Final results on the 13C(α,n)16O cross section at low energies at LUNA

Final results on the 13C(α,n)16O cross section at low energies at LUNA

It is well established that the 13C(α, n)16O reaction (Q=2.215 MeV) is the major neutron source feeding the s-process in low mass (1−3M⊙) Asymptotic Giant Branch (AGB) stars. In the last decades, several measurements have been performed. Nevertheless, no dataset reaches the Gamow window (140 keV...

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Bibliographische Detailangaben
Hauptverfasser: Ciani, Giovanni Francesc, Csedreki, Laszlo, Rapagnani, David, Best, Andreas, micola, Alba
Format: Tagungsbericht
Sprache:eng
Schlagworte:
Asymptotic giant branch stars
Asymptotic methods
Cross-sections
Laboratories
Neutrons
Uncertainty
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Zusammenfassung:It is well established that the 13C(α, n)16O reaction (Q=2.215 MeV) is the major neutron source feeding the s-process in low mass (1−3M⊙) Asymptotic Giant Branch (AGB) stars. In the last decades, several measurements have been performed. Nevertheless, no dataset reaches the Gamow window (140 keV
ISSN:2101-6275
2100-014X
DOI:10.1051/epjconf/202226008003