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X-ray spectrum emitted by the impact of 129Xe26+ of the different kinetic energies on Au surface

Liang Chang-Hui Zhang Xiao-An Li Yao-Zong Zhao Yong-Tao Xiao Guo-Qing

X-ray spectrum emitted by the impact of 129Xe26+ of the different kinetic energies on Au surface

Liang Chang-Hui, Zhang Xiao-An, Li Yao-Zong, Zhao Yong-Tao, Xiao Guo-Qing
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  • The characteristic X-ray spectra produced by the impact of 129Xe26+ with kinetic energies from 350 to 600 keV and from 1.8 to 3.9 MeV on Au surface are measured. It is found that 129Xe26+ with kinetic energies from 350 to 600 keV can excite only the characteristic X-ray spectra of Mα of Au, but 129Xe26+ with kinetic energies from 1.8 to 3.9 MeV can excite the characteristic X-ray spectra of Mζ, Mα, Mγ and Mδ. The relation between the characteristic X-ray intensity, the ratio of X-ray yield and the ion kinetic energy is analyzed. The kinetic energy threshold of L-X-ray of Xe emitted by Xe26+ is estimated.
    • Funds: Project supported by the National Natural Science Foundation of China (Grant No. 11075135), the Natural Science Foundation of Shaanxi Province, China (Grant No. 2010JM1012), and the Scientific Research Program of the Education Bureau of Shaanxi Province, China (Grant No. 14JK1803).
    [1]

    Schenkel T, Hamza A V, Barnes A V, Schneider D H 1999 Prog. Surf. Sci. 61 23

    [2]

    Aumayr F, Winter H P 2005 Nucl. Instrum. Meth. B 233 111

    [3]

    Phillips K J H, Mewe R, Harra-Murnion L K, Kaastra J S, Beiersdorfer P, Brown G V, Liedahl D A 1999 Astron. Astrophys. Suppl. Ser. 138 381

    [4]

    Yang Z H, Du S B, Zeng X T, Chang H W, Zhang B L, Wang W, Yu D Y, Cai X H 2009 Astron. J. 137 4020

    [5]

    Ma X W, Zhang R T, Zhang S F, Zhu X L, Feng W T, Guo D L, Li B, Liu H P, Li C Y, Wang J G, Yan S C, Zhang P J, Wang Q 2011 Phys. Rev. A 83 052707

    [6]

    Luo X W, Hu B T, Zhang C J, Wang J J, Chen C H 2010 Phys. Rev. A 81 052902

    [7]

    Zhang X A, Zhao Y T, Hoffmann D, Yang Z H, Chen X M, Xu Z F, Li F L, Xiao G Q 2011 Laser Part. Beams 29 265

    [8]

    Liang C H, Zhang X A, Li Y Z, Zhao Y T, Mei C X, Cheng R, Zhou X M, Lei Y, Wang X, Sun Y B, Xiao G Q 2013 Acta Phys. Sin. 62 063202 (in Chinese) [梁昌慧, 张小安, 李耀宗, 赵永涛, 梅策香, 程锐, 周贤明, 雷瑜, 王兴, 孙渊博, 肖国青 2013 物理学报 62 063202]

    [9]

    Zhou X M, Zhao Y T, Ren J R, Cheng R, Lei Y, Sun Y B, Xu G, Wang Y Y, Liu S D, Xiao G Q 2013 Chin. Phys. B 22 113402

    [10]

    Mei C X, Zhang X A, Zhao Y T, Zhou X M, Ren J R, Wang X, Lei Y, Sun Y B, Cheng R, Wang Y Y, Liang C H, Li Y Z, Xiao G Q 2013 Chin. Phys. B 22 103403

    [11]

    Wang X, Zhao Y T, Cheng R, Zhou X M, Xu G, Sun Y B, Lei Y, Wang Y Y, Ren J R, Yu Y, Li Y F, Zhang X A, Li Y Z, Liang C H, Xiao G Q 2012 Acta Phys. Sin. 61 193201 (in Chinese) [王兴, 赵永涛, 程锐, 周贤明, 徐戈, 孙渊博, 雷瑜, 王瑜玉, 任洁茹, 虞洋, 李永峰, 张小安, 李耀宗, 梁昌慧, 肖国青 2012 物理学报 61 193201]

