Atmospheric neutrinos as probes of neutrino-matter interactions

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 70, Issue 11, 2004, Pages

  Friedland, Alexander ^a   Lunardini, Cecilia ^b   Maltoni, Michele ^c  

^a LOS ALAMOS NATIONAL LABORATORY   (United States)

^b INSTITUTE FOR ADVANCED STUDY   (United States)

^c STONY BROOK UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ATMOSPHERE; EXPERIMENT; MASS; MOLECULAR INTERACTION; NEUTRINO; OSCILLATION; SENSITIVITY AND SPECIFICITY; SOLAR ENERGY; STANDARD;

EID: 10444287555     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.70.111301     Document Type: Article

References (33)

1. N. Fornengo, M. Maltoni, R. T. Bayo, and J. W. F. Valle, Phys. Rev. D 65, 013010 (2002).
2. M. Guzzo, P. C. de Holanda, M. Maltoni, H. Nunokawa, M. A. Tortola, and J. W. F. Valle, Nucl. Phys. B 629, 479 (2002).
3. M. C. Gonzalez-Garcia and M. Maltoni, Phys. Rev. D 70, 033010 (2004).
4. A. Friedland, C. Lunardini, and C. Pena-Garay, Phys. Lett. B 594, 347 (2004).
5. M. M. Guzzo, P. C. de Holanda, and O. L. G. Peres, Phys. Lett. B 591, 1 (2004).
6. O. G. Miranda, M. A. Tortola, and J. W. F. Valle, hep-ph/0406280.
7. A. Friedland, C. Lunardini, and M. Maltoni (in preparation).
8. R. Engel, T. K. Gaisser, and T. Staney, Phys. Lett. B 472, 113 (2000).
9. C. W. Kim and U. W. Lee, Phys. Lett. B 444, 204 (1998); O. L. G. Peres and A. Y. Smirnov, Phys. Lett. B 456, 204 (1999); M. C. Gonzalez-Garcia, M. Maltoni, and A. Y. Smirnov, hep-ph/0408170.
10. C. W. Kim and U. W. Lee, Phys. Lett. B 444, 204 (1998); O. L. G. Peres and A. Y. Smirnov, Phys. Lett. B 456, 204 (1999); M. C. Gonzalez-Garcia, M. Maltoni, and A. Y. Smirnov, hep-ph/0408170.
11. C. W. Kim and U. W. Lee, Phys. Lett. B 444, 204 (1998); O. L. G. Peres and A. Y. Smirnov, Phys. Lett. B 456, 204 (1999); M. C. Gonzalez-Garcia, M. Maltoni, and A. Y. Smirnov, hep-ph/0408170.
12. Rν) reduce to Eq. (3) upon the application of the Fierz transformation, see, e.g., S. Bergmann, Y. Grossman, and E. Nardi, Phys. Rev. D 60, 093008 (1999).
13. A. Friedland and C. Lunardini, Phys. Rev. D 68, 013007 (2003); J. High Energy Phys. 10 (2003) 043.
14. A. Friedland and C. Lunardini, Phys. Rev. D 68, 013007 (2003); J. High Energy Phys. 10 (2003) 043.
15. G. P. Zeller et al., Phys. Rev. Lett. 88, 091802 (2002); 90, 239902(E) (2003).
16. G. P. Zeller et al., Phys. Rev. Lett. 88, 091802 (2002); 90, 239902(E) (2003).
17. P. Vilain et al., Phys. Lett. B 335, 246 (1994).
18. S. Davidson, C. Pena-Garay, N. Rius, and A. Santamaria, J. High Energy Phys. 03 (2003) 011.
19. Z. Berezhiani and A. Rossi, Phys. Lett. B 535, 207 (2002).
20. ν.
21. τ one changes the phases of the eμ and eτ entries of the Hamiltonian.
22. Super-Kamiokande Collaboration, Y. Hayato, in Proceedings of the International Europhysics Conference on High Energy Physics, Aachen, 2003 [Eur. Phys. J. C 33, s829 (2004), supplement], http://eps2003.physik.rwth-aachen.de/ transparencies/07/index.php.
23. Super-Kamiokande Collaboration, Y. Hayato, in Proceedings of the International Europhysics Conference on High Energy Physics, Aachen, 2003 [Eur. Phys. J. C 33, s829 (2004), supplement], http://eps2003.physik.rwth-aachen.de/ transparencies/07/index.php.
24. M. Honda, T. Kajita, K. Kasahara, and S. Midorikawa, Phys. Rev. D 70, 043008 (2004).
25. M. Maltoni, T. Schweiz, M. A. Tortola, and J. W. F. Valle, hep-ph/0405172.
26. V. D. Barger, A. M. Gago, D. Marfatia, W. J. C. Teves, B. P. Wood, and R. Zukanovich Funchal, Phys. Rev. D 65, 053016 (2002).
27. It is for this reason that the NC information [23,24] was not used in our analysis here and in [4].
28. S. Fukuda et al., Phys. Rev. Lett. 85, 3999 (2000); H. Sobel, in Proceedings of the XIXth International Conference on Neutrino Physics and Astrophysics, Sudbury, Canada, 2000 [Nucl. Phys. (Proc. Suppl.) 91, 127 (2001)], http://nu2000.sno.laurentian.ca/H.Sobel/index.html; M. Shiozawa, in Proceedings of the XXth International Conference on Neutrino Physics and Astrophysics, Munich, 2002, http://neutrino2002. ph.tum.de/pages/transparencies/shiozawa/ index.html.
29. S. Fukuda et al., Phys. Rev. Lett. 85, 3999 (2000); H. Sobel, in Proceedings of the XIXth International Conference on Neutrino Physics and Astrophysics, Sudbury, Canada, 2000 [Nucl. Phys. (Proc. Suppl.) 91, 127 (2001)], http://nu2000.sno.laurentian.ca/H.Sobel/index.html; M. Shiozawa, in Proceedings of the XXth International Conference on Neutrino Physics and Astrophysics, Munich, 2002, http://neutrino2002. ph.tum.de/pages/transparencies/shiozawa/ index.html.
30. S. Fukuda et al., Phys. Rev. Lett. 85, 3999 (2000); H. Sobel, in Proceedings of the XIXth International Conference on Neutrino Physics and Astrophysics, Sudbury, Canada, 2000 [Nucl. Phys. (Proc. Suppl.) 91, 127 (2001)], http://nu2000.sno.laurentian.ca/H.Sobel/index.html; M. Shiozawa, in Proceedings of the XXth International Conference on Neutrino Physics and Astrophysics, Munich, 2002, http://neutrino2002. ph.tum.de/pages/transparencies/shiozawa/ index.html.
31. S. Fukuda et al., Phys. Rev. Lett. 85, 3999 (2000); H. Sobel, in Proceedings of the XIXth International Conference on Neutrino Physics and Astrophysics, Sudbury, Canada, 2000 [Nucl. Phys. (Proc. Suppl.) 91, 127 (2001)], http://nu2000.sno.laurentian.ca/H.Sobel/index.html; M. Shiozawa, in Proceedings of the XXth International Conference on Neutrino Physics and Astrophysics, Munich, 2002, http://neutrino2002. ph.tum.de/pages/transparencies/shiozawa/ index.html.
32. SNO Collaboration, S. N. Ahmed et al., Phys. Rev. Lett. 92, 181301 (2004).
33. T. Araki et al., hep-ex/0406035.