Astrophysical S-factors for H-burning stars
This dataset contains the latest recommendations of astrophysical S-factors for nuclear fusion reactions occurring in hydrogen-burning stars, included in the Solar Fusion III decadal review article (submitted for publication, e-print available at arXiv:2405.06470). The data includes S-factors and th...
| Autores: | , |
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| Tipo de documento: | conjunto de datos |
| Estado: | Versão publicada |
| Data de publicação: | 2024 |
| País: | España |
| Recursos: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositório: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/400989 |
| Acesso em linha: | http://hdl.handle.net/10261/400989 https://doi.org/10.20350/digitalCSIC/17585 |
| Access Level: | Acceso aberto |
| Palavra-chave: | Nuclear reactions Stellar astrophysics Nuclear astrophysics |
| Resumo: | This dataset contains the latest recommendations of astrophysical S-factors for nuclear fusion reactions occurring in hydrogen-burning stars, included in the Solar Fusion III decadal review article (submitted for publication, e-print available at arXiv:2405.06470). The data includes S-factors and their derivatives at zero energy (where available). That is, S(0), S´(0), S´´(0), in units of MeV·b, b, and b/MeV, respectively. Fractional uncertainties are also provided (marked as fr_err). Unavailable data are marked as NA. This data was used to compute the Standard Solar Models B23 / SF-III. For further information and references consult the Solar Fusion III article linked above. |
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