Indirect dark matter searches with neutrinos from the Galactic Centre region with the ANTARES and KM3NeT telescopes

Albert, A.; Alves, S.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Ardid, S.; Aubert, J. -J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bendahman, M.; Bertin, V.; Biagi, S.; Bissinger, M.; Boumaaza, J.; Bouta, M.; Bouwhuis, M. C.; Branzas, H.; Bruijn, R.; Brunner, J.; Busto, J.; Caiffi, B.; Capone, A.; Caramete, L.; Carr, J.; Carretero, V.; Celli, S.; Chabab, M.; Chau, T. N.; Cherkaoui El Moursli, R.; Chiarusi, T.; Circella, M.; Coleiro, A.; Colomer-Molla, M.; Coniglione, R.; Coyle, P.; Creusot, A.; Diaz, A. F.; de Wasseige, G.; Deschamps, A.; Distefano, C.; Di Palma, I.; Domi, A.; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; van Eeden, T.; van Eijk, D.; El Khayati, N.; Enzenhofer, A.; Fermani, P.; Ferrara, G.; Filippini, F.; Fusco, L. A.; Gatelet, Y.; Gay, P.; Glotin, H.; Gozzini, R.; Gracia Ruiz, R.; Graf, K.; Guidi, C.; Hallmann, S.; van Haren, H.; Heijboer, A. J.; Hello, Y.; Hernandez-Rey, J. J.; Hossl, J.; Hofestadt, J.; Huang, F.; Illuminati, G.; James, C. W.; Jisse-Jung, B.; de Jong, M.; de Jong, P.; Kadler, M.; Kalekin, O.; Katz, U.; Khan-Chowdhury, N. R.; Kouchner, A.; Kreykenbohm, I.; Kulikovskiy, V.; Lahmann, R.; Le Breton, R.; Lefevre, D.; Leonora, E.; Levi, G.; Lincetto, M.; Lopez-Coto, D.; Loucatos, S.; Maderer, L.; Manczak, J.; Marcelin, M.; Margiotta, A.; Marinelli, A.; Martinez-Mora, J. A.; Melis, K.; Migliozzi, P.; Moussa, A.; Muller, R.; Nauta, L.; Navas, S.; Nezri, E.; O'Fearraigh, B.; Paun, A.; Pavalas, G. E.; Pellegrino, C.; Perrin-Terrin, M.; Pestel, V.; Piattelli, P.; Pieterse, C.; Poire, C.; Popa, V.; Pradier, T.; Randazzo, N.; Reck, S.; Riccobene, G.; Romanov, A.; Sanchez-Losa, A.; Salesa Greus, F.; Samtleben, D. F. E.; Sanguineti, M.; Sapienza, P.; Schnabel, J.; Schumann, J.; Schussler, F.; Spurio, M.; Stolarczyk, Th.; Taiuti, M.; Tayalati, Y.; Tingay, S. J.; Vallage, B.; Van Elewyck, V.; Versari, F.; Viola, S.; Vivolo, D.; Wilms, J.; Zavatarelli, S.; Zegarelli, A.; Zornoza, J. D.; Zuniga, J.; Ageron, M.; Aiello, S.; Alshamsi, M.; Alves Garre, S.; Aly, Z.; Ambrosone, A.; Ameli, F.; Andre, M.; Androulakis, G.; Anguita, M.; Assal, W.; Bagatelas, C.; Basegmez du Pree, S.; Benfenati, F.; Berbee, E.; van den Berg, A. M.; Beurthey, S.; van