能量最小值和铁磁体的排序具有静态随机性
1Physics Department, Herbert H. Lehman College and Graduate School, The City University of New York, 250 Bedford Park Boulevard West, Bronx, NY 10468-1589, United States of America.
模拟显示,3D随机异构 (RA) 模型在温度下降时磁性顺序,这挑战了Imry-Ma论证. 然而,3D随机场 (RF) 模型会结到旋转玻璃状态,防止由于固定奇点而导致磁性排序.
科学领域:
- 凝聚物质物理学 凝聚物质物理学
- 统计力学就是统计力学.
- 计算物理学的计算物理.
背景情况:
- 伊姆里-马论据预测随机场 (RF) 和随机异构 (RA) 系统在有限维度下不应表现出长距离的磁顺序.
- 了解无序系统的磁性排序行为对于材料科学和凝聚物质物理学至关重要.
研究的目的:
- 为了研究2D和3D随机场和随机异构模型的磁顺序.
- 通过大规模的模拟来挑战或证实理论预测,特别是Imry-Ma论证.
主要方法:
- 在T=0凯尔文时,能量的最小化.
- 在高于0克尔文的温度下进行蒙特卡洛模拟.
- 在2D和3D网格中建模多达1.5亿个经典旋转.
主要成果:
- 3D RA模型在冷却时显示磁性排序,这与Imry-Ma的论证相矛盾.
- 在3D RA模型中,如果异构性超过交换相互作用,磁化就会减少,并出现一个旋转玻璃组件.
- 3D射频系统没有磁性顺序,而是由于固定奇点而结到相关的旋转玻璃状态.
结论:
- 在3D RA模型中,Imry-Ma论证对磁性排序的预测受到模拟结果的挑战.
- 奇点在防止3D射频系统中的磁性排序方面发挥着至关重要的作用.
- 具有竞争相互作用 (交换,随机场,异构) 的磁系统的行为是复杂的,取决于它们的相对强度.
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