频谱形状因子的冷却性质
Dimitrios Charamis1,2, Manas Kulkarni3, Jorge Kurchan2
1Université Paris Saclay, CEA, CNRS, IPhT, 91191 Gif-sur-Yvette, France.
Physical review. E
|February 20, 2026
概括
灭的光谱形状因子 (SFF) 不具有自我平均值,与其化对应物不同. 它的平均值和波动与冈贝尔分布保持一致,即使对于非赫密斯系统.
科学领域:
- 这是量子混沌.
- 统计力学 统计力学
- 随机矩阵理论 随机矩阵理论
背景情况:
- 光谱形状因子 (SFF) 描述了量子系统中的光谱统计.
- 对于赫密斯矩阵和非赫密斯矩阵,SFF的概括存在.
- 众所周知,SFF不是自我平均值.
研究的目的:
- 调查灭的SFF的属性,特别是它的对数和平均值.
- 将灭的SFF与其化对应物进行比较.
- 在晚期分析灭的SFF的波动.
主要方法:
- 研究了灭的SFF的平均值和对数.
- 对比了SFF的和冷平均值及其对数.
- 使用与冈贝尔分布相容的变量转换分析了SFF波动.
- 检查了分区函数的费舍尔零.
主要成果:
- 灭的SFF对赫密特和非赫密特病例都有自我平均值.
- 在高温下,SFF的冷却和冷却平均值与下载常数一致.
- 灭的SFF对数的波动很深,在分区函数的零点附近呈现尖峰.
- 灭的SFF对数的变量转换与冈贝尔分布相容.
结论:
- 冈贝尔分布的指数尾随是来自灭的SFF的深尖 (费舍尔零) 的采样.
- 这些发现适用于非赫密斯汉密尔顿和随机矩阵,扩展了以前的结果.
- 这项研究提供了对复杂量子系统的光谱统计的见解.
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