Two-loop radiative neutrino mechanism in an SU(3)LXU(1)N gauge model

Physical Review D

Volumn 63, Issue 9, 2001, Pages

  Kitabayashi, Teruyuki ^a   Yasuè, Masaki ^b  

^a Mitsubishi Electric System and Service Engineering Co Ltd   (Japan)

^b TOKAI UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; CALCULATION; MEASUREMENT; NEUTRON DOSIMETRY; OSCILLATION;

EID: 0034904497     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.63.095006     Document Type: Article

References (91)

1. SuperKamiokande collaboration, Y. Fukuda et al., Phys. Rev. Lett. 81, 1562 (1998);
2. Phys. Lett. B 433, 9 (1998);
3. 436, 33 (1998); see also K. Scholberg, hep-ex/9905016.
4. Y. Takeuchi, Talk given at the 30th International Conference on High Energy Physics (ICHEP2000), Osaka, Japan.
5. See, for example, J. N. Bahcall, P. I. Krastev, and A. Yu. Smirnov, Phys. Rev. D 58, 096016 (1998);
6. 60,093001 (1999); J. N. Bahcall, hep-ph/0002018;
7. M. C. Gonzalez-Garcia, P. C. de Holanda, C. Pena-Garay, and J. W. F. Valle, Nucl. Phys. B573, 3 (2000).
8. Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28, 870 (1962);
9. see also B. Pontecorvo, Zh. Éksp. Teor. Fiz. 34, 247 (1958)
10. [Sov. Phys. JETP 7, 172 (1958)];
11. 53, 1717 (1967)
12. [26, 984 (1968)];
13. V. Gribov and B. Pontecorvo, Phys. Lett. 28B, 493 (1969).
14. T. Yanagida, in Proceedings of the Workshop on Unified Theories and Baryon Number in the Universe, edited by O. Sawada and A. Sugamoto (KEK Report No.79-18, Tsukuba, 1979), p. 95;
15. Prog. Theor. Phys. 64, 1103 (1980);
16. M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity edited by P. van Nieuwenhuizen and D. Z. Freedmann (North-Holland, Amsterdam 1979), p. 315
17. R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980).
18. A. Zee, Phys. Lett. 93B, 389 (1980);
19. 161B, 141 (1985);
20. L. Wolfenstein, Nucl. Phys. B175, 93 (1980).
21. A. Zee, Nucl. Phys. B264, 99 (1986);
22. K. S. Babu, Phys. Lett. B 203, 132 (1988);
23. D. Chang, W-Y. Keung, and P. B. Pal, Phys. Rev. Lett. 61, 2420 (1988);
24. J. T. Peltoniemi, A. Yu. Smirnov, and J. W. F. Valle, Phys. Lett. B 286, 321 (1992).
25. For a model with VR , see D. Choudhury, R. Gandhi, J. A. Gracey, and B. Mukhopadhyaya, Phys. Rev. D 50, 3468 (1994).
26. For example, S. T. Petcov, Phys. Lett. 115B, 401 (1982);
27. K. S. Babu and V. S. Mathur, Phys. Lett. B 196, 218 (1987);
28. J. Liu, ibid. 216, 367 (1989);
29. D. Chang and W.-Y. Keung, Phys. Rev. D 39, 1386 (1989);
30. W. Grimus and H. Neufeld, Phys. Lett. B 237, 521 (1990);
31. B. K. Pal, Phys. Rev. D 44, 2261 (1991);
32. W. Grimus and G. Nardulli, Phys. Lett. B 271, 161 (1991);
33. A. Yu. Smirnov and Z. Tao, Nucl. Phys. B426, 415 (1994).
34. A. Yu. Smirnov and M. Tanimoto, Phys. Rev. D 55, 1665 (1997);
35. N. Gaur, A. Ghosa!, E. Ma, and P. Roy, ibid. 58, 071301 (1998);
36. C. Jarlskog, M. Matsuda, S. Skadhaùge, and M. Tanimoto, Phys. Lett. B 449, 240 (1999);
37. Y. Okamoto and M. Yasuè, Prog. Theor. Phys. 101, 1119 (1999);
38. P. H. Frampton and S. L. Glashow, Phys. Lett. B 461, 95 (1999);
39. G. C. McLaughlin and J. N. Ng, ibid. 455, 224 (1999);
40. A. S. Joshipura and S. D. Rindani, Phys. Lett. B 464, 239 (1999); J. E. Kim and J. S. Lee, hep-ph/9907452;
41. N. Haba, M. Matsuda, and M. Tanimoto, Phys. Lett. B 478, 351 (2000);
42. C-K. Chua, X-G. He, and W-Y. P. Hwang, ibid. 479, 224 (2000);
43. D. Chang and A. Zee, Phys. Rev. D 61, 071303 (2000);
44. K. Cheung and O. C. W. Kong, ibid. 61, 113012 (2000).
45. D. V. Ahluwalia, Mod. Phys. Lett. A 13, 2249 (1998);
