Welcome to the Home Page for Physics 570

Spring, 2007
Tuesday and Thursday, 5:30 - 7:00 PM , in Room 184


Albert Einstein (1879 - 1955)

spacetime diagram
for two black holes
colliding to become one

Einstein with Tagore

First, an Advertisement for General Relativity:

Einstein's theory of general relativity is a classic example of a field theory:
    a theory describing the behavior of a field that exists at every point and every time, and its interactions.
General relativity can lay claim to (at least) three differences from most other field theories:
it is unique in that the equations of motion of particles through the field may be derived directly from the theory itself;
the field is in fact the curvature itself of the very points and times at which it is defined---via their tidal variations;
the field interacts with itself. [This is not quite unique since there are other (quantum) fields that also do this: Yang-Mills theories.]

Some reasonable understanding of this subject should actually be a part of the education of any professional physicist!
In addition, you can hardly even keep up with the Science pages of the New York Times if you don't understand the underpinnings of modern cosmological research.

This course will certainly not completely prepare you for research in this area: it will be an overview with insufficient depth for that purpose.
     However, that is more likely than not exactly what you wanted anyway.

General Introduction

The purpose of this class will be to learn the theory of general relativity, Einstein's theory of relativistic gravity, as well as some basic applications, including at least solar-system tests of gravitational theories, black holes, gravitational waves, and cosmology, with others possible, although unlikely since it is only a one-semester course. The first half will focus primarily on the mathematics and basic structure of the theory, with relevant physical motivation and insight thrown in along the way, but the main applications in the second half.
Prerequisites: I assume you have a good foundation in undergraduate physics, particularly in classical mechanics, electromagnetism, and special relativity, and a mathematics background in advanced calculus, differential equations, and linear algebra. The mathematics of general relativity is differential geometry, but I am not assuming you have had any: we will spend a good fraction of the first half learning the relevant differential geometry.

Textbooks and Syllabus:

Handouts to supplement the texts: parts of the course will follow these closely.
They are Acrobat-readable (*.pdf) files that you should print out, at appropriate times during the course of the class.

    0. A useful summary of the Lorentz transformations of several useful physical quantities.
  1. Introduction and Conventions on Vectors, Tensors, and Matrices,     26 pages.
  2. Tangent Vectors and Differential Forms     23 pages.
  3. For the Sphere as a Manifold: Good Coordinate Charts and their use to understand the Magnetic Vector Potential for a Magnetic Monopole.
    Then some by C.N. Yang on the Dirac constraint because of the existence of magnetic monopoles.
  4. Some (older) Notes on Rotations in 3-space   17 pages.
  5. Important notes on Covariant Derivatives and Curvature; 25 pages.
  6. A discussion of Lie derivatives and Killing vectors; 10 pages. It has been modified, yet again, on 23 Febr., 2007, hopefully to make things more clear.
  7. A summary of local properties of spherically symmetric, static spacetimes; 8 pages;
    and also some notes on the Kruskal extensions.
  8. Discussion of observations made by a uniformly accelerating observer; 15 pages.
  9. The Kerr metric, for rotating stellar objects: some rather brief listings of properties and equations; 4 pages.
  10. the important, original paper on rotating black holes:
    Rotating Black Holes: Locally Nonrotating frames, energy extraction, and scalar synchrotron radiation
    ,
    by James M. Bardeen, William H. Press, and Saul A. Teukolsky, The Astrophysical Journal, 178, 347-369 (1972).
  11. Notes on Spinors and their use to study Minkowski-signature manifolds: 33 pages
  12. Notes on Robertson-Walker Spacetimes: 7 pages.
  13. Collapsing Dust Metric, from Tolman [3 pages]
  14. Recent Discussions of Current State of Cosmology, by a practicing relativist: George Ellis:

Exams and Homework Assignments: There will be two "mid-term examinations" during the course of the semester, but no final examination.
In addition, there will be (more or less) weekly homework assignments, with solutions posted after they have been turned in.
The grader for the course is Steve Flammia, who can be emailed by clicking on the link just previous, and who will also have some office hours for the class.

Homework Assignments Due Date Homework Solutions
HW #1, due 1 Febr. Solutions for HW #1
HW #2, due 1 Febr. Solutions for HW #2
HW #3, due 8 Febr. Solutions for HW #3
HW #4 due 15 Febr. Solutions for HW #4
HW #5 due 22 Febr. Solutions for HW #5
An Exam on 1 March, 2007 Solutions are available here.
HW #6 due 8 March. Solutions for HW #6
HW #7 due 22 March. Solutions for HW #7 Webpage showing Maple Worksheet
Downloadable Maple Worksheet for Orbits
[See note below]
HW #8 due 29 March. Solutions for HW #8 Webpage showing Maple Worksheet
Downloadable Maple Worksheet for Orbits
[See note below]
HW #9 due 5 April. Solutions for HW #9
HW #10 due 12 April. Solutions for HW #10
HW #11 due 19 April. Solutions for HW #11
The Second Exam on Thursday, 26 April, 2007 Solutions to the main exam are available here;
Solutions to the bonus section are available here.
Downloadable files require a right-click on the link, and then choosing "Save link as ...".

Homework assignments and Solutions are pdf-files, except when occasionally there will be an html-file for a portion of the solutions.
Solutions will be made available once the assignments have been turned in.
Homework is DUE at the beginning of the class period on the due date!

There are many modern software packages to perform tensor calculations; some discussion of this is given at this website of John Baez. As he seems to think also, I prefer the program grtensor, which is described in more detail in this linked webpage. After you have a reasonably-good understanding of how the process works, I see no reason why you shouldn't have an algebraic computing system do the work for you.

Links to Worldwide Relativity Information Sites

Links to Exciting Astronomy News

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Last updated/modified: 4 December, 2006