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, $\rm WIMP + WIMP \to b \bar b, W^+ W^-, \tau^+ \tau^-, \mu^{+} \mu^{-}$and$\nu \bar{\nu}$, 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.