group9
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group9 [2014/05/31 01:40] yuan created group9 |
group9 [2014/06/10 18:05] (current) dreyfuss |
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| - | === Roles === | + | ===== Our Project(a) on Ejecta ===== |
| - | * Alexander Dombos (analysis) | + | ==== Neutron Star Merger r-process ==== |
| - | * Fei Yuan (code) | + | |
| - | * Heiko Möller (parameter) | + | |
| - | === Topic === | + | Alison Dreyfuss, Sarah Schwartz, Julia Bliss |
| - | //(Preliminary)// | + | **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. |
| - | Simulate the effects of a near-Earth supernova explosion at 10 parsec (the "kill radius") and the resulting collision of the blast with solar wind. Will the supernova reach 1 AU? How does the answer depend on the: | + | === June 9 === |
| - | * supernova explosion energy, | + | * Some trajectories can be found here -> http://compact-merger.astro.su.se/downloads.html |
| - | * distance, and | + | * 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]] |
| - | * interstellar density? | + | * We got it running!!!! Yay! |
| + | === June 10 === | ||
| + | |||
| + | Sarah:: worked on presentation, looked at potentially getting ifort (nope.)\\ | ||
| + | Ali & Julia:: tried to make edits to get our network running, but everything is terrible forever. | ||
group9.1401514823.txt.gz · Last modified: 2014/05/31 01:40 by yuan
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