×
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

Super-light baryo-photons, weak gravity conjecture and exotic instantons in neutron-antineutron transitions

  • In companion papers A. Addazi, Nuovo Cim. C, 38(1):21 (2015), A. Addazi, Z. Berezhiani, and Y. Kamyshkov, arXiv:1607.00348, we have discussed current bounds on a new super-light baryo-photon, associated with a U(1)B-L gauge, from current neutron-antineutron data, which are competitive with Eötvös-type experiments. Here, we discuss the implications of possible baryo-photon detection in string theory and quantum gravity. The discovery of a very light gauge boson should imply violation of the weak gravity conjecture, carrying deep consequences for our understanding of holography, quantum gravity and black holes. We also show how the detection of a baryo-photon would exclude the generation of all B-L violating operators from exotic stringy instantons. We will argue against the common statement in the literature that neutron-antineutron data may indirectly test at least the 300-1000 TeV scale. Searches for baryo-photons can provide indirect information on the Planck (or string) scale (quantum black holes, holography and non-perturbative stringy effects). This strongly motivates new neutron-antineutron experiments with adjustable magnetic fields dedicated to the detection of super-light baryo-photons.
      PCAS:
  • 加载中
  • [1] Y. Chikashige, R. N. Mohapatra, and R. D. Peccei, Phys. Lett. B, 98:265(1981)
    [2] J. Schechter and J. W. F. Valle, Phys. Rev. D, 25:774(1982)
    [3] E. K. Akhmedov, Z. G. Berezhiani, R. N. Mohapatra, and G. Senjanovic, Phys. Lett. B, 299:90(1993) doi:10.1016/0370-2693(93)90887-N[hep-ph/9209285]
    [4] V. Berezinsky and J. W. F. Valle, Phys. Lett. B, 318:360(1993) doi:10.1016/0370-2693(93)90140-D[hep-ph/9309214].
    [5] Z. G. Berezhiani, A. Y. Smirnov and J. W. F. Valle, Phys. Lett. B, 291:99(1992) doi:10.1016/0370-2693(92)90126-O[hep-ph/9207209]
    [6] Z. G. Berezhiani and A. Rossi, Phys. Lett. B, 336:439(1994) doi:10.1016/0370-2693(94)90556-8[hep-ph/9407265]
    [7] M. Kachelriess, R. Tomas, and J. W. F. Valle, Phys. Rev. D, 62:023004(2000) doi:10.1103/PhysRevD.62.023004[hep-ph/0001039]
    [8] M. Lattanzi and J. W. F. Valle, Phys. Rev. Lett., 99:121301(2007) doi:10.1103/PhysRevLett.99.121301[arXiv:0705.2406[astro-ph]]
    [9] M. Lattanzi, S. Riemer-Srensen, M. Tortola, and J. W. F. Valle, Nucl. Instrum. Meth. A, 742:154(2014) doi:10.1016/j.nima.2013.09.009
    [10] S. M. Boucenna, S. Morisi, Q. Shafi, and J. W. F. Valle, Phys. Rev. D, 90(5):055023(2014) doi:10.1103/PhysRevD.90.055023[arXiv:1404.3198[hep-ph]]
    [11] N. Arkani-Hamed, L. Motl, A. Nicolis, and C. Vafa, JHEP, 0706:060(2007) doi:10.1088/1126-6708/2007/06/060[hep-th/0601001]
    [12] L. Susskind, hep-th/9501106
    [13] M. Baldo-Ceolin et al, Z. Phys. C, 63:409(1994)
    [14] D. G. Phillips, Ⅱ et al, Phys. Rept., 612:1(2016) doi:10.1016/j.physrep.2015.11.001[arXiv:1410.1100[hep-ex]]
    [15] Z. Berezhiani, Eur. Phys. J. C, 76(12):705(2016) doi:10.1140/epjc/s10052-016-4564-0[arXiv:1507.05478[hep-ph]]
    [16] D. A. Kirzhnitz, JETP Lett., 15:529(1972)
    [17] D. A. Kirzhnitz and A. D. Linde, Phys. Lett. B, 42:47(1972)
    [18] S. Weinberg, Phys. Rev. D, 9:3357(1974)
    [19] L. Dolan and R. Jackiw, Phys. Rev. D, 9:3320(1974)
    [20] R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett., 42:1651(1979); Phys. Rev. D, 20:3390(1979)
    [21] P. Langacker and S.-Y. Pi, Phys. Rev. Lett., 45:1(1980)
    [22] D. E. Morrissey and M. J. Ramsey-Musolf, New J. Phys., 14:125003(2012) doi:10.1088/1367-2630/14/12/125003[arXiv:1206.2942[hep-ph]]
