation on Rd. However, these results are still consistent with the following picture: u(k + 1)Hs ≤ 2u(k)Hs.

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NLS on R × T2

Global existence

For GWP: only need control locally in time. Expect same theory as in Rd. Verified in lower dimensions (Td: Bourgain, d = 2 or Sd: Burq-G´ erard-Tzvetkov). Even true in critical cases, e.g. T4 (Herr-Tataru-Tzvetkov, Ionescu-P.). Idea: Appropriate functional spaces to obtain small data theory. Large data, only obstruction is infinite concentration of energy at a point in space-time → blow-up analysis + concentration compactness → back to situation on Rd. However, these results are still consistent with the following picture: u(k + 1)Hs ≤ 2u(k)Hs.

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SLIDE 17

NLS on R × T2

Global existence

For GWP: only need control locally in time. Expect same theory as in Rd. Verified in lower dimensions (Td: Bourgain, d = 2 or Sd: Burq-G´ erard-Tzvetkov). Even true in critical cases, e.g. T4 (Herr-Tataru-Tzvetkov, Ionescu-P.). Idea: Appropriate functional spaces to obtain small data theory. Large data, only obstruction is infinite concentration of energy at a point in space-time → blow-up analysis + concentration compactness → back to situation on Rd. However, these results are still consistent with the following picture: u(k + 1)Hs ≤ 2u(k)Hs.

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SLIDE 18

NLS on R × T2

Global existence

For GWP: only need control locally in time. Expect same theory as in Rd. Verified in lower dimensions (Td: Bourgain, d = 2 or Sd: Burq-G´ erard-Tzvetkov). Even true in critical cases, e.g. T4 (Herr-Tataru-Tzvetkov, Ionescu-P.). Idea: Appropriate functional spaces to obtain small data theory. Large data, only obstruction is infinite concentration of energy at a point in space-time → blow-up analysis + concentration compactness → back to situation on Rd. However, these results are still consistent with the following picture: u(k + 1)Hs ≤ 2u(k)Hs.

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SLIDE 19

NLS on R × T2

Global existence

For GWP: only need control locally in time. Expect same theory as in Rd. Verified in lower dimensions (Td: Bourgain, d = 2 or Sd: Burq-G´ erard-Tzvetkov). Even true in critical cases, e.g. T4 (Herr-Tataru-Tzvetkov, Ionescu-P.). Idea: Appropriate functional spaces to obtain small data theory. Large data, only obstruction is infinite concentration of energy at a point in space-time → blow-up analysis + concentration compactness → back to situation on Rd. However, these results are still consistent with the following picture: u(k + 1)Hs ≤ 2u(k)Hs.

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SLIDE 20

NLS on R × T2

Global existence

For GWP: only need control locally in time. Expect same theory as in Rd. Verified in lower dimensions (Td: Bourgain, d = 2 or Sd: Burq-G´ erard-Tzvetkov). Even true in critical cases, e.g. T4 (Herr-Tataru-Tzvetkov, Ionescu-P.). Idea: Appropriate functional spaces to obtain small data theory. Large data, only obstruction is infinite concentration of energy at a point in space-time → blow-up analysis + concentration compactness → back to situation on Rd. However, these results are still consistent with the following picture: u(k + 1)Hs ≤ 2u(k)Hs.

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NLS on R × T2

Asymptotic behavior

Asymptotic behavior much more difficult on a “small” domain. On Td, various heuristic arguments related to “weak turbulence”: “generic solutions will explore all of phase space”, “solutions will cascade to large frequency” “creation of small scales” A related mathematical question was asked by Bourgain (00): Does there exist a solution such that u(0)H2 1, lim sup

t→+∞

u(t)H2 = ∞ ?

