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- W1517847314 abstract "The 22Ne(p,γ)23Na reaction is involved in the hydrogen burning neon-sodium cycle. In second-generation stars, where the central temperature is higher than 0.05 109 K, hydrogen burning can proceed also via the NeNa cycle. The 22Ne(p,γ)23Na cross section, dominated by a large number of resonances never measured directly, is still affected by large uncertainties." @default.
- W1517847314 created "2016-06-24" @default.
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- W1517847314 date "2014-01-01" @default.
- W1517847314 modified "2023-09-27" @default.
- W1517847314 title "First test on the22Ne(p,γ)23Na reaction at LUNA" @default.
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- W1517847314 doi "https://doi.org/10.1051/epjconf/20146607004" @default.
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