Lepton asymmetries and the growth of cosmological seed magnetic fields
NAGIOS: RODERIC FUNCIONANDO

Lepton asymmetries and the growth of cosmological seed magnetic fields

DSpace Repository

Lepton asymmetries and the growth of cosmological seed magnetic fields

Show full item record

View       (170.0Kb)

    
Semikoz, Victor B.; Furtado Valle, José Wagner Perfil
This document is a artículoDate2008

Este documento está disponible también en : http://hdl.handle.net/10550/47466
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 seeding the primordial Maxwellian magnetic field at EWPT.

    Semikoz, Victor B. Furtado Valle, José Wagner 2008 Lepton asymmetries and the growth of cosmological seed magnetic fields Journal of High Energy Physics 2008 3 067
http://dx.doi.org/10.1088/1126-6708/2008/03/067

This item appears in the following Collection(s)

Show full item record

Search DSpace

Advanced Search

Browse

Statistics