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The astrophysical r-process and its dependence on properties of nuclei far from stability: beta strength functions and neutron capture rates
It is shown that the astrophysical r-process and the question of its site are very sensitive to 'standard' nuclear physics parameters like the beta decay properties and neutron capture rates. Since for these quantities in almost all r-process calculations up to now, and also in all estimat...
| Autores principales: | , , , , |
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| Lenguaje: | eng |
| Publicado: |
CERN
1981
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.5170/CERN-1981-009.341 http://cds.cern.ch/record/878092 |