Classical relativistic model for spin dependence in a magnetized electron gas

D. B. Melrose and A. Mushtaq
Phys. Rev. E 83, 056404 – Published 26 May 2011

Abstract

The response of a cold electron gas is generalized to include the spin of the electron described by the relativistically correct quasiclassical Bargmann-Michel-Telegdi (BMT) equation. The magnetization of the electron gas is assumed to be along the background magnetic field B and the spin-dependent contribution to the response tensor is proportional to the magnitude of the magnetization. The dispersion equation is shown to be quadratic in the refractive index squared, and dispersion curves for the two wave modes are plotted for cases where the magnetic field associated with magnetization is comparable with B. Two intrinsically spin-dependent wave modes are identified: one bounded by two resonances and the other by two cutoffs. The counterpart of the z mode can escape without encountering a resonance or a cutoff.

    • Received 4 February 2011

    DOI:https://doi.org/10.1103/PhysRevE.83.056404

    ©2011 American Physical Society

    Authors & Affiliations

    D. B. Melrose1 and A. Mushtaq1,2,*

    • 1School of Physics, University of Sydney, NSW 2006, Australia
    • 2TPPD, PINSTECH, P. O. Nilore Islamabad 44000, Pakistan

    • *Corresponding author: msherpao@gmail.com

    Article Text (Subscription Required)

    Click to Expand

    References (Subscription Required)

    Click to Expand
    Issue

    Vol. 83, Iss. 5 — May 2011

    Reuse & Permissions
    Access Options
    Author publication services for translation and copyediting assistance advertisement

    Authorization Required


    ×
    ×

    Images

    ×

    Sign up to receive regular email alerts from Physical Review E

    Log In

    Cancel
    ×

    Search


    Article Lookup

    Paste a citation or DOI

    Enter a citation
    ×