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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Bibliographic Details
Published in:EPJ Web of conferences 2022-01, Vol.260, p.08003
Main Authors: Ciani, Giovanni Francesc, Csedreki, Laszlo, Rapagnani, David, Best, Andreas, micola, Alba
Format: Article
Language:English
Subjects:
Asymptotic giant branch stars
Asymptotic methods
Cross-sections
Laboratories
Neutrons
Uncertainty
Online Access:Get full text
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Summary: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