X-ray emission produced by interaction of slow highly charged \begin{document}${\boldsymbol{ {\rm{O}}^{q+}}}$\end{document} ions with Al surfaces

Author:

Zhang Bing-Zhang,Song Zhang-Yong,Liu Xuan,Qian Cheng,Fang Xing,Shao Cao-Jie,Wang Wei,Liu Jun-Liang,Xu Jun-Kui,Feng Yong,Zhu Zhi-Chao,Guo Yan-Ling,Chen Lin,Sun Liang-Ting,Yang Zhi-Hu,Yu De-Yang, , , ,

Abstract

<sec>The interaction of highly charged ions with solid surfaces is a very complex multi-body process. When the ions are close to the solid surfaces, the potential energy of the ions will be deposited in a tiny area of the target surfaces in a short time and then emitting X rays, which has important scientific significance and application in Astrophysics and plasma diagnosis. For experiments on the interaction of highly charged ions with surfaces, not only the X-ray energy spectrum but also the X-ray yield should be measured accurately. The precise measurement of the X-ray yield depends on the ability to accurately measure the beam-current intensity. In the past, the beam-current intensity was acquired by measuring the target current. Since the interaction between highly charged ions and solids involves the emission of secondary electrons, the actual measured target current is the sum of the initial beam-current intensity and the intensity caused by the secondary electrons, resulting in inaccurate X-ray yield calculations. In this experiment, a new analytical device, beam-current density meter, has been designed, which can measure the beam-current intensity with an accuracy of 0.1 nA. By measuring the current on the density meter instead of the target current, the influence of secondary electrons is almost avoided, and a more accurate X-ray yield is obtained.</sec><sec>This paper reports the characteristic X-ray spectra of oxygen atoms emitted from the interaction of 1.5–20 keV/<i>q</i> highly charged <inline-formula><tex-math id="M13">\begin{document}${\rm{O}} ^{q+} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M13.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M13.png"/></alternatives></inline-formula> ions with aluminum surfaces. For the X rays emitted by <inline-formula><tex-math id="M14">\begin{document}$ {\rm{O}}^{q+} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M14.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M14.png"/></alternatives></inline-formula>(<i>q</i> = 3, 5, 6) ions, the experimental results show that it is due to the close collisions with aluminum atoms after entering the surfaces, while the X rays emitted by <inline-formula><tex-math id="M15">\begin{document}${\rm{O}} ^{7+} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M15.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M15.png"/></alternatives></inline-formula> ions mainly come from the decay of hollow atoms. Under the condition of equal kinetic energy, the X-ray yield of <inline-formula><tex-math id="M16">\begin{document}${\rm{O}} ^{7+} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M16.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M16.png"/></alternatives></inline-formula> ions with K-shell vacancy is about one order of magnitude higher than that of <inline-formula><tex-math id="M17">\begin{document}$ {\rm{O}}^{q+} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M17.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M17.png"/></alternatives></inline-formula>(<i>q</i> = 3, 5, 6) ions, and X-ray yield of <inline-formula><tex-math id="M18">\begin{document}$ {\rm{O}}^{6+} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M18.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M18.png"/></alternatives></inline-formula> ions without<i> </i>K-shell vacancy is also significantly higher than that of <inline-formula><tex-math id="M19">\begin{document}${\rm{O}} ^{3+} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M19.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M19.png"/></alternatives></inline-formula> and <inline-formula><tex-math id="M20">\begin{document}$ {\rm{O}}^{5+} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M20.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M20.png"/></alternatives></inline-formula> ions. Generally, the X-ray yield and ionization cross-section is associated with the initial electron configuration of incident ions, and increases with the growth of ions kinetic energy. Based on the semi-classical approximation theory of binary collision, we have estimated the kinetic energy threshold for the emission of the K<sub>α</sub>-X rays of <inline-formula><tex-math id="M22">\begin{document}$ {\rm{O}}^{q+} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M22.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M22.png"/></alternatives></inline-formula>(<i>q</i> = 3, 5, 6) ions as interacting with the aluminum target. As the incident kinetic energy is lower than the kinetic energy threshold, for <inline-formula><tex-math id="M23">\begin{document}${\rm{O}} ^{6+} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M23.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="19-20210757_M23.png"/></alternatives></inline-formula> ions interacting with the sample, there may have a multi-electron excitation process that induces this K-electron ionization of the incident ions.</sec>

Publisher

Acta Physica Sinica, Chinese Physical Society and Institute of Physics, Chinese Academy of Sciences

Subject

General Physics and Astronomy

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3