Deviation of atmospheric mixing from maximal and structure in the leptonic flavor sector

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 69, Issue 9, 2004, Pages 12-

  Gouvêa, André ^a  

^a NORTHWESTERN UNIVERSITY   (United States)

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EID: 3042634910     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.69.093007     Document Type: Article

References (60)

1. Super-Kamiokande Collaboration, Y. Fukuda, Phys. Rev. Lett. 81, 1562 (1998).
2. B.T. Cleveland, Astrophys. J. 496, 505 (1998)
3. GALLEX Collaboration, W. Hampell, Phys. Lett. B 447, 127 (1999)
4. Super-Kamiokande Collaboration, S. Fukuda, Phys. Rev. Lett. 86, 5656 (2001)
5. Sage Collaboration, J.N. Abdurashitov, Zh. Éksp. Teor. Fiz. 122, 211 (2002) [J. Exp. Theor. Phys. 95, 181 (2002)];E. Belotti for the GNO Collaboration, talk at the VIIIth International Conference on Topics in Astroparticle and Underground Physics (TAUP 03), Seattle, 2003
6. SNO Collaboration, Q.R. Ahmad, Phys. Rev. Lett. 89, 011301 (2002)
7. SNO Collaboration, S.N. Ahmed, nucl-ex/0309004, and many references therein.
8. KamLAND Collaboration, K. Eguchi, Phys. Rev. Lett. 90, 021802 (2003).
9. Particle Data Group, K. Hagiwara, Phys. Rev. D 66, 010001 (2002).
10. A. de Gouvêa and H. Murayama, Phys. Lett. B 573, 94 (2003).
11. CHOOZ Collaboration, M. Apollonio, Phys. Lett. B 466, 415 (1999)
12. M. ApollonioEur. Phys. J. C 27, 331 (2003).
13. G.L. Fogli, Phys. Rev. D 69, 017301 (2004) for the most recent bound, including the revised super Kamiokande estimate for the atmospheric mass-squared difference 18.
14. See, for example, T. Moroi, J. High Energy Phys. 03, 019 (2000)
15. See also D. Chang, A. Masiero, and H. Murayama, Phys. Rev. D 67, 075013 (2003).
16. See, for example, A. de Gouvêa and J.W.F. Valle, Phys. Lett. B 501, 115 (2001).
17. L.J. Hall, H. Murayama, and N. Weiner, Phys. Rev. Lett. 84, 2572 (2000).
18. Y. Itow, hep-ex/0106019
19. D. Ayres, hep-ex/0210005
20. M.V. Diwan, Phys. Rev. D 68, 012002 (2003).
21. For a recent review of current proposals, see T. Nakaya, Nucl. Phys. B (Proc. Suppl.) 118, 210 (2003).
22. H. Minakata, Phys. Rev. D 68, 033017 (2003)
23. M.H. Shaevitz and J.M. Link, hep-ex/0306031;K. Heeger, talk at the Weak Interactions and Neutrinos Workshop, 2003 (WIN 03), Lake Geneva, October 6–11, 2003.
24. See also P. Huber, M. Lindner, T. Schwetz, and W. Winter, Nucl. Phys. B665, 487 (2003).
25. For recent reviews see R.N. Mahapatra, hep-ph/9910365
26. S.M. Barr and I. Dorsner, Nucl. Phys. B585, 79 (2000)
27. G. Altarelli and F. Feruglio, hep-ph/0206077
28. G. AltarelliF. Ferugliohep-ph/0306265
29. S.F. King, Rep. Prog. Phys. 67, 107 (2004), and references therein.
30. See, for example, H.S. Goh, R.N. Mohapatra, and S.P. Ng, Phys. Rev. D 68, 115008 (2003)
31. Phys. Rev. DC.H. Albright and S.M. Barr, 67, 013002 (2003)
32. H.D. Kim and S. Raby, J. High Energy Phys. 07, 014 (2003)
33. M.C. Chen and K.T. Mahanthappa, Phys. Rev. D 68, 017301 (2003) for some recent efforts.
34. See, for example, M. Maltoni, T. Schwetz, M.A. Tortola, and J.W.F. Valle, Phys. Rev. D 68, 113010 (2003), for the most recent attempt at fitting all solar, reactor, and atmospheric data, and many references therein.
35. J.A. Aguilar-Saavedra, Phys. Rev. D 67, 073026 (2003)
36. J.A. Aguilar-Saavedra, G.C. Branco, and F.R. Joaquim, (to be published) hep-ph/0310305.
37. S.F. King, Phys. Lett. B 439, 350 (1998)
38. S.F. KingNucl. Phys. B562, 57 (1999)
39. S. Davidson and S.F. King, Phys. Lett. B 445, 191 (1998).
40. Y. Hayato for the Super-Kamiokande Collaboration, talk at the International European Conference on High Energy Physics (HEP 2003), Aachen, Germany, 2003 [http://eps2003.physik.rwth-aachen.de].
41. A. de Gouvêa, A. Friedland, and H. Murayama, Phys. Lett. B 490, 125 (2000).
42. P.F. Harrison, D.H. Perkins, and W.G. Scott, Phys. Lett. B 530, 167 (2002)
43. Phys. Lett. BP.F. Harrison and W.G. Scott, 535, 163 (2002).
44. F. Vissani, hep-ph/9708483
45. V. Barger, S. Pakvasa, T. Weiler, and K. Whisnant, Phys. Lett. B 437, 107 (1998)
46. A. Baltz, A.S. Goldhaber, and M. Goldhaber, Phys. Rev. Lett. 81, 5730 (1998)
47. G. Altarelli and F. Feruglio, Phys. Lett. B 439, 112 (1998)
48. Phys. Lett. BM. Jezabek and Y. Sumino, 440, 327 (1998).
49. E. Ma and G. Rajasekaran, Phys. Rev. D 64, 113012 (2001)
50. E. Ma, Mod. Phys. Lett. A 17, 2361 (2002)
51. K. Babu, E. Ma, and J.W.F. Valle, Phys. Lett. B 552, 207 (2003).
52. G. Tzanakos, talk at the 5th International Workshop on Neutrino Factories and Superbeams, New York, 2003, http://www.cap.bnl.gov/nufact03/agenda.xhtml.; W.C. Louis, http://www.cap.bnl.gov/nufact03/agenda.xhtml
53. R. Bernstein, talk at the 5th International Workshop on Neutrino Factories and Superbeams, New York, 5–11 June 2003, http://www.cap.bnl.gov/nufact03/agenda.xhtml
54. T. Tabarelli de Fatis, Nucl. Phys. B, Proc. Suppl. 118, 118 (2003).
55. O.L.G. Peres and A.Yu. Smirnov, Nucl. Phys. B680, 479 (2004).
56. See, for example, C. Albright, hep-ex/0008064
57. M. Apollonio, hep-ph/0210192.
58. W. Grimus and L. Lavoura, J. High Energy Phys. 07, 045 (2001).
59. G. Altarelli, F. Feruglio, and I. Masina, J. High Energy Phys. 01, 035 (2003).
60. P.H. Frampton, S.T. Petcov, and W. Rodejohann, hep-ph/0401206.