A Cosmological Study in Massive Gravity theory
arXiv:1505.00743 · doi:10.1016/j.aop.2015.04.003
Abstract
A detailed study of the various cosmological aspects in massive gravity theory has been presented in the present work. For the homogeneous and isotropic FLRW model, the deceleration parameter has been evaluated, and, it has been examined whether there is any transition from deceleration to acceleration in recent past, or not. With the proper choice of the free parameters, it has been shown that the massive gravity theory is equivalent to Einstein gravity with a modified Newtonian gravitational constant together with a negative cosmological constant. Also, in this context, it has been examined whether the emergent scenario is possible, or not, in massive gravity theory. Finally, we have done a cosmographic analysis in massive gravity theory.
21 Pages, 5 figures, Published version
References in corpus (18)
- Resummation of Massive Gravity
- Massive gravity: nonlinear instability of the homogeneous and isotropic universe
- Exact Schwarzschild-de Sitter black holes in a family of massive gravity models
- Emergent Universe with Exotic Matter
- Self-accelerating Massive Gravity: Exact solutions for any isotropic matter distribution
- Anisotropic Friedmann-Robertson-Walker universe from nonlinear massive gravity
- Charged black holes in nonlinear massive gravity
- Lorentz Breaking Massive Gravity in Curved Space
- Is Emergent Universe a Consequence of Particle Creation Process?
- Massive gravity from bimetric gravity
- The Einstein static universe with torsion and the sign problem of the cosmological constant
- Emergent Universe in Brane World Scenario with Schwarzschild-de Sitter Bulk
- A graceful entrance to braneworld inflation
- Cosmic acceleration with a negative cosmological constant in higher dimensions
- Null Energy Condition violations in bimetric gravity
- Cosmology and perturbations in massive gravity
- Phantom crossing and quintessence limit in extended nonlinear massive gravity
- Self-Protection of Massive Cosmological Gravitons