Chiral fermion asymmetry in high-energy plasma simulations

DOI10.1080/03091929.2019.1591393zbMath1482.76153arXiv1808.06624OpenAlexW2888317318WikidataQ114640061 ScholiaQ114640061MaRDI QIDQ5065697

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Publication date: 22 March 2022

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1808.06624

zbMATH Keywords

turbulencenumerical simulationschiral magnetic effectMHD dynamosrelativistic magnetohydrodynamics (MHD)

Mathematics Subject Classification ID

Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (5)

Permanent mean spin source of the chiral magnetic effect in neutron stars ⋮ Self-exciting fluid dynamos ⋮ Cosmological constant, axial anomalies and photon mass dynamos from chiral fermionic torsion ⋮ Dynamo chiral plasma instabilities from charges and oscillations driven by torsion fluctuations ⋮ Introduction

Cites Work

• Quantum field theory in a magnetic field: from quantum chromodynamics to graphene and Dirac semimetals
• Strongly interacting matter in magnetic fields
• Relaxation of the chiral chemical potential in the dense matter of a neutron star
• Experimental demonstration of a homogeneous two-scale dynamo
• Magnetic helicity and cosmological magnetic field
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