Sekiguchi Fumiya, Budzinauskas Kestutis, Padmanabhan Prashant, Versteeg Rolf B, Tsurkan Vladimir, Kézsmárki István, Foggetti Francesco, Artyukhin Sergey, van Loosdrecht Paul H M
II. Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, D-50937, Köln, Germany.
Experimental Physics V, Center for Electronic Correlations and Magnetism, University of Augsburg, 86159, Augsburg, Germany.
Nat Commun. 2022 Jun 9;13(1):3212. doi: 10.1038/s41467-022-30829-z.
Formation of magnetic order alters the character of spin excitations, which then affects transport properties. We investigate the photoexcited ultrafast spin dynamics in different magnetic phases in Néel-type skyrmion host GaVS with time-resolved magneto-optical Kerr effect experiments. The coherent spin precession, whose amplitude is enhanced in the skyrmion-lattice phase, shows a signature of phase coexistence across the magnetic phase transitions. The incoherent spin relaxation dynamics slows down by a factor of two in the skyrmion-lattice/cycloid phases, indicating significant decrease in thermal conductivity triggered by a small change of magnetic field. The slow heat diffusion in the skyrmion-lattice/cycloid phases is attributed to the stronger magnon scattering off the domain walls formed in abundance in the skyrmion-lattice/cycloid phase. These results highlight the impact of spatial spin structure on the ultrafast heat transport in spin systems, providing a useful insight for the step toward ultrafast photocontrol of the magnets with novel spin orders.
磁序的形成改变了自旋激发的特性,进而影响输运性质。我们通过时间分辨磁光克尔效应实验,研究了尼尔型斯格明子宿主GaVS中不同磁相的光激发超快自旋动力学。相干自旋进动在斯格明子晶格相中其振幅增强,显示出跨磁相变的相共存特征。非相干自旋弛豫动力学在斯格明子晶格/摆线相减缓了两倍,表明由小磁场变化引发的热导率显著降低。斯格明子晶格/摆线相中的缓慢热扩散归因于在斯格明子晶格/摆线相中大量形成的畴壁上更强的磁振子散射。这些结果突出了空间自旋结构对自旋系统中超快热输运的影响,为迈向具有新型自旋序的磁体超快光控提供了有益的见解。