High Energy Astrophysics
If our eyes could see gravitational waves.... Image credit: NASA/C. Henze
In this course we will discuss a variety of “high-energy” phenomena that range from processes in compact binary systems over accretion onto black holes to the sources and detection of gravitational waves. Each time we begin by introducing (in some cases refreshing) the basic theoretical concepts, building a theoretical model and then confront the theoretical expectations with observations. The theoretical concepts contain elements from basic physics courses (e.g. classical mechanics or electrodynamics), gas dynamics and radiative processes. Knowledge in General Relativity is of course welcome, but not strictly needed for this course. The gravitational wave sources will be described by means of classical mechanics enhanced by additional effects. This course will allow you to apply fundamental physics concepts to understand some of the most violent events in the Universe.
The course is given during day time, and is part of the Master’s programme in Astronomy. The course is normally given in English.
Teacher
Evan O'Connor and Stephan Rosswog.
Correspondence via the course page in Athena.
Teaching Format
Instructions are given in the form of lectures (some on site, others via Zoom) and exercises. Participation in both lectures and exercises is mandatory.
Assessment
Assessment will be carried out during the course through exercises and a final, written exam. All exams and exercises are given in English.
Examiner
Evan O'Connor
Introduction to High-Energy Astrophysics av Rosswog and Brüggen, Cambridge University Press (2007).
Additional sources may be used for specific topics.
The academic advisor and student office can be contacted via studieinfo@astro.su.se.
