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《中国物理C》（英文）编辑部
2024年10月30日
Chinese Physics C> 2017, Vol. 41> Issue(5) : 053105 DOI: 10.1088/1674-1137/41/5/053105

Possible hadronic molecular states composed of S-wave heavy-light mesons

  • 1.

      Institute of Theoretical Physics, College of Physics and Electronic Engineering, Northwest Normal University,Lanzhou 730070, China

  • 2.

      Department of Physics, Southeast University, Nanjing 210094, China

  • We perform a systematical study of possible molecular states composed of the S wave heavy light mesons, where the S-D mixing and η-η' mixing are explicitly included. Our calculation indicates that the observed X(3872) could be a loosely shallow molecular state composed of DD* +h.c, while neither Zc(3900)/Zc(4020) nor Zb(10610)/Zb(10650) is supported to be a molecule. Some observed possible molecular states are predicted, which could be searched for by further experimental measurements.
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  • References

    [1] H. X. Chen, W. Chen, X. Liu, and S. L. Zhu, Phys. Rept., 639: 1 (2016)
    [2] S. K. Choi et al (Belle Collaboration), Phys. Rev. Lett., 91: 262001 (2003)
    [3] K. Abe et al (Belle Collaboration), arXiv:hep-ex/0505037
    [4] G. Gokhroo et al (Belle Collaboration), Phys. Rev. Lett., 97: 162002 (2006)
    [5] I. Adachi et al (Belle Collaboration), arXiv:0809.1224 [hep-ex]
    [6] I. Adachi et al (Belle Collaboration), arXiv:0810.0358 [hep-ex]
    [7] B. Aubert et al (BABAR Collaboration), Phys. Rev. D, 71: 071103 (2005)
    [8] B. Aubert et al (BABAR Collaboration), Phys. Rev. Lett., 93: 041801 (2004)
    [9] B. Aubert et al (BABAR Collaboration), Phys. Rev. D, 71: 052001 (2005)
    [10] B. Aubert et al (BABAR Collaboration), Phys. Rev. D, 73: 011101 (2006)
    [11] B. Aubert et al (BABAR Collaboration), Phys. Rev. Lett., 96: 052002 (2006)
    [12] B. Aubert et al (BABAR Collaboration), Phys. Rev. D, 74: 071101 (2006)
    [13] B. Aubert et al (BABAR Collaboration), Phys. Rev. D, 77: 011102 (2008)
    [14] D. E. Acosta et al (CDF II Collaboration), Phys. Rev. Lett., 93: 072001 (2004)
    [15] A. Abulencia et al (CDF Collaboration), Phys. Rev. Lett., 96: 102002 (2006)
    [16] A. Abulencia et al (CDF Collaboration), Phys. Rev. Lett., 98: 132002 (2007)
    [17] T. Aaltonen et al (CDF Collaboration), Phys. Rev. Lett., 103: 152001 (2009)
    [18] V. M. Abazov et al (D0 Collaboration), Phys. Rev. Lett., 93: 162002 (2004)
    [19] R. Aaij et al (LHCb Collaboration), Eur. Phys. J. C, 72: 1972 (2012)
    [20] R. Aaij et al (LHCb Collaboration), Phys. Rev. Lett., 110: 222001 (2013)
    [21] R. Aaij et al (LHCb Collaboration), Nucl. Phys. B, 886: 665 (2014)
    [22] R. Aaij et al (LHCb Collaboration), Phys. Rev. D, 92 (1): 011102 (2015)
    [23] M. Ablikim et al (BESIII Collaboration), Phys. Rev. Lett., 112 (9): 092001 (2014)
    [24] B. Aubert et al (BaBar Collaboration), Phys. Rev. D, 71: 031501 (2005)
    [25] M. Ablikim et al (BESIII Collaboration), Phys. Rev. Lett., 110: 252001 (2013)
    [26] Z. Q. Liu et al (Belle Collaboration), Phys. Rev. Lett., 110: 252002 (2013)
