Resonant leptogenesis in a predictive SO(10) grand unified model

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 70, Issue 3, 2004, Pages

  Albright, Carl H ^a,b   Barr, S M ^c  

^a NORTHERN ILLINOIS UNIVERSITY   (United States)

^b FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

^c UNIVERSITY OF DELAWARE   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; BARYON; LEPTON; MASS; MODEL; NEUTRINO; PREDICTION; SOLAR ENERGY;

EID: 19544362508     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.70.033013     Document Type: Article

References (52)

1. A sampling of some still successful grand unified models with their early references include the following: C.H. Albright and S.M. Barr, Phys. Rev. D 58, 013002 (1998); K.S. Babu, J.C. Pati, and F. Wilczek, Nucl. Phys. B566, 33 (2000); Mu-C. Chen and K.T. Mahanthappa, Phys. Rev. D 62, 113007 (2000); R. Kitano and Y. Mimura, ibid. 63, 016008 (2001); M. Bando and N. Maekawa, Prog. Theor. Phys. 106, 1255 (2001); T. Fukuyama and N. Okada, J. High Energy Phys. 11, 011 (2002); M. Bando and M. Obara, Prog. Theor. Phys. 109, 995 (2003); S.F. King and G.G. Ross, Phys. Lett. B 574, 239 (2003); H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Rev. D 68, 115008 (2003); M. Bando, S. Kaneko, M. Obara, and M. Tanimoto, Phys. Lett. B 580, 229 (2004); C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic, and F. Vissani, ibid. 588, 196 (2004).
2. A sampling of some still successful grand unified models with their early references include the following: C.H. Albright and S.M. Barr, Phys. Rev. D 58, 013002 (1998); K.S. Babu, J.C. Pati, and F. Wilczek, Nucl. Phys. B566, 33 (2000); Mu-C. Chen and K.T. Mahanthappa, Phys. Rev. D 62, 113007 (2000); R. Kitano and Y. Mimura, ibid. 63, 016008 (2001); M. Bando and N. Maekawa, Prog. Theor. Phys. 106, 1255 (2001); T. Fukuyama and N. Okada, J. High Energy Phys. 11, 011 (2002); M. Bando and M. Obara, Prog. Theor. Phys. 109, 995 (2003); S.F. King and G.G. Ross, Phys. Lett. B 574, 239 (2003); H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Rev. D 68, 115008 (2003); M. Bando, S. Kaneko, M. Obara, and M. Tanimoto, Phys. Lett. B 580, 229 (2004); C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic, and F. Vissani, ibid. 588, 196 (2004).
3. A sampling of some still successful grand unified models with their early references include the following: C.H. Albright and S.M. Barr, Phys. Rev. D 58, 013002 (1998); K.S. Babu, J.C. Pati, and F. Wilczek, Nucl. Phys. B566, 33 (2000); Mu-C. Chen and K.T. Mahanthappa, Phys. Rev. D 62, 113007 (2000); R. Kitano and Y. Mimura, ibid. 63, 016008 (2001); M. Bando and N. Maekawa, Prog. Theor. Phys. 106, 1255 (2001); T. Fukuyama and N. Okada, J. High Energy Phys. 11, 011 (2002); M. Bando and M. Obara, Prog. Theor. Phys. 109, 995 (2003); S.F. King and G.G. Ross, Phys. Lett. B 574, 239 (2003); H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Rev. D 68, 115008 (2003); M. Bando, S. Kaneko, M. Obara, and M. Tanimoto, Phys. Lett. B 580, 229 (2004); C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic, and F. Vissani, ibid. 588, 196 (2004).
