|
|
|
High-precision calculations of highly excited and autoionizing states of the nickel atom |
| Sheng-Bo Niu(牛生波)1, Jun-Yao Zhang(张钧尧)2,3, Rui Jin(金锐)4,†, and Yi-Zhi Qu(屈一至)1,‡ |
1 School of Optoelectronics, University of Chinese Academy of Sciences, Beijing 100049, China; 2 National Key Laboratory of Particle Transport and Separation Technology, Tianjin 300180, China; 3 Research Institute of Physical and Chemical Engineering of Nuclear Industry, Tianjin 300180, China; 4 National Key Laboratory of Computational Physics, Institute of Applied Physics and Computational Mathematics, Beijing 100088, China |
|
|
|
|
Abstract High-precision atomic data, including highly excited energy levels and their lifetimes, as well as autoionizing states, are essential for astrophysics, materials science, and energy research applications. Despite the increasing demand for high-precision databases, the availability of data concerning complex transition-metal atoms remains limited. In this work, we present a systematic high-precision theoretical study of highly excited and autoionizing states of the nickel atom for $J^{\pi } = 4^{-}$ symmetry, considering the indispensable correlation effects between bound and continuum configurations. Calculations for discrete highly excited states and autoionizing states are conducted under the same theoretical scheme, which employs the relativistic multichannel theory (RMCT), to obtain an eigenchannel scattering matrix that varies smoothly over a wide energy region. The scattering matrix is then used with the multichannel quantum defect theory (MQDT) to semi-analytically obtain highly excited states and autoionizing states. Excellent agreement is achieved between the theoretical results and existing experimental discrete levels with a maximum of 0.02% deviation. An abnormal lifetime variation of the autoionizing states along the same series is observed. The resonance energy, lifetime, and assignment of autoionizing states are systematically presented for the first time, with the objective of contributing to the fields of astrophysics, materials science, and energy research. The datasets presented in this paper, including the energy levels and lifetimes of autoionizing states, are openly available at https://doi.org/10.57760/sciencedb.j00113.00279.
|
Received: 21 October 2025
Revised: 23 November 2025
Accepted manuscript online: 09 December 2025
|
|
PACS:
|
31.15.ae
|
(Electronic structure and bonding characteristics)
|
| |
31.15.ag
|
(Excitation energies and lifetimes; oscillator strengths)
|
| |
31.15.V-
|
(Electron correlation calculations for atoms, ions and molecules)
|
|
| Fund: R. J. is supported by the Young Scientists Fund of the National Natural Science Foundation of China (Grant No. 12404296) and the Original Exploration Program of the National Natural Science Foundation of China (Grant No. 12450404). Y.-Z. Qu is supported by the National Natural Science Foundation of China (Grant No. U2430208). |
Corresponding Authors:
Rui Jin, Yi-Zhi Qu
E-mail: jin_rui@iapcm.ac.cn;yzqu@ucas.ac.cn
|
Cite this article:
Sheng-Bo Niu(牛生波), Jun-Yao Zhang(张钧尧), Rui Jin(金锐), and Yi-Zhi Qu(屈一至) High-precision calculations of highly excited and autoionizing states of the nickel atom 2026 Chin. Phys. B 35 063101
|
