NFYK11013U Gravitation and Cosmological Dynamics
Volume 2013/2014
Education
MSc Programme in
Physics
Content
- Dark matter, stellar and gas structures. Their properties, creation and development.
- Hydrostatic equilibrium, and its application on galaxies and galaxy clusters.
- Jeans equation, the solution hereof, and application on realistic systems.
- Equilibrium of collisionsless systems, Boltzmann equation. Potential theory. Stellar motions.
- Jeans theorem. Eddingtons method for equlibrated structures.
- Phase mixing and violent relaxation. Dynamical friction.
Learning Outcome
Skills
- Deep insight and certain application of the basic equations for cosmological structures.
- Superior description of the physics responsible for the structure of cosmological structures, including motions of stars, phase mixing, violent relaxation and dynamical friction.
- Detailed knowledge of the solutions of the Jeans equation, and its application to realistic systems.
- Certain application of the Jeans theorems for spherical systems.
- Detailed knowledge of the application of hydrostatic equilibrium for realistic systems.
- The ability to critically interpret scientific overview articles within the subject.
- The ability to apply knowledge about the structure of cosmological structures and dynamics in other major areas of astrophysics.
Knowledge
The student will achieve an understanding of the basic physical
processes responsible for the structure and dynamics of
cosmological structures.
In addition, the student will obtain knowledge of the fundamental
equations, which describe the structures consisting of stars, gas
and dark matter.
Competences
This course will provide the student with a qualitative
understanding of the profiles of cosmological structures. The
student will also develop the conceptual, mathematical and
numerical skills needed when studying the literature within the
subject and in wider astrophysical connections. The course will
establish a solid foundation for a M.Sc. project in
phenomenological or theoretical astrophysics.
Literature
"Galactic
Dynamics", Binney & Tremained, Princeton series in
astrophysics, 2008
Teaching and learning methods
Lectures, exercises and
projects work
Workload
- Category
- Hours
- Exam
- 0,5
- Lectures
- 28
- Preparation
- 103
- Project work
- 32,5
- Theory exercises
- 42
- Total
- 206,0
Sign up
Self Service at KUnet
As an exchange, guest and credit student - click here!
Continuing Education - click here!
As an exchange, guest and credit student - click here!
Continuing Education - click here!
Exam
- Credit
- 7,5 ECTS
- Type of assessment
- Oral examination, 25 minWithout time for preparation.
- Aid
- Without aids
- Marking scale
- 7-point grading scale
- Censorship form
- No external censorship
More internal examiners
Criteria for exam assesment
The grade 12 is given for:
The presentation where the student independently and with a clear overview documents his/her knowledge and understanding of all the points mentioned under Skills.
The presentation where the student independently and with a clear overview documents his/her knowledge and understanding of all the points mentioned under Skills.
Course information
- Language
- English
- Course code
- NFYK11013U
- Credit
- 7,5 ECTS
- Level
- Full Degree Master
- Duration
- 1 block
Offered every second year, odd study years (2013/14).
- Placement
- Block 3
- Schedule
- B
- Course capacity
- No restriction to number of participants
- Continuing and further education
- Study board
- Study Board of Physics, Chemistry and Nanoscience
Contracting department
- The Niels Bohr Institute
Course responsibles
- Steen Harle Hansen (hansen@nbi.ku.dk)
Saved on the
30-04-2013