Course syllabus
Course-PM
FFM071 / FIM450 FFM071 / FIM450 Gravitation and cosmology lp3 VT22 (7.5 hp)
This course is offered by the department of Physics.
The beginning of the course has been moved to January the 26th due to complications related to the covid-19 pandemic. The lectures scheduled for week 3 (4) will be recovered during week 6 (10).
Contact details
Examiner: Riccardo Catena. e-mail: catena@chalmers.se;
Student representatives:
Amanda Carlsson; amacar@student.chalmers.se
Elin Dufvenius Esping; delin@student.chalmers.se
Alicia Rey Alonso; aliciare@student.chalmers.se
Carl Henrik Rohdin; aranciohr@gmail.com
Linnea Ögren; linneaaogren@gmail.com
Course purpose
The purpose of the course is to introduce General Relativity to the student and then apply this theory to describe:
1) the dynamics of particles and electromagnetic fields in the presence of general gravitational fields;
2) gravitational waves
3) the evolution of our Universe
4) black holes
Schedule
Course literature
1) Main text book: "Gravitation and Cosmology", Steven Weinberg (Wiley 1972); available at Cremona
2) Lecture notes; available online at this webpage (see Course design section below)
3) Parts of chapters 5 and 6 from: "Spacetime and Geometry", Sean C. Carroll (Cambridge 2019); partly available on ArXiv as hep-th/9712019
Course design
The course is organised in 20 lectures of 1h and 45 min each (including a small break). Lectures will be held in FL64. The content of each lecture is specified below, where I also provide links to my notes.
Lecture 1 (pdf)
This lecture is primarily based on my notes and Chapters 1 and 3 (sections 3.1 and partly 3.2) from Weinberg's book. It focuses on:
The Principle of Relativity;
The Principle of Equivalence;
General Relativity as a theory of gravity.
Lecture 2 (pdf)
This lecture is based on Chapter 2 (sections 1 to 9) from Weinberg's book. It focuses on:
Lorentz transformations;
Lorentz Vectors and Tensors;
Particle Mechanics in Special Relativity
Electrodynamics in Special Relativity
Lecture 3 (pdf)
This lecture is based on my notes and Chapter 3 (sections 2 to 5) from Weinberg's book. It focuses on:
Locally inertial coordinate systems;
The geodesic equation;
Newtonian limit;
Gravitational redshift.
Lecture 4 (pdf)
This lecture is based on my notes and Chapter 4 (sections 2 to 7 and section 9) from Weinberg's book. It focuses on:
Tensors under general coordinate transformations;
Derivatives of tensors.
Lecture 5 (pdf)
This lecture is based on my notes and Chapters 4 (section 1) and 5 (sections 1 to 4) from Weinberg's book.
The Principle of General Covariance;
Particle Mechanics in General Relativity;
Electrodynamics in General Relativity;
Energy-momentum tensor;
Hydrodynamics and Hydrostatics in General Relativity.
Lecture 6 (pdf)
This lecture is based on my notes and Chapter 6 (sections 1 and 2 and 6 to 8) from Weinberg's book. It focuses on:
Riemann tensor - definition;
Riemann tensor - basic properties;
Lecture 7 (pdf)
This lecture is based on my notes and Chapter 6 (sections 3, 4 and 10) from Weinberg's book. It focuses on:
The equation of geodesic deviation;
Riemann tensor and gravitational fields;
Riemann tensor and non-Euclidean geometry;
Riemann tensor and the Principle of General Covariance.
Lecture 8 (pdf)
This lecture is based on my notes and Chapter 7 (sections 1 and 4 to 6) from Weinberg's book. It focuses on:
Einstein equations - derivation;
Einstein equations - solutions;
Einstein equations - nonlinearities.
Lecture 9 (pdf)
This lecture is based on my notes and Chapter 8 (section 1) from Weinberg's book. It focuses on:
Metric for a static and isotropic gravitational field;
Einstein equations in a static and isotropic gravitational field;
Harmonic coordinates.
