Spectroscopy and decay properties of charmonium

  • The mass spectra of charmonium are investigated using a Coulomb plus linear (Cornell) potential. Gaussian wave functions in position space as well as in momentum space are employed to calculate the expectation values of potential and kinetic energy respectively. Various experimental states (X(4660)(53S1), X(3872)(23P1), X(3900)(21P1), X(3915)(23P0) and X(4274)(33P1) etc.) are assigned as charmonium states. We also study the Regge trajectories, pseudoscalar and vector decay constants, electric and magnetic dipole transition rates, and annihilation decay widths for charmonium states.
      PCAS:
  • 加载中
  • [1] J.J. Aubert et al (E598), Phys. Rev. Lett., 33:1404 (1974)
    [2] J.E. Augustin et al (SLAC-SP-017), Phys. Rev. Lett., 33:1406 (1974)
    [3] N. Brambilla, S. Eidelman, B. Heltsley, R. Vogt, G. Bodwin et al, Eur. Phys. J. C, 71:1534 (2011)
    [4] C. Patrignani, P. D. Group, Chinese Physics C, 40:100001 (2016)
    [5] J. Siegrist et al, Phys. Rev. Lett., 36:700 (1976)
    [6] R. Brandelik et al (DASP), Phys. Lett. B, 76:361 (1978)
    [7] E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, and T. M. Yan, Phys. Rev. D, 21:203 (1980)
    [8] R. Aaij et al (LHCb), Phys. Rev. Lett., 111:101805 (2013)
    [9] X. L. Wang et al (Belle), Phys. Rev. Lett., 99:142002 (2007)
    [10] G. Pakhlova et al (Belle), Phys. Rev. Lett., 101:172001 (2008)
    [11] P. A. Rapidis et al, Phys. Rev. Lett., 39:526 (1977)
    [12] W. Bacino et al, Phys. Rev. Lett., 40:671 (1978)
    [13] G. S. Abrams et al, Phys. Rev. D, 21:2716 (1980)
    [14] M. Ablikim et al (BES), Phys. Lett. B, 652:238 (2007)
    [15] V. V. Anashin et al, Phys. Lett. B, 711:292 (2012)
    [16] K. Abe et al (Belle), Phys. Rev. Lett., 98:082001 (2007)
    [17] P. Pakhlov et al (Belle), Phys. Rev. Lett., 100:202001 (2008)
    [18] W. Sreethawong, K. Xu, Y. Yan (2013), 1306.2780
    [19] Z. H. Wang, Y. Zhang, L. Jiang, T. H. Wang, Y. Jiang, and G. L. Wang, Eur. Phys. J. C, 77(1):43 (2017)
    [20] V. Bhardwaj et al (Belle), Phys. Rev. Lett., 111(3):032001 (2013)
    [21] M. Ablikim et al (BESⅢ), Phys. Rev. Lett., 115(1):011803 (2015)
    [22] S. K. Choi et al (Belle), Phys. Rev. Lett., 91:262001 (2003)
    [23] D. Acosta et al (CDF), Phys. Rev. Lett., 93:072001 (2004)
    [24] V.M. Abazov et al (D0), Phys. Rev. Lett., 93:162002 (2004)
    [25] B. Aubert et al (BaBar), Phys. Rev. D, 71:071103 (2005)
    [26] S.K. Choi et al, Phys. Rev. D, 84:052004 (2011)
    [27] T. Aaltonen et al (CDF), Phys. Rev. Lett., 103:152001 (2009)
    [28] B. Aubert et al (BaBar), Phys. Rev. D, 77:111101 (2008)
    [29] A. Abulencia et al (CDF), Phys. Rev. Lett., 98:132002 (2007)
    [30] M. Ablikim et al (BESⅢ), Phys. Rev. Lett., 112(9):092001 (2014)
    [31] T. Barnes, S. Godfrey, Phys. Rev. D, 69:054008 (2004)
    [32] S. K. Choi et al (Belle Collaboration), Phys. Rev. Lett., 94:182002 (2005)
    [33] P. del Amo Sanchez et al (BaBar), Phys. Rev. D, 82:011101 (2010)
    [34] J.P. Lees et al (BaBar), Phys. Rev. D, 86:072002 (2012), 1207.2651
    [35] X. Liu, Z. G. Luo, and Z. F. Sun, Phys. Rev. Lett., 104:122001 (2010)
    [36] Z. Y. Zhou, Z. Xiao, and H. Q. Zhou, Phys. Rev. Lett., 115(2):022001 (2015)
    [37] S. Uehara et al (Belle), Phys. Rev. Lett., 96:082003 (2006)
    [38] B. Aubert et al (BaBar), Phys. Rev. D, 81:092003 (2010)
    [39] M. Ablikim et al (BESⅢ), Phys. Rev. Lett., 110:252001 (2013)
    [40] Z. Q. Liu et al (Belle), Phys. Rev. Lett., 110:252002 (2013)
    [41] T. Xiao, S. Dobbs, A. Tomaradze, and K. K. Seth, Phys. Lett. B, 727:366 (2013)
