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    American Physical Society (APS)
    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
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