Shear-free perfect fluids in general relativity II. Aligned, Petrov type III space-times

DOI10.1063/1.528849zbMath0850.76905OpenAlexW2085814367WikidataQ125879066 ScholiaQ125879066MaRDI QIDQ4713341

John Carminati

Publication date: 25 June 1992

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

Full work available at URL: https://doi.org/10.1063/1.528849

Mathematics Subject Classification ID

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

Related Items (6)

Algebraic invariants of the Riemann tensor in a four-dimensional Lorentzian space ⋮ Reviving the shear-free perfect fluid conjecture in general relativity ⋮ Investigations of \(f(R)\)-gravity counterparts of the general relativistic shear-free conjecture by illustrative examples ⋮ 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

Cites Work

• Observationally homogeneous shear-free perfect fluids
• A Petrov type-III perfect fluid solution of Einstein's equations
• 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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