Jorge L. Cervantes-Cota, George Smoot
This is a brief review of the standard model of cosmology. We first introduce
the FRW models and their flat solutions for energy fluids playing an important
role in the dynamics at different epochs. We then introduce different
cosmological lengths and some of their applications. The later part is
dedicated to the physical processes and concepts necessary to understand the
early and very early Universe and observations of it.
View original:
http://arxiv.org/abs/1107.1789
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