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We study some aspects of cosmological evolution in a universe described by a viable curvature corrected exponential $F(R)$ gravity model, in the presence of matter fluids consisting of collisional matter and radiation.
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A. de la Cruz-Dombriz, A. Dobado, A. L. Maroto, Phys.Rev.D77 (2008) 123515 [arXiv:0802.2999]
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A. Silvestri, M. Trodden, Rept. Prog. Phys. 72 (2009) 096901 [arXiv:0904.0024]
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K. Kleidis, N. K. Spyrou, Astron.Astrophys. 529 (2011) A26
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R. Myrzakulov, L. Sebastiani, S. Zerbini, Int.J.Mod.Phys. D22 (2013) 1330017 [arXiv:1302.4646]
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Md. Wali Hossain, R. Myrzakulov, M. Sami, E. N. Saridakis, Phys.Rev. D89 (2014) 123513
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