Schrodinger equations: Difference between revisions

From DispersiveWiki
Jump to navigationJump to search
No edit summary
mNo edit summary
 
(17 intermediate revisions by 3 users not shown)
Line 1: Line 1:
<div class="Section1">
==Overview==


==Non-linear Schrodinger equations==
There are many '''nonlinear Schrodinger equations''' in the literature, all of which are perturbations of one sort or another of the [[free Schrodinger equation]]. One general class of such equations takes the form
 
<center>'''Overview'''</center>
 
The free Schrodinger equation
 
<center><math>i \partial_t u + \Delta u = 0</math></center>
 
where u is a complex-valued function in <math>R \times R^d</math>, describes the evolution of a free non-relativistic quantum particle in d spatial dimensions. This equation can be modified in many ways, notably by adding a potential or an obstacle, but we shall be interested in non-linear perturbations such as


<center><math>i \partial_t u + \Delta u = f (u, \overline{u}, Du, D \overline{u})</math></center>
<center><math>i \partial_t u + \Delta u = f (u, \overline{u}, Du, D \overline{u})</math></center>


where <math>D</math> denotes spatial differentiation. In such full generality, we refer to this equation as a [[derivative non-linear Schrodinger equation]] (D-NLS). If the non-linearity does not contain derivatives then we refer to this equation as a [[semilinear Schrodinger equation]] (NLS). These equations (particularly the [[cubic NLS]]) arise as model equations from several areas of physics.
where <math>D</math> denotes spatial differentiation. In such full generality, we refer to this equation as a [[derivative non-linear Schrodinger equation]] (D-NLS). If the non-linearity does not contain derivatives then we refer to this equation as a [[semilinear Schrodinger equation]] (NLS). These equations (particularly the [[cubic NLS]]) arise as model equations from several areas of physics.
Some ''linear'' perturbations of the free Schrodinger equation are also of interest in the nonlinear theory (in part because one can view nonlinear equations as linear equations in which certain coefficients themselves depend on the solution).  For instance, one can add a potential term <math>Vu</math> to the right-hand side, yielding the [[Schrodinger equation with potential]].  Or one replace the Laplacian <math>\Delta = \partial_k \partial_k</math> with a covariant Laplacian <math>(\partial_k + i A_k)(\partial_k + i A_k)</math>, leading to the [[magnetic Schrodinger equation]].  Finally, one can replace the underlying spatial domain <math>R^d</math> with a Riemannian manifold <math>(M,g)</math>, and the Laplacian with the Laplace-Beltrami operator <math>\Delta_g</math>, yielding the [[Schrodinger equation on manifolds]].  One can also allow the manifolds to have boundaries (and assume appropriate boundary conditions), leading to the [[Schrodinger equation with obstacles]].
One can combine these linear perturbations with a nonlinear one, leading for instance to the [[NLS with potential]] and the [[NLS on manifolds and obstacles]].


One can generalize both the linear and nonlinear perturbations to these equations and consider
One can generalize both the linear and nonlinear perturbations to these equations and consider
the class of [[quasilinear Schrodinger equations]] or even [[fully nonlinear Schrodinger equations]].  Needless to say, these equations are significantly more difficult to analyse than the simpler model cases discussed above.
the class of [[quasilinear Schrodinger equations]] or even [[fully nonlinear Schrodinger equations]].  Needless to say, these equations are significantly more difficult to analyse than the simpler model cases discussed above.


==Unique continuation==
One can combine these nonlinear perturbations with a [[free Schrodinger equation|linear perturbation]], leading for instance to the [[NLS with potential]] and the [[NLS on manifolds and obstacles]].
 
A question arising by analogy from the theory of unique continuation in elliptic equations, and also in control theory, is the following: if u is a solution to a nonlinear Schrodinger equation, and u(t_0) and u(t_1) is specified on a domain D at two different times t_0, t_1, does this uniquely specify the solution everywhere at all other intermediate times?
 
