Interacting $F(R,T)$ gravity with modified Chaplygin gas
Ali R. Amani, S. L. Dehneshin

TL;DR
This paper explores a cosmological model combining $F(R,T)$ gravity with modified Chaplygin gas, analyzing its implications for universe expansion, stability, and scalar field reconstruction in a unified framework.
Contribution
It introduces a novel interacting model of $F(R,T)$ gravity with Chaplygin gas, including scalar field reconstruction and stability analysis in a unified cosmological setting.
Findings
The universe exhibits accelerated expansion in the model.
The model remains stable at late times based on sound speed analysis.
Cosmological parameters align with observational data across different epochs.
Abstract
In this paper, we have studied gravity as an arbitrary function of curvature and torsion scalars in Friedmann--Lema\^{\i}tre--Robertson--Walker (FLRW) background. Then, we have considered interacting model between gravity and modified Chaplygin gas. The novelty of this model is that the Universe includes both cases curvature and torsion, and one dominated by a Chaplygin gas. In order to calculate cosmological solutions, we obtained Friedmann equations and also equation of state (EoS) parameter of dark energy. By employing interacting model we considered the total energy density and the total pressure of Universe as the combination of components of dark energy and Chaplygin gas. Subsequently, we reconstructed the model by an origin of a scalar field entitled quintessence model with a field potential. The field potential has been calculated in terms of free parameters of…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Geophysics and Gravity Measurements
