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000435008 005__ 20250729163401.0
000435008 0247_ $$2doi$$a10.1140/epjc/s10052-019-6702-y
000435008 0247_ $$2ISSN$$a1434-6044
000435008 0247_ $$2ISSN$$a1434-6052
000435008 0247_ $$2datacite_doi$$a10.3204/PUBDB-2020-00504
000435008 0247_ $$2arXiv$$aarXiv:1612.05949
000435008 0247_ $$2altmetric$$aaltmetric:56727630
000435008 0247_ $$2inspire$$ainspire:1504897
000435008 0247_ $$2WOS$$aWOS:000460819300003
000435008 0247_ $$2openalex$$aopenalex:W2920882095
000435008 037__ $$aPUBDB-2020-00504
000435008 041__ $$aEnglish
000435008 082__ $$a530
000435008 0881_ $$aarXiv:1612.05949
000435008 088__ $$2arXiv$$aarXiv:1612.05949
000435008 1001_ $$0INSPIRE-00266703$$aAartsen, M. G.$$b0
000435008 245__ $$aErratum to: Search for annihilating dark matter in the Sun with 3 years of IceCube data
000435008 260__ $$aHeidelberg$$bSpringer$$c2019
000435008 3367_ $$2DRIVER$$aarticle
000435008 3367_ $$2DataCite$$aOutput Types/Journal article
000435008 3367_ $$0PUB:(DE-HGF)29$$2PUB:(DE-HGF)$$aReport$$mreport
000435008 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1580129684_23048
000435008 3367_ $$2BibTeX$$aARTICLE
000435008 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000435008 3367_ $$00$$2EndNote$$aJournal Article
000435008 500__ $$aErratum: Eur.Phys.J. C79 3 (2019) 214 ; 10.1140/epjc/s10052-019-6702-y;
000435008 520__ $$aWe present results from an analysis looking for dark matter annihilation in the Sun with the IceCube neutrino telescope. Gravitationally trapped dark matter in the Sun’s core can annihilate into Standard Model particles making the Sun a source of  GeV neutrinos. IceCube is able to detect neutrinos with energies >100 GeV while its low-energy infill array DeepCore extends this to >10 GeV. This analysis uses data gathered in the austral winters between May 2011 and May 2014, corresponding to 532 days of livetime when the Sun, being below the horizon, is a source of up-going neutrino events, easiest to discriminate against the dominant background of atmospheric muons. The sensitivity is a factor of two to four better than previous searches due to additional statistics and improved analysis methods involving better background rejection and reconstructions. The resultant upper limits on the spin-dependent dark matter-proton scattering cross section reach down to $1.46\times 10^{-5}$  pb for a dark matter particle of mass 500 GeV annihilating exclusively into $\tau ^{+}\tau ^{-}$ particles. These are currently the most stringent limits on the spin-dependent dark matter-proton scattering cross section for WIMP masses above 50 GeV.
000435008 536__ $$0G:(DE-HGF)POF3-613$$a613 - Matter and Radiation from the Universe (POF3-613)$$cPOF3-613$$fPOF III$$x0
000435008 588__ $$aDataset connected to CrossRef
000435008 650_7 $$2INSPIRE$$adark matter: direct detection
000435008 650_7 $$2INSPIRE$$aneutrino: detector
000435008 650_7 $$2INSPIRE$$aatmosphere: background
000435008 650_7 $$2INSPIRE$$amuon: atmosphere
000435008 650_7 $$2INSPIRE$$aWIMP: mass
000435008 650_7 $$2INSPIRE$$aIceCube
000435008 650_7 $$2INSPIRE$$ascattering
000435008 650_7 $$2INSPIRE$$asensitivity
