硅l -壳层离子的相对论mr-mp能级。

IF 8.6 1区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Astrophysical Journal Supplement Series Pub Date : 2018-01-01 Epub Date: 2018-01-15 DOI:10.3847/1538-4365/aa94d2
Juan A Santana, Nahyr A Lopez-Dauphin, Peter Beiersdorfer
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引用次数: 4

摘要

用相对论的多参考Møller-Plesset微扰理论方法计算了其能量,包括了nl到5f的价态和k空位态。通过与美国国家标准与技术研究院(NIST)在线数据库中列出的推荐数据进行比较,确定了计算能级能的准确性。价能级能的平均偏差在Si V的0.20 eV到Si XII的0.04 eV之间。对于k -空位态,NIST数据库中推荐的可用值仅限于Si XII和Si XIII。k空位态的平均能量偏差小于0.3 eV。这里提供的广泛而准确的数据集大大增加了可用参考能级能量的数量。我们希望我们的数据能够简化天体源和实验室产生的等离子体中Si的l -壳离子的线识别,并在缺乏更精确的实验室测量时作为能量参考。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

RELATIVISTIC MR-MP ENERGY LEVELS FOR L-SHELL IONS OF SILICON.

RELATIVISTIC MR-MP ENERGY LEVELS FOR L-SHELL IONS OF SILICON.

RELATIVISTIC MR-MP ENERGY LEVELS FOR L-SHELL IONS OF SILICON.

Level energies are reported for Si V, Si VI, Si VII, Si VIII, Si IX, Si X, Si XI and Si XII. The energies have been calculated with the relativistic Multi-Reference Møller-Plesset Perturbation Theory method and include valence and K-vacancy states with nl up to 5f. The accuracy of the calculated level energies is established by comparison with the recommended data listed in the National Institute of Standards and Technology (NIST) on-line database. The average deviation of valence level energies ranges from 0.20 eV in Si V to 0.04 eV in Si XII. For K-vacancy states, the available values recommended in the NIST database are limited to Si XII and Si XIII. The average energy deviation is below 0.3 eV for K-vacancy states. The extensive and accurate dataset presented here greatly augments the amount of available reference level energies. We expect our data to ease the line identification of L-shell ions of Si in celestial sources and laboratory generated plasmas, and to serve as energy references in the absence of more accurate laboratory measurements.

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来源期刊
Astrophysical Journal Supplement Series
Astrophysical Journal Supplement Series 地学天文-天文与天体物理
CiteScore
14.50
自引率
5.70%
发文量
264
审稿时长
2 months
期刊介绍: The Astrophysical Journal Supplement (ApJS) serves as an open-access journal that publishes significant articles featuring extensive data or calculations in the field of astrophysics. It also facilitates Special Issues, presenting thematically related papers simultaneously in a single volume.
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