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Radiative neutron capture: Hauser Feshbach vs. statistical resonances
The radiative neutron capture rates for isotopes of astrophysical interest are commonly calculated on the basis of the statistical Hauser Feshbach (HF) reaction model, leading to smooth and monotonically varying temperature-dependent Maxwellian-averaged cross sections (MACS). The HF approximation is...
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| Hlavní autoři: | , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Elsevier
2017-01-01
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| Edice: | Physics Letters B |
| Témata: | |
| On-line přístup: | http://www.sciencedirect.com/science/article/pii/S0370269316306815 |
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