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

group4

This is an old revision of the document!

Our group consists of:

  • Heiko Moeller
  • Charlie Akers
  • Tony Ahn

We are simulating the merger of two neutron stars, and analysing possible ramifications for the r-process, using the VH1 code.

We will use an initial trajectory based on the data from 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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