Newgravitational theories can be formulated using gauge theory with local Poincar´ e symmetry, which naturally leads to a spacetime with torsion. In this study, we explore a parametrization approach to the Hubble parameter within the framework of modified teleparallel Gauss-Bonnet gravity. This theory is based on the torsion invariant T and the teleparallel equivalent of the Gauss-Bonnet term TG, forming the F(T ,TG) gravity model. Notably, this modified gravity framework provides a unified explanation of cosmic evolution, encompassing early-time inflation and late time accelerated expansion, without requiring a cosmological constant. The results obtained from our analysis are consistent with recent cosmological observations, demonstrating a transition from a decelerating phase to an accelerating phase of cosmic expansion. By utilizing a combination of observational datasets, including Type Ia Supernovae(SNeIa), BaryonAcousticOscillations (BAO), Cosmic Microwave Background(CMB),andHubbleparameterH(z)measurements, wehaveconstrained the transition redshift zt, which marks the epoch when the universe shifts from deceleration to acceleration. Furthermore, we have determined the best-fit value of zt and compared the reconstructed evolution of the deceleration parameter q(z) and the equation of state parameter ω(z). The findings are in strong agreement with the standard ΛCDM model, reinforcing the validity of our approach.
Author
(s) Details
S. H.
Shekh
Department of Mathematics, S. P. M. Science and Gilani Arts,
Commerce College, Ghatanji, Dist. Yavatmal, Maharashtra 445301, India.
N.
Myrzakulov
Department of General and Theoretical Physics, L N Gumilyov
Eurasian National University, Astana 010008, Kazakhstan and Ratbay Myrzakulov
Eurasian International Centre for Theoretical Physics, Astana 010009,
Kazakhstan.
A.
Pradhan
Centre for Cosmology, Astrophysics and Space Science (CCASS), GLA
University, Mathura 281406, India.
A.
Mussatayeva
Department of General and Theoretical Physics, L N Gumilyov
Eurasian National University, Astana 010008, Kazakhstan and Department of
Physics and Chemistry, S. Seifullin Kazakh Agrotechnical University, Astana
010011, Kazakhstan.
A.
Bagde
Department of Mathematics, Late R. Bharti Arts, Commerce and Smt.
S. R. Bharti Science College, Arni, Dist. Yavatmal, Maharashtra 445301, India.
Please see the book here:- https://doi.org/10.9734/bpi/crpps/v8/4453
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