Low-energy resonances in the 22Ne(p,γ)23Na reaction directly observed at LUNA
The 22Ne(p,γ)23Na reaction is involved in the hydrogen burning neon-sodium (NeNa) cycle. This cycle is active in asymptotic giant branch stars (AGB) as well as in novae. In the Gamow window temperature range (30MK < T < 420 MK corresponding to proton center of mass energies 40 keV < E <...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2015-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/20159303004 |