Gravitational Waves Progenitors 7404-WA-PFG
Introduction: massive stars as GW progenitors
Compact object progenitors: black holes, neutron stars, white dwarfs. The cosmic gravitational wave background.
Stellar progenitors: massive stars and their astrophysics I. – Single stellar evolution
Stellar progenitors: massive stars and their astrophysics II. – Final stage and explosion
Stellar progenitors: massive stars and their astrophysics III. – Binary stars
Stellar populations in clusters and galaxies; the computational/statistical method of "synthetic populations"
GR, linearized Einstein equations, wave propagation through space-time
GW-detectors in past, present, future
Connected phenomena: supernovae, gamma-ray bursts
Cosmology, star-formation in the early, metal-poor Universe
Total student workload
Learning outcomes - knowledge
Learning outcomes - skills
Learning outcomes - social competencies
Teaching methods
Observation/demonstration teaching methods
Expository teaching methods
- participatory lecture
- discussion
- description
Exploratory teaching methods
- presentation of a paper
- seminar
Online teaching methods
- exchange and discussion methods
Prerequisites
Course coordinators
Assessment criteria
Assessment methods:
– oral examination: W1, W2, W3, U1, U2, U3, K1
Assessment criteria:
fail: below 50 pts (below 50%)
satisfactory: 50 pts (50%)
satisfactory plus: 60 pts (60%)
good: 70 pts (70%)
good plus: 75 pts (75%)
very good: 80 pts (80%)
Bibliography
https://global.oup.com/academic/product/gravitational-waves-pack-volumes-1-and-2-9780198755289?cc=pl&lang=en&
https://www.ucolick.org/~woosley/ay220-19/papers/pols11.pdf
https://iopscience.iop.org/article/10.1088/1742-6596/1263/1/012008
https://arxiv.org/abs/1806.05820
Additional information
Additional information (registration calendar, class conductors, localization and schedules of classes), might be available in the USOSweb system: