Neutrino flavor goniometry by high energy astrophysical beams

Modern Physics Letters A

Volumn 23, Issue 17-20, 2008, Pages 1313-1324

  Pakvasa, Sandip ^a  

^a UNIVERSITY OF HAWAII   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 47749131172     PISSN: 02177323     EISSN: None     Source Type: Journal    
DOI: 10.1142/s0217732308027680     Document Type: Conference Paper

References (78)

1. Descriptions of several KM3 detectors can be found at http://icecube.wisc.edu/ and at http://www.km3net.org/home.php.
2. The Auger detector is described at http://www.auger.org/; for the planned JEM-EUSO detector, see http://jemeuso.riken.jp/ or http://aquila.lbl.EUSO/.
3. Examples are ANITA:hep-ph/0503304, and SALSA:astro-ph/0412128.
4. S. Pakvasa, 9th International Symposium on Neutrino Telescopes, Venice, Italy, 6-9 Mar 2001, Venice 2001, Neutrino Telescopes, ed. M. Baldo-Ceolin, Vol. 2, p. 603; hep-ph/0105127.
5. Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theoret. Phys. 28, 870 (1962);
6. B. M. Pontecorvo, Zh. Eksp. Teor. Fiz. 53, 1717 (1967),
7. V. N. Gribov and B. M. Pontecorvo, Phys. Lett. B28, 493 (1969);
8. B. W. Lee, S. Pakvasa, R. Shrock, and H. Sugawara, Phys. Rev. Lett. 38, 937 (1977).
9. J. G. Learned and K. Mannheim, Ann. Rev. Nucl. Part. Sci. 50, 603 (2000), and references therein.
10. J. G. Learned and S. Pakvasa, Astropart. Phys. 3, 267 (1995), hep-ph/9405296.
11. P. Lipari, M. Lusignoli, and D. Meloni, Phys. Rev. D75, 123005 (2007); arXiv:0704.0718;
12. S. Pakvasa, W. Rodejohann, and T. J. Weiler, JHEP 02, 05 (2008), arXiv:0711.4517.
13. J. P. Rachen and P. Meszaros, Phys. Rev. D58, 123005 (1998); astro-ph/9802280;
14. M. Kacherliess, S. Ostapchenko, and R. Tomas, Phys. Rev. D77, 023007 (2008), arXiv:0708.3007.
15. L. Anchordoqui, H. Goldberg, F. Halzen, and T. Weiler, Phys. Lett. B593, 42 (2004), astro-ph/0311002.
16. V. S. Berezinsky and G. T. Zatsepin, Phys. Lett. B28, 423 (1969).
17. K. Greisen, Phys. Rev. Lett. 16, 748 (1966);
18. G. Zatsepin and V. Kuzmin, JETP Lett. 4, 78 (1966).
19. R. Engel, D. Seckel, and T. Stanev, Phys. Rev. D64, 093010 (2001), astro-ph/0101216.
20. M. C. Gonzalez-Garcia and M. Maltoni, arXiv:0704.1800.
21. P. F. Harrison, D. H. Perkins, and W. G. Scott, Phys. Lett. B530, 267 (2002), hep-ph/0202074.
22. M. Applonio et al., Eur. Phys. J. C2, 331 (2003), hep-ex/0301017.
23. H. Athar, M. Jezabek, and O. Yasuda, Phys. Rev. D62, 103007 (2000); hep-ph/0005104;
24. L. Bento, P. Keranen, and J. Maalampi, Phys. Lett. B476, 205 (2000); hep-ph/9912240.
25. L. A. Anchordoqui, H. Goldberg. F. Halzen, and T. J. Weiler, Phys. Lett. B621, 18 (2005), hep-ph/041003.
26. Z-Z. Xing, Phys. Rev. D74, 013009 (2006), hep-ph/ 065219;
27. W. Rodejohann, J. Cosmol. Astropart. Phys. 01, 029 (2007), hep-ph/0612047.
28. P. D. Serpico and M. Kacherliess, Phys. Rev. Lett. 94, 211102(2005).
29. K. Blum, Y. Nir, and E. Waxman, arXiv:0706.2070.
30. R. L. Awasthi and S. Choubey, Phys. Rev. D76, 113002 (2007), arXiv:0706.0399;
31. H. Athar, M. Jezabek, and O. Yasuda, Phys. Rev. D62 (2000), hep-ph/0005104.
32. D. B. Kaplan, A. E. Nelson, and N. Weiner, Phys. Rev. Lett. 93, 091801 (2004), hep-ph/0401099.
33. Super-Kamiokande collaboration, arXiv:0801.0776.
34. J. F. Beacom, N. Bell, D. Hooper, S. Pakvasa, and T. J. Weiler, Phys. Rev. Lett. 91, 181301 (2003); hep-ph/0211305.
35. S. Pakvasa, Physics Potential and Development of Muon Colliders, Mu 99, ed. D. Cline, San Francisco, AIP Conf. Proc. 542, 99 (2000), hep-ph/0004077.
36. G. Gelmini and M. Roncadelli, Phys. Lett. B99, 411 (1981).
