Related papers: First Searches for Dark Matter with the KM3NeT Neu…

Towards detecting super-GeV dark matter via annihilation to neutrinos

The next generation of neutrino telescopes will feature unprecedented sensitivities in the detection of neutrinos. Here we study the capabilities of a large-scale neutrino telescope, like the fully-operating KM3NeT experiment in the near…

High Energy Physics - Phenomenology · Physics 2023-08-16 L. Salvador Miranda , S. Basegmez du Pree , K. C. Y. Ng , A. Cheek , C. Arina

Search of Dark Matter Annihilation in the Galactic Centre using the ANTARES Neutrino Telescope

A search for high-energy neutrinos coming from the direction of the Galactic Centre is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. The event selection criteria are chosen to maximise the…

High Energy Astrophysical Phenomena · Physics 2016-08-08 ANTARES Collaboration , S. Adrián-Martínez , A. Albert , M. André , G. Anton , M. Ardid , J. -J. Aubert , B. Baret , J. Barrios-Martí , S. Basa , V. Bertin , S. Biagi , C. Bogazzi , R. Bormuth , M. Bou-Cabo , M. C. Bouwhuis , R. Bruijn , J. Brunner , J. Busto , A. Capone , L. Caramete , J. Carr , T. Chiarusi , M. Circella , R. Coniglione , H. Costantini , P. Coyle , A. Creusot , I. Dekeyser , A. Deschamps , G. DeBonis , C. Distefano , C. Donzaud , D. Dornic , D. Drouhin , A. Dumas , T. Eberl , D. Elsässer , A. Enzenhöfer , K. Fehn , I. Felis , P. Fermani , F. Folger , L. A. Fusco , S. Galatà , P. Gay , S. Geißelsöder , K. Geyer , V. Giordano , A. Gleixner , R. Gracia-Ruiz , K. Graf , H. vanHaren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , A. Herrero , J. Hößl , J. Hofestädt , C. Hugon , C. WJames , M. deJong , M. Kadler , O. Kalekin , U. Katz , D. Kießling , P. Kooijman , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , G. Lambard , D. Lattuada , D. Lefèvre , E. Leonora , S. Loucatos , M. Marcelin , A. Margiotta , J. A. Martínez-Mora , S. Martini , A. Mathieu , T. Michael , P. Migliozzi , A. Moussa , C. Mueller , M. Neff , E. Nezri , G. E. Păvălaş , C. Pellegrino , C. Perrina , P. Piattelli , V. Popa , T. Pradier , C. Racca , G. Riccobene , R. Richter , K. Roensch , A. Rostovtsev , M. Saldaña , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schmid , J. Schnabel , S. Schulte , F. Schüssler , T. Seitz , C. Sieger , M. Spurio , J. J. M. Steijger , Th. Stolarczyk , A. Sánchez-Losa , M. Taiuti , C. Tamburini , A. Trovato , M. Tselengidou , C. Tönnis , B. Vallage , C. Vallée , V. VanElewyck , E. Visser , D. Vivolo , S. Wagner , J. Wilms , J. D. Zornoza , J. Zúñiga

Prospects for detecting Dark Matter with neutrino telescopes in Intermediate Mass Black Holes scenarios

Current strategies of indirect Dark Matter detection with neutrino telescopes are based on the search for high-energy neutrinos from the Solar core or from the center of the Earth. Here, we propose a new strategy based on the detection of…

Astrophysics · Physics 2009-11-11 Gianfranco Bertone

Indirect Search for Dark Matter

Possible dark matter candidates are reviewed as well as indirect search methods based on annihilation or decay channels of these particles. Neutralino is presently the best particle candidate and its annihilation produces high energy…

Astrophysics · Physics 2016-08-16 José Antonio De Freitas Pacheco , Sébastien Peirani

Indirect detection of neutralino dark matter

Dark matter detection experiments are getting ever closer to the sensitivity needed to detect the primary particle physics candidates for nonbaryonic dark matter. Indirect detection methods include searching for antimatter and gamma rays,…

