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《中国物理C》(英文)编辑部
2024年10月30日

Update on two-zero textures of the Majorana neutrino mass matrix in light of recent T2K, Super-Kamiokande and NOvA results

  • The latest results from atmospheric and accelerator neutrino experiments indicate that the normal neutrino mass ordering m1 < m2 < m3, a maximal leptonic CP-violating phase δ = 270° and the second octant of neutrino mixing angle θ23 > 45° are favored. In light of new experimental results, we update previous phenomenological studies on two-zero textures of the Majorana neutrino mass matrix Mv, in the flavor basis where the charged-lepton mass matrix Ml is diagonal. When the 1σ ranges of neutrino mixing parameters are taken into account, only four (i.e., A1, 2 and B2,4) among seven two-zero patterns of Mv show the aforementioned features of neutrino mass spectrum, mixing angle θ23 and CP-violating phase δ, and thus are compatible with the latest neutrino oscillation data. The correlative relations among neutrino masses and mixing parameters have been derived analytically for these four patterns, and the allowed regions of neutrino mixing angles and the CP-violating phase are also given. Possible realizations of four viable two-zero textures via non-Abelian discrete flavor symmetries are discussed.
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  • [1] K. Abe et al (T2K Collaboration), Phys. Rev. Lett., 107: 041801 (2011)[arXiv:1106.2822]
    [2] P. Adamson et al (MINOS Collaboration), Phys. Rev. Lett., 107: 181802 (2011) [arXiv:1108.0015]
    [3] Y. Abe et al (Double Chooz Collaboration), Phys. Rev. Lett., 108: 131801 (2012) [arXiv:1112.6353]
    [4] F. P. An et al (Daya Bay Collaboration), Phys. Rev. Lett., 108: 171803 (2012) [arXiv:1203.1669]
    [5] J. K. Ahn et al (RENO Collaboration), Phys. Rev. Lett., 108: 191802 (2012) [arXiv:1204.0626]
    [6] Y. Abe et al (Double Chooz Collaboration), Phys. Rev. D, 86: 052008 (2012) [arXiv:1207.6632]
    [7] K. Abe et al (T2K Collaboration), Phys. Rev. D, 91: 072010 (2015) [arXiv:1502.01550]
    [8] J. Bian, First Results of ve Appearance Analysis at NOvA, talk given at the Meeting of the Division of Particles and Fields of the American Physical Society, August 4-8, 2015
    [9] C. Kachulis,SK Atmospheric Neutrino Results, talk given at the Meeting of the Division of Particles and Fields of the American Physical Society, August 4-8, 2015
    [10] J. Elevant and T. Schwetz, JHEP, 1509: 016 (2015), arXiv:1506.07685
    [11] A. Palazzo, arXiv:1509.03148
    [12] H. Fritzsch, Z. Z. Xing and S. Zhou, JHEP, 1109: 083 (2011) [arXiv:1108.4534]
    [13] P. O. Ludl, S. Morisi and E. Peinado, Nucl. Phys. B, 857: 411 (2012) [arXiv:1109.3393]
    [14] D. Meloni and G. Blankenburg, Nucl. Phys. B, 867: 749 (2013) [arXiv:1204.2706]
    [15] S. Weinberg, Phys. Rev. Lett., 43: 1566 (1979)
    [16] P. Minkowski, Phys. Lett. B, 67: 421 (1977)
    [17] T. Yanagida, in Proceedings of the Workshop on Unified Theory and the Baryon Number of the Universe, edited by O. Sawada and Sugamoto (Tsukuba: KEK, 1979), p. 95
    [18] M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity, edited by P. van Nieuwenhuizen and D.Z. Freeman (Amsterdam: North-Holland, 1979), p. 315
    [19] S. L. Glashow, in Quarks and Leptons, edited by M. Levy, et al. (New York: Plenum, 1980), p. 707
    [20] R. N. Mohapatra and G. Senjanović, Phys. Rev. Lett., 44: 912 (1980)
    [21] W. Konetschny and W. Kummer, Phys. Lett. B, 70: 433 (1977)
    [22] J. Schechter and J. W. F. Valle, Phys. Rev. D, 22: 2227 (1980)
    [23] T. P. Cheng and L. F. Li, Phys. Rev. D, 22: 2860 (1980)
    [24] M. Magg and C. Wetterich, Phys. Lett. B, 94: 61 (1980)
    [25] G. Lazarides, Q. Shafi, and C. Wetterich, Nucl. Phys. B, 181: 287 (1981)
    [26] R. N. Mohapatra and G. Senjanović, Phys. Rev. D, 23: 165 (1981)
    [27] R. Foot, H. Lew, X. G. He, and G. C. Joshi, Z. Phys. C, 44: 441 (1989)
    [28] P. A. R. Ade et al (Planck Collaboration), arXiv:1502.01589
    [29] P. H. Frampton, S. L. Glashow and D. Marfatia, Phys. Lett. B, 536: 79 (2002) [hep-ph/0201008]
    [30] Z. Z. Xing, Phys. Lett. B, 530: 159 (2002) [hep-ph/0201151]
    [31] Z. Z. Xing, Phys. Lett. B, 539: 85 (2002) [hep-ph/0205032]
    [32] W. L. Guo and Z. Z. Xing, Phys. Rev. D, 67: 053002 (2003) [hep-ph/0212142]
    [33] S. Kaneko and M. Tanimoto, Phys. Lett. B, 551: 127 (2003) [hep-ph/0210155]
    [34] G. C. Branco, R. Gonzalez Felipe, F. R. Joaquim, I. Masina, M. N. Rebelo and C. A. Savoy, Phys. Rev. D, 67: 073025 (2003) [hep-ph/0211001]
    [35] W. Grimus and P. O. Ludl, Phys. Lett. B, 700: 356 (2011) [arXiv:1104.4340]
    [36] M. Frigerio and A. Villanova del Moral, JHEP, 1307: 146 (2013) [arXiv:1303.5284]
    [37] D. Meloni, A. Meroni and E. Peinado, Phys. Rev. D, 89: 053009 (2014) [arXiv:1401.3207]
    [38] R. Gonzlez Felipe and H. Serdio, Nucl. Phys. B, 886: 75 (2014) [arXiv:1405.4263]
    [39] L. M. Cebola, D. Emmanuel-Costa and R. G. Felipe, Phys. Rev. D, 92: 025005 (2015) [arXiv:1504.06594]
    [40] M. C. Gonzalez-Garcia, M. Maltoni and T. Schwetz, JHEP, 1411: 052 (2014) [arXiv:1409.5439]
    [41] F. Capozzi, G. L. Fogli, E. Lisi, A. Marrone, D. Montanino and A. Palazzo, Phys. Rev. D, 89: 093018 (2014)
    [42] D. V. Forero, M. Tortola and J. W. F. Valle, Phys. Rev. D, 90: 093006 (2014) [arXiv:1405.7540]
    [43] H. Ps and W. Rodejohann, arXiv:1507.00170
    [44] S. M. Bilenky and C. Giunti, Int. J. Mod. Phys. A, 30 (04n05): 1530001 (2015) [arXiv:1411.4791]
    [45] S. M. Bilenky and C. Giunti, Mod. Phys. Lett., A 27: 1230015 (2012) [arXiv:1203.5250]
    [46] W. Rodejohann, Int. J. Mod. Phys. E, 20: 1833 (2011) [arXiv:1106.1334]
    [47] W. Grimus, A. S. Joshipura, L. Lavoura and M. Tanimoto, Eur. Phys. J. C, 36: 227 (2004) [hep-ph/0405016]
    [48] M. Hirsch, A. S. Joshipura, S. Kaneko and J. W. F. Valle, Phys. Rev. Lett., 99: 151802 (2007) [hep-ph/0703046]
    [49] E. Ma and G. Rajasekaran, Phys. Rev. D, 64: 113012 (2001) [hep-ph/0106291]
    [50] K. S. Babu, E. Ma and J. W. F. Valle, Phys. Lett. B, 552: 207 (2003) [hep-ph/0206292]
    [51] P. H. Gu, H. Zhang and S. Zhou, Phys. Rev. D, 74: 076002 (2006) [hep-ph/0606302]
    [52] G. Altarelli and F. Feruglio, Rev. Mod. Phys., 82: 2701 (2010) [arXiv:1002.0211]
    [53] H. Ishimori, T. Kobayashi, H. Ohki, Y. Shimizu, H. Okada and M. Tanimoto, Prog. Theor. Phys. Suppl., 183: 1 (2010) [arXiv:1003.3552]
    [54] S. F. King and C. Luhn, Rept. Prog. Phys., 76: 056201 (2013) [arXiv:1301.1340]
    [55] M. Fukugita and T. Yanagida, Phys. Lett. B, 174: 45 (1986)
    [56] S. Davidson, E. Nardi and Y. Nir, Phys. Rept., 466: 105 (2008) [arXiv:0802.2962]
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Get Citation
Shun Zhou. Update on two-zero textures of the Majorana neutrino mass matrix in light of recent T2K, Super-Kamiokande and NOvA results[J]. Chinese Physics C, 2016, 40(3): 033102. doi: 10.1088/1674-1137/40/3/033102
Shun Zhou. Update on two-zero textures of the Majorana neutrino mass matrix in light of recent T2K, Super-Kamiokande and NOvA results[J]. Chinese Physics C, 2016, 40(3): 033102.  doi: 10.1088/1674-1137/40/3/033102 shu
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Received: 2015-09-21
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    Supported in part by the Innovation Program of the Institute of High Energy Physics (Y4515570UI), National Youth Thousand Talents Program, and the CAS Center for Excellence in Particle Physics (CCEPP)