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NLS on R × T2

Few evidence for norm growth

Not possible if scattering or on Rd or on T1. Difficult to control solutions globally in time on a compact domain! No explicit solution whose norm do become unbounded. Besides the growth should be slow: [Bourgain] u(t)Hs A (1 + t)A (conjecture ≪ (log t)A). Example of nontrivial globally bounded solutions (KAM results [Kuksin, Bourgain. . . ]

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NLS on R × T2

Few evidence for norm growth

Not possible if scattering or on Rd or on T1. Difficult to control solutions globally in time on a compact domain! No explicit solution whose norm do become unbounded. Besides the growth should be slow: [Bourgain] u(t)Hs A (1 + t)A (conjecture ≪ (log t)A). Example of nontrivial globally bounded solutions (KAM results [Kuksin, Bourgain. . . ]

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NLS on R × T2

Few evidence for norm growth

Not possible if scattering or on Rd or on T1. Difficult to control solutions globally in time on a compact domain! No explicit solution whose norm do become unbounded. Besides the growth should be slow: [Bourgain] u(t)Hs A (1 + t)A (conjecture ≪ (log t)A). Example of nontrivial globally bounded solutions (KAM results [Kuksin, Bourgain. . . ]

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NLS on R × T2

Few evidence for norm growth

Not possible if scattering or on Rd or on T1. Difficult to control solutions globally in time on a compact domain! No explicit solution whose norm do become unbounded. Besides the growth should be slow: [Bourgain] u(t)Hs A (1 + t)A (conjecture ≪ (log t)A). Example of nontrivial globally bounded solutions (KAM results [Kuksin, Bourgain. . . ]

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NLS on R × T2

Few evidence for norm growth (II)

Some evidence of finite growth [Kuksin]. Importantly Arbitrary finite growth on T2 [CKSTT] Given ε > 0, s > 1 and K > 0, there exists a solution u of cubic NLS on T2 and a time T such that u(0)Hs < ε, u(T)Hs > K. Related results [Hani, Kaloshin-Guardia, Procesi-Haus]. Remark: Only shows no a priori uniform bound; it is possible that the growth saturates. Recent similar results for the cubic half-wave equation on R [G´ erard-Lenzman-Pocovnicu-Raphael].

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NLS on R × T2

Few evidence for norm growth (II)

Some evidence of finite growth [Kuksin]. Importantly Arbitrary finite growth on T2 [CKSTT] Given ε > 0, s > 1 and K > 0, there exists a solution u of cubic NLS on T2 and a time T such that u(0)Hs < ε, u(T)Hs > K. Related results [Hani, Kaloshin-Guardia, Procesi-Haus]. Remark: Only shows no a priori uniform bound; it is possible that the growth saturates. Recent similar results for the cubic half-wave equation on R [G´ erard-Lenzman-Pocovnicu-Raphael].

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NLS on R × T2

The space R × T2

Nice space to test these questions R × T2: Access to nice Fourier analysis. Partially compact. One can ask the following questions: what is the threshold for asymptotically linear behavior (i.e. scattering)? what happens beyond this? These questions can be completely answered in the context of noncompact quotients of Rd (R × T2 is the most interesting example).

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NLS on R × T2

The space R × T2

Nice space to test these questions R × T2: Access to nice Fourier analysis. Partially compact. One can ask the following questions: what is the threshold for asymptotically linear behavior (i.e. scattering)? what happens beyond this? These questions can be completely answered in the context of noncompact quotients of Rd (R × T2 is the most interesting example).

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NLS on R × T2

The space R × T2

Nice space to test these questions R × T2: Access to nice Fourier analysis. Partially compact. One can ask the following questions: what is the threshold for asymptotically linear behavior (i.e. scattering)? what happens beyond this? These questions can be completely answered in the context of noncompact quotients of Rd (R × T2 is the most interesting example).

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NLS on R × T2

Scattering

[Tzvetkov-Visciglia, Hani-P.]. One can have a “nice” scattering theory for (i∂t + ∆) u = |u|p−1u

  • n R × Td

if and only if one can have a nice scattering theory for this equation on R if and only if p ≥ 5. At the limit (p = 5), the result is still true but sequences of solutions lose compactness in new ways [Hani-P.].