Astrophysics · Physics 2009-10-31 L. Bergstrom

The Detection of Cold Dark Matter with Neutrino Telescopes

High energy neutrinos are produced by the annihilation of dark matter particles in our galaxy. These are presently searched for with large area, deep underground neutrino telescopes. Cold dark matter particles, trapped inside the sun, are…

High Energy Physics - Phenomenology · Physics 2009-09-25 F. Halzen , J. E. Jacobsen

The Indirect Detection of Halo Dark Matter

High energy particles are produced by the annihilation of dark matter particles in our galaxy. These are presently searched for using balloon-borne antiproton and positron detectors and large area, deep underground neutrino telescopes. Dark…

High Energy Physics - Phenomenology · Physics 2016-09-01 F. Halzen , J. E Jacobsen

Dark matter search with the ANTARES neutrino telescope

The ANTARES neutrino telescope was completed in 2008 with the installation of its twelfth line. Its scientific scope is very broad, but the two main goals are the observation of astrophysical sources and the indirect detection of dark…

High Energy Astrophysical Phenomena · Physics 2015-06-04 J. D. Zornoza

Indirect search for dark matter with neutrino telescopes

The quest to understand the nature dark matter is one of the most relevant ones in Particle Physics nowadays, since it constitutes most of the matter of the Universe and it is still unknown what it is made of. In order to answer to this…

High Energy Astrophysical Phenomena · Physics 2016-10-04 J. D. Zornoza

Detecting Asymmetric Dark Matter in the Sun with Neutrinos

Dark Matter (DM) may have a relic density that is in part determined by a particle/antiparticle asymmetry, much like baryons. If this is the case, it can accumulate in stars like the Sun to sizable number densities and annihilate to…

High Energy Physics - Phenomenology · Physics 2016-10-26 Kohta Murase , Ian M. Shoemaker

Results of dark matter searches with the ANTARES neutrino telescope

Neutrino telescopes have a wide scientic scope. One of their main goals is the detection of dark matter, for which they have specic advantages. Neutrino telescopes offer the possibility of looking at several kinds of sources, not all of…

High Energy Astrophysical Phenomena · Physics 2017-10-11 J. D. Zornoza , C. Toennis

Indirect search for Dark Matter with the ANTARES neutrino telescope

Relic neutralinos produced after the Big Bang are favoured candidates for Dark Matter. They can accumulate at the centre of massive celestial objects like our Sun. Their annihilation can result in a high-energy neutrino flux that could be…

Astrophysics · Physics 2019-08-13 Gordon Lim

Indirect dark matter search in the Galactic Centre with IceCube

It is assumed that dark matter can annihilate or decay into Standard Model particles which then can produce a neutrino flux detectable at IceCube. Such a signal can be emitted from the Galactic Center thanks to the high density of dark…

High Energy Astrophysical Phenomena · Physics 2023-08-15 Nhan Chau , Juan A. Aguilar

Robust Limits from Upcoming Neutrino Telescopes and Implications on Minimal Dark Matter Models

Experimental developments in neutrino telescopes are drastically improving their ability to constrain the annihilation cross-section of dark matter. In this paper, we employ an angular power spectrum analysis method to probe the galactic…

High Energy Physics - Phenomenology · Physics 2021-06-02 S. Basegmez du Pree , C. Arina , A. Cheek , A. Dekker , M. Chianese , S. Ando

First Search for Dark Matter Annihilation in the Sun Using the ANTARES Neutrino Telescope

A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the…

High Energy Astrophysical Phenomena · Physics 2015-06-15 ANTARES Collaboration , S. Adrián-Martinez , I. Al Samarai , A. Albert , M. André , M. Anghinolfi , G. Anton , L. Anton , S. Anvar , M. Ardid , T. Astraatmadjaote , J-J. Aubert , B. Baret , S. Basa , V. Bertin , S. Biagi , C. Bigongiari , C. Bogazzi , B. Bouhou , M. C. Bouwhuis , J. Brünner , J. Busto , A. Capone , C. Cârloganu , J. Carr , S. Cecchini , Z. Charif , Ph. Charvis , T. Chiarusi , M. Circella , F. Classen , R. Coniglione , L. Core , H. Costantini , P. Coyle , A. Creusot , C. Curtil , G. De Bonis , M. P. Decowski , I. Dekeyser , A. Deschamps , C. Distefano , C. Donzaud , D. Dornic , Q. Dorosti , D. Drouhin , A. Dumas , T. Eberl , U. Emanuele , A. Enzenhöfer , J-P. Ernenwein , S. Escoffier , K. Fehn , P. Fermani , S. Ferry , V. Flaminio , F. Folger , U. Fritsch , J-L. Fuda , S. Galatà , P. Gay , S. Geisselsöder , K. Geyer , G. Giacomelli , V. Giordano , A. Gleixner , J. P. Gómez-González , K. Graf , G. Guillard , G. Hallewell , M. Hamal , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , B. Herold , J. Hössl , C. C. Hsu , C. James , M. de Jong , M. Kadler , O. Kalekin , A. Kappesote , U. Katz , P. Kooijman , C. Kopper , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , G. Lambardote , G. Larosa , D. Lattuada , D. Lefèvre , E. Leonora , D. Lo Presti , H. Loehner , S. Loucatos , F. Louis , S. Mangano , M. Marcelin , A. Margiotta , J. A. Martinez-Mora , S. Martini , T. Montaruli , M. Morgantiote , H. Motz , C. Mueller , M. Neff , E. Nezri , D. Palioselitis , G. E. Pavalas , J. Petrovic , P. Piattelli , V. Popa , T. Pradier , C. Racca , C. Reed , G. Riccobene , R. Richter , C. Rivière , A. Robert , K. Roensch , A. Rostovtsev , M. Rujoiu , D. F. E. Samtleben , A. Sánchez-Losa , P. Sapienza , J. Schmid , J. Schnabel , S. Schulte , F. Schüssler , T. Seitz , R. Shanidze , F. Simeone , A. Spies , M. Spurio , J. J. M. Steijger , Th. Stolarczyk , M. Taiuti , C. Tamburini , A. Trovato , B. Vallage , C. Vallée , V. Van Elewyck , P. Vernin , E. Visser , S. Wagner , G. Wijnker , J. Wilms , E. de Wolf , K. Yatkin , H. Yepes , D. Zaborov , J. D. Zornoza , J. Zúñiga

Probing the Dark Matter mass and nature with neutrinos

We study the possible indirect neutrino signal from dark matter annihilations inside the solar interior for relatively light dark matter masses in the O(10) GeV range. Due to their excellent energy reconstruction capabilities, we focus on…

High Energy Physics - Phenomenology · Physics 2015-06-15 Mattias Blennow , Marcus Carrigan , Enrique Fernandez Martinez

Illuminating Very Heavy Dark Matter in the Earth with Tau Neutrinos

Dark matter accumulates in the center of the Earth as the planet plows through the dark matter halo in the Milky Way. Possible annihilation of dark matter to Standard Model particles can be probed in indirect dark matter searches. Among…

High Energy Physics - Phenomenology · Physics 2025-05-16 Tianyi Ding , Ali Kheirandish , Qinrui Liu

Search for neutrino emission from relic dark matter in the Sun with the Baikal NT200 detector

We have analyzed a data set taken over 2.76 years live time with the Baikal neutrino telescope NT200. The goal of the analysis is to search for neutrinos from dark matter annihilation in the center of the Sun. Apart from the conventional…

