Cosmology
3.0
creditsAverage Course Rating
Review of special relativity and an introduction to general relativity, Robertson-Walker metric, and Friedmann equation and solutions. Key transitions in the thermal evolution of the universe, including big bang nucleosynthesis, recombination, and reionization. The early universe (inflation), dark energy, dark matter, and the cosmic microwave background. Development of density perturbations, galaxy formation, and large-scale structure.
Fall 2014
Professor: Charles Bennett
Students appreciated that the course focused on a variety of interesting, yet relevant topics throughout the semester. Students were given the opportunity to learn about topics of their choice. Some students noted that there was a lack of feedback and heavy focus on the presentation. It was suggested that the course incorporate a different style of lecture to include presenters that are more versed on the given topic. Prospective students should know that little to no background is required, and the course is focused around a presentation.