Publication Date:
2016-03-05
Description:
Author(s): Leonardo Campanelli We analyze the evolution of superhorizon-scale magnetic fields from the end of inflation till today. Whatever is the mechanism responsible for their generation during inflation, we find that a given magnetic mode with wave number k evolves, after inflation, according to the values of k η e , n k , and Ω k … [Phys. Rev. D 93, 063501] Published Fri Mar 04, 2016
Keywords:
Cosmology
Print ISSN:
0556-2821
Electronic ISSN:
1089-4918
Topics:
Physics