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Related papers: IceCube and KM3NeT: Lessons and Relations

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The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly…

Instrumentation and Methods for Astrophysics · Physics 2016-07-27 S. Adrián-Martínez , M. Ageron , F. Aharonian , S. Aiello , A. Albert , F. Ameli , E. Anassontzis , M. Andre , G. Androulakis , M. Anghinolfi , G. Anton , M. Ardid , T. Avgitas , G. Barbarino , E. Barbarito , B. Baret , J. Barrios-Martí , B. Belhorma , A. Belias , E. Berbee , A. van den Berg , V. Bertin , S. Beurthey , V. van Beveren , N. Beverini , S. Biagi , A. Biagioni , M. Billault , M. Bond , R. Bormuth , B. Bouhadef , G. Bourlis , S. Bourret , C. Boutonnet , M. Bouwhuis , C. Bozza , R. Bruijn , J. Brunner , E. Buis , J. Busto , G. Cacopardo , L. Caillat , M. Calamai , D. Calvo , A. Capone , L. Caramete , S. Cecchini , S. Celli , C. Champion , R. Cherkaoui El Moursli , S. Cherubini , T. Chiarusi , M. Circella , L. Classen , R. Cocimano , J. A. B. Coelho , A. Coleiro , S. Colonges , R. Coniglione , M. Cordelli , A. Cosquer , P. Coyle , A. Creusot , G. Cuttone , A. D'Amico , G. De Bonis , G. De Rosa , C. De Sio , F. Di Capua , I. Di Palma , A. F. Díaz García , C. Distefano , C. Donzaud , D. Dornic , Q. Dorosti-Hasankiadeh , E. Drakopoulou , D. Drouhin , L. Drury , M. Durocher , T. Eberl , S. Eichie , D. van Eijk , I. El Bojaddaini , N. El Khayati , D. Elsaesser , A. Enzenhöfer , F. Fassi , P. Favali , P. Fermani , G. Ferrara , G. Frascadore , C. Filippidis , L. A. Fusco , T. Gal , S. Galatà , F. Garufi , P. Gay , M. Gebyehu , V. Giordano , N. Gizani , R. Gracia , K. Graf , T. Grégoire , G. Grella , R. Habel , S. Hallmann , H. van Haren , S. Harissopulos , T. Heid , A. Heijboer , E. Heine , S. Henry , J. J. Hernández-Rey , M. Hevinga , J. Hofestädt , C. M. F. Hugon , G. Illuminati , C. W. James , P. Jansweijer , M. Jongen , M. de Jong , M. Kadler , O. Kalekin , A. Kappes , U. F. Katz , P. Keller , G. Kieft , D. Kießling , E. N. Koffeman , P. Kooijman , A. Kouchner , V. Kulikovskiy , R. Lahmann , P. Lamare , A. Leisos , E. Leonora , M. Lindsey Clark , A. Liolios , C. D. Llorens Alvarez , D. Lo Presti , H. Löhner , A. Lonardo , M. Lotze , S. Loucatos , E. Maccioni , K. Mannheim , A. Margiotta , A. Marinelli , O. Mariş , C. Markou , J. A. Martínez-Mora , A. Martini , R. Mele , K. W. Melis , T. Michael , P. Migliozzi , E. Migneco , P. Mijakowski , A. Miraglia , C. M. Mollo , M. Mongelli , M. Morganti , A. Moussa , P. Musico , M. Musumeci , S. Navas , C. A. Nicolau , I. Olcina , C. Olivetto , A. Orlando , A. Papaikonomou , R. Papaleo , G. E. Păvălaş , H. Peek , C. Pellegrino , C. Perrina , M. Pfutzner , P. Piattelli , K. Pikounis , G. E. Poma , V. Popa , T. Pradier , F. Pratolongo , G. Pühlhofer , S. Pulvirenti , L. Quinn , C. Racca , F. Raffaelli , N. Randazzo , P. Rapidis , P. Razis , D. Real , L. Resvanis , J. Reubelt , G. Riccobene , C. Rossi , A. Rovelli , M. Saldaña , I. Salvadori , D. F. E. Samtleben , A. Sánchez García , A. Sánchez Losa , M. Sanguineti , A. Santangelo , D. Santonocito , P. Sapienza , F. Schimmel , J. Schmelling , V. Sciacca , M. Sedita , T. Seitz , I. Sgura , F. Simeone , I. Siotis , V. Sipala , B. Spisso , M. Spurio , G. Stavropoulos , J. Steijger , S. M. Stellacci , D. Stransky , M. Taiuti , Y. Tayalati , D. Tézier , S. Theraube , L. Thompson , P. Timmer , C. Tönnis , L. Trasatti , A. Trovato , A. Tsirigotis , S. Tzamarias , E. Tzamariudaki , B. Vallage , V. Van Elewyck , J. Vermeulen , P. Vicini , S. Viola , D. Vivolo , M. Volkert , G. Voulgaris , L. Wiggers , J. Wilms , E. de Wolf , K. Zachariadou , J. D. Zornoza , J. Zúñiga

