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We establish local-in-time Strichartz estimates for solutions of the model case Dirichlet wave equation inside cylindrical convex domains
$\Omega \subset \mathbb {R}^ 3$
with smooth boundary
$\partial \Omega \neq \emptyset $
. The key ingredients to prove Strichartz estimates are dispersive estimates, energy estimates, interpolation and
$TT^*$
arguments. Strichartz estimates for waves inside an arbitrary domain
$\Omega $
have been proved by Blair, Smith and Sogge [‘Strichartz estimates for the wave equation on manifolds with boundary’, Ann. Inst. H. Poincaré Anal. Non Linéaire26 (2009), 1817–1829]. We provide a detailed proof of the usual Strichartz estimates from dispersive estimates inside cylindrical convex domains for a certain range of the wave admissibility.
In this paper, we study global-in-time, weighted Strichartz estimates for the Dirac equation on warped product spaces in dimension
$n\geq 3$
. In particular, we prove estimates for the dynamics restricted to eigenspaces of the Dirac operator on the compact spin manifolds defining the ambient manifold under some explicit sufficient condition on the metric and estimates with loss of angular derivatives for general initial data in the setting of spherically symmetric and asymptotically flat manifolds.
In this chapterwe give a briefsurvey of basic results on the dispersive decay due to P. D’Ancona, M. Beals, M. Beceanu, M. B. Erdo?an, L. Fanelli, M. Goldberg,W. R. Green, V. A. Marchenko, B. Marshall, W. Strauss, S. Wainger, I. Rodnianski, W. Schlag, D. Tataru, K. Yajima, and others. Moreover, we present a new short and simplified proof of the fundamental results on the L^1-L^\infty dispersive decay forthe Schrödingerequation established by J.-L. Journé, A. Soffer, and C. D. Sogge.
We consider the linearization of the three-dimensional water waves equation with surface tension about a flat interface. Using oscillatory integral methods, we prove that solutions of this equation demonstrate dispersive decay at the somewhat surprising rate of ${{t}^{-5/6}}$. This rate is due to competition between surface tension and gravitation at $O(1)$ wave numbers and is connected to the fact that, in the presence of surface tension, there is a so-called “slowest wave”. Additionally, we combine our dispersive estimates with ${{L}^{2}}$ type energy bounds to prove a family of Strichartz estimates.
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