group4
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group4 [2014/06/09 14:11] 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 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. |
| - | We will use an initial trajectory 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). | ||
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| + | We will use an initial thermal profile based on the work of Stephan Rosswog, see http://compact-merger.astro.su.se/downloads.html | ||
group4.1402337482.txt.gz · Last modified: 2014/06/09 14:11 by akers
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