Relabeling symmetry in relativistic fluids and plasmas
Yohei Kawazura, Zensho Yoshida, Yasuhide Fukumoto

TL;DR
This paper derives a relativistic conservation law for canonical helicity from Noether's theorem using an action principle in Lagrangian coordinates, revealing why conventional helicity is not conserved in relativistic fluids and plasmas.
Contribution
It introduces a relativistic action principle for fluids and plasmas, deriving a new conservation law for relativistic canonical helicity and explaining the non-conservation of conventional helicity.
Findings
Derived relativistic canonical helicity conservation from Noether's theorem.
Explained the non-conservation of conventional helicity in relativistic settings.
Formulated a relativistic action principle for MHD and derived the relativistic cross helicity.
Abstract
The conservation of the recently formulated relativistic canonical helicity [Yoshida Z, Kawazura Y, and Yokoyama T 2014 J. Math. Phys. 55 043101] is derived from Noether's theorem by constructing an action principle on the relativistic Lagrangian coordinates (we obtain general cross helicities that include the helicity of the canonical vorticity). The conservation law is, then, explained by the relabeling symmetry pertinent to the Lagrangian label of fluid elements. Upon Eulerianizing the Noether current, the purely spatial volume integral on the Lagrangian coordinates is mapped to a space-time mixed three-dimensional integral on the four-dimensional Eulerian coordinates. The relativistic conservation law in the Eulerian coordinates is no longer represented by any divergence-free current; hence, it is not adequate to regard the relativistic helicity (represented by the Eulerian…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geomagnetism and Paleomagnetism Studies · Fluid Dynamics and Turbulent Flows
