User Tools

Site Tools


group4

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Next revision
Previous revision
group4 [2014/06/09 13:55]
akers created
group4 [2014/06/18 09:02]
ahn
Line 1: Line 1:
 Our group consists of: Our group consists of:
  
-Heiko Moeller +  * Heiko Moeller ​(parameter) 
-Charlie Akers +  ​* ​Charlie Akers (analysis) 
-Tony Ahn+  ​* ​Tony Ahn (code)
  
-We are simulating the merger of two neutron stars, ​and analysing possible ramifications for the r-process, using the VH1 code.+We are simulating the merger of two neutron stars, analysing possible ramifications for the r-process ​and comparing to the neutrino driven wind scenario, using the xnet code. 
 + 
 +The final version of xnet code can be found in [[https://​github.com/​phystory/​vRprocess.git]] 
 +Or, you can download tar file in [[https://​docmgmt.nscl.msu.edu/​share/​page/​site/​TALENT/​document-details?​nodeRef=workspace://​SpacesStore/​7dc780da-5fec-4403-82a6-1726dbaac284]] (login required). 
 + 
 +We will use an initial thermal profile based on the work of Stephan Rosswog, see http://​compact-merger.astro.su.se/​downloads.html
group4.txt · Last modified: 2014/06/18 09:02 by ahn