Impact factor of Chinese Physics C is 3.6 in 2023 Impact factor of Chinese Physics C is 3.6 in 2022 2021 Impact Factor 2.944
Advanced Search
Chinese Physics C > 2016, Vol. 40 > Issue(3): 033102 DOI: 10.1088/1674-1137/40/3/033102

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

  • 1.

    Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

  • 2.

    Center for High Energy Physics, Peking University, Beijing 100080, China

  • The latest results from atmospheric and accelerator neutrino experiments indicate that the normal neutrino mass ordering m 1< m 2< m 3, a maximal leptonic CP-violating phase δ= 270° and the second octant of neutrino mixing angle θ 23> 45° are favored. In light of new experimental results, we update previous phenomenological studies on two-zero textures of the Majorana neutrino mass matrix M v, in the flavor basis where the charged-lepton mass matrix M lis diagonal. When the 1σ ranges of neutrino mixing parameters are taken into account, only four (i.e., A 1, 2and B 2,4) among seven two-zero patterns of M vshow the aforementioned features of neutrino mass spectrum, mixing angle θ 23and 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.
      PCAS:
  • 加载中

  • References

    [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]

  • Access

    加载中

Get Citation
Shun Zhou. Update on two-zero textures of the Majorana neutrino mass matrix in light of recent T2K, Super-Kamiokande and NO vA 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 NO vA results[J]. Chinese Physics C, 2016, 40(3): 033102. doi:10.1088/1674-1137/40/3/033102 shu
Milestone
Received: 2015-09-21
Fund

    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)

Article Metric

Article Views(4165)
PDF Downloads(40)
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:

    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
    • Received Date:2015-09-21
    • Available Online:2016-02-29
    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 orderingm1<m2<m3, a maximal leptonic CP-violating phaseδ= 270° and the second octant of neutrino mixing angleθ23> 45° are favored. In light of new experimental results, we update previous phenomenological studies on two-zero textures of the Majorana neutrino mass matrixMv, in the flavor basis where the charged-lepton mass matrixMlis diagonal. When the 1σ ranges of neutrino mixing parameters are taken into account, only four (i.e.,A1, 2andB2,4) among seven two-zero patterns ofMvshow the aforementioned features of neutrino mass spectrum, mixing angleθ23and CP-violating phaseδ, 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.

        HTML

      Reference (56)

      目录

      Link
      IOPScience
      SCOAP3
      arXiv
      Chinese Physical Society
      Journal information
      Introduction
      Editorial Board
      Others
      Subscribe
      Contact us
      QQ: 1307685413
      Tel: +86-010-88235947
      Fax: +86-010-88233126
      E-mail: cpc@ihep.ac.cn

      • CPC Website

      • IOP Website

      • CPC WeChat

      Copyright © Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 京ICP备05002789号-1

      Supported by:Beijing Renhe Information Technology Co. Ltd E-mail:info@rhhz.net

      /

        Return
        Return
          Baidu
          map