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Dark Matter in a twisted bottle
The real projective plane is a compact, non-orientable orbifold of Euler characteristic 1 without boundaries, which can be described as a twisted Klein bottle. We shortly review the motivations for choosing such a geometry among all possible two-dimensional orbifolds, while the main part of the stud...
Autores principales: | , , , |
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Lenguaje: | eng |
Publicado: |
2012
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1007/JHEP01(2013)147 http://cds.cern.ch/record/1482553 |
_version_ | 1780926001748901888 |
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author | Arbey, Alexandre Cacciapaglia, Giacomo Deandrea, Aldo Kubik, Bogna |
author_facet | Arbey, Alexandre Cacciapaglia, Giacomo Deandrea, Aldo Kubik, Bogna |
author_sort | Arbey, Alexandre |
collection | CERN |
description | The real projective plane is a compact, non-orientable orbifold of Euler characteristic 1 without boundaries, which can be described as a twisted Klein bottle. We shortly review the motivations for choosing such a geometry among all possible two-dimensional orbifolds, while the main part of the study will be devoted to dark matter study and limits in Universal Extra Dimensional (UED) models based on this peculiar geometry. In the following we consider such a UED construction based on the direct product of the real projective plane with the standard four-dimensional Minkowski space-time and discuss its relevance as a model of a weakly interacting Dark Matter candidate. One important difference with other typical UED models is the origin of the symmetry leading to the stability of the dark matter particle. This symmetry in our case is a remnant of the six-dimensional Minkowski space-time symmetry partially broken by the compactification. Another important difference is the very small mass splitting between the particles of a given Kaluza-Klein tier, which gives a very important role to co-annihilation effects. Finally the role of higher Kaluza-Klein tiers is also important and is discussed together with a detailed numerical description of the influence of the resonances. |
id | cern-1482553 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2012 |
record_format | invenio |
spelling | cern-14825532023-10-04T08:13:27Zdoi:10.1007/JHEP01(2013)147http://cds.cern.ch/record/1482553engArbey, AlexandreCacciapaglia, GiacomoDeandrea, AldoKubik, BognaDark Matter in a twisted bottleParticle Physics - PhenomenologyThe real projective plane is a compact, non-orientable orbifold of Euler characteristic 1 without boundaries, which can be described as a twisted Klein bottle. We shortly review the motivations for choosing such a geometry among all possible two-dimensional orbifolds, while the main part of the study will be devoted to dark matter study and limits in Universal Extra Dimensional (UED) models based on this peculiar geometry. In the following we consider such a UED construction based on the direct product of the real projective plane with the standard four-dimensional Minkowski space-time and discuss its relevance as a model of a weakly interacting Dark Matter candidate. One important difference with other typical UED models is the origin of the symmetry leading to the stability of the dark matter particle. This symmetry in our case is a remnant of the six-dimensional Minkowski space-time symmetry partially broken by the compactification. Another important difference is the very small mass splitting between the particles of a given Kaluza-Klein tier, which gives a very important role to co-annihilation effects. Finally the role of higher Kaluza-Klein tiers is also important and is discussed together with a detailed numerical description of the influence of the resonances.The real projective plane is a compact, non-orientable orbifold of Euler characteristic 1 without boundaries, which can be described as a twisted Klein bottle. We shortly review the motivations for choosing such a geometry among all possible two-dimensional orbifolds, while the main part of the study will be devoted to dark matter study and limits in Universal Extra Dimensional (UED) models based on this peculiar geometry. In the following we consider such a UED construction based on the direct product of the real projective plane with the standard four-dimensional Minkowski space-time and discuss its relevance as a model of a weakly interacting Dark Matter candidate. One important difference with other typical UED models is the origin of the symmetry leading to the stability of the dark matter particle. This symmetry in our case is a remnant of the six-dimensional Minkowski space-time symmetry partially broken by the compactification. Another important difference is the very small mass splitting between the particles of a given Kaluza-Klein tier, which gives a very important role to co-annihilation effects. Finally the role of higher Kaluza-Klein tiers is also important and is discussed together with a detailed numerical description of the influence of the resonances.arXiv:1210.0384LYCEN-2012-03CERN-PH-TH-2012-211LYCEN 2012-03CERN-PH-TH-2012-211oai:cds.cern.ch:14825532012-10-02 |
spellingShingle | Particle Physics - Phenomenology Arbey, Alexandre Cacciapaglia, Giacomo Deandrea, Aldo Kubik, Bogna Dark Matter in a twisted bottle |
title | Dark Matter in a twisted bottle |
title_full | Dark Matter in a twisted bottle |
title_fullStr | Dark Matter in a twisted bottle |
title_full_unstemmed | Dark Matter in a twisted bottle |
title_short | Dark Matter in a twisted bottle |
title_sort | dark matter in a twisted bottle |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1007/JHEP01(2013)147 http://cds.cern.ch/record/1482553 |
work_keys_str_mv | AT arbeyalexandre darkmatterinatwistedbottle AT cacciapagliagiacomo darkmatterinatwistedbottle AT deandreaaldo darkmatterinatwistedbottle AT kubikbogna darkmatterinatwistedbottle |