Bianchi type-III stiff fluid cosmological model in general relativity

DOI10.1007/S10509-008-9954-9zbMath1172.83345OpenAlexW2042311418MaRDI QIDQ835531

Anita Bagora

Publication date: 28 August 2009

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-008-9954-9

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (5)

A dynamical system approach to Bianchi III cosmology for Hu-Sawicki type \(f(R)\) gravity ⋮ Some Bianchi type cosmological models in \(f(R)\) gravity ⋮ Effects of anisotropy on the sign-changeable interacting Tsallis holographic dark energy ⋮ Plane symmetric vacuum Bianchi type \(III\) cosmology in \(f(R)\) gravity ⋮ Thermodynamics of interacting new agegraphic dark energy and dark matter due to Bianchi type I model

Cites Work

• Inhomogeneous generalizations of Bianchi type-VI\(_ h\) universes with co-moving perfect fluid and radiation
• Topology and cosmology
• Spatially homogeneous and inhomogeneous cosmologies with equation of state p=mu
• Inhomogeneous generalizations of Bianchi type \(\text{VI}_ h\) universes with stiff perfect fluid and radiation
• Some Bianchi type III string cosmological models with bulk viscosity
• Tilted homogeneous cosmological models
• Plane symmetric self-gravitating fluids with pressure equal to energy density

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