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Masses of heavy-light mesons in Regge phenomenology

  • The masses of some orbitally and radially excited heavy-light mesons are calculated in Regge phenomenology. The results are in reasonable agreement with the experimental data and those given in many other theoretical approaches. Based on the calculation, we suggest that the recently observed D(2550), D(2600) and D(2760) can be assigned as the charmed members of the 21S0, 23S1 and 13D1 multiplets, respectively. Ds1*(2700)± may be assigned as the charm-strange member of the 23S1 state. The results may be helpful in understanding the nature of current and future experimentally observed heavy-light mesons.
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  • [1] Sanchez P et al. (BABAR collaboration). Phys. Rev. D, 2010, 82: 111101[2] Aubert B et al. (BABAR collaboration). Phys. Rev. Lett., 2006, 97: 222001[3] Brodzicka J et al. (Belle collaboration). Phys. Rev. Lett., 2008, 100: 092001[4] Aubert B et al. (BABAR collaboration). Phys. Rev. D, 2009, 80: 092003[5] Akers R et al. (OPAL collaboration). Z. Phys. C, 1995, 66: 19[6] Aaltonen T et al. (CDF collaboration). Phys. Rev. Lett., 2007, 99: 172001[7] Aaltonen T et al. (CDF collaboration). Phys. Rev. Lett., 2008, 100: 082001[8] Aaltonen T et al. (CDF collaboration). Phys. Rev. Lett., 2009, 102: 102003[9] Regge T. Nuovo Cim., 1959, 14: 951[10] Regge T. Nuovo Cim., 1960, 18: 947[11] Kawarabayashi K, Kitakado S, Yabuki H. Phys. Lett. B, 1969, 28: 432[12] Kaidalov A B. Z. Phys. C, 1982, 12: 63[13] Brisudova M M, Burakovsky L, Goldman T. Phys. Rev. D, 2000, 61: 054013[14] Anisovich A V, Anisovich V V, Sarantsev A V. Phys. Rev. D, 2000, 62: 051502(R)[15] Chan H M, Hsue C S, Quigg C et al. Phys. Rev. Lett., 1971, 26: 672[16] LI De-Min, MA Bing, LI Yu-Xiao et al. Eur. Phys. J. C, 2004, 37: 323[17] ZHANG Ai-Lin. Phys. Rev. D, 2005, 72: 017902[18] Afonin S S, Int. J. Mod. Phys. A, 2005, 22: 4537[19] CHIU Ting-Wai, HSIEH Tung-Han, HUANG Chao-Hsi et al. Phys. Lett. B, 2007, 651: 171[20] Davies C T H, Hornbostel K, Lepage G P et al. Phys. Lett. B, 1996, 382: 131[21] Ebert D, Faustov R N, Galkin V O. Phys. Rev. D, 2003, 67: 014027[22] LI De-Min, JI Peng-Fei, MA Bing. Eur. Phys. J. C, 2011, 71: 1582[23] Godfrey S. Phys. Rev. D, 2004, 70: 054017[24] Eichten E J, Quigg C. Phys. Rev. D, 1994, 49: 5845[25] Gershtein S S, Kiselev V V, Likhoded A K et al. Phys. Rev. D, 1995, 51: 3613[26] CHEN Yu-Qi, KUANG Yu-Ping. Phys. Rev. D, 1992, 46: 1165[27] Fulcher L P. Phys. Rev. D, 1999, 60: 074006[28] Patel B, Vinodkumar P C. J. Phys. G, 2009, 36: 035003[29] Gupta S N, Johnson J M. Phys. Rev. D, 1996, 53: 312[30] Gupta S N, Johnson J M. Phys. Rev. D, 1995, 51: 168[31] Matsuki T, Morii T, Sudoh K. Prog. Theor. Phys., 2007, 117:1077[32] Ebert D, Faustov R N, Galkin V O. Phys. Rev. D, 1998, 57: 5663[33] Ebert D, Faustov R N, Galkin V O. Mod. Phys. Lett. A, 2005, 20: 1887[34] Ebert D, Faustov R N, Galkin V O. Phys. Rev. D, 2009, 79: 114029[35] Ebert D, Faustov R N, Galkin V O. Eur. Phys. J. C, 2010, 66: 197[36] Di Pierro M, Eichten E. Phys. Rev. D, 2001, 64: 114004[37] GUO Xin-Heng, WEI Ke-Wei, WU Xing-Hua. Phys. Rev. D, 2008, 78: 056005[38] WEI Ke-Wei, GUO Xin-Heng. Phys. Rev. D, 2010, 81: 076005[39] WEI Ke-Wei, DONG Xin-Ping, L Gang. Int. J. Mod. Phys. A, 2011, 26: 2065[40] Nakamura K et al. (Particle Data Group). J. Phys. G, 2010, 37: 075021[41] GUO Feng-Kun, Meissner U G. Phys. Rev. D, 2011, 84: 014013[42] ZHONG Xian-Hui. Phys. Rev. D, 2010, 82: 114014[43] CHEN Bing, YUAN Ling, ZHANG Ai-Lin. Phys. Rev. D, 2011, 83: 114025[44] Godfrey S, Isgur N. Phys. Rev. D, 1985, 32: 189[45] Matsuki T, Morii T, Sudoh K. Eur. Phys. J. A, 2007, 31: 701[46] Badalian A M, Bakker B L G. Phys. Rev. D, 2011, 84: 034006[47] Colangelo P, De Fazio F, Nicotri S. Phys. Rev. D, 2008, 77: 014012[48] WANG Guo-Li, ZHANG Jin-Mei, WANG Zhi-Hui. Phys. Lett. B, 2009, 681: 326[49] CHEN Bing, WANG Deng-Xia, ZHANG Ai-Lin. Phys. Rev. D, 2009, 80: 071502
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QIN Zhen, DONG Xin-Ping and WEI Ke-Wei. Masses of heavy-light mesons in Regge phenomenology[J]. Chinese Physics C, 2013, 37(5): 053102. doi: 10.1088/1674-1137/37/5/053102
QIN Zhen, DONG Xin-Ping and WEI Ke-Wei. Masses of heavy-light mesons in Regge phenomenology[J]. Chinese Physics C, 2013, 37(5): 053102.  doi: 10.1088/1674-1137/37/5/053102 shu
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Received: 2012-06-26
Revised: 2012-08-16
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Masses of heavy-light mesons in Regge phenomenology

    Corresponding author: QIN Zhen,
    Corresponding author: DONG Xin-Ping,
    Corresponding author: WEI Ke-Wei,

Abstract: The masses of some orbitally and radially excited heavy-light mesons are calculated in Regge phenomenology. The results are in reasonable agreement with the experimental data and those given in many other theoretical approaches. Based on the calculation, we suggest that the recently observed D(2550), D(2600) and D(2760) can be assigned as the charmed members of the 21S0, 23S1 and 13D1 multiplets, respectively. Ds1*(2700)± may be assigned as the charm-strange member of the 23S1 state. The results may be helpful in understanding the nature of current and future experimentally observed heavy-light mesons.

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