COSMOLOGIA FÍSICA 2025
LECTURE NOTES
Introduction
01: A physical model for the Universe
02: The Euclid mission
The Homogeneous Universe
03: The zeroth order Universe
04: The metric and its degrees of freedom
05: The cosmological fluid
06: The background evolution
The Inhomogeneous Universe
07: The density contrast random field
08: Statistical properties of the density contrast field
09: Parameterization of the density contrast field
Structure formation
10: Newtonian perturbed fluid equations
11: Dark matter linear clustering
12: Baryonic matter linear clustering
HOMEWORK