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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(8) : 083107 DOI: 10.1088/1674-1137/41/8/083107

Study of radially excited Ds(21S0) and Ds(3P)

  • 1.

     Department of Physics, Shanghai University, Shanghai 200444, China

  • The unobserved JP=0- radial excitation Ds(21S0) is anticipated to have mass 2650 MeV (denoted as Ds(2650)). Study of hadronic production is an important way to identify highly excited states. We study hadronic production of Ds(2650) from higher excited resonances in a 3P0 model. Relevant hadronic partial decay widths are found to be very small, which implies it is difficult to observe Ds(2650) in hadronic decays of higher excited resonances. Hadronic decay widths of radially excited Ds(3P) have also been estimated. The total decay widths of four Ds(3P) are large, but the branching ratios in the Ds(2650)η channel are very small, which implies that it seems impossible to observe Ds(2650) in hadronic decays of Ds(3P). The dominant decay channels of the four Ds(3P) have been pointed out, and D1(2420), D1(2430), m D2*(2460), m D(2550), m D(2600), m (11D2)D(2750) and m D3*(2760) are possible to observe in hadronic production from Ds(3P).
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  • References

    [1] C. Patrignani et al (Particle Data Group), Chin. Phys. C, 40:100001 (2016)
    [2] S. Godfrey and N. Isgur, Phys. Rev. D, 32:189 (1985)
    [3] P.del Amo Sanchez et al (BABAR Collaboration), Phys. Rev. D, 82:111101 (2010)
    [4] R. Aaij et al (LHCb collaboration), J. High Energy Phys., 09:145 (2013)
    [5] R. Aaij et al (LHCb collaboration), Phys. Rev. D, 91:092002 (2015)
    [6] R. Aaij et al (LHCb collaboration), Phys. Rev. D, 92:032002 (2015)
    [7] J. Brodzicka et al (Belle Collaboration), Phys. Rev. Lett., 100:092001 (2008)
    [8] B. Aubert et al (BaBar Collaboration), Phys. Rev. D, 80:092003 (2009)
    [9] R. Aaij et al (LHCb collaboration), Phys. Rev. D, 90:072003 (2014)
    [10] R. Aaij et al (LHCb Collaboration), Phys. Rev. Lett., 113:162001 (2014)
    [11] P. Colangelo, F. De Fazio, F. Giannuzzi, and S. Nicotri, Phys. Rev. D, 86:054024 (2012)
    [12] S. Godfrey and K. Moats, Phys. Rev. D, 93:034035 (2016)
    [13] Zhi-Feng Sun, Jie-Sheng Yu, Xiang Liu, and Takayuki Matsuki, Phys. Rev. D, 82:111501(R) (2010)
    [14] Xian-Hui Zhong, Phys. Rev. D, 82:114014 (2010)
    [15] Zhi-Gang Wang, Phys. Rev. D, 83:014009 (2011)
    [16] Bing Chen, Ling Yuan, and Ailin Zhang, Phys. Rev. D, 83:114025 (2011)
    [17] Bing Chen, Xiang Liu, and Ailin Zhang, Phys. Rev. D, 92:034005 (2015)
    [18] Jing Ge, Dan-Dan Ye, and Ailin Zhang, Eur. Phys. J. C, 75:178 (2015)
    [19] Ze Zhao, Yu Tian, and Ailin Zhang, Phys. Rev. D, 94:114035 (2016)
    [20] Hua-Xing Chen, Wei Chen, Xiang Liu, Yan-Rui Liu, and Shi-Lin Zhu, arXiv:1609.08928
    [21] Qin-Tao Song, Dian-Yong Chen, Xiang Liu, and Takayuki Matsuki, Phys. Rev. D, 92:074011 (2015)
    [22] Qin-Tao Song, Dian-Yong Chen, Xiang Liu, and Takayuki Matsuki, Phys. Rev. D, 91:054031 (2015)
    [23] A.V. Evdokimov et al (SELEX Collaboration), Phys. Rev. Lett., 93:242001 (2004)
    [24] B. Aubert et al (BABAR Collaboration), arXiv:hep-ex/0408087
    [25] S. Godfrey and K. Moats, Phys Rev. D, 90:117501 (2014)
    [26] L. Micu, Nucl. Phys. B, 10:521 (1969)
    [27] A. Le Yaouanc, L. Oliver, O. Pne, and J.C. Raynal, Phys. Rev. D, 8:2223 (1973); 9, 1415 (1974); 11, 1272 (1975)
    [28] A. Le Yaouanc, L. Oliver, O. Pne, and J.C. Raynal, Phys. Lett. B, 71:397 (1977); 72, 57 (1977)
    [29] A. Le Yaouanc, L. Oliver, O. Pne, and J.C. Raynal, Hadron Transitions in the Quark Model (New York:Gordon and Breach Science Publishers, 1987)
    [30] Ze Zhao, Dan-Dan Ye, and Ailin Zhang, Phys. Rev. D, 94:114020 (2016)
    [31] Ling Yuan, Bing Chen, and Ailin Zhang, arXiv:1203.0370

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Yu Tian, Ze Zhao and Ai-Lin Zhang. Study of radially excited Ds(21S0) and Ds(3P)[J]. Chinese Physics C, 2017, 41(8): 083107. doi: 10.1088/1674-1137/41/8/083107
Yu Tian, Ze Zhao and Ai-Lin Zhang. Study of radially excited Ds(21S0) and Ds(3P)[J]. Chinese Physics C, 2017, 41(8): 083107.  doi: 10.1088/1674-1137/41/8/083107 shu
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Received: 2017-04-11
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    Supported by National Natural Science Foundation of China (11475111)

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Study of radially excited Ds(21S0) and Ds(3P)

    Corresponding author: Yu Tian,
    Corresponding author: Ze Zhao,
    Corresponding author: Ai-Lin Zhang,
  • 1. Department of Physics, Shanghai University, Shanghai 200444, China
  • Received Date: 2017-04-11
  • Available Online: 2017-08-05
Fund Project:  Supported by National Natural Science Foundation of China (11475111)

Abstract: The unobserved JP=0- radial excitation Ds(21S0) is anticipated to have mass 2650 MeV (denoted as Ds(2650)). Study of hadronic production is an important way to identify highly excited states. We study hadronic production of Ds(2650) from higher excited resonances in a 3P0 model. Relevant hadronic partial decay widths are found to be very small, which implies it is difficult to observe Ds(2650) in hadronic decays of higher excited resonances. Hadronic decay widths of radially excited Ds(3P) have also been estimated. The total decay widths of four Ds(3P) are large, but the branching ratios in the Ds(2650)η channel are very small, which implies that it seems impossible to observe Ds(2650) in hadronic decays of Ds(3P). The dominant decay channels of the four Ds(3P) have been pointed out, and D1(2420), D1(2430), m D2*(2460), m D(2550), m D(2600), m (11D2)D(2750) and m D3*(2760) are possible to observe in hadronic production from Ds(3P).

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