Search

Article

x

留言板

尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

姓名
邮箱
手机号码
标题
留言内容
验证码

X-ray spectrum emitted by the impact of 152Eu20+ of near Bohn velocity on Au surface

Liang Chang-Hui Zhang Xiao-An Li Yao-Zong Zhao Yong-Tao Mei Ce-Xiang Cheng Rui Zhou Xian-Ming Lei Yu Wang Xing Sun Yuan-Bo Xiao Guo-Qing

X-ray spectrum emitted by the impact of 152Eu20+ of near Bohn velocity on Au surface

Liang Chang-Hui, Zhang Xiao-An, Li Yao-Zong, Zhao Yong-Tao, Mei Ce-Xiang, Cheng Rui, Zhou Xian-Ming, Lei Yu, Wang Xing, Sun Yuan-Bo, Xiao Guo-Qing
PDF
Get Citation
  • The characteristic X-ray spectra produced by the impact of highly charged ions of 152Eu20+ with energies from 2.0 to 6.0 MeV on Au surface are measured. It is found that highly charged ions could excite both the characteristic X-ray spectra of Mζ, Mα and Mδ of Au and the characteristic X-ray spectra of Mα of Eu. The total X-ray yield increases with the ion kinetic energy increasing. The total production cross section of Au induced by Eu20+ is measured and compared with those obtained from the binary encounter approximation, plane-wave-Born approximation, and the energy-loss Coulomb deflection perturbed stationary state relativistic theoretical models.
    • 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), the Education Commission Foundation of Shaanxi Province, China (Grant No. 2010JK895) and Scientific Research Foundation of Xianyang Normal University, China (Grant No. 09XSYK106).
    [1]

    Chen X M, Jiang L J, Zhou P, Zhou C L, Gao Z M, Qiu X Y, Cui Y, Wang X A, Lou F J, L X Y, Jia J J, Chen L, Shao J, L Y, Wang F 2011 Chin. Phys. B 20 013402

    [2]

    Dong C Z, Fu Y B 2006 Acta Phys. Sin. 55 0107 (in Chinese) [董晨钟, 符彦飙 2006 物理学报 55 0107]

    [3]

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

    [4]

    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

    [5]

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

    [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 and Particle Beams 29 265

    [8]

    Song Z Y, Yang Z H, Xiao G Q, Xu Q M, Chen J, Yang B, Yang Z R 2011 Eur. Phys. J. D 64 197

    [9]

    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]

    [10]

    Xu Q M, Yang Z H, Du S B, Chang H W, Zhang Y P 2011 Acta Phys. Sin. 60 093202 (in Chinese) [徐秋梅,杨治虎,杜树斌,常宏伟,张艳萍2011 物理学报 60 093202]

    [11]

    Zhao Y T, Xiao G Q, Zhang X A, Yang Z H, Chen X M, Zhang Y P 2006 J. Atom. Mole. Phys. 23 23 (in Chinese) [赵永涛, 肖国青, 张小安, 杨治虎, 陈熙萌, 张艳萍 2006 原子与分子物理学报 23 23]

    [12]

    X-RAY DATA BOOKLET Center for X-ray Optics and Advanced Light Source Lawrence Berkeley National Laboratoryhttp: //xdblblgov/2012.10.23

    [13]

    Gu J, Dong C Z, Ding X B, Xie L Y 2006 J. Atom. Mol. Phys. 23 16 (in Chinese) [顾娟, 董晨钟, 丁晓彬, 颉录有 2006 原子与分子物理学报 23 16]

    [14]

    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]

    [15]

    Garcia J D, Fortner RJ, Kavanagh T M 1973 Rev. Mod. Phys. 45 111

    [16]

    Gryziński M 1965 Phys. Rev. A 138 336

    [17]

    Zhang H, Chen X, Yang Z, Xu J, Cui Y, Shao J, Zhang X, Zhao Y, Zhang Y, Xiao G 2010 Nucl. Instr. Meth. B 268 1564

    [18]

    Liu Z Q, Cipolla S J 1996 Comput. Phys. Commun. 97 315

    [19]

