Up-down asymmetry: A diagnostic for neutrino oscillations

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 57, Issue 5, 1998, Pages R2649-R2652

  Flanagan, John W ^a   Learned, John G ^a   Pakvasa, Sandip ^a  

^a UNIVERSITY OF HAWAII   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000221842     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.57.R2649     Document Type: Article

References (37)

1. IMB Collaboration, R. Clark, Phys. Rev. Lett. 79, 345 (1997).
2. R. Becker-Szendy, Phys. Rev. D 46, 3720 (1992).
3. D. Casper, Phys. Rev. Lett. 66, 2561 (1991).
4. Kamiokande Collaboration, Y. Oyama, hep-ex/9706008, 1997.
5. K. S. Hirata, Phys. Lett. B 205, 416 (1988).
6. Phys. Lett. BK. S. Hirata, 280, 146 (1992).
7. Phys. Lett. BY. Fukuda, 335, 237 (1994).
8. M. Goodman, Big Sky, CIPANP97, 1997.
9. Soudan Collaboration, W. W. M. Allison, Phys. Lett. B 391, 491 (1997).
10. J. G. Learned, S. Pakvasa, and T. J. Weiler, Phys. Lett. B 207, 79 (1988).
11. Phys. Lett. BV. Barger and K. Whisnant, 209, 365 (1988).
12. K. Hidaka, M. Honda, and S. Midorikawa, Phys. Rev. Lett. 61, 1537 (1988).
13. Y. Totsuka, Plenary Talk at the International Conference on Lepton-Photon Interactions, 1997, Hamburg.
14. See various papers on solar neutrinos in the Proceedings of the XVII International Conference on Neutrinos Physics and Astrophysics, Helsinki, Finland, 1996, edited by J. Maalampi and M. Roos (World Scientific, Singapore, 1997).
15. LSND Collaboration, C. Athanassopoulos, et al., nucl-ex/9709006, 1997.
16. C. AthanassopoulosPhys. Rev. C 54, 2685 (1996).
17. C. AthanassopoulosPhys. Rev. Lett. 77, 3082 (1996).
18. C. Y. Cardall and G. Fuller, Phys. Rev. D 53, 4421 (1996).
19. Phys. Rev. Dsee also M. Narayan, G. Rajasekaran, and S. Uma Sankar, 56, 437 (1997).
20. K. S. Babu, J. C. Pati, and F. Wilczek, Phys. Lett. B 359, 3521 (1995).
21. A. Acker and S. Pakvasa, Phys. Lett. B 397, 209 (1997).
22. Phys. Lett. BA. Acker, J. G. Learned, S. Pakvasa, and T. Weiler, 298, 149 (1993).
23. G. L. Fogli, E. Lisi, D. Montanino, and G. Scioscia, hep-ph/9607251, 1996.
24. G. Conforto, Astropart. Phys. 5, 146 (1996).
25. A. Acker, B. Balantekin, and F. Loreti, Phys. Rev. D 49, 328 (1994).
26. Phys. Rev. DJ. Pantaleone, 49, 2152 (1994).
27. P. F. Harrison, D. H. Perkins, and W. G. Scott, Phys. Lett. B 396, 186 (1997).
28. Phys. Lett. BP. F. HarrisonD. H. PerkinsW. G. Scott 349, 137 (1995).
29. R. Foot and R. Volkas, Phys. Rev. D 52, 6595 (1995).
30. J. Bunn, R. Foot, and R. Volkas, hep-ph/9702429, 1997.
31. M. Gasperini, Phys. Rev. D 38, 2635 (1988).
32. A. Halprin and C. N. Leung, Phys. Rev. Lett. 67, 1833 (1991).
33. Sidney Coleman and Sheldon L. Glashow, Phys. Lett. B 405, 249 (1997).
34. S. L. Glashow, A. Halprin, P. I. Krastev, C. N. Leung, and J. Pantaleone, Phys. Rev. D 56, 2433 (1997).
35. Phys. Rev. DJ. Pantaleone, A. Halprin, and C. N. Leung, 47, 4199 (1993).
36. T. Stanev (private communication).
37. V. Agrawal, T. K. Gaisser, P. Lipari, and T. Stanev, Phys. Rev. D 53, 1314 (1996);T. K. Gaisser and T. Stanev, in Proceedings of the 24th ICRC, Rome, 1995.