Analyzing the geometrical and dynamical parameters of modified Teleparallel-Gauss-Bonnet model

Abstract

To recreate the cosmological models, we employed the parametrization approach in modified teleparallel Gauss-Bonnet gravity. It has been interesting to apply the parametrization approach to investigate cosmological models. The real benefit of using this method is that the observational data may be incorporated to examine the cosmological models. Several cosmological parameters were examined, such as the Hubble parameter (H), the deceleration parameter (q), and the equation of state (EoS) parameter (w). The results obtained are consistent with recent cosmological findings in the conventional scenario. A transition scenario from a decelerating stage to an accelerating stage of cosmic evolution has been observed. The EoS parameter is also in the quintessence phase, which drives the accelerating expansion of the Universe. Also, we look at the violation of strong energy condition, which has become inevitable in the context of modified gravitational theory. Finally, we have performed the Om(z) diagnostic and also obtained the age of the Universe by using the data from the cosmological observations.

13 pages, 9 figures

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• Observational Constraints and Cosmographic Analysis of $f(T,T_G)$ Gravity and Cosmology
• Tracing cosmic evolution through Weyl-Type f(Q,T) gravity model: theoretical analysis and observational validation
• Noether Symmetries in $f(T,T_G)$ Cosmology
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• Generalized Ghost Pilgrim Dark Energy Fractal Cosmology with Observational Constraint
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• Growth factor in teleparallel Gauss-Bonnet gravity
• Late-Time Cosmic Acceleration in Ricci-Gauss-Bonnet Gravity via Gradient Descent Optimization