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Updated: Jun 11, 2025

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Photoelectron Imaging of Anions Illustrated by 310 Nm Detachment of F−
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在真空中Ni V和Fe V的光谱紫外线
J W Ward1,2, A J J Raassen3, A Kramida1
1National Institute of Standards and Technology, Gaithersburg, MD 20899-8422, USA.
概括
这项研究重新测量了铁 (Fe V) 和 (Ni V) 离子的原子波长,提高了数据的准确性. 这些增强的测量解决了白矮星观测中的不一致性,有助于测试细结构常数.
科学领域:
- 原子物理 原子物理
- 天体物理学 天体物理学
- 频谱学是一种光谱学.
背景情况:
- 准确的原子数据对于天体物理观测至关重要.
- 以前的Ni V () 和Fe V (铁) 波长数据存在不确定性,影响了白矮星研究.
- 像G191-B2B这样的白矮星被用来探测基本物理常数.
研究的目的:
- 重新测量和提高Fe V和Ni V原子波长的准确性.
- 为了纠正现有的Ni V数据中的系统校准错误.
- 为Ni V.提供一个优化的能量水平数据集.
主要方法:
- 在1200-1600 Å范围内对Fe V和Ni V光谱线进行实验性重新测量.
- 在Ni V波长中识别和纠正校准错误.
- 使用Ritz波长为Ni V. 的能量水平优化.
主要成果:
- 97 Fe V 和 123 Ni V 波长重新测量,不确定性约为 2 m.
- 额外的FeV和NiV波长报告的不确定性>2 mÅ.
- 在之前的Ni V波长中发现并纠正了一个系统错误.
结论:
- 改进的Fe V和Ni V实验室波长增强了天体物理学观测.
- 修正后的数据解决了微观结构常数在白矮星研究中的不一致性.
- 这项工作为在极端环境中探测基本物理提供了更可靠的数据集.
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