Abstract
In this paper, we reconstruct a suitable model in \(f(R,T)\) gravity, (where \(R\) is the Ricci scalar and \(T\) is the trace of the energy momentum tensor) which depict the current cosmic picture in more consistent way. The dynamical field equations are solved for generic anisotropic space-time. The solution of field equations helps us to determine the future cosmic evolution for both physical and kinematical quantities. We explore the nature of deceleration parameter, NEC and energy density for three different cases representing Bianchi type I, III and Kantowski-Sachs universe model. We find that this study favors the phantom cosmic evolution in all cases.
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Zubair, M., Ali Hassan, S.M. Dynamics of Bianchi type I, III and Kantowski-Sachs solutions in \(f(R,T)\) gravity. Astrophys Space Sci 361, 149 (2016). https://doi.org/10.1007/s10509-016-2737-9
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DOI: https://doi.org/10.1007/s10509-016-2737-9