Lepton flavor violation and neutrino mixings in a 3×2 seesaw model

Physical Review D

Volumn 68, Issue 5, 2003, Pages

  Dutta, Bhaskar ^a   Mohapatra, R N ^b  

^a UNIVERSITY OF REGINA   (Canada)

^b Bldg 142   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ANISOTROPY; ARTICLE; ELEMENTARY PARTICLE; ENERGY; LEPTON; MASS; MATHEMATICAL ANALYSIS; MODEL; NEUTRINO; THEORY;

EID: 0142213562     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.68.056006     Document Type: Article

References (98)

1. For recent reviews, see S. Bilenky, C. Giunti, J. Grifols, and E. Masso, Phys. Rep. 379, 64 (2003);
2. S. Pakvasa and J.W.F. Valle, hep-ph/0301061.
3. R. Kuchimanchi and R.N. Mohapatra, Phys. Rev. D 66, 051301(R) (2002);
4. Phys. Lett. B 552, 198 (2003).
5. D.S. Shaw and R.R. Volkas, Phys. Rev. D 47, 241 (1993);
6. R. Barbieri, L. Hall, and A. Romanino, Phys. Lett. B 401, 47 (1999);
7. K.S. Babu and R.N. Mohapatra, Phys. Rev. Lett. 83, 2522 (1999);
8. T. Blazek, S. Raby, and K. Tobe, Phys. Rev. D 62, 055001 (2000);
9. S. Raby, Phys. Lett. B 564, 119 (2003);
10. N. Maekawa, Phys. Lett. B ibid. 561, 273 (2003).
11. M. Gell-Mann, P. Rammond, and R. Slansky, in Supergravity, edited by D. Freedman et al. (North-Holland, Amsterdam, 1980);
12. T. Yanagida (unpublished);
13. R.N. Mohapatra and G. Senjanović, Phys. Rev. Lett. 44, 912 (1980);
14. S.L. Glashow (unpublished).
15. R. Barbieri, L. Hall, D. Smith, A. Strumia, and N. Weiner, J. High Energy Phys. 12, 017 (1998);
16. A. Joshipura and S. Rindani, Eur. Phys. J. C 14, 85 (2000);
17. R.N. Mohapatra, A. Perez-Lorenzana, and C.A. de S. Pires, Phys. Lett. B 474, 355 (2000);
18. T. Kitabayashi and M. Yasue, Phys. Rev. D 63, 095002 (2001);
19. Phys. Lett. B 508, 85 (2001);
20. Phys. Lett. B 524, 308 (2002);
21. L. Lavoura, Phys. Rev. D 62, 093011 (2000);
22. W. Grimus and L. Lavoura, Phys. Rev. D ibid. 62, 093012 (2000);
23. J. High Energy Phys. 09, 007 (2000);
24. J. High Energy Phys. 07, 045 (2001);
25. R.N. Mohapatra, Phys. Rev. D 64, 091301 (R) (2001);
26. K.S. Babu and R.N. Mohapatra, Phys. Lett. B 532, 77 (2002);
27. H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Lett. B ibid. 542, 116 (2002);
28. Duane A. Dicus, Hong-Jian He, and John N. Ng, Phys. Lett. B ibid. 536, 83 (2002);
29. Q. Shafi and Z. Tavart-kiladze, Phys. Lett. B ibid. 482, 1451 (2000);
30. τ symmetry were discussed in S. Petcov, Phys. Lett. 110B, 245 (1982).
31. F. Borzumati and A. Masiero, Phys. Rev. Lett. 57, 961 (1986);
32. L. Hall, V. Kostelecky, and S. Raby, Nucl. Phys. B267, 415 (1986).
33. J. Hisano, T. Moroi, K. Tobe, M. Yamaguchi, and T. Yanagida, Phys. Lett. B 357, 579 (1995);
34. J. Hisano, T. Moroi, K. Tobe, and M. Yamaguchi, Phys. Rev. D 53, 2442 (1996).
35. S.F. King and M. Oliveira, Phys. Rev. D 60, 035003 (1999);
36. J. Hisano and D. Nomura, Phys. Rev. D ibid. 59, 116005 (1999);
37. K.S. Babu, B. Dutta, and R.N. Mohapatra, Phys. Lett. B 458, 93 (1999);
38. W. Buchmuller, D. Delepine, and F. Vissani, Phys. Lett. B ibid. 459, 171 (1999);
39. J. Ellis, M. Gomez, G. Leontaris, S. Lola, and D. Na nopoulos, Eur. Phys. J. C 14, 319 (2000);
40. T. Blazek and S. King, Phys. Lett. B 518, 109 (2001);
41. S. Lavgnac, I. Masina, and C. Savoy, Phys. Lett. B ibid. 520, 269 (2001);
42. Nucl. Phys. B633, 139 (2002);
43. J. Casas and A. Ibarra, Nucl. Phys. ibid. B618, 171 (2001);
44. R. Gonzalez Felipe and F. Joaquim, J. High Energy Phys. 09, 015 (2001);
45. J. Sato, K. Tobe, and T. Yanagida, Phys. Lett. B 498, 189 (2001);
