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• W2036707580 abstract "The Einstein-Cartan-Sciama-Kibble theory of gravity removes the constraint of general relativity that the affine connection be symmetric by regarding its antisymmetric part, the torsion tensor, as a dynamical variable. The minimal coupling between the torsion tensor and Dirac spinors generates a spin-spin interaction which is significant in fermionic matter at extremely high densities. We show that such an interaction averts the unphysical big-bang singularity, replacing it with a cusp-like bounce at a finite minimum scale factor, before which the Universe was contracting. This scenario also explains why the present Universe at largest scales appears spatially flat, homogeneous and isotropic." @default.
• W2036707580 created "2016-06-24" @default.
• W2036707580 creator A5017028948 @default.
• W2036707580 date "2012-05-29" @default.
• W2036707580 modified "2023-09-23" @default.
• W2036707580 title "Nonsingular, big-bounce cosmology from spinor-torsion coupling" @default.
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• W2036707580 doi "https://doi.org/10.1103/physrevd.85.107502" @default.
• W2036707580 hasPublicationYear "2012" @default.
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