    [27] T. Xiao, S. Dobbs, A. Tomaradze, and K. K. Seth, Phys. Lett. B, 727: 366 (2013)
    [28] M. Ablikim et al (BESIII Collaboration), Phys. Rev. Lett., 112 (2): 022001 (2014)
    [29] M. Ablikim et al (BESIII Collaboration), Phys. Rev. Lett., 115: 112003 (2015)
    [30] M. Ablikim et al, arXiv:1509.05620 [hep-ex]
    [31] M. Ablikim et al (BESIII Collaboration), Phys. Rev. Lett., 111 (24): 242001 (2013)
    [32] M. Ablikim et al (BESIII Collaboration), Phys. Rev. Lett., 113: 212002 (2014)
    [33] M. Ablikim et al (BESIII Collaboration), Phys. Rev. Lett., 112: 132001 (2014)
    [34] M. Ablikim et al (BESIII Collaboration), Phys. Rev. Lett., 115: 182002 (2015)
    [35] T. Aaltonen et al (CDF Collaboration), Phys. Rev. Lett., 102: 242002 (2009)
    [36] T. Aaltonen et al (CDF Collaboration), arXiv:1101.6058 [hep-ex]
    [37] S. Chatrchyan et al (CMS Collaboration), Phys. Lett. B, 734: 261 (2014)
    [38] V. M. Abazov et al (D0 Collaboration), Phys. Rev. D, 89: 012004 (2014)
    [39] R. Aaij et al (LHCb Collaboration), arXiv:1606.07895 [hep-ex]
    [40] R. Aaij et al (LHCb Collaboration), arXiv:1606.07898 [hep-ex]
    [41] A. Bondar et al (Belle Collaboration), Phys. Rev. Lett., 108: 122001 (2012)
    [42] A. Garmash et al (Belle Collaboration), Phys. Rev. D, 91: 072003 (2015)
    [43] I. Adachi et al (Belle Collaboration), arXiv:1209.6450 [hep-ex]
    [44] A. Garmash et al (Belle Collaboration), Phys. Rev. Lett., 116: 212001 (2016)
    [45] P. Krokovny et al (Belle Collaboration), Phys. Rev. D, 88: 052016 (2013)
    [46] A. Abdesselam et al (Belle Collaboration), Phys. Rev. Lett., 117: 142001 (2016)
    [47] W. S. Hou, Phys. Rev. D,74: 017504 (2006)
    [48] G. Li and Z. Zhou, Phys. Rev. D, 91: 034020 (2015)
    [49] Q. Wu, G. Li, F. Shao, Q. Wang, R. Wang, Y. Zhang, and Y. Zheng, Adv. High Energy Phys., 2016: 3729050 (2016)
    [50] X. H. He et al (Belle Collaboration), Phys. Rev. Lett., 113: 142001 (2014)
    [51] Y. S. Kalashnikova, Phys. Rev. D, 72: 034010 (2005)
    [52] O. Zhang, C. Meng, and H. Q. Zheng, Phys. Lett. B, 680: 453 (2009)
    [53] Y. S. Kalashnikova and A. V. Nefediev, Phys. Rev. D, 80: 074004 (2009)
    [54] B. Q. Li and K. T. Chao, Phys. Rev. D, 79: 094004 (2009)
    [55] J. Ferretti, G. Galat, and E. Santopinto, Phys. Rev. C, 88: 015207 (2013)
    [56] E. J. Eichten, K. Lane, and C. Quigg, Phys. Rev. D, 69: 094019 (2004)
    [57] M. R. Pennington and D. J. Wilson, Phys. Rev. D, 76, 077502 (2007)
    [58] D. Y. Chen, arXiv:1611.00109 [hep-ph]
    [59] L. Maiani, F. Piccinini, A. D. Polosa, and V. Riquer, Phys. Rev. D, 71: 014028 (2015)
    [60] T. W. Chiu et al (TWQCD Collaboration), Phys. Rev., D, 73: 111503 (2006); 75: 019902 (2007)
    [61] D. Ebert, R. N. Faustov, and V. O. Galkin, Phys. Lett. B, 634: 214 (2006)
    [62] A. Ali, L. Maiani, A. D. Polosa, and V. Riquer, Phys. Rev. D, 91: 017502 (2015)
    [63] A. Ali, C. Hambrock, and W. Wang, Phys. Rev. D, 88: 054026 (2013)
    [64] W. Chen and S. L. Zhu, Phys. Rev. D, 83: 034010 (2011)
    [65] W. Chen, T. G. Steele, H. X. Chen, and S. L. Zhu, Phys. Rev. D, 92; 054002 (2015)
    [66] W. Chen, T. G. Steele, M. L. Du, and S. L. Zhu, Eur. Phys. J. C, 74: 2773 (2014)
