Academic Team

Course Content

Type: Optional– PEC&AC Track – 3rd Trimester

Module A. Introduction. The Homogeneous Universe
The standard Cosmological Model. Cosmological parameters.
Problems of the Big Bang model.
The Inflationary solution.

Module B: The Non-Homogeneous Universe: Perturbations in the Matter Distribution
Linear theory of perturbation evolution in Friedmann universes.
Non-linear perturbation theory: Zeldovich approximation and N-body simulations.

Module C: Background Radiation
Propagation of a radiation field in an inhomogeneous Friedmann Universe.
Origin of anisotropies in the Background Radiation: Sachs-Wolfe effect, integrated Sachs-Wolfe effect.
Acoustic oscillations on the last scattering surface. Adiabatic and isocurvature modes.
Recent observations and implications for structure formation models. Cosmological parameters.
Sunyaev-Zeldovich effect: hot gas in clusters and secondary anisotropies in the background radiation.

Module D: Large-Scale Structure
Observations of matter distribution.
Statistical methods in Cosmology.
Measurement of the correlation function and power spectrum from galaxy catalogs.
Luminosity functions and mass functions. Comparison between simulations and observations.
Baryon acoustic oscillations in the galaxy distribution. Spectroscopic and photometric surveys.
Determination of cosmological parameters from large-scale structure.

Module E: Gravitational Lenses
History. Basic concepts.
Equations of gravitational lensing effect.
Strong and weak lenses.
Applications in Cosmology.

Reading List

Teaching Plan Information

Course Schedule