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dc.contributor.authorAartsen, M.
dc.contributor.authorAbbasi, R.
dc.contributor.authorAbdou, Y.
dc.contributor.authorAckermann, M.
dc.contributor.authorAdams, J.
dc.contributor.authorAguilar, J.
dc.contributor.authorAhlers, M.
dc.contributor.authorAltmann, D.
dc.contributor.authorAuffenberg, J.
dc.contributor.authorBai, X.
dc.contributor.authorBaker, M.
dc.contributor.authorBarwick, S.
dc.contributor.authorBaum, V.
dc.contributor.authorBay, R.
dc.contributor.authorBeatty, J.
dc.contributor.authorBechet, S.
dc.contributor.authorBecker Tjus, J.
dc.contributor.authorBecker, K.
dc.contributor.authorBenabderrahmane, M.
dc.contributor.authorBenzvi, S.
dc.contributor.authorBerghaus, P.
dc.contributor.authorBerley, D.
dc.contributor.authorBernardini, E.
dc.contributor.authorBernhard, A.
dc.contributor.authorBertrand, D.
dc.contributor.authorBesson, D.
dc.contributor.authorBinder, G.
dc.contributor.authorBindig, D.
dc.contributor.authorBissok, M.
dc.contributor.authorBlaufuss, E.
dc.contributor.authorBlumenthal, J.
dc.contributor.authorBoersma, D.
dc.contributor.authorBohaichuk, S.
dc.contributor.authorBohm, C.
dc.contributor.authorBose, D.
dc.contributor.authorBöser, S.
dc.contributor.authorBotner, O.
dc.contributor.authorBrayeur, L.
dc.contributor.authorBretz, H.
dc.contributor.authorBrown, A.
dc.contributor.authorBruijn, R.
dc.contributor.authorBrunner, J.
dc.contributor.authorCarson, Michael
dc.contributor.authorCasey, J.
dc.contributor.authorCasier, M.
dc.contributor.authorChirkin, D.
dc.contributor.authorChristov, A.
dc.contributor.authorChristy, B.
dc.contributor.authorClark, K.
dc.contributor.authorClevermann, F.
dc.contributor.authorCoenders, S.
dc.contributor.authorCohen, S.
dc.contributor.authorCowen, D.
dc.contributor.authorCruz Silva, A.
dc.contributor.authorDanninger, M.
dc.contributor.authorDaughhetee, J.
dc.contributor.authorDavis, J.
dc.contributor.authorDay, M.
dc.contributor.authorDe Clercq, C.
dc.contributor.authorDe Ridder, S.
dc.contributor.authorDesiati, P.
dc.contributor.authorDe Vries, K.
dc.contributor.authorDe With, M.
dc.contributor.authorDeyoung, T.
dc.contributor.authorDíaz-Vélez, J.
dc.contributor.authorDunkman, M.
dc.contributor.authorEagan, R.
dc.contributor.authorEberhardt, B.
dc.contributor.authorEisch, J.
dc.contributor.authorEllsworth, R.
dc.contributor.authorEuler, S.
dc.contributor.authorEvenson, P.
dc.contributor.authorFadiran, O.
dc.contributor.authorFazely, A.
dc.contributor.authorFedynitch, A.
dc.contributor.authorFeintzeig, J.
dc.contributor.authorFeusels, T.
dc.contributor.authorFilimonov, K.
dc.contributor.authorFinley, C.
dc.contributor.authorFischer-Wasels, T.
dc.contributor.authorFlis, S.
dc.contributor.authorFranckowiak, A.
dc.contributor.authorFrantzen, K.
dc.contributor.authorFuchs, T.
dc.contributor.authorGaisser, T.
dc.contributor.authorGallagher, J.
dc.contributor.authorGerhardt, L.
dc.contributor.authorGladstone, L.
dc.contributor.authorGlüsenkamp, T.
dc.contributor.authorGoldschmidt, A.
dc.contributor.authorGolup, G.
dc.contributor.authorGonzalez, J.
dc.contributor.authorGoodman, J.
dc.contributor.authorGóra, D.
dc.contributor.authorGrandmont, D.
dc.contributor.authorGrant, D.
dc.date.accessioned2017-01-30T11:29:50Z
dc.date.available2017-01-30T11:29:50Z
dc.date.created2016-01-18T20:00:44Z
dc.date.issued2013
dc.identifier.citationAartsen, M. and Abbasi, R. and Abdou, Y. and Ackermann, M. and Adams, J. and Aguilar, J. and Ahlers, M. et al. 2013. IceCube search for dark matter annihilation in nearby galaxies and galaxy clusters. Physical Review D - Particles, Fields, Gravitation and Cosmology. 88 (12).
dc.identifier.urihttp://hdl.handle.net/20.500.11937/12296
dc.identifier.doi10.1103/PhysRevD.88.122001
dc.description.abstract

We present the results of a first search for self-annihilating dark matter in nearby galaxies and galaxy clusters using a sample of high-energy neutrinos acquired in 339.8 days of live time during 2009/10 with the IceCube neutrino observatory in its 59-string configuration. The targets of interest include the Virgo and Coma galaxy clusters, the Andromeda galaxy, and several dwarf galaxies. We obtain upper limits on the cross section as a function of the weakly interacting massive particle mass between 300 GeV and 100 TeV for the annihilation into bb¯, W+W−, τ+τ−, μ+μ−, and νν¯. A limit derived for the Virgo cluster, when assuming a large effect from subhalos, challenges the weakly interacting massive particle interpretation of a recently observed GeV positron excess in cosmic rays.

dc.titleIceCube search for dark matter annihilation in nearby galaxies and galaxy clusters
dc.typeJournal Article
dcterms.source.volume88
dcterms.source.number12
dcterms.source.issn1550-7998
dcterms.source.titlePhysical Review D - Particles, Fields, Gravitation and Cosmology
curtin.note

Copyright © 2013 by the American Physical Society

curtin.departmentDepartment of Exploration Geophysics
curtin.accessStatusOpen access


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