46. V. Barger, P. Pakvasa, T. J. Weiler, and K. Whisnant, Phys. Lett. B 437, 107 (1998);
47. A. Baltz, A. S. Goldhaber, and M. Goldhaber, Phys. Rev. Lett. 81, 5730 (1998);
48. M. Jezabek and Y. Sumino, Phys. Lett. B 440, 327 (1998);
49. R. N. Mohapatra and S. Nussinov, ibid. 441, 299 (1998);
50. Y. Nomura and T. Yanagida, Phys. Rev. D 59, 017303 (1999);
51. Q. Shafi and Z. Tavartkiladze, Phys. Lett. B 451, 129 (1999);
52. 482, 145 (2000);
53. I. Starcu and D. V. Ahluwalia, ibid. 460, 431 (1999);
54. H. Georgi and S. L. Glashow, Phys. Rev. D 61,097301 (2000);
55. R. N. Mohapatra, A. Pérez-Lorenzana, and C. A. de S. Pires, Phys. Lett. B 474, 355 (2000).
56. H. Fritzsch and Z. Xing, Phys. Lett. B 372, 265 (1996);
57. M. Fukugita, M. Tanimoto, and T. Yanagida, Phys. Rev. D 57, 4429 (1998);
58. M. Tanimoto, ibid. 59, 017304 (1999).
59. R. Barbieri, L. J. Hall, D. Smith, A. Strumia, and N. Weiner, J. High Energy Phys. 12, 017 (1998);
60. see also, S. T. Petcov, Phys. Lett. HOB, 245 (1982);
61. C. N. Leung and S. T. Petcov, ibid. 125B, 461 (1983); Zee [7].
62. F. Pisano and V. Pleitez, Phys. Rev. D 46, 410 (1992);
63. P. H. Frampton, Phys. Rev. Lett. 69, 2889 (1992);
64. D. Ng, Phys. Rev. D 49, 4805 (1994);
65. see also M. Singer, J. W. F. Valle, and J. Schechter, ibid. 22, 738 (1980).
66. Y. Okamoto and M. Yasuè, Phys. Lett. B 466, 267 (1999).
67. R. Barbieri and R. N. Mohapatra, Phys. Lett. B 218, 225 (1989);
68. J. Liu, ibid. 225, 148 (1989).
69. V. Pleitez and M, D. Tonasse, Phys. Rev. D 48, 5274 (1993);
70. F. Pisano, V. Pleitez, and M. D. Tonasse, hep-ph/9310230 v2;
71. P. H. Frampton, P. I. Krastev, and J. T. Liu, Mod. Phys. Lett. A 9, 761 (1994); M. B. Tully and G. C. Joshi, hep-ph/9810282;
72. see also J. W. F. Valle and M. Singer, Phys. Rev. D 28, 540 (1983).
73. For mechanisms of well-suppressed tree-level neutrino masses, see M. B. Tully and G. C. Joshi, hep-ph/0011172; J. C. Montera, C. A. Pires, and V. Pleitez, hep-ph/0011296.
74. For two-loop radiative models with the L' conservation, see L. Lavoura, Phys. Rev. D 62, 093011 (2000);
75. T. Kitabayashi and M. Yasue, Phys. Lett. B 490, 236 (2000).
76. For a model with (°, ), see T. Kitabayashi and M. Yasuè, hep-ph/0010087.
77. Singer, Valle, and Schechter [13]; F.-z. Chen, Phys. Lett. B 442, 223 (1998);
78. V. Pleitez and M. D. Tonasse, ibid. 430, 174 (1998).
79. Joshipura and Rindani [9]; Chang and Zee [9].
80. The simple extension would be to use !RlKk++ (as in Ref. [7]) and p' + tp'+tA'+ + . However, it is impossible to form an SU(3)XU(l)N singlet that contains p'+p' +.
81. Barbieri and Mohapatra [15].
82. S. L. Glashow and S. Weinberg, Phys. Rev. D 15, 1958 (1977);
83. H. Georgi and A. Pais, ibid. 19, 2746 (1979).
84. J. C. Montera, F. Pisano, and V. Pleitez, Phys. Rev. D 47, 2918 (1993);
85. M. Özer, ibid. 54, 4561 (1996).
86. For recent analysis, see N. Fomengo, M. C. Gonzalez-Garcia, and J. W. F. Valle, J. High Energy Phys. 7, 006 (2000);
87. Nucl. Phys. B580, 58 (2000).
88. The announcement that the VO solution seems to be disfavored at the 95% confidence level has been made by the SuperKamiokande Collaboration [2], However, it is stressed that this statement is not conclusive [28] and that theorists keep watching the VO solution to solar neutrino problem. See also C. E. C. Lima, H. M. Portella, and L. C. S. de Oliveira, hep-ph/0010038 v2;
89. R. Barbieri and A. Strumia, J. High Energy Phys. 12, 016 (2000).
90. Y. Takeuchi, a talk at Post Summer Institute 2000 on Neutrino Physics, 2000, Fuji-Yoshida, Japan.
91. Kitabayashi and Yasuè [18].