Abstract
In this work we investigate the higher dimensional FRW model in the presence of a non-perfect fluid in case of \(R^pexp(\lambda R)\) gravity. We use the dynamical system approach to find the set of fixed points for the cosmological system. The analysis of the phase space of this model has been extended with the aim of finding the stability of the universe, particularly whether the anisotropy in the model isotropizes in the future and a late times the universe evolves towards accelerated expansion.
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References
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Banik, S.K., Banik, D.K., Bhuyan, K. (2018). Phase Portraits of Higher Dimensional FRW Cosmology in \(R^pexp(\lambda R)\) Gravity Filled with Non-perfect Fluid. In: Naimuddin, M. (eds) XXII DAE High Energy Physics Symposium . Springer Proceedings in Physics, vol 203. Springer, Cham. https://doi.org/10.1007/978-3-319-73171-1_76
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DOI: https://doi.org/10.1007/978-3-319-73171-1_76
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