Resonant neutrino spin-flavor precession and supernova nucleosynthesis and dynamics

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 55, Issue 6, 1997, Pages 3265-3275

  Nunokawa, H ^a   Qian, Y Z ^a   Fuller, G M ^a  

^a UNIVERSITY OF WASHINGTON   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000700934     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.55.3265     Document Type: Article

References (36)

1. C. S. Lim and W. Marciano, Phys. Rev. D37, 1368 (1988).
2. E. Akhmedov, Phys. Lett. B213, 64 (1988);
3. See also, J. Schechter and J. W. F. Valle, Phys. Rev. D24, 1883 (1981);
4. 25, 283 (1982).
5. S. P. Mikheyev and A. Yu. Smirnov, Sov. J. Nucl. Phys.42, 913 (1985);
6. L. Wolfenstein, Phys. Rev. D17, 2369 (1978).
7. E. Kh. Akhmedov, A. Lanza, S. T. Petcov, and D. W. Sciama, Phys. Rev. D55, 515 (1997).
8. E. M. Burbidge, G. R. Burbidge, W. A. Fowler, and F. Hoyle, Rev. Mod. Phys.29, 547 (1957); A. G. W. Cameron
9. Publ. Astron. Soc. Pac.69, 201 (1957).
10. S. E. Woosley and E. Baron, Astrophys. J.391, 228 (1992);
11. S. E. Woosley, Astron. Astrophys. Suppl. Ser.97, 205 (1993).AAESB9
12. S. E. Woosley and R. D. Hoffman, Astrophys. J.395, 202 (1992);
13. B. S. Meyer, G. J. Mathews, W. M. Howard, S. E. Woosley, and R. D. Hoffman, 399, 656 (1992).
14. S. E. Woosley, J. R. Wilson, G. J. Mathews, R. D. Hoffman, and B. S. Meyer, Astrophys. J.433, 229 (1994).
15. Y.-Z. Qian, G. M. Fuller, G. J. Mathews, R. W. Mayle, J. R. Wilson, and S. E. Woosley, Phys. Rev. Lett.71, 1965 (1993).
16. B. S. Meyer, Astrophys. J.449, L55 (1995).
17. Y.-Z. Qian and S. E. Woosley, Astrophys. J.471, 331 (1996).
18. R. D. Hoffman, S. E. Woosley, and Y.-Z. Qian, Astrophys. J. (to be published);B. S. Meyer, L. Luo, and B. Brown, report, 1996 (unpublished).
19. G. M. Fuller, Y.-Z. Qian, and J. R. Wilson, in preparation.
20. Y.-Z. Qian, Nucl. Phys. A (to be published).
21. G. M. Fuller and B. S. Meyer, Astrophys. J.453, 792 (1995).
22. R. D. Hoffman, S. E. Woosley, G. M. Fuller, and B. S. Meyer, Astrophys. J.460, 478 (1996).
23. A. I. Derbin, A. V. Chernyi, L. A. Popeko, V. N. Muratova, G. A. Shishkina, and S. I. Bakhlanov, JETP Lett.57, 768 (1993).JTPLA2
24. G. G. Raffelt, Phys. Rev. Lett.64, 2856 (1990).
25. See for example, M. B. Voloshin, Sov. J. Nucl. Phys.48, 512 (1988);
26. K. S. Babu and R. Mohapatra, Phys. Rev. Lett.63, 228 (1988);
27. S. M. Barr, E. M. Freire, and A. Zee, 65, 2626 (1990);
28. D. Chang, W.-Y. Keung, S. Lipovaca, and G. Senjanovic, 67, 953 (1991).
29. Y.-Z. Qian and G. M. Fuller, Phys. Rev. D51, 1479 (1995);
30. G. Sigl, Phys. Rev. D51, 4035 (1995).
31. J. R. Wilson and R. W. Mayle (private communication).
32. S. J. Parke and T. P. Walker, Phys. Rev. Lett.57, 2322 (1986);
33. W. C. Haxton, Phys. Rev. D36, 2283 (1987).
34. E. Kh. Akhmedov and Z. G. Berezhiani, Nucl. Phys.B373, 479 (1992).
35. H. A. Bethe and J. R. Wilson, Astrophys. J.263, 386 (1985).
36. G. M. Fuller, R. W. Mayle, B. S. Meyer, and J. R. Wilson, Astrophys. J.389, 517 (1992).