NFYK21004U Computational Astrophysics
MSc Programme in Physics
MSc Programme in Physics with a minor subject
The course gives an introduction to numerical methods for contemporary computational astrophysics. It covers theory and practice for numerical methods including fluid and particle dynamics, gravitational collapse, and radiative energy transfer. It gives an overview of computational models for microphysical processes, such as cooling, heating, dust dynamics, and astrochemistry. The course exercises introduce and illustrate the methods applying them to concrete examples from astrophysics, and give a “hands-on” feeling for how and in what context they are used. During the course exercises, the students will build a highly modular yet simple core program based on Jupyter notebooks written in python, which includes most of the methods covered in the lectures. The course also touches on technical aspects, such as high performance computing and efficient code development.
- Modeling the dynamics of the interstellar medium, including fluids, magnetic fields, and heating and cooling.
- Modeling gravitational collapse
- Solving the radiation transfer equation
- Using radiative transfer in connection with analysis and modeling of observations
- Modeling particle dynamics and gas-particle interaction
The student will come to know the fundamental equations that govern astrophysical dynamics, including fluids, magnetic fields, radiative energy transfer and coupled gas-particle interaction, and how to solve them with modern numerical methods. In addition, the student will achieve knowledge of the basic computational techniques used in modern astrophysics including the principles of adaptive mesh refinement techniques and the difference between mesh and particle methods.
The course gives basic competences in numerical modelling, and will establish a foundation for a M.Sc. project based on numerical modelling.
See Absalon for final course material. The following is an example of expected course literature.
P. Bodenheimer, G. P. Laughlin, M. Rozyczka, T. Plewa, H. W. Yorke: “Numerical Methods in Astrophysics”. Complemented with lecture notes.
Academic qualifications equivalent to a BSc degree is recommended.
If you are registered with examination attempts in NFYK14018U Computational Astrophysics: Star and Planet Formation without having passed the course, you have to use your last examination attempts to pass the exam in NFYK21004U - Computational Astrophysics. You have a total of three examination attempts.
- Theory exercises
- 7,5 ECTS
- Type of assessment
- Continuous assessmentWritten assignment, 4 days
- Type of assessment details
- The exam consists of two parts:
The continuous part of the evaluation, wich consists of 2-3 exercises per week, counts for 50% of the final grade. The student must have turned in at least 60% of the weekly exercises.
A written 4-day report (Monday to Thursday) with an oral defense (Friday) counts for 50% of the final grade.
- All aids allowed
- Marking scale
- 7-point grading scale
- Censorship form
- No external censorship
two internal examiners; the course responsible and an internal censor.
The re-exam consists of two parts: A 4-day report (Monday to Thursday) with an oral defense (Friday) counting for 50% of the grade. New solutions to the weekly exercies can be handed in to cover the continuous part of the evaluation (50%) no later than 2 weeks before the start of the 4-day report.
Criteria for exam assesment
see learning outcome
- Course code
- 7,5 ECTS
- Full Degree Master
- 1 block
- Block 2
- Course capacity
- no limitation
The number of seats may be reduced in the late registration period
- Study Board of Physics, Chemistry and Nanoscience
- The Niels Bohr Institute
- Faculty of Science
- Troels Haugbølle (8-6a6377696471676e4270646b306d7730666d)