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Paper detail

Three-magnetic fields

A completely new mechanism to generate the observed amount of large-scale cosmological magnetic fields is introduced in the context of three-form inflation. The amplification of the fields occurs via fourth order dynamics of the vector perturbations and avoids the backreaction problem that plagues most previously introduced mechanisms.

preprint2012arXivOpen access
Tomi S. KoivistoFederico R. Urban
astro-ph.COhep-phhep-th
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Tomi S. KoivistoFederico R. Urban

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