Cosmological Dark Matter Amplification through Dark Torsion
arXiv:2004.06058 · doi:10.1088/1361-6382/abb2d2
Abstract
A cosmological approach based on considering a cosmic background with non-zero torsion is shown in order to give an option of explaining a possible phantom evolution, not ruled out according to the current observational data. We revise some aspects of the formal schemes on torsion and, according them, we develop a formalism which can be an interesting alternative for exploring Cosmology.
10 pages
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