FLRW Cosmological Model with Quadratic Functional Form in f(R, T) Theory of Gravity
Abstract
This work investigates a spatially homogeneous and isotropic flat Friedmann-Lemaître-Robertson-Walker (FLRW) universe within the context of f(R, T) gravity as introduced by Harko et al., [Phys. Rev. D, 84, 024020 (2011)]. The present work deals with the functional form f(R, T) = f1(R) + f2(T) with f1(R) = R + λ1R2 and f2(T) = 2λ2T where λ1 and λ2 are arbitrary constants, R and T being the Ricci scalar and the trace of the stress-energy tensor Tij respectively. We present a novel cosmological model in the framework of f(R, T) gravity, exploring the dynamics of the FLRW universe through an exact solution to the gravitational field equations. By employing an innovative ansatz for the Hubble parameter, H = α (1 + 1/t) where α is a positive constant, we capture a evolutionary history of the universe. This approach provides a natural pathway to investigate key cosmological parameters, such as the scale factor, deceleration parameter, jerk, snap, lerk parameters and energy conditions, revealing intriguing insights into the universe’s expansion dynamics. We also discuss the statefinder diagnostic. Our results offer a deeper understanding of cosmic evolution within the f(R, T) gravity framework.
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References
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