×
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

S-wave resonance contributions to B(s)0→ηc(2S+π-in the perturbative QCD factorization approach

  • By employing the perturbative QCD (PQCD) factorization approach, we study the quasi-two-body B(s)0→ ηc(2S+π- decays, where the pion pair comes from the S-wave resonance f0(X). The Breit-Wigner formula for the f0(500) and f0(1500) resonances and the Flatté model for the f0(980) resonance are adopted to parameterize the time-like scalar form factors in the two-pion distribution amplitudes. As a comparison, Bugg's model is also used for the wide f0(500) in this work. For decay rates, we found the following PQCD predictions:(a) B(Bs0→ηc(2S) f0(X)[π+π-]s)= ≤ ft (2.67-1.08+1.78)×10-5 when the contributions from f0(980) and f0(1500) are all taken into account; (b) B(B0→ηc(2S) f0(500)[π+π-]s)= ≤ ft (1.40 -0.56+0.92)×10-6 in the Breit-Wigner model and ≤ ft (1.53 +0.97-0.61 ight)×10-6 in Bugg's model.
      PCAS:
  • 加载中
  • [1] B. Aubert et al (BaBar collaboration), Phys. Rev. Lett., 90:091801(2003)
    [2] B. Aubert et al (BaBar Collaboration), Phys. Rev. D, 70:092001 (2004)
    [3] B. Aubert et al (BaBar Collaboration), Phys. Rev. D, 72:072003 (2005)
    [4] B. Aubert et al (BaBar Collaboration), Phys. Rev. D, 80:112001 (2009)
    [5] B. Aubert et al (BaBar Collaboration), Phys. Rev. D, 79:072006 (2009)
    [6] B. Aubert et al (BaBar Collaboration), Phys. Rev. D, 78:052005 (2008)
    [7] A. Garmash et al (Belle Collaboration), Phys. Rev. D, 75:012006 (2007)
    [8] A. Garmash et al (Belle Collaboration), Phys. Rev. Lett., 96:251803 (2006)
    [9] A. Garmash et al (Belle Collaboration), Phys. Rev. D, 71:092003 (2005)
    [10] J. Dalseno et al (Belle Collaboration), Phys. Rev. D, 79:072004 (2009)
    [11] R. Aaij et al (LHCb Collaboration), Phys. Rev. Lett., 111:101801 (2013)
    [12] R. Aaij et al (LHCb Collaboration), Phys. Rev. D, 90:112004 (2014)
    [13] R. Aaij et al (LHCb Collaboration), Phys. Rev. Lett., 112:011801 (2014)
    [14] R. Aaij et al (LHCb Collaboration), Phys. Rev. D, 86:052006 (2012)
    [15] R. Aaij et al (LHCb Collaboration), Phys. Rev. D, 89:092006 (2014)
    [16] R. Aaij et al (LHCb Collaboration), Phys. Rev. D, 87:052001 (2013)
    [17] R. Aaij et al (LHCb Collaboration), Phys. Rev. D, 90:012003 (2014)
    [18] R. Aaij et al (LHCb Collaboration), Phys. Lett. B, 742:38 (2015)
    [19] R. Aaij et al (LHCb Collaboration), Phys. Rev. D, 92:032002 (2015)
    [20] R. Aaij et al (LHCb Collaboration), Nucl. Phys. B, 871:403 (2013)
    [21] R. Aaij et al (LHCb Collaboration), arXiv:1702.08048
    [22] A. Furman, R. Kamiński, L. Leśniak, and B. Loiseau, Phys. Lett. B, 622:207 (2005)
    [23] B. El-Bennich et al, Phys. Rev. D, 74:114009 (2006)
    [24] B. El-Bennich et al, Phys. Rev. D, 79:094005 (2009); 83:039903 (2011)(E)
    [25] O. Leitner, J. P. Dedonder, B. Loiseau, and R. Kamiński, Phys. Rev. D, 81:094033 (2010); 82:119906 (2010)(E)
    [26] J. P. Dedonder et al, Acta Phys. Polon. B, 42:2013 (2011)
    [27] H. Y. Cheng and K. C. Yang, Phys. Rev. D, 66:054015 (2002)
    [28] H. Y. Cheng, C. K. Chua, and A. Soni, Phys. Rev. D, 72:094003 (2005)
    [29] H. Y. Cheng, C. K. Chua, and A. Soni, Phys. Rev. D, 76:094006 (2007)
    [30] H. Y. Cheng and C. K. Chua, Phys. Rev. D, 88:114014 (2013)
    [31] H. Y. Cheng and C. K. Chua, Phys. Rev. D, 89:074025 (2014)
    [32] H. Y. Cheng, C. K. Chua, and Z. Q. Zhang, Phys. Rev. D, 94:094015 (2016)
    [33] Y. Li, Phys. Rev. D, 89:094007 (2014); Sci. China Phys. Mech. Astron.. 58:031001 (2015)
