The role of shear in expanding \(G_ 2\) orthogonal perfect fluid models

DOI10.1023/A:1010235910986zbMath0878.53062OpenAlexW200338979MaRDI QIDQ1364926

Naresh Dadhich, L. K. Patel

Publication date: 4 January 1998

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

Full work available at URL: https://doi.org/10.1023/a:1010235910986

zbMATH Keywords

shearnonsingular expanding models

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (2)

Integrability conditions of quasi-Newtonian cosmologies in modified gravity ⋮ A comment on a paper by Dadhich and Patel

Cites Work

• Unnamed Item
• Relativistic Cosmology. I
• New and inhomogeneous cosmological models from the generalized Kerr--Schild transformation
• New class of inhomogeneous cosmological perfect-fluid solutions without big-bang singularity
• New non-separable diagonal cosmologies

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