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Cosmology

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 ar...

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Autor principal: Rubakov, V.A.
Lenguaje:eng
Publicado: 2015
Materias:
Acceso en línea:https://dx.doi.org/10.5170/CERN-2014-003.151
http://cds.cern.ch/record/2008931
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author Rubakov, V.A.
author_facet Rubakov, V.A.
author_sort Rubakov, V.A.
collection CERN
description 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.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2015
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spelling cern-20089312022-08-10T20:12:25Zdoi:10.5170/CERN-2014-003.151http://cds.cern.ch/record/2008931engRubakov, V.A.CosmologyAstrophysics and AstronomyIn 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.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.arXiv:1504.03587oai:cds.cern.ch:20089312015-04-14
spellingShingle Astrophysics and Astronomy
Rubakov, V.A.
Cosmology
title Cosmology
title_full Cosmology
title_fullStr Cosmology
title_full_unstemmed Cosmology
title_short Cosmology
title_sort cosmology
topic Astrophysics and Astronomy
url https://dx.doi.org/10.5170/CERN-2014-003.151
http://cds.cern.ch/record/2008931
work_keys_str_mv AT rubakovva cosmology