蘑菇直播

Osaamistavoitteet

At the end of this course, students will be able to explain, where and how elements have been formed in the universe. Students will be able to explain which factors have an effect on thermonuclear reaction rates and classify and list thermonuclear reactions as well as calculate reaction rates for basic thermonuclear reactions in stars. They will also be able to give examples of nuclear astrophysics experiments and research.

Suoritustavat

Assignments, examination

厂颈蝉盲濒迟枚

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

尝颈蝉盲迟颈别诲辞迟

Spring semester 2nd period, every two years starting spring 2018.

Kirjallisuus

Arviointiperusteet

The final grade is based on examination and assignments. At least half of the maximum points is needed to pass the course.

Esitietovaatimukset

Before enrolling to this course, students are expected to have a good understanding of the basic concepts in Nuclear Physics: nuclear mass and binding energy, mass excess; nuclear liquid drop model and shell model; radioactive decay law; beta and gamma decay and transition probabilities; cross section; fusion reactions and fission

Vastaavat opintojaksot

• FYSN440 Ydinastrofysiikka - 0 op