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Ultrafast magneto-optical spectroscopy of GaMnAs

机译:GaMnAs的超快磁光光谱

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摘要

Spin dynamics in the III-V dilute magnetic semiconductor GaMnAs is investigated by photo-induceddemagnetization. Experimental results obtained from two different time-dependent characterization techniques – “twocolor-probe” magneto-optical Kerr effect (TR-MOKE) and mid-infrared differential transmittance – are compared.Upon photo-excitation with a 100 fs, 3.1 eV light pulse, a long demagnetization time in the hundreds of picosecondstimescale is found by TR-MOKE, indicating a spin-dependent band structure in this material. In mid-infraredmeasurements, a positive increase of the differential transmittance is observed in the same time interval when the sampleis cooled below its Currie temperature. It is shown that this mid-infrared absorption feature is directly related toferromagnetism in this material. The magnetism-related component of the broad DC mid-infrared absorption peakcharacteristic of this p-type material could be observed with this time-resolved measurement. Experimental results weresimulated with a model describing the interaction between three thermal reservoirs (hole, spin and lattice) and takingthermal diffusion into account.
机译:通过光致退磁研究了III-V稀磁半导体GaMnAs中的自旋动力学。比较了从两种不同的随时间变化的表征技术获得的实验结果-“双色探针”磁光克尔效应(TR-MOKE)和中红外微分透射率。在100 fs,3.1 eV光脉冲下进行光激发,TR-MOKE发现在数百皮秒的时间范围内有很长的退磁时间,这表明这种材料具有自旋相关的能带结构。在中红外测量中,当样品冷却至其居里温度以下时,在相同的时间间隔内观察到差分透射率的正增加。结果表明,这种中红外吸收特征与该材料中的铁磁性直接相关。通过这种时间分辨的测量结果,可以观察到该p型材料的宽DC中红外吸收峰特性的磁性相关成分。用描述三个热储层(孔,自旋和晶格)之间的相互作用并考虑热扩散的模型模拟了实验结果。

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