A class of spherically symmetric solutions to Einstein s equations for a perfect fluid using non-comoving coordinates

DOI10.1088/0264-9381/20/9/316zbMath1030.83010OpenAlexW1973720347MaRDI QIDQ4409070

William Davidson

Publication date: 29 June 2003

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1088/0264-9381/20/9/316

zbMATH Keywords

expansionaccelerationshearRaychaudhuri equation

Mathematics Subject Classification ID

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)

On shearing fluids with homogeneous densities ⋮ A class of generalised Robinson-Trautman solutions in non-comoving coordinates

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