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All-flavour search for neutrinos from dark matter annihilations in the Milky Way with IceCube/DeepCore

  • Icecube Collaboration
  • Adelaide University
  • Technical University of Munich
  • German Electron Synchrotron
  • University of Canterbury
  • Université libre de Bruxelles
  • University of Wisconsin-Madison
  • Stockholm University
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Marquette University
  • Pennsylvania State University
  • Johannes Gutenberg University Mainz
  • Massachusetts Institute of Technology
  • RWTH Aachen University
  • South Dakota School of Mines & Technology
  • University of California at Irvine
  • University of California at Berkeley
  • Ohio State University
  • Ruhr University Bochum
  • University of Wuppertal
  • University of Rochester
  • Moscow Engineering Physics Institute
  • University of Maryland, College Park
  • University of Kansas
  • Lawrence Berkeley National Laboratory
  • Uppsala University
  • TU Dortmund University
  • Sungkyunkwan University
  • Vrije Universiteit Brussel
  • Georgia Institute of Technology

Research output: Contribution to journalArticlepeer-review

57 Scopus citations

Abstract

We present the first IceCube search for a signal of dark matter annihilations in the Milky Way using all-flavour neutrino-induced particle cascades. The analysis focuses on the DeepCore sub-detector of IceCube, and uses the surrounding IceCube strings as a veto region in order to select starting events in the DeepCore volume. We use 329 live-days of data from IceCube operating in its 86-string configuration during 2011–2012. No neutrino excess is found, the final result being compatible with the background-only hypothesis. From this null result, we derive upper limits on the velocity-averaged self-annihilation cross-section, ⟨ σAv ⟩ , for dark matter candidate masses ranging from 30 GeV up to 10 TeV, assuming both a cuspy and a flat-cored dark matter halo profile. For dark matter masses between 200 GeV and 10 TeV, the results improve on all previous IceCube results on ⟨ σAv ⟩ , reaching a level of 10- 23 cm3 s- 1, depending on the annihilation channel assumed, for a cusped NFW profile. The analysis demonstrates that all-flavour searches are competitive with muon channel searches despite the intrinsically worse angular resolution of cascades compared to muon tracks in IceCube.

Original languageEnglish
Article number531
JournalEuropean Physical Journal C
Volume76
Issue number10
DOIs
StatePublished - Oct 1 2016

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