Accelerating Universe scenario in anisotropic cosmology
arXiv:2208.13149 · doi:10.1016/j.cjph.2022.09.002
Abstract
In this paper, we investigate the exact solution of an anisotropic space-time in the context of gravity, where is the arbitrary function of the non-metricity scalar . Here, we consider a specific power-law form as , where , , and are free model parameters. Using power-law cosmology (), we analyze the physical behavior of cosmological parameters such as the energy density, pressure, EoS parameter, skewness parameter. Further, we validated the model with energy conditions and found that our \ cosmological model behaves like the quintessence model in the present and CDM in the future.
Minor revision in CJPHY. arXiv admin note: text overlap with arXiv:2208.08877
References in corpus (14)
- Large Scale Structure as a Probe of Gravitational Slip
- Energy Conditions in gravity
- Accelerated Expansion of the Universe in Non-minimally Coupled Gravity
- Cosmography in gravity
- Traversable wormhole geometries in gravity
- Anisotropic nature of space-time in gravity
- Anisotropic cosmological models in gravity with variable deceleration parameter
- Constraining gravity from energy conditions
- Cosmic acceleration and energy conditions in CDM symmetric teleparallel gravity
- Isotropization of locally rotationally symmetric Bianchi-I universe in -gravity
- Holographic dark energy in Gauss-Bonnet gravity with Granda-Oliveros cut-off
- Stability analysis of anisotropic Bianchi type-I cosmological model in teleparallel gravity
- Gravitational Waves from Preheating in Gauss-Bonnet Inflation
- Preheating and Reheating Constraints in Supersymmetric Braneworld Inflation
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