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Terahertz radiation from semiconductor surfaces in magnetic fields at high-density excitation

机译:在高密度激发下磁场中半导体表面的太赫兹辐射

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We investigated the radiation mechanisms of THz radiation from semiconductor surfaces at high-density excitation under a magnetic field. Excitation density dependences of radiation intensity and the waveforms of the terahertz radiations from InAs and semi-insulating InP surfaces were investigated with and without magnetic fields (0, 2T, and -2T). Substantial changes of the intensity and the waveforms including a polarity reversal were observed by changing the excitation densities. In InAs, the enhancement of the radiated energy is observed under a magnetic field of ±2 T and the radiated energy increases quadratically with increasing the excitation density below 0.1 μJ/cm~2. The behavior of the dependence for ±2 T changes clearly above 1 μJ/cm~2. The drastic change of the wave forms was observed at high density excitation and was explained by the polarity reversal of the THz wave induced by the magnetic field. The reversal originates from the crossover of the radiation mechanism of the magnetic induced component from the electrons in the accumulation layer to the diffusion current by the photogenerated electrons at high-density excitation under a magnetic field. In InP, the characteristic behavior including the polarity reversal of the angle independent component was observed in the crystal orientation angle dependence by changing the excitation density. These facts indicate that three different radiation mechanisms co-exist and that the dominant radiation mechanism changes with increasing the excitation density from the drift current for low-excitation density to the diffusion current and the optical rectification for high-excitation density.
机译:我们研究了磁场下高密度激发下半导体表面太赫兹辐射的辐射机理。研究了在有磁场和无磁场(0、2T和-2T)的情况下,辐射强度与来自InAs和半绝缘InP表面的太赫兹辐射波形的激发密度相关性。通过改变激发密度,观察到强度和包括极性反转在内的波形发生了实质性变化。在InAs中,在±2 T的磁场下观察到辐射能的增强,并且随着激发密度在0.1μJ/ cm〜2以下,辐射能呈二次方增加。在高于1μJ/ cm〜2时,±2 T的依存关系变化明显。在高密度激发下观察到波形的急剧变化,并通过磁场引起的太赫兹波的极性反转来解释。逆转起源于在磁场下高密度激发下光生电子所产生的磁感应成分的辐射机理从积累层中的电子到扩散电流的交叉。在InP中,通过改变激发密度,在晶体取向角依赖性中观察到包括角独立成分的极性反转的特性行为。这些事实表明,三种不同的辐射机制共存,并且主导的辐射机制随着激发密度的增加而变化,从低激发密度的漂移电流到高激发密度的扩散电流和光学整流。

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