4. A sampling of some still successful grand unified models with their early references include the following: C.H. Albright and S.M. Barr, Phys. Rev. D 58, 013002 (1998); K.S. Babu, J.C. Pati, and F. Wilczek, Nucl. Phys. B566, 33 (2000); Mu-C. Chen and K.T. Mahanthappa, Phys. Rev. D 62, 113007 (2000); R. Kitano and Y. Mimura, ibid. 63, 016008 (2001); M. Bando and N. Maekawa, Prog. Theor. Phys. 106, 1255 (2001); T. Fukuyama and N. Okada, J. High Energy Phys. 11, 011 (2002); M. Bando and M. Obara, Prog. Theor. Phys. 109, 995 (2003); S.F. King and G.G. Ross, Phys. Lett. B 574, 239 (2003); H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Rev. D 68, 115008 (2003); M. Bando, S. Kaneko, M. Obara, and M. Tanimoto, Phys. Lett. B 580, 229 (2004); C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic, and F. Vissani, ibid. 588, 196 (2004).
5. A sampling of some still successful grand unified models with their early references include the following: C.H. Albright and S.M. Barr, Phys. Rev. D 58, 013002 (1998); K.S. Babu, J.C. Pati, and F. Wilczek, Nucl. Phys. B566, 33 (2000); Mu-C. Chen and K.T. Mahanthappa, Phys. Rev. D 62, 113007 (2000); R. Kitano and Y. Mimura, ibid. 63, 016008 (2001); M. Bando and N. Maekawa, Prog. Theor. Phys. 106, 1255 (2001); T. Fukuyama and N. Okada, J. High Energy Phys. 11, 011 (2002); M. Bando and M. Obara, Prog. Theor. Phys. 109, 995 (2003); S.F. King and G.G. Ross, Phys. Lett. B 574, 239 (2003); H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Rev. D 68, 115008 (2003); M. Bando, S. Kaneko, M. Obara, and M. Tanimoto, Phys. Lett. B 580, 229 (2004); C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic, and F. Vissani, ibid. 588, 196 (2004).
6. A sampling of some still successful grand unified models with their early references include the following: C.H. Albright and S.M. Barr, Phys. Rev. D 58, 013002 (1998); K.S. Babu, J.C. Pati, and F. Wilczek, Nucl. Phys. B566, 33 (2000); Mu-C. Chen and K.T. Mahanthappa, Phys. Rev. D 62, 113007 (2000); R. Kitano and Y. Mimura, ibid. 63, 016008 (2001); M. Bando and N. Maekawa, Prog. Theor. Phys. 106, 1255 (2001); T. Fukuyama and N. Okada, J. High Energy Phys. 11, 011 (2002); M. Bando and M. Obara, Prog. Theor. Phys. 109, 995 (2003); S.F. King and G.G. Ross, Phys. Lett. B 574, 239 (2003); H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Rev. D 68, 115008 (2003); M. Bando, S. Kaneko, M. Obara, and M. Tanimoto, Phys. Lett. B 580, 229 (2004); C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic, and F. Vissani, ibid. 588, 196 (2004).
7. A sampling of some still successful grand unified models with their early references include the following: C.H. Albright and S.M. Barr, Phys. Rev. D 58, 013002 (1998); K.S. Babu, J.C. Pati, and F. Wilczek, Nucl. Phys. B566, 33 (2000); Mu-C. Chen and K.T. Mahanthappa, Phys. Rev. D 62, 113007 (2000); R. Kitano and Y. Mimura, ibid. 63, 016008 (2001); M. Bando and N. Maekawa, Prog. Theor. Phys. 106, 1255 (2001); T. Fukuyama and N. Okada, J. High Energy Phys. 11, 011 (2002); M. Bando and M. Obara, Prog. Theor. Phys. 109, 995 (2003); S.F. King and G.G. Ross, Phys. Lett. B 574, 239 (2003); H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Rev. D 68, 115008 (2003); M. Bando, S. Kaneko, M. Obara, and M. Tanimoto, Phys. Lett. B 580, 229 (2004); C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic, and F. Vissani, ibid. 588, 196 (2004).
