Magnetoplasmons in thin films in the Voigt configuration

M. S. Kushwaha and P. Halevi
Phys. Rev. B 36, 5960 – Published 15 October 1987
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Abstract

We have studied the magnetoplasma modes of a thin film, bounded by two dissimilar dielectrics, the applied magnetic field B0 being parallel to the interfaces and the waves propagating in a direction perpendicular to B0 (Voigt geometry). On the basis of local theory we have derived the exact dispersion relation that governs the propagation characteristics of both surface and bulk (or waveguide) modes. These waves are p (or TM) polarized and exhibit nonreciprocity with respect to their direction of propagation. An analytic solution for the propagation constant qz(ω) has been found in the nonretarded limit, valid for ω/c≪‖qz‖≪1/d, where d is the thickness of the film. In the limit ‖qz‖→∞ there are two surface modes whose limiting frequencies are given by εzz(ω)±iεyz(ω) sgn(qz)=-εj, where εij(ω) is an element of the dielectric tensor of the semiconductor, and ε1 and ε3 are the dielectric constants of the bounding media.

Moreover, in the nonretarded limit as B0 is increased, the upper mode changes its behavior from monotonically decreasing to monotonically increasing; for a simple model of εij(ω) this occurs at a critical value of the cyclotron-frequency to plasma-frequency ratio ωc/ωp=[εL(εL2/εj2-1)]12, where εL is the background dielectric constant and, for qz>0 (qz<0) the correct choice is j=3 (j=1). Then, for a given propagation direction, the upper surface mode degenerates into a horizontal line, i.e., the corresponding group velocity vanishes. We have also applied to the general dispersion relation a thin-film approximation βd≪1. This enables us to find an analytic solution in two cases: (1) a very thin semiconducting overlayer on a metallic substrate, giving rise to a splitting in the spectrum in the vicinity of the hybrid cyclotron-plasmon frequency with the creation of a gap; (2) a very thin, unsupported, magnetoplasma film in which case we find four polariton branches.

  • Received 19 March 1987

DOI:https://doi.org/10.1103/PhysRevB.36.5960

©1987 American Physical Society

Authors & Affiliations

M. S. Kushwaha and P. Halevi

  • Departamento de Fsica, Instituto de Ciencias, Universidad Autónoma de Puebla, Apartado Postal J-48, Puebla 72570 Mexico

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Vol. 36, Iss. 11 — 15 October 1987

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