How a conformally flat (GR)4 impacts Gauss-Bonnet gravity?
arXiv:2107.02889 · doi:10.1002/prop.202100088
Abstract
First and foremost, we show that a 4-dimensional conformally flat generalized Ricci recurrent spacetime is an Einstein manifold. We examine such a spacetime as a solution of -gravity theory and it is shown that the additional terms from the modification of the gravitational sector can be expressed as a perfect fluid. Several energy conditions are investigated with and . For both the models, weak, null and dominant energy conditions are satisfied while strong energy condition is violated, which is a good agreement with the recent observational studies which reveals that the current universe is in accelerating phase.
arXiv comment10 pages, 6 figures: Revised version submitted to Fortschritte der Physik - Progress of Physics
References in corpus (20)
- Dynamics of dark energy
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- The Cosmology of Modified Gauss-Bonnet Gravity
- Energy conditions in f(R)-gravity
- Dark energy problem: from phantom theory to modified Gauss-Bonnet gravity
- Energy Conditions in gravity
- Energy conditions in gravity
- On the stability of the cosmological solutions in f(R,G) gravity
- Dynamics of Inflation and Dark Energy from Gravity
- Energy conditions in gravity
- Inevitable ghost and the degrees of freedom in f(R,G) gravity
- Cosmological perfect fluids in Gauss-Bonnet gravity
- Cosmological dynamics of fourth order gravity with a Gauss-Bonnet term
- A Conformally Flat Generalized Ricci Recurrent Spacetime in F(R)-Gravity
- Exact spherically symmetric solutions in modified Gauss-Bonnet gravity from Noether symmetry approach
- Topological Static Spherically Symmetric vacuum Solutions in Gravity
- Energy Bounds in Gravity with Anisotropic Background