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The X ray emissions from Arq+ (the kinetic energy 150 keV and 1.2 MeV) beams impinging on Au surface are measured. The results show that the about 2 keV minimum-potential energy of Ar11+ and Ar12+ (150 keV) is necessary for exciting Au atoms to emit M-X rays. The kinetic energy threshold for exciting target atomic X ray emission is estimated by the semiclassical approximation theory of binary collision.
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Keywords:
- highly charged ion /
- X ray /
- threshold
[1] 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
[2] Ma X, 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
[3] 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, Lü X Y, Jia J J, Chen L, Shao J, Lü Y, Wang F 2011 Chin. Phys. B 20 013402
[4] Dong C Z, Fu Y B 2006 Acta Phys. Sin. 55 107 (in Chinese) [董晨钟, 符彦飙 2006 55 107]
[5] Hagstrum H D 1954 Phys. Rev. 96 336
[6] Ryufuku H, Sasaki K, Watanabe T 1980 Phys. Rev. A 21 745
[7] Niehaus A 1986 J. Phys. B 19 2925
[8] Burgdörfer J, Lerner P, Meyer F W 1991 Phys. Rev. A 44 5674
[9] Luo X W, Hu B T, Zhang C J, Wang J J, Chen C H 2010 Phys. Rev. A 81 052902
[10] Briand J P, de Billy L, Charles P, Essabaa S, Briand P, Geller R, Desclaux J P, Bliman S, Ristori C 1990 Phys. Rev. Lett. 65 159
[11] Hayderer G, Schmid M, Varga P, Winter H P, Aumayr F, Wirtz L, Lemell C, Burgdörfer J, Hägg L, Reinhold C O 1999 Phys. Rev. Lett. 83 3948
[12] Gregori G, Glenzer S H, Fournier K B, Campbell K M, Dewald E L, Jones O S, Hammer J H, Hansen S B, Wallace R J, Landen O L 2008 Phys. Rev. Lett. 101 045003
[13] Schenkel T, Hamza A V, Barnes A V, Schneider D H 1999 Prog. Surf. Sci. 61 23
[14] Zhang Y P, Yang Z H, Du S B, Chen X M, Zhao Y T, Zhang X A, Cui Y, Zhang H Q, Xu X, Shao J X, Xiao G Q 2005 Acta Phys. Sin. 54 3559 (in Chinese) [张艳萍, 杨治虎, 杜树斌, 陈熙萌, 赵永涛, 张小安, 崔莹, 张红强, 徐徐, 邵健雄, 肖国青 2005 54 3559]
[15] Lemell C, Stöckl J, Burgdörfer J, Betz G, Winter H P, Aumayr F 1998 Phys. Rev. Lett. 81 1965
[16] Winter H, Aumayr F 1999 J. Phys. B: At. Mol. Opt. Phys. 32 39
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[1] 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
[2] Ma X, 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
[3] 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, Lü X Y, Jia J J, Chen L, Shao J, Lü Y, Wang F 2011 Chin. Phys. B 20 013402
[4] Dong C Z, Fu Y B 2006 Acta Phys. Sin. 55 107 (in Chinese) [董晨钟, 符彦飙 2006 55 107]
[5] Hagstrum H D 1954 Phys. Rev. 96 336
[6] Ryufuku H, Sasaki K, Watanabe T 1980 Phys. Rev. A 21 745
[7] Niehaus A 1986 J. Phys. B 19 2925
[8] Burgdörfer J, Lerner P, Meyer F W 1991 Phys. Rev. A 44 5674
[9] Luo X W, Hu B T, Zhang C J, Wang J J, Chen C H 2010 Phys. Rev. A 81 052902
[10] Briand J P, de Billy L, Charles P, Essabaa S, Briand P, Geller R, Desclaux J P, Bliman S, Ristori C 1990 Phys. Rev. Lett. 65 159
[11] Hayderer G, Schmid M, Varga P, Winter H P, Aumayr F, Wirtz L, Lemell C, Burgdörfer J, Hägg L, Reinhold C O 1999 Phys. Rev. Lett. 83 3948
[12] Gregori G, Glenzer S H, Fournier K B, Campbell K M, Dewald E L, Jones O S, Hammer J H, Hansen S B, Wallace R J, Landen O L 2008 Phys. Rev. Lett. 101 045003
[13] Schenkel T, Hamza A V, Barnes A V, Schneider D H 1999 Prog. Surf. Sci. 61 23
[14] Zhang Y P, Yang Z H, Du S B, Chen X M, Zhao Y T, Zhang X A, Cui Y, Zhang H Q, Xu X, Shao J X, Xiao G Q 2005 Acta Phys. Sin. 54 3559 (in Chinese) [张艳萍, 杨治虎, 杜树斌, 陈熙萌, 赵永涛, 张小安, 崔莹, 张红强, 徐徐, 邵健雄, 肖国青 2005 54 3559]
[15] Lemell C, Stöckl J, Burgdörfer J, Betz G, Winter H P, Aumayr F 1998 Phys. Rev. Lett. 81 1965
[16] Winter H, Aumayr F 1999 J. Phys. B: At. Mol. Opt. Phys. 32 39
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