Matches in SemOpenAlex for { <https://semopenalex.org/work/W2103330400> ?p ?o ?g. }
- W2103330400 endingPage "847" @default.
- W2103330400 startingPage "824" @default.
- W2103330400 abstract "Radiative capture of nucleons at energies of astrophysical interest is one of the most important processes for nucleosynthesis. The nucleon capture can occur either by a compound nucleus reaction or by a direct process. The compound reaction cross sections are usually very small, specially for light nuclei. The direct capture proceeds either via the formation of a single-particle resonance, or a non-resonant capture process. In this work we calculate radiative capture cross sections and astrophysical S-factors for nuclei in the mass region A<20 using single-particle states. We carefully discuss the parameter fitting procedure adopted in the simplified two-body treatment of the capture process. Then we produce a detailed list of cases for which the model works well. Useful quantities, such as spectroscopic factors and asymptotic normalization coefficients, are obtained and compared to published data." @default.
- W2103330400 created "2016-06-24" @default.
- W2103330400 creator A5015453437 @default.
- W2103330400 creator A5016048500 @default.
- W2103330400 creator A5085944997 @default.
- W2103330400 date "2010-11-01" @default.
- W2103330400 modified "2023-10-16" @default.
- W2103330400 title "Radiative capture of nucleons at astrophysical energies with single-particle states" @default.
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