A spectroscopic investigation of the lowest electronic states of the I2+ cation as a candidate for detecting the time variation of fundamental constants

Yujie Zhao, Yali Tian, Xiaohu He, Ting Gong, Xiaocong Sun, Guqing Guo, Xuanbing Qiu, Xiang Yuan*, Jinjun Liu, Lunhua Deng, Chuanliang Li

*Corresponding author for this work

Research output: Contribution to JournalArticleAcademicpeer-review

Abstract

The four lowest Ω substates (X2Π3/2,g, X2Π1/2,g, A2Π3/2,u and A2Π1/2,u) of the I2+ cation have been studied by high-precision ab initio calculations in comparison with experimental high-resolution absorption spectra. The potential energy curves were calculated using the multi-reference configuration interaction (MRCI) method and Dirac method, respectively. Rovibrational levels of these electronic states were derived by solving the radial Schrödinger rovibrational equation. Molecular constants were obtained in fitting energy levels to a spectroscopic model. Using the fit spectroscopic constants and newly calculated transition dipole moment matrix elements, line strengths of vibronic bands in the A2Π3/2,u- X2Π3/2,g system, as well as Einstein A coefficients for 45 of these bands with ν′ = 11–19 and ν′′ = 1–5, have been derived. The Einstein A coefficients were used to compute radiative lifetimes of the ν′ = 11–19 vibrational levels of the A2Π3/2,u state. Enhancement factors for detecting the variation of the fine-structure constant (α) and the proton-to-electron mass ratio(µ) using transitions between nearly degenerate rovibronic levels of these low-lying states have been calculated.

Original languageEnglish
Article number111873
Pages (from-to)1-8
Number of pages8
JournalJournal of Molecular Spectroscopy
Volume399
Early online date2 Jan 2024
DOIs
Publication statusPublished - Jan 2024

Bibliographical note

Publisher Copyright:
© 2024 Elsevier Inc.

Funding

We are indebted to Prof. Wenli Zou (Northwest University, China) for his help on ab initio. This work was supported by the National Natural Science Foundation of China (52076145 and 12304403), the National Key Research and Development Program of China (2023YFF0718100), Fund Program for the Scientific Activities of Selected Returned Overseas Professionals in Shanxi Province (20230031), Shanxi Scholarship Council of China (2023-151), Fundamental Research Program of Shanxi Province (202303021221147,202203021222204 & 202303021212224), Taiyuan University of Science and Technology Scientific Research Initial Funding (20222121), Shanxi Province Scientific Research Initial Funding (20232033). J.L. acknowledges financial support from the NSF under Grant No. CHE-1454825. We are indebted to Prof. Wenli Zou ( Northwest University , China) for his help on ab initio. This work was supported by the National Natural Science Foundation of China ( 52076145 and 12304403 ), the National Key Research and Development Program of China (2023YFF0718100), Fund Program for the Scientific Activities of Selected Returned Overseas Professionals in Shanxi Province (20230031), Shanxi Scholarship Council of China (2023-151), Fundamental Research Program of Shanxi Province (202303021221147,202203021222204 & 202303021212224), Taiyuan University of Science and Technology Scientific Research Initial Funding (20222121), Shanxi Province Scientific Research Initial Funding (20232033). J.L. acknowledges financial support from the NSF under Grant No. CHE-1454825.

FundersFunder number
Fundamental Research Program of Shanxi Province202303021212224, 202303021221147, 202203021222204
Selected Returned Overseas Professionals in Shanxi Province20230031
Shanxi Province Scientific Research Initial Funding20232033
Taiyuan University of Science and Technology Scientific Research Initial Funding20222121
National Science FoundationCHE-1454825
National Natural Science Foundation of China12304403, 52076145
Shanxi Scholarship Council of China2023-151
Northwest University China
National Key Research and Development Program of China2023YFF0718100

    Keywords

    • Ab initio calculation
    • Enhancement factors
    • I
    • Radiative lifetime

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