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

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To access the full text documents, please follow this link: http://hdl.handle.net/2117/105020

dc.contributor	Centre Tecnològic de Vilanova i la Geltrú
dc.contributor	Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
dc.contributor.author	Albert, A.
dc.contributor.author	André, Michel
dc.contributor.author	Anghinolfi, Marco
dc.contributor.author	Anton, G.
dc.date	2017-06-10
dc.identifier.citation	Albert, A., Andre, M., Anghinolfi, M., Anton, G. Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope. "Physics letters B", 10 Juny 2017, vol. 769, p. 249-254.
dc.identifier.citation	0370-2693
dc.identifier.citation	10.1016/j.physletb.2017.03.063
dc.identifier.uri	http://hdl.handle.net/2117/105020
dc.language.iso	eng
dc.publisher	Elsevier
dc.relation	http://www.sciencedirect.com/science/article/pii/S037026931730254X
dc.rights	Attribution-NonCommercial-NoDerivs 3.0 Spain
dc.rights	info:eu-repo/semantics/openAccess
dc.rights	http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subject	Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject	Dark matter (Astronomy)
dc.subject	Neutrinos
dc.subject	Astrophysics
dc.subject	Milky Way
dc.subject	Dark matter
dc.subject	WIMP
dc.subject	Indirect detection
dc.subject	Neutrino telescope
dc.subject	Galactic Centre
dc.subject	ANTARES
dc.subject	Via Làctia
dc.subject	Matèria fosca (Astronomia)
dc.subject	Energia fosca (Astronomia)
dc.subject	Astrofísica
dc.subject	Neutrins
dc.title	Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope
dc.type	info:eu-repo/semantics/publishedVersion
dc.type	info:eu-repo/semantics/article
dc.description.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, 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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