Cosmological implications of f(R,Σ,T) gravity: A unified approach using OHD and SN ia data
Myrzakulov N. Shekh S.H. Pradhan A.
March 2025Elsevier B.V.
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
2025#862
This paper investigates the cosmological implications of the modified gravity framework known as f(R,Σ,T) gravity, focusing on its potential to unify and extend current cosmological models. The theory, introduced by Bakry and Ibraheem in 2023, combines the Ricci scalar, a scalar parameter representing torsion or other geometric properties, and the trace of the energy-momentum tensor. By analyzing observational Hubble data (OHD) and the Pantheon compilation of Type Ia Supernovae (SN Ia), we explore how this framework provides the accelerated expansion of the universe, the nature of dark energy, and phenomena like the Big Rip singularity. Employing the Friedmann-Robertson-Walker (FRW) metric and solving the modified field equations, we derive key cosmological parameters such as the Hubble constant and matter energy density parameter. These parameters are constrained through statistical analysis of observational data, yielding and from OHD, and from SN Ia. The evolution of the equation of state (EoS) parameter, isotropic pressure, and energy density is also investigated. By considering energy conditions and stability criteria, the study highlights the viability of gravity as an alternative framework to General Relativity and models. Our findings affirm the models compatibility with current observational evidence and its potential to the universes past and future dynamics.
Cosmology , H(z) parameterization , Modified gravity , Perfect fluid
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L N Gumilyov Eurasian National University, Astana, 010008, Kazakhstan
Department of Mathematics, S.P.M. Science and Gilani Arts, Commerce College, Yavatmal, Maharashtra, Ghatanji, 445301, India
Centre for Cosmology, Astrophysics and Space Science (CCASS) GLA University, Uttar Pradesh, Mathura, 281406, India
L N Gumilyov Eurasian National University
Department of Mathematics
Centre for Cosmology
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