neutronic
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neutronic [2014/06/11 20:07] lauer |
neutronic [2014/06/12 20:06] (current) yuan cleanup |
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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. | ||
| - | == Tsunghan Yeh: Inputs == | + | ===== Links ===== |
| - | * [x] Read Paper | + | * [[https://github.com/xrf/talent-astro-proj2|Code]] |
| - | * [x] Create network list/sunet- use premade scenario following Fisker_2007 (see references) | + | * [[https://wikihost.nscl.msu.edu/talent/lib/exe/fetch.php?media=neutronic.pdf|Presentation]] |
| - | * [x] Temperature profile- use Fisker premade scenario | + | |
| - | * [x] Determine initial molar abundances to altar ab_XRB file | + | |
| - | * [ ] PPT 3,4,7 | + | |
| - | == Amber Lauer: Code == | + | ===== Results ===== |
| - | * [x] Read Paper | + | * [[http://youtu.be/pHKFIH-Llqo|Video 1 (small nuclear network)]] |
| - | * [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, MS Excel eats a space column about half way down the file, was causing burst plotting errors. | + | * [[http://youtu.be/uV3hGIiyVgc|Video 2 (large nuclear network)]] |
| - | * [x] use .py script to make plots- | + | |
| - | * abundance plots working per Fei [[|python script]], [[|required file#1]], [[|required file#2]] | + | |
| - | * easier in excel | + | |
| - | * animation script working per Fei [[|python script]] | + | |
| - | * [ ] PPT 2,5,6, references | + | |
| - | == Fei Yuan: Analysis == | + | ===== Conclusion ===== |
| - | * [x] Read Paper | + | Since the initial X-ray burst is dependent on so few nuclei, almost no configuration can stop the burst behavior in a toy model. |
| - | * [x] 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) | + | |
| - | * [x] refine python scripts to read output, visualize | + | |
| - | * [ ] use .py script to make video | + | |
| - | * [ ] PPT 8,9,10 | + | |
| - | ===== Results ===== | + | ===== Log ===== |
| - | ===== Conclusion ===== | + | ==== Tsunghan Yeh: Inputs ==== |
| - | ===== Links ===== | + | * Read paper |
| + | * Create network list/sunet: use premade scenario following Fisker_2007 (see references in presentation) | ||
| + | * Temperature profile: use Fisker premade scenario | ||
| + | * Determine initial molar abundances to alter ab_XRB file | ||
| + | * PPT 3, 4, 7 | ||
| + | |||
| + | ==== Amber Lauer: Code ==== | ||
| + | |||
| + | * 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 | ||
| + | |||
| + | ==== Fei Yuan: Analysis ==== | ||
| + | |||
| + | * 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.1402531669.txt.gz · Last modified: 2014/06/11 20:07 by lauer
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