Magnetoresistance oscillations induced by high-intensity terahertz radiation

T. Herrmann, Z. D. Kvon, I. A. Dmitriev, D. A. Kozlov, B. Jentzsch, M. Schneider, L. Schell, V. V. Bel'kov, A. Bayer, D. Schuh, D. Bougeard, T. Kuczmik, M. Oltscher, D. Weiss, and S. D. Ganichev
Phys. Rev. B 96, 115449 – Published 27 September 2017

Abstract

We report on observation of pronounced terahertz radiation-induced magnetoresistivity oscillations in AlGaAs/GaAs two-dimensional electron systems, the terahertz analog of the microwave induced resistivity oscillations (MIRO). Applying high-power radiation of a pulsed molecular laser we demonstrate that MIRO, so far observed at low power only, are not destroyed even at very high intensities. Experiments with radiation intensity ranging over five orders of magnitude from 0.1 to 104W/cm2 reveal high-power saturation of the MIRO amplitude, which is well described by an empirical fit function I/(1+I/Is)β with β1. The saturation intensity Is is of the order of tens of watts per square centimeter and increases by a factor of 6 by increasing the radiation frequency from 0.6 to 1.1 THz. The results are discussed in terms of microscopic mechanisms of MIRO and compared to nonlinear effects observed earlier at significantly lower excitation frequencies.

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  • Received 22 June 2017
  • Revised 3 August 2017

DOI:https://doi.org/10.1103/PhysRevB.96.115449

©2017 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter & Materials Physics

Authors & Affiliations

T. Herrmann1, Z. D. Kvon2,3, I. A. Dmitriev1,4, D. A. Kozlov2,3, B. Jentzsch1, M. Schneider1, L. Schell1, V. V. Bel'kov4, A. Bayer1, D. Schuh1, D. Bougeard1, T. Kuczmik1, M. Oltscher1, D. Weiss1, and S. D. Ganichev1

  • 1Terahertz Center, University of Regensburg, 93040 Regensburg, Germany
  • 2Rzhanov Institute of Semiconductor Physics, 630090 Novosibirsk, Russia
  • 3Novosibirsk State University, 630090 Novosibirsk, Russia
  • 4Ioffe Institute, 194021 Saint Petersburg, Russia

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Issue

Vol. 96, Iss. 11 — 15 September 2017

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