* For the 1D cubic NLS, with D equal to a half-line, and u assumed to vanish on D, this is in [[Bibliography#Zg1997|Zg1997]].
* For general NLS with analytic non-linearity, and with u assumed compactly supported, this is in [[Bibliography#Bo1997b|Bo1997b]].
* For D the complement of a convex cone, and arbitrary NLS of polynomial growth with a bounded potential term, this is in [[Bibliography#KnPoVe2003|KnPoVe2003]]
* For D in a half-plane, and allowing potentials in various Lebesgue spaces, this is in [IonKn-p]
* A local unique continuation theorem (asserting that a non-zero solution cannot vanish on an open set) is in [[reference:Isk1993 Isk1993]]
 
 
 
 
 
 
==Quasilinear NLS (QNLS)==
 
These are general equations of the form
 
<center><math>u_t = i a(x,t,u,Du) D^2 u + b_1(x,t,u,Du) Du + b_2(x,t,u,Du) D<u>u</u> + first order terms</math>,</center>
 
where a, b_1, b_2, and the lower order terms are smooth functions of all variables.These general systems arise in certain physical models (see e.g. [[Bibliography#BdHaSau1997|BdHaSau1997]]).Also under certain conditions they can be derived from fully nonlinear Schrodinger equations by differentiating the equation.
 
In order to qualify as a quasilinear NLS, we require that the quadratic form a is real and elliptic.It is also natural to assume that the metric structure induced by a obeys a non-trapping condition (all geodesics eventually reach spatial infinity), as this is what is necessary for the optimal local smoothing estimate to occur.For a similar reason it is useful to assume that the magnetic field b_1 (or more precisely, the imaginary part of this field) is uniformly integrable along lines in space in the time independent case (for the time dependent case the criterion involves the bicharacteristic flow and is more complicated, see [[Bibliography#Ic1984|Ic1984]]); without this condition even the linear equation can be ill-posed.
 
A model example of QNLS is the equation
 
<center><math>\partial_t u = i (\Delta - V(x))u - 2iu h' (|u|^2 ) \Delta h(|u|^2) + i u g(|u|^2)</math></center>
 
 
for smooth functions <math>h,g</math>.
 
When V=0 local existence for small data is known in <math>H^6(R^n)</math> for <math>n=1,2,3</math> [[Bibliography#BdHaSau1997|BdHaSau1997]]
 
Under certain conditions on the initial data the LWP can be extended to GWP for n=2,3 [[Bibliography#BdHaSau1997|BdHaSau1997]].
 
For large data, LWP is known in <math>H^s(R^n)</math> for any n and any sufficiently large <math>s > s(n) </math>[[Bibliography#Col2002|Col2002]]
 
For suitable choices of V LWP is also known for <math>H^\infty(R^n)</math> for any n [[Bibliography#Pop2001|Pop2001]]; this uses the Nash-Moser iteration method.
 
In one dimension, the fully nonlinear Schrodinger equation has LWP in <math>H^\infty(R^n)</math> assuming a cubic nonlinearity [[Bibliography#Pop2001b|Pop2001b]].Other LWP results for the one-dimensional QNLS have been obtained by [LimPo-p] using gauge transform arguments.
 
In general dimension, LWP for data in <math>H^{s,2}</math> for sufficiently large s has been obtained in [KnPoVe-p] assuming non-trapping, and asymptotic flatness of the metric a and of the magnetic field <math>Im b_1</math> (both decaying like <math>1/|x|^2</math> or better up to derivatives of second order).
 
[[Category:Equations]]
 
</div>


The perturbative theory of nonlinear Schrodinger equations (and the [[NLS|semilinear Schrodinger equations]] in particular) rests on a number of [[Schrodinger estimates|linear and nonlinear estimates for the free Schrodinger equation]].




==Specific Schrodinger Equations==
==Specific Schrodinger Equations==


Monomial semilinear Schrodinger equations are indexed by the degree of the nonlinearity and the spatial domain. A taxonomy of these and other specific Schrodinger equations appears on the [[Schrodinger:specific equations|specific equations]] page.
Monomial [[semilinear Schrodinger equation]]s can indexed by the degree of the nonlinearity, as follows.


===Quadratic NLS===
===Quadratic NLS===


Equations of the form
[[NLS]] equations of the form


<math> i \partial_t u + \Delta u = Q(u, \overline{u})</math>
<math> i \partial_t u + \Delta u = Q(u, \overline{u})</math>


which <math>Q(u, \overline{u})</math> a quadratic function of its arguments are [[quadratic NLS|quadratic nonlinear Schrodinger equations]].
with <math>Q(u, \overline{u})</math> a quadratic function of its arguments are [[quadratic NLS|quadratic nonlinear Schrodinger equations]].  They are mass-critical in four dimensions.


