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- W2320625597 abstract "Nuclear astrophysics deals with the mechanism of the energy generation and element synthesis in various cosmic environments, by combining the astronomic observations with laboratory nuclear physics studies [1,2]. Therefore, understanding the underlying physical processes of star evolution relies on both, and in particular, studies of the relevant reaction network are of prime importance in reproducing the observed element abundances. The nuclear inputs need, according to different astronomic processes, mass, half-life, decay and reaction rates, separation energy etc. Among these, the single-particle or αcluster resonances close to the threshold are of fundamental importance in nuclear astrophysics, since their dominant role in determining the reaction rates and therefore the thermonuclear runway [3,4]. The properties of the resonances are normally obtained by analyzing an experimental excitation function. For a stable projectile and target combination, the excitation function can be measured precisely by changing the beam energy" @default.
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- W2320625597 date "2011-08-01" @default.
- W2320625597 modified "2023-10-14" @default.
- W2320625597 title "STUDY OF ELASTIC RESONANCE SCATTERING AT CIAE" @default.
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- W2320625597 doi "https://doi.org/10.1142/9789814360654_0038" @default.
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