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Precision measurements on oxygen formation in stellar helium burning with gamma-ray beams and a Time Projection Chamber
The carbon/oxygen (C/O) ratio at the end of stellar helium burning is the single most important nuclear input to stellar evolution theory. However, it is not known with sufficient accuracy, due to large uncertainties in the cross-section for the fusion of helium with (12)C to form (16)O, denoted as...
| Autores principales: | , , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Nature Publishing Group UK
2021
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8505630/ https://www.ncbi.nlm.nih.gov/pubmed/34635664 http://dx.doi.org/10.1038/s41467-021-26179-x |