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arXiv 1102.3524cond-mat.str-el
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B20螺旋磁网络中的A相起源

A-phase origin in B20 helimagnets

S. V. Maleyev

摘要:

本文解释了立方螺旋磁体($M n S i,F e G e$等)中A相的起源。结果表明,它的上界是自旋波不稳定性在$H_\perp>\sqrt{8/3}Δ=H_{A2}$的结果,其中$H_\perp$是垂直于螺旋轴的磁场,$\m k$和$Δ$分别是自旋波带隙.如果考虑到Dzyaloshinskiii-Moriya相互作用在不同自旋之间的作用,最后一个出现是由于自旋波相互作用。在$H_\perp\to H_{A2}$的磁能的1/S系列中的红外发散(IRD)负责较低的A相边界$H_{A1}$。结果表明,在所有的$T<T_C$上都存在A相,但在$T\ll T_C$上A相很窄,无法观察到。而在$T_C$之下的临界区,其宽度强烈增加。初步估计表明与现有的实验数据半定量协议。自旋波带隙的存在是我们考虑的一个关键点。在附录A中,我们以比以前的出版物更透明的形式介绍了它的推导。

英文摘要:

A-phase origin in cubic helimagnets ($M n S i,F e G e$ etc) is explained. It is shown that its upper bound is a result of the spin-wave instability at $H_\perp>\sqrt{8/3}Δ=H_{A2}$ where $H_\perp$ are the magnetic field perpendicular to the helix axis $\m k$ and $Δ$ the spin-wave gap respectively. The last appears due to the spin-wave interaction if one takes into account that the Dzyaloshinskii-Moriya interaction acts between different spins. The infra-red divergences (IRD) in the 1/S series for the magnetic energy at $H_\perp\to H_{A2}$ are responsible for the lower A-phase boundary $H_{A1}$. It is shown that the A-phase exists at all $T<T_C$ but if $T\ll T_C$ it is very narrow and can not be observed. However in the critical region just below $T_C$ its width increasing strongly. Preliminary estimations demonstrate semi-quantitative agreement with the existing experimental data. The existence of the spin-wave gap is a crucial point of our consideration. In Appendix A we present its derivation in more transparent form than in previous publication.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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