37. Y. Chikasige, R. Mohapatra, and R. Peccei, Phys. Rev. Lett. 45, 1926 (1980).
38. J. Valle, Phys. Lett. B131, 87 (1983);
39. G. Gelmini and J. Valle, ibid. B142, 181 (1983);
40. A. Joshipura, and S. Rindani, Phys. Rev. D46, 3008 (1992);
41. A. Acker, A. Joshipura and S. Pakvasa, Phys. Lett. B285, 371 (1992).
42. V. Barger, W-Y. Keung, and S. Pakvasa, Phys. Rev. D25, 907 (1982);
43. A. P. Lessa and O. L. G. Peres, Phys. Rev. D75 (2007), hep-ph/0701068.
44. J. F. Beacom, N. Bell, and S. Dodelson, Phys. Rev. Lett. 93, 121304(2004), hep-ph/0404585;
45. see also P. Serpico, Phys. Rev. Lett. 98, 171301 (2007), astro-ph/0701699.
46. Z. Chacko, L. J. Hall, T. Okui, and S. J. Oliver, Phys. Rev. D70, 085008 (2004), hep-ph/0312267.
47. N. F. Bell, E. Pierpaoli, and K. Sigurdson, Phys. Rev. D73, 063523 (2006), astro-ph/0511410;
48. S. Hannestad and G. Raffelt, Phys. Rev. D72, 103514 (2005), hep-ph/0509278.
49. K. Hirata et al., Phys. Rev. Lett. 58, 1497 (1988);
50. R. M. Bionta et al., ibid. 58, 1494 (1988).
51. K. Eguchi et al.; Phys. Rev. Lett. 92, 071301 (2004), hep-ex/0310047.
52. J. F. Beacom and N. Bell; Phys. Rev. D65, 113009 (2002), hep-ph/0204111; and references cited therein.
53. V. D. Barger, J. G. Learned, S. Pakvasa, and T. J. Weiler, Phys. Rev. Lett. 82. 2640 (1999), hep-ph/9810121;
54. V. Barger, J. G. Learned, P. Lipari, M. Lusignoli, S. Pakvasa, and T. J. Weiler, Phys. Lett. B462, 104 (1999), hep-ph/9907421;
55. Y. Ashie et al., Phys. Rev. Lett. 93, 101801 (2004), hep-ex/0404034.
56. S. Pakvasa, Lett. Nuov. Cim. 31, 497 (1981);
57. Y. Farzan and A. Smirnov, Phys. Rev. D65, 113001 (2002), hep-ph/0201105.
58. T. J. Weiler, W. A. Simmons, S. Pakvasa, and J. G. Learned, hep-ph/9411432.
59. P. Keranen, J. Maalampi, and J. T. Peltonieni, Phys. Lett. B461, 230 (1999), hep-ph/9901403.
60. J. F. Beacom, N. Bell, D. Hooper, S. Pakvasa, and T. J. Weiler, Phys. Rev. D69, 017303 (2004), hep- ph/0309267.
61. K. Enqvist, P. Keranen, and J. Maalampi, Phys. Lett. B438, 295 (1998), hep-ph/9806392.
62. G. Domokos and S. Kovesi-Domokos, Phys. Lett. B410, 57 (1997), hep-ph/9703265.
63. H. Minakata and A. Yu. Smirnov, Phys. Rev. D54, 3698 (1996), hep-ph/9601311.
64. V. D. Barger, S. Pakvasa, T. J. Weiler, and K. Whisnant, Phys. Rev. Lett. 85, 5055 (2000), hep-ph/0005197.
65. R. Fardon, A. E. Nelson, and N. Weiner, J. Cosmol. Astropart. Phys. 410, 005 (2004), astro-ph/0309800; P. Q. Hung, hep-ph/00010126.
66. P. Q. Hung, and H. Paes, Mod. Phys. Lett. A20, 209 (2006), astro-ph/0311131.
67. D. Hooper, D. Morgan and E. Winstanley, Phys. Lett. 609 206, (2005), hep-ph/0410094.
68. L. Wolfenstein, Nucl. Phys. B186, 147 (1981);
69. S. M. Bilenky and B. M. Pontecorvo, Sov. J. Nucl. Phys. 38, 248 (1983);
70. S. T. Petcov, Phys. Lett. B110, 245 (1982).
71. J. F. Beacom, N. Bell, D. Hooper, J. G. Learned, S. Pakvasa, and T. J. Weiler; Phys. Rev. Lett., 92 (2004), hep-ph/0307151;
72. see also P. Keranen, J. Maalampi, M. Myyrylainen and J. Riittinen, Phys. Lett. B574, 162 (2003), hep-ph/0307041 for similar considerations.
73. M. Kobayashi and C. S. Lim, Phys. Rev. D64, 013003 (2001), hep-ph/0012266.
74. J. F. Beacom, N. Bell, D. Hooper, S. Pakvasa, and T. J. Weiler; Phys. Rev. D68, 093005 (2003), hep-ph/0307025;
75. F. Halzen and D. Hooper, Rept. Prog. Phys. 65, 1025 (2002), astro-ph/0204527.
76. A. Karle, Nucl. Phys. Proc. Supp., 118 (2003), astro-ph/0209556;
77. A. Goldschmidt, Nucl. Phys. Proc. Suppl. 110, 516 (2002).
78. G. Barenboim and C. Quigg, Phys. Rev. D67, 073024 (2003), hep-ph/0301220.