    [42] M. Ablikim et al (BESⅢ), Phys. Rev. D, 92(9):092006 (2015)
    [43] T. Aaltonen et al (CDF), Phys. Rev. Lett., 102:242002 (2009)
    [44] S. Chatrchyan et al (CMS), Phys. Lett. B, 734:261 (2014)
    [45] V.M. Abazov et al (D0), Phys. Rev. Lett., 115(23):232001 (2015)
    [46] V.M. Abazov et al (D0), Phys. Rev. D, 89(1):012004 (2014)
    [47] X. Liu, S. L. Zhu, Phys. Rev. D, 80:017502 (2009); Phys. Rev.D, 85:019902 (2012)
    [48] T. Branz, T. Gutsche, and V. E. Lyubovitskij, Phys. Rev. D, 80:054019 (2009)
    [49] R. M. Albuquerque, M. E. Bracco, M. Nielsen, Phys. Lett. B, 678:186 (2009)
    [50] G. J. Ding, Eur. Phys. J. C, 64:297 (2009)
    [51] F. Stancu, J. Phys. G, 37:075017 (2010)
    [52] Z. G. Wang, Y. F. Tian, Int. J. Mod. Phys. A, 30:1550004 (2015)
    [53] V. V. Anisovich, M. A. Matveev, A. V. Sarantsev, and A. N. Semenova, Int. J. Mod. Phys. A, 30(32):1550186 (2015)
    [54] Z. G. Wang, Eur. Phys. J. C, 63:115 (2009)
    [55] N. Mahajan, Phys. Lett. B, 679:228 (2009)
    [56] R. Aaij et al (LHCb), Phys. Rev. D, 85:091103 (2012)
    [57] J. P. Lees et al (BaBar), Phys. Rev. D, 89(11):112004 (2014)
    [58] T. Aaltonen et al (CDF), Mod. Phys. Lett. A, 32(26):1750139 (2017)
    [59] R. Aaij et al (LHCb), Phys. Rev. D, 95(1):012002 (2017)
    [60] Q. F. L, Y. B. Dong, Phys. Rev. D, 94(7):074007 (2016)
    [61] T. Bhavsar, M. Shah, and P. C. Vinodkumar, Eur. Phys. J. C, 78(3):227 (2018)
    [62] P. Gonzlez, Phys. Rev. D, 92:014017 (2015)
    [63] P. Guo, T. Ypez-Martnez, A. P. Szczepaniak, Phys. Rev. D, 89(11):116005 (2014)
    [64] H. W. Ke, X. Q. Li, and Y. L. Shi, Phys. Rev. D, 87(5):054022 (2013)
    [65] D. Ebert, R. Faustov, and V. Galkin, Mod. Phys. Lett. A, 17:803 (2002)
    [66] N. Brambilla, eConf, C0610161:004 (2006), hep-ph/0702105
    [67] F. De Fazio, Phys. Rev. D, 79:054015 (2009); Phys. Rev.D, 83:099901 (2011)
    [68] G. C. Donald, C. Davies et al, Phys. Rev. D, 86:094501 (2012), 1208.2855
    [69] L. Liu, G. Moir, Peardon et al (Hadron Spectrum), JHEP, 07:126 (2012)
    [70] S. L. Zhu, Y. B. Dai, Phys. Rev. D, 59:114015 (1999)
    [71] V. A. Beilin, A. V. Radyushkin, Nucl. Phys.B, 260:61 (1985)
    [72] S. Godfrey, N. Isgur, Phys. Rev. D, 32:189 (1985)
    [73] T. Barnes, S. Godfrey, and E. S. Swanson, Phys. Rev. D, 72:054026 (2005)
    [74] B. Q. Li, C. Meng, and K. T. Chao (2012), 1201.4155
    [75] B. Q. Li, K. T. Chao, Phys. Rev. D, 79:094004 (2009)
    [76] L. Cao, Y. C. Yang, and H. Chen, Few Body Syst., 53:327 (2012)
    [77] J. Segovia, A. M. Yasser, D. R. Entem, and F. Fernandez, Phys. Rev. D, 78:114033 (2008)
    [78] E. Eichten et al, Phys. Rev. D, 17(11):3090 (1978)
    [79] W. J. Deng, H. Liu, L. C. Gui, X. H. Zhong, Phys. Rev. D, 95(3):034026 (2017)
    [80] S. Godfrey, K. Moats, Phys. Rev. D, 92(5):054034 (2015)
    [81] Y. Koma, M. Koma, H. Wittig, Phys. Rev. Lett, 97:122003 (2006)
    [82] N. Devlani, V. Kher, and A. K. Rai, Eur. Phys. J. A, 50(10):154 (2014)
    [83] V. Kher, N. Devlani, and A. K. Rai, Chinese Physics C, 41(7):073101 (2017), 1704.00439
    [84] V. Kher, N. Devlani, A.K. Rai, Chinese Physics C, Vol. 41,(No. 9), 093101 (2017)
    [85] N. Brambilla, A. Pineda, J. Soto, and A. Vairo, Rev. Mod. Phys., 77:1423 (2005)
    [86] N. Brambilla et al, Eur. Phys. J. C, 74(10):2981 (2014)
    [87] S. N. Gupta, J. M. Johnson, Phys. Rev. D, 51(1):168 (1995)
    [88] D. S. Hwang, C. Kim, W. Namgung, Phys. Lett. B, 406:117 (1997), hep-ph/9608392
    [89] A. K. Rai, B. Patel, and P. C. Vinodkumar, Phys. Rev. C, 78(5):055202 (2008)
    [90] A. K. Rai, R. H. Parmar, and P. C. Vinodkumar, J. Phys. G:Nucl. Part. Phys., 28(8):2275 (2002)
