Where do we stand with solar neutrino oscillations?

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 58, Issue 9, 1998, Pages

  Smirnov, A Yu ^c  

^a INSTITUTE FOR ADVANCED STUDY   (United States)

^b UNIVERSITY OF WISCONSIN MADISON   (United States)

^c ABDUS SALAM INTERNATIONAL CENTRE FOR THEORETICAL PHYSICS   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 1542573440     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.58.096016     Document Type: Article

References (102)

1. R. Davis, Jr., D. S. Harmer, and K. C. Hoffman, Phys. Rev. Lett. 20, 1205 (1968).
2. J. N. Bahcall, N. A. Bahcall, and G. Shaviv, Phys. Rev. Lett. 20, 1209 (1968).
3. J. N. Bahcall and R. Davis, Jr., Science 191, 264 (1976).
4. J. N. Bahcall, Neutrino Astrophysics (Cambridge University Press, Cambridge, England, 1989).
5. KAMIOKANDE Collaboration, Y. Fukuda, Phys. Rev. Lett. 77, 1683 (1996).
6. GALLEX Collaboration, P. Anselmann, Phys. Lett. B 342, 440 (1995);
7. Phys. Lett. BGALLEX Collaboration, W. Hampel, 388, 364 (1996).
8. SAGE Collaboration, V. Gavrin et al., in Neutrino 96, Proceedings of the XVII International Conference on Neutrino Physics and Astrophysics, Helsinki, edited by K. Huitu, K. Enqvist, and J. Maalampi (World Scientific, Singapore, 1997), p. 14;V. Gavrin et al., in Neutrino 98, Proceedings of the XVIII International Conference on Neutrino Physics and Astrophysics, Takayama, Japan, 1998, edited by Y. Suzuki and Y. Totsuka [Nucl. Phys. B (Proc. Suppl.) (in press)].
9. SuperKamiokande Collaboration, Y. Fukuda, Phys. Rev. Lett. 81, 1158 (1998).
10. R. Svoboda (for the SuperKamiokande Collaboration), ITP Conference on Solar neutrinos: News About SNUs, 1997 (unpublished), http://www.itp.ucsb.edu/online/snu/svoboda/;H. Sobel (for the SuperKamiokande Collaboration), Aspen Winter Conference on Particle Physics, 1998, Aspen, CO (unpublished). http://www.physics.arizona.edu/ ina/aspen98.html.
11. SuperKamiokande Collaboration, Y. Suzuki, in Neutrino 98 7.
12. L. Wolfenstein, Phys. Rev. D 17, 2369 (1978);
13. S. P. Mikheyev and A. Yu. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1985)];
14. S. P. MikheyevA. Yu. SmirnovNuovo Cimento C 9, 17 (1986).
15. V. N. Gribov and B. M. Pontecorvo, Phys. Lett. 28B, 493 (1969).
16. A. B. McDonald, in Proceedings of the 9th Lake Louise Winter Institute, edited by A. Astbury (World Scientific, Singapore, 1994), p. 1.
17. C. Arpesella et al., BOREXINO proposal, Vols. 1 and 2, edited by G. Bellini et al. (Univ. of Milano, Milano, 1992).
18. J. N. Bahcall, Phys. Rev. C 56, 3391 (1997).
19. J. N. Bahcall, Phys. Rev. C 54, 411 (1996).
20. J. N. Bahcall and R. Ulrich, Rev. Mod. Phys. 60, 297 (1988).
21. J. N. Bahcall, M. Kamionkowski, and A. Sirlin, Phys. Rev. D 51, 6146 (1995).
22. J. N. Bahcall, E. Lisi, D. E. Alburger, L. De Braeckeleer, S. J. Freedman, and J. Napolitano, Phys. Rev. C 54, 411 (1996).
23. J. N. Bahcall, S. Basu, and M. H. Pinsonneault, Phys. Lett. B 433, 1 (1998).
