nu_rnet
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nu_rnet [2014/06/05 17:20] 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?650|Schematic representation of the evolutionary stages from stellar core collapse. (Ref. H.Th. Janka, arXiv:astro-ph/0612072)}} | + | {{:core-collapse_figure.png?650|}} |
| + | Fig: Schematic representation of the evolutionary stages from stellar core collapse. (Ref. H.Th. Janka, arXiv:astro-ph/0612072) | ||
| =====Method and aims:===== | =====Method and aims:===== | ||
nu_rnet.txt · Last modified: 2014/06/06 09:18 by schutrumpg
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