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.
Rubakov, V A
[1]
- Moscow, INR (Russian Federation)
Citation Formats
Rubakov, V A.
Cosmology [2011 European School of High-Energy Physics].
CERN: N. p.,
2014.
Web.
Rubakov, V A.
Cosmology [2011 European School of High-Energy Physics].
CERN.
Rubakov, V A.
2014.
"Cosmology [2011 European School of High-Energy Physics]."
CERN.
@misc{etde_22548627,
title = {Cosmology [2011 European School of High-Energy Physics]}
author = {Rubakov, V A}
abstractNote = {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.}
place = {CERN}
year = {2014}
month = {Jul}
}
title = {Cosmology [2011 European School of High-Energy Physics]}
author = {Rubakov, V A}
abstractNote = {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.}
place = {CERN}
year = {2014}
month = {Jul}
}