在周期表中对原子轨道的相对论效应:从自旋分离的迪拉克-库伦布-布莱特哈密尔顿的洞察力
Chad E Hoyer1, Kailey E Holen1
1Department of Chemistry and Biochemistry, University of Texas at El Paso, El Paso, Texas 79968, USA. cehoyer@utep.edu.
Physical chemistry chemical physics : PCCP
|February 17, 2026
概括
相对论的哈密尔顿理论显著改变了重元素的轨道能量. 迪拉克 - 库伦 (DC),迪拉克 - 库伦 - 盖恩特 (DCG) 和迪拉克 - 库伦 - 布莱特 (DCB) 的哈密尔顿之间的替换会导致大的转移,特别是在核心轨道上.
科学领域:
- 量子化学 是一个量子化学.
- 原子物理 原子物理
- 计算化学的计算化学
背景情况:
- 相对论效应对于准确描述重元素至关重要.
- 不同的相对论汉密尔顿 (DC,DCG,DCB) 以不同的精度近似这些效应.
- 了解哈密尔顿引发的轨道属性的变化是理论预测的关键.
研究的目的:
- 为了研究不同相对论哈密尔顿对原子轨道特征的影响.
- 量化能量转移和占有轨道的辐射性质的变化.
- 在相对论计算中识别潜在的错误取消.
主要方法:
- 使用自旋分离的狄拉克-库伦 (DC),狄拉克-库伦-格昂特 (DCG) 和狄拉克-库伦-布莱特 (DCB) 哈密尔顿.
- 计算的轨道能量,辐射期望值和辐射分布函数.
- 分析了周期表不同块的重元素.
主要成果:
- 哈密尔顿置换 (X2C到DC,DC到DCG) 导致重元素轨道的能量转移大 (>0.1 eV).
- DCG与DCB的替换显著影响了深层到浅核轨道能量.
- 没有观察到辐射预期值或分布函数的显著变化 (>0.01 bohr).
结论:
- 相对论的哈密尔顿选择对轨道能量产生了关键的影响,即使对于标量-相对论近似值.
- 对于f轨道,确定了一个潜在的错误取消机制.
- 辐射属性对研究的哈密尔顿变化基本上没有敏感性.
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