$f(R, T)$ Gravity Bouncing Universe with Cosmological Parameters

Fuente: arXiv
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Autori principali: Malik, Adnan, Naz, Tayyaba, Rauf, Aimen, Shamir, M. Farasat, Yousaf, Z.
Natura: Preprint
Pubblicazione: 2024
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author Malik, Adnan
Naz, Tayyaba
Rauf, Aimen
Shamir, M. Farasat
Yousaf, Z.
author_facet Malik, Adnan
Naz, Tayyaba
Rauf, Aimen
Shamir, M. Farasat
Yousaf, Z.
contents The basic aim of this manuscript is to investigate the cosmological solutions in the context of the modified $f(R, T)$ theory of gravity, where $R$ is the Ricci scalar and $T$ is the trace of the energy-momentum tensor. For our current work, we consider the Friedmann-Robertson-Walker space-time for finding the solutions of field equations. We investigate the nature of universe by considering acceleration expansion of universe, ultra relativistic universe, sub-relativistic universe, dust universe, radiation universe, stiff universe. Moreover, we apply the power law technique by taking two different $f(R, T)$ gravity models to observe the expanding nature of the universe. The bouncing scenario is also discussed by choosing some particular values of the model parameters and observed the energy conditions, which are satisfied for a successful bouncing model. It is also concluded that some solutions in $f(R, T)$ theory of gravity supports the concept of exotic matter and accelerated expansion of the universe due to a large amount of negative pressure.
format Preprint
id arxiv_https___arxiv_org_abs_2403_15847
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle $f(R, T)$ Gravity Bouncing Universe with Cosmological Parameters
Malik, Adnan
Naz, Tayyaba
Rauf, Aimen
Shamir, M. Farasat
Yousaf, Z.
General Relativity and Quantum Cosmology
The basic aim of this manuscript is to investigate the cosmological solutions in the context of the modified $f(R, T)$ theory of gravity, where $R$ is the Ricci scalar and $T$ is the trace of the energy-momentum tensor. For our current work, we consider the Friedmann-Robertson-Walker space-time for finding the solutions of field equations. We investigate the nature of universe by considering acceleration expansion of universe, ultra relativistic universe, sub-relativistic universe, dust universe, radiation universe, stiff universe. Moreover, we apply the power law technique by taking two different $f(R, T)$ gravity models to observe the expanding nature of the universe. The bouncing scenario is also discussed by choosing some particular values of the model parameters and observed the energy conditions, which are satisfied for a successful bouncing model. It is also concluded that some solutions in $f(R, T)$ theory of gravity supports the concept of exotic matter and accelerated expansion of the universe due to a large amount of negative pressure.
title $f(R, T)$ Gravity Bouncing Universe with Cosmological Parameters
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2403.15847