    [12]

    Liang C H, Zhang X A, Li Y Z, Zhao Y T, Xiao G Q 2010 Acta Phys. Sin. 59 6059 (in Chinese) [梁昌慧, 张小安, 李耀宗, 赵永涛, 肖国青 2010 物理学报 59 6059]

    [13]

    Liang C H, Zhang X A, Li Y Z 2013 Nucl. Phys. Rev. 30 63 (in Chinese) [梁昌慧, 张小安, 李耀宗 2013 原子核物理评论 30 63]

    [14]

    Albert C T, Janos K, David T A, Eric M G, Malcolm R H, Jeffrey B K, Yan W L, Arthur L R, James H U, Kwang J K, Ingolf L, Piero P, Herman W, Gwyn P W, James H S 2009 X-ray Data Booklet (Berkeley: Lawrence Berkeley National Laboratory) p16

    [15]

    Burgdörfer J, Lerner P, Meyer F W 1991 Phys. Rev. A 44 5674

    [16]

    Awaya Y, Kambara T, Kanai Y 1999 Int. J. Mass Spectrom. 192 49

    [17]

    Zou X R, Shao J X, Chen X M, Cui Y 2010 Acta Phys. Sin. 59 6064 (in Chinese) [邹贤容, 邵剑雄, 陈熙萌, 崔莹 2010 物理学报 59 6064]

    [18]

    Li Y Z, Zhang X A, Liang C H, Zhao Y T, Cheng R, Zhou X M, Wang X, Lei Y, Sun Y B, Xu G, Li J Y, Xiao G Q 2011 J. At. Mol. Phys. 28 795 (in Chinese) [李耀宗, 张小安, 梁昌慧, 赵永涛, 程锐, 周贤明, 王兴, 雷瑜, 孙渊博, 徐戈, 李锦玉, 肖国青 2011 原子与分子物理学报 28 795]

    [19]

    Singh Y, Tribedi L C 2002 Phys. Rev. A 66 062709

  • [1]

    Schenkel T, Hamza A V, Barnes A V, Schneider D H 1999 Prog. Surf. Sci. 61 23

    [2]

    Aumayr F, Winter H P 2005 Nucl. Instrum. Meth. B 233 111

    [3]

    Phillips K J H, Mewe R, Harra-Murnion L K, Kaastra J S, Beiersdorfer P, Brown G V, Liedahl D A 1999 Astron. Astrophys. Suppl. Ser. 138 381

    [4]

    Yang Z H, Du S B, Zeng X T, Chang H W, Zhang B L, Wang W, Yu D Y, Cai X H 2009 Astron. J. 137 4020

    [5]

    Ma X W, Zhang R T, Zhang S F, Zhu X L, Feng W T, Guo D L, Li B, Liu H P, Li C Y, Wang J G, Yan S C, Zhang P J, Wang Q 2011 Phys. Rev. A 83 052707

    [6]

    Luo X W, Hu B T, Zhang C J, Wang J J, Chen C H 2010 Phys. Rev. A 81 052902

    [7]

    Zhang X A, Zhao Y T, Hoffmann D, Yang Z H, Chen X M, Xu Z F, Li F L, Xiao G Q 2011 Laser Part. Beams 29 265

    [8]

    Liang C H, Zhang X A, Li Y Z, Zhao Y T, Mei C X, Cheng R, Zhou X M, Lei Y, Wang X, Sun Y B, Xiao G Q 2013 Acta Phys. Sin. 62 063202 (in Chinese) [梁昌慧, 张小安, 李耀宗, 赵永涛, 梅策香, 程锐, 周贤明, 雷瑜, 王兴, 孙渊博, 肖国青 2013 物理学报 62 063202]

    [9]

    Zhou X M, Zhao Y T, Ren J R, Cheng R, Lei Y, Sun Y B, Xu G, Wang Y Y, Liu S D, Xiao G Q 2013 Chin. Phys. B 22 113402

    [10]