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NLS on R × T2

Scattering

[Tzvetkov-Visciglia, Hani-P.]. One can have a “nice” scattering theory for (i∂t + ∆) u = |u|p−1u

  • n R × Td

if and only if one can have a nice scattering theory for this equation on R if and only if p ≥ 5. At the limit (p = 5), the result is still true but sequences of solutions lose compactness in new ways [Hani-P.].

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NLS on R × T2

This only leaves one possibility for an interesting behavior: the cubic equation on R × Td. Infinite growth [HPTV, Tzvetkov-P.] Let s > 5/8, s = 1. There exists solutions of the cubic NLS on R × T2 such that lim sup

t→+∞

U(t)Hs = ∞. Not true (for small data) on R × T (some form of complete integrability). True even for some 0 < s < 1 despite the conservation laws at s = 0 and s = 1! Contrast with recent results of Killip-Visan, Koch-Tataru for the completely integrable case.

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NLS on R × T2

This only leaves one possibility for an interesting behavior: the cubic equation on R × Td. Infinite growth [HPTV, Tzvetkov-P.] Let s > 5/8, s = 1. There exists solutions of the cubic NLS on R × T2 such that lim sup

t→+∞

U(t)Hs = ∞. Not true (for small data) on R × T (some form of complete integrability). True even for some 0 < s < 1 despite the conservation laws at s = 0 and s = 1! Contrast with recent results of Killip-Visan, Koch-Tataru for the completely integrable case.

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NLS on R × T2

This only leaves one possibility for an interesting behavior: the cubic equation on R × Td. Infinite growth [HPTV, Tzvetkov-P.] Let s > 5/8, s = 1. There exists solutions of the cubic NLS on R × T2 such that lim sup

t→+∞

U(t)Hs = ∞. Not true (for small data) on R × T (some form of complete integrability). True even for some 0 < s < 1 despite the conservation laws at s = 0 and s = 1! Contrast with recent results of Killip-Visan, Koch-Tataru for the completely integrable case.

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NLS on R × T2

This only leaves one possibility for an interesting behavior: the cubic equation on R × Td. Infinite growth [HPTV, Tzvetkov-P.] Let s > 5/8, s = 1. There exists solutions of the cubic NLS on R × T2 such that lim sup

t→+∞

U(t)Hs = ∞. Not true (for small data) on R × T (some form of complete integrability). True even for some 0 < s < 1 despite the conservation laws at s = 0 and s = 1! Contrast with recent results of Killip-Visan, Koch-Tataru for the completely integrable case.

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NLS on R × T2

Appearance of the resonant system

Solutions expected to decay over time, (i∂t + ∆) u = |u|2u (∼ ε2u) to first order, solutions evolve linearly. Conjugate out the linear flow u(t) = eit∆R×Td F(t), i∂tF = N[F, F, F]

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NLS on R × T2

Appearance of the resonant system

Solutions expected to decay over time, (i∂t + ∆) u = |u|2u (∼ ε2u) to first order, solutions evolve linearly. Conjugate out the linear flow u(t) = eit∆R×Td F(t), i∂tF = N[F, F, F]

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NLS on R × T2

Appearance of the resonant system

Solutions expected to decay over time, (i∂t + ∆) u = |u|2u (∼ ε2u) to first order, solutions evolve linearly. Conjugate out the linear flow u(t) = eit∆R×Td F(t), i∂tF = N[F, F, F] FN[F, G, H](ξ, p) =

  • q−r+s=p
  • R2 eitΦ

Fq(ξ − η) Gr(ξ − η − θ) Hs(ξ − θ)dηdθ, Φ := |p|2 − |q|2 + |r|2 − |s|2 + 2ηθ

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NLS on R × T2

Appearance of the resonant system II

i∂tF = N[F, F, F] FN[F, G, H](ξ, p) =

  • q−r+s=p
  • R2 eitΦ

Fq(ξ − η, t) Gr(ξ − η − θ, t) Hs(ξ − θ, t)dηdθ, Φ := |p|2 − |q|2 + |r|2 − |s|2 + 2ηθ Expect ∂tF ≪ ε2 so main time dependence is in the phase. If |Φ| ≥ 1, can integrate terms through a normal form: i∂t F = N|Φ|≪1[F, F, F] + O(F 5), F − F = O(F 3) Quintic nonlinearities lead to scattering: can be neglected after a long enough time.

