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《中国物理C》(英文)编辑部
2024年10月30日

Broken S3L×S3R flavor symmetry and leptonic CP violation

  • In the framework of the canonical seesaw model, we present a simple but viable scenario to explicitly break an S3L×S3R flavor symmetry in the leptonic sector. It turns out that the leptonic flavor mixing matrix is completely determined by the mass ratios of the charged leptons (i.e., me/mμ and mμ/mτ) and those of light neutrinos (i.e., m1/m2 and m2/m3). The latest global-fit results of the three neutrino mixing angles θ12, θ13, θ23 and two neutrino mass-squared differences △ m212, △ m312 at the 3σ level are used to constrain the parameter space of m1/m2, m2/m3. The predictions for the mass spectrum and flavor mixing are highlighted:(1) the neutrino mass spectrum shows a hierarchical pattern and a normal ordering, e.g., m1 ≈ 2.2 meV, m2 ≈ 8.8 meV and m3 ≈ 52.7 meV; (2) only the first octant of θ23 is allowed, namely, 41.8° ≤ θ23 ≤ 43.3° (3) the Dirac CP-violating phase δ ≈ -22° deviates significantly from the maximal value -90°. All these predictions are ready to be tested in ongoing and forthcoming neutrino oscillation experiments. Moreover, we demonstrate that the cosmological matter-antimatter asymmetry can be explained via resonant leptogenesis, including the individual lepton-flavor effects. In our scenario, leptonic CP violation at low-and high-energy scales is closely connected.
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  • [1] T. Kajita, Rev. Mod. Phys., 88(3):030501(2016)
    [2] A. B. McDonald, Rev. Mod. Phys., 88(3):030502(2016)
    [3] B. Pontecorvo, Sov. Phys. JETP, 6:429(1957); Zh. Eksp. Teor. Fiz., 33:549(1957)
    [4] Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theor. Phys., 28:870(1962)
    [5] C. Patrignani et al (Particle Data Group), Chin. Phys. C, 40(10):100001(2016)
    [6] F. Capozzi, E. Lisi, A. Marrone, D. Montanino, and A. Palazzo, Nucl. Phys. B, 908:218(2016), arXiv:1601.07777
    [7] F. Capozzi, E. Di Valentino, E. Lisi, A. Marrone, A. Melchiorri, and A. Palazzo, Phys. Rev. D, 95(9):096014(2017), arXiv:1703.04471
    [8] D. V. Forero, M. Tortola, and J. W. F. Valle, Phys. Rev. D, 90(9):093006(2014), arXiv:1405.7540
    [9] F. An et al (JUNO Collaboration), J. Phys. G 43(3):030401(2016), arXiv:1507.05613
    [10] S. B. Kim, Nuovo Cim. C, 39(4):317(2017)
    [11] K. Abe et al (T2K Collaboration), Nucl. Instrum. Meth. A, 659:106(2011), arXiv:1106.1238
    [12] D. S. Ayres et al (NOvA Collaboration), NOvA:Proposal to Build a 30 Kiloton Off-Axis Detector to Study e Oscillations in the NuMI Beamline, hep-ex/0503053
    [13] R. Acciarri et al (DUNE Collaboration), Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE):Volume 2:The Physics Program for DUNE at LBNF, arXiv:1512.06148
    [14] P. Minkowski, Phys. Lett. B, 67:421(1977)
    [15] T. Yanagida, In Proceedings of the Workshop on Unified Theory and the Baryon Number of the Universe:edited by O. Sawada and A. Sugamoto, (KEK, Tsukuba, 1979), p.95
