TIME VARIABLE COSMOLOGICAL CONSTANT OF HOLOGRAPHIC ORIGIN WITH INTERACTION IN BRANS–DICKE THEORY
DOI10.1142/S0218271812500058zbMath1263.83136arXiv1203.4906OpenAlexW3105452253MaRDI QIDQ4914226
Li-Na Ma, Mo-Lin Liu, Ya-Bo Wu, Jian-Bo Lu
Publication date: 18 April 2013
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1203.4906
Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) 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 (2)
Cites Work
- A dark energy model characterized by the age of the Universe
- Combined constraints on modified Chaplygin gas model from cosmological observed data: Markov chain Monte Carlo approach
- The holographic dark energy in non-flat Brans-Dicke cosmology
- Generalized holographic and Ricci dark energy models
- Holographic dark energy in a cyclic universe
- Inflation with holographic dark energy
- CONSTRAINT ON THE KINEMATICAL AND DYNAMICAL MODEL FROM THE LATEST OBSERVATIONAL DATA
- Mach's Principle and a Relativistic Theory of Gravitation
- Reconstructing the interaction between dark matter and holographic dark energy
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Probable Values of the Cosmological Constant in a Holographic Theory
- Holographic dark energy in Brans-Dicke theory
- The confrontation between general relativity and experiment
This page was built for publication: TIME VARIABLE COSMOLOGICAL CONSTANT OF HOLOGRAPHIC ORIGIN WITH INTERACTION IN BRANS–DICKE THEORY