8. A sampling of some still successful grand unified models with their early references include the following: C.H. Albright and S.M. Barr, Phys. Rev. D 58, 013002 (1998); K.S. Babu, J.C. Pati, and F. Wilczek, Nucl. Phys. B566, 33 (2000); Mu-C. Chen and K.T. Mahanthappa, Phys. Rev. D 62, 113007 (2000); R. Kitano and Y. Mimura, ibid. 63, 016008 (2001); M. Bando and N. Maekawa, Prog. Theor. Phys. 106, 1255 (2001); T. Fukuyama and N. Okada, J. High Energy Phys. 11, 011 (2002); M. Bando and M. Obara, Prog. Theor. Phys. 109, 995 (2003); S.F. King and G.G. Ross, Phys. Lett. B 574, 239 (2003); H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Rev. D 68, 115008 (2003); M. Bando, S. Kaneko, M. Obara, and M. Tanimoto, Phys. Lett. B 580, 229 (2004); C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic, and F. Vissani, ibid. 588, 196 (2004).
9. A sampling of some still successful grand unified models with their early references include the following: C.H. Albright and S.M. Barr, Phys. Rev. D 58, 013002 (1998); K.S. Babu, J.C. Pati, and F. Wilczek, Nucl. Phys. B566, 33 (2000); Mu-C. Chen and K.T. Mahanthappa, Phys. Rev. D 62, 113007 (2000); R. Kitano and Y. Mimura, ibid. 63, 016008 (2001); M. Bando and N. Maekawa, Prog. Theor. Phys. 106, 1255 (2001); T. Fukuyama and N. Okada, J. High Energy Phys. 11, 011 (2002); M. Bando and M. Obara, Prog. Theor. Phys. 109, 995 (2003); S.F. King and G.G. Ross, Phys. Lett. B 574, 239 (2003); H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Rev. D 68, 115008 (2003); M. Bando, S. Kaneko, M. Obara, and M. Tanimoto, Phys. Lett. B 580, 229 (2004); C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic, and F. Vissani, ibid. 588, 196 (2004).
10. A sampling of some still successful grand unified models with their early references include the following: C.H. Albright and S.M. Barr, Phys. Rev. D 58, 013002 (1998); K.S. Babu, J.C. Pati, and F. Wilczek, Nucl. Phys. B566, 33 (2000); Mu-C. Chen and K.T. Mahanthappa, Phys. Rev. D 62, 113007 (2000); R. Kitano and Y. Mimura, ibid. 63, 016008 (2001); M. Bando and N. Maekawa, Prog. Theor. Phys. 106, 1255 (2001); T. Fukuyama and N. Okada, J. High Energy Phys. 11, 011 (2002); M. Bando and M. Obara, Prog. Theor. Phys. 109, 995 (2003); S.F. King and G.G. Ross, Phys. Lett. B 574, 239 (2003); H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Rev. D 68, 115008 (2003); M. Bando, S. Kaneko, M. Obara, and M. Tanimoto, Phys. Lett. B 580, 229 (2004); C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic, and F. Vissani, ibid. 588, 196 (2004).
11. A sampling of some still successful grand unified models with their early references include the following: C.H. Albright and S.M. Barr, Phys. Rev. D 58, 013002 (1998); K.S. Babu, J.C. Pati, and F. Wilczek, Nucl. Phys. B566, 33 (2000); Mu-C. Chen and K.T. Mahanthappa, Phys. Rev. D 62, 113007 (2000); R. Kitano and Y. Mimura, ibid. 63, 016008 (2001); M. Bando and N. Maekawa, Prog. Theor. Phys. 106, 1255 (2001); T. Fukuyama and N. Okada, J. High Energy Phys. 11, 011 (2002); M. Bando and M. Obara, Prog. Theor. Phys. 109, 995 (2003); S.F. King and G.G. Ross, Phys. Lett. B 574, 239 (2003); H.S. Goh, R.N. Mohapatra, and S.-P. Ng, Phys. Rev. D 68, 115008 (2003); M. Bando, S. Kaneko, M. Obara, and M. Tanimoto, Phys. Lett. B 580, 229 (2004); C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic, and F. Vissani, ibid. 588, 196 (2004).
