A novel teleparallel dark energy model
arXiv:1402.2256 · doi:10.1142/S0218271816500255
Abstract
Although equivalent to general relativity, teleparallel gravity is conceptually speaking a completely different theory. In this theory, the gravitational field is described by torsion, not by curvature. By working in this context, a new model is proposed in which the four-derivative of a canonical scalar field representing dark energy is nonminimally coupled to the "vector torsion". This type of coupling is motivated by the fact that a scalar field couples to torsion through its four-derivative, which is consistent with local spacetime kinematics regulated by the de Sitter group . It is found that the current state of accelerated expansion of the Universe corresponds to a late-time attractor that can be (i) a dark-energy-dominated de Sitter solution (), (ii) a quintessence-type solution with , or (iii) a phantom-type dark energy.
15 pages, 2 figures, 3 tables
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Cited by in corpus (29)
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- Einstein-Cartan Cosmologies
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