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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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Lenguaje: | eng |
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2015
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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. |
id | cern-2008931 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2015 |
record_format | invenio |
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 |