Optics of spin-noise-induced gyrotropy of an asymmetric microcavity

S. V. Poltavtsev, I. I. Ryzhov, R. V. Cherbunin, A. V. Mikhailov, N. E. Kopteva, G. G. Kozlov, K. V. Kavokin, V. S. Zapasskii, P. V. Lagoudakis, and A. V. Kavokin
Phys. Rev. B 89, 205308 – Published 13 May 2014

Abstract

The optical gyrotropy noise of a high-finesse semiconductor Bragg microcavity with an embedded quantum well (QW) is studied at different detunings of the photon mode with respect to the QW exciton resonances. A strong suppression of the noise magnitude for the photon mode frequencies lying above exciton resonances is found. We show that such a critical behavior of the observed optical noise power is specific to asymmetric Fabry-Perot resonators. As follows from our analysis, at a certain level of intracavity loss, the reflectivity of the asymmetric resonator vanishes, while the polarimetric sensitivity to the gyrotropy changes dramatically when moving across the critical point. The results of model calculations are in a good agreement with our experimental data on the spin noise in a single-quantum-well microcavity and are confirmed also by the spectra of the photoinduced Kerr rotation in the pump-probe experiments.

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  • Received 31 January 2014
  • Revised 7 April 2014

DOI:https://doi.org/10.1103/PhysRevB.89.205308

©2014 American Physical Society

Authors & Affiliations

S. V. Poltavtsev1, I. I. Ryzhov1, R. V. Cherbunin1, A. V. Mikhailov1, N. E. Kopteva1, G. G. Kozlov1, K. V. Kavokin1,2, V. S. Zapasskii1, P. V. Lagoudakis3, and A. V. Kavokin1,3

  • 1Spin-Optics Laboratory, St. Petersburg State University, 198504 St. Petersburg, Russia
  • 2A. F. Ioffe Physical-Technical Institute, Russian Academy of Sciences, 194021 St. Petersburg, Russia
  • 3Department of Physics & Astronomy, University of Southampton, Southampton SO17 1BJ, United Kingdom

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Issue

Vol. 89, Iss. 20 — 15 May 2014

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