12. A.D. Sakharov, Pis'ma Zh. Éksp. Teor. Fiz. 5, 32 (1967) [JETP Lett. 5, 24 (1967)].
13. A.D. Sakharov, Pis'ma Zh. Éksp. Teor. Fiz. 5, 32 (1967) [JETP Lett. 5, 24 (1967)].
14. J.A. Harvey and M.S. Turner, Phys. Rev. D 42, 3344 (1990).
15. M. Fukugita and T. Yanagida, Phys. Lett. B 174, 45 (1986).
16. M. Flanz, E.A. Paschos, U. Sarkar, and J. Weiss, Phys. Lett. B 389, 693 (1996); L. Covi and E. Roulet, ibid. 399, 113 (1997).
17. M. Flanz, E.A. Paschos, U. Sarkar, and J. Weiss, Phys. Lett. B 389, 693 (1996); L. Covi and E. Roulet, ibid. 399, 113 (1997).
18. J. Ellis, M. Raidal, and T. Yanagida, Phys. Lett. B 546, 228 (2002); E.Kh. Akhmedov, M. Frigerio, and A.Yu. Smirnov, J. High Energy Phys. 09, 021 (2003).
19. J. Ellis, M. Raidal, and T. Yanagida, Phys. Lett. B 546, 228 (2002); E.Kh. Akhmedov, M. Frigerio, and A.Yu. Smirnov, J. High Energy Phys. 09, 021 (2003).
20. A. Pilaftsis and T.E.J. Underwood, Nucl. Phys. B692, 303 (2004).
21. C.H. Albright, K.S. Babu, and S.M. Barr, Phys. Rev. Lett. 81, 1167 (1998).
22. C.H. Albright and S.M. Barr, Phys. Rev. Lett. 85, 244 (2000); Phys. Rev. D 62, 093008 (2000).
23. C.H. Albright and S.M. Barr, Phys. Rev. Lett. 85, 244 (2000); Phys. Rev. D 62, 093008 (2000).
24. L. Wolfenstein, Phys. Rev. D 17, 2369 (1978); S.P. Mikheyev and A.Yu. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1985)].
25. L. Wolfenstein, Phys. Rev. D 17, 2369 (1978); S.P. Mikheyev and A.Yu. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1985)].
26. L. Wolfenstein, Phys. Rev. D 17, 2369 (1978); S.P. Mikheyev and A.Yu. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1985)].
27. B. Pontecorvo, Zh. Éksp. Teor. Fiz. 33, 549 (1957) [Sov. Phys. JETP 6, 429 (1957)]; 34, 247 (1957) [ibid. 7, 172 (1958)]; Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28, 870 (1962).
28. B. Pontecorvo, Zh. Éksp. Teor. Fiz. 33, 549 (1957) [Sov. Phys. JETP 6, 429 (1957)]; 34, 247 (1957) [ibid. 7, 172 (1958)]; Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28, 870 (1962).
29. B. Pontecorvo, Zh. Éksp. Teor. Fiz. 33, 549 (1957) [Sov. Phys. JETP 6, 429 (1957)]; 34, 247 (1957) [ibid. 7, 172 (1958)]; Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28, 870 (1962).
30. B. Pontecorvo, Zh. Éksp. Teor. Fiz. 33, 549 (1957) [Sov. Phys. JETP 6, 429 (1957)]; 34, 247 (1957) [ibid. 7, 172 (1958)]; Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28, 870 (1962).
31. B. Pontecorvo, Zh. Éksp. Teor. Fiz. 33, 549 (1957) [Sov. Phys. JETP 6, 429 (1957)]; 34, 247 (1957) [ibid. 7, 172 (1958)]; Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28, 870 (1962).
