Thermodynamics of the Stephani Universes

DOI10.1063/1.531126zbMath0824.76100arXivgr-qc/9411021OpenAlexW2086262445MaRDI QIDQ4836824

Roberto A. Sussman, Hernando Quevedo

Publication date: 9 November 1995

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9411021

zbMATH Keywords

isometry groupfree parameterGibbs-Duhem relationFriedman-Robertson-Walker cosmologiesconformally flat solutionirrotational perfect fluid sourceunphysical temperature evolution law

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of differential geometry to physics (53Z05) Thermodynamics and heat transfer (80A99) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (3)

Entropy and anisotropy ⋮ On the thermodynamical interpretation of perfect fluid solutions of the Einstein equations with no symmetry ⋮ Towards a physical interpretation for the Stephani universes

Cites Work

• On the global geometry of the Stephani Universe
• On shear free normal flows of a perfect fluid
• Fluid spacetimes admitting a conformal Killing vector parallel to the velocity vector
• Killing vectors in conformally flat perfect fluid spacetimes
• On spherically symmetric shear-free perfect fluid configurations (neutral and charged). II. Equation of state and singularities
• On the space-times admitting a synchronization of constant curvature
• Global aspects of shear-free perfect fluids in general relativity
• Conformal Killing vectors in Robertson-Walker spacetimes
• Shear-free normal cosmological models
• Bulk viscosity and matter creation in inhomogeneous cosmologies with a shear-free fluid source

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