46. X.J. Bi, Y.B. Dai, and X.Y. Qi, Phys. Rev. D 63, 096008 (2001);
47. X.J. Bi, Y.B. Dai, and X.Y. Qi, Phys. Rev. D 66, 076006 (2002);
48. G. Cvetic, C. Dib, C.S. Kim, and J.D. Kim, Phys. Rev. D ibid. 66, 034008 (2002);
49. J. Ellis, J. Hisano, S. Lola, and M. Raidal, Nucl. Phys. B621, 208 (2002);
50. A. Kageyama, S. Kaneko, N. Shimoyama, and M. Tanimoto, Phys. Lett. B 527, 206 (2002);
51. D. Chang, A. Masiero, and H. Murayama, Phys. Rev. D 67, 075013 (2003);
52. J. Ellis, J. Hisano, M. Raidal, and Y. Shimizu, Phys. Rev. D ibid. 66, 115013 (2002);
53. F. Deppisch, H. Pas, A. Redelbach, R. Ruckl, and Y. Shimizu, Eur. Phys. J. 128, 365 (2003);
54. K. Babu and C. Kolda, Phys. Rev. Lett. 89, 241802 (2002);
55. A. Rossi, Phys. Rev. D 66, 075003 (2002);
56. I. Masina and C. Savoy, hep-ph/0211283;
57. A. Masiero, S. Vempati, and O. Vives, Nucl. Phys. B649, 189 (2003);
58. M. Raidal and A. Strumia, Phys. Lett. B 553, 72 (2003);
59. T. Fukuyama, T. Kikuchi, and N. Okada, hep-ph/0304190;
60. S. Kaneko, M. Katsumata, and M. Tanimoto, hep-ph/0305014.
61. K.S. Babu, B. Dutta, and R.N. Mohapatra, Phys. Rev. D 67, 076006 (2003).
62. See meg.web.psi.ch/docs/progress/jun2002/report.ps
63. C.L. Bennett et al., astro-ph/0302207;
64. D.N. Spergel et al., astro-ph/0302209.
65. A. Chamsheddine, R. Arnowitt, and P. Nath, N= 1 Supergravity (World Scientific, Singapore, 1984);
66. R. Barbieri, S. Farrara, and C. Savoy, Phys. Lett. 119B, 343 (1982);
67. L. Hall, J. Lykken, and S. Weinberg, Phys. Rev. D 27, 2359 (1983).
68. G. Kribs, hep-ph/0304256.
69. E. Witten, Phys. Lett. 117B, 324 (1982).
70. S.F. King, Nucl. Phys. B576, 85 (2000);
71. S.F. King and N.N Singh, Nucl. Phys. ibid. B596, 81 (2001);
72. Grimus and Lavoura [5].
73. For application of the 3 × 2 seesaw to leptogenesis, see P. Frampton, S.L. Glashow, and T. Yanagida, Phys. Lett. B 548, 119 (2002);
74. T. Endoh, S. Kaneko, S. Kang, T. Morozumi, and M. Tanimoto, Phys. Rev. Lett. 89, 231601 (2002).
75. G. Fogli, G. Lettera, E. Lisi, A. Marrone, A. Palazzo, and A. Rotunno, Phys. Rev. D 66, 093008 (2002).
76. P. Igo-Kemenes (unpublished).
77. M. Alam et al., Phys. Rev. Lett. 74, 2885 (1995).
78. J. Ellis, T. Falk, and K. Olive, Phys. Lett. B 444, 367 (1998);
79. J. Ellis, T. Falk, K. Olive, and M. Srednicki, Astropart. Phys. 13, 181 (2000);
80. R. Arnowitt, B. Dutta, and Y. Santoso, hep-ph/0010244;
81. Nucl. Phys. B606, 59 (2001);
82. J. Ellis, T. Falk, G. Ganis, K. Olive, and M. Srednicki, Phys. Lett. B 510, 236 (2001);
83. J. Ellis, T. Falk, G. Ganis, K. Olive, and M. Srednicki, Phys. Lett. B 510, 413(E) (2001);
84. M. Gomez and J. Vergados, Phys. Lett. B ibid. 512, 252 (2001);
85. M. Gomez, G. Lazarides, and C. Pallis, Phys. Rev. D 61, 123512 (2000);
86. Phys. Lett. B 487, 313 (2000).
87. L. Ibanez and C. Lopez, Nucl. Phys. B233, 511 (1984).
88. J. Ellis, K. Olive, Y. Santoso, and V. Spanos, Phys. Lett. B 565, 176 (2003);
89. H. Baer and C. Balasz, hep-ph/0303114;
90. R. Ar nowitt, B. Dutta, T. Kamon, and V. Khotilovich (unpublished).
91. R. Arnowitt, B. Dutta, B. Hu, and Y. Santoso, Phys. Lett. B 505, 177 (2001).
92. g - 2 Collaboration, F.E. Gray, hep-ex/0305043.
93. M. Davier, S. Eidelman, A. Hocker, and Z. Zhang, Eur. Phys. J. C 27, 497 (2003).
94. K. Hagiwara, A. Martin, D. Nomura, and T. Teubner, Phys. Lett. B 557, 69 (2003).
95. A. Nyffeler, hep-ph/0305135.
96. R. Arnowitt and B. Dutta, hep-ph/0211417.
97. R. Arnowitt, B. Dutta, T. Kamon, and M. Tanaka, Phys. Lett. B 538, 121 (2002).
98. Amowitt, Dutta, and Santoso [20].