Relativistic Particle and Relativistic Fluids: Magnetic Moment and Spin-Orbit Interactions

Dimitra Karabali and V. P. Nair
Phys. Rev. D 90, 105018 – Published 12 November 2014

Abstract

We consider relativistic charged-particle dynamics and relativistic magnetohydrodynamics using symplectic structures and actions given in terms of coadjoint orbits of the Poincaré group. The particle case is meant to clarify some points such as how minimal coupling (as defined in the text) leads to a gyromagnetic ratio g=2 and to set the stage for fluid dynamics. The general group-theoretic framework is further explained and is then used to set up Abelian magnetohydrodynamics including spin effects. An interesting new physical effect is precession of spin density induced by gradients in pressure and energy density. The Euler equation (the dynamics of the velocity field) is also modified by gradients of the spin density.

  • Received 22 June 2014

DOI:https://doi.org/10.1103/PhysRevD.90.105018

© 2014 American Physical Society

Authors & Affiliations

Dimitra Karabali1,* and V. P. Nair2,†

  • 1Department of Physics and Astronomy, Lehman College of the CUNY, Bronx, New York 10468, USA
  • 2Physics Department, City College of the CUNY, New York, New York 10031, USA

  • *dimitra.karabali@lehman.cuny.edu
  • vpn@sci.ccny.cuny.edu

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Issue

Vol. 90, Iss. 10 — 15 November 2014

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