×
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

Decay rates and electromagnetic transitions of heavy quarkonia

  • The electromagnetic radiative transition widths for heavy quarkonia, as well as digamma and digluon decay widths, are computed in the framework of the extended harmonic confinement model (ERHM) and Coulomb plus power potential (CPPv) with varying potential index v. The outcome is compared with the values obtained from other theoretical models and experimental results. While the mass spectra, digamma and digluon widths from ERHM as well as CPPv=1 are in good agreement with experimental data, the electromagnetic transition widths span over a wide range for the potential models considered here making it difficult to prefer a particular model over the others because of the lack of experimental data for most transition widths.
      PCAS:
  • 加载中
  • [1] Wiedner U. Progress in Particle and Nucl. Phys., 2011, 66: 477
    [2] Brambilla N et al. hep-ph/0412158
    [3] Caswell W E, Lepage G P. Phys. Lett. B, 1986, 167: 437
    [4] Bodwin G T, Braaten E, Lepage G P. Phys. Rev. D, 1995, 51: 1125; 1997, 55: 5853
    [5] Pineda A, Soto J. Nucl. Phys. Proc. Suppl., 1998, 64: 428. [arXiv:hep-ph/9707481]
    [6] Brambilla N, Pineda A, Soto J, Vairo A. Nucl. Phys. B, 2000, 566: 275. [arXiv:hep-ph/9907240]
    [7] Brambilla N et al. Eur. Phys. J. C, 2011, 71: 1534
    [8] Mitchell R E et al. (CLEO collaboration). Phys. Rev. Lett., 2009, 102: 011801; 2011, 106: 159903
    [9] Brambilla N, JIA Y, Vairo A. Phys. Rev. D, 2006, 73: 054005
    [10] Barnes T, Godfrey S, Swanon E S. Phys. Rev. D, 2005, 72: 054026
    [11] Vinodkumar P C, Pandya J N, Bannur V M, Khadkikar S B. Eur. Phys. J., A, 1999, 4: 83
    [12] Pandya J N, Vinodkumar P C. Pramana J. Phys., 2001, 57: 821
    [13] Rai A K, Pandya J N, Vinodkumar P C. Eur. Phys. Jnl. A, 2008, 38: 77; Jnl. Phys. G, 2005, 31: 1453
    [14] Rai A K, Parmar R H, Vinodkumar P C. Jnl. Phys. G, 2002, 28: 2275
    [15] Rai A K, Vinodkumar P C. Pramana J. Phys., 2006, 66: 953
    [16] Rai A K, Patel B, Vinodkumar P C. Phys. Rev. C, 2008, 78: 055202
    [17] Rai A K, Pandya J N, Vinodkumar P C. Nucl. Phys. A, 2007, 782: 406; Indian J. Phys. A, 2006, 80: 387
    [18] Buchmüller W, Tye S H H. Phys. Rev. D, 1981, 24: 132
    [19] Khadkikar S B, Gupta S K. Phys. Lett. B, 1983, 124: 523
    [20] Gupta S K, Khadkikar S B. Phys. Rev. D, 1987, 36: 307
    [21] Jena S N, Behera M R, Panda S. Phys. Rev. D, 1996, 54: 11
    [22] Olive K A et al. (Particle Data Group). Chin. Phys. C, 2014, 38: 090001
    [23] Parmar A et al. Nucl. Phys. A, 2010, 848: 299
    [24] Patel B, Vinodkumar P C. J. Phys. G: Nucl. Part. Phys., 2009 36: 035003
    [25] Kwong Waikwok et al. Phys. Rev. D, 1988, 37: 3210
    [26] Barbieri R, Caffo M, Gatto R, Remiddi E. Nucl. Phys. B, 1981, 192: 61
    [27] Mangano M, Petrelli A. Phys. Lett. B, 1945, 352: 445
    [28] Lansberg J P, Pham T N. Phys. Rev. D, 2009, 79: 094016
    [29] Shah M, Parmar A, Vinodkumar P C. Phys. Rev. D, 2012, 86: 034015
    [30] B. Quing Li, K. Ta Chao. Phys. Rev. D, 2009, 79: 094004; Bai Quing Li, Kung- Ta Chao. Commun. Theor. Phys., 2009, 52: 653
    [31] Schuler G A, Berends F A, van Gulik R. Nucl. Phys. B, 1998, 523: 423
    [32] Ahmady M R, Mendel R R. Phys. Rev. D, 1995, 51: 141
    [33] Laverty J T, Radford S F, Repko W W. arXiv:0901.3917 [hep-ph]
    [34] Ebert D, Faustov N, Galkin V O. Phys. Rev. D, 2003, 67: 014027
    [35] Radford S F, Repko W W. Phys. Rev. D, 2007, 75: 074031
    [36] Brambilla N et al. CERN Yellow Report 2005-005. arxiv://hep-ph/0412158
    [37] Anisovich V V, Dakhno L G, Matveev M A, Nikonov V A, Sarantsev A V. Phys. Atom. Nucl., 2007, 70: 63
    [38] Lähde T A. Nucl. Phys. A, 2003, 714: 183
    [39] Gupta Suraj N, Johnson James M, Repko Wayne W. Phys. Rev. D, 1996, 54: 2075. arXiv:hep-ph/9606349
  • 加载中

Get Citation
J. N. Pandya, N. R. Soni, N. Devlani and A. K. Rai. Decay rates and electromagnetic transitions of heavy quarkonia[J]. Chinese Physics C, 2015, 39(12): 123101. doi: 10.1088/1674-1137/39/12/123101
J. N. Pandya, N. R. Soni, N. Devlani and A. K. Rai. Decay rates and electromagnetic transitions of heavy quarkonia[J]. Chinese Physics C, 2015, 39(12): 123101.  doi: 10.1088/1674-1137/39/12/123101 shu
Milestone
Received: 2014-12-23
Revised: 2015-06-26
Fund

    Supported by University Grants Commission, India for Major Research Project F. No.42-775/2013(SR) (J N Pandya) and Dept. of Science and Technology, India, under SERC fast track scheme SR/FTP/PS-152/2012 (A K Rai)

Article Metric

Article Views(1560)
PDF Downloads(31)
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:

Decay rates and electromagnetic transitions of heavy quarkonia

    Corresponding author: J. N. Pandya,
Fund Project:  Supported by University Grants Commission, India for Major Research Project F. No.42-775/2013(SR) (J N Pandya) and Dept. of Science and Technology, India, under SERC fast track scheme SR/FTP/PS-152/2012 (A K Rai)

Abstract: The electromagnetic radiative transition widths for heavy quarkonia, as well as digamma and digluon decay widths, are computed in the framework of the extended harmonic confinement model (ERHM) and Coulomb plus power potential (CPPv) with varying potential index v. The outcome is compared with the values obtained from other theoretical models and experimental results. While the mass spectra, digamma and digluon widths from ERHM as well as CPPv=1 are in good agreement with experimental data, the electromagnetic transition widths span over a wide range for the potential models considered here making it difficult to prefer a particular model over the others because of the lack of experimental data for most transition widths.

    HTML

Reference (39)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return