The purpose of this course is to provide a general overview of the observational basis for our modern view of cosmology. This course will include a significant discussion of the major tests used to establish the age of the universe; the Hubble constant; the dark matter, dark energy, and baryonic content of the universe; the matter power spectrum; and the ‘w’ parameter. This course is being designed to complement “Origin and Evolution of the Universe.”
The primary objectives of this course are for students to be learn the general observational techniques and physical principles for making a wide variety of inferences about the current state, evolution, and origin/age of the universe.
See MSc schedules
Mode of instruction
- Observational Cosmology, 2010, Stephen Serjeant (Cambridge University Press)
More information about signing up for your classes at the Faculty of Science can be found here
Exchange and Study Abroad students, please see the Prospective students website for information on how to apply.