week3
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| - | ====== TALENT ====== | + | ====== SCHEDULE ====== |
| - | ===== Training in Advanced Low Energy Nuclear Theory ===== | + | |
| - | {{:talent.png?600|www.nucleartalent.org}} | + | |
| - | ===== Course 7: Nuclear Theory for Astrophysics ===== | + | |
| Lecturers: **[[BrianFields|Brian D. Fields]]**, **[[RaphHix|William Raphael Hix]]**, **[[HendrikSchatz|Hendrik Schatz]]**, **[[GailMcLaughlin|Gail McLaughlin]]**, **[[GeorgeFuller|George Fuller]]** | Lecturers: **[[BrianFields|Brian D. Fields]]**, **[[RaphHix|William Raphael Hix]]**, **[[HendrikSchatz|Hendrik Schatz]]**, **[[GailMcLaughlin|Gail McLaughlin]]**, **[[GeorgeFuller|George Fuller]]** | ||
| + | ---- | ||
| + | **{{:outline.pdf|Schedule}}**, **[[Week1|Week 1]]**, **[[Week2|Week 2]]**, **[[Week3|Week 3]]** | ||
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| * [[Gail3|Gail 3]]: Role of nuclear data in determining the abundance pattern | * [[Gail3|Gail 3]]: Role of nuclear data in determining the abundance pattern | ||
| - | * [[George3|George 3]]: Gravitational collapse of massive stars, neutrinos and nucleosynthesis | + | * [[George3|George 3]]: Weak Interaction pre-, peri- and post-collapse |
| * Will discuss weak interaction physics during pre-collapse, hydrostatic evolution; the nuclear and weak interaction physics of collapse | * Will discuss weak interaction physics during pre-collapse, hydrostatic evolution; the nuclear and weak interaction physics of collapse | ||
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| * Will explore how models of core collapse supernova/compact object merger r-process nucleosynthesis and issues in primordial nucleosynthesis and the cosmic microwave background could be impacted by new neutrino sector physics | * Will explore how models of core collapse supernova/compact object merger r-process nucleosynthesis and issues in primordial nucleosynthesis and the cosmic microwave background could be impacted by new neutrino sector physics | ||
| - | {{:week3.jpg?nolink&1200|}} | + | |
week3.1398692925.txt.gz · Last modified: 2014/04/28 09:48 by cyburt
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