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dc.contributor.authorAbbasi, R.
dc.contributor.authorAbdou, Y.
dc.contributor.authorAbu-Zayyad, T.
dc.contributor.authorAdams, J.
dc.contributor.authorAguilar, J.
dc.contributor.authorAhlers, M.
dc.contributor.authorAndeen, K.
dc.contributor.authorAuffenberg, J.
dc.contributor.authorBai, X.
dc.contributor.authorBaker, M.
dc.contributor.authorBarwick, S.
dc.contributor.authorBay, R.
dc.contributor.authorBazo Alba, J.
dc.contributor.authorBeattie, K.
dc.contributor.authorBeatty, J.
dc.contributor.authorBechet, S.
dc.contributor.authorBecker, J.
dc.contributor.authorBecker, K.
dc.contributor.authorBenabderrahmane, M.
dc.contributor.authorBerdermann, J.
dc.contributor.authorBerghaus, P.
dc.contributor.authorBerley, D.
dc.contributor.authorBernardini, E.
dc.contributor.authorBertrand, D.
dc.contributor.authorBesson, D.
dc.contributor.authorBissok, M.
dc.contributor.authorBlaufuss, E.
dc.contributor.authorBoersma, D.
dc.contributor.authorBohm, C.
dc.contributor.authorBolmont, J.
dc.contributor.authorBotner, O.
dc.contributor.authorBradley, L.
dc.contributor.authorBraun, J.
dc.contributor.authorBreder, D.
dc.contributor.authorCarson, Michael
dc.contributor.authorCastermans, T.
dc.contributor.authorChirkin, D.
dc.contributor.authorChristy, B.
dc.contributor.authorClem, J.
dc.contributor.authorCohen, S.
dc.contributor.authorCowen, D.
dc.contributor.authorD'Agostino, M.
dc.contributor.authorDanninger, M.
dc.contributor.authorDay, C.
dc.contributor.authorDe Clercq, C.
dc.contributor.authorDemirörs, L.
dc.contributor.authorDepaepe, O.
dc.contributor.authorDescamps, F.
dc.contributor.authorDesiati, P.
dc.contributor.authorDe Vries-Uiterweerd, G.
dc.contributor.authorDeyoung, T.
dc.contributor.authorDíaz-Vélez, J.
dc.contributor.authorDreyer, J.
dc.contributor.authorDumm, J.
dc.contributor.authorDuvoort, M.
dc.contributor.authorEdwards, W.
dc.contributor.authorEhrlich, R.
dc.contributor.authorEisch, J.
dc.contributor.authorEllsworth, R.
dc.contributor.authorEngdegård, O.
dc.contributor.authorEuler, S.
dc.contributor.authorEvenson, P.
dc.contributor.authorFadiran, O.
dc.contributor.authorFazely, A.
dc.contributor.authorFeusels, T.
dc.contributor.authorFilimonov, K.
dc.contributor.authorFinley, C.
dc.contributor.authorFoerster, M.
dc.contributor.authorFox, B.
dc.contributor.authorFranckowiak, A.
dc.contributor.authorFranke, R.
dc.contributor.authorGaisser, T.
dc.contributor.authorGallagher, J.
dc.contributor.authorGanugapati, R.
dc.contributor.authorGerhardt, L.
dc.contributor.authorGladstone, L.
dc.contributor.authorGoldschmidt, A.
dc.contributor.authorGoodman, J.
dc.contributor.authorGozzini, R.
dc.contributor.authorGrant, D.
dc.contributor.authorGriesel, T.
dc.contributor.authorGroß, A.
dc.contributor.authorGrullon, S.
dc.contributor.authorGunasingha, R.
dc.contributor.authorGurtner, M.
dc.contributor.authorHa, C.
dc.contributor.authorHallgren, A.
dc.contributor.authorHalzen, F.
dc.contributor.authorHan, K.
dc.contributor.authorHanson, K.
dc.contributor.authorHasegawa, Y.
dc.contributor.authorHelbing, K.
dc.contributor.authorHerquet, P.
dc.contributor.authorHickford, S.
dc.contributor.authorHill, G.
dc.date.accessioned2017-01-30T11:32:46Z
dc.date.available2017-01-30T11:32:46Z
dc.date.created2016-09-12T08:37:02Z
dc.date.issued2010
dc.identifier.citationAbbasi, R. and Abdou, Y. and Abu-Zayyad, T. and Adams, J. and Aguilar, J. and Ahlers, M. and Andeen, K. et al. 2010. Limits on a muon flux from Kaluza-Klein dark matter annihilations in the Sun from the IceCube 22-string detector. Physical Review D - Particles, Fields, Gravitation and Cosmology. 81 (5).
dc.identifier.urihttp://hdl.handle.net/20.500.11937/12773
dc.identifier.doi10.1103/PhysRevD.81.057101
dc.description.abstract

A search for muon neutrinos from Kaluza-Klein dark matter annihilations in the Sun has been performed with the 22-string configuration of the IceCube neutrino detector using data collected in 104.3 days of live time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured lightest Kaluza-Klein particle (LKP) WIMPs in the Sun and converted to limits on the LKP-proton cross sections for LKP masses in the range 250-3000 GeV. These results are the most stringent limits to date on LKP annihilation in the Sun. © 2010 The American Physical Society.

dc.titleLimits on a muon flux from Kaluza-Klein dark matter annihilations in the Sun from the IceCube 22-string detector
dc.typeJournal Article
dcterms.source.volume81
dcterms.source.number5
dcterms.source.issn1550-7998
dcterms.source.titlePhysical Review D - Particles, Fields, Gravitation and Cosmology
curtin.departmentDepartment of Exploration Geophysics
curtin.accessStatusFulltext not available


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