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2024年10月30日

Massive and massless neutrinos on unbalanced seesaws

  • The observation of neutrino oscillations requires new physics beyond the standard model (SM). A SM-like gauge theory with p lepton families can be extended by introducing q heavy right-handed Majorana neutrinos but preserving its SU(2)L×U(1)Y gauge symmetry. The overall neutrino mass matrix M turns out to be a symmetric (p+q)×(p+q) matrix. Given p>q, the rank of $M$ is in general equal to 2q,corresponding to 2q non-zero mass eigenvalues. The existence of (p-q) massless left-handed Majorana neutrinos is an exact consequence of the model, independent of the usual approximation made in deriving the Type-I seesaw relation between the effective p×p light Majorana neutrino mass matrix Mν and the q×q heavy Majorana neutrino mass matrix MR. In other words, the numbers of massive left- and right-handed neutrinos are fairly matched. A good example to illustrate this "seesaw fair play rule" is the minimal seesaw model with p=3 and q=2, in which one massless neutrino sits on the unbalanced seesaw.
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  • [1] . Ahmad Q R et al. (SNO Collaboration). Phys. Rev. Lett.,2002, 89: 0113012. Jung C K et al. Ann. Rev. Nucl. Part. Sci., 2001, 51: 4513. Eguchi K et al. (KamLAND Collaboration). Phys. Rev.Lett., 2003, 90: 021802; Apollonio M et al. (CHOOZ Collaboration). Phys. Lett. B, 1998, 420: 397; Boehm F etal. (Palo Verde Collaboration). Phys. Rev. Lett., 2000, 84:37644. Ahn M H et al. (K2K Collaboration). Phys. Rev. Lett.,2003, 90: 0418015. Fritzsch H, XING Z Z. Prog. Part. Nucl. Phys., 2000, 45:1; Altarelli G, Feruglio F. New J. Phys., 2004, 6: 106; Mohapatra R N, Smirnov A Yu. Ann. Rev. Nucl. Part. Sci.,2006, 56: 5696. Minkowski P. Phys. Lett. B, 1977, 67: 421; Yanagida T. In:Sawada O, Sugamoto A ed. Proceedings of the Workshop on Unified Theory and the Baryon Number of the Universe. KEK, Tsukuba, 1979. 95; Gell-Mann M, Ramond P,Slansky R. In: van Nieuwenhuizen F, Freedman D ed. Supergravity. North Holland, Amsterdam, 1979. 315; Glashow S L. In: Lévy M et al. ed. Quarks and Leptons. New York:Plenum, 1980. 707; Mohapatra R N, Senjanovic G. Phys.Rev. Lett., 1980, 44: 9127. Fukugita M, Yanagida T. Phys. Lett. B, 1986, 174: 458. Frampton P, Glashow S L, Yanagida T. Phys. Lett. B, 2002,548: 119. GUO W L, XING Z Z, ZHOU S. Int. J. Mod.Phys. E, 2007, 16: 19. Schechter J, Valle J W F. Phys. Rev. D, 1980, 22: 222710. LIAO Y. Nucl. Phys. B, 2006, 749: 153; Eur. Phys. J. C,2007, 49: 78311. XING Z Z. Int. J. Mod. Phys. A, 2004, 19: 112. XING Z Z, ZHOU S. HEP NP, 2006, 30: 82813. Horn R A, Johnson C R. Matrix Analysis. Cambridge:Cambridge University Press, 198514. Strumia A, Vissani F. hep-ph/060605415. CHANG S, KANG S K, Kim S. Phys. Lett. B, 2004, 597:78; XING Z Z, ZHOU S. hep-ph/0607302; LUO S, XINGZ Z. Phys. Lett. B, 2007, 646: 242; Kitabayashi T. hep-ph/0703303; CHAN A H, Fritzsch H, XING Z Z. arXiv 0704.3153; Friedberg R, Lee T D. arXiv 0705.415616. Harrison P F, Perkins D H, Scott W G. Phys. Lett. B,2002, 530: 167; XING Z Z. Phys. Lett. B, 2002, 533: 85;Harrison P F, Scott W G. Phys. Lett. B, 2002, 535: 163;HE X G, Zee A. Phys. Lett. B, 2003, 560: 8717. MEI J W, XING Z Z. Phys. Rev. D, 2004, 69: 073003;LUO S, XING Z Z. Phys. Lett. B, 2006, 637: 279
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XING Zhi-Zhong. Massive and massless neutrinos on unbalanced seesaws[J]. Chinese Physics C, 2008, 32(2): 96-99. doi: 10.1088/1674-1137/32/2/004
XING Zhi-Zhong. Massive and massless neutrinos on unbalanced seesaws[J]. Chinese Physics C, 2008, 32(2): 96-99.  doi: 10.1088/1674-1137/32/2/004 shu
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Received: 2007-06-07
Revised: 1900-01-01
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Massive and massless neutrinos on unbalanced seesaws

    Corresponding author: XING Zhi-Zhong,
  • Institute of High Energy Physics, CAS, Beijing 100049, China2 Interdisciplinary Center for Theoretical Study, University of Science and Technology of China, Hefei 230026, China

Abstract: The observation of neutrino oscillations requires new physics beyond the standard model (SM). A SM-like gauge theory with p lepton families can be extended by introducing q heavy right-handed Majorana neutrinos but preserving its SU(2)L×U(1)Y gauge symmetry. The overall neutrino mass matrix M turns out to be a symmetric (p+q)×(p+q) matrix. Given p>q, the rank of $M$ is in general equal to 2q,corresponding to 2q non-zero mass eigenvalues. The existence of (p-q) massless left-handed Majorana neutrinos is an exact consequence of the model, independent of the usual approximation made in deriving the Type-I seesaw relation between the effective p×p light Majorana neutrino mass matrix Mν and the q×q heavy Majorana neutrino mass matrix MR. In other words, the numbers of massive left- and right-handed neutrinos are fairly matched. A good example to illustrate this "seesaw fair play rule" is the minimal seesaw model with p=3 and q=2, in which one massless neutrino sits on the unbalanced seesaw.

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