| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1854518 | Progress in Particle and Nuclear Physics | 2011 | 6 Pages |
Abstract
The 14N(p,γ)15O reaction controls the rate of the carbon–nitrogen–oxygen (CNO) cycle of stellar hydrogen burning. The reaction proceeds by capture to the ground state and several excited states in 15O. Several studies of this reaction have recently been performed in the low energy range 150
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Physical Sciences and Engineering
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Nuclear and High Energy Physics
Authors
M. Marta,