Plato's fire and the neutrino mass matrix

Modern Physics Letters A

Volumn 17, Issue 36, 2002, Pages 2361-2369

  Ma, Ernest ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Discrete lepton flavor symmetry; Neutrino mass matrix; Neutrino oscillations

Indexed keywords

ELEMENTARY PARTICLE; FIRE; FLAVOR; GEOMETRY; MATHEMATICAL ANALYSIS; OSCILLATION; RADIATION; SHORT SURVEY; SOLAR ENERGY; THEORY;

EID: 0037202922     PISSN: 02177323     EISSN: None     Source Type: Journal    
DOI: 10.1142/S021773230200909X     Document Type: Short Survey

References (22)

1. Q. R. Ahmad et al., SNO collab., Phys. Rev. Lett. 89, 011301; 011302 (2002).
2. S. Fukuda et al., Super-Kamiokande collab., Phys. Rev. Lett. 86, 5656 (2001) and references therein; Q. R. Ahmad et al., SNO collab., ibid. 87, 071301 (2001).
3. S. Fukuda et al., Super-Kamiokande collab., Phys. Rev. Lett. 86, 5656 (2001) and references therein; Q. R. Ahmad et al., SNO collab., ibid. 87, 071301 (2001).
4. S. Fukuda et al., Super-Kamiokande collab., Phys. Rev. Lett. 85, 3999 (2000) and references therein.
5. V. Barger et al., Phys. Lett. B537, 179 (2002); A. Bandyopadhyay et al., ibid. B540, 14 (2002); J. N. Bahcall et al., JHEP 07, 054 (2002); P. Aliani et al., hep-ph/0205053; P. C. de Holanda and A. Yu. Smirnov, hep-ph/0205241; A. Strumia et al., Phys. Lett. B541, 327 (2002); G. L. Fogli et al., Phys. Rev. D66, 053010 (2002); M. Maltoni et al., hep-ph/0207227, Phys. Rev. D, in press.
6. V. Barger et al., Phys. Lett. B537, 179 (2002); A. Bandyopadhyay et al., ibid. B540, 14 (2002); J. N. Bahcall et al., JHEP 07, 054 (2002); P. Aliani et al., hep-ph/0205053; P. C. de Holanda and A. Yu. Smirnov, hep-ph/0205241; A. Strumia et al., Phys. Lett. B541, 327 (2002); G. L. Fogli et al., Phys. Rev. D66, 053010 (2002); M. Maltoni et al., hep-ph/0207227, Phys. Rev. D, in press.
7. V. Barger et al., Phys. Lett. B537, 179 (2002); A. Bandyopadhyay et al., ibid. B540, 14 (2002); J. N. Bahcall et al., JHEP 07, 054 (2002); P. Aliani et al., hep-ph/0205053; P. C. de Holanda and A. Yu. Smirnov, hep-ph/0205241; A. Strumia et al., Phys. Lett. B541, 327 (2002); G. L. Fogli et al., Phys. Rev. D66, 053010 (2002); M. Maltoni et al., hep-ph/0207227, Phys. Rev. D, in press.
8. V. Barger et al., Phys. Lett. B537, 179 (2002); A. Bandyopadhyay et al., ibid. B540, 14 (2002); J. N. Bahcall et al., JHEP 07, 054 (2002); P. Aliani et al., hep-ph/0205053; P. C. de Holanda and A. Yu. Smirnov, hep-ph/0205241; A. Strumia et al., Phys. Lett. B541, 327 (2002); G. L. Fogli et al., Phys. Rev. D66, 053010 (2002); M. Maltoni et al., hep-ph/0207227, Phys. Rev. D, in press.
9. V. Barger et al., Phys. Lett. B537, 179 (2002); A. Bandyopadhyay et al., ibid. B540, 14 (2002); J. N. Bahcall et al., JHEP 07, 054 (2002); P. Aliani et al., hep-ph/0205053; P. C. de Holanda and A. Yu. Smirnov, hep-ph/0205241; A. Strumia et al., Phys. Lett. B541, 327 (2002); G. L. Fogli et al., Phys. Rev. D66, 053010 (2002); M. Maltoni et al., hep-ph/0207227, Phys. Rev. D, in press.
10. V. Barger et al., Phys. Lett. B537, 179 (2002); A. Bandyopadhyay et al., ibid. B540, 14 (2002); J. N. Bahcall et al., JHEP 07, 054 (2002); P. Aliani et al., hep-ph/0205053; P. C. de Holanda and A. Yu. Smirnov, hep-ph/0205241; A. Strumia et al., Phys. Lett. B541, 327 (2002); G. L. Fogli et al., Phys. Rev. D66, 053010 (2002); M. Maltoni et al., hep-ph/0207227, Phys. Rev. D, in press.
11. V. Barger et al., Phys. Lett. B537, 179 (2002); A. Bandyopadhyay et al., ibid. B540, 14 (2002); J. N. Bahcall et al., JHEP 07, 054 (2002); P. Aliani et al., hep-ph/0205053; P. C. de Holanda and A. Yu. Smirnov, hep-ph/0205241; A. Strumia et al., Phys. Lett. B541, 327 (2002); G. L. Fogli et al., Phys. Rev. D66, 053010 (2002); M. Maltoni et al., hep-ph/0207227, Phys. Rev. D, in press.
12. V. Barger et al., Phys. Lett. B537, 179 (2002); A. Bandyopadhyay et al., ibid. B540, 14 (2002); J. N. Bahcall et al., JHEP 07, 054 (2002); P. Aliani et al., hep-ph/0205053; P. C. de Holanda and A. Yu. Smirnov, hep-ph/0205241; A. Strumia et al., Phys. Lett. B541, 327 (2002); G. L. Fogli et al., Phys. Rev. D66, 053010 (2002); M. Maltoni et al., hep-ph/0207227, Phys. Rev. D, in press.
13. M. Apollonio et al., Phys. Lett. B466, 415 (1999);
14. F. Boehm et al., Phys. Rev. D64, 112001 (2001).
15. E. Ma, hep-ph/0207352, Phys. Rev. D, in press.
16. S. Weinberg, Phys. Rev. Lett. 43, 1566 (1979).
17. E. Ma, Phys. Rev. Lett. 81, 1171 (1998).
18. E. Ma and G. Rajasekaran, Phys. Rev. D64, 113012 (2001); E. Ma, Mod. Phys. Lett. A17, 289; 627 (2002).
19. E. Ma and G. Rajasekaran, Phys. Rev. D64, 113012 (2001); E. Ma, Mod. Phys. Lett. A17, 289; 627 (2002).
20. K. S. Babu, E. Ma, and J. W. F. Valle, hep-ph/0206292, Phys. Lett. B, in press.
21. Evidence for mo in the range 0.11 to 0.56 eV has been claimed by H. V. Klapdor-Kleingrothaus et al., Mod. Phys. Lett. A16, 2409 (2001); see also comments by C. E. Aalseth et al., Mod. Phys. Lett. A17, 1475 (2002), and the reply by H. V. Klapdor-Kleingrothaus, hep-ph/0205228.
22. Evidence for mo in the range 0.11 to 0.56 eV has been claimed by H. V. Klapdor-Kleingrothaus et al., Mod. Phys. Lett. A16, 2409 (2001); see also comments by C. E. Aalseth et al., Mod. Phys. Lett. A17, 1475 (2002), and the reply by H. V. Klapdor-Kleingrothaus, hep-ph/0205228.