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Reconstruction of some cosmological models in f(R,T) cosmology

  • Regular Article - Theoretical Physics
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Abstract

In this paper, we reconstruct cosmological models in the framework of f(R,T) gravity, where R is the Ricci scalar and T is the trace of the stress-energy tensor. We show that the dust fluid reproduces ΛCDM, phantom–non-phantom era and phantom cosmology. Further, we reconstruct different cosmological models, including the Chaplygin gas, and scalar field with some specific forms of f(R,T). Our numerical simulation for the Hubble parameter shows good agreement with the BAO observational data for low redshifts, z<2.

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Authors and Affiliations

  1. Eurasian International Center for Theoretical Physics, Eurasian National University, Astana, 010008, Kazakhstan

    Mubasher Jamil, D. Momeni & Ratbay Myrzakulov

  2. Center for Advanced Mathematics and Physics, National University of Sciences and Technology, H-12, Islamabad, Pakistan

    Mubasher Jamil

  3. Department of Mathematics, COMSATS Institute of Information Technology (CIIT), Sahiwal campus, Pakistan

    Muhammad Raza

Authors
  1. Mubasher Jamil
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  2. D. Momeni
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  3. Muhammad Raza
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  4. Ratbay Myrzakulov
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Correspondence to Mubasher Jamil.

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Jamil, M., Momeni, D., Raza, M. et al. Reconstruction of some cosmological models in f(R,T) cosmology. Eur. Phys. J. C 72, 1999 (2012). https://doi.org/10.1140/epjc/s10052-012-1999-9

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  • DOI: https://doi.org/10.1140/epjc/s10052-012-1999-9

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