Early universe in scalar-tensor theory

DOI10.1007/S10773-008-9668-3zbMath1161.83473OpenAlexW2007347975MaRDI QIDQ1008143

C. P. Singh, Aroonkumar Beesham

Publication date: 24 March 2009

Published in: International Journal of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10773-008-9668-3

zbMATH Keywords

cosmologyinflationary phaseradiation-dominated phaseRobertson-Walker models

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Cites Work

• Unnamed Item
• Unified description of the early universe
• Cosmological models with variable cosmological and gravitational ``constants and bulk viscous models
• A spatially-flat cosmological model
• Solutions to the field equations and the deceleration parameter
• Cosmological models with variable gravitational and cosmological ``constants
• Early universe with variable gravitational and cosmological constants
• EARLY HOMOGENEOUS UNIVERSE WITH VARIABLE COSMOLOGICAL CONSTANT: KINEMATICS TESTS
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• The cosmological constant problem
• UNIFIED DESCRIPTION OF EARLY UNIVERSE WITH VARIABLE GRAVITATIONAL AND COSMOLOGICAL "CONSTANTS"
• A new basis for cosmology

This page was built for publication: Early universe in scalar-tensor theory