Accelerating Kantowski-Sachs Universe in (, )Gravity

AbstractThe present investigation deals with the (, ) gravity, which was recently attracted attention of many cosmologists. In thistheory, the gravitational action is formulated using an arbitrary function (, ) where represents the non-metricity scalarand denotes the trace of the energy-momentum tensor. In this paper, we have investigated Kantowski-Sachs cosmologicalmodels in the context of (, )gravity under the influence of wet dark fluid. A functional form (, ) = +, where andare constants, is chosen for derivation. We analyze three different models and obtained the exact solution of thefield equations by considering i) special form of deceleration parameter = −1 + ii) hyperbolic scale factor () = sinh() iii) the scale factor () = which generates a time-dependent deceleration parameter. We also studied some physical and kinematical parameters of the investigated models and discussed their behavior graphically.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-06-12
DOI
https://doi.org/10.5281/zenodo.20657044
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
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article

Accelerating Kantowski-Sachs Universe in (, )Gravity

M.T. Sarode, V.G. Mete, A. S. Nimkar
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
article

Accelerating Kantowski-Sachs Universe in (, )Gravity

M.T. Sarode, V.G. Mete, A. S. Nimkar
article en

Abstract

AbstractThe present investigation deals with the (, ) gravity, which was recently attracted attention of many cosmologists. In thistheory, the gravitational action is formulated using an arbitrary function (, ) where represents the non-metricity scalarand denotes the trace of the energy-momentum tensor. In this paper, we have investigated Kantowski-Sachs cosmologicalmodels in the context of (, )gravity under the influence of wet dark fluid. A functional form (, ) = +, where andare constants, is chosen for derivation. We analyze three different models and obtained the exact solution of thefield equations by considering i) special form of deceleration parameter = −1 + ii) hyperbolic scale factor () = sinh() iii) the scale factor () = which generates a time-dependent deceleration parameter. We also studied some physical and kinematical parameters of the investigated models and discussed their behavior graphically.

Zenodo (CERN European Organization for Nuclear Research)
G.S. Science, Arts And Commerce College (IN)
Openalex Percentile: Top 6%
Cosmology and Gravitation Theories
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