Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/104344
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Type: | Journal article |
Title: | All-flavour search for neutrinos from dark matter annihilations in the Milky Way with IceCube/DeepCore |
Author: | Aartsen, M.G. Abraham, K. Ackermann, M. Adams, J. Aguilar, J.A. Ahlers, M. Ahrens, M. Altmann, D. Andeen, K. Anderson, T. Ansseau, I. Anton, G. Archinger, M. Arguelles, C. Arlen, T.C. Auffenberg, J. Axani, S. Bai, X. Barwick, S.W. Baum, V. et al. |
Citation: | European Physical Journal C: Particles and Fields, 2016; 76(10):531-1-531-14 |
Publisher: | Springer-Verlag |
Issue Date: | 2016 |
ISSN: | 1434-6044 1434-6052 |
Statement of Responsibility: | M.G. Aartsen … G.C. Hill … S. Robertson … A. Wallace … B.J. Whelan … et al. (IceCube Collaboration) |
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 intrinsicallyworse angular resolution of cascades compared to muon tracks in IceCube. |
Description: | Published online: 28 September 2016 |
Rights: | © The Author(s) 2016. Open Access This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. |
DOI: | 10.1140/epjc/s10052-016-4375-3 |
Grant ID: | ARC |
Published version: | http://dx.doi.org/10.1140/epjc/s10052-016-4375-3 |
Appears in Collections: | Aurora harvest 8 Physics publications |
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hdl_104344.pdf | Published version | 1.44 MB | Adobe PDF | View/Open |
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