# Production and decay of K-shell hollow krypton in collisions with 52 -   197 MeV/u bare xenon ions

**Authors:** Caojie Shao, Deyang Yu, Xiaohong Cai, Xi Chen, Kun Ma, Jarah Evslin,, Yingli Xue, Wei Wang, Yury. S. Kozhedub, Rongchun Lu, Zhangyong Song, Mingwu, Zhang, Junliang Liu, Bian Yang, Yipan Guo, Jianming Zhang, Fangfang Ruan,, Yehong Wu, Yuezhao Zhang, Chenzhong Dong, Ximeng Chen, and Zhihu Yang

arXiv: 1706.03460 · 2017-09-13

## TL;DR

This study measures X-ray spectra of K-shell hollow krypton atoms produced in collisions with high-energy xenon ions, revealing energy shifts, vacancy ratios, and comparing results with relativistic calculations.

## Contribution

It provides the first detailed measurements of K-shell hollow krypton atom spectra in heavy-ion collisions and compares experimental data with advanced theoretical models.

## Key findings

- Energy shifts of X-ray transitions are quantified.
- The ratio of hollow to singly ionized krypton atoms is 14-24%.
- Experimental results align with relativistic coupled channel calculations.

## Abstract

X-ray spectra of K-shell hollow krypton atoms produced in single collisions with 52 - 197 MeV/u Xe54+ ions are measured in a heavy-ion storage ring equipped with an internal gas-jet target. Energy shifts of the K{\alpha}_1,2^s, K{\alpha}_1,2^(h,s), and K\b{eta}_1,3^s transitions are obtained. Thus, the average number of the spectator L-vacancies presented during the x-ray emission is deduced. From the relative intensities of the K{\alpha}_1,2^s and K{\alpha}_1,2^(h,s) transitions, the ratio of K-shell hollow krypton to singly K-shell ionized atoms is determined to be 14 - 24%. In the considered collisions, the K-vacancies are mainly created by the direct ionization which cannot be calculated within the perturbation descriptions. The experimental results are compared with a relativistic coupled channel calculation performed within the independent particle approximation.

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Source: https://tomesphere.com/paper/1706.03460