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自旋噪声的拉曼散射模型

Raman scattering model of the spin noise.

作者信息

Kozlov G G, Fomin A A, Petrov M Yu, Ryzhov I I, Zapasskii V S

出版信息

Opt Express. 2021 Feb 15;29(4):4770-4782. doi: 10.1364/OE.415034.

Abstract

The mechanism of formation of the polarimetric signal observed in the spin noise spectroscopy (SNS) is analyzed from the viewpoint of the light scattering theory. A rigorous calculation of the polarimetric signal (Faraday rotation or ellipticity) recorded in the SNS is presented in the approximation of single scattering. We show that it is most correctly to consider this noise as a result of scattering of the probe light beam by fluctuating susceptibility of the medium. Fluctuations of the gyrotropic (antisymmetric) part of the susceptibility tensor lead to appearance of the typical for the SNS Faraday rotation noise at the Larmor frequency. At the same time, fluctuations of linear anisotropy of the medium (symmetric part of the susceptibility tensor) give rise to the ellipticity noise of the probe beam spectrally localized at the double Larmor frequency. The results of the theoretical analysis well agree with the experimental data on the ellipticity noise in cesium vapor.

摘要

从光散射理论的角度分析了自旋噪声光谱学(SNS)中观测到的偏振信号的形成机制。在单次散射近似下,给出了SNS中记录的偏振信号(法拉第旋转或椭圆率)的严格计算。我们表明,最正确的是将这种噪声视为探测光束被介质的波动磁化率散射的结果。磁化率张量的旋光(反对称)部分的波动导致在拉莫尔频率出现SNS典型的法拉第旋转噪声。同时,介质的线性各向异性(磁化率张量的对称部分)的波动产生了频谱上位于两倍拉莫尔频率的探测光束的椭圆率噪声。理论分析结果与铯蒸汽中椭圆率噪声的实验数据吻合良好。

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