neutronic
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neutronic [2014/06/12 18:35] yuan finalize wiki |
neutronic [2014/06/12 18:41] yuan update layout |
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| - | ===== Neutronic ===== | + | ====== Neutronic ====== |
| - | ==== Abstract ==== | + | ===== Abstract ===== |
| Modelling XRB nucleosynthesis in XNET following the model of the <del>Dissertation of Lau 2012</del> Fisker 2007, using the premade model for CNO XRB. | Modelling XRB nucleosynthesis in XNET following the model of the <del>Dissertation of Lau 2012</del> Fisker 2007, using the premade model for CNO XRB. | ||
| - | Goal: Create video of working burst nuclides chart. Vary initial metallicity still using Fisker thermal trajectory, see if burst still occurs. Vary initial h/he ratio within metallicity still using Fisker thermal trajectory, see if burst still occurs. Create videos of stalled burst nuclides charts. | + | ===== Goals ===== |
| - | ==== Log ==== | + | * Create video of working burst nuclides chart. |
| + | * Vary initial metallicity still using Fisker thermal trajectory, see if burst still occurs. | ||
| + | * Vary initial H/He ratio within metallicity still using Fisker thermal trajectory, see if burst still occurs. | ||
| + | * Create videos of stalled burst nuclides charts. | ||
| - | == Tsunghan Yeh: Inputs == | + | ===== Links ===== |
| + | |||
| + | * [[https://github.com/xrf/talent-astro-proj2|Code]] | ||
| + | * [[https://wikihost.nscl.msu.edu/talent/lib/exe/fetch.php?media=neutronic.pdf|Presentation]] | ||
| + | |||
| + | ===== Log ===== | ||
| + | |||
| + | ==== Tsunghan Yeh: Inputs ==== | ||
| * Read Paper | * Read Paper | ||
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| * PPT 3,4,7 | * PPT 3,4,7 | ||
| - | == Amber Lauer: Code == | + | ==== Amber Lauer: Code ==== |
| * Read Paper | * Read Paper | ||
| Line 27: | Line 37: | ||
| * PPT 2,5,6, references | * PPT 2,5,6, references | ||
| - | == Fei Yuan: Analysis == | + | ==== Fei Yuan: Analysis ==== |
| * Read Paper | * Read Paper | ||
| Line 37: | Line 47: | ||
| * PPT 8,9,10 | * PPT 8,9,10 | ||
| - | ==== Results ==== | + | ===== Results ===== |
| * [[http://youtu.be/pHKFIH-Llqo|Video 1 (small nuclear network)]] | * [[http://youtu.be/pHKFIH-Llqo|Video 1 (small nuclear network)]] | ||
| * [[http://youtu.be/uV3hGIiyVgc|Video 2 (large nuclear network)]] | * [[http://youtu.be/uV3hGIiyVgc|Video 2 (large nuclear network)]] | ||
| - | ==== Conclusion ==== | + | ===== Conclusion ===== |
| Since the initial X-ray burst is dependent on so few nuclei, almost no configuration can stop the burst behavior in a toy model. | Since the initial X-ray burst is dependent on so few nuclei, almost no configuration can stop the burst behavior in a toy model. | ||
| - | |||
| - | ==== Links ==== | ||
| - | |||
| - | * [[https://github.com/xrf/talent-astro-proj2|Git repository]] | ||
| - | * [[https://github.com/xrf/talent-astro-proj2/raw/master/presentation.pdf|Presentation]] | ||
neutronic.txt · Last modified: 2014/06/12 20:06 by yuan
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