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> 2018, Vol. 42> Issue(4) : 042002 DOI: 10.1088/1674-1137/42/4/042002

An overview of n and n' decays at BESⅢ

  • 1.

     Institute of High Energy Physics, Chinese Academy of Science, Beijing 100049, China

  • 2.

     University of Chinese Academy of Sciences, Beijing 100049, China

  • 3.

     Guangxi Normal University, Guilin 541004, China

  • 4.

      Uppsala University, Box 516, SE-75120 Uppsala, Sweden

  • 5.

      Guangxi Normal University, Guilin 541004, China

  • The world's largest sample of J/ψ events, 1.31 billion events accumulated at the BESⅢ detector, provides a unique opportunity to investigate n and n' physics via two-body J/ψ radiative or hadronic decays. For many n' decay channels the low background data samples are up to three orders of magnitude larger than collected in any previous experiment. Here we review the most significant results on n and n' obtained at BESⅢ so far. The analyses range from detailed studies of common decay dynamics, observations of new radiative and Dalitz decays, and searches for rare/forbidden decays with sensitivity up to B~10-5. Finally, prospects of forthcoming runs at the J/ψ peak for n and n' physics are discussed.
      PCAS:
  • 加载中

  • References

    [1] A. Pevsner et al, Phys. Rev. Lett., 7:421 (1961)
    [2] G. R. Kalbfleisch et al, Phys. Rev. Lett., 12:527 (1964)
    [3] M. Goldberg et al, Phys. Rev. Lett., 12:546 (1964)
    [4] J. Gasser and H. Leutwyler, Annals Phys., 158:142 (1984)
    [5] J. Wess and B. Zumino, Phys. Lett. B, 37:95 (1971)
    [6] E. Witten, Nucl. Phys. B, 223:422 (1983)
    [7] J. Bijnens, A. Bramon, and F. Cornet, Z. Phys. C, 46:599 (1990)
    [8] J. J. Sakurai, Annals Phys., 11:1 (1960)
    [9] L. G. Landsberg, Phys. Rept., 128:301 (1985)
    [10] R. Kaiser and H. Leutwyler, Eur. Phys. J. C, 17:623 (2000)
    [11] M. Ablikim et al (BESⅢ), Phys. Rev. Lett., 118:012001 (2017)
    [12] M. Ablikim et al (BESⅢ), Phys. Rev. D, 92:012001 (2015)
    [13] M. Ablikim et al (BESⅢ), Phys. Rev. D, 92:051101 (2015)
    [14] M. Ablikim et al (BESⅢ), Phys. Rev. D, 96:012005 (2017)
    [15] M. Ablikim et al (BESⅢ), Phys. Rev. Lett., 112:251801 (2014); Phys. Rev. Lett., 113:039903 (2014)
    [16] M. Ablikim et al (BESⅢ), Nucl. Instrum. Meth. A, 614:345 (2010)
    [17] C. Patrignani et al (Particle Data Group), Chin. Phys. C, 40:100001 (2016)
    [18] M. Ablikim et al (BESⅢ), Chin. Phys. C, 36:915 (2012)
    [19] M. Ablikim et al (BESⅢ), Chin. Phys. C, 41:013001 (2017)
    [20] M. Ablikim et al (BESⅢ), Phys. Rev. D, 92:012014 (2015)
    [21] D. G. Sutherland, Phys. Lett., 23:384 (1966)
    [22] J. S. Bell and D. G. Sutherland, Nucl. Phys., B4:315 (1968)
    [23] R. Baur, J. Kambor, and D. Wyler, Nucl. Phys. B, 460:127 (1996)
    [24] C. Ditsche, B. Kubis, and U.-G. Meissner, Eur. Phys. J. C, 60:83 (2009)
    [25] H. Leutwyler, Phys. Lett. B, 378:313 (1996)
    [26] H. Osborn and D. J. Wallace, Nucl. Phys. B, 20:23 (1970)
    [27] J. Gasser and H. Leutwyler, Nucl. Phys. B, 250:539 (1985)
