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(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).
      PCAS:
  • 加载中

  • 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

  • Access

    加载中

Get Citation
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
Milestone
Received: 2017-04-11
Fund

    Supported by National Natural Science Foundation of China (11475111)

Article Metric

Article Views(1445)
PDF Downloads(20)
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:

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).

    HTML

Reference (31)

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