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NLS on R × T2

Appearance of the resonant system II

i∂tF = N[F, F, F] FN[F, G, H](ξ, p) =

  • q−r+s=p
  • R2 eitΦ

Fq(ξ − η, t) Gr(ξ − η − θ, t) Hs(ξ − θ, t)dηdθ, Φ := |p|2 − |q|2 + |r|2 − |s|2 + 2ηθ Expect ∂tF ≪ ε2 so main time dependence is in the phase. If |Φ| ≥ 1, can integrate terms through a normal form: i∂t F = N|Φ|≪1[F, F, F] + O(F 5), F − F = O(F 3) Quintic nonlinearities lead to scattering: can be neglected after a long enough time.

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NLS on R × T2

Appearance of the resonant system II

i∂tF = N[F, F, F] FN[F, G, H](ξ, p) =

  • q−r+s=p
  • R2 eitΦ

Fq(ξ − η, t) Gr(ξ − η − θ, t) Hs(ξ − θ, t)dηdθ, Φ := |p|2 − |q|2 + |r|2 − |s|2 + 2ηθ Expect ∂tF ≪ ε2 so main time dependence is in the phase. If |Φ| ≥ 1, can integrate terms through a normal form: i∂t F = N|Φ|≪1[F, F, F] + O(F 5), F − F = O(F 3) Quintic nonlinearities lead to scattering: can be neglected after a long enough time.

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NLS on R × T2

Appearance of the resonant system

We are left with i∂tF = R′[F, F, F] FR′[F, G, H](ξ, p) =

  • q−r+s=p
  • R2 eitΦϕ(Φ)

Fq(ξ − η, t) Gr(ξ − η − θ, t) Hs(ξ − θ, t)dηdθ, Φ := |p|2 − |q|2 + |r|2 − |s|2 + 2ηθ Main contribution comes from stationary phase η = θ = 0.

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NLS on R × T2

Appearance of the resonant system

We are left with i∂t F(ξ, p, t) = π t

  • q−r+s=p,

|q|2−|r|2+|s|2=|p|2

  • Fq(ξ, t)

Fr(ξ, t) Fs(ξ, t) This is, for each fixed ξ an ODE which is the resonant system of the cubic NLS on T2. At this point, it is a derivative analysis from the work of CKSTT to create solutions that grow.

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SLIDE 45

NLS on R × T2

Appearance of the resonant system

We are left with i∂t F(ξ, p, t) = π t

  • q−r+s=p,

|q|2−|r|2+|s|2=|p|2

  • Fq(ξ, t)

Fr(ξ, t) Fs(ξ, t) This is, for each fixed ξ an ODE which is the resonant system of the cubic NLS on T2. At this point, it is a derivative analysis from the work of CKSTT to create solutions that grow.

slide-46
SLIDE 46

NLS on R × T2

Appearance of the resonant system

We are left with i∂t F(ξ, p, t) = π t

  • q−r+s=p,

|q|2−|r|2+|s|2=|p|2

  • Fq(ξ, t)

Fr(ξ, t) Fs(ξ, t) This is, for each fixed ξ an ODE which is the resonant system of the cubic NLS on T2. At this point, it is a derivative analysis from the work of CKSTT to create solutions that grow.

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SLIDE 47

NLS on R × T2

Why R × T2 and not T2?

Although one would expect growth to appear more easily on T2, this remains an open question. All the results about growth so far rely on special solutions for the resonant system that grow. Key difference between R × T2 and T2: validity of approximation Equ(u) ≃ RS(u) + O(u5).

  • n R × T2, quintic terms scatter and thus are perturbative globally

in time.

slide-48
SLIDE 48

NLS on R × T2

Why R × T2 and not T2?