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

  • [1]

    Chen X M, Jiang L J, Zhou P, Zhou C L, Gao Z M, Qiu X Y, Cui Y, Wang X A, Lou F J, L X Y, Jia J J, Chen L, Shao J, L Y, Wang F 2011 Chin. Phys. B 20 013402

    [2]

    Dong C Z, Fu Y B 2006 Acta Phys. Sin. 55 0107 (in Chinese) [董晨钟, 符彦飙 2006 物理学报 55 0107]

    [3]

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

    [4]

    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

    [5]

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

    [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 and Particle Beams 29 265

    [8]

    Song Z Y, Yang Z H, Xiao G Q, Xu Q M, Chen J, Yang B, Yang Z R 2011 Eur. Phys. J. D 64 197

    [9]

    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]

    [10]

    Xu Q M, Yang Z H, Du S B, Chang H W, Zhang Y P 2011 Acta Phys. Sin. 60 093202 (in Chinese) [徐秋梅,杨治虎,杜树斌,常宏伟,张艳萍2011 物理学报 60 093202]

    [11]

    Zhao Y T, Xiao G Q, Zhang X A, Yang Z H, Chen X M, Zhang Y P 2006 J. Atom. Mole. Phys. 23 23 (in Chinese) [赵永涛, 肖国青, 张小安, 杨治虎, 陈熙萌, 张艳萍 2006 原子与分子物理学报 23 23]

    [12]

    X-RAY DATA BOOKLET Center for X-ray Optics and Advanced Light Source Lawrence Berkeley National Laboratoryhttp: //xdblblgov/2012.10.23

    [13]

    Gu J, Dong C Z, Ding X B, Xie L Y 2006 J. Atom. Mol. Phys. 23 16 (in Chinese) [顾娟, 董晨钟, 丁晓彬, 颉录有 2006 原子与分子物理学报 23 16]

    [14]

    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]

    [15]

    Garcia J D, Fortner RJ, Kavanagh T M 1973 Rev. Mod. Phys. 45 111

    [16]

    Gryziński M 1965 Phys. Rev. A 138 336

    [17]

    Zhang H, Chen X, Yang Z, Xu J, Cui Y, Shao J, Zhang X, Zhao Y, Zhang Y, Xiao G 2010 Nucl. Instr. Meth. B 268 1564

    [18]

    Liu Z Q, Cipolla S J 1996 Comput. Phys. Commun. 97 315

    [19]

