arXivDaily arXiv每日学术速递 周一至周五更新
北美退伍军人节(Veterans Day),12 日无更新
arXiv 0707.3477cond-mat.stat-mech
收藏

Dy2Ti2O7自旋冰:受抑磁体中涌现星系团的一个试验事例

Dy2Ti2O7 Spin Ice: a Test Case for Emergent Clusters in a Frustrated Magnet

Taras Yavors'kii, Tom Fennell, Michel J. P. Gingras, Steven T. Bramwell

摘要:

Dy2Ti2O7是一种几何阻挫磁性材料,具有从1 K延伸到低至60 mK的强相关自旋冰制度。在自旋冰制度的扩散弹性中子散射强度可以很好地描述弱相互作用的六角形自旋团簇的现象学模型,调用在其他几何挫折磁铁。我们提出了一个高度精炼的微观理论Dy2Ti2O7,包括远程偶极和交换相互作用的第三近邻,这表明,集群是纯粹虚构的这种材料。复合自旋团簇及其相关散射模式的出现,实际上是强关联状态下辅助关联微调的一个指标。

英文摘要:

Dy2Ti2O7 is a geometrically frustrated magnetic material with a strongly correlated spin ice regime that extends from 1 K down to as low as 60 mK. The diffuse elastic neutron scattering intensities in the spin ice regime can be remarkably well described by a phenomenological model of weakly interacting hexagonal spin clusters, as invoked in other geometrically frustrated magnets. We present a highly refined microscopic theory of Dy2Ti2O7 that includes long-range dipolar and exchange interactions to third nearest neighbors and which demonstrates that the clusters are purely fictitious in this material. The seeming emergence of composite spin clusters and their associated scattering pattern is instead an indicator of fine-tuning of ancillary correlations within a strongly correlated state.

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。

↑