Ricci dark energy in Chern-Simons modified gravity
arXiv:1306.6638 · doi:10.1140/epjc/s10052-013-2500-0
Abstract
In this work, we have considered the Ricci dark energy model, where the energy density of the universe is proportional to the Ricci scalar curvature, in the dynamic Chern-Simons modified gravity. We show that in this context the evolution of the scale factor is similar to that displayed by the modified Chaplygin gas.
7 pages; to appear in EPJC
References in corpus (5)
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Cited by in corpus (10)
- Holographic Dark Energy Models and Higher Order Generalizations in Dynamical Chern-Simons Modified Gravity
- Ricci dark energy in bumblebee gravity model
- Comment on Ricci dark energy in Chern-Simons modified gravity
- A stable flat entropy-corrected FRW universe
- Ricci-Gauss-Bonnet holographic dark energy in Chern-Simons modified gravity: A flat FLRW quintessence-dominated universe
- Ricci Dark Energy of Amended FRW Universe in Chern-Simon Modified Gravity
- Cosmological Analysis of Modified Holographic Ricci Dark Energy in Chern-Simons Modified Gravity
- The Rényi holographic dark energy model in Chern-Simons gravity: some cosmological implications
- Note on Dark Energy and Cosmic Transit in a scale-invariance cosmology
- Some cosmological features of 4D Gauss-Bonnet gravity with varying cosmological constant