Target characterizations for direct measurement of the 13C(α, n)16O reaction at LUNA 400
The 13C(α, n)16O reaction is the main neutron source for the s-process in low mass AGB stars. Although several direct measurements have been performed, no dataset reaches the Gamow window due to the low cross section. Moreover a dominant component of systematic uncertainty comes from target behaviou...
Gorde:
| Egile Nagusiak: | , , , , |
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| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
EDP Sciences
2017-01-01
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| Saila: | EPJ Web of Conferences |
| Sarrera elektronikoa: | https://doi.org/10.1051/epjconf/201716501012 |
| Etiketak: |
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