Standard

Gravitational four-fermion interaction in the early Universe. / Rudenko, A. S.; Khriplovich, I. B.

In: Physics-Uspekhi, Vol. 57, No. 2, 01.01.2014, p. 167-170.

Research output: Contribution to journal › Article › peer-review

Harvard

Rudenko, AS & Khriplovich, IB 2014, 'Gravitational four-fermion interaction in the early Universe', Physics-Uspekhi, vol. 57, no. 2, pp. 167-170. https://doi.org/10.3367/UFNe.0184.201402f.0177

APA

Rudenko, A. S., & Khriplovich, I. B. (2014). Gravitational four-fermion interaction in the early Universe. Physics-Uspekhi, 57(2), 167-170. https://doi.org/10.3367/UFNe.0184.201402f.0177

Vancouver

Rudenko AS, Khriplovich IB. Gravitational four-fermion interaction in the early Universe. Physics-Uspekhi. 2014 Jan 1;57(2):167-170. https://doi.org/10.3367/UFNe.0184.201402f.0177

Author

Rudenko, A. S. ; Khriplovich, I. B. / Gravitational four-fermion interaction in the early Universe. In: Physics-Uspekhi. 2014 ; Vol. 57, No. 2. pp. 167-170.

BibTeX

@article{1bd92c70c8d743d8a05f9af3a4b51efa,
title = "Gravitational four-fermion interaction in the early Universe",
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 ultra-relativistic energy-momentum tensor are included. We demonstrate that gravitational four-fermion interaction does not result in a Big Bounce.",
author = "Rudenko, {A. S.} and Khriplovich, {I. B.}",
year = "2014",
month = jan,
day = "1",
doi = "10.3367/UFNe.0184.201402f.0177",
language = "English",
volume = "57",
pages = "167--170",
journal = "Physics-Uspekhi",
issn = "1063-7869",
publisher = "Turpion Ltd.",
number = "2",

}

RIS

TY - JOUR

T1 - Gravitational four-fermion interaction in the early Universe

AU - Rudenko, A. S.

AU - Khriplovich, I. B.

PY - 2014/1/1

Y1 - 2014/1/1

N2 - 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 ultra-relativistic energy-momentum tensor are included. We demonstrate that gravitational four-fermion interaction does not result in a Big Bounce.

AB - 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 ultra-relativistic energy-momentum tensor are included. We demonstrate that gravitational four-fermion interaction does not result in a Big Bounce.

UR - http://www.scopus.com/inward/record.url?scp=84900817693&partnerID=8YFLogxK

U2 - 10.3367/UFNe.0184.201402f.0177

DO - 10.3367/UFNe.0184.201402f.0177

M3 - Article

AN - SCOPUS:84900817693

VL - 57

SP - 167

EP - 170

JO - Physics-Uspekhi

JF - Physics-Uspekhi

SN - 1063-7869

IS - 2

ER -

ID: 36639987