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

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dc.contributor.author Jamil, M.,
dc.contributor.author Momeni, D.,
dc.contributor.author Raza, M.,
dc.contributor.author Myrzakulov, R.
dc.date.accessioned 2012-07-02T11:10:58Z
dc.date.available 2012-07-02T11:10:58Z
dc.date.issued 2012-07-02
dc.identifier.uri http://dspace.enu.kz/handle/data/1461
dc.description.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–nonphantom 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. en_US
dc.language.iso en en_US
dc.subject 2,805 en_US
dc.title Reconstruction of some cosmological models in f(R,T) cosmology en_US

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