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Photoinduced magnetization wave in diluted magnetic semiconductors

机译:稀释磁半导体中的光诱导磁化波

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We derive an evolutional equation incorporating the processes of spin-polarization transfer from an electron to a magnetic ion subsystem of a diluted magnetic semiconductor along with spin-lattice relaxation and spatial spin diffusion. Above equation has been obtained for nonequilibrium magnetization due to exchange scattering of photoexcited charge carriers by magnetic ions. We show that the mechanism of a band gap narrowing due to exchange scattering requires relatively low optical power to reach an optical bistability for pump frequency range close to crystal band gap. In a bulk crystal, only relatively small local area with essential magnetization enhancement can absorb optical power, thus forming a photoinduced magnetization wave. Spatial spin diffusion can be responsible for a motion of such magnetization wave. We solve above derived equation both analytically for one-dimensional case and numerically otherwise and perform its stability analysis. We also evaluate numerically possible threshold of photoinduced magnetization wave excitation for typical diluted magnetic semiconductor A1-xIIMnxBVI and estimate its length and velocity of propagation.
机译:我们推出了一种进化方程,其包括从电子到稀释的磁半导体的磁离子子系统的自旋极化转移的过程以及旋转晶格松弛和空间自旋扩散。由于磁离子的光屏蔽电荷载体的交换散射,已经获得了以上方程。我们表明,由于交换散射引起的带隙缩小的机制需要相对低的光功率来达到靠近晶带隙的泵频率范围的光学双稳态。在散装晶体中,只有相对较小的局部区域,具有必要的磁化增强可以吸收光功率,从而形成光致磁化波。空间自旋扩散可以负责这种磁化波的运动。我们在分析到一维壳体和数值否则地解决了上面的衍生方程,否则以其他方式进行稳定性分析。我们还评估典型的稀释磁半导体A1-XIIMNXBVI的光抑制磁化波激励的数值可能的阈值,并估计其长度和传播的速度。

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