Protecting the primordial baryon asymmetry in the SU(2)L triplet Higgs model compatible with KamLAND and WMAP

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 70, Issue 5, 2004, Pages

  Hasegawa, K ^a  

^a KOBE UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

ANISOTROPY; ARTICLE; BARYON; MECHANICAL PROBE; MICROWAVE RADIATION; OSCILLATION; PHYSICAL MODEL; PHYSICS;

EID: 84927778110     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.70.054002     Document Type: Article

References (61)

1. Super-Kamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 81, 1562 (1998); Phys. Rev. Lett. 82, 2644 (1999); Phys. Rev. Lett. 85, 3999 (2000).
2. Super-Kamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 81, 1562 (1998); Phys. Rev. Lett. 82, 2644 (1999); Phys. Rev. Lett. 85, 3999 (2000).
3. Super-Kamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 81, 1562 (1998); Phys. Rev. Lett. 82, 2644 (1999); Phys. Rev. Lett. 85, 3999 (2000).
4. N. Fornengo, M. C. Gonzalez-Garcia, and J. W. F. Valle, Nucl. Phys. B 580, 58 (2000); T. Toshito, hep-ex/0105023 .
5. N. Fornengo, M. C. Gonzalez-Garcia, and J. W. F. Valle, Nucl. Phys. B 580, 58 (2000); T. Toshito, hep-ex/0105023 .
6. M. C. Gonzalez-Garcia, M. Maltoni, C. Pena-Garay, and J. W. F. Valle, Phys. Rev. D 63, 033005 (2001).
7. SNO Collaboration, Q. R. Ahmad et al., Phys. Rev. Lett. 87, 071301 (2001).
8. J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Pene-Garay, J. High Energy Phys.08 (2001) 014; V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Lett. B 537, 179 (2002).
9. J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Pene-Garay, J. High Energy Phys.08 (2001) 014; V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Lett. B 537, 179 (2002).
10. CHOOZ Collaboration, M. Apollonio et al., Phys. Lett. B 420, 397 (1998); Phys. Lett. B 466, 415 (1999).
11. CHOOZ Collaboration, M. Apollonio et al., Phys. Lett. B 420, 397 (1998); Phys. Lett. B 466, 415 (1999).
12. KamLAND Collaboration, K. Eguchi et al., Phys. Rev. Lett. 90, 021802 (2003).
13. J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Pene-Garay, J. High Energy Phys. 02 (2003) 009.
14. M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 67, 093003 (2003).
15. WMAP CollaborationC. L. Bennett et al., Astrophys. J. Suppl. Ser. 148, 1 (2003).
16. WMAP Collaboration, D. N. Spergel et al., Astrophys. J. Suppl. Ser. 148, 175 (2003).
17. S. Hannestad, J. Cosmol. Astropart. Phys. 05 (2003) 004.
18. Ø. Elgarøy and O. Lahav, J. Cosmol. Astropart Phys. 04 (2003) 004.
19. A. Pierce and H. Murayama, Phys. Lett. B 581, 218 (2004).
20. T. Yanagida, in Proceedings of the Workshop on the Unified Theory and Baryon Number in the Universe, Tsukuba, Japan, edited by O. Sawada and A. Sugamoto (KEK Report No. 7918, 1979), p. 95.
21. M. Gell-Mann, P. Rammond, and R. Slansky, in Supergravity, edited by P. van Niewenhuizen and D. Z. Freedman (North-Holland, Amsterdam, 1979), p. 315.
