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Department of Physics and Astronomy, Michigan State University National Superconducting Cyclotron Laboratory

group4

Our group consists of:

  • Heiko Moeller (parameter)
  • Charlie Akers (analysis)
  • Tony Ahn (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

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