Highest-energy cosmic rays from fermi-degenerate relic neutrinos consistent with super-kamiokande results

Physical Review Letters

Volumn 82, Issue 26, 1999, Pages 5202-5204

  Gelmini, Graciela ^a   Kusenko, Alexander ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

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Indexed keywords

EID: 4243319124     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.82.5202     Document Type: Article

References (58)

1. A. D. Dolgov and D. P. Kirilova, J. Mosc. Phys. Soc., 1, 217 (1991);
2. A. D. Dolgov, Phys. Rep., 222, 309 (1992).
3. A. Casas, W. Y. Cheng, and G. Gelmini, Nucl. Phys., B538, 297 (1999).
4. J. A. Harvey and E. W. Kolb, Phys. Rev. D, 24, 2090 (1981);
5. J. Liu and G. Segrè, Phys. Rev. D, 48, 4609 (1993);
6. B. Bajc, A. Riotto, and G. Senjanović, Phys. Rev. Lett., 81, 1355 (1998).
7. A. Linde, Phys. Rev. D, 14, 3345 (1976);
8. P. Langacker, G. Segrè, and S. Soni, Phys. Rev. D, 26, 3425 (1982);
9. J. Liu and G. Segrè, Phys. Lett. B, 338, 259 (1994).
10. P. Pal and K. Kar, Phys. Lett. B, 451, 136 (1999).
11. I. Affleck and M. Dine, Nucl. Phys., B249, 361 (1985).
12. R. Foot, M. J. Thompson, and R. R. Volkas, Phys. Rev. D, 53, 5349 (1996);
13. X. Shi, Phys. Rev. D, 54, 2753 (1996).
14. K. Greisen, Phys. Rev. Lett., 16, 748 (1966);
15. G. T. Zatsepin and V. A. Kuzmin, Pis'ma Zh. Eksp. Teor. Fiz., 4, 114 (1966)
16. G. T. Zatsepin, V. A. Kuzmin [JETP Lett., 4, 78 (1966)].
17. D. J. Bird, et al., Phys. Rev. Lett., 71, 3401 (1993);
18. D. J. Bird Astrophys. J., 424, 491 (1994).
19. S. Yoshida, et al., Astropart. Phys., 3, 151 (1995).
20. S. Yoshida and M. Teshima, Prog. Theor. Phys., 89, 833 (1993);
21. F. A. Aharonian and J. W. Cronin, Phys. Rev. D, 50, 1892 (1994);
22. J. W. Elbert and P. Sommers, Astrophys. J., 441, 151 (1995).
23. F. Halzen, R. A. Vazquez, T. Stanev, and V. P. Vankov, Astropart. Phys., 3, 151 (1995).
24. V. Berezinsky, M. Kachelriess, and A. Vilenkin, Phys. Rev. Lett., 79, 4302 (1997);
25. V. A. Kuzmin and V. A. Rubakov, Phys. At. Nucl., 61, 1028 (1998)
26. V. A. Kuzmin, V. A. Rubakov [Yad. Fiz., 61, 1122 (1998)];
27. M. Birkel and S. Sarkar, Astropart. Phys., 9, 297 (1998);
28. V. Kuzmin and I. Tkachev, JETP Lett., 68, 271 (1998);
29. K. Benakli, J. Ellis, and D. V. Nanopoulos, Phys. Rev. D, 59, 047301 (1999).
30. C. T. Hill, D. N. Schramm, and T. P. Walker, Phys. Rev. D, 36, 1007 (1987);
31. G. Sigl, D. N. Schramm, and P. Bhattacharjee, Astropart. Phys., 2, 401 (1994);
32. V. Berezinsky, X. Martin, and A. Vilenkin, Phys. Rev. D, 56, 2024 (1997).
33. D. J. Chung, G. R. Farrar, and E. W. Kolb, Phys. Rev. D, 57, 4606 (1998);
34. G. R. Farrar and P. Biermann, Phys. Rev. Lett., 81, 3579 (1998);
35. I. F. Albuquerque, G. R. Farrar, and E. W. Kolb, Phys. Rev. D, 59, 015021 (1999).
36. G. Domokos and S. Kovesi-Domokos, Phys. Rev. Lett., 82, 1366 (1999).
37. D. Fargion, B. Mele, and A. Salis, astro-ph/970029.
38. T. Weiler, hep-ph/9710431.
39. E. Waxman, astro-ph/9804023.
40. H. Kang and G. Steigman, Nucl. Phys., B372, 494 (1992).
41. Particle Data Group, Eur. Phys. J. C, 3, 201 (1998).
42. R. V. Wagoner, W. A. Fowler, and F. Hoyle, Astrophys. J., 148, 3 (1967);
43. A. Yahil and G. Beaudet, Astrophys. J., 206, 26 (1976);
44. Y. David and H. Reeves, in Physical Cosmology, R. Balian, J. Audouze, and D. N. Schramm (North-Holland, Amsterdam, 1980);
45. J. N. Fry and C. J. Hogan, Phys. Rev. Lett., 49, 1783 (1982);
46. R. J. Scherrer, Mon. Not. R. Astron. Soc., 205, 683 (1983);
47. N. Terazawa and K. Sato, Astrophys. J., 294, 9 (1985);
48. K. Olive, D. N. Schramm, D. Thomas, and T. Walker, Phys. Lett. B, 265, 239 (1991);
49. G. Starkman, Phys. Rev. D, 45, 476 (1992).
50. K. Freese, E. W. Kolb, and M. S. Turner, Phys. Rev. D, 27, 1689 (1983).
51. J. Adams and S. Sarkar, in Proceedings of the ICTP Workshop on Physics of Relic Neutrinos, Trieste, Italy, 1998 (to be published).
52. M. Dine, L. Randall, and S. Thomas, Phys. Rev. Lett., 75, 398 (1995);
53. M. Dine, L. Randall, S. Thomas Nucl. Phys., B458, 291 (1996);
54. J. A. Casas and G. B. Gelmini, Phys. Lett. B, 410, 3 (1997);
55. B. A. Campbell, M. K. Gaillard, H. Murayama, and K. A. Olive, Nucl. Phys., B538, 351 (1999);
56. M. Axenides, E. G. Floratos, G. K. Leontaris, and N. D. Tracas, hep-ph/9811371.
57. A. Kusenko and M. Shaposhnikov, Phys. Lett. B, 418, 46 (1998);
58. K. Enqvist and J. McDonald, Phys. Lett. B, 425, 309 (1998).