Gravitational four-fermion interaction and dynamics of the early Universe

Fuente: arXiv
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Main Authors: Khriplovich, I. B., Rudenko, A. S.
Format: Preprint
Published: 2013
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author Khriplovich, I. B.
Rudenko, A. S.
author_facet Khriplovich, I. B.
Rudenko, A. S.
contents If torsion exists, it generates gravitational four-fermion interaction (GFFI), essential on the Planck scale. We analyze the influence of this interaction on the Friedmann-Lemaitre-Robertson-Walker (FLRW) cosmology. Explicit analytical solution is derived for the problem where both the energy-momentum tensor generated by GFFI and the common ultrarelativistic energy-momentum tensor are included. We demonstrate that gravitational four-fermion interaction does not result in Big Bounce.
format Preprint
id arxiv_https___arxiv_org_abs_1303_1348
institution arXiv
publishDate 2013
record_format arxiv
spellingShingle Gravitational four-fermion interaction and dynamics of the early Universe
Khriplovich, I. B.
Rudenko, A. S.
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
If torsion exists, it generates gravitational four-fermion interaction (GFFI), essential on the Planck scale. We analyze the influence of this interaction on the Friedmann-Lemaitre-Robertson-Walker (FLRW) cosmology. Explicit analytical solution is derived for the problem where both the energy-momentum tensor generated by GFFI and the common ultrarelativistic energy-momentum tensor are included. We demonstrate that gravitational four-fermion interaction does not result in Big Bounce.
title Gravitational four-fermion interaction and dynamics of the early Universe
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/1303.1348