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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.authorAndeen, K.
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.authorBeattie, K.
dc.contributor.authorBeatty, J.
dc.contributor.authorBechet, S.
dc.contributor.authorBecker Tjus, J.
dc.contributor.authorBecker, K.
dc.contributor.authorBell, M.
dc.contributor.authorBenabderrahmane, M.
dc.contributor.authorBenzvi, S.
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.authorBindig, D.
dc.contributor.authorBissok, M.
dc.contributor.authorBlaufuss, E.
dc.contributor.authorBlumenthal, J.
dc.contributor.authorBoersma, D.
dc.contributor.authorBohm, C.
dc.contributor.authorBose, D.
dc.contributor.authorBöser, S.
dc.contributor.authorBotner, O.
dc.contributor.authorBrayeur, L.
dc.contributor.authorBrown, A.
dc.contributor.authorBruijn, R.
dc.contributor.authorBrunner, J.
dc.contributor.authorBuitink, S.
dc.contributor.authorCarson, Michael
dc.contributor.authorCasey, J.
dc.contributor.authorCasier, M.
dc.contributor.authorChirkin, D.
dc.contributor.authorChristy, B.
dc.contributor.authorClevermann, F.
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.authorDe Clercq, C.
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.authorDunkman, M.
dc.contributor.authorEagan, 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.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.authorFranke, R.
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.authorGoodman, J.
dc.contributor.authorGóra, D.
dc.contributor.authorGrant, D.
dc.contributor.authorGroß, A.
dc.contributor.authorGrullon, S.
dc.contributor.authorGurtner, M.
dc.contributor.authorHa, C.
dc.contributor.authorHaj Ismail, A.
dc.date.accessioned2017-01-30T12:55:13Z
dc.date.available2017-01-30T12:55:13Z
dc.date.created2016-01-18T20:00:42Z
dc.date.issued2013
dc.identifier.citationAbbasi, R. and Abdou, Y. and Ackermann, M. and Adams, J. and Aguilar, J. and Ahlers, M. and Altmann, D. et al. 2013. Search for relativistic magnetic monopoles with IceCube. Physical Review D - Particles, Fields, Gravitation and Cosmology. 87 (2).
dc.identifier.urihttp://hdl.handle.net/20.500.11937/26768
dc.identifier.doi10.1103/PhysRevD.87.022001
dc.description.abstract

We present the first results in the search for relativistic magnetic monopoles with the IceCube detector, a subsurface neutrino telescope located in the South Polar ice cap containing a volume of 1  km3. This analysis searches data taken on the partially completed detector during 2007 when roughly 0.2  km3 of ice was instrumented. The lack of candidate events leads to an upper limit on the flux of relativistic magnetic monopoles of Φ90%C.L.~3×10−18  cm−2 sr−1 s−1 for β ≥0.8. This is a factor of 4 improvement over the previous best experimental flux limits up to a Lorentz boost γ below 107. This result is then interpreted for a wide range of mass and kinetic energy values.

dc.titleSearch for relativistic magnetic monopoles with IceCube
dc.typeJournal Article
dcterms.source.volume87
dcterms.source.number2
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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