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group9 [2014/06/09 13:47] dreyfuss |
group9 [2014/06/09 18:03] dreyfuss |
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**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. | **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 == | + | === June 9 === |
- | Julia:: has trajectories for temperature, density for NN merger from [[http://arxiv.org/pdf/1307.2939v2.pdf|Korobkin work]] (specific data unavailable - part of ongoing collaboration) | + | * Some trajectories can be found here -> http://compact-merger.astro.su.se/downloads.html |
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+ | * We struggled with recompiling to get the code to include NSE (nuclear statistic equilibrium), but it ended up working. We followed the steps on [[https://wikihost.nscl.msu.edu/talent/doku.php?id=nu_rnet|this other group's page]]. |