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arXiv 0909.5638cond-mat.stat-mech
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具有最近邻相互作用的球模型的微正则熵

Microcanonical entropy of the spherical model with nearest-neighbour interactions

Michael Kastner

摘要:

对于最近邻相互作用的球形模型,微正则熵s(e,m)是在热力学极限下对每个自旋的能量e和磁化强度m的所有可访问值进行解析计算的。熵函数被发现是凹的(尽管不是严格凹的),这意味着微正则和正则系综是等价的,尽管自旋必须服从球形约束的长程性质。两个过渡线被确定在(e,m)-平面,从铁磁和反铁磁分离顺磁相。将所得的微正则相图与更熟悉的正则相图进行比较。

英文摘要:

For the spherical model with nearest-neighbour interactions, the microcanonical entropy s(e,m) is computed analytically in the thermodynamic limit for all accessible values of the energy e and the magnetization m per spin. The entropy function is found to be concave (albeit not strictly concave), implying that the microcanonical and the canonical ensembles are equivalent, despite the long-range nature of the spherical constraint the spins have to obey. Two transition lines are identified in the (e,m)-plane, separating a paramagnetic phase from a ferromagnetic and an antiferromagnetic one. The resulting microcanonical phase diagram is compared to the more familiar canonical one.

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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