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arXiv 2004.11591cond-mat.str-el
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磁电材料Sr $_3$ Co PDMATHAAB Fe $_{24}$ O $_{41}$的磁畴和磁泡结构观察

Observation of magnetic domain and bubble structures in magnetoelectric Sr$_3$Co$_2$Fe$_{24}$O$_{41}$

H. Nakajima, H. Kawase, K. Kurushima, A. Kotani, T. Kimura, S. Mori

摘要:

用Lorentz显微镜研究了Z型六角铁氧体Sr $_3$ Co $_2$ Fe $_{24}$ O $_{41}$中的磁畴和磁泡结构。这种六角铁氧体表现出室温磁电效应,这归因于其横向锥形自旋结构(TC相)。在加热时,TC相转变成亚铁磁相,其在六方$ab$平面中的磁矩在410和480 K之间(FM 2相),并且转变成另一亚铁磁相,其磁矩平行于$c$轴,在490和680 K之间(FM 1相)。因此,在本研究中,观察到Sr $_3$ Co $_2$ Fe $_{24}$ O $_{41}$中的磁畴结构随温度显著变化。在TC相中,在将样品从FM2冷却到TC相后观察到不规则的精细磁畴。在FM 1相中,形成了平行于$c$轴的条纹状磁畴壁,其具有亮暗对比度对。在施加外部磁场时,条纹状磁畴壁转变成磁泡。磁泡的拓扑结构取决于外磁场($H$)方向和易磁化$c$轴之间的角度。即,对于$H//c$,生成拓扑数$N$ = 1(I型)的磁泡,而当磁场从c轴倾斜5°时,生成拓扑数$N$ = 0(II型)的磁泡。我们将Sr $_3$ Co $_2$ Fe $_{24}$ O $_{41}$的高磁晶各向异性归因于FM 1相中磁泡的出现。

英文摘要:

The magnetic domain and bubble structures in the Z-type hexaferrite Sr$_3$Co$_2$Fe$_{24}$O$_{41}$ were investigated using Lorentz microscopy. This hexaferrite exhibits a room-temperature magnetoelectric effect that is attributed to its transverse conical spin structure (TC phase). Upon heating, the TC phase transforms into a ferrimagnetic phase with magnetic moments in the hexagonal $ab$ plane between 410 and 480 K (FM2 phase) and into another ferrimagnetic phase with moments parallel to the $c$ axis between 490 and 680 K (FM1 phase). Accordingly, in this study, the magnetic domain structures in Sr$_3$Co$_2$Fe$_{24}$O$_{41}$ were observed to change dramatically with temperature. In the TC phase, irregular fine magnetic domains were observed after cooling the specimen from the FM2 to TC phase. In the FM1 phase, striped magnetic domain walls with pairs of bright and dark contrast were formed parallel to the $c$ axis. Upon applying an external magnetic field, the striped magnetic domain walls transformed into magnetic bubbles. The topology of the magnetic bubbles was dependent on the angle between the external magnetic field ($H$) direction and the easy $c$ axis. Namely, magnetic bubbles with the topological number $N$ = 1 (type I) were created for $H//c$, whereas magnetic bubbles with $N$ = 0 (type II) were created when the magnetic field was tilted from the c axis by 5°. We attribute the high magnetocrystalline anisotropy of Sr$_3$Co$_2$Fe$_{24}$O$_{41}$ to the emergence of magnetic bubbles in the FM1 phase.

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