Extended holographic Ricci dark energy in chameleon Brans-Dicke cosmology
From MaRDI portal
Publication:2396944
DOI10.1155/2013/414615zbMath1362.83026arXiv1305.5159OpenAlexW2094791352WikidataQ58995608 ScholiaQ58995608MaRDI QIDQ2396944
Publication date: 29 May 2017
Published in: ISRN High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1305.5159
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) Astrophysical cosmology (85A40)
Related Items
Cites Work
- Dynamics of the self-interacting chameleon cosmology
- Holographic dark energy in chameleon tachyon cosmology
- Power-law entropy corrected holographic dark energy model
- Cosmic acceleration in Brans-Dicke cosmology
- The holographic dark energy in non-flat Brans-Dicke cosmology
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Dark energy and gravity
- CHAMELEON COSMOLOGY MODEL DESCRIBING THE PHANTOM DIVIDE LINE CROSSING
- The cosmological constant and dark energy
- The holographic principle
- Mach's Principle and a Relativistic Theory of Gravitation
- Exact solutions of Brans–Dicke cosmology with decaying vacuum density
- DYNAMICS OF DARK ENERGY
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- ΛCDM epoch reconstruction from F ( R , G ) and modified Gauss–Bonnet gravities
- CURVATURE QUINTESSENCE
- THEORETICAL MODELS OF DARK ENERGY
- Statefinder Diagnosis for the Extended Holographic Ricci Dark Energy Model without and with Interaction
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- SELF INTERACTING BRANS–DICKE COSMOLOGY AND QUINTESSENCE
