General Relativity is Einstein's theory of gravity. Here he shows that gravity should not be described as a force, as in Newton's theory, but as a consequence of spacetime curvature. This course is about this remarkable discovery.
The course begins by introducing the basic ideas behind the theory, such as the equivalence principle, how to describe curved spaces in terms of a metric, and the importance of special relativity as a locally valid theory. These insights are then used to study the Schwarzschild spacetime – the spacetime outside a spherically symmetric mass distribution, such as a planet, star or black hole. Thereafter we move on to the more mathematical parts of the theory, introducing tensors, the concept of parallel transport, the covariant derivative and the Riemann curvature tensor. After a discussion of the stress energy tensor we are then able to write down Einstein's equation, describing the connection between spacetime curvature and matter. In the last part of the course we discuss some important consequences of the theory, such as black holes, cosmology and gravitational waves.
This is an advanced level course given in half pace during daytime. It is recommended (but not mandatory) for the Master's programme in theoretical physics.
The teaching consists of lectures, problem solving sessions and assignments with feedback.
The examination consists of a written part and an oral part.
Course responsible and teacher:
Sören Holst, phone: 08-5537 8740, email: email@example.com
ScheduleThis is a preliminary schedule and is subject to continuous change. For this reason, we do not recommend print-outs. At the start of the course, your institution will advise where you can find your schedule during the course.
Course literatureNote that the course literature can be changed up to two months before the start of the course.
James B. Hartle: Gravity - an Introduction to Einstein's General Relativity (Addison Wesley 2003, ISBN: 0-8053-8662-9)
Academic advisor at the Department of Physics: