×
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

Testing B-violating signatures from exotic instantons in future colliders

  • We discuss possible implications of exotic stringy instantons for baryon-violating signatures in future colliders. In particular, we discuss high-energy quark collisions and Λ-Λ transitions. In principle, the Λ-Λ process can be probed by high-luminosity electron-positron colliders. However, we find that an extremely high luminosity is needed in order to provide a (somewhat) stringent bound compared to the current data on m NN→ππ,KK. On the other hand, (exotic) instanton-induced six-quark interactions can be tested in near future high-energy colliders beyond LHC, at energies around 20-100 m TeV. The Super proton-proton Collider (SppC) would be capable of such measurement given the proposed energy level of 50-90 TeV. Comparison with other channels is made. In particular, we show the compatibility of our model with neutron-antineutron and m NN→ππ,KK bounds.
      PCAS:
  • 加载中
  • [1] , e.g., CP violation in the quark sector and D0-D0 mixing
    [2] A. Addazi and M. Bianchi, JHEP, 1412:089(2014)
    [3] A. Addazi, JHEP, 1504:153(2015)
    [4] A. Addazi and M. Bianchi, JHEP, 1507:144(2015)
    [5] A. Addazi and M. Bianchi, JHEP, 1506:012(2015)
    [6] A. Addazi, Mod. Phys. Lett. A, 31(17):1650109(2016)
    [7] A. Addazi, Electron. J. Theor. Phys., 13(35):39(2016)
    [8] A. Addazi, Int. J. Mod. Phys. A, 31(16):1650084(2016)
    [9] A. Addazi, Phys. Lett. B, 757:462(2016)
    [10] A. Addazi, arXiv:1510.02911[hep-ph], MGM14(C15-07-12)
    [11] A. Addazi, M. Bianchi, and G. Ricciardi, JHEP, 1602:035(2016)
    [12] A. Addazi, J. W. F. Valle, and C. A. Vaquera-Araujo, Phys. Lett. B, 759:471(2016)
    [13] A. Addazi and M. Khlopov, Mod. Phys. Lett. A, 31(19):1650111(2016)
    [14] M. Bianchi and M. Samsonyan, Int. J. Mod. Phys. A, 24:5737(2009)
    [15] V. A. Kuzmin, V. A. Rubakov, and M. E. Shaposhnikov, Phys. Lett. B, 155:36(1985)
    [16] V. A. Kuzmin, V. A. Rubakov, and M. E. Shaposhnikov, Phys. Lett. B, 191:171(1987)
    [17] L. E. Ibanez and A. M. Uranga, JHEP, 0703:052(2007)
    [18] R. Blumenhagen, M. Cvetic, D. Lust, R. Richter, and T. Weigand, Phys. Rev. Lett., 100:061602(2008)
    [19] M. Cvetic, J. Halverson, P. Langacker and R. Richter, JHEP, 1010:094(2010)
    [20] A. Sagnotti, Open Strings and their Symmetry Groups, IN Cargese 1987, Proceedings, Nonperturbative Quantum Field Theory, 521-528 AND ROME Ⅱ UNIV.-ROM2F-87-025(87,REC.MAR.88) 12p[hep-th/0208020]
    [21] G. Pradisi and A. Sagnotti, Phys. Lett. B, 216:59(1989)
    [22] A. Sagnotti, Phys. Lett. B, 294:196(1992)
    [23] M. Bianchi and A. Sagnotti, Phys. Lett. B, 247:517(1990)
    [24] M. Bianchi, G. Pradisi, and A. Sagnotti, Nucl. Phys. B, 376:365(1992)
    [25] M. Bianchi, G. Inverso, J. F. Morales, and D. R. Pacifici, JHEP, 1401:128(2014)
    [26] L. A. Anchordoqui, I. Antoniadis, D. C. Dai, W. Z. Feng, H. Goldberg, X. Huang, D. Lust, and D. Stojkovic et al, Phys. Rev. D, 90(6):066013(2014)
    [27] L. A. Anchordoqui, H. Goldberg, D. Lust, S. Stieberger, and T. R. Taylor, Mod. Phys. Lett. A, 24:2481(2009)
    [28] C. Kokorelis, hep-th/0309070