Lecture 10 (pdf)
This lecture is based on my notes and Chapter 8 (sections 2 to 4) from Weinberg's book. It focuses on:
The Schwarzshild solution;
Eddington and Robertson corrections;
Geodesic equation in a static and isotropic gravitational field.
Lecture 11 (pdf)
This lecture is based on my notes and Chapter 8 (sections 5 to 7) from Weinberg's book. It focuses on:
The deflection of light by the sun;
Precession of perihelia;
Radar echo delay.
Lecture 12 (pdf)
This lecture is based on my notes and Chapter 10 (sections 1, 2 and part of section 4) from Weinberg's book. It focuses on:
The weak-field approximation;
Gravitational wave solutions - homogeneous case;
Gravitational wave solutions - inhomogeneous case.
Lecture 13 (pdf)
This lecture is based on my notes and Chapter 10 (sections 4 and 5) from Weinberg's book. It focuses on:
Energy loss by gravitational radiation;
Non-relativistic sources;
Detection of gravitational waves.
Lecture 14 (pdf)
This lecture is based on my notes and Chapter 12 (sections 1 to 4) from Weinberg's book. It focuses on:
The principle of least action;
The matter action and the energy-momentum tensor;
The gravitational action and Einstein equations.
Lecture 15 (pdf)
This lecture is based on my notes and Chapter 13 (sections 1 and 2) from Weinberg's book. It focuses on:
Killing vectors;
Homogeneous, isotropic and maximally symmetric spaces;
Spaces of constant curvature.
Lecture 16 (pdf)
This lecture is based on my notes and Chapter 13 (sections 2 to 5) from Weinberg's book. It focuses on:
The metric of maximally symmetric tensors;
Spaces with maximally symmetric subspaces;
Tensors in a maximally symmetric space.
Lecture 17 (pdf)
This lecture is based on my notes and Chapter 14 (sections 1 to 3) from Weinberg's book. It focuses on:
The Cosmological Principle;
The Robertson-Walker metric;
The cosmological red shift.
Lecture 18 (pdf)
This lecture is based on my notes and Chapter 15 (sections 1 to 3) from Weinberg's book. It focuses on:
Friedmann equation;
Luminosity distance in Friedmann models.
Lecture 19 (pdf)
This lecture is based on my notes and Chapter 5 from Carroll's book. It focuses on:
Schwarzshild geodesics revisited;
Schwarzshild black holes.
Lecture 20
In preparation for the oral exam, this lecture will be devoted to answering students's questions on the content of the course.
Changes made since the last occasion
The course will be taught in person.
Learning objectives and syllabus
During the course the student is expected to acquire a basic understanding of the concepts and principles of General Relativity and a working knowledge of the mathematics used in this field. Specifically, the student should be able to discuss and explain the physical ideas behind the phenomena described by Einstein's theory of gravity, General Relativity, and in a skilful way use the relevant mathematical methods in problem-solving.
Learning objectives:
- The Principle of Relativity: the role of coordinate transformations in Physics
- The Principle of Equivalence and why General Relativity is a theory of gravity
- The mathematical methods used in General Relativity, including tensor analysis
- Einstein's equations: how to derive and solve them
- Why the presence of matter and energy affects the geometry of spacetime
- The basic tests of General Relativity, such as the bending of light in a gravitational field
- Gravitational waves
- The role of General Relativity in Cosmology: maximally symmetric spaces
- The Cosmological Principle and its implications
- The standard Model of Cosmology
- Black holes
Examination form
The examination is divided into two mandatory parts (with grading weights given below):
1) Home problems (weight: 40%) to be published on Canvas. Each set of problems assigns 40 points. 20 points in each set are required to be admitted to the oral exam.
2) Oral exam (weight: 60%). It consists in a 10 minute-long blackboard presentation on a topic chosen by the student among the ones addressed in the course followed by 40 minutes of questions on the concepts and equations discussed in the course. The student will be asked to re-derive some of these equations on the blackboard.
Please register for the oral exam by using the link below:
Oral exams will be held in room Origo 4141
Course summary:
| Date | Details | Due |
|---|---|---|