On the effective inertial mass density of a dissipative fluid

DOI10.1016/S0375-9601(01)00818-0zbMath0997.82033arXivgr-qc/0112010OpenAlexW3098836914MaRDI QIDQ1607317

Luis Herrera

Publication date: 31 July 2002

Published in: Physics Letters. A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0112010

zbMATH Keywords

relaxation timenonequilibriumdissipative fluideffective inertial mass density

Mathematics Subject Classification ID

Irreversible thermodynamics, including Onsager-Machlup theory (82C35)

Related Items (7)

Relativistic charged spheres: compact stars, compactness and stable configurations ⋮ Shear-free radiating collapse model via Karmarkar condition in f(R) gravity ⋮ Structure scalars in dissipative axial system in \(f(R)\) gravity ⋮ Cylindrically symmetric relativistic fluids: a study based on structure scalars ⋮ Hydrodynamic properties of dissipative fluids associated with tilted observers ⋮ THE INERTIA OF HEAT AND ITS ROLE IN THE DYNAMICS OF DISSIPATIVE COLLAPSE ⋮ The Weyl tensor and equilibrium configurations of self-gravitating fluids

Cites Work

• Unnamed Item
• Unnamed Item
• Dissipative collapse through the critical point
• Breakdown of the linear approximation in the perturbative analysis of heat conduction in relativistic systems
• Dissipative fluids out of hydrostatic equilibrium
• Thermal conduction before relaxation in slowly rotating fluids
• The contraction of gravitating spheres
• The Thermodynamics of Irreversible Processes. III. Relativistic Theory of the Simple Fluid

This page was built for publication: On the effective inertial mass density of a dissipative fluid