[1] Seaton M J, Yan Y, Mihalas D and Pradhan A K 1994 Mon. Not. R. Astron. Soc. 266 805 [2] Bautista M A 1999 Astron. Astrophys. Suppl. Ser. 137 529 [3] Melendez M and Bautista M A 2005 Astron. Astrophys. 436 1123 [4] Lennard W N, Whaling W, Scalo J M and Testerman L 1975 Astrophys. J. 197 517 [5] Hillebrandt W and Niemeyer J C 2000 Annu. Rev. Astron. Astrophys. 38 191 [6] Jorissen A 2004 Phys. Scr. T112 73 [7] Mazzali P A, Ropke F K, Benetti S and Hillebrandt W 2007 Science 315 825 [8] Suzuki T, Honma M, Mao H, Otsuka T and Kajino T 2011 Phys. Rev. C 83 044619 [9] Shi X, Huang H, Jacobson B and Chang Y C 2012 Astrophys. J. 747 20 [10] Pain J C, Gilleron F and Comet M 2017 Atoms 5 22 [11] Watson W D 1969 Astrophys. J. 157 375 [12] Kessler T, Bruck K, Baktash C, Beene J R, Geppert C, Havener C C, Krause H F, Liu Y, Schultz D R and Stracener D W 2007 J. Phys. B: At. Mol. Opt. Phys. 40 4413 [13] Dawra D, Dimri M, Singh A K, Jha A K S, Pandey R K and Mohan M 2022 Eur. Phys. J. D 76 59 [14] Mou N, Zhang X, Lin Q, Yang X, Han L, Cao L and Yang D 2023 Nucl. Eng. Technol. 55 2139 [15] Gning M T and Sakho I 2024 Phys. Part. Nucl. Lett. 21 1014 [16] Sardar S, Bilal M, Bari M A, Nazir R T, Hannan A, Salahuddin M and Nasim M H 2016 Mon. Not. R. Astron. Soc. 458 1504 [17] Nahar S N and Bautista M A 2001 Astrophys. J. Suppl. Ser. 137 201 [18] Singh J, Jha A K S and Mohan M 2010 Astrophys. J. Suppl. Ser. 186 334 [19] Seaton M J 1966 Proc. Phys. Soc. 88 801 [20] Lu K T 1971 Phys. Rev. A 4 579 [21] Lee C M and Lu K T 1973 Phys. Rev. A 8 1241 [22] Lee C M 1974 Phys. Rev. A 10 584 [23] Jin R, Han X Y, Gao X and Li J M 2017 Sci. Rep. 7 11589 [24] Zou Y, Tong X M and Li J M 1995 Acta Phys. Sin. 44 50 (in Chinese) [25] Xiaomin T, Yu Z and Jiaming L 1995 Chin. Phys. Lett. 12 351 [26] Huang W, Zou Y, Tong X M and Li J M 1995 Phys. Rev. A 52 2770 [27] Aymar M, Greene C H and Luc-Koenig E 1996 Rev. Mod. Phys. 68 1015 [28] Zhang J Y, Xiong J Y, Zhou H R, Zhu C H, Sun H M, Wang L D, Chai J J and Li Y F 2025 Spectroc. Acta Pt. B-Atom. Spectr. 231 107249 [29] Zhang J Y, National Key Laboratory of Particle Transport and Separation Technology, Tianjin, Private Communication [30] Gao X and Li J M 2012 Chin. Phys. Lett. 29 033101 [31] Gao X, Jin R, Zeng D L, Han X Y, Yan J and Li J M 2015 Phys. Rev. A 92 052712 [32] Breit G and Wigner E 1936 Phys. Rev. 49 519 [33] Wigner E P 1955 Phys. Rev. 98 145 [34] Smith F T 1960 Phys. Rev. 118 349 [35] Bartschat K and Burke P G 1986 Comput. Phys. Commun. 41 75 [36] Peng Y L, Han X Y, Wang M S and Li J M 2005 J. Phys. B: At. Mol. Opt. Phys. 38 3825 [37] Quigley L and Berrington K 1996 J. Phys. B: At. Mol. Opt. Phys. 29 4529 [38] Quigley L, Berrington K and Pelan J 1998 Comput. Phys. Commun. 114 225 [39] Liu J, Niu Y F and Long W H 2025 Chin. Phys. C 49 064104 [40] Gu M F 2008 Can. J. Phys. 86 675 |
| No Suggested Reading articles found! |
|
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|
Cited |
|
|
|
|
Altmetric
|
|
blogs
Facebook pages
Wikipedia page
Google+ users
|
Online attention
Altmetric calculates a score based on the online attention an article receives. Each coloured thread in the circle represents a different type of online attention. The number in the centre is the Altmetric score. Social media and mainstream news media are the main sources that calculate the score. Reference managers such as Mendeley are also tracked but do not contribute to the score. Older articles often score higher because they have had more time to get noticed. To account for this, Altmetric has included the context data for other articles of a similar age.
View more on Altmetrics
|
|
|