Cosmological evolution of non-interacting and interacting holographic dark energy model in Brans–Dicke theory
DOI10.1142/S0219887818501244zbMath1390.83479OpenAlexW2795275191WikidataQ125809646 ScholiaQ125809646MaRDI QIDQ4643919
Publication date: 29 May 2018
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0219887818501244
Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Gravitational energy and conservation laws; groups of motions (83C40) Exact solutions to problems in general relativity and gravitational theory (83C15) Equations of motion in general relativity and gravitational theory (83C10)
Related Items (2)
Cites Work
- FRW models with particle creation in Brans-Dicke theory
- Holographic dark energy in Brans-Dicke theory with logarithmic form of scalar field
- The holographic dark energy in non-flat Brans-Dicke cosmology
- Mach's Principle and a Relativistic Theory of Gravitation
- DYNAMICS OF DARK ENERGY
- FRIEDMANN EQUATION FOR BRANS–DICKE COSMOLOGY
- COSMIC CONSTRAINTS ON HOLOGRAPHIC DARK ENERGY IN BRANS–DICKE THEORY VIA MARKOV-CHAIN MONTE-CARLO METHOD
- CURVATURE QUINTESSENCE
- The world as a hologram
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- The cosmological constant problem
- CAN BRANS–DICKE SCALAR FIELD ACCOUNT FOR DARK ENERGY AND DARK MATTER?
- New Agegraphic Dark Energy in Brans–Dicke Theory
- Holographic dark energy in Brans-Dicke theory
- Holographic dark energy in Brans-Dicke theory
- The cosmological constant
- An alternative to quintessence
- Interacting quintessence
- The confrontation between general relativity and experiment
This page was built for publication: Cosmological evolution of non-interacting and interacting holographic dark energy model in Brans–Dicke theory