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group4 [2014/06/09 14:14] akers |
group4 [2014/06/18 09:02] (current) ahn |
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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 xnet 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. |
- | We will use an initial thermal profile based on the data from http://compact-merger.astro.su.se/downloads.html | + | 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 |