×
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 noncommutative spacetimes and violations of the Pauli Exclusion Principle through underground experiments

  • We propose to deploy limits that arise from different tests of the Pauli Exclusion Principle:i) to provide theories of quantum gravity with experimental guidance; ii) to distinguish, among the plethora of possible models, the ones that are already ruled out by current data; iii) to direct future attempts to be in accordance with experimental constraints. We first review experimental bounds on nuclear processes forbidden by the Pauli Exclusion Principle, which have been derived by several experimental collaborations making use of various detector materials. Distinct features of the experimental devices entail sensitivities on the constraints hitherto achieved that may differ from one another by several orders of magnitude. We show that with choices of these limits, well-known examples of flat noncommutative space-time instantiations of quantum gravity can be heavily constrained, and eventually ruled out. We devote particular attention to the analysis of the κ-Minkowski and θ-Minkowski noncommutative spacetimes. These are deeply connected to some scenarios in string theory, loop quantum gravity, and noncommutative geometry. We emphasize that the severe constraints on these quantum spacetimes, although they cannot rule out theories of top-down quantum gravity to which they are connected in various ways, provide a powerful limitation for those models. Focus on this will be necessary in the future.
      PCAS:
  • 加载中
  • [1] W. Pauli, Phys. Rev., 58:716 (1940) doi:10.1103/PhysRev.58.716
    [2] A. M. L. Messiah and O. W. Greenberg, Phys. Rev., 136:B248 (1964) doi:10.1103/PhysRev.136.B248
    [3] O. W. Greenberg and A. M. L. Messiah, Phys. Rev., 138:B1155 (1965) doi:10.1103/PhysRev.138.B1155
    [4] G. Gentile, NuovoCimento, 17:493 (1940)
    [5] H. S. Green, Phys. Rev., 90:270 (1953) doi:10.1103/PhysRev.90.270
    [6] A. Y. Ignatiev and V. A. Kuzmin, JETP Lett., 47:4 (1988)
    [7] V. N. Gavrin, A. Y. Ignatiev, and V. A. Kuzmin, Phys. Lett. B, 206:343 (1988) doi:10.1016/0370-2693(88)91518-3
    [8] O. W. Greenberg, Phys. Rev. Lett., 64:705 (1990)
    [9] R. N. Mohapatra, Phys. Lett. B, 242:407 (1990)
    [10] O. W. Greenberg, R. C. Hilborn, Fund.Phys., 29:397 (1999)
    [11] J. Collins, A. Perez, D. Sudarsky, L. Urrutia, and H. Vucetich, Phys. Rev. Lett., 93:191301 (2004) doi:10.1103/PhysRevLett.93.191301 gr-qc/0403053
    [12] R. Jackiw, Nucl. Phys. Proc. Suppl., 108:30 (2002)[hep-th/0110057]; Letter of Heisenberg to Peierls (1930), Wolfgang Pauli, Scientific Correspondence, Vol. Ⅱ, p.15, Ed. Karl von Meyenn, Springer-Verlag, 1985; Letter of Pauli to Oppenheimer (1946), Wolfgang Pauli, Scientific Correspondence, Vol. Ⅲ, p.380, Ed. Karl von Meyenn, Springer-Verlag, 1993
    [13] H. Snyder, Phys. Rev., 71:38 (1947)
    [14] C. N. Yang, Phys. Rev., 72:874 (1947)
    [15] A. Addazi and A. Marciano, arXiv:1707.05347[hep-th]
    [16] J. Frohlich and K. Gawedzki, In Vancouver 1993, Proceedings, Mathematical quantum theory, vol. 1 57-97, and Preprint-Gawedzki, K. (rec.Nov.93) 44 p[hep-th/9310187]
    [17] A.H. Chamseddine and J. Frhlich, Some Elements of Connes? Noncommutative Geometry and Space-time Geometry:in:Yang Festschrift:eds. C.S. Liu and S.-F. Yau (International Press, Boston, 1995) 10-34
    [18] J. Frohlich, O. Grandjean, and A. Recknagel, In Les Houches 1995, Quantum symmetries 221-385[hep-th/9706132]
    [19] A. Connes, M. R. Douglas, and A. S. Schwarz, JHEP, 9802:003 (1998) doi:10.1088/1126-6708/1998/02/003[hep-th/9711162]
    [20] N. Seiberg and E. Witten, JHEP, 9909:032 (1999) doi:10.1088/1126-6708/1999/09/032[hep-th/9908142]
    [21] G. Amelino-Camelia, L. Smolin, and A. Starodubtsev, Class. Quant. Grav., 21:3095 (2004) doi:10.1088/0264-9381/21/13/002[hep-th/0306134]
    [22] L. Freidel and E. R. Livine, Phys. Rev. Lett., 96:221301 (2006) doi:10.1103/PhysRevLett.96.221301[hep-th/0512113]
    [23] F. Cianfrani, J. Kowalski-Glikman, D. Pranzetti, and G. Rosati, Phys. Rev. D, 94(8):084044 (2016) doi:10.1103/PhysRevD.94.084044 arXiv:1606.03085[hep-th]
    [24] G. Amelino-Camelia, M. M. da Silva, M. Ronco, L. Cesarini, and O. M. Lecian, Phys. Rev. D, 95(2):024028 (2017) doi:10.1103/PhysRevD.95.024028 arXiv:1605.00497[gr-qc]
    [25] G. Amelino-Camelia, M. M. da Silva, M. Ronco, L. Cesarini, and O. M. Lecian, Phys. Rev. D, 95:024028 (2017) arXiv:1605.00497
    [26] S. Brahma, M. Ronco, G. Amelino-Camelia and A. Marciano, Phys. Rev. D, 95(4):044005 (2017) arXiv:1610.07865
    [27] S. Brahma, A. Marciano, and M. Ronco, arXiv:1707.05341[hep-th]
    [28] S. Alexander, A. Marciano, and L. Modesto, Phys. Rev. D, 85:124030 (2012) arXiv:1202.1824[hep-th]
    [29] M. Arzano and A. Marciano, Phys. Rev. D, 76:125005 (2007) arXiv:0707.1329
    [30] G. Amelino-Camelia, G. Gubitosi, A. Marciano, P. Martinetti, and F. Mercati, Phys. Lett. B, 671:298 (2009) arXiv:0707.1863
    [31] G. Amelino-Camelia, A. Marciano and D. Pranzetti, Int. J. Mod. Phys. A, 24:5445 (2009) arXiv:0709.2063
    [32] G. Amelino-Camelia, F. Briscese, G. Gubitosi, A. Marciano, P. Martinetti, and F. Mercati, Phys. Rev. D, 78:025005 (2008) arXiv:0709.4600
    [33] G. Amelino-Camelia, G. Gubitosi, A. Marciano, P. Martinetti, F. Mercati, D. Pranzetti, and R. A. Tacchi, Prog. Theor. Phys. Suppl., 171:65 (2007) arXiv:0710.1219
    [34] A. Marciano, Arabian J. Sci. Eng., 33:365 (2008)
    [35] A. Marciano, A brief overview of quantum field theory with deformed symmetries and their relation with quantum gravity, arXiv:1003.0395
    [36] A. Agostini, G. Amelino-Camelia, M. Arzano, A. Marciano, and R. A. Tacchi, Mod. Phys. Lett. A, 22:1779 (2007) arXiv:hep-th/0607221
    [37] M. Arzano and A. Marciano, Phys. Rev. D, 75:081701 (2007) arXiv:hep-th/0701268
    [38] G. Amelino-Camelia, M. Arzano and A. Marciano, Frascati Phys. Ser., 43:155 (2007)
    [39] A. Marciano, G. Amelino-Camelia, N. R. Bruno, G. Gubitosi, G. Mandanici, and A. Melchiorri, JCAP, 1006:030 (2010) arXiv:1004.1110
    [40] G. Amelino-Camelia, A. Marciano, M. Matassa and G. Rosati, Testing quantum-spacetime relativity with gamma-ray telescopes arXiv:1006.0007
    [41] G. Amelino-Camelia, A. Marciano, M. Matassa, and G. Rosati, Phys. Rev. D, 86:124035 (2012) arXiv:1206.5315
    [42] L. Alvarez-Gaume and M. A. Vazquez-Mozo, Nucl. Phys. B, 668:293 (2003) doi:10.1016/S0550-3213(03)00582-0[hep-th/0305093]
    [43] S. Majid, Foundations of quantum group theory, (CUP 1995, Cambridge)
    [44] R. Oeckl, Nucl. Phys. B, 581:559 (2000) doi:10.1016/S0550-3213(00)00281-9[hep-th/0003018]
    [45] M. Chaichian, P. P. Kulish, K. Nishijima, and A. Tureanu, Phys. Lett. B, 604:98 (2004) doi:10.1016/j.physletb.2004. 10.045[hep-th/0408069]
    [46] P. Aschieri, C. Blohmann, M. Dimitrijevic, F. Meyer, P. Schupp, and J. Wess, Class. Quant. Grav., 22:3511 (2005) doi:10.1088/0264-9381/22/17/011[hep-th/0504183]
    [47] A. P. Balachandran, T. R. Govindarajan, C. Molina, and P. Teotonio-Sobrinho, JHEP, 0410:072 (2004) doi:10.1088/1126-6708/2004/10/072[hep-th/0406125]
    [48] M. Arzano and J. Kowalski-Glikman, Phys. Lett. B, 760:69 (2016) doi:10.1016/j.physletb.2016.06.048 arXiv:1605.01181[hep-th]
    [49] A. P. Balachandran, G. Mangano, A. Pinzul, and S. Vaidya, Int. J. Mod. Phys. A, 21:3111 (2006) doi:10.1142/S0217751X06031764[hep-th/0508002]
    [50] M. Chaichian, A. D. Dolgov, V. A. Novikov, and A. Tureanu, Phys. Lett. B, 699:177 (2011) doi:10.1016/j.physletb.2011.03.026 arXiv:1103.0168[hep-th]
    [51] M. Chaichian, K. Nishijima, and A. Tureanu, Phys. Lett. B, 568:146 (2003) doi:10.1016/j.physletb.2003.06.009[hep-th/0209008]
    [52] A. Pichler et al, J. Phys. Conf. Ser., 718(5):052030 (2016) doi:10.1088/1742-6596/718/5/052030 arXiv:1602.00898[physics.ins-det]
    [53] H. Ejiri et al, Nucl. Phys. B (Proc. Suppl.), 28A:219 (1992)
    [54] R. Bernabei et al, Eur. Phys. J. C, 62:327 (2009) doi:10.1140/epjc/s10052-009-1068-1
    [55] N. Abgrall et al, Eur. Phys. J. C, 76(11):619 (2016) doi:10.1140/epjc/s10052-016-4467-0 arXiv:1610.06141[nucl-ex]
    [56] G. Bellini et al (Borexino Collaboration), Phys. Rev. C, 81:034317 (2010)
    [57] Y. Suzuki et al (Kamiokande Collaboration), Phys. Lett. B, 311:357 (1993) doi:10.1016/0370-2693(93)90582-3
    [58] R. Bernabei et al, Phys. Lett. B, 460:236 (1999)
    [59] V. Gayral, J. M. Gracia-Bondia, B. Iochum, T. Schucker, and J. C. Varilly, Commun. Math. Phys., 246:569 (2004) doi:10.1007/s00220-004-1057-z[hep-th/0307241]
    [60] B. Iochum, T. Masson, T. Schucker, and A. Sitarz, Rept. Math. Phys., 68:37 (2011) doi:10.1016/S0034-4877(11)60026-8 arXiv:1004.4190[hep-th]
    [61] M. Matassa, J. Geom. Phys., 76:136 (2014) doi:10.1016/j.geomphys.2013.10.023 arXiv:1212.3462[math-ph]
    [62] M. Arzano, Phys. Rev. D, 77:025013 (2008) doi:10.1103/PhysRevD.77.025013 arXiv:0710.1083[hep-th]
    [63] M. Arzano, A. Hamma, and S. Severini, Mod. Phys. Lett. A, 25:437 (2010) doi:10.1142/S0217732310032603 arXiv:0806.2145[hep-th]
    [64] L. Freidel, J. Kowalski-Glikman, and S. Nowak, Int. J. Mod. Phys. A, 23:2687 (2008) doi:10.1142/S0217751X08040421 arXiv:0706.3658[hep-th]
    [65] M. Daszkiewicz, J. Lukierski, and M. Woronowicz, Phys. Rev. D, 77:105007 (2008) doi:10.1103/PhysRevD.77.105007 arXiv:0708.1561[hep-th]
    [66] N. Arkani-Hamed, S. Dimopoulos, and G. R. Dvali, Phys. Rev. D, 59:086004 (1999) doi:10.1103/PhysRevD.59.086004[hep-ph/9807344]
    [67] N. Arkani-Hamed, S. Dimopoulos, and G. R. Dvali, Phys. Lett. B, 429:263 (1998) doi:10.1016/S0370-2693(98)00466-3[hep-ph/9803315]
    [68] G. R. Dvali, G. Gabadadze, M. Kolanovic, and F. Nitti, Phys. Rev. D, 64:084004 (2001) doi:10.1103/PhysRevD.64.084004[hep-ph/0102216]
    [69] E. Costa et al, Nature, 387:783-785 (1997) arXiv:astro-ph/9706065[astro-ph]
    [70] G. Amelino-Camelia, J. R. Ellis, N. E. Mavromatos, D. V. Nanopoulos, and S. Sarkar, Nature, 393:763-765 (1998) arXiv:astro-ph/9712103
    [71] J. Granot (Fermi LAT and GBM collaborations), p.321-328 of the Proceedings of the 44th Rencontres de Moriond on Very High Energy Phenomena in the Universe:eConf C09-02-01.2 arXiv:0905.2206[astro-ph.HE]
    [72] G. Amelino-Camelia and L. Smolin, Phys. Rev. D, 80:084017 (2009) arXiv:0906.3731[astro-ph.HE]
    [73] R.J. Nemiro, J. Holmes, and R. Connolly, Phys. Rev. Lett., 108:231103 (2012) arXiv:1109.5191[astro-ph.CO]
    [74] G. Amelino-Camelia, Living Rev. Rel., 16:5 (2013) arXiv:0806.0339
    [75] J. Albert et al (MAGIC Collaboration), Phys. Lett. B, 668:253-257 (2008) arXiv:0708.2889[astro-ph]
    [76] F. Aharonian et al (HESS Collaboration), Phys. Rev. Lett., 101:170402 (2008) arXiv:0810.3475[astro-ph]
    [77] G. Ghirlanda, G. Ghisellini, and L. Nava, Astron. Astrophys., 510:L7 (2010) arXiv:0909.0016[astro-ph.HE]
    [78] A.A. Abdo et al (Fermi LAT and Fermi GBM), Nature, 462:331-334 (2009)
    [79] A. Abramowski et al (HESS Collaboration), Astropart. Phys., 34:738-747 (2011) arXiv:1101.3650[astro-ph.HE]
    [80] O. Bertolami and C. S. Carvalho, Phys. Rev. D, 61:103002 (2000) arXiv:gr-qc/9912117
    [81] G. Amelino-Camelia, Int. J. Mod. Phys. D, 12:1633 (2003) arXiv:gr-qc/0305057
    [82] P. Mszros, S. Kobayashi, S. Razzaque, and B. Zhang, in R. Ouyed ed., Proceedings of the First Niels Bohr Summer Institute on Beaming and Jets in Gamma Ray Bursts (NBSI), Copenhagen, Denmark, August 12-30, 2002, eConf C0208122 (Stanford University, Stanford, 2003) arXiv:astro-ph/0305066
    [83] E. Waxman, Philos. Trans. R. Soc. London, Ser. A, 365:1323-1334 (2007) arXiv:astro-ph/0701170
    [84] U. Jacob and T. Piran, Nature Phys., 3:87-90 (2007)
    [85] G. Amelino-Camelia and L. Smolin, Phys. Rev. D, 80:084017 (2009) arXiv:0906.3731[astro-ph.HE]
    [86] G. Amelino-Camelia, D. Guetta, and T. Piran, Astrophys. J., 806(2):269 (2015) doi:10.1088/0004-637X/806/2/269
  • 加载中