    [16] M. Gell-Mann, P. Ramond, and R. Slansky, In Supergravity:edited by P. van Nieuwenhuizen and D. Z. Freeman, (North-Holland, Amsterdam, 1979), p. 315
    [17] S. L. Glashow, In Quarks and Leptons:edited by M. Levy et al, (Plenum, New York, 1980), p. 707
    [18] R. N. Mohapatra, and G. Senjanovic, Phys. Rev. Lett., 44:912(1980)
    [19] Z. Z. Xing and S. Zhou, Neutrinos in particle physics, astronomy and cosmology, (Springer-Verlag, Berlin Heidelberg, 2011)
    [20] H. Harari, H. Haut, and J. Weyers, Phys. Lett. B, 78:459(1978)
    [21] C. D. Froggatt and H. B. Nielsen, Nucl. Phys. B, 147:277(1979)
    [22] Y. Koide, Z. Phys. C, 45:39(1989)
    [23] M. Tanimoto, Phys. Rev. D, 41:1586(1990)
    [24] P. Kaus and S. Meshkov, Phys. Rev. D, 42:1863(1990)
    [25] G. C. Branco, J. I. Silva-Marcos, and M. N. Rebelo, Phys. Lett. B, 237:446(1990)
    [26] H. Fritzsch and J. Plankl, Phys. Lett. B, 237:451(1990)
    [27] H. Fritzsch and D. Holtmannspotter, Phys. Lett. B, 338:290(1994), hep-ph/9406241
    [28] G. C. Branco and J. I. Silva-Marcos, Phys. Lett. B, 359:166(1995), hep-ph/9507299
    [29] H. Fritzsch and Z. Z. Xing, Phys. Lett. B, 372:265(1996), hep-ph/9509389
    [30] Z. Z. Xing, J. Phys. G, 23:1563(1997), hep-ph/9609204
    [31] M. Fukugita, M. Tanimoto, and T. Yanagida, Phys. Rev. D, 57:4429(1998), hep-ph/9709388
    [32] A. Mondragon and E. Rodriguez-Jauregui, Phys. Rev. D, 59:093009(1999), hep-ph/9807214
    [33] H. Fritzsch and Z. Z. Xing, Prog. Part. Nucl. Phys., 45:1(2000), hep-ph/9912358
    [34] N. Haba, Y. Matsui, N. Okamura, and T. Suzuki, Phys. Lett. B, 489:184(2000), hep-ph/0005064
    [35] G. C. Branco and J. I. Silva-Marcos, Phys. Lett. B, 526:104(2002), hep-ph/0106125
    [36] M. Fujii, K. Hamaguchi, and T. Yanagida, Phys. Rev. D, 65:115012(2002), hep-ph/0202210
    [37] P. F. Harrison and W. G. Scott, Phys. Lett. B, 557:76(2003), hep-ph/0302025
    [38] J. Kubo, A. Mondragon, M. Mondragon, and E. Rodriguez-Jauregui, Prog. Theor. Phys., 109:795(2003); Prog. Theor. Phys., 114:287(2005), hep-ph/0302196
    [39] S. L. Chen, M. Frigerio, and E. Ma, Phys. Rev. D, 70:073008(2004); Phys. Rev. Dm 70:079905(2004), hep-ph/0404084
    [40] H. Fritzsch and Z. Z. Xing, Phys. Lett. B, 598:237(2004), hep-ph/0406206
    [41] W. Rodejohann and Z. Z. Xing, Phys. Lett. B, 601:176(2004), hep-ph/0408195
    [42] T. Araki, J. Kubo, and E. A. Paschos, Eur. Phys. J. C, 45:465(2006), hep-ph/0502164
    [43] T. Teshima, Phys. Rev. D, 73:045019(2006), hep-ph/0509094
    [44] T. Kimura, Prog. Theor. Phys., 114:329(2005)
    [45] R. N. Mohapatra, S. Nasri, and H. B. Yu, Phys. Lett. B, 639:318(2006), hep-ph/0605020
    [46] Y. Koide, Eur. Phys. J. Cm 50:809(2007), hep-ph/0612058
    [47] A. Mondragon, M. Mondragon, and E. Peinado, Phys. Rev. D, 76:076003(2007), arXiv:0706.0354
    [48] Z. Z. Xing, D. Yang, and S. Zhou, Phys. Lett. B, 690:304(2010), arXiv:1004.4234