    Mei C X, Zhang X A, Zhao Y T, Zhou X M, Ren J R, Wang X, Lei Y, Sun Y B, Cheng R, Wang Y Y, Liang C H, Li Y Z, Xiao G Q 2013 Chin. Phys. B 22 103403

    [11]

    Wang X, Zhao Y T, Cheng R, Zhou X M, Xu G, Sun Y B, Lei Y, Wang Y Y, Ren J R, Yu Y, Li Y F, Zhang X A, Li Y Z, Liang C H, Xiao G Q 2012 Acta Phys. Sin. 61 193201 (in Chinese) [王兴, 赵永涛, 程锐, 周贤明, 徐戈, 孙渊博, 雷瑜, 王瑜玉, 任洁茹, 虞洋, 李永峰, 张小安, 李耀宗, 梁昌慧, 肖国青 2012 物理学报 61 193201]

    [12]

    Liang C H, Zhang X A, Li Y Z, Zhao Y T, Xiao G Q 2010 Acta Phys. Sin. 59 6059 (in Chinese) [梁昌慧, 张小安, 李耀宗, 赵永涛, 肖国青 2010 物理学报 59 6059]

    [13]

    Liang C H, Zhang X A, Li Y Z 2013 Nucl. Phys. Rev. 30 63 (in Chinese) [梁昌慧, 张小安, 李耀宗 2013 原子核物理评论 30 63]

    [14]

    Albert C T, Janos K, David T A, Eric M G, Malcolm R H, Jeffrey B K, Yan W L, Arthur L R, James H U, Kwang J K, Ingolf L, Piero P, Herman W, Gwyn P W, James H S 2009 X-ray Data Booklet (Berkeley: Lawrence Berkeley National Laboratory) p16

    [15]

    Burgdörfer J, Lerner P, Meyer F W 1991 Phys. Rev. A 44 5674

    [16]

    Awaya Y, Kambara T, Kanai Y 1999 Int. J. Mass Spectrom. 192 49

    [17]

    Zou X R, Shao J X, Chen X M, Cui Y 2010 Acta Phys. Sin. 59 6064 (in Chinese) [邹贤容, 邵剑雄, 陈熙萌, 崔莹 2010 物理学报 59 6064]

    [18]

    Li Y Z, Zhang X A, Liang C H, Zhao Y T, Cheng R, Zhou X M, Wang X, Lei Y, Sun Y B, Xu G, Li J Y, Xiao G Q 2011 J. At. Mol. Phys. 28 795 (in Chinese) [李耀宗, 张小安, 梁昌慧, 赵永涛, 程锐, 周贤明, 王兴, 雷瑜, 孙渊博, 徐戈, 李锦玉, 肖国青 2011 原子与分子物理学报 28 795]

    [19]

    Singh Y, Tribedi L C 2002 Phys. Rev. A 66 062709

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  • Received Date:  31 December 2013
  • Accepted Date:  06 May 2014
  • Published Online:  20 August 2014

X-ray spectrum emitted by the impact of 129Xe26+ of the different kinetic energies on Au surface

  • 1. Ion Beam and Optical Physical Laboratory, Xianyang Normal University, Xianyang 712000, China;
  • 2. Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China
Fund Project:  Project supported by the National Natural Science Foundation of China (Grant No. 11075135), the Natural Science Foundation of Shaanxi Province, China (Grant No. 2010JM1012), and the Scientific Research Program of the Education Bureau of Shaanxi Province, China (Grant No. 14JK1803).

Abstract: The characteristic X-ray spectra produced by the impact of 129Xe26+ with kinetic energies from 350 to 600 keV and from 1.8 to 3.9 MeV on Au surface are measured. It is found that 129Xe26+ with kinetic energies from 350 to 600 keV can excite only the characteristic X-ray spectra of Mα of Au, but 129Xe26+ with kinetic energies from 1.8 to 3.9 MeV can excite the characteristic X-ray spectra of Mζ, Mα, Mγ and Mδ. The relation between the characteristic X-ray intensity, the ratio of X-ray yield and the ion kinetic energy is analyzed. The kinetic energy threshold of L-X-ray of Xe emitted by Xe26+ is estimated.

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