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Search for neutrinos from dark matter self-annihilations in the center of the Milky Way with 3 years of IceCube/DeepCore

dc.contributor.authorIceCube Collaboration
dc.contributor.authorKopper, S.
dc.contributor.authorNakarmi, P.
dc.contributor.authorPepper, J.A.
dc.contributor.authorToale, P.A.
dc.contributor.authorWilliams, D.R.
dc.contributor.otherRWTH Aachen University
dc.contributor.otherUniversity of Adelaide
dc.contributor.otherUniversity of Alaska System
dc.contributor.otherUniversity of Alaska Anchorage
dc.contributor.otherUniversity of Texas System
dc.contributor.otherUniversity of Texas Arlington
dc.contributor.otherClark Atlanta University
dc.contributor.otherUniversity System of Georgia
dc.contributor.otherGeorgia Institute of Technology
dc.contributor.otherSouthern University System
dc.contributor.otherSouthern University & A&M College
dc.contributor.otherUniversity of California System
dc.contributor.otherUniversity of California Berkeley
dc.contributor.otherUnited States Department of Energy (DOE)
dc.contributor.otherLawrence Berkeley National Laboratory
dc.contributor.otherHumboldt University of Berlin
dc.contributor.otherRuhr University Bochum
dc.contributor.otherUniversity of Wurzburg
dc.contributor.otherUniversite Libre de Bruxelles
dc.contributor.otherVrije Universiteit Brussel
dc.contributor.otherMassachusetts Institute of Technology (MIT)
dc.contributor.otherChiba University
dc.contributor.otherUniversity of Canterbury
dc.contributor.otherUniversity System of Maryland
dc.contributor.otherUniversity of Maryland College Park
dc.contributor.otherUniversity System of Ohio
dc.contributor.otherOhio State University
dc.contributor.otherUniversity of Copenhagen
dc.contributor.otherNiels Bohr Institute
dc.contributor.otherDortmund University of Technology
dc.contributor.otherMichigan State University
dc.contributor.otherUniversity of Alberta
dc.contributor.otherUniversity of Erlangen Nuremberg
dc.contributor.otherUniversity of Geneva
dc.contributor.otherGhent University
dc.contributor.otherUniversity of California Irvine
dc.contributor.otherUniversity of Kansas
dc.contributor.otherUniversity of Wisconsin System
dc.contributor.otherUniversity of Wisconsin Madison
dc.contributor.otherJohannes Gutenberg University of Mainz
dc.contributor.otherMarquette University
dc.contributor.otherUniversity of Mons
dc.contributor.otherTechnical University of Munich
dc.contributor.otherUniversity of Munster
dc.contributor.otherUniversity of Delaware
dc.contributor.otherYale University
dc.contributor.otherUniversity of Oxford
dc.contributor.otherDrexel University
dc.contributor.otherSouth Dakota School Mines & Technology
dc.contributor.otherUniversity of Rochester
dc.contributor.otherOskar Klein Centre
dc.contributor.otherStockholm University
dc.contributor.otherState University of New York (SUNY) System
dc.contributor.otherState University of New York (SUNY) Stony Brook
dc.contributor.otherSungkyunkwan University (SKKU)
dc.contributor.otherUniversity of Alabama Tuscaloosa
dc.contributor.otherPennsylvania Commonwealth System of Higher Education (PCSHE)
dc.contributor.otherPennsylvania State University
dc.contributor.otherPennsylvania State University - University Park
dc.contributor.otherUppsala University
dc.contributor.otherUniversity of Wuppertal
dc.contributor.otherHelmholtz Association
dc.contributor.otherDeutsches Elektronen-Synchrotron (DESY)
dc.contributor.otherUniversity of Tokyo
dc.date.accessioned2022-08-02T15:11:23Z
dc.date.available2022-08-02T15:11:23Z
dc.date.issued2017
dc.description.abstractWe present a search for a neutrino signal from dark matter self-annihilations in the Milky Way using the IceCube Neutrino Observatory (IceCube). In 1005 days of data we found no significant excess of neutrinos over the background of neutrinos produced in atmospheric air showers from cosmic ray interactions. We derive upper limits on the velocity averaged product of the dark matter self-annihilation cross section and the relative velocity of the dark matter particles \(\langle \sigma_A v\rangle\). Upper limits are set for dark matter particle candidate masses ranging from 10 GeV up to 1 TeV while considering annihilation through multiple channels. This work sets the most stringent limit on a neutrino signal from dark matter with mass between 10 and 100 GeV, with a limit of 1.18 · 10⁻²³ cm³ s⁻¹ for 100 GeV dark matter particles self-annihilating via τ⁺τ⁻ to neutrinos (assuming the Navarro-Frenk-White dark matter halo profile).en_US
dc.format.mimetypeapplication/pdf
dc.identifier.citationAartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Al Samarai, I., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Auffenberg, J., Axani, S., Bagherpour, H., Bai, X., Barron, J. P., Barwick, S. W., … Zoll, M. (2017). Search for neutrinos from dark matter self-annihilations in the center of the Milky Way with 3 years of IceCube/DeepCore. In The European Physical Journal C (Vol. 77, Issue 9). Springer Science and Business Media LLC. https://doi.org/10.1140/epjc/s10052-017-5213-y
dc.identifier.doi10.1140/epjc/s10052-017-5213-y
dc.identifier.orcidhttps://orcid.org/0000-0003-2740-9714
dc.identifier.urihttps://ir.ua.edu/handle/123456789/8665
dc.languageEnglish
dc.language.isoen_US
dc.publisherSpringer
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/
dc.subjectGAMMA-RAYS
dc.subjectPERFORMANCE
dc.subjectSPECTRUM
dc.subjectPhysics, Particles & Fields
dc.subjectPhysics
dc.titleSearch for neutrinos from dark matter self-annihilations in the center of the Milky Way with 3 years of IceCube/DeepCoreen_US
dc.typetext
dc.typeArticle

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