arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2102.02780cond-mat.mes-hall
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法拉第几何中的共振自旋放大

Resonant spin amplification in Faraday geometry

P. Schering, E. Evers, V. Nedelea, D. S. Smirnov, E. A. Zhukov, D. R. Yakovlev, M. Bayer, G. S. Uhrig, A. Greilich

摘要:

我们证明了实现共振自旋放大(RSA)效应在法拉第几何中的磁场施加平行于光致自旋极化,使没有RSA是预期的。然而,模型的考虑预测,它可以实现一个中心的自旋与波动的自旋环境相互作用。作为演示,我们选择了一个系综的单电荷(In,Ga)As/GaAs量子点,其中居民电子自旋与周围的核自旋相互作用。在法拉第几何中观察RSA需要高重复率的强泵浦脉冲,并且可以通过自旋惯性效应来增强。它为测量载流子的纵向$g$因子提供了最直接、最可靠的工具。

英文摘要:

We demonstrate the realization of the resonant spin amplification (RSA) effect in Faraday geometry where a magnetic field is applied parallel to the optically induced spin polarization so that no RSA is expected. However, model considerations predict that it can be realized for a central spin interacting with a fluctuating spin environment. As a demonstrator, we choose an ensemble of singly-charged (In,Ga)As/GaAs quantum dots, where the resident electron spins interact with the surrounding nuclear spins. The observation of RSA in Faraday geometry requires intense pump pulses with a high repetition rate and can be enhanced by means of the spin-inertia effect. Potentially, it provides the most direct and reliable tool to measure the longitudinal $g$ factor of the charge carriers.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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