week3
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| - | ====== TALENT ====== | + | ====== SCHEDULE ====== |
| - | ===== Training in Advanced Low Energy Nuclear Theory ===== | + | Lecturers: **[[BrianFields|Brian D. Fields]]**, **[[RaphHix|William Raphael Hix]]**, **[[HendrikSchatz|Hendrik Schatz]]**, **[[GailMcLaughlin|Gail McLaughlin]]**, **[[GeorgeFuller|George Fuller]]** |
| - | {{:talent.png?600|www.nucleartalent.org}} | + | ---- |
| - | ===== Course 7: Nuclear Theory for Astrophysics ===== | + | **{{:outline.pdf|Schedule}}**, **[[Week1|Week 1]]**, **[[Week2|Week 2]]**, **[[Week3|Week 3]]** |
| + | ---- | ||
| ==== Week 3 ==== | ==== Week 3 ==== | ||
| - | {{:week3.jpg?nolink&1200|}} | + | |
| + | ==== Monday, June 9, 2014 ==== | ||
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| + | * [[Gail1|Gail 1]]: Review of potential r-process sites | ||
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| + | * [[George1|George 1]]: Neutrinos, the weak interaction, and primordial nucleosynthesis I | ||
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| + | * Will discuss decoupling and freeze-out of particles in the early universe, with special emphasis on neutrino decoupling | ||
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| + | ==== Tuesday, June 10, 2014 ==== | ||
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| + | * [[Gail2|Gail 2]]: Weak interactions in the r-process | ||
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| + | * [[George2|George 2]]: Neutrinos, the weak interaction, and primordial nucleosynthesis II | ||
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| + | * Continuation of lecture (1), but now with an emphasis on the coupling of neutrinos and isospin, and therefore nucleosynthesis | ||
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| + | ==== Wednesday, June 11, 2014 ==== | ||
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| + | * [[Gail3|Gail 3]]: Role of nuclear data in determining the abundance pattern | ||
| + | |||
| + | * [[George3|George 3]]: Weak Interaction pre-, peri- and post-collapse | ||
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| + | * Will discuss weak interaction physics during pre-collapse, hydrostatic evolution; the nuclear and weak interaction physics of collapse | ||
| + | |||
| + | ==== Thursday, June 12, 2014 ==== | ||
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| + | * [[George4|George 4]]: Neutrino Physics | ||
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| + | * Will discuss neutrino flavor oscillations, neutrino spin flip, and other issues in neutrino physics relevant for nuclear astrophysics | ||
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| + | * [[George5|George 5]]: Outstanding issues in neutrino physics, compact object physics, and cosmology | ||
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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 | ||
| + | |||
week3.txt · Last modified: 2014/05/14 09:53 by cyburt
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