Accelerated expansion of the universe model with parametrization of $q(z)$ in $f(R,L_m)$ theory of gravity

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Main Authors: Patle, Khomesh R., Singh, G. P., Garg, Romanshu
Format: Preprint
Published: 2025
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author Patle, Khomesh R.
Singh, G. P.
Garg, Romanshu
author_facet Patle, Khomesh R.
Singh, G. P.
Garg, Romanshu
contents In this research work, we explore the late-time accelerated expansion of the universe within the framework of modified gravity, specifically $f(R, L_m)$ theory, by considering two non-linear models: $f(R, L_{m}) = \frac{R}{2}+(1+ηR) L_{m}$ and $f(R, L_{m}) = \frac{R}{2}+ L_{m}^η$, where $η$ is a free parameter. Adopting a parametric form of the deceleration parameter $q(z)$, we derive a quadratic expression for the normalized Hubble parameter. By use of Bayesian statistical analysis with the $χ^{2}$-minimization approach, we determine the median values of the model parameters for both the cosmic chronometer (CC) and the joint (CC+Pantheon) dataset. Furthermore, we examine the fundamental cosmological parameters: energy density, pressure, the equation of state (EoS) parameter and energy conditions. The cosmographic parameters are thoroughly analyzed and the present age of the universe is estimated based on this model.
format Preprint
id arxiv_https___arxiv_org_abs_2506_15789
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Accelerated expansion of the universe model with parametrization of $q(z)$ in $f(R,L_m)$ theory of gravity
Patle, Khomesh R.
Singh, G. P.
Garg, Romanshu
General Relativity and Quantum Cosmology
In this research work, we explore the late-time accelerated expansion of the universe within the framework of modified gravity, specifically $f(R, L_m)$ theory, by considering two non-linear models: $f(R, L_{m}) = \frac{R}{2}+(1+ηR) L_{m}$ and $f(R, L_{m}) = \frac{R}{2}+ L_{m}^η$, where $η$ is a free parameter. Adopting a parametric form of the deceleration parameter $q(z)$, we derive a quadratic expression for the normalized Hubble parameter. By use of Bayesian statistical analysis with the $χ^{2}$-minimization approach, we determine the median values of the model parameters for both the cosmic chronometer (CC) and the joint (CC+Pantheon) dataset. Furthermore, we examine the fundamental cosmological parameters: energy density, pressure, the equation of state (EoS) parameter and energy conditions. The cosmographic parameters are thoroughly analyzed and the present age of the universe is estimated based on this model.
title Accelerated expansion of the universe model with parametrization of $q(z)$ in $f(R,L_m)$ theory of gravity
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2506.15789