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Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Journal 01 Jun 2017Embargo end date: 01 Jan 2016 Netherlands, Australia, Spain, Netherlands, Italy, Spain, Italy, France, Spain, Italy, Italy, Italy, Italy, Italy, Spain, Italy Publisher:Elsevier BVJournal:Physics Letters B, volume 769, pages 249-254 (issn: 0370-2693, Copyright policy )Funded by:ANR | UnivEarthS, ANR | OCEVU, ANR | Amidex +1 projects
Authors: T. Grégoire; J. Carr; Steffen Hallmann; Alexis Coleiro; Thomas Eberl; C. Mueller; R. Bormuth; +127 Authors

doi: 10.1016/j.physletb.2017.03.063 , 10.48550/arxiv.1612.04595

arXiv: 1612.04595 , http://arxiv.org/abs/1612.04595

handle: 11588/931390 , 11368/3003310 , 11245.1/81e75cb2-1110-4da6-b013-86d1a851b51e , 11386/4781486 , 11573/951799 , 11567/865545 , 11591/464277 , 11585/585690 , 2117/105020 , 20.500.11937/57878

Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope

Abstract

Using data recorded with the ANTARES telescope from 2007 to 2015, a new search for dark matter annihilation in the Milky Way has been performed. Three halo models and five annihilation channels, $\rm WIMP + WIMP \to b \bar b, W^+ W^-, ��^+ ��^-, ��^{+} ��^{-}$ and $��\bar��$, with WIMP masses ranging from 50 $\frac{\text{GeV}}{\text{c}^2}$ to 100 $\frac{\text{TeV}}{\text{c}^2}$, were considered. No excess over the expected background was found, and limits on the thermally averaged annihilation cross--section were set.

6 pages, 6 figures submitted to Physics Letters B. Erratum accepted by Physics Letters B

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Netherlands, Australia, Spain, Netherlands, Italy, Spain, Italy, France, Spain, Italy, Italy, Italy, Italy, Italy, Spain, Italy
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Keywords

Astrofísica, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Nuclear and High Energy Physics, WIMP, QC1-999, FOS: Physical sciences, Astrophysics, Neutrino telescope, Energia fosca (Astronomia), 530, Dark matter, Àrees temàtiques de la UPC::Física::Astronomia i astrofísica, Neutrins, Neutrinos, Neutrino Telescope, Via Làctia, Galactic Centre, High Energy Astrophysical Phenomena (astro-ph.HE), ANTARES, Physics, ANTARES; Dark matter; Galactic Centre; Indirect detection; Neutrino telescope; WIMP; Nuclear and High Energy Physics, ANTARES; Dark matter; Galactic Centre; Indirect detection; Neutrino telescope; WIMP, Milky Way, Dark matter (Astronomy), FISICA APLICADA, :Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], Indirect detection, Matèria fosca (Astronomia), Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR.HE] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]

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citations
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BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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impulse
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