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Update on two-zero textures of the Majorana neutrino mass matrix in light of recent T2K, Super-Kamiokande and NOvA results

    Corresponding author: Shun Zhou,
  • 1. Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
  • 2. Center for High Energy Physics, Peking University, Beijing 100080, China
Fund Project:  Supported in part by the Innovation Program of the Institute of High Energy Physics (Y4515570UI), National Youth Thousand Talents Program, and the CAS Center for Excellence in Particle Physics (CCEPP)

Abstract: The latest results from atmospheric and accelerator neutrino experiments indicate that the normal neutrino mass ordering m1 < m2 < m3, a maximal leptonic CP-violating phase δ = 270° and the second octant of neutrino mixing angle θ23 > 45° are favored. In light of new experimental results, we update previous phenomenological studies on two-zero textures of the Majorana neutrino mass matrix Mv, in the flavor basis where the charged-lepton mass matrix Ml is diagonal. When the 1σ ranges of neutrino mixing parameters are taken into account, only four (i.e., A1, 2 and B2,4) among seven two-zero patterns of Mv show the aforementioned features of neutrino mass spectrum, mixing angle θ23 and CP-violating phase δ, and thus are compatible with the latest neutrino oscillation data. The correlative relations among neutrino masses and mixing parameters have been derived analytically for these four patterns, and the allowed regions of neutrino mixing angles and the CP-violating phase are also given. Possible realizations of four viable two-zero textures via non-Abelian discrete flavor symmetries are discussed.

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