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Multipole analysis of IceCube data to search for dark matter accumulated in the Galactic halo: IceCube Collaboration
Ist Teil von
The European physical journal. C, Particles and fields, 2015, Vol.75 (1), p.1-16, Article 20
Ort / Verlag
Berlin/Heidelberg: Springer Berlin Heidelberg
Erscheinungsjahr
2015
Quelle
Alma/SFX Local Collection
Beschreibungen/Notizen
Dark matter which is bound in the Galactic halo might self-annihilate and produce a flux of stable final state particles, e.g. high energy neutrinos. These neutrinos can be detected with IceCube, a cubic-kilometer sized Cherenkov detector. Given IceCube’s large field of view, a characteristic anisotropy of the additional neutrino flux is expected. In this paper we describe a multipole method to search for such a large-scale anisotropy in IceCube data. This method uses the expansion coefficients of a multipole expansion of neutrino arrival directions and incorporates signal-specific weights for each expansion coefficient. We apply the technique to a high-purity muon neutrino sample from the Northern Hemisphere. The final result is compatible with the null-hypothesis. As no signal was observed, we present limits on the self-annihilation cross-section averaged over the relative velocity distribution
⟨
σ
A
v
⟩
down to
1.9
×
10
-
23
cm
3
s
-
1
for a dark matter particle mass of 700–1,000 GeV and direct annihilation into
ν
ν
¯
. The resulting exclusion limits come close to exclusion limits from
γ
-ray experiments, that focus on the outer Galactic halo, for high dark matter masses of a few TeV and hard annihilation channels.