Transit cosmological models in Myrzakulov F(R,T) gravity theory
arXiv:2401.00686 · doi:10.1140/epjc/s10052-024-12904-5
Abstract
In the present paper, we investigate some exact cosmological models in Myrzakulov gravity theory. We have considered the arbitrary function where is an arbitrary constant, are respectively, the Ricci-scalar curvature and the torsion. We have solved the field equations in a flat FLRW spacetime manifold for Hubble parameter and using the MCMC analysis, we have estimated the best fit values of model parameters with regions, for two observational datasets like and Pantheon SNe Ia datasets. Using these best fit values of model parameters, we have done the result analysis and discussion of the model. We have found a transit phase decelerating-accelerating universe model with transition redshifts . The effective dark energy equation of state varies as and the present age of the universe is found as Gyrs, respectively for two datasets.
22 pages, 11 figures
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- Exact Cosmology in Myrzakulov Gravity
- FLRW Cosmology in Metric-Affine Gravity
- Myrzakulov gravity: cosmological implications and constraints
- Myrzakulov Gravity in Vielbein Formalism: A Study in Weitzenböck Spacetime
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- Chaplygin and Polytropic gases Teleparallel Robertson-Walker gravity solutions