On the stabilization of solutions of the wave equation in domains with star-shaped boundaries. (Q1432700)

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scientific article; zbMATH DE number 2074954
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On the stabilization of solutions of the wave equation in domains with star-shaped boundaries.
scientific article; zbMATH DE number 2074954

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    On the stabilization of solutions of the wave equation in domains with star-shaped boundaries. (English)
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    15 June 2004
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    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.
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    decay rates
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    local energy
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    wave equation
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    Helmholtz equation
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