Lepton asymmetries and the growth of cosmological seed magnetic fields
arXiv:0704.3978 · doi:10.1088/1126-6708/2008/03/067
Abstract
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.
4 pages, no figures, final published version available online at http://www.iop.org/EJ/abstract/1029-8479/2008/03/067
Cited by in corpus (3)
- Quantum field theory in a magnetic field: From quantum chromodynamics to graphene and Dirac semimetals
- Lepton asymmetry growth in the symmetric phase of an electroweak plasma with hypermagnetic fields versus its washing out by sphalerons
- Strong First Order Phase Transition and Violation in the Compact 341 Model