Home > Publications database > Erratum to: Search for annihilating dark matter in the Sun with 3 years of IceCube data > print

001     435008
005     20250729163401.0
024 7 _ |a 10.1140/epjc/s10052-019-6702-y
|2 doi
024 7 _ |a 1434-6044
|2 ISSN
024 7 _ |a 1434-6052
|2 ISSN
024 7 _ |a 10.3204/PUBDB-2020-00504
|2 datacite_doi
024 7 _ |a arXiv:1612.05949
|2 arXiv
024 7 _ |a altmetric:56727630
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024 7 _ |a inspire:1504897
|2 inspire
024 7 _ |a WOS:000460819300003
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024 7 _ |a openalex:W2920882095
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037 _ _ |a PUBDB-2020-00504
041 _ _ |a English
082 _ _ |a 530
088 1 _ |a arXiv:1612.05949
088 _ _ |a arXiv:1612.05949
|2 arXiv
100 1 _ |a Aartsen, M. G.
|0 INSPIRE-00266703
|b 0
245 _ _ |a Erratum to: Search for annihilating dark matter in the Sun with 3 years of IceCube data
260 _ _ |a Heidelberg
|c 2019
|b Springer
336 7 _ |a article
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336 7 _ |a Output Types/Journal article
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336 7 _ |a Report
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336 7 _ |a Journal Article
|b journal
|m journal
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|s 1580129684_23048
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336 7 _ |a ARTICLE
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336 7 _ |a JOURNAL_ARTICLE
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336 7 _ |a Journal Article
|0 0
|2 EndNote
500 _ _ |a Erratum: Eur.Phys.J. C79 3 (2019) 214 ; 10.1140/epjc/s10052-019-6702-y;
520 _ _ |a We 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.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF3-613)
|0 G:(DE-HGF)POF3-613
|c POF3-613
|f POF III
|x 0
588 _ _ |a Dataset connected to CrossRef
650 _ 7 |a dark matter: direct detection
|2 INSPIRE
650 _ 7 |a neutrino: detector
|2 INSPIRE
650 _ 7 |a atmosphere: background
|2 INSPIRE
650 _ 7 |a muon: atmosphere
|2 INSPIRE
650 _ 7 |a WIMP: mass
|2 INSPIRE
650 _ 7 |a IceCube
|2 INSPIRE
650 _ 7 |a scattering
|2 INSPIRE
650 _ 7 |a sensitivity
|2 INSPIRE
650 _ 7 |a statistics
|2 INSPIRE
650 _ 7 |a horizon
|2 INSPIRE
693 _ _ |0 EXP:(DE-H253)IceCube-20150101
|5 EXP:(DE-H253)IceCube-20150101
|e IceCube South Pole Neutrino Observatory
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