Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope
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, View the MathML source and View the MathML source, with WIMP masses ranging from View the MathML source t...
| Authors: | , , , |
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| Format: | article |
| Publication Date: | 2017 |
| Country: | España |
| Institution: | Universitat Politècnica de Catalunya (UPC) |
| Repository: | UPCommons. Portal del coneixement obert de la UPC |
| Language: | English |
| OAI Identifier: | oai:upcommons.upc.edu:2117/105020 |
| Online Access: | https://hdl.handle.net/2117/105020 https://dx.doi.org/10.1016/j.physletb.2017.03.063 |
| Access Level: | Open access |
| Keyword: | Dark matter (Astronomy) Neutrinos Astrophysics Milky Way Dark matter WIMP Indirect detection Neutrino telescope Galactic Centre ANTARES Via Làctia Matèria fosca (Astronomia) Energia fosca (Astronomia) Astrofísica Neutrins Àrees temàtiques de la UPC::Física::Astronomia i astrofísica |
| Summary: | 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, View the MathML source and View the MathML source, with WIMP masses ranging from View the MathML source to View the MathML source, were considered. No excess over the expected background was found, and limits on the thermally averaged annihilation cross-section were set. |
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