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2017/18 Taught Postgraduate Module Catalogue

PHYS5390M General Relativity

15 creditsClass Size: 60

Module manager: Dr Stuart Lumsden
Email: s.l.lumsden@leeds.ac.uk

Taught: Semester 1 (Sep to Jan) View Timetable

Year running 2017/18

Pre-requisite qualifications

Level 2 Physics or equivalent

Module replaces

PHYS5160M

This module is not approved as an Elective

Objectives

At the end of this module, students should be able to:
- explain the physical and mathematical principles of general relativity;
- derive (or, in complex cases, describe the derivation of) equations governing spacetime geometry and the motion of particles in curved spacetimes;
- describe the geometrical structures of Schwarzschild and Robertson-Walker spacetimes and their physical interpretations;
- solve simple problems related to differential geometry and tensor calculus; particle motion and light propagation in Schwarzschild and Robertson-Walker spacetimes; the standard cosmological model.

Learning outcomes
Demonstrate an understanding of most fundamental laws and principles of physics, along with their application to a variety of areas in physics, some of which are at (or are informed by) the forefront of the discipline;
Solve advanced problems in physics using appropriate mathematical tools;
Use mathematical techniques and analysis to model physical behaviour and interpret mathematical descriptions of physical phenomena;
Communicate complex scientific ideas concisely, accurately and informatively;
Manage own learning and make use of appropriate texts, research articles and other primary sources.

Skills outcomes
Ability to solve physical problems using mathematics.
Ability to grasp a complex body of ideas.


Syllabus

Review of special relativity. Lorentz transformations; geometrical structure of Minkowski spacetime. Impossibility of describing gravitational forces.

Geometry of space and time. Spacetime as a differentiable manifold. Differential geometry and tensor calculus. Affine connection: parallel transport, covariant derivative, curvature, geodesics. Metric: definition of length and angle, metric connection.

General relativity I. Principle of equivalence. Motion of test particles in curved spacetime; Newtonian limit; gravitational forces.

General relativity II Effect of matter on spacetime geometry; Einstein's field equations; Newtonian limit; gravitational fields.

Gravitational effects of a spherical body. Schwarzschild solution. Meaning of distances and times. Tests of general relativity. Black holes.

Cosmology. Friedmann - Lemaitre models. The standard hot big bang model. The early universe

Teaching methods

Delivery typeNumberLength hoursStudent hours
Lecture221.0022.00
Private study hours128.00
Total Contact hours22.00
Total hours (100hr per 10 credits)150.00

Private study

Examples: 40 hours;
Exam preparation: 28 hours;
Reading and assimilation: 60 hours.

Opportunities for Formative Feedback

4 x homework assignments (not assessed)

Methods of assessment


Exams
Exam typeExam duration% of formal assessment
Standard exam (closed essays, MCQs etc)2 hr 30 mins100.00
Total percentage (Assessment Exams)100.00

Normally resits will be assessed by the same methodology as the first attempt, unless otherwise stated

Reading list

The reading list is available from the Library website

Last updated: 26/04/2017

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