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Courses/lectures
Introduction to Theoretical Nuclear Physics and Astrophysics - Lecture 4
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Europe/Berlin
Seminar room (basement) (Excellence Cluster 'Universe')
Seminar room (basement)
Excellence Cluster 'Universe'
Description
Title: Stellar nucleosynthesis and reaction networks
keywords: stellar evolution (brief intro), stellar nucleosynthesis (hydrostatic burning phases) of massive (and AGB) stars, s-process, explosive nucleosynthesis (r-, p-, nu-p-process), X-ray bursts (rp-process), big bang nucleosynthesis, solar neutrino problem, definition of astrophysical reaction rates, reaction networks (definition, special cases of equilibria (NSE, QSE, ng-gn)), sensitivity to nuclear input, cross sections for astrophysics: Hauser-Feshbach model, direct capture, DWBA)
keywords: stellar evolution (brief intro), stellar nucleosynthesis (hydrostatic burning phases) of massive (and AGB) stars, s-process, explosive nucleosynthesis (r-, p-, nu-p-process), X-ray bursts (rp-process), big bang nucleosynthesis, solar neutrino problem, definition of astrophysical reaction rates, reaction networks (definition, special cases of equilibria (NSE, QSE, ng-gn)), sensitivity to nuclear input, cross sections for astrophysics: Hauser-Feshbach model, direct capture, DWBA)