000435008 650_7 $$2INSPIRE$$astatistics
000435008 650_7 $$2INSPIRE$$ahorizon
000435008 693__ $$0EXP:(DE-H253)IceCube-20150101$$5EXP:(DE-H253)IceCube-20150101$$eIceCube South Pole Neutrino Observatory$$x0
000435008 7001_ $$0P:(DE-H253)PIP1014130$$aAckermann, M.$$b1
000435008 7001_ $$0INSPIRE-00324614$$aAdams, J.$$b2
000435008 7001_ $$0INSPIRE-00383940$$aAguilar, J. A.$$b3
000435008 7001_ $$0INSPIRE-00324621$$aAhlers, M.$$b4
000435008 7001_ $$aAhrens, M.$$b5
000435008 7001_ $$0INSPIRE-00479170$$aAltmann, D.$$b6
000435008 7001_ $$0INSPIRE-00324637$$aAndeen, K.$$b7
000435008 7001_ $$aAnderson, T.$$b8
000435008 7001_ $$aAnsseau, I.$$b9
000435008 7001_ $$aAnton, G.$$b10
000435008 7001_ $$aArchinger, M.$$b11
000435008 7001_ $$0INSPIRE-00350180$$aArgüelles, C.$$b12
000435008 7001_ $$0INSPIRE-00324642$$aAuffenberg, J.$$b13
000435008 7001_ $$0INSPIRE-00479204$$aAxani, S.$$b14
000435008 7001_ $$0INSPIRE-00324657$$aBai, X.$$b15
000435008 7001_ $$0INSPIRE-00324671$$aBarwick, S. W.$$b16
000435008 7001_ $$0INSPIRE-00479210$$aBaum, V.$$b17
000435008 7001_ $$0INSPIRE-00065262$$aBay, R.$$b18
000435008 7001_ $$0INSPIRE-00065336$$aBeatty, J. J.$$b19
000435008 7001_ $$0INSPIRE-00479225$$aBecker Tjus, J.$$b20
000435008 7001_ $$0INSPIRE-00149717$$aBecker, K.-H.$$b21
000435008 7001_ $$0INSPIRE-00148267$$aBenZvi, S.$$b22
000435008 7001_ $$0INSPIRE-00324725$$aBerley, D.$$b23
000435008 7001_ $$0P:(DE-H253)PIP1003794$$aBernardini, E.$$b24
000435008 7001_ $$0INSPIRE-00245670$$aBernhard, A.$$b25
000435008 7001_ $$0INSPIRE-00324734$$aBesson, D. Z.$$b26
000435008 7001_ $$0INSPIRE-00479238$$aBinder, G.$$b27
000435008 7001_ $$0INSPIRE-00264119$$aBindig, D.$$b28
000435008 7001_ $$0INSPIRE-00324747$$aBissok, M.$$b29
000435008 7001_ $$0INSPIRE-00067417$$aBlaufuss, E.$$b30
000435008 7001_ $$aBlot, S.$$b31
000435008 7001_ $$0INSPIRE-00324763$$aBohm, C.$$b32
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000435008 7001_ $$aBos, F.$$b34
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000435008 7001_ $$0INSPIRE-00326506$$aBöser, S.$$b36
000435008 7001_ $$0INSPIRE-00068476$$aBotner, O.$$b37
000435008 7001_ $$0INSPIRE-00324783$$aBraun, J.$$b38
000435008 7001_ $$0INSPIRE-00479240$$aBrayeur, L.$$b39
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000435008 7001_ $$aBurgman, A.$$b42
000435008 7001_ $$aCarver, T.$$b43
000435008 7001_ $$0INSPIRE-00479293$$aCasier, M.$$b44
000435008 7001_ $$aCheung, E.$$b45
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000435008 7001_ $$0INSPIRE-00212595$$aChristov, A.$$b47
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000435008 7001_ $$0INSPIRE-00074241$$aConrad, J. M.$$b52
000435008 7001_ $$0INSPIRE-00074832$$aCowen, D. F.$$b53
000435008 7001_ $$aCross, R.$$b54
000435008 7001_ $$aDay, M.$$b55
000435008 7001_ $$ade André, J. P. A. M.$$b56
000435008 7001_ $$0INSPIRE-00324889$$aDe Clercq, C.$$b57
000435008 7001_ $$adel Pino Rosendo, E.$$b58
000435008 7001_ $$0INSPIRE-00150573$$aDembinski, H.$$b59
000435008 7001_ $$0INSPIRE-00479339$$aDe Ridder, S.$$b60
000435008 7001_ $$0INSPIRE-00324924$$aDesiati, P.$$b61
000435008 7001_ $$0INSPIRE-00150514$$ade Vries, K. D.$$b62
