dorsal/arxiv
View SchemaAlpha Clustering and the stellar nucleosynthesis of carbon
| Authors | H. Oberhummer, H. Krauss, K. Grün, T. Rauscher, H. Abele, P. Mohr, G. Staudt |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9310016 |
| URL | https://arxiv.org/abs/nucl-th/9310016 |
| DOI | 10.1007/BF01288967 |
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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"abstract": "The astrophysical S--factor and reaction rates for the triple--alpha process\nare calculated in the direct--capture model. It is shown that the stellar\ncarbon production is extremely sensitive to small variations in the N--N\ninteraction.",
"arxiv_id": "nucl-th/9310016",
"authors": [
"H. Oberhummer",
"H. Krauss",
"K. Gr\u00fcn",
"T. Rauscher",
"H. Abele",
"P. Mohr",
"G. Staudt"
],
"categories": [
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],
"doi": "10.1007/BF01288967",
"title": "Alpha Clustering and the stellar nucleosynthesis of carbon",
"url": "https://arxiv.org/abs/nucl-th/9310016"
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