TY - JOUR
T1 - Indirect Dark Matter Searches with the ANTARES and KM3NeT Neutrino Telescopes
AU - ANTARESy Collaborations
AU - KM3NeT Collaborations
AU - Albert, A.
AU - Alves, S.
AU - André, M.
AU - Anghinolfi, M.
AU - Anton, G.
AU - Ardid, M.
AU - Ardid, S.
AU - Aubert, J. J.
AU - Aublin, J.
AU - Baret, B.
AU - Basa, S.
AU - Belhorma, B.
AU - Bendahman, M.
AU - Bertin, V.
AU - Biagi, S.
AU - Bissinger, M.
AU - Boumaaza, J.
AU - Bouta, M.
AU - Bouwhuis, M. C.
AU - Brânzas, H.
AU - Bruijn, R.
AU - Brunner, J.
AU - Busto, J.
AU - Caiffi, B.
AU - Capone, A.
AU - Caramete, L.
AU - Carr, J.
AU - Carretero, V.
AU - Celli, S.
AU - Chabab, M.
AU - Chau, T. N.
AU - Cherkaoui El Moursli, R.
AU - Chiarusi, T.
AU - Circella, M.
AU - Coleiro, A.
AU - Colomer-Molla, M.
AU - Coniglione, R.
AU - Coyle, P.
AU - Creusot, A.
AU - Díaz, A. F.
AU - De Wasseige, G.
AU - Deschamps, A.
AU - Distefano, C.
AU - Domi, A.
AU - Donzaud, C.
AU - Dornic, D.
AU - Eberl, T.
AU - Van Eeden, T.
AU - Van Eijk, D.
AU - Razzaque, S.
N1 - Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)
PY - 2021
Y1 - 2021
N2 - Neutrino telescopes perform an indirect search for dark matter (DM) through its annihilation into standard model channels yielding neutrinos, for a broad range of WIMP masses. The ANTARES detector, anchored to the Mediterranean seabed at a depth of about 2500 m, looks for a DM signal from two promising neutrino sources from WIMP annihilation: the Galactic Center and the Sun. We present the latest results on ANTARES indirect detection in a wide range of WIMP masses and decay channels, and give a future prospect on sensitivities of DM searches with the KM3NeT detector, the next-generation neutrino telescope, currently under deployment in the Mediterranean Sea. These experiments have specific advantages, complementary to other detection strategies, and can provide a smoking-gun signal. The geographical location of ANTARES and KM3NeT is particularly well suited for searches in the Galactic Center, allowing for the world-best sensitivity for WIMP annihilation.
AB - Neutrino telescopes perform an indirect search for dark matter (DM) through its annihilation into standard model channels yielding neutrinos, for a broad range of WIMP masses. The ANTARES detector, anchored to the Mediterranean seabed at a depth of about 2500 m, looks for a DM signal from two promising neutrino sources from WIMP annihilation: the Galactic Center and the Sun. We present the latest results on ANTARES indirect detection in a wide range of WIMP masses and decay channels, and give a future prospect on sensitivities of DM searches with the KM3NeT detector, the next-generation neutrino telescope, currently under deployment in the Mediterranean Sea. These experiments have specific advantages, complementary to other detection strategies, and can provide a smoking-gun signal. The geographical location of ANTARES and KM3NeT is particularly well suited for searches in the Galactic Center, allowing for the world-best sensitivity for WIMP annihilation.
UR - http://www.scopus.com/inward/record.url?scp=85129452849&partnerID=8YFLogxK
M3 - Conference article
AN - SCOPUS:85129452849
SN - 1824-8039
VL - 398
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 174
T2 - 2021 European Physical Society Conference on High Energy Physics, EPS-HEP 2021
Y2 - 26 July 2021 through 30 July 2021
ER -