Perturbations of a class of locally rotationally symmetric cosmologies with applications to dissipative fluids

DOI10.1088/1361-6382/ac9bc7OpenAlexW4306825246MaRDI QIDQ5045978

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Publication date: 8 November 2022

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

Full work available at URL: https://doi.org/10.1088/1361-6382/ac9bc7

zbMATH Keywords

perturbation theorycosmologydissipative fluids

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Cites Work

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• Invariant construction of solutions to Einstein's field equations - LRS perfect fluids II
• The covariant approach to LRS perfect fluid spacetime geometries
• Tensor perturbations in anisotropically curved cosmologies
• Second-order perturbation theory: a covariant approach involving a barotropic equation of state
• Relativistic Cosmology
• 1+1+2 gravitational perturbations on LRS class II spacetimes: decoupling gravito-electromagnetic tensor harmonic amplitudes
• The Thermodynamics of Irreversible Processes. III. Relativistic Theory of the Simple Fluid

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