    [49] T. Teshima and Y. Okumura, Phys. Rev. D, 84:016003(2011), arXiv:1103.6127
    [50] S. Zhou, Phys. Lett. B, 704:291(2011), arXiv:1106.4808
    [51] P. V. Dong, H. N. Long, C. H. Nam, and V. V. Vien, Phys. Rev. D, 85:053001(2012), arXiv:1111.6360
    [52] S. Dev, R. R. Gautam, and L. Singh, Phys. Lett. B, 708:284(2012), arXiv:1201.3755
    [53] F. Gonzalez Canales, A. Mondragon, and M. Mondragon, Fortsch. Phys., 61:546(2013), arXiv:1205.4755
    [54] R. Jora, J. Schechter, and M. N. Shahid, Int. J. Mod. Phys. A, 28:1350028(2013), arXiv:1210.6755
    [55] F. Gonzlez Canales, A. Mondragn, M. Mondragn, U. J. Salda na Salazar, and L. Velasco-Sevilla, Phys. Rev. D, 88:096004(2013), arXiv:1304.6644
    [56] C. Arbelez, A. E. Crcamo Hernndez, S. Kovalenko, and I. Schmidt, arXiv:1602.03607
    [57] M. J. S. Yang, Phys. Lett. B, 760:747(2016), arXiv:1604.07896
    [58] J. Xu, X. Yang, and D. Yang, Mod. Phys. Lett. A, 31(24):1650131(2016)
    [59] S. Pramanick and A. Raychaudhuri, Phys. Rev. D, 94(11):115028(2016), arXiv:1609.06103
    [60] E. Barradas-Guevara, O. Flix-Beltrn, F. Gonzalez-Canales, and M. Zeleny-Mora, arXiv:1704.03474
    [61] H. Fritzsch, Z. Z. Xing, and D. Zhang, arXiv:1705.01391
    [62] M. Fukugita and T. Yanagida, Phys. Lett. B, 174:45(1986)
    [63] A. Pilaftsis, Phys. Rev. D, 56:5431(1997), hep-ph/9707235
    [64] A. Pilaftsis and T. E. J. Underwood, Nucl. Phys. B, 692:303(2004), hep-ph/0309342
    [65] Z. Z. Xing, H. Zhang and S. Zhou, Phys. Rev. D, 77:113016(2008), arXiv:0712.1419
    [66] Z. Z. Xing, H. Zhang, and S. Zhou, Phys. Rev. D, 86:013013(2012), arXiv:1112.3112
    [67] K. Abe et al (Hyper-Kamiokande Working Group), arXiv:1412.4673
    [68] E. Wildner et al, Adv. High Energy Phys., 2016:8640493(2016), arXiv:1510.00493
    [69] J. Cao et al, Phys. Rev. ST Accel. Beams, 17:090101(2014), arXiv:1401.8125
    [70] M. Blennow, P. Coloma, and E. Fernndez-Martinez, JHEP, 1603:197(2016), arXiv:1511.02859
    [71] Y. Wang and Z. Z. Xing, Adv. Ser. Direct. High Energy Phys., 26:371(2016), arXiv:1504.06155
    [72] K. N. Abazajian et al (CMB-S4 Collaboration), CMB-S4 Science Book, First Edition, arXiv:1610.02743
    [73] W. Buchmuller, P. Di Bari, and M. Plumacher, Annals Phys., 315:305(2005), hep-ph/0401240
    [74] W. Buchmuller, R. D. Peccei, and T. Yanagida, Ann. Rev. Nucl. Part. Sci., 55:311(2005), hep-ph/0502169
    [75] S. Davidson, E. Nardi, and Y. Nir, Phys. Rept., 466:105(2008), arXiv:0802.2962
    [76] T. Hambye, New J. Phys., 14:125014(2012), arXiv:1212.2888
    [77] R. Barbieri, P. Creminelli, A. Strumia, and N. Tetradis, Nucl. Phys. B, 575:61(2000), hep-ph/9911315
    [78] A. Abada, S. Davidson, F. X. Josse-Michaux, M. Losada, and A. Riotto, JCAP, 0604:004(2006), hep-ph/0601083
    [79] E. Nardi, Y. Nir, E. Roulet, and J. Racker, JHEP, 0601:164(2006), hep-ph/0601084
    [80] P. A. R. Ade et al (Planck Collaboration), Astron. Astrophys., 594:A13(2016), arXiv:1502.01589
    [81] Z. Z. Xing and S. Zhou, Phys. Lett. B, 653:278(2007), hep-ph/0607302
