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Uspekhi Fizicheskikh Nauk, 2014, Volume 184, Number 2, Pages 177–181
DOI: https://doi.org/10.3367/UFNr.0184.201402f.0177 (Mi ufn4883) 		 
This article is cited in 1 scientific paper (total in 1 paper)

CONFERENCES AND SYMPOSIA. 100th ANNIVERSARY OF THE BIRTH OF I Ya POMERANCHUK

Gravitational four-fermion interaction in the early Universe

A. S. Rudenkoab, I. B. Khriplovichab

a Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences, Novosibirsk
b Novosibirsk State University
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DOI: https://doi.org/10.3367/UFNr.0184.201402f.0177
Abstract: 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 cosmology. An explicit analytic 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 a Big Bounce.
Received: November 23, 2013
Accepted: June 5, 2013
English version:
Physics–Uspekhi, 2014, Volume 57, Issue 2, Pages 167–170
DOI: https://doi.org/10.3367/UFNe.0184.201402f.0177
Bibliographic databases:
Document Type: Article
PACS: 04.20.-q, 04.62.+v, 98.80.-k
Language: Russian
Citation: A. S. Rudenko, I. B. Khriplovich, “Gravitational four-fermion interaction in the early Universe”, UFN, 184:2 (2014), 177–181; Phys. Usp., 57:2 (2014), 167–170
Citation in format AMSBIB
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    CONFERENCES AND SYMPOSIA
    This publication is cited in the following 1 articles:
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