gravity and cosmology
arXiv:1405.0519 · doi:10.1088/1475-7516/2014/12/021
Abstract
We present an extension of gravity, allowing for a general coupling of the torsion scalar with the trace of the matter energy-momentum tensor . The resulting theory is a new modified gravity, since it is different from all the existing torsion or curvature based constructions. Applied to a cosmological framework, it leads to interesting phenomenology. In particular, one can obtain a unified description of the initial inflationary phase, the subsequent non-accelerating, matter-dominated expansion, and then the transition to a late-time accelerating phase. Additionally, the effective dark energy sector can be quintessence or phantom-like, or exhibit the phantom-divide crossing during the evolution. Moreover, in the far future the universe results either to a de Sitter exponential expansion, or to eternal power-law accelerated expansions. Finally, a detailed study of the scalar perturbations at the linear level reveals that cosmology can be free of ghosts and instabilities for a wide class of ansatzes and model parameters.
31 pages, 15 figures; matches published version
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Cited by in corpus (20)
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- gravity models with observational constraints
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- gravitational baryogenesis
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