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Anisotropic dark energy universe in f(Q, T) gravity with observational constraints.
- Source :
-
Canadian Journal of Physics . 2024, Vol. 102 Issue 2, p85-95. 11p. - Publication Year :
- 2024
-
Abstract
- Aim of this paper is to investigate an anisotropic locally rotationally symmetric (LRS) Bianchi type-I space–time in the context of the recently proposed f(Q, T) gravity, where Q is the non-metricity scalar and T is energy–momentum tensor. We have considered f(Q, T) = αQ + βT a linear form, where α and β are model parameters. We have analyzed the exact solution of LRS Bianchi type-I space–time by assuming relation between metric potential A = Bn, where n is arbitrary non-zero real number. To study the anisotropic nature of the dynamical dark energy, we assume that the skewness parameters are time dependent and n ≠ 1. We have constrained to our model by using observational Hubble dataset. Onwards, discussed the physical behavior of cosmological parameters such as energy density, pressure, EoS parameter, deceleration parameter and, Energy conditions. [ABSTRACT FROM AUTHOR]
- Subjects :
- *DARK energy
*GRAVITY
*REAL numbers
*ENERGY density
*SPACETIME
UNIVERSE
Subjects
Details
- Language :
- English
- ISSN :
- 00084204
- Volume :
- 102
- Issue :
- 2
- Database :
- Academic Search Index
- Journal :
- Canadian Journal of Physics
- Publication Type :
- Academic Journal
- Accession number :
- 175192271
- Full Text :
- https://doi.org/10.1139/cjp-2023-0127