The effect of thermal radiation on singularities in the dark universe

DOI10.1142/S0219887821501139arXiv2103.08430OpenAlexW3137114311MaRDI QIDQ6125310

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Publication date: 11 April 2024

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2103.08430

zbMATH Keywords

singularityviscositythermal radiationdark fluid

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Cites Work

• Viscous inflationary universe models
• The null energy condition and cosmology
• \(f(R)\) gravity constrained by PPN parameters and stochastic background of gravitational waves
• Quantum de Sitter cosmology and phantom matter
• Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
• Dark energy and viscous cosmology
• Viscous brane cosmology with a brane-bulk energy interchange term
• Inflationary universe in terms of a van der Waals viscous fluid
• From a bounce to the dark energy era with F(R) gravity
• Viscous cosmology for early- and late-time universe

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