New cosmological solutions in massive gravity theory
arXiv:1510.05720
Abstract
In this paper we present some new cosmological solutions in massive gravity theory. Some homogeneous and isotropic solutions correctly describe accelerated evolutions for the universe. The study was realized considering a specific form to the fiducial metric and found different functions and constant parameters of the theory that guarantees the conservation of the energy momentum tensor. Several accelerating cosmologies were found, all of them reproducing a cosmological constant term proportional to the graviton mass, with a de Sitter type solution for the scale factor. We have also verified that when the fiducial metric is close to the physical metric the solutions are absent, except for some specific open cases.
17 pages, text revised
References in corpus (14)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Theoretical Aspects of Massive Gravity
- Resolving the Ghost Problem in non-Linear Massive Gravity
- Hubble parameter measurement constraints on the cosmological deceleration-acceleration transition redshift
- On Non-Linear Actions for Massive Gravity
- Ghosts in Massive Gravity
- Phases of massive gravity
- Anisotropic Friedmann-Robertson-Walker universe from nonlinear massive gravity
- New Cosmological Solutions in Massive Gravity
- Exact self-accelerating cosmologies in the ghost-free bigravity and massive gravity
- Exact self-accelerating cosmologies in the ghost-free massive gravity -- the detailed derivation
- New Kinetic Interactions for Massive Gravity?
- Classical and quantum massive cosmology for the open FRW universe