    [34] S. Krnkl, T. Mannel, and J. Virto, Nucl. Phys. B, 899, 247 (2015)
    [35] C. Wang, Z. H. Zhang, Z. Y. Wang, and X. H. Guo, Eur. Phys. J. C, 75:536 (2015)
    [36] Z. H. Zhang, X. H. Guo, and Y. D. Yang, Phys. Rev. D, 87:076007 (2013)
    [37] I. Bediaga and P. C. Magalh aes, arXiv:1512.09284
    [38] S. Fajfer, T. N. Pham, and A. Prapotnik, Phys. Rev. D, 70:034033 (2004)
    [39] C. H. Chen and H. n. Li, Phys. Lett. B, 561:258 (2003)
    [40] C. H. Chen and H. n. Li, Phys. Rev. D, 70:054006 (2004)
    [41] W. F. Wang, H. C. Hu, H. n. Li, and C. D. L, Phys. Rev. D, 89:074031 (2014)
    [42] W. F. Wang, H. n. Li, W. Wang, and C. D. L, Phys. Rev. D, 91:094024 (2015)
    [43] W. F. Wang and H. n. Li, Phys. Lett. B, 763:29 (2016)
    [44] Y. Li, A. J. Ma, W. F. Wang, and Z. J. Xiao, Eur. Phys. J. C, 76:675 (2016)
    [45] Z. Rui, Y. Li and W. F. Wang, Eur. Phys. J. C, 77:199 (2017)
    [46] A. J. Ma, Y. Li, W. F. Wang, and Z. J. Xiao, arXiv:1611.08786
    [47] Y. Li, A. J. Ma, W. F. Wang, and Z. J. Xiao, Phys. Rev. D, 95:056008 (2017)
    [48] M. Gronau and J. L. Rosner, Phys. Lett. B, 564:90 (2003)
    [49] G. Engelhard, Y. Nir, and G. Raz, Phys. Rev. D, 72:075013 (2005)
    [50] M. Gronau and J. L. Rosner, Phys. Rev. D, 72:094031 (2005)
    [51] M. Imbeault and D. London, Phys. Rev. D, 84:056002 (2011)
    [52] M. Gronau, Phys. Lett. B, 727:136 (2013)
    [53] B. Bhattacharya, M. Gronau, and J. L. Rosner, Phys. Lett. B, 726:337 (2013)
    [54] B. Bhattacharya et al, Phys. Rev. D, 89:074043 (2014)
    [55] D. Xu, G. N. Li, and X. G. He, Phys. Lett. B, 728:579 (2014)
    [56] D. Xu, G. N. Li, and X. G. He, Int. J. Mod. Phys. A, 29:1450011 (2014)
    [57] X. G. He, G. N. Li, and D. Xu, Phys. Rev. D, 91:014029 (2015)
    [58] I. Bediaga, T. Frederico, and O. Loureno, Phys. Rev. D, 89:094013 (2014)
    [59] J. H. A. Nogueira et al, Phys. Rev. D, 92:054010 (2015)
    [60] N. R. -L. Lorier, M. Imbeault, and D. London, Phys. Rev. D, 84:034040 (2011)
    [61] Y. Y. Keum, H. n. Li, and A. I. Sanda, Phys. Lett. B, 504:6 (2001); Phys. Rev. D, 63:054008 (2001); C. D. L, K. Ukai, and M. Z. Yang, Phys. Rev. D, 63:074009 (2001)
    [62] H. n. Li, Prog. Part. Nucl. Phys., 51:85 (2003) and references therein
    [63] D. Mller et al, Fortschr. Physik., 42:101 (1994)
    [64] M. Diehl, T. Gousset, B. Pire, and O. Teryaev, Phys. Rev. Lett., 81:1782 (1998); M. Diehl, T. Gousset, and B. Pire, Phys. Rev. D, 62:073014 (2000); P. Hagler, B. Pire, L. Szymanowski, and O. V. Teryaev, Eur. Phys. J. C, 26:261 (2002)
    [65] M. V. Polyakov, Nucl. Phys. B, 555:231 (1999)
    [66] A. G. Grozin, Sov. J. Nucl. Phys., 38:289-292 (1983); A. G. Grozin, Theor. Math. Phys., 69:1109-1121 (1986)
    [67] U. G. Meiner, and W. Wang, Phys. Lett. B, 730:336 (2014)
    [68] S. M. Flatt, Phys. Lett. B, 63:228 (1976)
    [69] D.V. Bugg, J. Phys. G, 34:151 (2007); Phys. Rev. D, 78:074023 (2014)
    [70] R. Garca-Martn, R. Kamiński, J. R. Pelez, J. Ruiz de Elvira, and F. J. Yndurin, Phys. Rev. D, 83:074004 (2011)
    [71] X. W. Kang, B. Kubis, C. Hanhart, and U. G. Mei ner, Phys. Rev. D, 89:053015 (2014)
    [72] S.-K. Choi et al (Belle Collaboration), Phys. Rev. Lett., 89:102001 (2002)
    [73] B. Aubert et al (BaBar Collaboration), Phys. Rev. Lett., 92:142002 (2004)
    [74] C. H. Chang and H. n. Li, Phys. Rev. D, 71:114008 (2005)
    [75] R. Zhou et al, Eur. Phys. J. C, 75:293 (2015)
    [76] C. Patrignani et al (Particle Data Group), Chin. Phys. C, 40:100001 (2016)
  • 加载中