    [29] M. Cvetic, J. Halverson, and R. Richter, JHEP, 0912:063(2009)
    [30] P. Anastasopoulos, M. Bianchi, E. Dudas, and E. Kiritsis, JHEP, 0611:057(2006)
    [31] P. Anastasopoulos, F. Fucito, A. Lionetto, G. Pradisi, A. Racioppi, and Y.S. Stanev, Phys. Rev. D, 78:085014(2008)
    [32] M. Bianchi and E. Kiritsis, Nucl. Phys. B, 782:26(2007)
    [33] R. Blumenhagen, J. P. Conlon, S. Krippendorf, S. Moster, and F. Quevedo, JHEP, 0909:007(2009)
    [34] L. Aparicio, M. Cicoli, S. Krippendorf, A. Maharana, F. Muia, and F. Quevedo, JHEP, 1411:071(2014)
    [35] D. J. Gross and P. F. Mende, Nucl. Phys. B, 303:407(1988)
    [36] X. W. Kang, H. B. Li, G. R. Lu, and A. Datta, Int. J. Mod. Phys. A, 26:2523(2011)
    [37] X. W. Kang, J. Haidenbauer, and U.-G. Mei ner, JHEP, 1402:113(2014)
    [38] J. Haidenbauer, X.-W. Kang, and U.-G. Mei ner, Nucl. Phys. A, 929:102(2014)
    [39] X. W. Kang, J. Haidenbauer, and U. G. Mei ner, Phys. Rev. D, 91(7):074003(2015)
    [40] J. Haidenbauer, C. Hanhart, X. W. Kang, and U. G. Mei脽ner, Phys. Rev. D, 92(5):054032(2015)
    [41] X. W. Kang, H. B. Li, and G. R. Lu, Phys. Rev. D, 81:051901(2010) X. W. Kang, H. B. Li, and G. R. Lu, arXiv:1008.2845[hep-ph]
    [42] see the corresponding review section in
    [43] X. W. Kang, B. Kubis, C. Hanhart, and U. G. Mei ner, Phys. Rev. D, 89:053015(2014)
    [44] K. A. Olive et al (Particle Data Group Collaboration), Chin. Phys. C, 38:090001(2014)
    [45] M. Ablikim et al (BESⅢ Collaboration), Nucl. Instrum. Meth. A, 614:345(2010); D. M. Asner et al, Int. J. Mod. Phys. A, 24:S1(2009); H. B. Li, Front. Phys., 12:121301(2017)
    [46] See e.g., M. Ablikim et al (BESⅢ Collaboration), Phys. Rev. Lett., 115(9):091803(2015)
    [47] U. Tamponi et al (Belle Collaboration), Phys. Rev. Lett., 115(14):142001(2015)
    [48] A. Abdesselam et al (BaBar and Belle Collaborations), Phys. Rev. Lett., 115(12):121604(2015)
    [49] M. Baldo-Ceolin et al, Z. Phys. C, 63:409(1994)
    [50] K. Abe et al (Super-Kamiokande Collaboration), Phys. Rev. D, 91:072006(2015)
    [51] A. S. Kronfeld, R. S. Tschirhat, U. Al. Binni, W. Altmannshofer, C. Ankenbrandt, K. Babu, S. Banerjee, and M. Bass et al, Project X:Physics Opportunities, arXiv:1306.5009[hep-ex] 12 Jul 2013
    [52] M. I. Buchoff and M. Wagman, Phys. Rev. D, 93(1):016005(2016)
    [53] G. Dvali, D. Pirtskhalava, Phys. Lett. B, 699:78-86(2011) arXiv:1011.0114[hep-ph]
    [54] G. Dvali, arXiv:1101.2661[hep-th]
    [55] G. Dvali, A. Franca, and C. Gomez, arXiv:1204.6388[hep-th]
    [56] G. Dvali and C. Gomez, JCAP, 1207:015(2012)
    [57] A. Addazi, Int. J. Mod. Phys. A, 31(04n05):1650009(2016)
    [58] A. Addazi and G. Esposito, Int. J. Mod. Phys. A, 30(15):1550103(2015)
    [59] G. Dvali and C. Gomez, arXiv:1005.3497[hep-th]
    [60] G. Dvali and C. Gomez, Eur. Phys. J. C, 74:2752(2014)
    [61] G. Dvali and C. Gomez, Black Hole Macro-Quantumness, arXiv:1212.0765[hep-th]
    [62] G. Dvali, C. Gomez, R. S. Isermann, D. Lst, and S. Stieberger, Nucl. Phys. B, 893:187(2015)
    [63] M. Cvetic, R. Richter, and T. Weigand, Phys. Rev. D, 76:086002(2007)
    [64] R. Blumenhagen, M. Cvetic, S. Kachru, and T. Weigand, Ann. Rev. Nucl. Part. Sci., 59:269(2009)
  • 加载中