High Energy Astrophysical Phenomena · Physics 2014-08-12 A. D. Avrorin , A. V. Avrorin , V. M. Aynutdinov , R. Bannasch , I. A. Belolaptikov , D. Yu. Bogorodsky , V. B. Brudanin , N. M. Budnev , I. A. Danilchenko , S. V. Demidov , G. V. Domogatsky , A. A. Doroshenko , A. N. Dyachok , Zh-A. M. Dzhilkibaev , S. V. Fialkovsky , A. R. Gafarov , O. N. Gaponenko , K. V. Golubkov , T. I. Gress , Z. Honz , K. G. Kebkal , O. G. Kebkal , K. V. Konishchev , E. N. Konstantinov , A. V. Korobchenko , A. P. Koshechkin , F. K. Koshel , V. A. Kozhin , V. F. Kulepov , D. A. Kuleshov , V. I. Ljashuk , M. B. Milenin , R. A. Mirgazov , E. A. Osipova , A. I. Panfilov , L. V. Panjkov , A. A. Perevalov , E. N. Pliskovsky , V. A. Poleshuk , M. I. Rozanov , V. F. Rubtsov , E. V. Rjabov , B. A. Shaybonov , A. A. Sheifler , A. V. Skurikhin , A. A. Smagina , O. V. Suvorova , B. A. Tarashchansky , S. A. Yakovlev , A. V. Zagorodnikov , V. A. Zhukov , V. L. Zurbanov

The Online Data Filter for the KM3NeT Neutrino Telescopes

The KM3NeT research infrastructure comprises two neutrino telescopes located in the deep waters of the Mediterranean Sea, namely ORCA and ARCA. KM3NeT/ORCA is designed for the measurement of neutrino properties and KM3NeT/ARCA for the…

