Gravitational four-fermion interaction and dynamics of the early Universe

11 Sept 2013, 17:30
20m
Oral We - 4

Speaker

Prof. Iosif Khriplovich (Budker Institute of Nuclear Physics, Novosibirsk)

Description

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. 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 GFFI does not result in Big Bounce.

Primary author

Prof. Iosif Khriplovich (Budker Institute of Nuclear Physics, Novosibirsk)

Co-author

Alexander Rudenko (Budker Institute of Nuclear Physics, Novosibirsk)

Presentation materials