Possible tomography of the Sun’s magnetic field with solar neutrinos

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 57, Issue 12, 1998, Pages 7108-7119

  Pulido, João ^a  

^a INSTITUTO SUPERIOR TÉCNICO   (Portugal)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001738847     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.57.7108     Document Type: Article

References (60)

1. R. Davis, D. S. Harmer, and K. C. Hoffman, Phys. Rev. Lett. 20, 1205 (1968).
2. S. Degl’Innocenti, W. A. Dziembowski, G. Fiorentini, and B. Ricci, Astropart. Phys.7, 77 (1997).
3. A. Cisneros, Astrophys. Space Sci. 10, 87 (1971).
4. M. B. Voloshin, M. I. Vysotsky, and L. B. Okun, Sov. J. Nucl. Phys. 44, 440 (1986);
5. Sov. J. Nucl. Phys.M. B. Voloshin and M. I. Vysotsky, 44, 544 (1986).
6. J. K. Rowley, B. T. Cleveland, and R. Davis, in Solar Neutrinos and Neutrino Astronomy, edited by M. L. Cherry, K. Lande, and W. A. Fowler (AIP Conf. Proc. No. 126) (AIP, New York, 1985), p. 1; R. Davis, 7th Workshop on Grand Unification: ICOBAN ’86, edited by J. Arafune (unpublished);R. Davis, B. T. Cleveland, and J. K. Rowley, Proceedings of 20th International Cosmic Ray Conference, Moscow, 1987 (unpublished), Vol. 4, p. 328.
7. J. N. Bahcall, G. B. Field, and W. H. Press, Astrophys. J. 320, L69 (1987).
8. B. W. Filippone and P. Vogel, Phys. Lett. B 246, 546 (1990).
9. J. W. Bieber, Nature (London) 348, 407 (1990).
10. X. Shi, D. N. Schramm, R. Rosner, and D. S. Dearborn, Comments Nucl. Part. Phys. 21, 151 (1993).
11. Homestake Collaboration, K. Lande, in Neutrino ’96, Proceedings of the 17th International Conference on Neutrino Physics and Astrophysics, Helsinki, Finland, edited by K. Enqvist, K. Huitu, and J. Maalampi (World Scientific, Singapore, 1997), p. 25.
12. Kamiokande Collaboration, Y. Suzuki, in Neutrino ’96 10, p. 73.
13. SAGE Collaboration, V. N. Gavrin, in Neutrinos ’96 10, p. 14.
14. Gallex Collaboration, M. Cribier, in TAUP ’97, 5th International Workshop on Topics in Astroparticle and Underground Physics, Gran Sasso, Assergi, Italy, 1997 (unpublished).
15. SuperKamiokande Collaboration, J. Hill, in Proceedings of the XXXII Rencontre de Moriond, 1997 (unpublished).
16. G. Walther, Phys. Rev. Lett. 79, 4522 (1998).
17. S. Turck-Chieze and I. Lopes, Astrophys. J. 408, 347 (1993).
18. S. Turck-Chieze, S. Cahen, M. Casse, and C. Doom, Astrophys. J. 335, 415 (1988).
19. C. R. Proffit, Astrophys. J. 425, 849 (1994).
20. O. Richard, Astron. Astrophys. 312, 1000 (1996).
21. S. Degl’Innocenti, Astron. Astrophys., Suppl. Ser. 123, 1 (1997).
22. J. N. Bahcall and M. H. Pinsonneault, Rev. Mod. Phys. 67, 781 (1995).
23. J. N. Bahcall, in Neutrino ’96 10, p. 56.
24. L. Wolfenstein, Phys. Rev. D 17, 2369 (1978);
25. Phys. Rev. DL. Wolfenstein20, 2634 (1979);
26. S. P. Mikheyev and A. Smirnov, Sov. J. Nucl. Phys. 42, 913 (1985).
27. P. F. Harrison, Phys. Lett. B 374, 111 (1996).
28. C. S. Lim and W. J. Marciano, Phys. Rev. D 37, 1368 (1988);
29. E. K. Akhmedov, Phys. Lett. B 213, 64 (1988);
30. E. K. Akhmedov, Sov. J. Nucl. Phys. 48, 382 (1988).
31. E. Roulet, Phys. Rev. D 44, R935 (1991);
32. M. M. Guzzo, A. Masiero, and S. T. Petcov, Phys. Lett. B 260, 154 (1991);
33. J. Pulido, Mod. Phys. Lett. A 8, 1273 (1993);
34. P. I. Krastev and J. N. Bahcall, talk given at Symposium on Flavour Changing Neutral Currents: Present and Future Studies (FCNC 97), Santa Monica, CA, 1997, astro-ph/9703267.
35. W. Kwong and S. P. Rosen, Phys. Rev. Lett. 73, 369 (1994).
36. P. I. Krastev and S. T. Petcov, Phys. Lett. B 395, 69 (1997).
37. J. N. Bahcall, Phys. Lett. B 338, 276 (1994).
38. L. Wolfenstein and P. I. Krastev, Phys. Rev. D 55, 4405 (1997).
39. K. M. Heeger and R. G. H. Robertson, Phys. Rev. Lett. 77, 3720 (1996).
40. V. Castellani, Phys. Rep. 281, 309 (1997).
41. V. Berezinsky, Comments Nucl. Part. Phys. 21, 249 (1994).
42. Particle Data Group, R. M. Barnett, Phys. Rev. D 54, 1 (1996).
43. J. N. Bahcall and R. K. Ulrich, Rev. Mod. Phys. 60, 297 (1988).
44. L. Landau, Phys. Z. Sowjetunion 2, 46 (1932);
45. C. Zener, Proc. R. Soc. London A137, 696 (1932);
46. E. C. G. Stueckelberg, Helv. Phys. Acta 5, 369 (1932).
47. J. Pulido, Phys. Rep. 211, 167 (1992).
48. A. Dar and G. Shaviv, Astrophys. J. 468, 933 (1996).
49. S. J. Parke, Phys. Rev. Lett. 57, 1275 (1996).
50. J. Pulido, Phys. Rev. D 48, 1492 (1993).
51. E. K. Akhmedov and O. V. Bychuk, Sov. Phys. JETP 68, 250 (1989).
52. E. K. Akhmedov, A. Lanza, and S. T. Petcov, Phys. Lett. B 303, 85 (1993).
53. E. K. Akhmedov, A. Lanza, and S. T. Petcov, Phys. Lett. B 348, 124 (1995).
54. A. B. Balantekin, P. J. Hatchell, and F. Loreti, Phys. Rev. D 41, 3583 (1990).
55. S. Nussinov and Y. Rephaeli, Phys. Rev. D 36, 2278 (1987);
56. I. Goldman, Phys. Rev. Lett. 60, 1789 (1988)
57. Phys. Rev. Lett.G. Lattimer and J. Cooperstein, 61, 23 (1988);
58. R. Barbieri and R. N. Mohapatra, Phys. Rev. Lett. 61, 27 (1988);
59. D. Notzold, Phys. Rev. D 38, 1658 (1988).
60. S. M. Barr, E. M. Freire, and A. Zee, Phys. Rev. Lett. 65, 2626 (1990).