×
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

Re-study of the contribution of scalar potential and spectra of cc, bb and bc(bc) families

  • We indicated in our previous work that for QED the role of the scalar potential which appears at the loop level is much smaller than that of the vector potential and is in fact negligible. But the situation is different for QCD, one reason is that the loop effects are more significant because αs is much larger than α, and second the non-perturbative QCD effects may induce a sizable scalar potential. In this work, we study phenomenologically the contribution of the scalar potential to the spectra of charmonia, bottomonia and bc(bc) families. Taking into account both vector and scalar potentials, by fitting the well measured charmonia and bottomonia spectra, we re-fix the relevant parameters and test them by calculating other states of not only the charmonia and bottomonia families, but also the bc family. We also consider the Lamb shift of the spectra.
      PCAS:
  • 加载中
  • [1] Quigg C, Rosner J L. Phys. Rept., 2004, 56: 1672 Brambilla N et al. (Quarkonium Working Group).arXiv:hep-ph/04121583 ZHANG F, FU B, CHEN J. Phys. Rev. A, 2008, 78:040101(R)4 KE H W, LI Z, CHEN J L, DING Y B, LI X Q. Int. J.Mod. Phys. A, 2010, 25: 11235 ZHANG Y J, CHAO K T. Phys. Rev. Lett., 2007, 98:0920036 GONG B,WANG J X. Phys. Rev. Lett., 2009, 102: 1620037 Leviatan A. Phys. Rev. Lett., 2004, 92: 202501; 219902;Int. J. Mod. Phys. E, 2005, 14: 111; Phys. Rev. Lett.,2009, 103: 0425028 YUAN X H, KE H W, LI X Q. arXiv:1011.4629 [hep-ph]9 Lucha W, Rupprecht H, Schoberl F F. Phys. Rev. D, 1992,46: 108810 Lucha W, Schoberl F F, Gromes D. Phys. Rept., 1991, 200:12711 DING Y B, QIN D H, CHAO K T. Phys. Rev. D, 1991,44: 356212 Hoang A H, Manohar A V, Stewart I W. Phys. Rev. D,2001, 64: 01403313 Titard S, Yndurain F J. Phys. Rev. D, 1994, 49: 6007;Phys. Rev. D, 1995, 51: 634814 Brambilla N, Pineda A, Soto J, Vairo A. Nucl. Phys. B,2000, 566: 275; Brambilla N, Pineda A, Soto J, Vairo A.Rev. Mod. Phys., 2005, 77: 142315 KE H W, LI X Q. Sci. China G, 2010, 53: 201916 Eichten E et al. Phys. Rev. Lett., 1975, 34: 369; Phys. Rev.D, 1978, 17: 3090; Phys. Rev. D, 1980, 21: 20317 CAI C H, LEI L. HEP NP, 2003, 27(11): 100518 Silbar R, Goldman T. [arXiv:1001.2514v1]19 DING Y B, LI X Q, SHEN P N. Commun. Theor. Phys.,2000, 33: 61320 Nakamura K et al. (Particle Data Group). J. Phys. G, 2010,37: 07502121 Press William H et al. Numerical Recipes: the Art of Scienti c Computing. New York: Cambridge University Press,200722 DING H Q. Phys. Lett. B, 1988, 200: 13323 Bali G S, Schilling K. Phys. Rev. D, 1992, 46: 263624 Schnitzer H J. Phys. Rev. D, 1978, 18: 348225 Khadkikar S B, Gupta S K. Phys. Lett. B, 1983, 124: 523;Vinodkumar P C, Vijayakumar K B, Khadkikar S B. Pramana,1992, 39: 4726 Greiner W, Reinhardt J. Quantum Electrodynamics.Berlin: Springer, 199227 Pineda A, Yndurain F J. Phys. Rev. D, 1998, 58: 094022;Phys. Rev. D, 2000, 61: 07750528 Billoire A. Phys. Lett. B, 1980, 92: 34329 Fischler W. Nucl. Phys. B, 1977, 129: 15730 Peter M. Phys. Rev. Lett., 1997, 78: 60231 Schroder Y. Phys. Lett. B, 1999, 447: 321; Crater H W,Yoon J H, Wong C Y. Phys. Rev. D, 2009, 79: 03401132 Godfrey S. Phys. Rev. D, 2004, 70: 05401733 Ebert D, Faustov R N, Galkin V O. Phys. Rev. D, 2003,67: 01402734 KE H W, WANG G L, LI X Q, CHANG C H. Sci. ChinaG, 2010, 53: 202535 Franklin J. Mod. Phys. Lett. A, 1999, 14: 2409; de CastroA S, Franklin J. arXiv:hep-ph/0011137; Int. J. Mod. Phys.A, 2000, 15: 4355;36 van Beveren E, Dullemond C, Rupp G. Phys. Rev. D, 1980,21: 772; 22: 787; van Beveren E, Rupp G. arXiv:1009.1778[hep-ph]; arXiv:1009.3395 [hep-ph]37 Eichten E, Gottfried K, Kinoshita T, Lane K D, Yan T M.Phys. Rev. D, 1978, 17: 3090; 1980, 21: 313; Phys. Rev.D, 1980, 21: 20338 Barchielli A, Brambilla N, Prosperi G M. Nuovo Cim. A,1990, 103: 5939 Cohen-Tannoudji C, Diu B, Laloe F. Quantum Mechanics, 2 Volume Set. NewYork: John Wiley Sons, Inc., 200640 McClary R, Byers N. Phys. Rev. D, 1983, 28: 1692
  • 加载中

Get Citation
YUAN Xu-Hao, KE Hong-Wei, DING Yi-Bing and LI Xue-Qian. Re-study of the contribution of scalar potential and spectra of cc, bb and bc(bc) families[J]. Chinese Physics C, 2012, 36(2): 117-126. doi: 10.1088/1674-1137/36/2/003
YUAN Xu-Hao, KE Hong-Wei, DING Yi-Bing and LI Xue-Qian. Re-study of the contribution of scalar potential and spectra of cc, bb and bc(bc) families[J]. Chinese Physics C, 2012, 36(2): 117-126.  doi: 10.1088/1674-1137/36/2/003 shu
Milestone
Received: 2011-05-06
Revised: 2011-07-29
Article Metric

Article Views(2274)
PDF Downloads(323)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
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:

Re-study of the contribution of scalar potential and spectra of cc, bb and bc(bc) families

    Corresponding author: KE Hong-Wei,

Abstract: We indicated in our previous work that for QED the role of the scalar potential which appears at the loop level is much smaller than that of the vector potential and is in fact negligible. But the situation is different for QCD, one reason is that the loop effects are more significant because αs is much larger than α, and second the non-perturbative QCD effects may induce a sizable scalar potential. In this work, we study phenomenologically the contribution of the scalar potential to the spectra of charmonia, bottomonia and bc(bc) families. Taking into account both vector and scalar potentials, by fitting the well measured charmonia and bottomonia spectra, we re-fix the relevant parameters and test them by calculating other states of not only the charmonia and bottomonia families, but also the bc family. We also consider the Lamb shift of the spectra.

    HTML

Reference (1)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return