Impact factor of Chinese Physics C is 3.6 in 2023 Impact factor of Chinese Physics C is 3.6 in 2022 2021 Impact Factor 2.944
Advanced Search
×
近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。
本刊再次郑重声明：
（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。
（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。
                  
《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.
      PCAS:
  • 加载中

  • 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)

  • Access

    加载中

Get Citation
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
Milestone
Received: 2016-11-30
Revised: 2017-01-05
Fund

    Supported by NSFC (11375240, 11565023)

Article Metric

Article Views(1447)
PDF Downloads(42)
Cited by(0)
Policy on re-use
To reuse of Open Access content published by CPC, for content published under the terms of the Creative Commons Attribution 3.0 license (“CC CY”), the users don’t need to request permission to copy, distribute and display the final published version of the article and to create derivative works, subject to appropriate attribution.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

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.

    HTML

Reference (145)

目录

Link
IOPScience
SCOAP3
arXiv
Chinese Physical Society
Journal information
Introduction
Editorial Board
Others
Subscribe
Contact us
QQ: 1307685413
Tel: +86-010-88235947
Fax: +86-010-88233126
E-mail: cpc@ihep.ac.cn

  • CPC Website

  • IOP Website

  • CPC WeChat

Copyright © Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 京ICP备05002789号-1

Supported by: Beijing Renhe Information Technology Co. Ltd  E-mail: info@rhhz.net

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return