Spacetime and Black Holes (Physics 264)

Sean Carroll

Fall quarter, 2005

gvs-einstein

(simulation of image distortion by a black hole, from Werner Benger’s raytracing page)

Description

This course offers an introduction to general relativity, Einstein’s theory of gravitation, particularly as applied to black holes. After a review of special relativity and a discussion of the notion of four-dimensional spacetime, the basic tools of physics in a curved spacetime will be introduced (especially the metric tensor characterizing distances in spacetime, the generalization of partial derivatives to covariant derivatives, and the geodesic equation governing the motion of free particles). The Schwarzschild solution describing both black holes and the exteriors of stars and planets will be presented, and the behavior of objects in a Schwarzschild spacetime will be extensively studied. The course will conclude by introducing further mathematical tools (the Riemann tensor) and the dynamical equations relating energy/momentum to spacetime curvature (Einstein’s equations).

Prerequisites

In University-speak, the requirements are Physics 185 and either Math 204 or Math 221, or permission of the instructor. You should be familiar with basic mechanics, matrices, and partial differential equations, as well as special relativity. As everyone knows, general relativity involves a good deal of mathematics, especially differential geometry and tensor calculus. We will develop these tools as we go along, so no prior experience is necessary; more important will be a willingness to assimilate new concepts and notations and quickly put them to use (what is sometimes called “mathematical maturity”). Ambitious second-year students should be able to take the course, with the understanding that we will be introducing a substantial set of unfamiliar ideas.

Grading

The final grade will be based 60% on problem sets and 40% on a take-home final exam. You are encouraged to talk to your fellow students about the problem sets, but make sure that what you hand in is produced by you.

Dates and Times

The course will meet on Tuesdays and Thursdays, 12:00-1:20 p.m., in Kersten 105. There will also be a weekly recitation session led by the TA, Wednesdays at 5:30-6:30.

Personnel

Sean Carroll, Professor
Ishai Ben-Dov, Teaching Assistant

Outline

  • Introduction (Hartle chapters 1-3)
  • Special Relativity and Flat Spacetime (4-5)
  • Curvature of Spacetime (6-7)
  • Physics in Curved Spacetime (8)
  • The Schwarzschild Solution (9)
  • Black Holes (12-13)
  • Einstein’s Equation and Further Topics (20-22)

Problem Sets

Problem sets will be handed out on Thursdays, due the following Thursday. Sets are posted here in pdf.

Books

Click on the titles to see the amazon.com entry for each book. You can even buy them online if you like.

Other Resources

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