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Berlin 2012 – wissenschaftliches Programm

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HL: Fachverband Halbleiterphysik

HL 32: Transport Properties I (mainly Spin Physics and Magnetic Fields)

HL 32.10: Vortrag

Dienstag, 27. März 2012, 12:30–12:45, EW 203

Interplay of spin and orbital magnetogyrotropic photogalvanic effects in InSb-based quantum wells — •Sebastian Stachel1, Peter Olbrich1, Christina Zoth1, Ursula Hagner1, Thomas Stangl1, Cynthia Karl1, Peter Lutz1, Vasily Bel’kov2, Leonid Golub2, Steve K. Clowes3, Tim Ashley4, Adam M. Gilbertson5, and Sergey D. Ganichev11Terahertz Center, University of Regensburg, Regensburg, Germany — 2Ioffe Institute, St. Petersburg, Russia — 3Advanced Technology Institute and SEPNet, University of Surrey, UK — 4School of Engineering, University of Warwick, UK — 5Blackett Laboratory, Imperial College, UK

Here we report on the observation and detailed study of the magnetic-field induced photocurrents in n-doped InSb/InAlSb quantum wells (QWs). We show that the intraband absorption of terahertz radiation in QWs causes a dc electric current in the presence of an in-plane magnetic field. While at moderate magnetic fields B the photocurrent depends linear on B, at high magnetic fields it becomes nonlinear and inverses its sign. The generation of this current is analyzed in terms of electron gas heating and asymmetric scattering in k-space [1]. We show that due to the narrow gap, strong magnetic proberty and strong spin-orbit coupling this effect is substantially enhanced compared to other III-V materials. It is demonstrated that the strong nonlinear behavior is due to a nonlinear Zeeman spin splitting. [1] V.V. Belkov and S.D. Ganichev, Sem. Sci. Tec. 23, 114003 (2008)

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