The discovery of high-energy astrophysical neutrinos by IceCube has opened a new window to the Universe. However, the origin of these neutrinos is still a mystery, and some of them could be a result of dark matter interactions such as…

Neutrino observatories such as IceCube, Cubic Kilometre Neutrino Telescope (KM3NeT), and Super-Kamiokande cover a broad energy range that enables the study of both atmospheric neutrinos and astrophysical neutrinos. IceCube and KM3NeT focus…

High Energy Astrophysical Phenomena · Physics 2025-01-31 Shiqi Yu

We review the state of the art in the detection of extreme high-energy neutrinos, focusing on the IceCube and KM3NeT neutrino telescopes. IceCube, operating deep in Antarctic ice, and KM3NeT, a new array in the Mediterranean Sea, employ…

High Energy Astrophysical Phenomena · Physics 2025-09-17 Lu Lu , Tianlu Yuan

KM3NeT is a future research infrastructure in the Mediterranean Sea, hosting a multi-cubic-kilometre neutrino telescope and nodes for Earth and Sea sciences. In this report we shortly summarise the genesis of the KM3NeT project and present…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Ulrich F. Katz

I will discuss the motivations for Neutrino Astronomy and its prospects given the current experimental scenario, which is the main focus of this paper. I will also go through the first results of the IceCube detector deep in the ice and of…

Instrumentation and Methods for Astrophysics · Physics 2010-12-13 Teresa Montaruli

The observation of high-energy extraterrestrial neutrinos is one of the most promising future options to increase our knowledge on non-thermal processes in the universe. Neutrinos are e.g. unavoidably produced in environments where…

Astrophysics · Physics 2009-11-11 Ulrich F. Katz

High energy neutrinos produced in astrophysical processes will allow for a new way of studying the universe. In order to detect the expected flux of high energy neutrinos from specific astrophysical sources, neutrino telescopes of a scale…

Astrophysics · Physics 2019-08-14 P. A. Rapidis

This talk describes the complete IceCube neutrino telescope and summarizes some results obtained while the detector was under construction.

High Energy Astrophysical Phenomena · Physics 2011-08-10 Thomas K. Gaisser

High-energy neutrino telescopes such as IceCube or KM3NeT issue public alerts describing the characteristics of possible astrophysical high-energy neutrino events. This information, particularly with respect to the arrival direction and the…

High Energy Astrophysical Phenomena · Physics 2023-06-22 Thierry Pradier

To complement the IceCube neutrino telescope currently under construction at the South Pole, the three Mediterranean neutrino telescope projects ANTARES, NEMO and NESTOR have joined forces to develop, construct and operate a km^3-scale…

Astrophysics · Physics 2019-08-14 A. Kappes

IceCube, a cubic kilometer neutrino telescope will be capable of probing neutrino-nucleon interactions in the ultrahigh energy regime, far beyond the energies reached by colliders. In this article we introduce a new observable that combines…

High Energy Physics - Phenomenology · Physics 2008-11-26 Matias M. Reynoso , Oscar A. Sampayo

Theoretical predictions for neutrino fluxes indicate that km$^{3}$ scale detectors are needed to detect certain astrophysical sources. The three Mediterranean experiments, ANTARES, NEMO and NESTOR are working together on a design study,…

Astrophysics · Physics 2019-08-14 J. Carr , D. Dornic , F. Jouvenot , G. Maurin

The KM3NeT collaboration recently reported the observation of KM3-230213A, a neutrino event with an energy exceeding 100 PeV, more than an order of magnitude higher than the most energetic neutrino in IceCube's catalog. Given its longer…

High Energy Physics - Phenomenology · Physics 2026-03-17 Vedran Brdar , Dibya S. Chattopadhyay

Search for ultra high-energy neutrino induced reactions, as part of a comprehensive probe of the neutrino sky and also investigation of the particle nature of the dark matter, with unique sensitivity to cold dark matter particles are…

Astrophysics · Physics 2017-08-23 A. R. Fazely

With the completion of the first cubic-kilometer class neutrino telescopes, IceCube, the race for the discovery of the first cosmic high-energy neutrino sources enters into a new phase. The usage of neutrinos as cosmic messengers has the…

High Energy Astrophysical Phenomena · Physics 2011-11-01 Alexander Kappes

Kilometer-scale neutrino detectors such as IceCube are discovery instruments covering nuclear and partile physics, cosmology and astronomy. Examples of their multidisciplinary mission include the search for the particle nature of dark…

Astrophysics · Physics 2015-06-24 F. Halzen

KM3NeT is a deep-sea research infrastructure being constructed in the Mediterranean Sea. It will host the next generation Cherenkov neutrino telescope and nodes for a deep sea multidisciplinary observatory, providing oceanographers, marine…

Instrumentation and Methods for Astrophysics · Physics 2014-08-08 Annarita Margiotta

The year 2008 has witnessed remarkable steps in developing high energy neutrino telescopes. IceCube at the South Pole has been deployed with 40 of its planned 80 strings and reached half a cubic kilometer instrumented volume, in the…

Astrophysics · Physics 2009-11-13 Christian Spiering

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
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