    [67] Z. G. Wang, Commun. Theor. Phys., 63: 466 (2015)
    [68] C. F. Qiao and L. Tang, Eur. Phys. J. C, 74: 2810 (2014)
    [69] Z. G. Wang, Int. J. Mod. Phys. A, 30: 1550168 (2015)
    [70] D. V. Bugg, Europhys. Lett., 96: 11002 (2011)
    [71] D. V. Bugg, arXiv:1101.1659 [hep-ph]
    [72] D. Y. Chen and X. Liu, Phys. Rev. D, 84: 094003 (2011) [arXiv:1106.3798 [hep-ph]]
    [73] D. Y. Chen, X. Liu, and T. Matsuki, Phys. Rev. D, 88: 036008 (2013)
    [74] D. Y. Chen and X. Liu, Phys. Rev. D, 84: 034032 (2011)
    [75] D. Y. Chen, X. Liu, and S. L. Zhu, Phys. Rev. D, 84: 074016 (2011)
    [76] D. Y. Chen, X. Liu, and T. Matsuki, Phys. Rev. Lett., 110: 232001 (2013)
    [77] E. S. Swanson, Phys. Lett. B, 588: 189 (2004)
    [78] Y. R. Liu, X. Liu, W. Z. Deng, and S. L. Zhu, Eur. Phys. J. C, 56: 63 (2008)
    [79] C. E. Thomas and F. E. Close, Phys. Rev. D, 78: 034007 (2008)
    [80] X. Liu, Z. G. Luo, Y. R. Liu, and S. L. Zhu, Eur. Phys. J. C, 61: 411 (2009)
    [81] M. T. AlFiky, F. Gabbiani, and A. A. Petrov, Phys. Lett. B, 640: 238 (2006)
    [82] I. W. Lee, A. Faessler, T. Gutsche, and V. E. Lyubovitskij, Phys. Rev. D, 80: 094005 (2009)
    [83] W. Chen, H. y. Jin, R. T. Kleiv, T. G. Steele, M. Wang, and Q. Xu, Phys. Rev. D, 88: 045027 (2013)
    [84] Y. Dong, A. Faessler, T. Gutsche, S. Kovalenko, and V. E. Lyubovitskij, Phys. Rev. D, 79: 094013 (2009)
    [85] Y. Dong, A. Faessler, T. Gutsche, and V. E. Lyubovitskij, Phys. Rev. D, 90: 074032 (2014)
    [86] M. Harada and Y. L. Ma, Prog. Theor. Phys., 126: 91 (2011)
    [87] E. Braaten, H.-W. Hammer, and T. Mehen, Phys. Rev. D, 82: 034018 (2010)
    [88] F. Aceti, M. Bayar, E. Oset, A. Martinez Torres, K. P. Khemchandani, J. M. Dias, F. S. Navarra, and M. Nielsen, Phys. Rev. D, 90: 016003 (2014)
    [89] Z. F. Sun, J. He, X. Liu, Z. G. Luo, and S. L. Zhu, Phys. Rev. D, 84: 054002 (2011)
    [90] Z. F. Sun, Z. G. Luo, J. He, X. Liu, and S. L. Zhu, Chin. Phys. C, 36: 194 (2012)
    [91] Z. G. Wang and T. Huang, Eur. Phys. J. C, 74: 2891 (2014)
    [92] Q. Wu, G. Li, F. Shao, and R. Wang, Phys. Rev. D, 94: 014015 (2016)
    [93] G. Li, Eur. Phys. J. C, 73: 2621 (2013)
    [94] Y. Dong, A. Faessler, T. Gutsche, and V. E. Lyubovitskij, phys. Rev. D, 88: 014030 (2013)
    [95] Y. Dong, A. Faessler, T. Gutsche and V. E. Lyubovitskij, Phys. Rev. D, 89: 034018 (2014)
    [96] G. Li, X. H. Liu, and Z. Zhou, Phys. Rev. D, 90: 054006 (2014)
    [97] T. Gutsche, M. Kesenheimer, and V. E. Lyubovitskij, Phys. Rev. D, 90: 094013 (2014)
    [98] A. Esposito, A. L. Guerrieri, and A. Pilloni, Phys. Lett. B, 746: 194 (2015)
    [99] H. W. Ke, Z. T. Wei, and X. Q. Li, Eur. Phys. J. C, 73: 2561 (2013)
    [100] D. Y. Chen and Y. B. Dong, Phys. Rev. D, 93: 014003 (2016)
    [101] N. Mahajan, Phys. Lett. B, 679: 228 (2009)
    [102] G. J. Ding, Eur. Phys. J. C, 64: 297 (2009)
    [103] R. Molina and E. Oset, Phys. Rev. D, 80: 114013 (2009)
    [104] X. Liu and H. W. Ke, Phys. Rev. D, 80: 034009 (2009)
    [105] J. R. Zhang and M. Q. Huang, Phys. Rev. D, 80: 056004 (2009)
    [106] X. Liu and S. L. Zhu, Phys. Rev. D, 80: 017502 (2009); 85: 019902 (2012)
