Neutrino decay as an explanation of atmospheric neutrino observations

Physical Review Letters

Volumn 82, Issue 13, 1999, Pages 2640-2643

  Barger, V ^a,b   Learned, J G ^c   Pakvasa, S ^c   Weiler, T J ^d  

^a FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

^b University of Wisconsin Madison   (United States)

^c UNIVERSITY OF HAWAII   (United States)

^d VANDERBILT UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 4243217950     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.82.2640     Document Type: Article

References (39)

1. Super-Kamiokande Collaboration, Y. Fukuda, et al. Phys. Rev. Lett. 81, 1562, (1998).
2. V. Barger, and K. Whisnant, Phys. Lett. B. 209, 365, (1988).
3. Phys. Lett. B. J. G. Learned, S. Pakvasa, and T. J. Weiler, 207, 79, (1988).
4. K. Hidaka, M. Honda, and S. Midorikawa, Phys. Rev. Lett. 61, 1537, (1988).
5. E. Ma, and P. Roy, Phys. Rev. Lett. 80, 4637, (1998).
6. Y. Grossman, and M. P. Worah, hep-ph/9807511.
7. G. Brooijmans, hep-ph/9808498.
8. M. C. Gonzalez-Garcia, et al. hep-ph/9809531.
9. D. L. Britton, et al. Phys. Rev. D. 49, 28, (1994).
10. Particle Data Group, C. Caso, et al. Eur. Phys. J. C. 3, 1, (1998).
11. G. Gelmini, and M. Roncadelli, Phys. Lett. 99B, 411, (1981).
12. Y. Chicashige, R. N. Mohapatra, and R. Peccei, Phys. Lett. 98B (1980).
13. A. Acker, A. Joshipura, and S. Pakvasa, Phys. Lett. B. 285, 371, (1992).
14. G. Gelmini, and J. W. F. Valle, Phys. Lett. 142B, 181, (1984).
15. K. Choi, and A. Santamaria, Phys. Lett. B. 267, 504, (1991).
16. A. S. Joshipura, Report No. PRL-TH-91/6.
17. A. S. Joshipura, and S. Rindani, Phys. Rev. D. 46, 3000, (1992).
18. A. Acker, S. Pakvasa, and J. Pantaleone, Phys. Rev. D. 45, R1, (1992).
19. V. Barger, W.-Y. Keung, and S. Pakvasa, Phys. Rev. D. 25, 907, (1982).
20. J. N. Bahcall, P. Krastev, and A. Smirnov, hep-ph/9807216.
21. N. Hata, and P. Langacker, Phys. Rev. D. 56, 6107, (1997).
22. LSND Collaboration, C. Athanassopoulos, et al. Phys. Rev. Lett. 81, 1774, (1998).
23. Phys. Rev. Lett. C. Athanassopoulos, 77, 3082, (1996).
24. C. Athanassopoulos, Phys. Rev. C. 54, 2685, (1996).
25. T. P. Walker, et al. Astrophys. J. 376, 71, (1991).
26. S. Burles, K. M. Nollett, J. N. Truran, and M. S. Turner, astro-ph/9901157.
27. N. Hata, et al. Phys. Rev. Lett. 75, 3977, (1995).
28. N. Hata, Phys. Rev. D. 55, 540, (1997).
29. G. Steigman, astro-ph/9803055.
30. P. J. Kernan, and S. Sarkar, Phys. Rev. D. 54, R3681, (1996).
31. C. J. Copi, D. N. Schramm, and M. S. Turner, Phys. Rev. D. 55, 3389, (1997).
32. B. D. Fields, K. Kainulainen, K. A. Olive, and D. Thomas, New Astron. 1, 77, (1996).
33. K. A. Olive, and D. Thomas, Astropart. Phys. 7, 27, (1997).
34. E. Lisi, S. Sarkar, and F. L. Villante, hep-ph/9901404.
35. N. F. Bell, R. R. Volkas, and Y. Y. W. Wong, hep-ph/9809363.
36. N. F. Bell, R. Foot, and R. R. Volkas, Phys. Rev. D. 58, 105 010, (1998), and references therein.
37. X. Shi, and G. M. Fuller, astro-ph/9810075. astro-ph/9812232.
38. R. Foot, and R. R. Volkas, astro-ph/9811067.
39. G. G. Raffelt, Stars as Laboratories for Fundamental Physics, (The University of Chicago Press, Chicago, 1996), p. 564.