Lepton asymmetries and the growth of cosmological seed magnetic fields

Details Lepton asymmetries and the growth of cosmological seed magnetic fields Lepton asymmetries and the growth of cosmological seed magnetic fields

2007-04-30

arxiv.org/abs/0704.3978v2

JHEP 0803:067,2008

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages, no figures, final published version available online at http://www.iop.org/EJ/abstract/1029-8479/2008/03/067

Scientific paper

10.1088/1126-6708/2008/03/067

Primordial cosmological hypermagnetic fields polarize the early
Universe plasma prior to the electroweak phase transition (EWPT).
As a result of the long range parity violating gauge interaction present in
the Standard Model their magnitude gets amplified, opening a new, perturbative
way, of accounting for the observed intergalactic magnetic fields.

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