A dark energy model in a scalar tensor theory of gravitation

DOI10.1007/s10509-011-0852-1zbMath1270.83038OpenAlexW2000689888MaRDI QIDQ422182

D. Neelima, V. U. M. Rao, G. Sree Devi Kumari

Publication date: 16 May 2012

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

Full work available at URL: https://doi.org/10.1007/s10509-011-0852-1

zbMATH Keywords

scalar-tensor theorydark energy cosmological model

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (9)

A quantum space behind simple quantum mechanics ⋮ LRS Bianchi type-II universe with cosmic strings and bulk viscosity in a modified theory of gravity ⋮ Kaluza-Klein universe with cosmic strings and bulk viscosity in \(f(R,T)\) gravity ⋮ LRS Bianchi type-I dark energy cosmological model in Brans-Dicke theory of gravitation ⋮ Bianchi type-III dark energy model in \(f(R,T)\) gravity ⋮ Two fluid scenario for dark energy model in a scalar-tensor theory of gravitation ⋮ Non-existence of Bianchi type-III bulk viscous string cosmological model in \(f(R,T)\) gravity ⋮ A five dimensional Kaluza-Klein bulk viscous string cosmological model in Brans-Dicke scalar-tensor theory of gravitation ⋮ Bianchi type II, VIII \& IX cosmological model with magnetized anisotropic dark energy in Brans-Dicke theory of gravitation

Cites Work

• Bianchi type-I anisotropic dark energy model with constant deceleration parameter
• Inhomogeneous plane symmetric models in a scalar-tensor theory
• Mach's Principle and a Relativistic Theory of Gravitation
• Cosmological Imprint of an Energy Component with General Equation of State

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