Abstract
The astrophysical S-factor for the \({}^6\text {Li}(\text {p},\gamma ){}^7\text {Be}\) reaction is calculated in a cluster-model framework. The p-\({}^6\text {Li}\) interaction is determined fitting elastic scattering data. Then the astrophysical S-factor is predicted, obtaining a nice agreement with the available experimental data. Moreover we try to include in our model the resonance presented in a recent experimental work.
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Gnech, A., Elisa Marcucci, L. (2019). Theoretical Calculation of the p-\({}^6\text {Li}\) Radiative Capture. In: Formicola, A., Junker, M., Gialanella, L., Imbriani, G. (eds) Nuclei in the Cosmos XV. Springer Proceedings in Physics, vol 219. Springer, Cham. https://doi.org/10.1007/978-3-030-13876-9_64
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DOI: https://doi.org/10.1007/978-3-030-13876-9_64
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