    [28] J. Kambor, C. Wiesendanger, and D. Wyler, Nucl. Phys. B, 465:215 (1996)
    [29] A. V. Anisovich and H. Leutwyler, Phys. Lett. B, 375:335 (1996)
    [30] J. Bijnens and K. Ghorbani, JHEP, 11:030 (2007)
    [31] S. P. Schneider, B. Kubis, and C. Ditsche, JHEP, 02:028 (2011)
    [32] K. Kampf, M. Knecht, J. Novotny, and M. Zdrahal, Phys. Rev. D, 84:114015 (2011)
    [33] G. Colangelo, S. Lanz, H. Leutwyler, and E. Passemar, PoS, EPS-HEP2011:304 (2011)
    [34] G. Colangelo, S. Lanz, H. Leutwyler, and E. Passemar, Phys. Rev. Lett., 118:022001 (2017)
    [35] P. Guo et al, Phys. Rev. D, 92:054016 (2015)
    [36] F. Ambrosino et al (KLOE), JHEP, 05:006 (2008)
    [37] J. Bijnens and J. Gasser, Phys. Scripta, T99:34 (2002)
    [38] B. Borasoy and R. Nissler, Eur. Phys. J. A, 26:383 (2005)
    [39] J. G. Layter et al, Phys. Rev. D, 7:2565 (1973)
    [40] A. Abele et al (Crystal Barrel), Phys. Lett. B, 417:197 (1998)
    [41] P. Adlarson et al (WASA-at-COSY), Phys. Rev. C, 90:045207 (2014)
    [42] A. Anastasi et al (KLOE-2), JHEP, 05:019 (2016)
    [43] C. O. Gullstrom, A. Kupsc and A. Rusetsky, Phys. Rev. C, 79:028201 (2009)
    [44] F. Ambrosino et al (KLOE), Phys. Lett. B, 694:16 (2011)
    [45] C. Adolph et al (WASA-at-COSY), Phys. Lett. B, 677:24 (2009)
    [46] S. Prakhov et al (Crystal Ball at MAMI, A2), Phys. Rev. C, 79:035204 (2009)
    [47] M. N. Achasov et al, JETP Lett., 73:451 (2001); Pisma Zh. Eksp. Teor. Fiz., 73:511 (2001)
    [48] A. Abele et al (Crystal Barrel), Phys. Lett. B, 417:193 (1998)
    [49] D. Alde et al (Serpukhov-Brussels-Annecy (LAPP), SovietCERN), Z. Phys. C, 25:225 (1984),[Yad. Fiz., 40:1447 (1984)]
    [50] M. Ablikim et al (BESⅢ), Phys. Rev. D, 83:012003 (2011)
    [51] M. Ablikim et al (BESⅢ), arXiv:1709.04627[hep-ex]
    [52] R. Escribano, P. Masjuan and J. J. Sanz-Cillero, JHEP, 05:094 (2011)
    [53] V. Dorofeev et al, Phys. Lett. B, 651:22 (2007)
    [54] A. M. Blik et al, Phys. Atom. Nucl., 71:2124 (2008),[Yad. Fiz.71,2161 (2008)]
    [55] P. Adlarson et al, arXiv:1709.04230
    [56] B. Kubis and S. P. Schneider, Eur. Phys. J. C, 62:511 (2009)
    [57] T. Isken, B. Kubis, S. P. Schneider, and P. Stofier, Eur. Phys. J. C, 77:489 (2017)
    [58] F. G. Binon et al (Serpukhov-Brussels-Annecy (LAPP)), Phys. Lett., 140B:264 (1984)
    [59] D. Alde et al (Serpukhov-Brussels-Los AlamosAnnecy (LAPP)), Z. Phys. C, 36:603 (1987)
    [60] M. Ablikim et al (BESⅢ), Phys. Rev. Lett., 108:182001 (2012)
    [61] D. J. Gross, S. B. Treiman, and F. Wilczek, Phys. Rev. D, 19:2188 (1979)
    [62] B. Borasoy, U.-G. Meissner, and R. Nissler, Phys. Lett. B, 643:41 (2006)
    [63] P. Naik et al (CLEO), Phys. Rev. Lett., 102:061801 (2009)
    [64] F.-K. Guo, B. Kubis, and A. Wirzba, Phys. Rev. D, 85:014014 (2012)
    [65] D. Parashar, Phys. Rev. D, 19:268 (1979)
    [66] M. Ablikim et al (BESⅢ), arXiv:1712.01525[hep-ex]
    [67] M. Gell-Mann, D. Sharp, and W. G. Wagner, Phys. Rev. Lett., 8:261 (1962)
    [68] W. Bartel et al (JADE), Phys. Lett. B, 113:190 (1982)
    [69] H. J. Behrend et al (CELLO), Phys. Lett. B, 114:378 (1982),[Erratum:Phys. Lett.125B,518 (1983)]
    [70] C. Berger et al (PLUTO), Phys. Lett. B, 142:125 (1984)
    [71] M. Althofi et al (TASSO), Phys. Lett. B, 147:487 (1984)
    [72] H. Aihara et al (TPC/Two Gamma), Phys. Rev. D, 35:2650 (1987)
    [73] H. Albrecht et al (ARGUS), Phys. Lett. B, 199:457 (1987)
    [74] S. I. Bityukov et al, Z. Phys. C, 50:451 (1991)
    [75] M. Benayoun et al, Z. Phys. C, 58:31 (1993)
    [76] A. Abele et al (Crystal Barrel), Phys. Lett. B, 402:195 (1997)
    [77] M. Acciarri et al (L3), Phys. Lett. B, 418:399 (1998)
    [78] F. Stollenwerk, C. Hanhart, A. Kupsc, U. G. Meissner, and A. Wirzba, Phys. Lett. B, 707:184 (2012)
    [79] P. Adlarson et al (WASA-at-COSY), Phys. Lett. B, 707:243 (2012)
    [80] D. Babusci et al (KLOE), Phys. Lett. B, 718:910 (2013)
    [81] C. Hanhart, A. Kupsc, U. G. Meiner, F. Stollenwerk, and A. Wirzba, Eur. Phys. J. C, 73:2668 (2013); Eur. Phys. J. C, 75:242 (2015)
    [82] G. J. Gounaris and J. J. Sakurai, Phys. Rev. Lett., 21:244 (1968)
    [83] R. Garcia-Martin, R. Kaminski, J. R. Pelaez, J. Ruiz de Elvira, and F. J. Yndurain, Phys. Rev. D, 83:074004 (2011)
    [84] B. Kubis and J. Plenter, Eur. Phys. J. C, 75:283 (2015)
    [85] M. Ablikim et al (BESⅢ), Phys. Rev. D, 87:092011 (2013)
    [86] A. Faessler, C. Fuchs, and M. I. Krivoruchenko, Phys. Rev. C, 61:035206 (2000)
    [87] B. Borasoy and R. Nissler, Eur. Phys. J. A, 33:95 (2007)
    [88] T. Petri, arXiv:1010.2378[nucl-th]
    [89] E. Czerwinski et al, arXiv:1010.2378[nucl-th]
    [90] T. Blum et al, arXiv:1311.2198[hep-ph]
    [91] V. M. Budnev and V. A. Karnakov, Pisma Zh. Eksp. Teor. Fiz., 29:439 (1979)
    [92] R. I. Dzhelyadin et al, Phys. Lett. B, 88:379 (1979); JETP Lett., 30:359 (1979)
    [93] A. Bramon and E. Masso, Phys. Lett. B, 104:311 (1981)
    [94] L. Ametller, L. Bergstrom, A. Bramon, and E. Masso, Nucl. Phys. B, 228:301 (1983)
    [95] L. Ametller, J. Bijnens, A. Bramon, and F. Cornet, Phys. Rev. D, 45:986 (1992)
    [96] H. J. Behrend et al (CELLO), Z. Phys. C, 49:401 (1991)
    [97] C. Terschlsen, S. Leupold, and M. F. M. Lutz, Eur. Phys. J. A, 48:190 (2012)
    [98] R. Jora, Nucl. Phys. Proc. Suppl., 207-208:224 (2010)
    [99] R. Escribano, PoS, QNP2012:079 (2012)
    [100] M. Ablikim et al (BESⅢ), Phys. Rev. D, 87:012009 (2013)
    [101] M. Ablikim et al (BES), Phys. Rev. Lett., 97:202002 (2006)
    [102] M. Ablikim et al (BESⅢ), Phys. Rev. D, 87:032006 (2013)
    [103] P. Fayet, Phys. Rev. D, 74:054034 (2006)
    [104] P. Fayet, Phys. Rev. D, 75:115017 (2007)
    [105] M. Ablikim et al (BESⅢ), Phys. Rev. D, 84:032006 (2011)
    [106] C. Jarlskog and E. Shabalin, Phys. Scripta, T99:23 (2002)
    [107] M. Ablikim et al (BESⅢ), Phys. Rev. D, 93:072008 (2016)
    [108] L. Bergstrom and H. R. Rubinstein, Phys. Lett. B, 203:183 (1988)
    [109] D. N. Gao, Phys. Rev. D, 96:093003 (2017)
    [110] C. Q. Geng, J. N. Ng, and T. H. Wu, Mod. Phys. Lett. A, 17:1489 (2002)
    [111] D. N. Gao, Mod. Phys. Lett. A, 17:1583 (2002)