===Cubic NLS===
===Cubic NLS===


The [[cubic NLS| cubic nonlinear Schrodinger equation]] is of the form
The [[cubic NLS|cubic nonlinear Schrodinger equation]] is of the form


<math> i \partial_t u + \Delta u = \pm |u|^2 u</math>
<math> i \partial_t u + \Delta u = \pm |u|^2 u</math>
They are [[completely integrable]] in one dimension, mass-critical in two-dimensions, and energy-critical in four dimensions.


===Quartic NLS===
===Quartic NLS===


 
A [[NLS|nonlinear Schrodinger equation]] with nonlinearity of degree 4 is a [[quartic NLS|quartic nonlinear Schrodinger equation]].
A nonlinear Schrodinger equation with nonlinearity of degree 4 is a [[quartic NLS|quartic nonlinear Schrodinger equation]].


===Quintic NLS===
===Quintic NLS===


Equations of the form
[[NLS]] equations of the form


<math> i \partial_t u + \Delta u = \pm |u|^4 u</math>
<math> i \partial_t u + \Delta u = \pm |u|^4 u</math>


are [[quintic NLS|quintic nonlinear Schrodinger equations]].
are [[quintic NLS|quintic nonlinear Schrodinger equations]].  They are mass-critical in one dimension and energy-critical in three dimensions.


===Septic NLS===
===Septic NLS===


Equations of the form  
[[NLS]] equations of the form  
 


<math> i \partial_t u + \Delta u = \pm |u|^6 u</math>
<math> i \partial_t u + \Delta u = \pm |u|^6 u</math>
Line 114: Line 57:
===<math>L^2</math>-critical NLS===
===<math>L^2</math>-critical NLS===


The nonlinear Schrodinger equation
The [[NLS|nonlinear Schrodinger equation]]
 


<math> i \partial_t u + \Delta u = \pm |u|^{\frac{4}{d}} u</math>
<math> i \partial_t u + \Delta u = \pm |u|^{\frac{4}{d}} u</math>
Line 123: Line 65:
===Higher order NLS===
===Higher order NLS===


 
One can study higher-order NLS equations in which the Laplacian is replaced by a higher power. One class of such examples comes from the infinite hierarchy of commuting flows arising from the completely integrable [[cubic NLS]] on <math>R</math>. Another is the [[nonlinear Schrodinger-Airy system]].  A third class arises from the elliptic case of the [[Zakharov-Schulman system]].
One can study higher-order NLS equations in which the Laplacian is replaced by a higher power.One class of such examples comes from the infinite hierarchy of commuting flows arising from the completely integrable [Schrodinger:cubic NLS| cubic NLS] on <math>R</math> .Another is the [kdv:Schrodinger_Airy nonlinear Schrodinger-Airy equation].


===Schrodinger maps===
===Schrodinger maps===


A geometric Schodinger equation that has been intensively studied is the [[Schrodinger maps|Schrodinger map equation]].
A geometric [[derivative non-linear Schrodinger equation]] that has been intensively studied is the [[Schrodinger maps|Schrodinger map equation]].  This is the Schrodinger counterpart of the [[wave maps equation]].


===Cubic DNLS on <math>R</math>===
===Cubic DNLS on <math>R</math>===


The [[cubic DNLS on R]] deriviative cubic nonlinear Schrodinger equation has nonlinearity of the form <math>i \partial_x (|u|^2 u).</math>
The [[cubic DNLS on R|deriviative cubic nonlinear Schrodinger equation]] has nonlinearity of the form <math>i \partial_x (|u|^2 u).</math>


===Hartree Equation===
===Hartree Equation===


The [[Hartree equation|Hartree equation]] has a nonlocal nonlinearity given by convolution.
The [[Hartree equation]] has a nonlocal nonlinearity given by convolution, as does the very similar [[Schrodinger-Poisson system]], and certain cases of the [[Davey-Stewartson system]].


===Maxwell-Schrodinger system===
===Maxwell-Schrodinger system===


A Schrodinger-wave system closely related to the [wave:Maxwell-Klein-Gordon|Maxwell-Klein-Gordon equation]] is the [[Maxwell-Schrodinger system]].
A Schrodinger-wave system closely related to the [[Maxwell-Klein-Gordon equation]] is the [[Maxwell-Schrodinger system]].


