Ogasawara T, Ohgushi K, Tomioka Y, Takahashi K S, Okamoto H, Kawasaki M, Tokura Y
Correlated Electron Research Center (CERC), National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba 305-8562, Japan.
Phys Rev Lett. 2005 Mar 4;94(8):087202. doi: 10.1103/PhysRevLett.94.087202. Epub 2005 Mar 3.
Ultrafast photoinduced spin dynamics has been investigated by time-resolved magneto-optical Kerr spectroscopy for various ferromagnetic and ferrimagnetic compounds: FeCr2S4, CoCr2S4, CuCr2Se4, CdCr2Se4, La0.6Sr0.4MnO3, and SrRuO3. The temporal demagnetization process, which is observed commonly for all the compounds, essentially consists of two components: One is an instantaneous change which originates perhaps from multiple emissions of magnetic excitations during nonradiative decay of photoexcited carriers, and the other is a delayed response due to thermalization of the spin system. The time constant of the delayed change depends strongly on materials and is scaled with the magnetocrystalline anisotropy, indicating that spin-orbit coupling is a dominant interaction for this process.
FeCr2S4、CoCr2S4、CuCr2Se4、CdCr2Se4、La0.6Sr0.4MnO3和SrRuO3,研究了超快光致自旋动力学。在所有化合物中普遍观察到的时间退磁过程,主要由两个部分组成:一个是瞬时变化,它可能源于光激发载流子非辐射衰变过程中磁激发的多次发射;另一个是由于自旋系统热化引起的延迟响应。延迟变化的时间常数强烈依赖于材料,并与磁晶各向异性成比例,这表明自旋轨道耦合是该过程的主导相互作用。