  • Access

    加载中

Get Citation
Shuang-shi Fang, Andrzej Kupsc and Dai-hui Wei. An overview of n and n' decays at BESⅢ[J]. Chinese Physics C, 2018, 42(4): 042002. doi: 10.1088/1674-1137/42/4/042002
Shuang-shi Fang, Andrzej Kupsc and Dai-hui Wei. An overview of n and n' decays at BESⅢ[J]. Chinese Physics C, 2018, 42(4): 042002.  doi: 10.1088/1674-1137/42/4/042002 shu
Milestone
Received: 2017-12-15
Fund

    Supported by National Natural Science Foundation of China (NSFC) (11565006, 11675184, 11735014)

Article Metric

Article Views(1725)
PDF Downloads(36)
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:

An overview of n and n' decays at BESⅢ

    Corresponding author: Shuang-shi Fang,
    Corresponding author: Andrzej Kupsc,
    Corresponding author: Dai-hui Wei,
  • 1. Institute of High Energy Physics, Chinese Academy of Science, Beijing 100049, China
  • 2. University of Chinese Academy of Sciences, Beijing 100049, China
  • 3. Guangxi Normal University, Guilin 541004, China
  • 4.  Uppsala University, Box 516, SE-75120 Uppsala, Sweden
  • 5.  Guangxi Normal University, Guilin 541004, China
  • Received Date: 2017-12-15
  • Available Online: 2018-04-05
Fund Project:  Supported by National Natural Science Foundation of China (NSFC) (11565006, 11675184, 11735014)

Abstract: The world's largest sample of J/ψ events, 1.31 billion events accumulated at the BESⅢ detector, provides a unique opportunity to investigate n and n' physics via two-body J/ψ radiative or hadronic decays. For many n' decay channels the low background data samples are up to three orders of magnitude larger than collected in any previous experiment. Here we review the most significant results on n and n' obtained at BESⅢ so far. The analyses range from detailed studies of common decay dynamics, observations of new radiative and Dalitz decays, and searches for rare/forbidden decays with sensitivity up to B~10-5. Finally, prospects of forthcoming runs at the J/ψ peak for n and n' physics are discussed.

    HTML

Reference (111)

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