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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