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Title: Amplification of mean magnetic field and magnetic helicity production in hot lepton plasma of early universe

Abstract

We argue that the magnetic helicity conservation is violated at the lepton stage in the evolution of early Universe owing to the parity violation in the Standard Model of electroweak interactions. As a result, a cosmological magnetic field which can be a seed for the galactic dynamo obtains from the beginning a substantial magnetic helicity which has to be taken into account in the magnetic helicity balance at the later stage of galactic dynamo. The particle physics mechanism suggested in our works depends neither on helicity of matter turbulence with plasma vortices resulting in the standard {alpha} effect in dynamo theory nor on general rotation. The mechanism can result in a self-exitation of an (almost) uniform cosmological magnetic field.

Authors:
;  [1]
  1. Russian Academy of Sciencies (IZMIRAN), Institute of the Terrestrial Magnetism, Ionosphere and Radiowave Propagation (Russian Federation)
Publication Date:
OSTI Identifier:
21075959
Resource Type:
Journal Article
Resource Relation:
Journal Name: Physics of Atomic Nuclei; Journal Volume: 70; Journal Issue: 1; Other Information: DOI: 10.1134/S1063778807010176; Copyright (c) 2007 Nauka/Interperiodica; Article Copyright (c) 2007 Pleiades Publishing, Ltd; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; AMPLIFICATION; EVOLUTION; HELICITY; LEPTONS; MAGNETIC FIELDS; PARITY; PLASMA; ROTATION; STANDARD MODEL; TURBULENCE; UNIVERSE; WEAK INTERACTIONS; WEINBERG-SALAM GAUGE MODEL

Citation Formats

Semikoz, V. B., E-mail: semikoz@izmiran.rssi.ru, and Sokoloff, D. D. Amplification of mean magnetic field and magnetic helicity production in hot lepton plasma of early universe. United States: N. p., 2007. Web. doi:10.1134/S1063778807010176.
Semikoz, V. B., E-mail: semikoz@izmiran.rssi.ru, & Sokoloff, D. D. Amplification of mean magnetic field and magnetic helicity production in hot lepton plasma of early universe. United States. doi:10.1134/S1063778807010176.
Semikoz, V. B., E-mail: semikoz@izmiran.rssi.ru, and Sokoloff, D. D. Mon . "Amplification of mean magnetic field and magnetic helicity production in hot lepton plasma of early universe". United States. doi:10.1134/S1063778807010176.
@article{osti_21075959,
title = {Amplification of mean magnetic field and magnetic helicity production in hot lepton plasma of early universe},
author = {Semikoz, V. B., E-mail: semikoz@izmiran.rssi.ru and Sokoloff, D. D.},
abstractNote = {We argue that the magnetic helicity conservation is violated at the lepton stage in the evolution of early Universe owing to the parity violation in the Standard Model of electroweak interactions. As a result, a cosmological magnetic field which can be a seed for the galactic dynamo obtains from the beginning a substantial magnetic helicity which has to be taken into account in the magnetic helicity balance at the later stage of galactic dynamo. The particle physics mechanism suggested in our works depends neither on helicity of matter turbulence with plasma vortices resulting in the standard {alpha} effect in dynamo theory nor on general rotation. The mechanism can result in a self-exitation of an (almost) uniform cosmological magnetic field.},
doi = {10.1134/S1063778807010176},
journal = {Physics of Atomic Nuclei},
number = 1,
volume = 70,
place = {United States},
year = {Mon Jan 15 00:00:00 EST 2007},
month = {Mon Jan 15 00:00:00 EST 2007}
}
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