This module aims to provide students with the essential concepts of the standard cosmological model, universe evolution, structure formation,
as well as composition, evolution, morphology and dynamics of galaxies.
Basics of the standard cosmological model, Frieddman equations, universe evolution, initial perturbations and their role in CMB fluctuations and large structure formation.
Fundamental aspects of the largest structures of the universe and of data analysis in cosmology.
Basic aspects of galaxy morphology and content, stellar evolution, and role of gaseous content of galaxies.
Chemical and dynamic evolution of galaxies. Rotation curves and their role in galactic mass determination.
Master in Particle Physics and Physics of the Cosmos