    [107] R. M. Albuquerque, M. E. Bracco, and M. Nielsen, Phys. Lett. B, 678: 186 (2009)
    [108] J. R. Zhang and M. Q. Huang, J. Phys. G, 37: 025005 (2010)
    [109] Z. G. Wang, Eur. Phys. J. C, 74: 2963 (2014)
    [110] X. Chen, X. L, R. Shi, and X. Guo, Nucl. Phys. B, 909: 243 (2016)
    [111] T. Branz, T. Gutsche, and V. E. Lyubovitskij, Phys. Rev. D, 80: 054019 (2009)
    [112] M. T. Li, W. L. Wang, Y. B. Dong, and Z. Y. Zhang, J. Phys. G 40: 015003 (2013)
    [113] Y. Yang, J. Ping, C. Deng, and H. S. Zong, J. Phys. G, 39: 105001 (2012)
    [114] J. R. Zhang, M. Zhong, and M. Q. Huang, Phys. Lett. B, 704: 312 (2011)
    [115] Y. Dong, A. Faessler, T. Gutsche, and V. E. Lyubovitskij, J. Phys. G, 40: 015002 (2013)
    [116] G. Li, F. l. Shao, C. W. Zhao, and Q. Zhao, Phys. Rev. D, 87: 034020 (2013)
    [117] M. Cleven, Q. Wang, F. K. Guo, C. Hanhart, U. G. Meissner and Q. Zhao, Phys. Rev. D, 87: 074006 (2013)
    [118] X. Li and M. B. Voloshin, Phys. Rev. D, 86: 077502 (2012)
    [119] T. Mehen and J. W. Powell, Phys. Rev. D, 84: 114013 (2011)
    [120] J. Carlson and R. Schiavilla, Rev. Mod. Phys., 70: 743 (1998)
    [121] R. G. Arnold, C. E. Carlson, and F. Gross, Phys. Rev. C, 23: (1981) 363
    [122] R. Casalbuoni, A. Deandrea, N. Di Bartolomeo, R. Gatto, F. Feruglio, and G. Nardulli, Phys. Rept., 281: 145 (1997)
    [123] H. Y. Cheng, C. Y. Cheung, G. L. Lin, Y. C. Lin, T. M. Yan, and H. L. Yu, Phys. Rev. D, 47: 1030 (1993)
    [124] T. M. Yan, H. Y. Cheng, C. Y. Cheung, G. L. Lin, Y. C. Lin, and H. L. Yu, Phys. Rev. D, 46: 1148 (1992)
    [125] M. B. Wise, Phys. Rev. D, 45: 2188 (1992)
    [126] G. Burdman and J. F. Donoghue, Phys. Lett. B, 280: 287 (1992)
    [127] A. F. Falk and M. E. Luke, Phys. Lett. B, 292: 119 (1992)
    [128] C. Isola, M. Ladisa, G. Nardulli, and P. Santorelli, Phys. Rev. D, 68: 114001 (2003)
    [129] M. Bando, T. Kugo, and K. Yamawaki, Phys. Rept., 164: 217 (1988)
    [130] D. Coffman et al (MARK-III Collaboration), Phys. Rev. D, 38: 2695 (1988); 40: 3788 (1989)
    [131] J. Jousset et al (DM2 Collaboration), Phys. Rev. D, 41: 1389 (1990)
    [132] N. A. Tornqvist, Nuovo Cim. A, 107: 2471 (1994)
    [133] N. A. Tornqvist, Z. Phys. C, 61: 525 (1994)
    [134] M. P. Locher, Y. Lu, and B. S. Zou, Z. Phys. A, 347: 281 (1994)
    [135] X. Q. Li, D. V. Bugg, and B. S. Zou, Phys. Rev. D, 55: 1421 (1997)
    [136] N. Moiseyev Phys. Rept., 302: 212-293 (1988)
    [137] J.-Y. Guo, M. Yu, J. Wang, B.-M. Yao, and P. Jiao, Comput. Phys. Commun. 181}: 550 (2010)
    [138] Q. Liu, Z.-M. Niu, and J.-Y. Guo, Phys. Rev. A, 87: 052122 (2013)
    [139] J. Y. Guo, X. Z. Fang, P. Jiao, J. Wang, and B. M. Yao, Phys. Rev. C, 82: 034318 (2010)
    [140] Q. Liu, J. Y. Guo, Z. M. Niu, and S. W. Chen, Phys. Rev. C, 86: 054312 (2012)
    [141] A. D. Alhaidari, H. A. Yamani, and M. S. Abdelmonem, Phys. Rev. A, 63: 062708 (2001)
    [142] Y. R. Liu and Z. Y. Zhang, Phys. Rev. C, 80: 015208 (2009)
    [143] N. Li and S. L. Zhu, Phys. Rev. D, 86: 074022 (2012)
    [144] J. He, Phys. Rev. D, 92: 034004 (2015)
    [145] S. Ohkoda, Y. Yamaguchi, S. Yasui, K. Sudoh, and A. Hosaka, Phys. Rev. D, 86: 014004 (2012)

