Shear-free perfect fluids in general relativity. I. Petrov type N Weyl tensor
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Publication:3771928
DOI10.1063/1.527446zbMath0633.76132OpenAlexW2049410687MaRDI QIDQ3771928
Publication date: 1987
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1063/1.527446
vorticityEinstein equationsmetric propertiesWeyl conformal tensorshear-free perfect fluidmodel for cosmological mattersource stress-tensor
Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)
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Cites Work
- Characterization of locally rotationally symmetric space-times
- 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
- A class of shear-free perfect fluids in general relativity. II
- An Approach to Gravitational Radiation by a Method of Spin Coefficients
