Magnetic helicity in plasma of chiral fermions electroweakly interacting with inhomogeneous matter
DOI10.1016/J.NUCLPHYSB.2020.115049zbMath1479.82056arXiv2005.09358OpenAlexW3026073532MaRDI QIDQ2230246
Publication date: 17 September 2021
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2005.09358
Electromagnetic interaction; quantum electrodynamics (81V10) Weak interaction in quantum theory (81V15) Statistical mechanics of plasmas (82D10) Kinetic theory of gases in time-dependent statistical mechanics (82C40) Galactic and stellar dynamics (85A05) Statistical mechanics of magnetic materials (82D40) Fermionic systems in quantum theory (81V74)
Cites Work
- Generation of strong magnetic fields in dense quark matter driven by the electroweak interaction of quarks
- The physics and astrophysics of neutron stars. With a foreword by Valeria Ferrari, Jerome Margueron and Jose A. Pons
- Quantal phase factors accompanying adiabatic changes
- Magnetic helicity evolution in a neutron star accounting for the Adler-Bell-Jackiw anomaly
- Permanent mean spin source of the chiral magnetic effect in neutron stars
- Generation of the relic neutrino asymmetry in a hot plasma of the early universe
- Stable magnetic fields in stellar interiors
This page was built for publication: Magnetic helicity in plasma of chiral fermions electroweakly interacting with inhomogeneous matter
