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000084124 088__ $$2arXiv$$aarXiv:0711.0353
000084124 1001_ $$aWikström, G.
000084124 1112_ $$0C07-07-03$$2inspire$$a30th International Cosmic Ray Conference$$cMerida$$d2007-07-03 - 2007-07-11$$gICRC2007$$wMexico
000084124 1101_ $$aDESY$$bStandort Zeuthen
000084124 245__ $$aProspect of Dark Matter Detection in IceCube
000084124 260__ $$aCiudad de Mexico$$bUniversidad Nacional Autonoma de Mexico$$c2007
000084124 300__ $$a135-138
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000084124 520__ $$aThe IceCube neutrino telescope, under construction at the South Pole, currently consists of 22 IceCube strings and 19 AMANDA strings.  Combining the two arrays leads to a large instrumented volume with AMANDA as a dense core, an ideal situation for indirect detection of WIMP dark matter annihilations in the Sun. From simulations we calculate the current detector’s sensitivity for solar WIMP neutrinos and find that it improves considerably compared to AMANDA-II. The improvement is due to a combination of reduced trigger thresholds and larger detector volume which permits the use of veto against muonic background.
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000084124 693__ $$0EXP:(DE-H253)IceCube-20150101$$5EXP:(DE-H253)IceCube-20150101$$eIceCube South Pole Neutrino Observatory$$x0
000084124 693__ $$0EXP:(DE-H253)AMANDA-20170101$$5EXP:(DE-H253)AMANDA-20170101$$eAntarctic Muon And Neutrino Detector Array$$x1
000084124 7001_ $$aIceCube Collaboration$$eCollaboration author
000084124 7870_ $$0PUBDB-2016-01641$$aCaballero, Rogelio et.al.$$dCiudad de Mexico : Universidad Nacional Autonoma de Mexico, 2007$$iIsPartOf$$rarXiv:0711.0353$$tProceedings, 30th International Cosmic Ray Conference (ICRC 2007)
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