Dissipative fluids out of hydrostatic equilibrium

DOI10.1088/0264-9381/15/2/014zbMath0913.76101arXivgr-qc/9710099OpenAlexW3101130740MaRDI QIDQ4219796

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Publication date: 14 February 1999

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9710099

zbMATH Keywords

viscositystability conditionthermal conductioncausality conditionMüller-Israel-Stewart second-order phenomenological theory

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (8)

Thermal conduction before relaxation in slowly rotating fluids ⋮ Relativistic dissipative cosmological models and Abel differential equation ⋮ CAUSAL BULK VISCOUS COSMOLOGIES IN CONFORMALLY FLAT SPACETIME ⋮ Causal heat transport in inhomogeneous cosmologies ⋮ The active gravitational mass of a heat conducting sphere out of hydrostatic equilibrium. ⋮ Measuring the strength of dissipative inflation ⋮ Hyperbolic theories of dissipation: Why and when do we need them? ⋮ On the effective inertial mass density of a dissipative fluid

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