Friedmann Cosmology with Bulk Viscosity: A Concrete Model for Dark Energy

DOI10.1088/0253-6102/52/2/36zbMath1181.83242arXiv0812.4904OpenAlexW2007563773MaRDI QIDQ5852225

Xu Dou, Xin-he Meng

Publication date: 26 January 2010

Published in: Communications in Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0812.4904

zbMATH Keywords

bulk viscosityunification of dark matter and dark energydark energy cosmology

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (4)

Bianchi type-\(I\) bulk viscosity with a DE cosmological model ⋮ Viscous Ricci dark energy and generalized second law of thermodynamics in modified f(R, T) gravity ⋮ Two-fluid dark energy models in Bianchi type-III universe with variable deceleration parameter ⋮ Exact solutions of a causal viscous FRW cosmology within the Israel-Stewart theory through factorization

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