Beveren, V.; Billault, M.; Boettcher, M.; Bou Cabo, M.; Boutonnet, C.; Bouvet, G.; Bozza, C.; Bruno, R.; Buis, E.; Buompane, R.; Caillat, L.; Calvo, D.; Campion, S.; Carduner, H.; Castaldi, P.; Cereseto, R.; Champion, C.; Chau, N.; Chen, A.; Cherubini, S.; Chiarella, V.; Cocimano, R.; Coelho, J. A. B.; Colonges, S.; Cosquer, A.; Cresta, M.; Cruz, A.; Cuttone, G.; D'Amico, A.; Dallier, R.; De Martino, B.; De Palma, M.; Diego-Tortosa, D.; Dorr, M.; Eddyamoui, A.; El Bojaddaini, I.; Eljarrari, H.; Elsaesser, D.; Espinosa, V.; Filipovic, M. D.; Fransen, J.; Gajanana, D.; Gal, T.; Garcia Mendez, J.; Garcia Soto, A.; Garcon, E.; Garufi, F.; Gatius, C.; Geisselbrecht, N.; Gialanella, L.; Giorgio, E.; Gozzini, S. R.; Grella, G.; Guderian, D.; Guillon, B.; Gutierrez, M.; Haefner, J.; Hamdaoui, H.; Hekalo, A.; Hennig, L.; Henry, S.; Idrissi Ibnsalih, W.; Ilioni, A.; Janezashvili, D.; Jansweijer, P.; Kalaczynski, P.; Katz, U. F.; Kayzel, F.; Keller, P.; Kistauri, G.; van der Knaap, F.; Kooijman, P.; Kreter, M.; Labalme, M.; Lagier, P.; Lamare, P.; Lamoureux, M.; Larosa, G.; Lastoria, C.; Laurence, J.; Lazo, A.; Le Guirriec, E.; Le Stum, S.; Lehaut, G.; Leonardi, O.; Leone, F.; Lerouvillois, C.; Lesrel, J.; Lessing, N.; Lindsey Clark, M.; Lipreau, T.; LLorens Alvarez, C.; Lonardo, A.; Longhitano, F.; Lumb, N.; Majumdar, J.; Marini, A.; Markou, C.; Martin, L.; Martini, A.; Marzaioli, F.; Mastroianni, S.; Miele, G.; Migneco, E.; Mijakowski, P.; Miranda, L. S.; Mollo, C. M.; Mongelli, M.; Musico, P.; Musumeci, M.; Nicolau, C. A.; Nkosi, B.; O'Sullivan, M.; Orlando, A.; Ottonello, G.; Ottonello, S.; Palacios Gonzalez, J.; Papalashvili, G.; Papaleo, R.; Pastore, C.; Pellegrini, G.; Pisanti, O.; Pratolongo, F.; Probst, I.; Puhlhofer, G.; Pulvirenti, S.; Quemener, G.; Rapicavoli, A.; Razzaque, S.; Real, D.; Rigalleau, L.; Rovelli, A.; Royon, J.; Santangelo, A.; Santonocito, D.; Schmelling, J.; Schneider, M. F.; Schutte, H. M.; Seneca, J.; Sgura, I.; Shanidze, R.; Sharma, A.; Sinopoulou, A.; Spisso, B.; Stavropoulos, D.; Steijger, J.; Stellacci, S. M.; Tatone, F.; Tenllado, E.; Tezier, D.; Thakore, T.; Theraube, S.; Thiersen, H.; Timmer, P.; Tsagkli, S.; Tsourapis, V.; Tzamariudaki, E.; Tzanetatos, D.; Valieri, C.; Vasileiadis, G.; Wojaczynski, R.; Dewolf, E.; Yousfi, T.; Zito, D.; Zywucka, N.