Get Citation
Andrea Addazi, Pierluigi Belli, Rita Bernabei and Antonino Marcianò. Testing noncommutative spacetimes and violations of the Pauli Exclusion Principle through underground experiments[J]. Chinese Physics C, 2018, 42(9): 094001. doi: 10.1088/1674-1137/42/9/094001
Andrea Addazi, Pierluigi Belli, Rita Bernabei and Antonino Marcianò. Testing noncommutative spacetimes and violations of the Pauli Exclusion Principle through underground experiments[J]. Chinese Physics C, 2018, 42(9): 094001.  doi: 10.1088/1674-1137/42/9/094001 shu
Milestone
Received: 2018-04-24
Article Metric

Article Views(1721)
PDF Downloads(44)
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 noncommutative spacetimes and violations of the Pauli Exclusion Principle through underground experiments

    Corresponding author: Andrea Addazi,
    Corresponding author: Pierluigi Belli,
    Corresponding author: Rita Bernabei,
  • 1.  Center for Field Theory and Particle Physics &
  • 2.  INFN sezione Roma &ldquo

Abstract: We propose to deploy limits that arise from different tests of the Pauli Exclusion Principle:i) to provide theories of quantum gravity with experimental guidance; ii) to distinguish, among the plethora of possible models, the ones that are already ruled out by current data; iii) to direct future attempts to be in accordance with experimental constraints. We first review experimental bounds on nuclear processes forbidden by the Pauli Exclusion Principle, which have been derived by several experimental collaborations making use of various detector materials. Distinct features of the experimental devices entail sensitivities on the constraints hitherto achieved that may differ from one another by several orders of magnitude. We show that with choices of these limits, well-known examples of flat noncommutative space-time instantiations of quantum gravity can be heavily constrained, and eventually ruled out. We devote particular attention to the analysis of the κ-Minkowski and θ-Minkowski noncommutative spacetimes. These are deeply connected to some scenarios in string theory, loop quantum gravity, and noncommutative geometry. We emphasize that the severe constraints on these quantum spacetimes, although they cannot rule out theories of top-down quantum gravity to which they are connected in various ways, provide a powerful limitation for those models. Focus on this will be necessary in the future.

    HTML

Reference (86)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return