Chapitres

1. Observational background
2. Structure formation via gravitational instability
1. linear theory
2. non-linear evolution
3. numerical simulations.
3. Statistical description of density fluctuations
1. random fields
2. power spectrum and two-point correlation function
3. higher order moments.
4. Primordial power spectrum, transfer function, free streaming and the cold-dark-matter (CDM) model
5. Cosmological parameters that describe the inhomogeneous CDM universe.
   

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Résumé

Bibliographie

Any standard textbook of cosmology will do. Lecture slides include all the relevant topics and specific references.