FYSS3440 Nuclear Astrophysics (6 cr)
Description
Abundances and observations
Stellar evolution, different types of stars
Nuclear reactions
Primordial nucleosynthesis: origin of hydrogen and helium
Hydrogen burning: pp chains and CNO cycles, energy production in the Sun
Helium burning: triple alpha process, origin of carbon and oxygen
Advanced burning stages: carbon, neon, oxygen and silicon burning, nuclear statistical equilibrium, core collapse supernovae
Origin of heavier elements: neutron capture processes s and r, other processes (i, p and rp)
Programme(s) to run nuclear reaction network codes and data libraries
Learning outcomes
At the end of this course, students can:
explain where and how chemical elements have been formed in the Universe
classify stars based on their evolution and observations
know different reaction types and factors affecting the reaction rates in stars
name current reserach topics in nuclear astrophysics
Description of prerequisites
Nuclear Physics FYSS3301-302, or equivalent knowledge
Basic understanding of nuclear mass and binding energy, mass excess; nuclear liquid drop model and shell model; radioactive decay; cross section; fusion and fission
Study materials
Lecture material in Moodle
Literature
- Christian Iliadis: Nuclear Physics of Stars. Wiley-VCH. ISBN: 978-3-527-40602-9; ISBN: 978-3-527-40602-9
- Rolfs & Rodney: Cauldrons in the Cosmos
Completion methods
Method 1
Method 2
Teaching (6 cr)
Independent study (6 cr)
Exercises and final exam, or only the final exam