Wave estimates: Difference between revisions

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Solutions to the linear wave equation and its perturbations are either estimated in mixed space-time norms <math>L^q_t L^r_x</math>, or in <math>X^{s,b}_{}</math> spaces, defined by
Solutions to the linear wave equation and its perturbations are either estimated in mixed space-time norms $L^q_t L^r_x$, or in $X^{s,b}$ spaces, defined by
$$\| u \|_{X^{s,b}} = \| \langle\xi\rangle^s \langle|\xi| - |\tau|\rangle^b \hat{u} ( \tau, \xi )\|_2 $$


<center><math>\| u \|_{X^{s,b}} = \| <\xi>^s <|\xi| - |\tau|>^b \hat{u} ( \tau, \xi )\|_2 </math></center>
Linear space-time estimates are known as [[Strichartz estimates]]. They are especially useful for the [[NLW|semilinear NLW without derivatives]], and also have applications to other non-linearities, although the results obtained are often non-optimal (Strichartz estimates do not exploit any null structure of the equation). The $X^{s,b}$ spaces are used primarily for [[bilinear wave estimates|bilinear estimates]], although more recently [[multilinear wave estimates|multilinear estimates have begun to appear]]. These spaces first appear in one-dimension in [[RaRe1982]] and in higher dimensions in [[Be1983]] in the context of [[propagation of singularities]]; they were used implicitly for LWP in [[KlMa1993]], while the Schrodinger and KdV analogues were developed in [[Bo1993]], [[Bo1993b]].
 
Linear space-time estimates are known as [[Strichartz estimates]]. They are especially useful for the [[NLW|semilinear NLW without derivatives]], and also have applications to other non-linearities, although the results obtained are often non-optimal (Strichartz estimates do not exploit any null structure of the equation). The <math>X^{s,b}_{}</math> spaces are used primarily for [[bilinear wave estimates|bilinear estimates], although more recently [[multilinear wave estimates|multilinear estimates have begun to appear]]. These spaces first appear in one-dimension in [[RaRe1982]] and in higher dimensions in [[Be1983]] in the context of [[propagation of singularities]]; they were used implicitly for LWP in [[KlMa1993]], while the Schrodinger and KdV analogues were developed in [[Bo1993]], [[Bo1993b]].


== Specific wave estimates ==
== Specific wave estimates ==


* [[Linear wave estimates]] ([[Strichartz estimates|Strichartz]], etc.)
* [[Linear wave estimates]] ([[Strichartz estimates|Strichartz]], [[Morawetz-type estimates|Morawetz-KSS]], [[Weighted Strichartz estimates|Weighted Strichartz]], etc.)
* [[Bilinear wave estimates]]
* [[Bilinear wave estimates]]
* [[Multilinear wave estimates]]
* [[Multilinear wave estimates]]

Latest revision as of 22:28, 8 March 2011

Solutions to the linear wave equation and its perturbations are either estimated in mixed space-time norms $L^q_t L^r_x$, or in $X^{s,b}$ spaces, defined by $$\| u \|_{X^{s,b}} = \| \langle\xi\rangle^s \langle|\xi| - |\tau|\rangle^b \hat{u} ( \tau, \xi )\|_2 $$

Linear space-time estimates are known as Strichartz estimates. They are especially useful for the semilinear NLW without derivatives, and also have applications to other non-linearities, although the results obtained are often non-optimal (Strichartz estimates do not exploit any null structure of the equation). The $X^{s,b}$ spaces are used primarily for bilinear estimates, although more recently multilinear estimates have begun to appear. These spaces first appear in one-dimension in RaRe1982 and in higher dimensions in Be1983 in the context of propagation of singularities; they were used implicitly for LWP in KlMa1993, while the Schrodinger and KdV analogues were developed in Bo1993, Bo1993b.

Specific wave estimates