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• W3103091523 endingPage "1650038" @default.
• W3103091523 startingPage "1650038" @default.
• W3103091523 abstract "We examine the evolution of universe in [Formula: see text] gravity where [Formula: see text] is the Ricci curvature and [Formula: see text] is the trace of energy–momentum tensor. We focus on the specific form [Formula: see text] and explicitly find out the relation between [Formula: see text] and state of equation [Formula: see text] by adiabatic condition. All possible modes of evolution of the scale factor for the five kinds of state of equation, [Formula: see text] are exhibited. We simulate numerically the plots of redshift versus distance modulus for three interesting modes and then obtain the good fitting curve compared with the astronomical observation data." @default.
• W3103091523 created "2020-11-23" @default.
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• W3103091523 date "2016-03-01" @default.
• W3103091523 modified "2023-10-13" @default.
• W3103091523 title "The cosmology in f(R,τ) gravity without dark energy" @default.
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• W3103091523 doi "https://doi.org/10.1142/s0218271816500383" @default.
• W3103091523 hasPublicationYear "2016" @default.
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