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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 Or, you can download tar file in (login required).

We will use an initial thermal profile based on the work of Stephan Rosswog, see

group4.txt · Last modified: 2014/06/18 09:02 by ahn