24. E. Adelberger, Rev. Mod. Phys. (to be published).
25. C. W. Johnson, E. Kolbe, S. E. Koonin, and K. Langanke, Astrophys. J. 392, 320 (1992).
26. S. M. Bilenky and C. Giunti, “Implications of CHOOZ Results for the Decoupling of Solar and Atmospheric Neutrino Oscillations,” hep-ph/9802201.
27. CHOOZ Collaboration, M. Apollonio, Phys. Lett. B 420, 397 (1998).
28. J. N. Bahcall, M. H. Pinsonneault, S. Basu, and J. Christensen-Dalsgaard, Phys. Rev. Lett. 78, 171 (1997).
29. J. N. Bahcall and M. H. Pinsonneault, Rev. Mod. Phys. 64, 885 (1992).
30. J. N. Bahcall and M. H. Pinsonneault, Rev. Mod. Phys. 67, 781 (1995).
31. N. Hata, S. Bludman, and P. Langacker, Phys. Rev. D 49, 3622 (1994).
32. S. Parke, Phys. Rev. Lett. 74, 839 (1995).
33. K. M. Heeger and R. G. H. Robertson, Phys. Rev. Lett. 77, 3720 (1996).
34. J. N. Bahcall and P. I. Krastev, Phys. Rev. D 53, 4211 (1996).
35. J. N. Bahcall and H. A. Bethe, Phys. Rev. Lett. 65, 2233 (1990).
36. N. Hata and P. Langacker, Phys. Rev. D 52, 420 (1995).
37. G. L. Fogli, E. Lisi, and D. Montanino, Phys. Rev. D 49, 3626 (1994);
38. see also G. L. Fogli and E. Lisi, Astropart. Phys. 3, 185 (1995).
39. V. Berezinsky, G. Fiorentini, and M. Lissia, Phys. Lett. B 341, 38 (1995).
40. N. Hata and P. Langacker, Phys. Rev. D 50, 632 (1993).
41. P. Krastev and S. T. Petcov, Phys. Rev. Lett. 72, 1960 (1994);
42. P. KrastevS. T. PetcovNucl. Phys. B449, 605 (1995).
43. E. Gates, L. M. Krauss, and M. White, Phys. Rev. D 51, 2631 (1995).
44. T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1987).
45. E. Calabresu, N. Ferrari, G. Fiorentini, and M. Lissia, Astropart. Phys. 4, 159 (1995).
46. M. Maris and S. T. Petcov, Phys. Rev. D 56, 7444 (1997).
47. Z. Berezhiani and A. Rossi, Phys. Rev. D 51, 5229 (1995).
48. J. N. Bahcall and P. I. Krastev, Phys. Rev. C 56, 2839 (1997).
49. P. Krastev and S. T. Petcov, Phys. Lett. B 207, 64 (1988);
50. Phys. Lett. BP. KrastevS. T. Petcov214, 661(E) (1988);
51. Phys. Lett. Bsee also S. T. Petcov, 200, 373 (1988);
52. Phys. Lett. BS. T. Petcov214, 139 (1988).
53. B. T. Cleveland, Astrophys. J. 496, 505 (1998);
54. B. T. Cleveland, Nucl. Phys. B (Proc. Suppl.) 38, 47 (1995);
55. R. Davis, Prog. Part. Nucl. Phys. 32, 13 (1994).
56. P. I. Krastev and S. T. Petcov, Phys. Lett. B 299, 99 (1993);
57. G. L. Fogli, E. Lisi, and D. Montanino, Phys. Rev. D 54, 2048 (1996).
58. A. J. Baltz and J. Weneser, Phys. Rev. D 50, 5971 (1994);
59. Phys. Rev. DA. J. BaltzJ. Weneser51, 3960 (1995).
60. P. Krastev and A. Smirnov, Phys. Lett. B 338, 282 (1994).
61. P. Krastev and S. Petcov, Phys. Rev. D 53, 1665 (1996).
62. S. Nussinov, Phys. Lett. 63B, 201 (1976).
63. P. F. Harrison, D. H. Perkins, and W. G. Scott, Phys. Lett. B 349, 137 (1995);
64. Phys. Lett. BP. F. HarrisonD. H. PerkinsW. G. Scott396, 186 (1997).
65. R. Foot and R. R. Volkas, Phys. Rev. D 52, 6595 (1995).
66. G. Comforto, A. Marchionni, F. N. Martelli, F. Vetrano, M. Lanfranchi, and G. Torricelli-Ciamponi, Astropart. Phys. 5, 147 (1996).
