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group4 [2014/06/09 14:11] akers |
group4 [2014/06/09 16:09] akers |
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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, using the xnet code. |
- | We will use an initial trajectory based on the data from: http://compact-merger.astro.su.se/downloads.html | + | We will use an initial thermal profile based on the work of Stephan Rosswog, see http://compact-merger.astro.su.se/downloads.html |