Neutrino-induced neutron spallation and supernova [Formula Presented]-process nucleosynthesis

Physical Review C - Nuclear Physics

Volumn 55, Issue 3, 1997, Pages 1532-1544

  Qian, Y Z ^a,b   Haxton, W C ^b   Langanke, K ^a,c   Vogel, P ^a,b  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b UNIVERSITY OF WASHINGTON   (United States)

^c AARHUS UNIVERSITY   (Denmark)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0031481608     PISSN: 05562813     EISSN: 1089490X     Source Type: Journal    
DOI: 10.1103/PhysRevC.55.1532     Document Type: Article

References (31)

1. See, for example, G. J. Mathews and J. J. Cowan, Nature (London)345, 491 (1990)
2. K.-L. Kratz, J.-P. Bitouzet, F.-K. Thielemann, P. Möller, and B. Pfeiffer, Astrophys. J.403, 216 (1993)
3. S. E. Woosley, J. R. Wilson, G. J. Mathews, R. D. Hoffman, and B. S. Meyer, Astrophys. J.433, 229 (1994)
4. S. E. Woosley and R. D. Hoffman, Astrophys. J.395, 202 (1992)
5. D. K. Nadyozhin and I. V. Panov, in Proceedings of the International Symposium on Weak and Electromagnetic Interactions in Nuclei (WEIN-92), edited by Ts. D. Vylov (World Scientific, Singapore, 1993).
6. K.-L. Kratz, F.-K. Thielemann, W. Hillebrandt, P. Möller, V. Harms, A. Wöhr, and J. W. Truran, J. Phys. G14, S331 (1988)
7. G. M. Fuller and B. S. Meyer, Astrophys. J.453, 792 (1995)
8. G. C. McLaughlin and G. M. Fuller, Astrophys. J.464, L143 (1996)
9. G. V. Domogatskii and D. K. Nadëzhin, Sov. Astron.22, 297 (1978)
10. G. C. McLaughlin and G. M. Fuller, Astrophys. J.455, 202 (1995)
11. H.-T. Janka and W. Hillebrandt, Astron. Astrophys.224, 49 (1989)
12. J. R. Wilson (private communication)
13. and as cited in Y.-Z. Qian and G. M. Fuller, Phys. Rev. D52, 656 (1995)
14. B. A. Brown and B. H. Wildenthal, Annu. Rev. Nucl. Part. Sci.38, 29 (1988)
15. K. Langanke, D. J. Dean, P. B. Radha, Y. Alhassid, and S. E. Koonin, Phys. Rev. C52, 718 (1995)
16. K. Nakayama, A. Pio Galeão, and F. Krmpotić, Phys. Lett.114B, 217 (1982)
17. A. Gavron, in Computational Nuclear Physics, edited by K. Langanke, J. A. Maruhn, and S. E. Koonin (Springer-Verlag, New York, 1993), Vol. 2.
18. P. Möller, J. R. Nix, W. D. Myers, and W. J. Swiatecki, At. Data Nucl. Data Tables59, 185 (1995)
19. S. E. Woosley, D. H. Hartmann, R. D. Hoffman, and W. C. Haxton, Astrophys. J.356, 272 (1990)
20. S. W. Bruenn and W. C. Haxton, 376, 678 (1991).
21. E. Kolbe, K. Langanke, S. Krewald, and F.-K. Thielemann, Phys. Rep.227, 37 (1993)
22. T. W. Donnelly, J. Dubach, and W. C. Haxton, Nucl. Phys.A251, 353 (1975)
23. See, J. Rapaport and E. Sugarbaker, Annu. Rev. Nucl. Part. Sci.44, 109 (1994) for a collection of (Formula presented)-measured GT-strength profiles
24. P. B. Radha, D. J. Dean, S. E. Koonin, and K. Langanke (in preparation).
25. E. Kolbe, K. Langanke, S. Krewald, and F.-K. Thielemann, Nucl. Phys.A540, 599 (1992)
26. Y.-Z. Qian and S. E. Woosley, Astrophys. J.471, 331 (1996); ASJOABR. D. Hoffman, S. E. Woosley, and Y.-Z. Qian, ibid. (submitted).
27. See for example, S. Goriely and M. Arnould, Astron. Astrophys.312, 327 (1996)
28. P. Möller, J. R. Nix, and K.-L. Kratz, At Data Nucl. Data Tables (submitted).
29. F. Käppeler, H. Beer, and K. Wisshak, Rep. Prog. Phys.52, 945 (1989)
30. B. Chen, J. Dobaczewski, K.-L. Kratz, K. Langanke, B. Pfeiffer, F.-K. Thielemann, and P. Vogel, Phys. Lett. B355, 37 (1995)
31. F. Käppeler, S. Jaag, Z. Y. Bao, and G. Reffo, Astrophys. J.366, 605 (1991). ASJOAB