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Neutrino probes of the nature of light dark matter

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Neutrino probes of the nature of light dark matter

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dc.contributor.author Agarwalla, Sanjib Kumar
dc.contributor.author Blennow, Mattias
dc.contributor.author Fernández Martínez, Enrique
dc.contributor.author Mena Requejo, Olga
dc.date.accessioned 2014-09-11T07:57:48Z
dc.date.available 2014-09-11T07:57:48Z
dc.date.issued 2011
dc.identifier.citation Agarwalla, Sanjib Kumar Blennow, Mattias Fernández Martínez, Enrique Mena Requejo, Olga 2011 Neutrino probes of the nature of light dark matter Journal Of Cosmology And Astroparticle Physics 09 9 004
dc.identifier.uri http://hdl.handle.net/10550/37720
dc.description.abstract Dark matter particles gravitationally trapped inside the Sun may annihilate into Standard Model particles, producing a flux of neutrinos. The prospects of detecting these neutrinos in future multi-kt neutrino detectors designed for other physics searches are explored here. We study the capabilities of a 34/100 kt liquid argon detector and a 100 kt magnetized iron calorimeter detector. These detectors are expected to determine the energy and the direction of the incoming neutrino with unprecedented precision allowing for tests of the dark matter nature at very low dark matter masses, in the range of 10-25 GeV. By suppressing the atmospheric background with angular cuts, these techniques would be sensitive to dark matter-nucleon spin-dependent cross sections at the fb level, reaching down to a few ab for the most favorable annihilation channels and detector technology.
dc.language.iso eng
dc.relation.ispartof Journal Of Cosmology And Astroparticle Physics, 2011, vol. 09, num. 9, p. 004
dc.subject Física
dc.title Neutrino probes of the nature of light dark matter
dc.type journal article es_ES
dc.date.updated 2014-09-11T07:57:48Z
dc.identifier.doi 10.1088/1475-7516/2011/09/004
dc.identifier.idgrec 097560
dc.rights.accessRights open access es_ES

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