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    Polarization of x-rays emitted in radiative recombination into bare ions: Role of spin-flip transitions

    Tianluo Luo1, Zhencen He2,1, Zhihao Yang3, Yunping Wang1, Stephan Fritzsche4,5,6, Xiang Gao7,8,*, and Zhimin Hu1,†

    • *Contact author: xgao@csrc.ac.cn
    • †Contact author: huzhimin@scu.edu.cn

    Phys. Rev. A 113, 012826 – Published 29 January, 2026

    DOI: https://doi.org/10.1103/dkmt-wct6

    Abstract

    Systematic theoretical calculations on the polarization properties of x-rays emitted in K-shell radiative recombination (RR) into bare ions are carried out, with particular emphasis on the role of spin-flip transitions in Kr36+, Sn50+, W74+, and Bi83+ ions. The calculated linear polarization of K-shell RR x-rays from bare Kr36+ ions with spin-flip contribution shows good agreement with previous measurement performed at the Tokyo electron-beam ion trap [Rev. Sci. Instrum. 92, 063101 (2021)], demonstrating the necessity of accounting for spin-flip contributions to the angle-differential cross sections. This agreement provides clear identification of spin-flip contribution to the polarization of RR x-rays for the lightest bare ions studied so far. In addition, we show that spin-flip contribution to the linear polarization of the K-shell RR x-rays increases significantly with both incident electron energy and atomic number Z. This trend suggests that further measurements of the linear polarization of K-shell RR x-rays by varying the electron energy and atomic number Z may offer enhanced sensitivity to spin-flip transitions.

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