FRW Cosmology in F(R,T) gravity
arXiv:1207.1039 · doi:10.1140/epjc/s10052-012-2203-y
Abstract
In this paper, we consider a theory of gravity with a metric-dependent torsion namely the gravity, where is the curvature scalar and is the torsion scalar. We study a geometric root of such theory. In particular we give the derivation of the model from the geometrical point of view. Then we present the more general form of gravity with two arbitrary functions and give some of its particular cases. In particular, the usual and gravity theories are the particular cases of the gravity. In the cosmological context, we find that our new gravitational theory can describes the accelerated expansion of the universe.
14 pages
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- Thermodynamics of the viscous gravity in the new agegraphic dark energy model
- Estimation of Cosmological Parameters, Stability Analysis and Energy Conditions in Viable Modified Gravity
- Effective equation of state in modified gravity and observational constraints
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- Phantom energy supported wormhole model in gravity assuming conformal motion
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- Cosmologies in theory with non-minimal coupling between geometry and matter
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