Generation of Bianchi type V universes filled with a perfect fluid
From MaRDI portal
Publication:5935650
DOI10.1023/A:1002796730405zbMath0971.76106OpenAlexW1652288691MaRDI QIDQ5935650
U. Camci, Ismail Tarhan, Ihsan Onur Yilmaz, Hüsnü Baysal, Ilhami Yavuz
Publication date: 14 August 2001
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1023/a:1002796730405
Relativistic cosmology (83F05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (9)
Bianchi type V cosmological models with varying cosmological term ⋮ Dark energy models with variable equation of state parameter ⋮ Stiff domain walls in creation-field cosmology ⋮ Bianchi type-V cosmological model with purely magnetic solution ⋮ Bianchi type I universe with constant deceleration parameter in creation-field cosmology ⋮ Some exact Bianchi type-V perfect fluid cosmological models with heat flow and decaying vacuum energy density \(\Lambda \): expressions for some observable quantities ⋮ Transit dark energy string cosmological models with perfect fluid in F(R,T)-gravity ⋮ Generalized Chaplygin gas dominated anisotropic Bianchi type-I cosmological models ⋮ Bianchi type-I string cosmological model in creation-field
This page was built for publication: Generation of Bianchi type V universes filled with a perfect fluid