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    Observation of QED Effects, Breit Interaction, and Electron Correlation in Highly Charged Au Ions Produced by a High-Power Laser

    Bubo Ma1,2,*, Jieru Ren1,*,†, Shaoyi Wang3,*, Shizheng Zhang1, Ziqian Zhao1, Xuyang Luo1, Mingzhe Yang1, Wenqing Wei1, Wen Jiang1 et al.

    Xing Wang1, Yifang Gao1, Dieter H. H. Hoffmann1, Zhongfeng Xu1, Jianxing Li1, Xueguang Ren1, Quanping Fan3, Zhigang Deng3, Wei Qi3, Bo Cui3, Yuchi Wu3, Zhurong Cao3, Zongqing Zhao3, Yuqiu Gu3, Guoqing Zhang4, Chenzhong Dong4, Leifeng Cao5, Rui Cheng6, Shaoping Zhu3,7, Weimin Zhou3,‡, Luyou Xie4,§, and Yongtao Zhao1,∥

    • *These authors contributed equally to this work.
    • †Contact author: renjieru@xjtu.edu.cn
    • ‡Contact author: zhouwm@caep.cn
    • §Contact author: xiely@nwnu.edu.cn
    • ∥Contact author: zhaoyongtao@xjtu.edu.cn

    Phys. Rev. Lett. 136, 143201 – Published 10 April, 2026

    DOI: https://doi.org/10.1103/6qn5-7rm8

    Abstract

    We report on measurements of extreme ultraviolet (EUV) radiation from highly charged gold ions in laser-produced plasma to investigate the quantum electrodynamics (QED) effects, Breit interaction, and electron correlation (EC) effects which play a crucial role in determining the energy levels of high-Z, highly charged ions. Specifically, we analyze emission lines from the 4s  S21/2−4p  P21/2 and 4d  D23/2−4f  F25/2 transitions in Cu-like Au ions (Au50+), where the ground state consists of a filled M-shell and a single 4s electron in the outermost shell. Utilizing the multiconfiguration Dirac-Hartree-Fock (MCDHF) method, we systematically calculated the energy levels and transition wavelengths. Our results show that only when QED effects, Breit interaction, finite nuclear size (FNS) corrections, and EC effects with sufficient electron configurations are included do the theoretical predictions align with experimental observations. By combining state-of-the-art experiments with high-precision computations, we resolve the long-standing discrepancies in the spectrum of Cu-like Au ions, providing the first quantitative delineation of QED effects, Breit interaction, FNS corrections, and EC effects on its energy levels. Our methodology is directly applicable to other highly charged ions, which are crucial for modeling astrophysical and laboratory plasmas.

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