group9
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group9 [2014/05/31 01:59] yuan add title and links |
group9 [2014/06/09 18:13] dreyfuss |
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| - | ====== HAℓF ====== | + | ===== Our Project(a) on Ejecta ===== |
| - | ===== Roles ===== | + | ==== Neutron Star Merger r-process ==== |
| - | * **Analysis:** Alexander Dombos | + | Alison Dreyfuss, Sarah Schwartz, Julia Bliss |
| - | * **Code:** Fei Yuan | + | |
| - | * **Parameter:** Heiko Möller | + | |
| - | ===== Topic ===== | + | **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. |
| - | //(Preliminary)// | + | === June 9 === |
| - | 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: | + | * 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 [[https://wikihost.nscl.msu.edu/talent/doku.php?id=nu_rnet|this other group's page]] | |
| - | * supernova explosion energy, | + | * We got it running!!!! Yay! |
| - | * distance, and | + | |
| - | * interstellar density? | + | |
| - | + | ||
| - | ===== External links ===== | + | |
| - | + | ||
| - | * [[https://github.com/xrf/talent-astro-proj1|Git repository]] | + | |
| - | * [[https://docmgmt.nscl.msu.edu/share/page/site/TALENT/documentlibrary#filter=path%7C/Course7_2014/Projects/Project1/group9|Document library]] | + | |
group9.txt · Last modified: 2014/06/10 18:05 by dreyfuss
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