纯自旋系统中的姆佩姆巴效应:空间相关性在初始状态中的作用的普遍图像
Sohini Chatterjee1, Soumik Ghosh1, Nalina Vadakkayil1,2
1Theoretical Sciences Unit and School of Advanced Materials, <a href="https://ror.org/0538gdx71">Jawaharlal Nehru Centre for Advanced Scientific Research</a>, Jakkur P.O., Bangalore 560064, India.
Physical review. E
|August 20, 2024
概括
较热的磁系统比较冷的系统冷却速度更快,在磁相转换中表现出Mpemba效应 (ME). 这种在模拟中观察到的偏磁体中更快的排序,为ME现象提供了洞察力.
科学领域:
- 物理 物理学 物理
- 凝聚物质物理学 凝聚物质物理学
- 统计力学 统计力学
背景情况:
- 姆佩巴效应 (ME) 描述了反直觉的现象,即热水比冷水更快地结.
- 最近的努力探索了水以外的各种物理系统中的ME.
- 了解ME的潜在机制是一个持续的科学挑战.
研究的目的:
- 在磁相转换的背景下研究Mpemba效应.
- 为了确定更热的磁体系统是否比较冷的磁体系统更快地排序.
- 探索 ME 对不同模型系统的普遍适用性.
主要方法:
- 在Ising和q-state Potts模型中使用蒙特卡洛模拟.
- 模拟中的各种交互范围和空间维度.
- 分析了在低于基里点的温度灭后的能量衰变和有序增长.
主要成果:
- 证实,更热的偏磁铁比较冷的偏磁铁更快地经历铁磁性排序.
- 在不同的模型中观察到这种效应一致,没有丧.
- 确定了ME强度和初始空间相关性之间的缩放关系.
结论:
- 姆佩姆巴效应可以表现为磁性相位过渡,更热的系统订购速度更快.
- 观察到的现象是一般的,并且独立于顺序-参数波动或过渡顺序.
- 这些发现有助于更广泛地了解不同物理系统中Mpemba效应.
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