Determination of the initial flavor composition of ultrahigh-energy neutrino fluxes with neutrino telescopes

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 74, Issue 1, 2006, Pages

  Xing, Zhi Zhong ^a   Zhou, Shun ^a  

^a NONE

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Indexed keywords

EID: 33746293249     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.74.013010     Document Type: Article

References (32)

1. J.G. Learned and K. Mannheim, Annu. Rev. Nucl. Part. Sci. 50, 679 (2000); ARPSDF 0163-8998 10.1146/annurev.nucl.50.1.679
2. F. Halzen and D. Hooper, Rep. Prog. Phys. 65, 1025 (2002); RPPHAG 0034-4885 10.1088/0034-4885/65/7/201
3. J.J. Aubert, in Proceedings of the 3rd International Workshop on Neutrino Oscillations in Venice, 2006.
4. F. Halzen and D. Saltzberg, Phys. Rev. Lett. 81, 4305 (1998); PRLTAO 0031-9007 10.1103/PhysRevLett.81.4305
5. F. Halzen, astro-ph/0602132, and references therein.
6. Q.R. Ahmad (SNO Collaboration), Phys. Rev. Lett. 89, 011301 (2002). PRLTAO 0031-9007 10.1103/PhysRevLett.89.011301
7. For a review, see C.K. Jung, Annu. Rev. Nucl. Part. Sci. 51, 451 (2001). ARPSDF 0163-8998 10.1146/annurev.nucl.51.101701.132421
8. K. Eguchi (KamLAND Collaboration), Phys. Rev. Lett. 90, 021802 (2003). PRLTAO 0031-9007 10.1103/PhysRevLett.90.021802
9. M.H. Ahn (K2K Collaboration), Phys. Rev. Lett. 90, 041801 (2003). PRLTAO 0031-9007 10.1103/PhysRevLett.90.041801
10. J.F. Beacom and N.F. Bell, Phys. Rev. D 65, 113009 (2002); PRVDAQ 0556-2821 10.1103/PhysRevD.65.113009
11. J.F. Beacom, N.F. Bell, D. Hooper, S. Pakvasa, and T.J. Weiler, Phys. Rev. Lett. 90, 181301 (2003); PRLTAO 0031-9007 10.1103/PhysRevLett.90.181301
12. J.F. Beacom N.F. Bell D. Hooper S. Pakvasa T.J. Weiler Phys. Rev. D 69, 017303 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.69.017303
13. G. Barenboim and C. Quigg, Phys. Rev. D 67, 073024 (2003); PRVDAQ 0556-2821 10.1103/PhysRevD.67.073024
14. C. Quigg, hep-ph/0603372.
15. J.F. Beacom, N.F. Bell, D. Hooper, S. Pakvasa, and T.J. Weiler, Phys. Rev. D 68, 093005 (2003); PRVDAQ 0556-2821 10.1103/PhysRevD.68.093005
16. J.F. Beacom N.F. Bell D. Hooper S. Pakvasa T.J. Weiler Phys. Rev. D 72, 019901(E) (2005). PRVDAQ 0556-2821 10.1103/PhysRevD.72.019901
17. W. Winter, hep-ph/0604191.
18. P. Bhattacharjee and N. Gupta, hep-ph/0501191.
19. P.D. Serpico and M. Kachelrieß, Phys. Rev. Lett. 94, 211102 (2005); PRLTAO 0031-9007 10.1103/PhysRevLett.94.211102
20. P.D. Serpico, Phys. Rev. D 73, 047301 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.73.047301
21. J.G. Learned and S. Pakvasa, Astropart. Phys. 3, 267 (1995). APHYEE 0927-6505 10.1016/0927-6505(94)00043-3
22. L.A. Anchordoqui, H. Goldberg, F. Halzen, and T.J. Weiler, Phys. Lett. B 593, 42 (2004); PYLBAJ 0370-2693 10.1016/j.physletb.2004.04.054
23. R.M. Crocker, Astrophys. J. 622, 892 (2005). ASJOAB 0004-637X 10.1086/427972
24. Note that the neutron beam source is now controversial, as this scenario seems not to be really desirable if the cosmic rays from the Galactic center are isotropic (see, e.g., B. Revenu, in Proceedings of the 29th International Cosmic Ray Conference, Pune, 2005).
25. J.P. Rachen and P. Meszaros, Phys. Rev. D 58, 123005 (1998); PRVDAQ 0556-2821 10.1103/PhysRevD.58.123005
26. T. Kashti and E. Waxman, Phys. Rev. Lett. 95, 181101 (2005). PRLTAO 0031-9007 10.1103/PhysRevLett.95.181101
27. J. Ahrens (IceCube Collaboration), Nucl. Phys. B, Proc. Suppl. NPBSE7 0920-5632 118, 371 (2003). 10.1016/S0920-5632(03)01335-5
28. S. Eidelman (Particle Data Group), Phys. Lett. B 592, 1 (2004); PYLBAJ 0370-2693 10.1016/j.physletb.2004.06.001
29. Z.Z. Xing, Int. J. Mod. Phys. A 19, 1 (2004). IMPAEF 0217-751X 10.1142/S0217751X04016969
30. M. Apollonio (CHOOZ Collaboration), Phys. Lett. B 420, 397 (1998); PYLBAJ 0370-2693 10.1016/S0370-2693(97)01476-7
31. F. Boehm (Palo Verde Collaboration), Phys. Rev. Lett. 84, 3764 (2000). PRLTAO 0031-9007 10.1103/PhysRevLett.84.3764
32. A. Strumia and F. Vissani, Nucl. Phys. NUPBBO 0550-3213 B726, 294 (2005). 10.1016/j.nuclphysb.2005.07.031