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neutronic [2014/06/12 18:36] yuan Change presentation link |
neutronic [2014/06/12 18:41] yuan |
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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]] | ||
+ | |||
+ | ===== Results ===== | ||
+ | |||
+ | * [[http://youtu.be/pHKFIH-Llqo|Video 1 (small nuclear network)]] | ||
+ | * [[http://youtu.be/uV3hGIiyVgc|Video 2 (large nuclear network)]] | ||
+ | |||
+ | ===== 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. | ||
+ | |||
+ | ===== 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 | ||
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* PPT 2,5,6, references | * PPT 2,5,6, references | ||
- | == Fei Yuan: Analysis == | + | ==== Fei Yuan: Analysis ==== |
* Read Paper | * Read Paper | ||
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* make video with [[https://github.com/xrf/talent-astro-proj2/blob/master/plot-chart|script]] | * make video with [[https://github.com/xrf/talent-astro-proj2/blob/master/plot-chart|script]] | ||
* PPT 8,9,10 | * PPT 8,9,10 | ||
- | |||
- | ==== Results ==== | ||
- | |||
- | * [[http://youtu.be/pHKFIH-Llqo|Video 1 (small nuclear network)]] | ||
- | * [[http://youtu.be/uV3hGIiyVgc|Video 2 (large nuclear network)]] | ||
- | |||
- | ==== 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. | ||
- | |||
- | ==== Links ==== | ||
- | |||
- | * [[https://github.com/xrf/talent-astro-proj2|Git repository]] | ||
- | * [[https://wikihost.nscl.msu.edu/talent/lib/exe/fetch.php?media=neutronic.pdf|Presentation]] | ||