Instrumentation and Methods for Astrophysics · Physics 2025-10-16 O. Adriani , S. Aiello , A. Albert , A. R. Alhebsi , M. Alshamsi , S. Alves Garre , A. Ambrosone , F. Ameli , M. Andre , L. Aphecetche , M. Ardid , S. Ardid , J. Aublin , F. Badaracco , L. Bailly-Salins , Z. Bardacova , B. Baret , A. Bariego-Quintana , Y. Becherini , M. Bendahman , F. Benfenati Gualandi , M. Benhassi , M. Bennani , D. M. Benoit , E. Berbee , E. Berti , V. Bertin , P. Betti , S. Biagi , M. Boettcher , D. Bonanno , S. Bottai , A. B. Bouasla , J. Boumaaza , M. Bouta , M. Bouwhuis , C. Bozza , R. M. Bozza , H. Branzas , F. Bretaudeau , M. Breuhaus , R. Bruijn , J. Brunner , R. Bruno , E. Buis , R. Buompane , J. Busto , B. Caiffi , D. Calvo , A. Capone , F. Carenini , V. Carretero , T. Cartraud , P. Castaldi , V. Cecchini , S. Celli , L. Cerisy , M. Chabab , A. Chen , S. Cherubini , T. Chiarusi , M. Circella , R. Clark , R. Cocimano , J. A. B. Coelho , A. Coleiro , A. Condorelli , R. Coniglione , P. Coyle , A. Creusot , G. Cuttone , R. Dallier , A. De Benedittis , G. De Wasseige , V. Decoene , P. Deguire , I. Del Rosso , L. S. Di Mauro , I. Di Palma , A. F. Diaz , D. Diego-Tortosa , C. Distefano , A. Domi , C. Donzaud , D. Dornic , E. Drakopoulou , D. Drouhin , J. -G. Ducoin , P. Duverne , R. Dvornicky , T. Eberl , E. Eckerova , A. Eddymaoui , T. van Eeden , M. Eff , D. van Eijk , I. El Bojaddaini , S. El Hedri , S. El Mentawi , A. Enzenhofer , G. Ferrara , M. D. Filipovic , F. Filippini , D. Franciotti , L. A. Fusco , T. Gal , J. Garcia Mendez , A. Garcia Soto , C. Gatius Oliver , N. Geiselbrecht , E. Genton , H. Ghaddari , L. Gialanella , B. K. Gibson , E. Giorgio , I. Goos , P. Goswami , S. R. Gozzini , R. Gracia , B. Guillon , C. Haack , H. van Haren , A. Heijboer , L. Hennig , J. J. Hernandez-Rey , A. Idrissi , W. Idrissi Ibnsalih , G. Illuminati , R. Jaimes , O. Janik , D. Joly , M. de Jong , P. de Jong , B. J. Jung , P. Kalaczynski , J. Keegans , V. Kikvadze , G. Kistauri , C. Kopper , A. Kouchner , Y. Y. Kovalev , L. Krupa , V. Kueviakoe , V. Kulikovskiy , R. Kvatadze , M. Labalme , R. Lahmann , M. Lamoureux , G. Larosa , C. Lastoria , J. Lazar , A. Lazo , S. Le Stum , G. Lehaut , V. Lemaitre , E. Leonora , N. Lessing , G. Levi , M. Lindsey Clark , F. Longhitano , F. Magnani , J. Majumdar , L. Malerba , F. Mamedov , A. Manfreda , A. Manousakis , M. Marconi , A. Margiotta , A. Marinelli , C. Markou , L. Martin , M. Mastrodicasa , S. Mastroianni , J. Mauro , K. C. K. Mehta , G. Miele , P. Migliozzi , E. Migneco , M. L. Mitsou , C. M. Mollo , L. Morales-Gallegos , N. Mori , A. Moussa , I. Mozun Mateo , R. Muller , M. R. Musone , M. Musumeci , S. Navas , A. Nayerhoda , C. A. Nicolau , B. Nkosi , B. O Fearraigh , V. Oliviero , A. Orlando , E. Oukacha , L. Pacini , D. Paesani , J. Palacios Gonzalez , G. Papalashvili , P. Papini , V. Parisi , A. Parmar , E. J. Pastor Gomez , C. Pastore , A. M. Paun , G. E. Pavalas , S. Pena Martinez , M. Perrin-Terrin , V. Pestel , M. Petropavlova , P. Piattelli , A. Plavin , C. Poire , T. Pradier , J. Prado , S. Pulvirenti , C. A. Quiroz-Rangel , N. Randazzo , A. Ratnani , S. Razzaque , I. C. Rea , D. Real , G. Riccobene , J. Robinson , A. Romanov , E. Ros , A. Saina , F. Salesa Greus , D. F. E. Samtleben , A. Sanchez Losa , S. Sanfilippo , M. Sanguineti , D. Santonocito , P. Sapienza , M. Scaringella , M. Scarnera , J. Schnabel , J. Schumann , J. Seneca , N. Sennan , P. A. Sevle Myhr , I. Sgura , R. Shanidze , Chengyu Shao , A. Sharma , Y. Shitov , F. Simkovic , A. Simonelli , A. Sinopoulou , B. Spisso , M. Spurio , O. Starodubtsev , D. Stavropoulos , I. Stekl , D. Stocco , M. Taiuti , G. Takadze , Y. Tayalati , H. Thiersen , S. Thoudam , I. Tosta e Melo , B. Trocme , V. Tsourapis , E. Tzamariudaki , A. Ukleja , A. Vacheret , V. Valsecchi , V. Van Elewyck , G. Vannoye , E. Vannuccini , G. Vasileiadis , F. Vazquez de Sola , A. Veutro , S. Viola , D. Vivolo , A. van Vliet , E. de Wolf , I. Lhenry-Yvon , S. Zavatarelli , D. Zito , J. D. Zornoza , J. Zuniga

Sensitivity of the KM3NeT/ARCA neutrino telescope to point-like neutrino sources

KM3NeT will be a network of deep-sea neutrino telescopes in the Mediterranean Sea. The KM3NeT/ARCA detector, to be installed at the Capo Passero site (Italy), is optimised for the detection of high-energy neutrinos of cosmic origin. Thanks…

