The compact stars - white dwarfs, neutron stars, and black holes - are the end state of stellar evolution. The conditions in and around these objects are extreme as compared to terrestrial standards, and they are responsible for some of the most powerful and dynamic phenomena in the universe. This course introduces the physics of strong gravity and dense matter required to understand compact stars and their observational manifestations.

Independent study of a topic of special interest to the student under individual supervision by a faculty member. May be repeated once for credit. Prerequisite: Instructor permission.

May be repeated once for credit. Prerequisite: Instructor permission.

This course covers topics associated with cosmology, the branch of astrophysics dealing with the origin and evolution of the Universe. The course begins with a historical overview and then focuses on three main areas: expansion of the universe, the early universe, and large-scale structure.

Under supervision, the student undertakes or assists with a current research problem. This course may be repeated for credit.

For doctoral dissertation, taken under the supervision of a dissertation director.