    [91] E. Eichten, S. Godfrey, H. Mahlke, and J. L. Rosner, Rev. Mod. Phys., 80:1161 (2008)
    [92] M. B. Voloshin, Prog. Part. Nucl. Phys., 61:455 (2008)
    [93] O. Lakhina, E. S. Swanson, Phys. Rev. D, 74:014012 (2006)
    [94] R. Van Royen, V. Weisskopf, Nuovo Cim. A, 50:617 (1967)
    [95] E. Braaten, S. Fleming, Phys. Rev. D, 52(1):181 (1995)
    [96] D. S. Hwang, G. H. Kim, Phys. Rev. D, 55(11):6944 (1997)
    [97] G. J. Ding, J. J. Zhu, and M. L. Yan, Phys. Rev. D, 77:014033 (2008)
    [98] Q. F. Lu, T. T. Pan, Y. Y. Wang, E. Wang, and D. M. Li, Phys. Rev. D, 94(7):074012 (2016)
    [99] F. K. Guo, C. Hanhart, G. Li, U. G. Meissner, and Q. Zhao, Phys. Rev. D, 82:034025 (2010)
    [100] S. F. Radford, W. W. Repko, M. J. Saelim, Phys. Rev. D, 80(3):034012 (2009)
    [101] J. Segovia, P. G. Ortega, D. R. Entem, and F. Fernndez, Phys. Rev. D, 93(7):074027 (2016)
    [102] W. Kwong, P. B. Mackenzie, R. Rosenfeld, and J. L. Rosner, Phys. Rev. D, 37:3210 (1988)
    [103] W. Kwong, J. L. Rosner, Phys. Rev. D, 38:279 (1988)
    [104] A. Bradley, A. Khare, Z. Phys. C, 8:131 (1981)
    [105] G. Belanger, P. Moxhay, Phys. Lett. B, 199:575 (1987)
    [106] Bhaghyesh, K.B. Vijaya Kumar, and A. P. Monteiro, J. Phys. G, 38:085001 (2011)
    [107] H. Negash, S. Bhatnagar, Int. J. Mod. Phys. E, 25(08):1650059 (2016)
    [108] J. H. Yang, S. K. Lee, E. J. Kim, and J. B. Choi (2015), 1506.04481
    [109] D. Ebert, R. Faustov, V. Galkin, Eur. Phys. J. C, 71:1825 (2011)
    [110] S. F. Radford, W. W. Repko, Phys. Rev. D, 75:074031 (2007)
    [111] D. Ebert, R. N. Faustov, and V. O. Galkin, Phys. Rev. D, 67:014027 (2003)
    [112] M. A. Sultan, N. Akbar, B. Masud, F. Akram, Phys. Rev. D, 90(5):054001 (2014)
    [113] S. Godfrey, N. Isgur, Phys. Rev. D, 32:189 (1985)
    [114] D. Ebert, R. Faustov, and V. Galkin, Eur. Phys. J. C, 66:197 (2010)
    [115] A. Parmar, B. Patel, and P. Vinodkumar, Nucl. Phys. A, 848:299 (2010)
    [116] N. Brambilla et al (Quarkonium Working Group) (2004), hepph/0412158
    [117] E. J. Eichten, K. Lane, and C. Quigg, Phys. Rev. Lett., 89:162002 (2002), hep-ph/0206018
    [118] P. P. D'Souza, M. Bhat, A. P. Monteiro, and K. B. Vijaya Kumar (2017)
    [119] Bhaghyesh, K. B. Vijaya Kumar, and Y. L. Ma, Int. J. Mod. Phys. A, 27:1250011 (2012)
    [120] F. Giannuzzi, Phys. Rev. D, 78:117501 (2008)
    [121] J. T. Laverty, S. F. Radford, and W. W. Repko (2009), 0901.3917
    [122] C. R. Munz, Nucl. Phys. A, 609:364 (1996)
    [123] C. S. Kim, T. Lee, and G. L. Wang, Phys. Lett. B, 606:323 (2005)
    [124] D. Ebert, R. N. Faustov, V. O. Galkin, Mod. Phys. Lett. A, 18:601 (2003)
    [125] N. A. Tornqvist, Phys. Lett. B, 590:209 (2004)
    [126] E. Braaten, M. Lu, Phys. Rev. D, 76:094028 (2007)
    [127] M. Albaladejo, F. K. Guo, C. Hanhart, U. G. Meiner, J. Nieves, A. Nogga, and Z. Yang, Chin. Phys. C, 41(12):121001 (2017)
    [128] C. Hanhart, Yu. S. Kalashnikova, A. E. Kudryavtsev, and A. V. Nefediev, Phys. Rev. D, 76:034007 (2007)
    [129] L. Maiani, F. Piccinini, A. D. Polosa, and V. Riquer, Phys. Rev. D, 71:014028 (2005), hep-ph/0412098
    [130] M. Nielsen, S. J. Brodsky (2018), 1802.09652
    [131] C. W. Zhao, G. Li, X. H. Liu, and F. L. Shao, Eur. Phys. J. C, 73:2482 (2013)
    [132] X. Liu, Z. G. Luo, and Z. F. Sun, Phys. Rev. Lett., 104:122001 (2010)
    [133] F. K. Guo, C. Hanhart, G. Li, U. G. Meissner, and Q. Zhao, Phys. Rev. D, 83:034013 (2011)
    [134] G. Li, Q. Zhao, Phys. Lett. B, 670:55 (2008)
    [135] G. Li, Q. Zhao, Phys. Rev. D, 84:074005 (2011)
    [136] S. S. Afonin, I. V. Pusenkov, EPJ Web Conf., 125:04006 (2016)
  • 加载中

