The Origin of the Elements
DOI :
https://doi.org/10.17307/wsc.v0i0.43Résumé
There are about 35 nuclei found in nature, which are not susceptible to neutron capture and are explained by the p-process. The modeling for this process requires thousands of nuclear reactions involving both stable and unstable nuclei including (α,α), (α,p) and (α,γ) reactions. In a recent experiment, the cross section of the reaction 120Te(α,p)123I was measured in the energy range of astrophysical interest for the p-process. The α beam from the Notre Dame FN Tandem Van de Graaff accelerator bombarded highly enriched self-supporting 120Te targets and the γ-rays from the activated 123I was counted with a pair of Ge clover detectors in close geometry.Â
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Lesher, S. R., & Arend, A. (2012). The Origin of the Elements. Proceedings of the Wisconsin Space Conference. https://doi.org/10.17307/wsc.v0i0.43
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Astronomy and Cosmology
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This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.