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000435008 7001_ $$0INSPIRE-00479340$$ade With, M.$$b64
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000435008 7001_ $$0INSPIRE-00150592$$aDíaz-Vélez, J. C.$$b66
000435008 7001_ $$adi Lorenzo, V.$$b67
000435008 7001_ $$aDujmovic, H.$$b68
000435008 7001_ $$0INSPIRE-00324945$$aDumm, J. P.$$b69
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000435008 7001_ $$0INSPIRE-00479378$$aEberhardt, B.$$b71
000435008 7001_ $$aEhrhardt, T.$$b72
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000435008 7001_ $$aHignight, J.$$b111
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000435008 7001_ $$0INSPIRE-00479524$$aHuang, F.$$b116
000435008 7001_ $$aHuber, M.$$b117
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000435008 7001_ $$aMahn, K. B. M.$$b169
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000435008 7001_ $$0INSPIRE-00325675$$aMontaruli, T.$$b184
000435008 7001_ $$aMoulai, M.$$b185
000435008 7001_ $$0P:(DE-H253)PIP1003726$$aNahnhauer, R.$$b186
000435008 7001_ $$0INSPIRE-00240770$$aNaumann, U.$$b187
000435008 7001_ $$aNeer, G.$$b188
000435008 7001_ $$0INSPIRE-00479692$$aNiederhausen, H.$$b189
000435008 7001_ $$0INSPIRE-00479701$$aNowicki, S. C.$$b190
000435008 7001_ $$0INSPIRE-00112225$$aNygren, D. R.$$b191
000435008 7001_ $$0INSPIRE-00479718$$aObertacke Pollmann, A.$$b192
000435008 7001_ $$0INSPIRE-00325724$$aOlivas, A.$$b193
000435008 7001_ $$0INSPIRE-00263446$$aO'Murchadha, A.$$b194
000435008 7001_ $$0INSPIRE-00370808$$aPalczewski, T.$$b195
000435008 7001_ $$aPandya, H.$$b196
000435008 7001_ $$aPankova, D. V.$$b197
000435008 7001_ $$aPeiffer, P.$$b198
000435008 7001_ $$aPenek, Ö.$$b199
000435008 7001_ $$0INSPIRE-00479731$$aPepper, J. A.$$b200
000435008 7001_ $$0INSPIRE-00089886$$aPérez de los Heros, C.$$b201
000435008 7001_ $$0INSPIRE-00325791$$aPieloth, D.$$b202
000435008 7001_ $$0INSPIRE-00479759$$aPinat, E.$$b203
000435008 7001_ $$0INSPIRE-00117727$$aPrice, P. B.$$b204
000435008 7001_ $$0INSPIRE-00325845$$aPrzybylski, G. T.$$b205
000435008 7001_ $$0INSPIRE-00479763$$aQuinnan, M.$$b206
000435008 7001_ $$aRaab, C.$$b207
000435008 7001_ $$0INSPIRE-00479777$$aRädel, L.$$b208
000435008 7001_ $$0INSPIRE-00479787$$aRameez, M.$$b209$$eCorresponding author
000435008 7001_ $$0INSPIRE-00325859$$aRawlins, K.$$b210
000435008 7001_ $$0INSPIRE-00479790$$aReimann, R.$$b211
000435008 7001_ $$aRelethford, B.$$b212
000435008 7001_ $$aRelich, M.$$b213
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000435008 7001_ $$0INSPIRE-00479801$$aRichman, M.$$b216
000435008 7001_ $$0INSPIRE-00479813$$aRiedel, B.$$b217
000435008 7001_ $$0INSPIRE-00479826$$aRobertson, S.$$b218
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000435008 7001_ $$aSandrock, A.$$b226
000435008 7001_ $$aSandroos, J.$$b227
000435008 7001_ $$0INSPIRE-00123274$$aSarkar, S.$$b228
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000435008 7001_ $$aStettner, J.$$b243
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000435008 7001_ $$0INSPIRE-00129085$$aStokstad, R. G.$$b246
000435008 7001_ $$aStößl, A.$$b247
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