Get Citation
Andrea Addazi, Xian-Wei Kang and Maxim Yu. Khlopov. Testing B-violating signatures from exotic instantons in future colliders[J]. Chinese Physics C, 2017, 41(9): 093102. doi: 10.1088/1674-1137/41/9/093102
Andrea Addazi, Xian-Wei Kang and Maxim Yu. Khlopov. Testing B-violating signatures from exotic instantons in future colliders[J]. Chinese Physics C, 2017, 41(9): 093102.  doi: 10.1088/1674-1137/41/9/093102 shu
Milestone
Received: 2017-03-14
Revised: 2017-05-10
Fund

    A. A.'s work was supported in part by the MIUR research grant Theoretical Astroparticle Physics PRIN 2012CPPYP7. XWK's work is partly supported by the DFG and the NSFC through funds provided to the Sino-German CRC 110 Symmetries and the Emergence of Structure in QCD when he was in Jlich, and by MOST, Taiwan, (104-2112-M-001-022) from April 2017. The work by MK was performed within the framework of the Center FRPP Supported by MEPhI Academic Excellence Project (contract 02.03.21.0005, 27.08.2013), supported by the Ministry of Education and Science of Russian Federation, project 3.472.2014/K and grant RFBR 14-22-03048

Article Metric

Article Views(1600)
PDF Downloads(28)
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:

Testing B-violating signatures from exotic instantons in future colliders

    Corresponding author: Xian-Wei Kang, andrea.addazi@infn.lngs.it
  • 1.  Dipartimento di Fisica, Università
  • 2. Institute of Physics, Academia Sinica, Taipei 115
  • 3. Institute for Advanced Simulation, Jü
  • 4. Centre for Cosmoparticle Physics Cosmion
  • 5. APC laboratory 10, rue Alice Domon et Lé
Fund Project:  A. A.'s work was supported in part by the MIUR research grant Theoretical Astroparticle Physics PRIN 2012CPPYP7. XWK's work is partly supported by the DFG and the NSFC through funds provided to the Sino-German CRC 110 Symmetries and the Emergence of Structure in QCD when he was in Jlich, and by MOST, Taiwan, (104-2112-M-001-022) from April 2017. The work by MK was performed within the framework of the Center FRPP Supported by MEPhI Academic Excellence Project (contract 02.03.21.0005, 27.08.2013), supported by the Ministry of Education and Science of Russian Federation, project 3.472.2014/K and grant RFBR 14-22-03048

Abstract: We discuss possible implications of exotic stringy instantons for baryon-violating signatures in future colliders. In particular, we discuss high-energy quark collisions and Λ-Λ transitions. In principle, the Λ-Λ process can be probed by high-luminosity electron-positron colliders. However, we find that an extremely high luminosity is needed in order to provide a (somewhat) stringent bound compared to the current data on m NN→ππ,KK. On the other hand, (exotic) instanton-induced six-quark interactions can be tested in near future high-energy colliders beyond LHC, at energies around 20-100 m TeV. The Super proton-proton Collider (SppC) would be capable of such measurement given the proposed energy level of 50-90 TeV. Comparison with other channels is made. In particular, we show the compatibility of our model with neutron-antineutron and m NN→ππ,KK bounds.

    HTML

Reference (64)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return