    [82] J. Zhang and S. Zhou, JHEP, 1509:065(2015), arXiv:1505.04858
    [83] S. Blanchet and P. Di Bari, JCAP, 0606:023(2006), hep-ph/0603107
    [84] S. Blanchet and P. Di Bari, JCAP, 0703:018(2007), hep-ph/0607330
    [85] H. Ishimori, T. Kobayashi, H. Ohki, Y. Shimizu, H. Okada, and M. Tanimoto, Prog. Theor. Phys. Suppl., 183:1(2010), arXiv:1003.3552
    [86] W. Grimus and P. O. Ludl, J. Phys. A, 45:233001(2012), arXiv:1110.6376
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Zong-guo Si, Xing-hua Yang and Shun Zhou. Broken S3L×S3R flavor symmetry and leptonic CP violation[J]. Chinese Physics C, 2017, 41(11): 113105. doi: 10.1088/1674-1137/41/11/113105
Zong-guo Si, Xing-hua Yang and Shun Zhou. Broken S3L×S3R flavor symmetry and leptonic CP violation[J]. Chinese Physics C, 2017, 41(11): 113105.  doi: 10.1088/1674-1137/41/11/113105 shu
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Received: 2017-06-19
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Broken S3L×S3R flavor symmetry and leptonic CP violation

    Corresponding author: Zong-guo Si,
    Corresponding author: Xing-hua Yang,
    Corresponding author: Shun Zhou,
  • 1.  School of Physics, Shandong University, Jinan, Shandong 250100, China
  • 2. Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
  • 3. School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
  • 4. Center for High Energy Physics, Peking University, Beijing 100871, China
Fund Project:  Supported by NNSFC (11325525), National Recruitment Program for Young Professionals and CAS Center for Excellence in Particle Physics (CCEPP)

Abstract: In the framework of the canonical seesaw model, we present a simple but viable scenario to explicitly break an S3L×S3R flavor symmetry in the leptonic sector. It turns out that the leptonic flavor mixing matrix is completely determined by the mass ratios of the charged leptons (i.e., me/mμ and mμ/mτ) and those of light neutrinos (i.e., m1/m2 and m2/m3). The latest global-fit results of the three neutrino mixing angles θ12, θ13, θ23 and two neutrino mass-squared differences △ m212, △ m312 at the 3σ level are used to constrain the parameter space of m1/m2, m2/m3. The predictions for the mass spectrum and flavor mixing are highlighted:(1) the neutrino mass spectrum shows a hierarchical pattern and a normal ordering, e.g., m1 ≈ 2.2 meV, m2 ≈ 8.8 meV and m3 ≈ 52.7 meV; (2) only the first octant of θ23 is allowed, namely, 41.8° ≤ θ23 ≤ 43.3° (3) the Dirac CP-violating phase δ ≈ -22° deviates significantly from the maximal value -90°. All these predictions are ready to be tested in ongoing and forthcoming neutrino oscillation experiments. Moreover, we demonstrate that the cosmological matter-antimatter asymmetry can be explained via resonant leptogenesis, including the individual lepton-flavor effects. In our scenario, leptonic CP violation at low-and high-energy scales is closely connected.

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