Abstract
The astrophysical S-factor and reaction rates for the triple-alpha process are calculated in the direct-capture model. It is shown that the stellar carbon production is extremely sensitive to small variations in the N-N interaction.
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Oberhummer, H. et al. (1995). Alpha clustering and the stellar nucleosynthesis of carbon. In: Anagnostatos, G.S., von Oertzen, W. (eds) Atomic and Nuclear Clusters. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-79696-8_17
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DOI: https://doi.org/10.1007/978-3-642-79696-8_17
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