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

  • [1] Liang Chang-Hui, Li Yao-Zong, Zhang Xiao-An, Zhao Yong-Tao, Xiao Guo-Qing. X-ray spectrum emitted by the impact of 129Xeq+ on Mo surface. Acta Physica Sinica, 2010, 59(9): 6059-6063. doi: 10.7498/aps.59.6059
    [2] 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. Acta Physica Sinica, 2014, 63(16): 163201. doi: 10.7498/aps.63.163201
    [3] Liang Chang-Hui, Zhang Xiao-An, Li Yao-Zong, Zhao Yong-Tao, Mei Ce-Xiang, Zhou Xian-Ming, Xiao Guo-Qing. Study of X-ray spectrum emitted due to the impact of 129Xeq+ on different ion's charge on Au. Acta Physica Sinica, 2015, 64(5): 053201. doi: 10.7498/aps.64.053201
    [4] Chen Xi-Meng, Cui Ying, Zhang Hong-Qiang, Xu Xu, Shao Jian-Xiong, Zhang Xiao-An, Yang Zhi-Hu, Song Zhang-Yong, Zhang Yan-Ping, Zhao Yong-Tao, Yu De-Yang, Cai Xiao-Hong. X-ray emission produced by interaction of highly ionized Arq+ ions with metallic targets. Acta Physica Sinica, 2006, 55(5): 2221-2227. doi: 10.7498/aps.55.2221
    [5] Wang Dang-Chao, Mei Ce-Xiang, Niu Chao-Ying, Dai Bin, Zhang Xiao-An, Yang Zhi-Hu, Wang Wei, Xiao Guo-Qing. Cobalt-like-Xe-induced infrared light and x-ray emission at Ni surface. Acta Physica Sinica, 2009, 58(10): 6920-6925. doi: 10.7498/aps.58.6920
    [6] Cui Ying, Zhang Hong-Qiang, Shao Jian-Xiong, Du Juan, Liu Yu-Wen, Chen Xi-Meng, Zhang Xiao-An, Yang Zhi-Hu, Song Zhang-Yong, Ruan Fang-Fang, Zhu Ke-Xin, Shao Cao-Jie, Lu Rong-Chun, Yu De-Yang, Cai Xiao-Hong. X-ray spectra produced by interaction of Ar16+ and Ar17+ with Zr. Acta Physica Sinica, 2008, 57(2): 803-807. doi: 10.7498/aps.57.803
    [7] Zhang Xiao-An, Mei Ce-Xiang, Zhao Yong-Tao, Cheng Rui, Wang Xing, Zhou Xian-Ming, Lei Yu, Sun Yuan-Bo, Xu Ge, Ren Jie-Ru. X-ray emission of C6+ pulsed ion beams of CSR impacting on Au target. Acta Physica Sinica, 2013, 62(17): 173401. doi: 10.7498/aps.62.173401
    [8] Chen Xi-Meng, Zhang Hong-Qiang, Cui Ying, Shao Jian-Xiong, Xu Xu, Li Fu-Li, Zhao Yong-Tao, Xiao Guo-Qing, Yang Zhi-Hu, Zhang Yan-Ping, Zhang Xiao-An. The x-ray spectra of hollow atoms. Acta Physica Sinica, 2005, 54(1): 85-88. doi: 10.7498/aps.54.85
    [9] Wang Xing, Zhao Yong-Tao, Cheng Rui, Zhou Xian-Ming, Xu Ge, Sun Yuan-Bo, Lei Yu, Wang Yu-Yu, Ren Jie-Ru, Yu Yang, Li Yong-Feng, Zhang Xiao-An, Li Yao-Zong, Liang Chang-Hui, Xiao Guo-Qing. Multiple ionization effect of Ta induced by heavy ions. Acta Physica Sinica, 2012, 61(19): 193201. doi: 10.7498/aps.61.193201
    [10] Li Yao-Zong, Zhang Xiao-An, Liang Chang-Hui, Zhao Yong-Tao, Cheng Rui, Zhou Xian-Ming, Wang Xing, Lei Yu, Sun Yuan-Bo, Xu Ge. Au L X-ray and Xe M X-ray emission following 129Xe30+ ion impact on Au surface. Acta Physica Sinica, 2012, 61(6): 063201. doi: 10.7498/aps.61.063201
  • Citation:
Metrics
  • Abstract views:  937
  • PDF Downloads:  530
  • Cited By: 0
Publishing process
  • Received Date:  23 October 2012
  • Accepted Date:  06 January 2013
  • Published Online:  20 March 2013

X-ray spectrum emitted by the impact of 152Eu20+ of near Bohn velocity on Au surface

  • 1. Ion Beam and Optical Physical Joint Laboratory of Xianyang Normal University and Institute of Modern Physics Chinese Academy of Sciences,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), the Education Commission Foundation of Shaanxi Province, China (Grant No. 2010JK895) and Scientific Research Foundation of Xianyang Normal University, China (Grant No. 09XSYK106).

Abstract: The characteristic X-ray spectra produced by the impact of highly charged ions of 152Eu20+ with energies from 2.0 to 6.0 MeV on Au surface are measured. It is found that highly charged ions could excite both the characteristic X-ray spectra of Mζ, Mα and Mδ of Au and the characteristic X-ray spectra of Mα of Eu. The total X-ray yield increases with the ion kinetic energy increasing. The total production cross section of Au induced by Eu20+ is measured and compared with those obtained from the binary encounter approximation, plane-wave-Born approximation, and the energy-loss Coulomb deflection perturbed stationary state relativistic theoretical models.

Reference (19)

Catalog

    /

    返回文章
    返回