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氮元素是宇宙中丰度较高的元素,测量其丰度可以用来研究星体的演化过程.最近不断发展的X射线卫星探测器已经可以在很高的能量分辨和灵敏性上探测特征X射线,用于天文学研究.这些特征X射线谱的分析,离不开精确的理论和计算的数据.
使用复旋转方法方法计算N2+-N5+离子的K壳层洞态能量级和宽度
【摘 要】
：
氮元素是宇宙中丰度较高的元素,测量其丰度可以用来研究星体的演化过程.最近不断发展的X射线卫星探测器已经可以在很高的能量分辨和灵敏性上探测特征X射线,用于天文学研究.这
【机 构】
：
中国科技大学近代物理系,北京应用物理与计算数学研究所
【出 处】
：
第十八届全国原子与分子物理学术会议
【发表日期】
：
2015年8期
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