Cosmology of Holographic and New Agegraphic Models
arXiv:1310.1067 · doi:10.7566/JPSJ.82.064001
Abstract
We consider the theory, where is the scalar curvature and is the trace of energy-momentum tensor, as an effective description for the holographic and new agegraphic dark energy and reconstruct the corresponding functions. In this study, we concentrate on two particular models of gravity namely, and . We conclude that the derived models can represent phantom or quintessence regimes of the universe which are compatible with the current observational data. In addition, the conditions to preserve the generalized second law of thermodynamics are established.
27 pages, 12 figures
References in corpus (10)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- f(R,T) gravity
- Modified teleparallel gravity: inflation without inflaton
- A New Model of Agegraphic Dark Energy
- Thermodynamics in gravity with phantom crossing
- Quintessence reconstruction of the new agegraphic dark energy model
- Generalized second law in modified theory of gravity
- Reconstructing f(R) modified gravity from ordinary and entropy-corrected versions of the holographic and new agegraphic dark energy models
- Reconstructing f(R) theory according to holographic dark energy
- Reconstructing Theory from Ricci Dark Energy
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