On the stabilization of solutions of the wave equation in domains with star-shaped boundaries. (Q1432700)
From MaRDI portal
| This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: On the stabilization of solutions of the wave equation in domains with star-shaped boundaries. |
scientific article; zbMATH DE number 2074954
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | On the stabilization of solutions of the wave equation in domains with star-shaped boundaries. |
scientific article; zbMATH DE number 2074954 |
Statements
On the stabilization of solutions of the wave equation in domains with star-shaped boundaries. (English)
0 references
15 June 2004
0 references
The author studies the decay rates at \(t\to\infty\) of the local energy \[ \int_{\Omega\cap \{| x| \leq R\}} (| u_t(t,x)| ^2+| \nabla u(t,x)| ^2)\,dx \] of solutions to the wave equation \(u_{tt}=\Delta u\) considered in a bounded domain \(\Omega\) with a smooth boundary, and supplemented with the Dirichlet boundary conditions and with initial data. The reasoning is based on suitable estimates of solutions to the Helmholtz equation \(\Delta v+k^2v=-h\) with the Dirichlet boundary condition.
0 references
decay rates
0 references
local energy
0 references
wave equation
0 references
Helmholtz equation
0 references