Although one would expect growth to appear more easily on T2, this remains an open question. All the results about growth so far rely on special solutions for the resonant system that grow. Key difference between R × T2 and T2: validity of approximation Equ(u) ≃ RS(u) + O(u5).

  • n R × T2, quintic terms scatter and thus are perturbative globally

in time.

slide-49
SLIDE 49

NLS on R × T2

Why R × T2 and not T2?

Although one would expect growth to appear more easily on T2, this remains an open question. All the results about growth so far rely on special solutions for the resonant system that grow. Key difference between R × T2 and T2: validity of approximation Equ(u) ≃ RS(u) + O(u5).

  • n R × T2, quintic terms scatter and thus are perturbative globally

in time.

slide-50
SLIDE 50

NLS on R × T2

Why R × T2 and not T2?

Although one would expect growth to appear more easily on T2, this remains an open question. All the results about growth so far rely on special solutions for the resonant system that grow. Key difference between R × T2 and T2: validity of approximation Equ(u) ≃ RS(u) + O(u5).

  • n R × T2, quintic terms scatter and thus are perturbative globally

in time.

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SLIDE 51

NLS on R × T2

Quite challenging finding appropriate norms in which to close the nonlinear estimates, especially in the low-regularity case s < 1 when solutions are unbounded in L∞. need to control over long time solutions of a nonintegrable ODE whose solutions can grow. Idea: use 2 norms A “Strong norm” which provides good control on the solutions (e.g. ∆u, xe−it∆u ∈ L2) but which grows slowly over time A “Weak norm” which remains bounded uniformly in time. Corresponds to a conservation law for the resonant system.

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NLS on R × T2

Quite challenging finding appropriate norms in which to close the nonlinear estimates, especially in the low-regularity case s < 1 when solutions are unbounded in L∞. need to control over long time solutions of a nonintegrable ODE whose solutions can grow. Idea: use 2 norms A “Strong norm” which provides good control on the solutions (e.g. ∆u, xe−it∆u ∈ L2) but which grows slowly over time A “Weak norm” which remains bounded uniformly in time. Corresponds to a conservation law for the resonant system.

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NLS on R × T2

Modified scattering

Modified scattering for the cubic NLS on R × T2 [HPTV, P.-Tzvetkov] Let s > 1, there exists a norm X such that any ID small in X leads to a global solution of the cubic NLS on R × T2. Moreover, this solution satisfies a modified scattering in the sense that there exists a solution of the equation ∂t Gp(ξ, t) =

  • p+q2=q1+q3

|p|2+|q2|2=|q1|2+|q3|2

  • Gq1(ξ, t)

Gq2(ξ, t) Gq3(ξ, t) such that U(t) − eit∆R×T2G(π ln t)Hs → 0.

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NLS on R × T2

Exotic solutions

All solutions to the resonant system i∂tap =

  • q−r+s=p,

|q|2−|r|2+|s|2=|p|2

aqaras correspond to an asymptotic behavior of the cubic NLS: many unusual behaviors! Growth, beating effect. . . A key missing point: good understanding of the solutions of the resonant system.

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SLIDE 55

NLS on R × T2

Exotic solutions

All solutions to the resonant system i∂tap =

  • q−r+s=p,

|q|2−|r|2+|s|2=|p|2

aqaras correspond to an asymptotic behavior of the cubic NLS: many unusual behaviors! Growth, beating effect. . . A key missing point: good understanding of the solutions of the resonant system.

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SLIDE 56

NLS on R × T2

A physical space formula for the resonant system

One can also obtain a formula for the resonant system in the physical space: a function f (x, t) =

  • p∈Zd

ap(t)eip,x is a solution if i∂tf = 2π

α=0

e−iα∆ eiα∆f (x, t) · eiα∆f (x, t) · eiα∆f (x, t)

which is the Hamiltonian associated to the “averaged perturbation” Hav = 2π

α=0

  • X

|eiα∆f |4dνdα.