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《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.
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  • [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
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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
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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.

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