General Relativity
Full course description
General Relativity is the best theory of gravity that we have. It refines and supersedes the classical Newtonian theory of Universal Gravitation, and leads to many interesting and exotic predictions about the Universe and objects within it. In this course, we will build up the General Theory of Relativity, the relation between curved spacetimes and matter and energy, study the mathematics needed to do the necessary calculations, and apply it to some interesting cases. Among those are Schwarzschild black holes, Friedmann-Robertson-Walker Universes, and gravitational waves.
Course objectives
- To understand the theory of Special Relativity as a tensor theory;
- To reformulate gravity as curvature of spacetime;
- To understand tensor algebra as a mathematical apparatus;
- To be able to calculate spacetime curvature in the presence of mass and energy;
- To be able to calculate motion in curved spacetime;
- To understand black holes, cosmology, and gravitational waves as specific examples of thetheory learned.
Prerequisites
- PHY2001
- PHY3002
Co-requisites
- None
Recommended reading
- Lecture Notes by the lecturer (available as download);
- Recommended: “Gravity”, by James B. Hartle;
- Recommended: “Gravitation & Cosmology”, by Stephen Weinberg (note: this text is mathematically advanced).
PHY3006
Period 5
7 Apr 2025
6 Jun 2025
ECTS credits:
5.0Coordinator:
Teaching methods:
PBL, Work in subgroups, Skills, Lecture(s)Assessment methods:
Attendance, Written exam, Observation