Early cosmological models with bulk viscosity in Brans-Dicke theory

DOI10.1023/A:1000704023085zbMath0903.53069OpenAlexW106666213MaRDI QIDQ1270724

C. P. Singh, Shri Ram

Publication date: 3 November 1998

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

Full work available at URL: https://doi.org/10.1023/a:1000704023085

zbMATH Keywords

Brans-Dicke theoryevolution of Friedmann models with zero curvaturephysical properties of cosmological solutionstime dependent bulk viscosity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of differential geometry to physics (53Z05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (5)

FRW models with particle creation in Brans-Dicke theory ⋮ Bulk viscous Bianchi type I barotropic fluid cosmological model with varying \(\Lambda \) and functional relation on Hubble parameter ⋮ A Bianchi type-II dark-energy cosmology with a decaying \(\Lambda\)-term in the Brans-Dicke theory of gravity ⋮ Some Bianchi type-II cosmological models in Brans-Dicke theory ⋮ Early viscous universe with variable cosmological and gravitational constants in higher dimensional space time

This page was built for publication: Early cosmological models with bulk viscosity in Brans-Dicke theory