0000000000224753

AUTHOR

Dmitry Sokoloff

showing 2 related works from this author

Lepton asymmetries and primordial hypermagnetic helicity evolution

2012

The hypermagnetic helicity density at the electroweak phase transition (EWPT) exceeds many orders of magnitude the galactic magnetic helicity density. Together with previous magnetic helicity evolution calculations after the EWPT and hypermagnetic helicity conversion to the magnetic one at the EWPT, the present calculation completes the description of the evolution of this important topological feature of cosmological magnetic fields. It suggests that if the magnetic field seeding the galactic dynamo has a primordial origin, it should be substantially helical. This should be taken into account in scenarios of galactic magnetic field evolution with a cosmological seed.

PhysicsPhase transitionParticle physicsQuantitative Biology::BiomoleculesCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsElectroweak interactionFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesHelicityMagnetic fieldHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Orders of magnitude (time)Magnetic helicity0103 physical sciences010306 general physicsDynamoLeptonAstrophysics - Cosmology and Nongalactic Astrophysics
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Is the baryon asymmetry of the Universe related to galactic magnetic fields?

2009

A tiny hypermagnetic field generated before the electroweak phase transition (EWPT) associated to the generation of elementary particle masses can polarize the early Universe hot plasma at huge redshifts z >= 10(15). The anomalous violation of the right-handed electron current characteristic of the EWPT converts the lepton asymmetry into a baryon asymmetry. Under reasonable approximations, the magnetic field strength inferred by requiring such "leptogenic'' origin for the observed baryon asymmetry of the Universe matches the large-scale cosmological magnetic field strengths estimated from current astronomical observations.

PhysicsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaMagnetic fieldHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetryElectron currentHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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