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dc.contributor.authorTrotta, Roberto-
dc.contributor.authorRuiz de Austri, Roberto-
dc.contributor.authorHeros, C. P. de los-
dc.date.issued2009-08-26-
dc.identifier.citationJournal of cosmology and astroparticle physics 8: 34 (2009)en_US
dc.identifier.issn1475-7516-
dc.identifier.uri10261/19745-
dc.description.abstractWe study in detail the ability of the nominal configuration of the IceCube neutrino telescope (with 80 strings) to probe the parameter space of the Constrained MSSM (CMSSM) favoured by current collider and cosmological data. Adopting conservative assumptions about the galactic halo model and the expected experiment performance, we find that IceCube has a probability between 2% and 12% of achieving a 5 sigma detection of dark matter annihilation in the Sun, depending on the choice of priors for the scalar and gaugino masses and on the astrophysical assumptions. We identify the most important annihilation channels in the CMSSM parameter space favoured by current constraints, and we demonstrate that assuming that the signal is dominated by a single annihilation channel can lead to large systematic errors in the inferred WIMP annihilation cross section. We demonstrate that similar to 66% of the CMSSM parameter space violates the equilibrium condition between capture and annihilation in the center of the Sun. By cross-correlating our predictions with direct detection methods, we conclude that if IceCube does detect a neutrino flux from the Sun at high significance while direct detection experiments do not find a signal above a spin-independent cross section sigma(SI)(p) greater than or similar to 7 x 10(-9) pb, the CMSSM will be strongly disfavoured, given standard astrophysical assumptions for the WIMP distribution. This result is robust with respect to a change of priors. We argue that the proposed low-energy DeepCore extension of IceCube will be an ideal instrument to focus on relevant CMSSM areas of parameter space.en_US
dc.description.sponsorshipThe authors would like to thank Tobias Bruch, Annika Peter and Timothy Sumner for useful conversations and suggestions. The work of R.R. has been supported in part by MEC (Spain) under grant FPA2007-60323, by Generalitat Valenciana under grant PROMETEO/2008/069 and by the Spanish Consolider-Ingenio 2010 Programme CPAN (CSD2007-00042). R.T. would like to thank the Galileo Galilei Institute for Theoretical Physics for the hospitality and the INFN and the EU FP6 Marie Curie Research and Training Network “UniverseNet” (MRTN-CT-2006-035863) for partial support. R.R. and R.T. would like to thank the European Network of Theoretical Astroparticle Physics ENTApP ILIAS/N6 under contract number RII3-CT-2004-506222 for financial support. The use of the “Ciclope” cluster of the IFT-UAM/CSIC is also acknowledged.en_US
dc.language.isoengen_US
dc.publisherInstitute of Physics Publishingen_US
dc.rightsopenAccessen_US
dc.subjectdark matter experimentsen_US
dc.subjectdark matter theoryen_US
dc.subjectneutrino detectorsen_US
dc.subjectneutrino astronomyen_US
dc.titleProspects for dark matter detection with IceCube in the context of the CMSSMen_US
dc.typeartículoen_US
dc.identifier.doi10.1088/1475-7516/2009/08/034-
dc.description.peerreviewedPeer revieweden_US
dc.relation.publisherversionhttp://dx.doi.org/10.1088/1475-7516/2009/08/034en_US
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