|
|
|
Spectroscopic study of odd-parity excited levels of atomic gadolinium in the 28700-31500 cm-1 region using a three-color three-step resonance ionization pathway |
| Jun-Yao Zhang(张钧尧)1,2,3, Kai-Chen Ma(马恺宸)2, Jing-Yi Xiong(熊静逸)2, Li-De Wang(王立德)1,2,3, Cai-Hua Zhu(朱才华)2, Jun-Jie Chai(柴俊杰)1,2,3, and Yun-Fei Li(李云飞)1,2,† |
1 National Key Laboratory of Particle Transport and Separation Technology, Tianjin 300180, China; 2 Research Institute of Physical and Chemical Engineering of Nuclear Industry, Tianjin 300180, China; 3 Tianjin Key Laboratory of Stable Isotope Materials Technology, Tianjin 300180, China |
|
|
|
|
Abstract The three-color, three-step resonance ionization spectroscopy technique was employed to investigate the odd-parity excited states of gadolinium in the 28700-31500 cm$^{-1}$ energy region. Spectra scanned without $\lambda _1$ led to the identification of 101 interference peaks, which were excluded from subsequent studies. A total of 40 odd-parity excited states were observed from scans of nine even-parity lower levels, including 19 states reported here for the first time. Unique $J$ values were assigned to 39 levels using the electric dipole selection rule. Comparison with previous studies confirms the reliability of the present results, with the absolute energy accuracy estimated to be better than $\pm 0.1$ cm$^{-1}$.
|
Received: 06 September 2025
Revised: 10 October 2025
Accepted manuscript online: 14 October 2025
|
|
PACS:
|
32.80.Zb
|
(Autoionization)
|
| |
82.80.Ms
|
(Mass spectrometry (including SIMS, multiphoton ionization and resonance ionization mass spectrometry, MALDI))
|
| |
42.55.Mv
|
(Dye lasers)
|
|
| Fund: This research was supported by the Tianjin Science and Technology Program Project (No. 24ZXZSSS00530). |
Corresponding Authors:
Yun-Fei Li
E-mail: Ipce_liyf@mails.cneic.com.cn
|
Cite this article:
Jun-Yao Zhang(张钧尧), Kai-Chen Ma(马恺宸), Jing-Yi Xiong(熊静逸), Li-De Wang(王立德), Cai-Hua Zhu(朱才华), Jun-Jie Chai(柴俊杰), and Yun-Fei Li(李云飞) Spectroscopic study of odd-parity excited levels of atomic gadolinium in the 28700-31500 cm-1 region using a three-color three-step resonance ionization pathway 2026 Chin. Phys. B 35 073201
|
[1] Peper M, Li Y, Knapp D Y, Bileska M, Ma S, Liu G, Peng P, Zhang B, Horvath S P, Burgers A P and Thompson J D 2025 Phys. Rev. X 15 011009 [2] Hovhannesyan G and Lepers M 2023 Phys. Scr. 98 025407 [3] Klempka M, Elantkowska M, Furmann B, Ruczkowski J, Głowacki P, Mieloch S and Stefańska D 2025 J. Quant. Spectrosc. Radiat. Transf. 347 109632 [4] Sahoo A C, Mandal P K, Mukherjee J, Dev V and Shah M L 2022 J. Quant. Spectrosc. Radiat. Transf. 292 108352 [5] D’yachkov A B, Gorkunov A A, Labozin A V, Mironov S M, Firsov V A, Tsvetkov G O and Panchenko V Ya 2023 Bull. Lebedev Phys. Inst. 50 S187 [6] Fujiwara T, Kobayashi T and Midorikawa K 2019 Sci. Rep. 9 1754 [7] Luck R E, Kovtyukh V V and Andrievsky S M 2006 Astron. J. 132 902 [8] Nahar S N and Hinojosa-Aguirre G 2024 Atoms 12 22 [9] Guiglion G, De Laverny P, Recio-Blanco A and Prantzos N 2018 Astron. Astrophys. 619 A143 [10] Nahar S N 2024 Atoms 12 24 [11] Mishenina T, Pignatari M, Gorbaneva T, Cote B, Lopez A Y, Thielemann F K and Soubiran C 2022 Mon. Not. Roy. Astron. Soc. 516 3786 [12] Den Hartog E A, Lawler J E, Sneden C and Cowan J J 2006 Astrophys. J. Suppl. Ser. 167 292 [13] Spina L, Meléndez J, Karakas A I, Santos L D, Bedell M, Asplund M, Ramírez I, Yong D, Alves-Brito A, Bean J L and Dreizler S 2017 Mon. Not. Roy. Astron. Soc. 474 2580 [14] Niki H, Motoki K, Yasui M, Horiuchi Y, Tokita S and Izawa Y 2006 J. Nucl. Sci. Technol. 43 427 [15] Sankari M and Suryanarayana M V 2015 J. Nucl. Eng. Radiat. Sci. 1 041017 [16] Sankari M, Suryanarayana M V and Gangadharan S 1999 J. Nucl. Mater. 264 122 [17] Van Kleef Th A M, Blaise J andWyart J F 1971 J. Phys. France 32 609 [18] Qu J N, Zhou Z Y, Zhu L Z, Lin F C 1991 Chin. J. Lasers 18 659 [19] Miyabe M, Wakaida I and Arisawa T 1996 J. Phys. B: At. Mol. Opt. Phys. 29 4073 [20] Miyabe M, Oba M and Wakaida I 1998 J. Phys. B: At. Mol. Opt. Phys. 31 4559 [21] Jim-Tae K, Jonghong Y, Yongjoo R, Jongmin L 2000 J. Korean Phys. Soc. 37 701 [22] Zhang J Y, Xiong J Y, Wei S Q, Li Y F and Lu X Y 2023 Acta Phys. Sin. 72 193203 (in Chinese) [23] Zhang J Y, Lu X Y, Li Y F and Chai J J 2024 Eur. Phys. J. D 78 95 [24] 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 [25] Miyabe M andWakaida I 1997 J. Phys. B: At. Mol. Opt. Phys. 30 4193 [26] Miyabe M,Wakaida I and Arisawa T 1997 Z. Phys. D-Atoms Mol. Clusters 39 181 [27] Kramida A, Ralchenko Yu, Reader J, NIST ASD Team 2024 NIST Atomic Spectra Database (ver. 5.12) [Online]. 2025, Gaithersburg, MD: National Institute of Standards and Technology. DOI: 10.18434/T4W30F [28] Zhang Z M, Wang Z C, Wang Q L, Ma X K, Wang Z X, Hua Z X, Yao G X, Yang X Y, Sun Z F, Qin Z B and Zheng X F 2024 J. Chem. Phys. 160 164201 [29] Elizarov A Y and Tupitsyn I I 2007 J. Phys. B: At. Mol. Opt. Phys. 40 1991 [30] Yar A, Ali R and Baig M A 2013 Phys. Rev. A 88 033405 |
| 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
|
|
|