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- W2025673755 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<Ep<500 keV and only one set of data from an experiment performed in 1987 extends up to 3 MeV. In order to obtain a reliable extrapolation of the excitation curve to astrophysical energy, R-matrix fits need data covering the widest possible range of energy. In a first phase, the experimental investigation has been performed at the Laboratory for Underground Nuclear Astrophysics (LUNA) 400 kV accelerator in an energy range that sensitively tests such fits, placed deep underground in the Gran Sasso facility in Italy, using a composite germanium detector. In a second phase, the reaction has been studied at the high-current FZD Tandetron in Dresden (Germany), in the energy region from 0.6 to 2.5 MeV. The astrophysical motivation, setup, and data analysis are presented." @default.
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- W2025673755 date "2011-04-01" @default.
- W2025673755 modified "2023-09-24" @default.
- W2025673755 title "Experimental study of the 14N(p,γ)15O reaction at high and low energies" @default.
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- W2025673755 doi "https://doi.org/10.1016/j.ppnp.2011.01.025" @default.
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