group9
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group9 [2014/05/31 01:59] yuan add title and links |
group9 [2014/06/06 16:58] dreyfuss |
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| - | ====== HAℓF ====== | + | ===== Our Project(a) on Ejecta ===== |
| - | ===== Roles ===== | + | ==== Neutron Star Merger r-process ==== |
| - | * **Analysis:** Alexander Dombos | + | **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. |
| - | * **Code:** Fei Yuan | + | |
| - | * **Parameter:** Heiko Möller | + | |
| - | ===== Topic ===== | ||
| - | |||
| - | //(Preliminary)// | ||
| - | |||
| - | 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: | ||
| - | |||
| - | * supernova explosion energy, | ||
| - | * 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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