Towards a physical interpretation for the Stephani universes

DOI10.1023/A:1001934118532zbMath0976.83029arXivgr-qc/9908019MaRDI QIDQ5931062

Roberto A. Sussman

Publication date: 2 May 2001

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9908019

zbMATH Keywords

Einstein equationsperfect fluid solutionsStephani universes

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (2)

Local thermal equilibrium and ideal gas Stephani universes ⋮ A class of cosmological solutions in induced matter theory with conformally flat bulk space

Cites Work

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• Isometric embedding of the spherically symmetric Stephani universe: Some explicit examples
• Ideal gas sources for the Lemaître-Tolman-Bondi metrics
• On the thermodynamical interpretation of perfect fluid solutions of the Einstein equations with no symmetry
• Cosmological Physics
• Thermodynamics of the Stephani Universes
• Time-Dependent Internal Solutions for Spherically Symmetrical Bodies in General Relativity: II. Adiabatic Radial Motions of Uniformly Dense Spheres
• Gravitational Bounce in General Relativity

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