Abstract
In this paper, we have constructed the cosmological model of the universe in f(R, T) theory of gravity in a Bianchi type \(\mathrm{VI}_h\) universe for the functional f(R, T) in the form \(f(R,T)=\mu R+\mu T\), where R and T are respectively Ricci scalar and trace of energy momentum tensor and \(\mu \) is a constant. We have made use of the hyperbolic scale factor to find the physical parameters and metric potentials defined in the space-time. The physical parameters are constrained from different representative values to build up a realistic cosmological model aligned with the observational behaviour. The state finder diagnostic pair is found to be in the acceptable range. The energy conditions of the model are also studied.
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Acknowledgements
BM acknowledges the DST, New Delhi, India for providing facilities through DST-FIST lab, Department of Mathematics, where a part of this work was done. FME acknowledges the Department of Mathematics, BITS – Pilani, Hyderabad Campus, where a part of this work was done. The authors are thankful to the anonymous referees for their comments and suggestions for the improvement of the paper.
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Esmaeili, F.M., Mishra, B. Behaviour of physical parameters in extended gravity with hyperbolic function. J Astrophys Astron 39, 59 (2018). https://doi.org/10.1007/s12036-018-9553-2
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DOI: https://doi.org/10.1007/s12036-018-9553-2