
(the WMAP [Wilkinson Microwave Anisotropy Probe] satellite, from the WMAP Home Page)
Physics 371 is a graduate-level introduction to cosmology, the study of the structure and evolution of the universe. As a post-candidacy 300-level course, it is appropriate for students in all specialties, with only standard first-year courses as prerequisites. The course will describe the basics of the standard Big-Bang model and some currently popular extensions thereof. Beginning with an overview of our observed universe, we will discuss the basics of relativistic cosmology, thermodynamics and relic abundances, scalar-field cosmology including dark energy and inflation, large-scale structure, and the cosmic microwave background.
Grading: The final grade will be based 50% on problem sets and 50% on a final paper. 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.
Here is the postscipt file for something handed out in class: A No-Nonsense Introduction to General Relativity.
Here are guidelines for the final paper (pdf).
And here, now that the course is over, are the actual final papers turned in by the students.
Classes will meet Tuesdays and Thursdays from 1:30 to 2:50 p.m.,
in Kersten 103.
The first day of class is Tuesday 28 March.
Proposals for the final papers are due in class on
Thursday May 4th. The papers themselves will be are due at noon on Friday,
June 2, in my office (RI262).
Sean Carroll, Professor
Jing Shu, Grader
Problem sets will be handed out
on Thursdays, due the following Thursday. Check the
messages page to see if there are
corrections or updates to the problem sets between when they are
handed out and when they are due. These are pdf files.
Click on the titles to see the
amazon.com
entry for each book. You can even buy them online if you like.
Here are some review articles you might find useful:
Dates
Personnel
Office: RI 262
Office Phone: 773/702-7635
Email: carroll [at] theory.uchicago.edu
Office Hours: after class, or as requested.
Email: jshu [at] uchicago.edu
Outline (subject to change)
Problem Sets
Books
This is the main text, although we won't follow it slavishly. It
provides a direct and accessible introduction to the most important
ideas in the toolbox of a working early-universe cosmologist. (Written
before the discovery of CMB anisotropies, the sections on perturbations
and structure are less up-to-date.)
More up-to-date than K&T, but burdened by an overwhelming amount of
preliminary material. A very useful reference.
An excellent and up-to-date book. Interested primarily in the evolution
of perturbations and CMB anisotropies, with a lot of GR-based calculations,
which is why we aren't using it for this course.
A focused introduction on cosmological perturbations, from their
origin in inflation to their observation as CMB anisotropies and
large-scale structure.
A comprehensive overview of numerous topics in physical cosmology.
("Physical" cosmology is, I think, supposed to distinguish the
down-to-earth style favored by astrophysicists from the speculative
flights of fancy indulged in by particle theorists.)
Dennis Overbye, Lonely Hearts of the Cosmos (Little, Brown
and Company, 1999).
Two great popular-level books on modern cosmology.
Other Resources
And here are links to some other relevant sites:
Sean M. Carroll
Enrico Fermi Institute
University of Chicago
5460 S. Ellis Ave.
Chicago, IL 60637
Office: 773/702-7635 Fax: 773/834-2222
carroll [at] theory.uchicago.edu