    [23] A. Addazi and M. Bianchi, JHEP, 1412:089(2014) doi:10.1007/JHEP12(2014)089[arXiv:1407.2897[hep-ph]]
    [24] A. Addazi, JHEP, 1504:153(2015) doi:10.1007/JHEP04(2015)153[arXiv:1501.04660[hep-ph]]
    [25] A. Addazi and M. Bianchi, JHEP, 1507:144(2015) doi:10.1007/JHEP07(2015)144[arXiv:1502.01531[hep-ph]]
    [26] A. Addazi and M. Bianchi, JHEP, 1506:012(2015) doi:10.1007/JHEP06(2015)012[arXiv:1502.08041[hep-ph]]
    [27] A. Addazi, Mod. Phys. Lett. A, 31(17):1650109(2016) doi:10.1142/S0217732316501091[arXiv:1504.06799[hep-ph]]
    [28] A. Addazi, Electron. J. Theor. Phys., 13(35):39(2016)[arXiv:1505.00625[hep-ph]]
    [29] A. Addazi, Int. J. Mod. Phys. A, 31(16):1650084(2016) doi:10.1142/S0217751X16500846[arXiv:1505.02080[hep-ph]]
    [30] A. Addazi, Phys. Lett. B, 757:462(2016) doi:10.1016/j.physletb.2016.04.018[arXiv:1506.06351[hep-ph]]
    [31] A. Addazi, M. Bianchi, and G. Ricciardi, JHEP, 1602:035(2016) doi:10.1007/JHEP02(2016)035[arXiv:1510.00243[hep-ph]]
    [32] A. Addazi, J. W. F. Valle, and C. A. Vaquera-Araujo, Phys. Lett. B, 759:471(2016) doi:10.1016/j.physletb.2016.06.015[arXiv:1604.02117[hep-ph]]
    [33] A. Addazi and M. Khlopov, Mod. Phys. Lett. A, 31(19):1650111(2016) doi:10.1142/S021773231650111X[arXiv:1604.07622[hep-ph]]
    [34] A. Addazi, Mod. Phys. Lett. A, 32(02):1750014(2016) doi:10.1142/S0217732317500146[arXiv:1607.01203[hep-th]]
    [35] A. Addazi, X. W. Kang, and M. Y. Khlopov, arXiv:1705.03622[hep-ph], to appear in Chinese Phys. C
    [36] L. E. Ibanez and A. M. Uranga, JHEP, 0703:052(2007) doi:10.1088/1126-6708/2007/03/052[hep-th/0609213]
    [37] R. Blumenhagen, M. Cvetic, and T. Weigand, Nucl. Phys. B, 771:113(2007) doi:10.1016/j.nuclphysb.2007.02.016[hep-th/0609191]
    [38] L. E. Ibanez, A. N. Schellekens, and A. M. Uranga, JHEP, 0706:011(2007) doi:10.1088/1126-6708/2007/06/011[arXiv:0704.1079[hep-th]]
    [39] R. Blumenhagen, M. Cvetic, S. Kachru, and T. Weigand, Ann. Rev. Nucl. Part. Sci., 59:269(2009) doi:10.1146/annurev.nucl.010909.083113[arXiv:0902.3251[hep-th]]
    [40] R. Blumenhagen, M. Cvetic, R. Richter, and T. Weigand, JHEP, 0710:098(2007) doi:10.1088/1126-6708/2007/10/098[arXiv:0708.0403[hep-th]]
    [41] R. Blumenhagen, M. Cvetic, D. Lust, R. Richter, and T. Weigand, Phys. Rev. Lett., 100:061602(2008) doi:10.1103/PhysRevLett.100.061602[arXiv:0707.1871[hep-th]]
    [42] M. Cvetic, J. Halverson, P. Langacker, and R. Richter, JHEP, 1010:094(2010) doi:10.1007/JHEP10(2010)094[arXiv:1001.3148[hep-th]]
    [43] H. Abe, T. Kobayashi, Y. Tatsuta, and S. Uemura, Phys. Rev. D, 92(2):026001(2015) doi:10.1103/PhysRevD.92.026001[arXiv:1502.03582[hep-ph]]
    [44] M. Cvetic, J. Halverson, and R. Richter, JHEP, 0912:063(2009) doi:10.1088/1126-6708/2009/12/063[arXiv:0905.3379[hep-th]]
    [45] T. A. Wagner, S. Schlamminger, J. H. Gundlach, and E. G. Adelberger, Class. Quant. Grav., 29:184002(2012)[arXiv:1207.2442[gr-qc]]
    [46] M. I. Buchoff and M. Wagman, Phys. Rev. D, 93(1):016005(2016) doi:10.1103/PhysRevD.93.016005[arXiv:1506.00647[hep-ph]]
    [47] E. D. Davis and A. R. Young, Phys. Rev. D, 95(3):036004(2017) doi:10.1103/PhysRevD.95.036004[arXiv:1611.04205[nucl-ex]]
    [48] D. McKeen and A. E. Nelson, Phys. Rev. D, 94(7):076002(2016) doi:10.1103/PhysRevD.94.076002[arXiv:1512.05359[hep-ph]]
    [49] E. J. Copeland, M. Sami, and S. Tsujikawa, Int. J. Mod. Phys. D, 15:1753(2006) doi:10.1142/S021827180600942X[hep-th/0603057]
    [50] J. Frieman, M. Turner, and D. Huterer, Ann. Rev. Astron. Astrophys., 46:385(2008) doi:10.1146/annurev.astro.46.060407.145243[arXiv:0803.0982[astro-ph]]
    [51] Y. F. Cai, E. N. Saridakis, M. R. Setare, and J. Q. Xia, Phys. Rept., 493:1(2010) doi:10.1016/j.physrep.2010.04.001[arXiv:0909.2776[hep-th]]
  • 加载中

