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--- nu_rnet [2014/05/30 17:30]
schutrumpg created
+++ nu_rnet [2014/06/05 13:54]
schutrumpg
@@ Line 1: / Line 1: @@
-Members:
+**[Group 7]**
+*** Group name:**  $\nu$Rnet
+*** Members:**
 Tony Ahn: Analysis person
 Tsung-han Yeh: Parameter person
 Bastian Schuetrumpf: Code person
+*** Motivation**
+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:**
+- To simulate r-process using x-net
+- To change Ye considering effects of the neutrino driven wind
+- To find change of the r-process path and change of the abundance pattern
+*** Input Parameters:**
+At first we had to set a reasonable temperature and density trajectory for a neutrino driven wind in which the r-process takes place. We take a realistic trajectory from Raphael Hix the temperature and density profile looks like this:
+{{ :out.jpg?200 |}}

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