==Schrodinger estimates==


 
[[Category:Schrodinger]]
Solutions to the linear Schrodinger equation and its perturbations are either estimated in mixed space-time norms <math>L^q_t L^r_x</math> or <math>L^r_x L^q_t</math>, or in <math>X^{s,b}</math> spaces, defined by
[[Category:Equations]]
::<math>\| u \|_{X^{s,b}} = \| u \|_{s,b} := \| \langle \xi\rangle^s  \langle \tau -|\xi|^2\rangle^b \hat{u} \|_{L^2_{\tau,\xi}}.</math>
 
Note that these spaces are not invariant under conjugation.
 
Linear space-time estimates in which the space norm is evaluated first are known as Strichartz estimates.  They are useful for NLS without derivatives, but are much less useful for derivative non-linearities.  Other linear estimates include smoothing estimates and maximal function estimates.    The X^{s,b} spaces are used primarily for bilinear estimates, although more recently multilinear estimates have begun to appear.  These spaces and estimates first appear in the context of the Schrodinger equation in [Bo1993], although the analogous spaces for the wave equation appeared earlier [RaRe1982], [Be1983] in the context of propogation of singularities.  See also [Bo1993b], [KlMa1993].
 
[[Category:Estimates]]
 
 
See [[Schrodinger estimates]]
 
<div class="MsoNormal" style="text-align: center"><center>
----
</center></div>

Latest revision as of 03:44, 8 February 2011

Overview

There are many nonlinear Schrodinger equations in the literature, all of which are perturbations of one sort or another of the free Schrodinger equation. One general class of such equations takes the form

where denotes spatial differentiation. In such full generality, we refer to this equation as a derivative non-linear Schrodinger equation (D-NLS). If the non-linearity does not contain derivatives then we refer to this equation as a semilinear Schrodinger equation (NLS). These equations (particularly the cubic NLS) arise as model equations from several areas of physics.

One can generalize both the linear and nonlinear perturbations to these equations and consider the class of quasilinear Schrodinger equations or even fully nonlinear Schrodinger equations. Needless to say, these equations are significantly more difficult to analyse than the simpler model cases discussed above.

One can combine these nonlinear perturbations with a linear perturbation, leading for instance to the NLS with potential and the NLS on manifolds and obstacles.

The perturbative theory of nonlinear Schrodinger equations (and the semilinear Schrodinger equations in particular) rests on a number of linear and nonlinear estimates for the free Schrodinger equation.


Specific Schrodinger Equations

Monomial semilinear Schrodinger equations can indexed by the degree of the nonlinearity, as follows.

Quadratic NLS

NLS equations of the form

with a quadratic function of its arguments are quadratic nonlinear Schrodinger equations. They are mass-critical in four dimensions.

Cubic NLS

The cubic nonlinear Schrodinger equation is of the form

They are completely integrable in one dimension, mass-critical in two-dimensions, and energy-critical in four dimensions.

Quartic NLS

A nonlinear Schrodinger equation with nonlinearity of degree 4 is a quartic nonlinear Schrodinger equation.

Quintic NLS

NLS equations of the form

are quintic nonlinear Schrodinger equations. They are mass-critical in one dimension and energy-critical in three dimensions.

Septic NLS

NLS equations of the form

are septic nonlinear Schrodinger equations.

-critical NLS

The nonlinear Schrodinger equation

posed for is scaling invariant in . This family of nonlinear Schrodinger equations is therefore called the mass critical nonlinear Schrodinger equation.

Higher order NLS

One can study higher-order NLS equations in which the Laplacian is replaced by a higher power. One class of such examples comes from the infinite hierarchy of commuting flows arising from the completely integrable cubic NLS on . Another is the nonlinear Schrodinger-Airy system. A third class arises from the elliptic case of the Zakharov-Schulman system.

Schrodinger maps

A geometric derivative non-linear Schrodinger equation that has been intensively studied is the Schrodinger map equation. This is the Schrodinger counterpart of the wave maps equation.

Cubic DNLS on

The deriviative cubic nonlinear Schrodinger equation has nonlinearity of the form

Hartree Equation

The Hartree equation has a nonlocal nonlinearity given by convolution, as does the very similar Schrodinger-Poisson system, and certain cases of the Davey-Stewartson system.

Maxwell-Schrodinger system

A Schrodinger-wave system closely related to the Maxwell-Klein-Gordon equation is the Maxwell-Schrodinger system.