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Cosmic dynamics in \({F(R,\phi)}\) gravity

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Abstract

In this paper we consider FRW cosmology in \({F(R,\phi)}\) gravity. It is shown that in particular cases the bouncing behavior may appears in the model whereas the equation of state (EoS) parameter may crosses the phantom divider. For the dynamical universe, quantitatively we also find parameters in the model which satisfies two independent tests:the model independent Cosmological Redshift Drift (CRD) test and the type Ia supernova luminosity distances.

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Authors and Affiliations

  1. Department of Physics, University of Guilan, Rasht, Iran

    H. Farajollahi, F. Milani & F. Tayebi

  2. Department of Science, Payam Noor University, Bijar, Iran

    M. Setare

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  1. H. Farajollahi
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  2. M. Setare
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  3. F. Milani
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  4. F. Tayebi
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Correspondence to H. Farajollahi.

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Farajollahi, H., Setare, M., Milani, F. et al. Cosmic dynamics in \({F(R,\phi)}\) gravity. Gen Relativ Gravit 43, 1657–1669 (2011). https://doi.org/10.1007/s10714-011-1148-z

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  • DOI: https://doi.org/10.1007/s10714-011-1148-z

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