Observationally homogeneous shear-free perfect fluids

DOI10.1007/BF00758973zbMath0664.76158OpenAlexW2004842474MaRDI QIDQ1115783

C. B. Collins, J. M. Lang

Publication date: 1988

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

Full work available at URL: https://doi.org/10.1007/bf00758973

zbMATH Keywords

barotropic equation of statehypersurface-homogeneous spacetimesshear-free perfect fluidsUniform Thermal Histories

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (8)

Higher symmetries in a class of cosmological models ⋮ Homogeneous and hypersurface-homogeneous shear-free perfect fluids in general relativity ⋮ Type-N, shear-free, perfect-fluid spacetimes with a barotropic equation of state ⋮ Reviving the shear-free perfect fluid conjecture in general relativity ⋮ Shear-free perfect fluids in general relativity II. Aligned, Petrov type III space-times ⋮ Theorems on shear-free perfect fluids with their Newtonian analogues ⋮ Shear-free perfect fluids in general relativity: Gravito-magnetic spacetimes ⋮ Shear-free perfect fluids with a \(\gamma\)-law equation of state

Uses Software

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Cites Work

• Tilted homogeneous cosmological models
• Isotropic solutions of the Einstein-Boltzmann equations
• A class of shear-free perfect fluids in general relativity. I
• Shear-free perfect fluids with zero magnetic Weyl tensor
• Shear-free perfect fluids in general relativity. I. Petrov type N Weyl tensor

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