Combined search for dark matter from the Galactic Centre with the ANTARES and IceCube neutrino telescopes

The ANTARES and IceCube neutrino telescopes have independently searched for neutrinos from dark matter pair-annihilation in the Galactic Centre, and placed limits on the velocity-averaged WIMP annihilation crosssection 〈σν〉. To date, the most stringent limits were obtained by the ANTARES neutrino te...

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Bibliographic Details
Published inEPJ Web of Conferences Vol. 207; p. 4007
Main Authors Gozzini, Sara Rebecca, Iovine, Nadège, Aguilar Sánchez, Juan Antonio, Baur, Sebastian, Zornoza Gómez, Juan de Dios
Format Journal Article Conference Proceeding
LanguageEnglish
Published Les Ulis EDP Sciences 2019
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Summary:The ANTARES and IceCube neutrino telescopes have independently searched for neutrinos from dark matter pair-annihilation in the Galactic Centre, and placed limits on the velocity-averaged WIMP annihilation crosssection 〈σν〉. To date, the most stringent limits were obtained by the ANTARES neutrino telescope for WIMP masses > 100 GeV/c 2 , closely followed by the limits of the IceCube experiment for WIMP masses up to 1 TeV/c 2 . Here we present the sensitivities of a combined search for dark matter in the Galactic Centre using data from both experiments in a WIMP mass range from 100 GeV/c 2 to 1 TeV/c 2 . This analysis includes IceCube data collected with the complete 86-strings detector from 2012 to 2015 and ANTARES data from 2007 to 2015. The two data sets were combined using a common likelihood framework, and before unblinding the combined sensitivities to 〈σν〉 are shown.
ISSN:2100-014X
2101-6275
2100-014X
DOI:10.1051/epjconf/201920704007