An anomalous flux of neutrinos produced in hypothetical annihilations or decays of dark matter inside a source would produce a signal observable with neutrino telescopes. As suggested by observations, a conspicuous amount of dark matter is believed to accumulate in the centre of our Galaxy, which is in neat visibility for the Mediterranean underwater telescopes ANTARES and KM3NeT. Searches have been conducted with a maximum likelihood method to identify the presence of a dark matter signature in the neutrino flux measured by ANTARES. Results of all-flavour searches for WIMPs with masses from 50 GeV/c2 up to 100 TeV/c2 over the whole operation period from 2007 to 2020 are presented here. Alternative scenarios which propose a dark matter candidate in the heavy sector extensions of the Standard Model would produce a clear signature in the ANTARES telescope, that can exploit its view of the Galactic Centre up to high energies. The presentation of Galactic Centre searches is completed with ongoing analyses and future potential of the KM3NeT telescope, in phased construction in the Mediterranean Sea.

Indirect dark matter searches with neutrinos from the Galactic Centre region with the ANTARES and KM3NeT telescopes

Albert A.;Alves S.;Andre M.;Anghinolfi M.;Anton G.;Ardid M.;Ardid S.;Aubert J. -J.;Aublin J.;Baret B.;Basa S.;Belhorma B.;Bendahman M.;Bertin V.;Biagi S.;Bissinger M.;Boumaaza J.;Bouta M.;Bouwhuis M. C.;Branzas H.;Bruijn R.;Brunner J.;Busto J.;Caiffi B.;Capone A.;Caramete L.;Carr J.;Carretero V.;Celli S.;Chabab M.;Chau T. N.;Cherkaoui El Moursli R.;Chiarusi T.;Circella M.;Coleiro A.;Colomer-Molla M.;Coniglione R.;Coyle P.;Creusot A.;Diaz A. F.;de Wasseige G.;Deschamps A.;Distefano C.;Di Palma I.;Domi A.;Donzaud C.;Dornic D.;Drouhin D.;Eberl T.;van Eeden T.;van Eijk D.;El Khayati N.;Enzenhofer A.;Fermani P.;Ferrara G.;Filippini F.;Fusco L. A.;Gatelet Y.;Gay P.;Glotin H.;Gozzini R.;Gracia Ruiz R.;Graf K.;Guidi C.;Hallmann S.;van Haren H.;Heijboer A. J.;Hello Y.;Hernandez-Rey J. J.;Hossl J.;Hofestadt J.;Huang F.;Illuminati G.;James C. W.;Jisse-Jung B.;de Jong M.;de Jong P.;Kadler M.;Kalekin O.;Katz U.;Khan-Chowdhury N. R.;Kouchner A.;Kreykenbohm I.;Kulikovskiy V.;Lahmann R.;Le Breton R.;Lefevre D.;Leonora E.;Levi G.;Lincetto M.;Lopez-Coto D.;Loucatos S.;Maderer L.;Manczak J.;Marcelin M.;Margiotta A.;Marinelli A.;Martinez-Mora J. A.;Melis K.;Migliozzi P.;Moussa A.;Muller R.;Nauta L.;Navas S.;Nezri E.;O'Fearraigh B.;Paun A.;Pavalas G. E.;Pellegrino C.;Perrin-Terrin M.;Pestel V.;Piattelli P.;Pieterse C.;Poire C.;Popa V.;Pradier T.;Randazzo N.;Reck S.;Riccobene G.;Romanov A.;Sanchez-Losa A.;Salesa Greus F.;Samtleben D. F. E.;Sanguineti M.;Sapienza P.;Schnabel J.;Schumann J.;Schussler F.;Spurio M.;Stolarczyk Th.;Taiuti M.;Tayalati Y.;Tingay S. J.;Vallage B.;Van Elewyck V.;Versari F.;Viola S.;Vivolo D.;Wilms J.;Zavatarelli S.;Zegarelli A.;Zornoza J. D.;Zuniga J.;Ageron M.;Aiello S.;Alshamsi M.;Alves Garre S.;Aly Z.;Ambrosone A.;Ameli F.;Andre M.;Androulakis G.;Anguita M.;Assal W.;Bagatelas C.;Basegmez du Pree S.;Benfenati F.;Berbee E.;van den Berg A. M.;Beurthey