COSMOLOGIA FÍSICA 2026

LECTURE NOTES 

Introduction
00: Welcome
01: A physical model for the Universe

The Homogeneous Universe 
02: The zeroth order Universe 
03: The background dynamics
04: The concordance model

The Inhomogeneous Universe 
05: The density contrast
06: Statistical properties of the density contrast field I
07: Statistical properties of the density contrast field II
08: Parameterization of the density contrast field

Structure formation
09: Newtonian perturbed equations
10: Dark matter linear clustering
11: Baryonic matter linear clustering
12: Cosmic microwave background anisotropies
13: Relativistic perturbed equations

Cosmological probes
14: Supernova surveys

HOMEWORK 
HW1: due March 13th
HW2: due April 1st
HW3: due April 9th
HW4: due April 24th
HW5: due May 14th
HW6: due May 28th

TOPICS for the PRESENTATIONS
List of topics: presentations on July 7th

RESOURCES
Cosmology History (Baumann)
LCDM problems