Variable deceleration parameter and dark energy models

DOI10.1142/S0219887816500559zbMath1339.83078MaRDI QIDQ2805578

Binaya K. Bishi

Publication date: 12 May 2016

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

zbMATH Keywords

dark energyvariable deceleration parameter\(f(R,T)\) modified gravity

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) Astrophysical cosmology (85A40)

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Cites Work

• LRS Bianchi type-II universe with cosmic strings and bulk viscosity in a scalar tensor theory of gravitation
• Bianchi type-III dark energy model in a Saez-Ballester scalar-tensor theory
• Bianchi type-III dark energy model in \(f(R,T)\) gravity
• Bianchi type-I universe with cosmological constant and quadratic equation of state in \(f(R, T)\) modified gravity
• The cosmological constant and dark energy
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

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