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Ming-Zhu Liu, Duo-Jie Jia and Dian-Yong Chen. Possible hadronic molecular states composed of S-wave heavy-light mesons[J]. Chinese Physics C, 2017, 41(5): 053105. doi: 10.1088/1674-1137/41/5/053105
Ming-Zhu Liu, Duo-Jie Jia and Dian-Yong Chen. Possible hadronic molecular states composed of S-wave heavy-light mesons[J]. Chinese Physics C, 2017, 41(5): 053105.  doi: 10.1088/1674-1137/41/5/053105 shu
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Received: 2016-11-30
Revised: 2017-01-05
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    Supported by NSFC (11375240, 11565023)

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Possible hadronic molecular states composed of S-wave heavy-light mesons

    Corresponding author: Duo-Jie Jia,
    Corresponding author: Dian-Yong Chen,
  • 1.  Institute of Theoretical Physics, College of Physics and Electronic Engineering, Northwest Normal University,Lanzhou 730070, China
  • 2.  Department of Physics, Southeast University, Nanjing 210094, China
  • Received Date: 2016-11-30
  • Accepted Date: 2017-01-05
  • Available Online: 2017-05-05
Fund Project:  Supported by NSFC (11375240, 11565023)

Abstract: We perform a systematical study of possible molecular states composed of the S wave heavy light mesons, where the S-D mixing and η-η' mixing are explicitly included. Our calculation indicates that the observed X(3872) could be a loosely shallow molecular state composed of DD* +h.c, while neither Zc(3900)/Zc(4020) nor Zb(10610)/Zb(10650) is supported to be a molecule. Some observed possible molecular states are predicted, which could be searched for by further experimental measurements.

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