dorsal/arxiv
View SchemaBe7(p,gamma)B8 and the high-energy solar neutrino flux
| Authors | Attila Csoto |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9704053 |
| URL | https://arxiv.org/abs/nucl-th/9704053 |
| Journal | Heavy Ion Physics 6 (1997) 103 |
Abstract
The importance of the Be7(p,gamma)B8 reaction in predicting the high-energy solar neutrino flux is discussed. I present a microscopic eight-body model and a potential model for the calculation of the Be7(p,gamma)B8 cross section.
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"abstract": "The importance of the Be7(p,gamma)B8 reaction in predicting the high-energy\nsolar neutrino flux is discussed. I present a microscopic eight-body model and\na potential model for the calculation of the Be7(p,gamma)B8 cross section.",
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"title": "Be7(p,gamma)B8 and the high-energy solar neutrino flux",
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