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nu_rnet [2014/06/05 15:44] schutrumpg |
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It is possible that electron fraction Ye will affect the neutron density resulting in the abundance pattern of the r-process. | It is possible that electron fraction Ye will affect the neutron density resulting in the abundance pattern of the r-process. | ||
- | {{:core-collapse_figure.png?500|}} | + | {{:core-collapse_figure.png?650|}} |
Fig. Schematic representation of the evolutionary stages from stellar core collapse. (Ref. H.Th. Janka, arXiv:astro-ph/0612072) | Fig. Schematic representation of the evolutionary stages from stellar core collapse. (Ref. H.Th. Janka, arXiv:astro-ph/0612072) | ||
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{{ :nuclide_chart.jpg?700 |}} | {{ :nuclide_chart.jpg?700 |}} | ||
+ | The black squares mark the stable isotopes. |