Welcome to the Home Page for Physics 570

Spring, 2010
Monday and Wednesday, 5:30 - 7:00 PM , in Room 184

>
Albert Einstein (1879 - 1955)
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spacetime diagram
for two black holes
colliding to become one
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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 if they can be fitted into a one-semester course.
  The first third to half will focus primarily on the mathematics and basic structure of the theory, with relevant physical motivation and insight thrown in along the way, with the major applications coming after that.
  
Prerequisites:
I assume you have a good foundation in standard undergraduate physics: classical mechanics, electromagnetism, and the usual junior-level special relativity. Also you should have a mathematics background in 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 portion of the course learning the relevant differential geometry.
An extended/advanced course in special relativity is NOT necessary. Only the basic ideas of spacetime, 4-vectors, Minkowski diagrams, etc. are needed from special relativity; our time will mostly be concerned with questions involving gravitational fields in 4-dimensional spacetime.

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, 4 pages.
  1. Introduction and Conventions on Vectors, Tensors, and Matrices,     25 pages.
  2. Tangent Vectors and Differential Forms     32 pages.
  3. Important notes on Covariant Derivatives and Curvature; 40 pages.
  4. For the Sphere as a Manifold: Good Coordinate Charts, 5 pages, with figure, and their use to understand
    the Magnetic Vector Potential for a Magnetic Monopole, 12 pages, including the above on projective coordinates for the sphere.
    Then some by C.N. Yang on the Dirac constraint because of the existence of magnetic monopoles, 27 pages.
  5. Some notes on the Lorentz group and its subgroup, rotations in 3-space   27 pages.
  6. A discussion of Lie derivatives and Killing vectors; 11 pages.
  7. A summary of local properties of spherically symmetric, static spacetimes; 9 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. An invited paper on colliding(plane) gravitational waves by Valería Ferrari, presented at the 1989 conference of the Society for General Relativity and Gravitation (GRG), in Boulder, Colorado.
  13. Notes on Robertson-Walker Spacetimes: 7 pages.
  14. Collapsing Dust Metric, from Tolman [3 pages]
  15. 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 Jonathan Allen who may be found in class, if you need to set up an appointment to talk with him about grading questions.

Homework Assignments Due Date Homework Solutions
HW #1, due 27 Jan. Solutions for HW #1
HW #2, due 3 Febr. Solutions for HW #2
HW #3, due 10 Febr. Solutions for HW #3
HW #4 due 17 Febr. Solutions for HW #4
HW #5 due 24 Febr. Solutions for HW #5
HW #6 due 8 March (Monday) Solutions for HW #6
An Exam on 10 March, 2010 Solutions are available here.
HW #7 due 24 March. Solutions for HW #7
HW #8 due 7 April. Solutions for HW #8
HW #9 due 14 April. Solutions for HW #9
HW #10 due 21 April. Solutions for HW #10
An Exam on 28 April, 2010 Solutions are available here.
Usable Maple files are downloadable; they 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.
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 January, 2010