Get Citation
Virendrasinh Kher and Ajay Kumar Rai. Spectroscopy and decay properties of charmonium[J]. Chinese Physics C, 2018, 42(8): 083101. doi: 10.1088/1674-1137/42/8/083101
Virendrasinh Kher and Ajay Kumar Rai. Spectroscopy and decay properties of charmonium[J]. Chinese Physics C, 2018, 42(8): 083101.  doi: 10.1088/1674-1137/42/8/083101 shu
Milestone
Received: 2018-03-29
Article Metric

Article Views(1783)
PDF Downloads(73)
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:

Spectroscopy and decay properties of charmonium

  • 1. Applied Physics Department, Polytechnic, The M. S. University of Baroda, Vadodara 390002, Gujarat, India
  • 2. Department of Applied Physics, Sardar Vallabhbhai National Institute of Technology, Surat 395007, Gujarat, India
  • 3.  Department of Applied Physics, Sardar Vallabhbhai National Institute of Technology, Surat 395007, Gujarat, India

Abstract: The mass spectra of charmonium are investigated using a Coulomb plus linear (Cornell) potential. Gaussian wave functions in position space as well as in momentum space are employed to calculate the expectation values of potential and kinetic energy respectively. Various experimental states (X(4660)(53S1), X(3872)(23P1), X(3900)(21P1), X(3915)(23P0) and X(4274)(33P1) etc.) are assigned as charmonium states. We also study the Regge trajectories, pseudoscalar and vector decay constants, electric and magnetic dipole transition rates, and annihilation decay widths for charmonium states.

    HTML

Reference (136)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return