Cosmology

Standard candles are important for determining cosmological distances. Image credit: NASA
This course is an introduction to Cosmology. We follow the course book quite closely and first develop the basic description within Big Bang theory and general relativity to grasp the Friedmann equations required to calculate the evolution of the universe. We also target specific epochs in the universe, from early time Big Bang Nucleosynthesis to the Recombination era which released the Cosmic Microwave background. Inflation is mentioned rather briefly.
The course is given during day time, and is part of the Bachelor’s programme in Astronomy. It can also be taken as a free-standing course. The course is given in English.
Teaching Format
Lectures, exercise sessions for calculations and presentations by students.
Assessment
Written exam.
Examiner
Ragnhild Lunnan
Introduction to Cosmology, Barbara Ryden, Second edition, Cambridge University Press





