Generalized Magnetofluid Connections in Relativistic Magnetohydrodynamics
Plasma Physics
2015-05-05 v1 High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
Space Physics
Abstract
The concept of magnetic connections is extended to non-ideal relativistic magnetohydrodynamical plasmas. Adopting a general set of equations for relativistic magnetohydrodynamics including thermal-inertial, thermal electromotive, Hall and current-inertia effects, we derive a new covariant connection equation showing the existence of generalized magnetofluid connections that are preserved during the dissipationless plasma dynamics. These connections are intimately linked to a general antisymmetric tensor that unifies the electromagnetic and fluid fields, allowing the extension of the magnetic connection notion to a much broader concept.
Keywords
Cite
@article{arxiv.1502.07461,
title = {Generalized Magnetofluid Connections in Relativistic Magnetohydrodynamics},
author = {Felipe A. Asenjo and Luca Comisso},
journal= {arXiv preprint arXiv:1502.07461},
year = {2015}
}
Comments
Accepted for publication in Physical Review Letters