32. S.M. Barr, Phys. Rev. Lett. 92, 101601 (2004).
33. C.H. Albright and S.M. Barr, Phys. Rev. D 69, 073010 (2004).
34. S.M. Barr and S. Raby, Phys. Rev. Lett. 79, 4748 (1997).
35. C.D. Froggatt and H.B. Nielsen, Nucl. Phys. B147, 277 (1979).
36. C.H. Albright and S.M. Barr, Phys. Rev. D 64, 073010 (2001).
37. H. Georgi and C. Jarlskog, Phys. Lett. 86B, 297 (1979).
38. Particle Data Group, K. Hagiwara et al., Phys. Rev. D 66, 010001 (2002).
39. G.L. Fogli, E. Lisi, A. Marrone, and D. Montanino, Phys. Rev. D 67, 093006 (2003); Super-Kamiokande Collaboration, M.B. Smy et al., ibid. 69, 011104(R) (2004).
40. G.L. Fogli, E. Lisi, A. Marrone, and D. Montanino, Phys. Rev. D 67, 093006 (2003); Super-Kamiokande Collaboration, M.B. Smy et al., ibid. 69, 011104(R) (2004).
41. A. Pilaftsis, Phys. Rev. D 56, 5431 (1997).
42. E.W. Kolb and M.S. Turner, The Early Universe (Addison-Wesley, Redwood City, CA, 1990); A. Pilaftsis, Int. J. Mod. Phys. A 14, 1811 (1999); M. Flanz and E.A. Paschos, Phys. Rev. D 58, 113009 (1998).
43. E.W. Kolb and M.S. Turner, The Early Universe (Addison-Wesley, Redwood City, CA, 1990); A. Pilaftsis, Int. J. Mod. Phys. A 14, 1811 (1999); M. Flanz and E.A. Paschos, Phys. Rev. D 58, 113009 (1998).
44. E.W. Kolb and M.S. Turner, The Early Universe (Addison-Wesley, Redwood City, CA, 1990); A. Pilaftsis, Int. J. Mod. Phys. A 14, 1811 (1999); M. Flanz and E.A. Paschos, Phys. Rev. D 58, 113009 (1998).
45. See, e.g., L. Covi, E. Roulet, and F. Vissani, Phys. Lett. B 384, 169 (1996).
46. D.N. Spergel et al., Astrophys. J., Suppl. Ser. 148, 175 (2003).
47. G.F. Giudice, A. Notari, M. Raidal, A. Riotto, and A. Strumia, Nucl. Phys. B685, 89 (2004).
48. M.A. Luty, Phys. Rev. D 45, 455 (1992); W. Buchmüller and T. Yanagida, Phys. Lett. B 302, 240 (1993); H. Murayama and T. Yanagida, ibid. 322, 349 (1994); R. Jeannerot, Phys. Rev. Lett. 77, 3292 (1996).
49. M.A. Luty, Phys. Rev. D 45, 455 (1992); W. Buchmüller and T. Yanagida, Phys. Lett. B 302, 240 (1993); H. Murayama and T. Yanagida, ibid. 322, 349 (1994); R. Jeannerot, Phys. Rev. Lett. 77, 3292 (1996).
50. M.A. Luty, Phys. Rev. D 45, 455 (1992); W. Buchmüller and T. Yanagida, Phys. Lett. B 302, 240 (1993); H. Murayama and T. Yanagida, ibid. 322, 349 (1994); R. Jeannerot, Phys. Rev. Lett. 77, 3292 (1996).
51. M.A. Luty, Phys. Rev. D 45, 455 (1992); W. Buchmüller and T. Yanagida, Phys. Lett. B 302, 240 (1993); H. Murayama and T. Yanagida, ibid. 322, 349 (1994); R. Jeannerot, Phys. Rev. Lett. 77, 3292 (1996).
52. M. Kawasaki, K. Kohri, and T. Moroi, astro-ph/0402490.