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Volumn 60, Issue 5, 1999, Pages

Gravitationally violated U(1) symmetry and neutrino anomalies

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EID: 17244378941     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.60.053002     Document Type: Article
Times cited : (18)

References (51)
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    • T. Kajita, in Neutrino 98, Proceedings of the XVIIIth International Conference on Neutrino Physics and Astrophysics, Takayama, Japan, 1998, edited by Y. Suzuki and Y. Totsuka [Nucl. Phys. B. (Proc. Suppl.) (to be published)]
    • Phys. Rev. Lett.Y. Fukuda81, 1562 (1998);T. Kajita, in Neutrino 98, Proceedings of the XVIIIth International Conference on Neutrino Physics and Astrophysics, Takayama, Japan, 1998, edited by Y. Suzuki and Y. Totsuka [Nucl. Phys. B. (Proc. Suppl.) (to be published)].
    • (1998) Phys. Rev. Lett. , vol.81 , pp. 1562
    • Fukuda, Y.1
  • 12
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    • See, e.g., R. N. Mohapatra and Palash B. Pal, Massive Neutrinos in Physics and Astrophysics (World Scientific, Singapore, 1991)
    • See, e.g., R. N. Mohapatra and Palash B. Pal, Massive Neutrinos in Physics and Astrophysics (World Scientific, Singapore, 1991).
  • 13
    • 85037207240 scopus 로고    scopus 로고
    • hep-ph/9807235
    • R. Barbieri, Report No. hep-ph/9807235.
    • Barbieri, R.1
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    • 85037231583 scopus 로고    scopus 로고
    • hep-ph/9807327
    • E.J. Chun, Report No. hep-ph/9807327
    • Chun, E.J.1
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  • 23
    • 85037183946 scopus 로고    scopus 로고
    • Y. Suzuki, in Neutrino 98, Proceedings of the XVIIIth International Conference on Neutrino Physics and Astrophysics, Takayama, Japan, 1998, edited by Y. Suzuki and Y. Totsuka [Nucl. Phys. B (Proc. Suppl.) (to be published)]
    • Y. Suzuki, in Neutrino 98, Proceedings of the XVIIIth International Conference on Neutrino Physics and Astrophysics, Takayama, Japan, 1998, edited by Y. Suzuki and Y. Totsuka [Nucl. Phys. B (Proc. Suppl.) (to be published)].
  • 25
    • 85037255594 scopus 로고    scopus 로고
    • Note that the (Formula presented) symmetry allows a nondiagonal charged lepton mass matrix mixing (Formula presented) and (Formula presented) with some angle (Formula presented) The effect of this is to replace the angle (Formula presented) in Eq. (1) by (Formula presented) This combination needs to be large
    • Note that the (Formula presented) symmetry allows a nondiagonal charged lepton mass matrix mixing (Formula presented) and (Formula presented) with some angle (Formula presented) The effect of this is to replace the angle (Formula presented) in Eq. (1) by (Formula presented) This combination needs to be large.
  • 26
    • 33750639446 scopus 로고
    • K.S. Babu, Talk at the Trieste Conference on Quarks and leptons: Masses and Mixing, Trieste, Italy, 1996
    • R.N. Mohapatra and G. Senjanovic, Phys. Rev. D 23, 165 (1981);K.S. Babu, Talk at the Trieste Conference on Quarks and leptons: Masses and Mixing, Trieste, Italy, 1996
    • (1981) Phys. Rev. D , vol.23 , pp. 165
    • Mohapatra, R.N.1    Senjanovic, G.2
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    • Ernest Ma and Utpal Sarkar, Phys. Rev. Lett. 80, 5716 (1998).
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  • 38
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    • Note that parameters of some of these quartic terms would need to be fine tuned in order to obtain the doublet vev at the electroweak scale. This fine tuning is a reflection of the familiar gauge hierarchy problem and can be avoided by considering a supersymmetric version of the model
    • Note that parameters of some of these quartic terms would need to be fine tuned in order to obtain the doublet vev at the electroweak scale. This fine tuning is a reflection of the familiar gauge hierarchy problem and can be avoided by considering a supersymmetric version of the model.


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