Get Citation
Ai-Jun Ma, Ya Li, Wen-Fei Wang and Zhen-Jun Xiao. S-wave resonance contributions to B(s)0→ηc(2S+π-in the perturbative QCD factorization approach[J]. Chinese Physics C, 2017, 41(8): 083105. doi: 10.1088/1674-1137/41/8/083105
Ai-Jun Ma, Ya Li, Wen-Fei Wang and Zhen-Jun Xiao. S-wave resonance contributions to B(s)0→ηc(2S+π-in the perturbative QCD factorization approach[J]. Chinese Physics C, 2017, 41(8): 083105.  doi: 10.1088/1674-1137/41/8/083105 shu
Milestone
Received: 2017-03-17
Fund

    Supported by National Natural Science Foundation of China (11235005,11547038)

Article Metric

Article Views(1846)
PDF Downloads(19)
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:

S-wave resonance contributions to B(s)0→ηc(2S+π-in the perturbative QCD factorization approach

    Corresponding author: Ai-Jun Ma,
    Corresponding author: Ya Li,
    Corresponding author: Wen-Fei Wang,
    Corresponding author: Zhen-Jun Xiao,
  • 1.  Department of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing 210023, China
  • 2.  Institute of Theoretical Physics, Shanxi University, Taiyuan, Shanxi 030006, China
  • 3. Department of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing 210023, China
  • 4. Jiangsu Key Laboratory for Numerical Simulation of Large Scale Complex Systems, Nanjing Normal University, Nanjing 210023, China
Fund Project:  Supported by National Natural Science Foundation of China (11235005,11547038)

Abstract: By employing the perturbative QCD (PQCD) factorization approach, we study the quasi-two-body B(s)0→ ηc(2S+π- decays, where the pion pair comes from the S-wave resonance f0(X). The Breit-Wigner formula for the f0(500) and f0(1500) resonances and the Flatté model for the f0(980) resonance are adopted to parameterize the time-like scalar form factors in the two-pion distribution amplitudes. As a comparison, Bugg's model is also used for the wide f0(500) in this work. For decay rates, we found the following PQCD predictions:(a) B(Bs0→ηc(2S) f0(X)[π+π-]s)= ≤ ft (2.67-1.08+1.78)×10-5 when the contributions from f0(980) and f0(1500) are all taken into account; (b) B(B0→ηc(2S) f0(500)[π+π-]s)= ≤ ft (1.40 -0.56+0.92)×10-6 in the Breit-Wigner model and ≤ ft (1.53 +0.97-0.61 ight)×10-6 in Bugg's model.

    HTML

Reference (76)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return