S.;van Beveren V.;Billault M.;Boettcher M.;Bou Cabo M.;Boutonnet C.;Bouvet G.;Bozza C.;Bruno R.;Buis E.;Buompane R.;Caillat L.;Calvo D.;Campion S.;Carduner H.;Castaldi P.;Cereseto R.;Champion C.;Chau N.;Chen A.;Cherubini S.;Chiarella V.;Cocimano R.;Coelho J. A. B.;Colonges S.;Cosquer A.;Cresta M.;Cruz A.;Cuttone G.;D'Amico A.;Dallier R.;De Martino B.;De Palma M.;Diego-Tortosa D.;Dorr M.;Eddyamoui A.;El Bojaddaini I.;Eljarrari H.;Elsaesser D.;Espinosa V.;Filipovic M. D.;Fransen J.;Gajanana D.;Gal T.;Garcia Mendez J.;Garcia Soto A.;Garcon E.;Garufi F.;Gatius C.;Geisselbrecht N.;Gialanella L.;Giorgio E.;Gozzini S. R.;Grella G.;Guderian D.;Guillon B.;Gutierrez M.;Haefner J.;Hamdaoui H.;Hekalo A.;Hennig L.;Henry S.;Idrissi Ibnsalih W.;Ilioni A.;Janezashvili D.;Jansweijer P.;Kalaczynski P.;Katz U. F.;Kayzel F.;Keller P.;Kistauri G.;van der Knaap F.;Kooijman P.;Kreter M.;Labalme M.;Lagier P.;Lamare P.;Lamoureux M.;Larosa G.;Lastoria C.;Laurence J.;Lazo A.;Le Guirriec E.;Le Stum S.;Lehaut G.;Leonardi O.;Leone F.;Lerouvillois C.;Lesrel J.;Lessing N.;Lindsey Clark M.;Lipreau T.;LLorens Alvarez C.;Lonardo A.;Longhitano F.;Lumb N.;Majumdar J.;Marini A.;Markou C.;Martin L.;Martini A.;Marzaioli F.;Mastroianni S.;Miele G.;Migneco E.;Mijakowski P.;Miranda L. S.;Mollo C. M.;Mongelli M.;Musico P.;Musumeci M.;Nicolau C. A.;Nkosi B.;O'Sullivan M.;Orlando A.;Ottonello G.;Ottonello S.;Palacios Gonzalez J.;Papalashvili G.;Papaleo R.;Pastore C.;Pellegrini G.;Pisanti O.;Pratolongo F.;Probst I.;Puhlhofer G.;Pulvirenti S.;Quemener G.;Rapicavoli A.;Razzaque S.;Real D.;Rigalleau L.;Rovelli A.;Royon J.;Santangelo A.;Santonocito D.;Schmelling J.;Schneider M. F.;Schutte H. M.;Seneca J.;Sgura I.;Shanidze R.;Sharma A.;Sinopoulou A.;Spisso B.;Stavropoulos D.;Steijger J.;Stellacci S. M.;Tatone F.;Tenllado E.;Tezier D.;Thakore T.;Theraube S.;Thiersen H.;Timmer P.;Tsagkli S.;Tsourapis V.;Tzamariudaki E.;Tzanetatos D.;Valieri C.;Vasileiadis G.;Wojaczynski R.;deWolf E.;Yousfi T.;Zito D.;Zywucka N.

2022

Abstract

An anomalous flux of neutrinos produced in hypothetical annihilations or decays of dark matter inside a source would produce a signal observable with neutrino telescopes. As suggested by observations, a conspicuous amount of dark matter is believed to accumulate in the centre of our Galaxy, which is in neat visibility for the Mediterranean underwater telescopes ANTARES and KM3NeT. Searches have been conducted with a maximum likelihood method to identify the presence of a dark matter signature in the neutrino flux measured by ANTARES. Results of all-flavour searches for WIMPs with masses from 50 GeV/c2 up to 100 TeV/c2 over the whole operation period from 2007 to 2020 are presented here. Alternative scenarios which propose a dark matter candidate in the heavy sector extensions of the Standard Model would produce a clear signature in the ANTARES telescope, that can exploit its view of the Galactic Centre up to high energies. The presentation of Galactic Centre searches is completed with ongoing analyses and future potential of the KM3NeT telescope, in phased construction in the Mediterranean Sea.