High Energy Astrophysical Phenomena · Physics 2021-03-10 The KM3NeT Collaboration , S. Aiello , S. E. Akrame , F. Ameli , E. G. Anassontzis , M. Andre , G. Androulakis , M. Anghinolfi , G. Anton , M. Ardid , J. Aublin , T. Avgitas , C. Bagatelas , G. Barbarino , B. Baret , J. Barrios-Martí , A. Belias , E. Berbee , A. van den Berg , V. Bertin , S. Biagi , A. Biagioni , C. Biernoth , J. Boumaaza , S. Bourret , M. Bouta , M. Bouwhuis , C. Bozza , H. Brânzas , M. Bruchner , R. Bruijn , J. Brunner , E. Buis , R. Buompane , J. Busto , D. Calvo , A. Capone , S. Celli , M. Chabab , N. Chau , S. Cherubini , V. Chiarella , T. Chiarusi , M. Circella , R. Cocimano , J. A. B. Coelho , A. Coleiro , M. Colomer Molla , R. Coniglione , P. Coyle , A. Creusot , G. Cuttone , A. D'Onofrio , R. Dallier , C. De Sio , I. Di Palma , A. F. Díaz , D. Diego-Tortosa , C. Distefano , A. Domi , R. Donà , C. Donzaud , D. Dornic , M. Dörr , M. Durocher , T. Eberl , D. van Eijk , I. El Bojaddaini , H. Eljarrari , D. Elsaesser , A. Enzenhöfer , P. Fermani , G. Ferrara , M. D. Filipovic , L. A. Fusco , T. Gal , A. Garcia , F. Garufi , L. Gialanella , E. Giorgio , A. Giuliante , S. R. Gozzini , R. Gracia , K. Graf , D. Grasso , T. Grégoire , G. Grella , S. Hallmann , H. Hamdaoui , H. van Haren , T. Heid , A. Heijboer , A. Hekalo , J. J. Hernández-Rey , J. Hofestädt , G. Illuminati , C. W. James , M. Jongen , M. de Jong , P. de Jong , M. Kadler , P. Kalaczynski , O. Kalekin , U. F. Katz , N. R. Khan Chowdhury , D. Kiessling , E. N. Koffeman , P. Kooijman , A. Kouchner , M. Kreter , V. Kulikovskiy , M. Kunhikannan-Kannichankandy , R. Lahmann , G. Larosa , R. Le Breton , F. Leone , E. Leonora , G. Levi , M. Lincetto , A. Lonardo , F. Longhitano , D. Lopez Coto , M. Lotze , L. Maderer , G. Maggi , J. Manczak , K. Mannheim , A. Margiotta , A. Marinelli , C. Markou , L. Martin , J. A. Martínez-Mora , A. Martini , F. Marzaioli , R. Mele , K. W. Melis , P. Migliozzi , E. Migneco , P. Mijakowski , L. S. Miranda , C. M. Mollo , M. Morganti , M. Moser , A. Moussa , R. Muller , M. Musumeci , L. Nauta , S. Navas , C. A. Nicolau , C. Nielsen , B. Ó Fearraigh , M. Organokov , A. Orlando , S. Ottonello , V. Panagopoulos , G. Papalashvili , R. Papaleo , G. E. Păvălaş , C. Pellegrino , M. Perrin-Terrin , P. Piattelli , K. Pikounis , O. Pisanti , C. Poirè , G. Polydefki , V. Popa , M. Post , T. Pradier , G. Pühlhofer , S. Pulvirenti , L. Quinn , F. Raffaelli , N. Randazzo , S. Razzaque , D. Real , L. Resvanis , J. Reubelt , G. Riccobene , M. Richer , L. Rigalleau , A. Rovelli , M. Saffer , I. Salvadori , D. F. E. Samtleben , A. Sánchez Losa , M. Sanguineti , A. Santangelo , D. Santonocito , P. Sapienza , J. Schumann , V. Sciacca , J. Seneca , I. Sgura , R. Shanidze , A. Sharma , F. Simeone , A. Sinopoulou , B. Spisso , M. Spurio , D. Stavropoulos , J. Steijger , S. M. Stellacci , B. Strandberg , D. Stransky , T. Stüven , M. Taiuti , F. Tatone , Y. Tayalati , E. Tenllado , T. Thakore , A. Trovato , E. Tzamariudaki , D. Tzanetatos , V. Van Elewyck , F. Versari , S. Viola , D. Vivolo , J. Wilms , E. de Wolf , D. Zaborov , J. D. Zornoza , J. Zúñiga