Department of Astronomy and Astrophysics
University of Chicago
Cosmic Microwave Background
MF 1:30-2:50 ERC 583
This course will have be composed of 2 parts. The first half will be lecture based with the goal of estabilishing a common denominator. The second half
will be more research based.
Requirement for this course is a final project to be presented in class.
Prerequisite for the course is graduate level cosmology and general relativity.
The H0 Tension Taylor Hoyt
Effect of Modified Gravity on CMB
How to Compute Primordial Non-Gaussianities Sam Passaglia
Making Next Generation CMB Detectors Amy Tang
Bayesian Statistics and the CMB Dimitrios Tanoglidis