| Autor: |
Reifarth, R., Alpizar-Vicente, A., Hatarik, R., Bredeweg, T. A., Esch, E.-I., Greife, U., Haight, R. C., Kronenberg, A., O'Donnell, J. M., Rundberg, R. S., Schwantes, J. M., Ullmann, J. L., Vieira, D. J., Wouters, J. M. |
| Předmět: |
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| Zdroj: |
AIP Conference Proceedings; 2005, Vol. 769 Issue 1, p1323-1326, 4p |
| Abstrakt: |
One of the most interesting nuclear physics challenges is obtaining a detailed understanding of the nucleosynthesis processes of the elements. Knowledge about the stellar sites, and how they are governed by stellar evolution and cosmology are crucial in understanding the overall picture. Information on reaction rates for neutron- and charged-particle-induced reactions have a direct impact on existing stellar models. Except for the stable isotopes, very few neutron-induced reactions in the energy range of interest have been measured to date. DANCE measurements on stable and unstable isotopes will provide many of the missing key reactions that are needed to understand the nucleosynthesis of the heavy elements. © 2005 American Institute of Physics [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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