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Our Project(a) on Ejecta
Neutron Star Merger r-process
Alison Dreyfuss, Sarah Schwartz, Julia Bliss
Prompt:: Determine, using the literature, representative conditions for tidal ejection of material from neutron star mergers and for neutrino driven winds. Calculate, using the reaction network, abundance patterns for each and compare the results. Discuss why the patterns look different.
June 9
- Some trajectories can be found here → http://compact-merger.astro.su.se/downloads.html
- We struggled with recompiling to get the code to include NSE (nuclear statistic equilibrium), but it ended up working. We followed the steps on this other group's page
- We got it running!!!! Yay!
group9.1402352036.txt.gz · Last modified: 2014/06/09 18:13 by dreyfuss
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