6533b821fe1ef96bd127c2c6

RESEARCH PRODUCT

Lepton asymmetries and the growth of cosmological seed magnetic fields

José W. F. ValleVictor B. Semikoz

subject

PhysicsNuclear and High Energy PhysicsPhase transitionParticle physicsElectroweak interactionAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaParity (physics)PlasmaAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsMagnetic fieldHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Lepton

description

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.

10.1088/1126-6708/2008/03/067http://hdl.handle.net/10550/47466