For ideal-gas relativistic fluids with a physical vacuum boundary, the linearized equations satisfy a priori energy estimates in weighted H^{2k} spaces.
The compressible euler equations in a physical vacuum: A comprehensive eulerian approach
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A priori estimates for the linearized relativistic Euler equations with a physical vacuum boundary and an ideal gas equation of state
For ideal-gas relativistic fluids with a physical vacuum boundary, the linearized equations satisfy a priori energy estimates in weighted H^{2k} spaces.