67. A. Acker and S. Pakvasa, Phys. Lett. B 397, 209 (1997);
68. Phys. Lett. BA. Acker, S. Pakvasa, J. Leaned and T. Weiler, 298, 149 (1993).
69. P. I. Krastev and S. T. Petcov, Phys. Lett. B 395, 69 (1997).
70. S. P. Mikheyev and A. Yu. Smirnov, in ’86 Massive Neutrinos in Astrophysics and in Particle Physics, Proceedings of the Sixth Moriond Workshop, edited by O. Fackler and Y. Trân Thanh Vân (Editions Frontières, Gif-sur-Yvette, France, 1986), p. 355;
71. J. Bouchez, Z. Phys. C 32, 499 (1986);
72. M. Cribier, W. Hampel, J. Rich, and D. Vignaud, Phys. Lett. B 182, 89 (1986);
73. M. L. Cherry and K. Lande, Phys. Rev. D 36, 3571 (1987);
74. S. Hiroi, H. Sakuma, T. Yanagida, and M. Yoshimura, Phys. Lett. B 198, 403 (1987);
75. S. Hiroi, H. Sakuma, T. Yanagida, and M. Yoshimura, Prog. Theor. Phys. 78, 1428 (1987);
76. A. Dar, A. Mann, Y. Melina, and D. Zajfman, Phys. Rev. D 35, 3607 (1988);
77. M. Spiro and D. Vignaud, Phys. Lett. B 242, 279 (1990).
78. A. J. Baltz and J. Weneser, Phys. Rev. D 35, 528 (1987).
79. A. J. Baltz and J. Weneser, Phys. Rev. D 37, 3364 (1988).
80. J. N. Bahcall, Phys. Rev. D 44, 1644 (1991).
81. W. Kwong and S. P. Rosen, Phys. Rev. Lett. 68, 748 (1992);
82. P. I. Krastev and A. Yu. Smirnov, Phys. Lett. B 338, 282 (1994);
83. W. Kwong and S. P. Rosen, Phys. Rev. D51, 6159 (1995);
84. P. I. Krastev and S. T. Petcov, Nucl. Phys. B449, 605 (1995).
85. R. S. Raghavan, Phys. Rev. Lett. 78, 3618 (1997).
86. J. N. Bahcall and P. Krastev, Phys. Lett. B (to be published), hep-ph/9807525.
87. E. Bellotti, “Proposal for a Permanent Gallium Neutrino Observatory (GNO) at Laboratori Nazionali Del Gran Sasso,” http://kosmopc.mpi-hd.mpg.de/gallex/gallex.html, February (1996).
88. GONG Collaboration, J. Christensen-Dalsgaard, Science 272, 1286 (1996);
89. J. N. Bahcall and M. H. Pinsonneault, Rev. Mod. Phys. 67, 781 (1995);
90. A. Kovetz and G. Shaviv, Astrophys. J. 426, 787 (1994);
91. V. Castellani, S. Degl’Innocenti, G. Fiorentini, L. M. Lissia, and B. Ricci, Phys. Lett. B 324, 425 (1994);
92. J. Christensen-Dalsgaard, Europhys. News 25, 71 (1994);
93. X. Shi, D. N. Schramm, and D. S. P. Dearborn, Phys. Rev. D 50, 2414 (1994);
94. A. Dar and G. Shaviv, Astrophys. J. 468, 933 (1996);
95. V. Castellani, S. Degl’Innocenti, and G. Fiorentini, Astron. Astrophys. 271, 601 (1993);
96. S. Turck-Chièze and I. Lopes, Astrophys. J. 408, 347 (1993);
97. G. Berthomieu, J. Provost, P. Morel, and Y. Lebreton, Astron. Astrophys. 268, 775 (1993);
98. J. N. Bahcall and M. H. Pinsonneault, Rev. Mod. Phys. 64, 885 (1992);
99. I.-J. Sackman, A. I. Boothroyd, and W. A. Fowler, Astrophys. J. 360, 727 (1990);
100. J. N. Bahcall and R. K. Ulrich, Rev. Mod. Phys. 60, 297 (1988);
101. O. Richard, S. Vauclair, C. Charbonnel, and W. A. Dziembowski, Astron. Astrophys. 312, 1000 (1996);
102. F. Ciacio, S. Degl’Innocenti, and B. Ricci, Astron. Astrophys., Suppl. Ser. 123, 449 (1997).