FYSS3440 Nuclear Astrophysics (6 cr)
Description
Content
Basic concepts in nuclear astrophysics; selected astrophysical aspects: stellar evolution, novae, core-collapse supernovae, type I x-ray bursts, neutron-star mergers, solar system abundances; nuclear reactions and in particular thermonuclear reactions; primordial nucleosynthesis; hydrostatic hydrogen burning in stars: pp chains and CNO cycles; explosive hydrogen burning in stars: rp process; helium burning in stars: production of carbon and oxygen in stars; carbon, neon, oxygen and silicon burning in stars; nucleosynthesis beyond the iron peak: s-, r- and p-processes; examples of nuclear astrophysics experiments
Completion methods
Assignments, examination
Assessment details
The final grade is based on examination and assignments. At least half of the maximum points is needed to pass the course.
Learning outcomes
Additional information
Spring semester 2nd period, every two years starting spring 2018.
Description of prerequisites
Literature
- Christian Iliadis: Nuclear Physics of Stars. Wiley-VCH. ISBN: 978-3-527-40602-9; ISBN: 978-3-527-40602-9