Some cosmological features of 4D Gauss-Bonnet gravity with varying cosmological constant
arXiv:2205.01096 · doi:10.1142/S0219887823500536
Abstract
We explore some cosmological features of the newly suggested 4D Gauss-Bonnet gravity through two different models assuming a varying cosmological constant. Observational constraints, such as the cosmic transit and the flat curvature, have been considered in constructing the models. The cosmology in the current work has been probed using a given scale factor derived from the desired cosmic behavior which is the inverse of the usual viewpoint. The stability and cosmography have been studied for the two models.
References in corpus (15)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- f(R,T) gravity
- Dark torsion as the cosmic speed-up
- Modified teleparallel gravity: inflation without inflaton
- Modified f(R) gravity consistent with realistic cosmology: from matter dominated epoch to dark energy universe
- Extended Gravity Cosmography
- Energy conditions in the epoch of galaxy formation
- From inflation to dark energy in the non-minimal modified gravity
- Dynamical vacuum energy in the expanding Universe confronted with observations: a dedicated study
- Vacuum models with a linear and a quadratic term in H: structure formation and number counts analysis
- Exact solutions, finite time singularities and non-singular universe models from a variety of cosmologies
- 4D Gauss-Bonnet gravity: cosmological constraints, tension and large scale structure
- Gaugino condensation in an improved heterotic M-theory
- Cosmological determination to the values of the prefactors in the logarithmic corrected entropy-area relation