This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision Next revision Both sides next revision | ||
nu_rnet [2014/06/05 17:16] schutrumpg |
nu_rnet [2014/06/05 17:20] schutrumpg |
||
---|---|---|---|
Line 13: | Line 13: | ||
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|}} | + | {{:core-collapse_figure.png?650|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) | + | |
=====Method and aims:===== | =====Method and aims:===== | ||
Line 67: | Line 65: | ||
====Results==== | ====Results==== | ||
==$Y_e=0.2$== | ==$Y_e=0.2$== | ||
- | {{ :ev20.png?300 |}} | + | {{ :ev20.png?400 |}} |
==$Y_e=0.25$== | ==$Y_e=0.25$== | ||
- | {{ :ev25.png?300 |}} | + | {{ :ev25.png?400 |}} |
==$Y_e=0.4$== | ==$Y_e=0.4$== | ||
- | {{ :ev40.png?300 |}} | + | {{ :ev40.png?400 |}} |