London Centre for Nanotechnology and Department of Physics and Astronomy, University College London, London, UK.
J Phys Condens Matter. 2011 Mar 23;23(11):112201. doi: 10.1088/0953-8984/23/11/112201. Epub 2011 Feb 28.
Dimensional analysis is shown to give an insight into the non-ergodic behaviour of spin ice below its apparent 'spin freezing' temperature. Expressions are derived for the temperature-dependent magnetic susceptibility that are found to be highly consistent with the previously reported field cooled and zero field cooled magnetization of the spin ice dysprosium titanate, Dy(2)Ti(2)O(7), as well as with the theory of a 'magnetolyte', including Debye-Hückel screening and Wien dissociation. The spin freezing is inferred to reflect the inability of the quasi-free magnetic charges or 'monopoles' that comprise the magnetolyte to fully screen an applied magnetic field on the timescale of an experiment. The apparent freezing temperature (T(f)≈0.65 K) is identified as the point where the Debye screening length becomes greater than the Bjerrum association distance for charge pairs. Combining these dimensional arguments with Onsager's theory of the Wien effect, it is shown that magnetization data at relatively high field (Snyder et al 2004 Phys. Rev. B 69 064414) may be used to estimate the elementary magnetic charge of spin ice, as well as the temperature-dependent monopole density. Evidence is presented of a non-equilibrium population of monopoles below T≈0.2 K. It is also shown how Onsager's microscopic theory of field-induced monopole pair separation naturally suggests the 'magnetization jumps' in Dy(2)Ti(2)O(7) observed at applied fields of the order of ∼ 0.1 T. It is concluded that the results of dimensional analysis, when combined with Onsager's theory, provide an accurate, albeit approximate, description of the properties of Dy(2)Ti(2)O(7), that could be improved by the development of a lattice theory of the Wien effect, or tested on other spin ice materials.
维度分析表明,在自旋冰的表观“自旋冻结”温度以下,它可以深入了解非遍历行为。推导出了与温度有关的磁化率表达式,这些表达式与先前报道的自旋冰钇钛酸镝 Dy(2)Ti(2)O(7)的场冷却和零场冷却磁化率非常一致,也与“磁体液”理论一致,包括德拜-休克尔屏蔽和维恩离解。自旋冻结被推断为反映了构成磁体液的准自由磁荷或“磁单极子”在实验时间尺度上无法完全屏蔽外加磁场。表观冻结温度(T(f)≈0.65 K)被确定为德拜屏蔽长度大于电荷对的贝杰龙缔合距离的点。将这些维度论点与 Onsager 的维恩效应理论结合起来,可以表明在相对较高的磁场下(Snyder 等人,2004 年,Phys. Rev. B 69 064414)的磁化率数据可用于估计自旋冰的基本磁荷以及与温度有关的磁单极密度。提出了在 T≈0.2 K 以下存在磁单极子的非平衡分布的证据。还表明,Onsager 的微观理论如何自然地表明在施加约 0.1 T 的磁场时,Dy(2)Ti(2)O(7)中观察到的“磁化跳跃”。结论是,维度分析的结果与 Onsager 的理论相结合,提供了对 Dy(2)Ti(2)O(7)性质的准确但近似的描述,如果开发出维恩效应的晶格理论,或者在其他自旋冰材料上进行测试,该描述可以得到改进。