Astrophysical Processes (902F3)
15 credits, Level 7 (Masters)
This module covers:
- Basic properties of interstellar medium and intergalactic medium
- Radiative transfer
- Emission and absorption lines, line shapes
- Hyperfine transitions, 21-cm line of hydrogen
- Gunn-Peterson effect, Lyman-alpha forest, Damped Lyman Alpha systems
- Radiative heating and cooling processes
- Compton heating/cooling, Sunyaev-Zeldovich effect
- Emission by accelerating changes, retarded potentials, thermal bremstrahlung
- Applications of Special Relativity in Astrophysics, relativistic beaming
- Plasma effects, Faraday rotation, Synchrotron emission
- HII regions, re-ionization
By the end of the courses, you should be able to:
- Understand qualitatively the key physical phenomena occurring in the interstellar and intergalactic media and achieve basic familiarity with the relevant physical processes.
- Receive some initial exposure to the scientific research methods and current scientific literature, be able to critically read and summarize papers.
- Be able solve simple physical problems in the areas covered by the course.
33%: Practical (Workshop)
30%: Coursework (Problem Set)
70%: Examination (Unseen examination)
Contact hours and workload
This module is approximately 150 hours of work. This breaks down into about 33 hours of contact time and about 117 hours of independent study. The University may make minor variations to the contact hours for operational reasons, including timetabling requirements.
This module is running in the academic year 2020/21. We also plan to offer it in future academic years. It may become unavailable due to staff availability, student demand or updates to our curriculum. We’ll make sure to let our applicants know of such changes to modules at the earliest opportunity.
This module is offered on the following courses: