Cubic NLS on R4: Difference between revisions

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{{equation
| name = Cubic NLS on <math>\R^4</math>
| equation = <math>iu_t + \Delta u = \pm |u|^2 u</math>
| fields = <math>u: \R \times \R^4 \to \mathbb{C}</math>
| data = <math>u(0) \in H^s(\R^4)</math>
| hamiltonian = [[Hamiltonian]]
| linear = [[free Schrodinger equation|Schrodinger]]
| nonlinear = [[semilinear]]
| critical = <math>\dot H^1(\R)</math>
| criticality = mass-supercritical;<br> energy-critical;<br> scattering-subcritical
| covariance = [[Galilean]]
| lwp = <math>H^s(\R)</math> for <math>s \geq 1</math>
| gwp = <math>H^s(\R)</math> for <math>s \geq 1</math> (+)<br>or for <math>s \geq 1</math>, small norm (-)
| parent = [[cubic NLS]]
| special = -
| related = [[quintic NLS on R3]]
}}
The theory of the [[cubic NLS]] in R^4 is as follows.
The theory of the [[cubic NLS]] in R^4 is as follows.


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* LWP is known for <math>s \ge 1\,</math> [[CaWe1990]].
* LWP is known for <math>s \ge 1\,</math> [[CaWe1990]].
** For <math>s=1\,</math> the time of existence depends on the profile of the data as well as the norm.
** For <math>s=1\,</math> the time of existence depends on the profile of the data as well as the norm.
** For <math>s<1\,</math> we have ill-posedness, indeed the H^s norm can get arbitrarily large arbitrarily quickly [[CtCoTa-p2]]. In the focusing case we have instantaneous blowup from the virial identity and scaling.
** For <math>s<1\,</math> we have ill-posedness, indeed the H^s norm can get arbitrarily large arbitrarily quickly [[CtCoTa-p2]]. In the focusing case we have instantaneous blowup from the [[virial identity]] and scaling.
* GWP and scattering for <math>s\ge 1\,</math> in the radial case [[Bo1999]]. A major obstacle is that the Morawetz estimate only gives <math>L^4\,</math>-type spacetime control rather than <math>L^6\,.</math>
* GWP and scattering for <math>s\ge 1\,</math> (Ryckman-Visan)
** For small non-radial <math>H^1\,</math> data one has GWP and scattering. In fact one has scattering whenever the solution has a bounded <math>L^6\,</math> norm in spacetime.
** In the radial case this is in [[Bo1999]].  
 
** For small energy data this is in [[CaWe1990]].
<br /> The large data non-radial case is still open, and very interesting. The main difficulty is infinite speed of propagation and the possibility that the <math>H^1\,</math> norm could concentrate at several different places simultaneously.


[[Category:Schrodinger]]
[[Category:Schrodinger]]
[[Category:Equations]]
[[Category:Equations]]

Latest revision as of 06:24, 21 July 2007

Cubic NLS on
Description
Equation
Fields
Data class
Basic characteristics
Structure Hamiltonian
Nonlinearity semilinear
Linear component Schrodinger
Critical regularity
Criticality mass-supercritical;
energy-critical;
scattering-subcritical
Covariance Galilean
Theoretical results
LWP for
GWP for (+)
or for , small norm (-)
Related equations
Parent class cubic NLS
Special cases -
Other related quintic NLS on R3


The theory of the cubic NLS in R^4 is as follows.

  • Scaling is .
  • LWP is known for CaWe1990.
    • For the time of existence depends on the profile of the data as well as the norm.
    • For we have ill-posedness, indeed the H^s norm can get arbitrarily large arbitrarily quickly CtCoTa-p2. In the focusing case we have instantaneous blowup from the virial identity and scaling.
  • GWP and scattering for (Ryckman-Visan)
    • In the radial case this is in Bo1999.
    • For small energy data this is in CaWe1990.