Chapters
- Observational
background
- Structure
formation via gravitational
instability
- linear
theory
- non-linear
evolution
- numerical
simulations.
- Statistical
description of density fluctuations
- random
fields
- power
spectrum and two-point correlation
function
- higher
order moments.
- Primordial
power spectrum, transfer function,
free streaming and the
cold-dark-matter (CDM) model
- Cosmological
parameters that describe the
inhomogeneous CDM universe.
Abstract
Bibliography
Any
standard textbook of cosmology will do.
Lecture slides include all the relevant
topics and specific references.
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