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Scalar Field Cosmology in f(R,T) Gravity with Λ

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Abstract

We study the behavior of cosmological parameters, massive and massless scalar fields (normal or phantom) with a scalar potential in f(R, T) theory of gravity for a flat Friedmann-Robertson-Walker (FRW) universe. To get exact solutions to the modified field equations, we use the f(R, T) = R + 2f(T) model by Harko et al. (T. Harko et al., Phys. Rev. D 84, 024020 (2011)), where R is the Ricci scalar and T is the trace of the energy momentum tensor. Our cosmological parameter solutions agree with the recent observational data. Finally, we discuss our results with various graphics.

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Authors and Affiliations

  1. Department of Physics, Зanakkale Onsekiz Mart University, Arts and Sciences Faculty, Terzioğlu Campus, Çanakkale, 17020, Turkey

    Sezgin Aygün

  2. Department of Mathematics, Зanakkale Onsekiz Mart University, Arts and Sciences Faculty, Terzioğlu Campus, Çanakkale, 17020, Turkey

    Can Aktaş

  3. Department of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad, 500078, India

    Pradyumn Kumar Sahoo

  4. Department of Mathematics, Lovely Professional University, Phagwara, Jalandhar, Panjab, 144401, India

    Binaya K. Bishi

Authors
  1. Sezgin Aygün
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  2. Can Aktaş
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  3. Pradyumn Kumar Sahoo
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  4. Binaya K. Bishi
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Correspondence to Sezgin Aygün.

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Aygün, S., Aktaş, C., Sahoo, P.K. et al. Scalar Field Cosmology in f(R,T) Gravity with Λ. Gravit. Cosmol. 24, 302–307 (2018). https://doi.org/10.1134/S0202289318030039

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  • DOI: https://doi.org/10.1134/S0202289318030039

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