Abstract
In these lectures we first concentrate on the cosmological problems which, hopefully, have to do with the new physics to be probed at the LHC: the nature and origin of dark matter and generation of matter-antimatter asymmetry. We give several examples showing the LHC cosmological potential. These are WIMPs as cold dark matter, gravitinos as warm dark matter, and electroweak baryogenesis as a mechanism for generating matter-antimatter asymmetry. In the remaining part of the lectures we discuss the cosmological perturbations as a tool for studying the epoch preceeding the conventional hot stage of the cosmological evolution.
Cite
CITATION STYLE
Rubakov, V. A. (2014). Cosmology. In 2011 European School of High-Energy Physics, ESHEP 2011 - Proceedings (pp. 151–195). CERN-European Organization for Nuclear Research. https://doi.org/10.7551/mitpress/13711.003.0009
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