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nu_rnet [2014/06/02 16:38] ahn |
nu_rnet [2014/06/02 16:46] ahn |
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*** Motivation** | *** Motivation** | ||
- | It is possible that neutrino driven wind 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?500|}} | ||
+ | Fig. Schematic representation of the evolutionary stages from stellar core collapse. (Ref. H.Th. Janka, arXiv:astro-ph/0612072) | ||
*** Method:** | *** Method:** |