Get Citation
Andrea Addazi. Super-light baryo-photons, weak gravity conjecture and exotic instantons in neutron-antineutron transitions[J]. Chinese Physics C, 2018, 42(5): 053103. doi: 10.1088/1674-1137/42/5/053103
Andrea Addazi. Super-light baryo-photons, weak gravity conjecture and exotic instantons in neutron-antineutron transitions[J]. Chinese Physics C, 2018, 42(5): 053103.  doi: 10.1088/1674-1137/42/5/053103 shu
Milestone
Received: 2018-02-26
Article Metric

Article Views(1522)
PDF Downloads(16)
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:

Super-light baryo-photons, weak gravity conjecture and exotic instantons in neutron-antineutron transitions

    Corresponding author: Andrea Addazi,

Abstract: In companion papers A. Addazi, Nuovo Cim. C, 38(1):21 (2015), A. Addazi, Z. Berezhiani, and Y. Kamyshkov, arXiv:1607.00348, we have discussed current bounds on a new super-light baryo-photon, associated with a U(1)B-L gauge, from current neutron-antineutron data, which are competitive with Eötvös-type experiments. Here, we discuss the implications of possible baryo-photon detection in string theory and quantum gravity. The discovery of a very light gauge boson should imply violation of the weak gravity conjecture, carrying deep consequences for our understanding of holography, quantum gravity and black holes. We also show how the detection of a baryo-photon would exclude the generation of all B-L violating operators from exotic stringy instantons. We will argue against the common statement in the literature that neutron-antineutron data may indirectly test at least the 300-1000 TeV scale. Searches for baryo-photons can provide indirect information on the Planck (or string) scale (quantum black holes, holography and non-perturbative stringy effects). This strongly motivates new neutron-antineutron experiments with adjustable magnetic fields dedicated to the detection of super-light baryo-photons.

    HTML

Reference (51)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return