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Antimatter signals of singlet scalar dark matter
We consider the singlet scalar model of dark matter and study the expected antiproton and positron signals from dark matter annihilations. The regions of the viable parameter space of the model that are excluded by present data are determined, as well as those regions that will be probed by the fort...
Autores principales: | , , |
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Formato: | info:eu-repo/semantics/article |
Lenguaje: | eng |
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2009
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Acceso en línea: | http://cds.cern.ch/record/1207015 |
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author | Goudelis, A Mambrini, Y Yaguna, C |
author_facet | Goudelis, A Mambrini, Y Yaguna, C |
author_sort | Goudelis, A |
collection | CERN |
description | We consider the singlet scalar model of dark matter and study the expected antiproton and positron signals from dark matter annihilations. The regions of the viable parameter space of the model that are excluded by present data are determined, as well as those regions that will be probed by the forthcoming experiment AMS-02. In all cases, different propagation models are investigated, and the possible enhancement due to dark matter substructures is analyzed. We find that the antiproton signal is more easily detectable than the positron one over the whole parameter space. For a typical propagation model and without any boost factor, AMS-02 will be able to probe --via antiprotons-- the singlet model of dark matter up to masses of 600 GeV. Antiprotons constitute, therefore, a promising signal to constraint or detect the singlet scalar model. |
format | info:eu-repo/semantics/article |
id | cern-1207015 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2009 |
record_format | invenio |
spelling | cern-12070152019-09-30T06:29:59Z http://cds.cern.ch/record/1207015 eng Goudelis, A Mambrini, Y Yaguna, C Antimatter signals of singlet scalar dark matter Particle Physics - Phenomenology We consider the singlet scalar model of dark matter and study the expected antiproton and positron signals from dark matter annihilations. The regions of the viable parameter space of the model that are excluded by present data are determined, as well as those regions that will be probed by the forthcoming experiment AMS-02. In all cases, different propagation models are investigated, and the possible enhancement due to dark matter substructures is analyzed. We find that the antiproton signal is more easily detectable than the positron one over the whole parameter space. For a typical propagation model and without any boost factor, AMS-02 will be able to probe --via antiprotons-- the singlet model of dark matter up to masses of 600 GeV. Antiprotons constitute, therefore, a promising signal to constraint or detect the singlet scalar model. info:eu-repo/grantAgreement/EC/FP7/237920 info:eu-repo/semantics/openAccess Education Level info:eu-repo/semantics/article http://cds.cern.ch/record/1207015 2009-09-16 |
spellingShingle | Particle Physics - Phenomenology Goudelis, A Mambrini, Y Yaguna, C Antimatter signals of singlet scalar dark matter |
title | Antimatter signals of singlet scalar dark matter |
title_full | Antimatter signals of singlet scalar dark matter |
title_fullStr | Antimatter signals of singlet scalar dark matter |
title_full_unstemmed | Antimatter signals of singlet scalar dark matter |
title_short | Antimatter signals of singlet scalar dark matter |
title_sort | antimatter signals of singlet scalar dark matter |
topic | Particle Physics - Phenomenology |
url | http://cds.cern.ch/record/1207015 http://cds.cern.ch/record/1207015 |
work_keys_str_mv | AT goudelisa antimattersignalsofsingletscalardarkmatter AT mambriniy antimattersignalsofsingletscalardarkmatter AT yagunac antimattersignalsofsingletscalardarkmatter |