group4
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group4 [2014/06/09 16:18] akers |
group4 [2014/06/18 09:02] (current) ahn |
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| 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 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. | ||
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| + | 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 | We will use an initial thermal profile based on the work of Stephan Rosswog, see http://compact-merger.astro.su.se/downloads.html | ||
group4.1402345088.txt.gz ยท Last modified: 2014/06/09 16:18 by akers
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