驱动居里-魏斯模型的比热

Elena Rufeil Fiori, Christian Maes, Robbe Vidts
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引用次数: 0

摘要

在标准铁磁库里-韦斯模型中应用时周期磁场会使自旋系统处于稳定的失衡状态。我们回顾了磁滞如何受到磁场振幅和频率的影响,以及如何辨别与振幅和频率相关的(动态)临界温度。耗散功率测量磁滞环的面积,并随温度变化。多余的热量决定了非平衡比热,从而产生准静态响应。我们计算的比热似乎在临界温度时出现了发散,这与平衡情况截然不同。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Specific heat of the driven Curie-Weiss model
Applying a time-periodic magnetic field to the standard ferromagnetic Curie-Weiss model brings the spin system in a steady out-of-equilibrium condition. We recall how the hysteresis gets influenced by the amplitude and the frequency of that field, and how an amplitude- and frequency-dependent (dynamical) critical temperature can be discerned. The dissipated power measures the area of the hysteresis loop and changes with temperature. The excess heat determines a nonequilibrium specific heat giving the quasistatic response. We compute that specific heat, which appears to diverge at the critical temperature, quite different from the equilibrium case.
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