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nu_rnet [2014/06/02 16:36] ahn |
nu_rnet [2014/06/02 16:46] ahn |
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- | [Group 7] | + | **[Group 7]** |
- | * Group name: $\nu$Rnet | + | *** Group name:** $\nu$Rnet |
- | * Members: | + | *** Members:** |
Tony Ahn: Analysis person | Tony Ahn: Analysis person | ||
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Bastian Schuetrumpf: Code person | Bastian Schuetrumpf: Code person | ||
- | * Motivation | + | *** Motivation** |
- | It is possible that neutrino driven wind will affect the neutron density resulting in the abundance pattern of the r-process. | + | |
- | {{:core-collapse_figure.png?200|}} | + | 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|}} | ||
+ | Fig. Schematic representation of the evolutionary stages from stellar core collapse. (Ref. H.Th. Janka, arXiv:astro-ph/0612072) | ||
+ | |||
+ | *** Method:** | ||
- | * Method: | ||
- To simulate r-process using x-net | - To simulate r-process using x-net | ||