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Effect of a primordial magnetic field on the inflaton decay process in a warm inflation scenario
Author(s) -
BasteroGil M.,
Piccinelli G.,
Sanchez A.
Publication year - 2015
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.201512220
Subject(s) - inflaton , physics , inflation (cosmology) , dissipative system , inflationary epoch , quantum electrodynamics , coupling (piping) , magnetic field , theoretical physics , astrophysics , cosmology , metric expansion of space , quantum mechanics , dark energy , mechanical engineering , engineering
Magnetic fields appear everywhere in the Universe. Their widespread presence at high redshifts and very large scales suggests that their origin could be primordial. In particular, their presence during the inflationary epoch can certainly not be ruled out. In the warm inflation scenario, the coupling of the inflaton to other bosonic and fermionic fields gives rise to dissipative effects that modify the inflationary dynamics. Since primordial magnetic fields could have an effect on both the effective inflationary potential and the inflaton decay process, their contribution must be considered together with the finite temperature corrections. We review here their effect on the inflationary potential and present preliminary results of their intervention in the dissipation process. (© 2015 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)