Search for secluded dark matter towards the Galactic Centre with the ANTARES neutrino telescope
Creators: name: Albert, A.
name: Alves, S.
name: Andre, M.
name: Anghinolfi, M.
name: Anton, G.
name: Ardid, M.
name: Ardid, S.
name: Aubert, J.-J.
name: Aublin, J.
name: Baret, B.
name: Basa, S.
name: Belhorma, B.
name: Bendahman, M.
name: Benfenati, F.
name: Bertin, V.
name: Biagi, S.
name: Bissinger, M.
name: Boumaaza, J.
name: Bouta, M.
name: Bouwhuis, M. C.
name: Branzas, H.
name: Bruijn, R.
name: Brunner, J.
name: Busto, J.
name: Caiffi, B.
name: Calvo, D.
name: Capone, A.
name: Caramete, L.
name: Carr, J.
name: Carretero, V.
name: Celli, S.
name: Chabab, M.
name: Chau, T. N.
name: Cherkaoui El Moursli, R.
name: Chiarusi, T.
name: Circella, M.
name: Coleiro, A.
name: Coniglione, R.
name: Coyle, P.
name: Creusot, A.
name: Diaz, A. F.
name: de Wasseige, G.
name: Distefano, C.
name: Di Palma, I.
name: Domi, A.
name: Donzaud, C.
name: Dornic, D.
name: Drouhin, D.
name: Eberl, T.
name: van Eeden, T.
name: van Eijk, D.
name: Khayati, N. El
name: Enzenhoefer, A.
name: Fermani, P.
name: Ferrara, G.
name: Filippini, F.
name: Fusco, L.
name: Gatelet, Y.
name: Gay, P.
name: Glotin, H.
name: Gozzini, R.
name: Ruiz, R. Gracia
name: Graf, K.
name: Guidi, C.
name: Hallmann, S.
name: van Haren, H.
name: Heijboer, A. J.
name: Hello, Y.
name: Hernandez-Rey, J. J.
name: Hoessl, J.
name: Hofestaedt, J.
name: Huang, F.
name: Illuminati, G.
name: James, C. W.
name: Jisse-Jung, B.
name: de Jong, M.
name: de Jong, P.
name: Kadler, M.
name: Kalekin, O.
name: Katz, U.
name: Khan-Chowdhury, N. R.
name: Kouchner, A.
name: Kreykenbohm, I.
name: Kulikovskiy, V.
name: Gualda, C. Lagunas
name: Lahmann, R.
name: Breton, R. Le
name: LeStum, S.
name: Lefevre, D.
name: Leonora, E.
name: Levi, G.
name: Lincetto, M.
name: Lopez-Coto, D.
name: Loucatos, S.
name: Maderer, L.
name: Manczak, J.
name: Marcelin, M.
name: Margiotta, A.
name: Marinelli, A.
name: Martinez-Mora, J. A.
name: Martino, B.
name: Melis, K.
name: Migliozzi, P.
name: Moussa, A.
name: Muller, R.
name: Nauta, L.
name: Navas, S.
name: Nezri, E.
name: Fearraigh, B. O.
name: Paun, A.
name: Pavalas, G. E.
name: Pellegrino, C.
name: Perrin-Terrin, M.
name: Pestel, V.
name: Piattelli, P.
name: Pieterse, C.
name: Poire, C.
name: Popa, V.
name: Pradier, T.
name: Randazzo, N.
name: Real, D.
name: Reck, S.
name: Riccobene, G.
name: Romanov, A.
name: Sala, F.
name: Sanchez-Losa, A.
name: Salesa Greus, F.
name: Samtleben, D. F. E.
name: Sanguineti, M.
name: Sapienza, P.
name: Schnabel, J.
name: Schumann, J.
name: Schuessler, F.
name: Seneca, J.
name: Spurio, M.
name: Stolarczyk, Th.
name: Taiuti, M.
name: Tayalati, Y.
name: Tingay, S. J.
name: Vallage, B.
name: Van Elewyck, V.
name: Versari, F.
name: Viola, S.
name: Vivolo, D.
name: Wilms, J.
name: Zavatarelli, S.
name: Zegarelli, A.
name: Zornoza, J. D.
name: Zuniga, J.
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2022
Subjects: subject: 530
subject: dark matter: mass
subject: neutrino: detector
subject: neutrino: energy: high
subject: dark matter: annihilation
subject: up: mass
subject: scale: new physics
subject: cross section: annihilation
subject: TeV
subject: ANTARES
subject: unitarity
subject: mediation
subject: WIMP
subject: solids
subject: galaxy
subject: dark matter experiments
subject: neutrino experiments
subject: ultra high energy photons and neutrinos

description: Searches for dark matter (DM) have not provided any solid evidence for the existence of weakly interacting massive particles in the GeV-TeV mass range. Coincidentally, the scale of new physics is being pushed by collider searches well beyond the TeV domain. This situation strongly motivates the exploration of DM masses much larger than a TeV. Secluded scenarios contain a natural way around the unitarity bound on the DM mass, via the early matter domination induced by the mediator of its interactions with the Standard Model. High-energy neutrinos constitute one of the very few direct accesses to energy scales above a few TeV. An indirect search for secluded DM signals has been performed with the ANTARES neutrino telescope using data from 2007 to 2015. Upper limits on the DM annihilation cross section for DM masses up to 6 PeV are presented and discussed.