Exact Cosmology in Myrzakulov Gravity
arXiv:2402.02123 · doi:10.1140/epjc/s10052-024-12983-4
Abstract
In this paper, we have investigated some exact cosmological models in Myrzakulov gravity using a flat Friedmann-Lematre-Robertson-Walker (FLRW) spacetime metric. We have considered the modified Lagrangian function as , where are respectively the Ricci curvature scalar and the torsion scalar with respect to non-special connection, and is a model parameter. We have obtained two exact solutions in two different situations for the scale factor . Using this scale factor, we have obtained various geometrical parameters to investigate cosmological properties of the universe. We have obtained the best fit values of model parameters through the MCMC analysis of two types latest observational datasets like and Pantheon SNe Ia samples, with \& regions. We have performed a comparative and relativistic study of geometrical and cosmological parameters. In model-I, we have found that the effective equation of state (EoS) parameter varies in the range while in the model-II, it varies as . We have found that both models are transit phase (decelerating to accelerating) universe with transition redshift in the range and present age of the universe Gyrs.
25 pages, 34 figures
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- Metric-Affine Myrzakulov Gravity Theories: Models, Applications and Theoretical Developments
- Constrained transit cosmological models in -gravity
- Einstein-Gauss-Bonnet-Myrzakulov Gravity from : Numerical Insights and Torsion-Gauss-Bonnet Dynamics in Weitzenböck Spacetime
- Electromagnetic Sources Teleparallel Robertson--Walker -Gravity Solutions
- Chaplygin and Polytropic gases Teleparallel Robertson-Walker gravity solutions