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@INPROCEEDINGS{Danninger:95922,
      author       = {Danninger, M. and Strahler, E. and DESY},
      collaboration = {{IceCube Collaboration}},
      title        = {{S}earches for {D}ark {M}atter {A}nnihilations in the {S}un
                      with {I}ce{C}ube and {D}eep{C}ore in the 79-string
                      {C}onfiguration},
      address      = {Beijing},
      publisher    = {Institute of Physics},
      reportid     = {PHPPUBDB-18954},
      pages        = {292},
      year         = {2011},
      abstract     = {Dark matter could be indirectly detected through the
                      observation of neutrinos produced as part of
                      itsself-annihilation process. Possible signatures are an
                      excess neutrino flux from the Sun, where dark matter could
                      begravitationally trapped. The recent commissioning of the
                      full DeepCore sub-array, a low-energy extension of
                      theIceCube neutrino observatory, offers exciting
                      opportunities for neutrino physics in the energy region of
                      10 GeV to 1 TeV.DeepCore’s improved energy reach will, in
                      particular, provide sensitivity to neutrinos from attractive
                      WIMP candidates,like the neutralino or the lightest
                      Kaluza-Klein particle (LKP), down to WIMP masses in the
                      region of about 50 GeV.This will lead to stringent upper
                      limits on the flux of muons from dark matter annihilations
                      in the Sun and constraints onWIMP-proton cross-sections. We
                      report on the search for dark matter annihilations in the
                      Sun with the IceCube neutrinodetector in the 79-string
                      configuration, which includes the full DeepCore sub-array.
                      Furthermore, we review the impactsof IceCube observations of
                      the Sun upon supersymmetric (SUSY) dark matter models.},
      month         = {Aug},
      date          = {2011-08-11},
      organization  = {32nd International Cosmic Ray
                       Conference, Beijing (China), 11 Aug
                       2011 - 18 Aug 2011},
      cin          = {ZNP(-2012)},
      cid          = {$I:(DE-H253)ZNP_-2012_-20130307$},
      pnm          = {52x - Programm Astroteilchenphysik - Topic unbekannt
                      (POF2-52x)},
      pid          = {G:(DE-HGF)POF2-52x},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)8},
      eprint       = {1111.2738},
      howpublished = {arXiv:1111.2738},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1111.2738;\%\%$},
      url          = {https://bib-pubdb1.desy.de/record/95922},
}