neutronic
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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 ===== |
| + | |||
| + | * 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. | ||
| + | |||
| + | ===== 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 | ||
| + | * Create network list/sunet- use premade scenario following Fisker_2007 (see references) | ||
| + | * Temperature profile- use Fisker premade scenario | ||
| + | * Determine initial molar abundances to altar ab_XRB file | ||
| + | * PPT 3,4,7 | ||
| - | ==Tsunghan Yeh: Inputs== | + | ==== Amber Lauer: Code ==== |
| - | *[x] Read Paper | + | |
| - | *[x] Create network list/sunet- use premade scenario following Fisker_2007 (see references) | + | |
| - | *[x] Temperature profile- use Fisker premade scenario | + | |
| - | *[ ] Determine initial molar abundances to altar ab_XRB file | + | |
| - | *[ ] PPT 3,4,7 | + | |
| - | ==Amber Lauer: Code Person== | + | |
| - | *[x] Read Paper | + | |
| - | *[x] Study Xnet: made a clearer set of instructions for running non-default library: [[https://docmgmt.nscl.msu.edu/share/proxy/alfresco/api/node/content/workspace/SpacesStore/7f083725-bf8b-4544-8bd6-0758dfe92545/reaction%20network%20instructions|rxn net instructions]], ran XRB-CNO example, | + | |
| - | *[ ] use .py script to make video | + | |
| - | *[ ] PPT 2,5,6, references | + | |
| - | ==Fei Yuan: Analysis== | + | |
| - | *[x] Read Paper | + | |
| - | *[x] design end objective | + | |
| - | * [ ] Integrate the energy generated at the surface and compare to surface photon emission | + | |
| - | * [ ] vary metallicities to identify burst conditions (see abstract) | + | |
| - | * [ ] refine python scripts to read output, visualize | + | |
| - | * [ ] PPT 8,9,10 | + | |
| - | =====Results===== | + | * Read Paper |
| + | * Study Xnet: made a clearer set of instructions for running non-default library: [[https://docmgmt.nscl.msu.edu/share/proxy/alfresco/api/node/content/workspace/SpacesStore/7f083725-bf8b-4544-8bd6-0758dfe92545/reaction%20network%20instructions|rxn net instructions]], ran XRB-CNO example, MS Excel eats a space column about half way down the file, was causing burst plotting errors. | ||
| + | * Use scripts to make plots- | ||
| + | * abundance plots working | ||
| + | * easier in Excel | ||
| + | * animation script working | ||
| + | * PPT 2,5,6, references | ||
| - | =====Conclusion===== | + | ==== Fei Yuan: Analysis ==== |
| - | =====Links===== | + | * Read Paper |
| + | * Design end objective | ||
| + | * <del>Integrate the energy generated at the surface and compare to surface photon emission</del> (goal changed) | ||
| + | * vary metallicities to identify burst conditions (see abstract) | ||
| + | * refine python scripts to [[https://github.com/xrf/talent-astro-proj2/blob/master/tso_reader.py|read output]], visualize | ||
| + | * make video with [[https://github.com/xrf/talent-astro-proj2/blob/master/plot-chart|script]] | ||
| + | * PPT 8,9,10 | ||
| - | * [[https://github.com/xrf/talent-astro-proj2|Git repository]] | ||
neutronic.txt · Last modified: 2014/06/12 20:06 by yuan
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