Neutrinos on Earth and in the heavens

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 61, Issue 9, 2000, Pages

  Georgi, Howard ^a   Glashow, S L ^a  

^a HARVARD UNIVERSITY   (United States)

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Indexed keywords

EID: 17044422499     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.61.097301     Document Type: Article

References (19)

1. For a recent review, see J. R. Primack, SCIPP-96-59-REV, in the Proceedings of Midrasha Mathematicae in Jerusalem: Winter School in Dynamical Systems, Jerusalem, Israel, 1997, astro-ph/9707285.
2. A good recent review is R. N. Mohapatra, Nucl. Phys. B (Proc. Suppl.) 77, 376 (1999).
3. Other recent papers on the subject include: J.W.F. Valle, hep-ph/9509306
4. H. Minakata and O. Yasuda, Nucl. Phys. B523, 597 (1997)
5. F. Vissani, hep-ph/9708483
6. H. Minakata and O. Yasuda, Phys. Rev. D 56, 1692 (1997).
7. For a recent discussion of the full range of possibilities, see A. Y. Smirnov, “Lepton mixing: Small, large, maximal?,” hep-ph/9907296.
8. The neutrino mass matrix we are led to coincides with the “bimaximal mixing matrix” described by V. Barger, S. Pakvasa, T. J. Weiler, and K. Whisnant, Phys. Lett. B 437, 107 (1998).
9. See R. Barbieri, J. High Energy Phys. 12, 017 (1998).
10. Super-Kamiokande Collaboration, Y. Fukuda, Phys. Rev. Lett. 81, 1562 (1998).
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12. Kate Scholberg for the Super-Kamiokande Collaboration, K. Scholberg, hep-ex/9905016. We have taken this limit from Fig. 10.
13. For example, Y. Suzuki, in Proceedings of the XVIII International Conference on Neutrino Physics and Astrophysics, Takayama, Japan, 1998.
14. For example, J. N. Bahcall, Phys. Rev. D 58, 096016 (1998).
15. S. Nussinov, Phys. Lett. 63B, 201 (1976);see 10 for other references and for a critique of this possibility.
16. L. Baudis, Phys. Lett. B 407, 219 (1997).
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18. V. Barger, K. Whisnant, and R. J. N. Phillips, Phys. Rev. D 24, 538 (1981)
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