Torsion gravity with non-minimally coupled fermionic field: some cosmological models
arXiv:1412.4674 · doi:10.1103/PhysRevD.91.043528
Abstract
We investigate some cosmological models arising from a non-minimal coupling of a fermionic field to gravity in the geometrical setting of Einstein-Cartan-Sciama-Kibble gravity. The role played by the non-minimal coupling together with torsion in facing problems such as cosmological singularity, inflation and dark energy is discussed.
15 pages, no figures, updated and extended version
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Cited by in corpus (5)
- Extended Gravity Cosmography
- The commutator algebra of covariant derivative as general framework for extended gravity. The Rastall theory case and the role of the torsion
- Different types of torsion and their effect on the dynamics of fields
- Spinor fields in -gravity
- Corrections to Higgs width decay into a fermion pair from gravitational torsion