22. R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980).
23. J. Schechter and J. W. F. Valle, Phys. Rev. D 22, 2227 (1980).
24. G. Lazarides, Q. Shafi, and C. Wetterich, Nucl. Phys. B 181, 287 (1981).
25. A. Zee, Phys. Lett. B 93, 389 (1980).
26. E. Ma, M. Raidal, and U. Sarkar, Phys. Rev. Lett. 85, 3769 (2000).
27. E. Ma, M. Raidal, and U. Sarkar, Nucl. Phys. B 615, 313 (2001).
28. W. Grimus, hep-ph/0307149.
29. J. Erler and P. Langacker, Phys. Lett. B 456, 68 (1999).
30. E. J. Chun, K. Y. Lee, and S. C. Park, Phys. Lett. B 566, 142 (2003).
31. M. Kakizaki, Y. Ogura, and F. Shima, Phys. Lett. B 566, 210 (2003).
32. M. Yoshimura, Phys. Rev. Lett. 41, 281 (1978).
33. S. M. Barr, G. Segre, and H. A. Weldon, Phys. Rev. D 20, 2494 (1979).
34. V. A. Kuzmin, V. A. Rubakov, and M. E. Shaposhnikov, Phys. Lett. B 155, 36 (1985).
35. A. G. Cohen, D. B. Kaplan, and A. E. Nelson, Annu. Rev. Nucl. Part. Sci. 43, 27 (1993).
36. M. Fukugita and T. Yanagida, Phys. Lett. B 174, 45 (1986).
37. I. Affleck and M. Dine, Nucl. Phys. B 249, 361 (1985).
38. G. 't Hooft, Phys. Rev. Lett. 37, 8 (1976).
39. N. S. Manton, Phys. Rev. D 28, 2019 (1983).
40. F. R. Klinkharmmar and N. S. Manton, Phys. Rev. D 30, 2212 (1984).
41. P. Arnold, D. Son, and L. G. Yaffe, Phys. Rev. D 55, 6264 (1997).
42. D. Bodeker, G. D. Moore, and K. Rummukainen, Phys. Rev. D 61, 056003 (2000).
43. A. D. Sakharov, JETP Lett. 5, 24 (1967).
44. E. Ma and U. Sarkar, Phys. Rev. Lett. 80, 5716 (1998).
45. G. Lazarides and Q. Shafi, Phys. Rev. D 58, 071702 (1998).
46. G. Lazarides, Phys. Lett. B 452, 227 (1999).
47. J. N. Fry, K. A. Olive, and M. S. Turner, Phys. Rev. D 22, 2953 (1980).
48. J. N. Fry, K. A. Olive, and M. S. Turner, Phys. Rev. D 22, 2977 (1980).
49. M. Fukugita and T. Yanagida, Phys. Rev. D 42, 1285 (1990).
50. J. A. Harvey and M. S. Turner, Phys. Rev. D 42, 3344 (1990).
51. A. E. Nelson and S. M. Barr, Phys. Lett. B 246, 141 (1990).
52. W. Buchmuller and T. Yanagida, Phys. Lett. B 302, 240 (1993).
53. W. Fischer, G. F. Giudice, R. G. Leigh, and S. Paban, Phys. Lett. B 258, 45 (1990).
54. B. A. Campbell, S. Davidson, J. Ellis, and K. A. Olive, Phys. Lett. B 297, 118 (1992).
55. J. M. Cline, K. Kainulainen, and K. A. Olive, Phys. Rev. Lett. 71, 2372 (1993); Phys. Rev. D 49, 6394 (1994).
56. J. M. Cline, K. Kainulainen, and K. A. Olive, Phys. Rev. Lett. 71, 2372 (1993); Phys. Rev. D 49, 6394 (1994).
57. H. Dreiner and G. G. Ross, Nucl. Phys. B 410, 188 (1993).
58. K. Hasegawa, Phys. Rev. D 69, 013002 (2004).
59. N. Haba, K. Hamaguchi, and T. Suzuki, Phys. Lett. B 519, 243 (2001).
60. K. Hasegawa, C. S. Lim, and K. Ogure, Phys. Rev. D 68, 053006 (2003).
61. i(i = 1-4) are small enough to neglect δV. It is shown in [22] that even if we add δV, the same mass matrix of the neutrinos is obtained.