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Related papers: Neutrino Physics with the IceCube Detector

200 papers

IceCube is a km^3 scale neutrino detector being constructed deep in the Antarctic ice. When complete, IceCube will consist of 4800 optical modules deployed on 80 strings between 1450 and 2450 m of depth. During the 2007-2008 data taking…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Erik Strahler

The IceCube Neutrino Observatory is a cubic kilometer-sized detector designed to detect neutrinos of astrophysical origin. However, muons created by cosmic rays interacting in the atmosphere pose a significant background for these…

High Energy Astrophysical Phenomena · Physics 2021-07-22 Sarah Mancina , Manuel Silva

IceCube is the first representative of the km^3 class of neutrino telescopes and currently the most sensitive detector to high-energy neutrinos. Its main mission is to search for Galactic and extragalactic sources of high-energy neutrinos,…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Alexander 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

IceCube is a 1 km^3 neutrino detector now being built at the Amundsen-Scott South Pole Station. It consists of 4800 Digital Optical Modules (DOMs) which detect Cherenkov radiation from the charged particles produced in neutrino…

Instrumentation and Detectors · Physics 2019-08-13 Spencer R. Klein

The IceCube observatory located at the South Pole is a cubic-kilometre optical Cherenkov telescope primarily designed for the detection of high-energy astrophysical neutrinos. IceCube became fully operational in 2010, after a seven-year…

High Energy Astrophysical Phenomena · Physics 2018-11-20 Markus Ahlers , Klaus Helbing , Carlos Pérez de los Heros

Encompasing a volume of ~1 km^3 of glacial ice at the South Pole, IceCube is currently the worlds largest neutrino detector. It consists of 5160 optical modules on 86 strings in a depth between 1450m and 2450m, as well as 324 optical…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Sebastian Böser

IceCube is a 1 km$^3$ neutrino observatory being built to study neutrino production in active galactic nuclei, gamma-ray bursts, supernova remnants, and a host of other astrophysical sources. High-energy neutrinos may signal the sources of…

Astrophysics · Physics 2019-08-14 Spencer R. Klein

The IceCube Neutrino Observatory, deployed inside the deep glacial ice at the South Pole, is the largest neutrino telescope in the world. While eight years have passed since IceCube discovered a diffuse flux of high-energy astrophysical…

High Energy Astrophysical Phenomena · Physics 2021-09-15 Chiara Bellenghi , Theo Glauch , Christian Haack , Tomas Kontrimas , Hans Niederhausen , Rene Reimann , Martin Wolf

The IceCube Neutrino Observatory is a one-cubic-kilometer-sized neutrino telescope deployed deep in the Antarctic ice at the South Pole. One of IceCube's major goals is finding the origins of astrophysical high-energy neutrinos. In 2022,…

High Energy Astrophysical Phenomena · Physics 2023-08-25 Chiara Bellenghi , Martin Ha Minh , Tomas Kontrimas , Elena Manao , Rasmus Ørsøe , Martin Wolf

The 1 km$^3$ IcCube neutrino observatory was built to find high-energy neutrinos that are associated with the sources of ultra-high energy cosmic rays. Its 5,160 optical sensors detect Cherenkov light from the charged particles produced…

High Energy Astrophysical Phenomena · Physics 2018-10-02 Spencer R. Klein

High-energy neutrinos are uniquely suited to study a large variety of physics as they traverse the universe almost untouched, in contrast to conventional astronomical messengers like photons or cosmic rays which are limited by interactions…

Astrophysics · Physics 2019-08-14 Carsten Rott

In this chapter, we describe how the IceCube Neutrino Observatory transformed a cubic kilometer of natural ice at the geographic South Pole into a neutrino telescope. The concept of using the neutrino as an astronomical messenger is as old…

High Energy Astrophysical Phenomena · Physics 2024-11-26 Francis Halzen , John Kelley

The IceCube Neutrino Observatory is a cubic-kilometer-scale high-energy neutrino detector built into the ice at the South Pole. Construction of IceCube, the largest neutrino detector built to date, was completed in 2011 and enabled the…

Instrumentation and Methods for Astrophysics · Physics 2024-02-08 IceCube Collaboration , M. G. Aartsen , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. Ahrens , D. Altmann , K. Andeen , T. Anderson , I. Ansseau , G. Anton , M. Archinger , C. Argüelles , R. Auer , J. Auffenberg , S. Axani , J. Baccus , X. Bai , S. Barnet , S. W. Barwick , V. Baum , R. Bay , K. Beattie , J. J. Beatty , J. Becker Tjus , K. -H. Becker , T. Bendfelt , S. BenZvi , D. Berley , E. Bernardini , A. Bernhard , D. Z. Besson , G. Binder , D. Bindig , M. Bissok , E. Blaufuss , S. Blot , D. Boersma , C. Bohm , M. Börner , F. Bos , D. Bose , S. Böser , O. Botner , A. Bouchta , J. Braun , L. Brayeur , H. -P. Bretz , S. Bron , A. Burgman , C. Burreson , T. Carver , M. Casier , E. Cheung , D. Chirkin , A. Christov , K. Clark , L. Classen , S. Coenders , G. H. Collin , J. M. Conrad , D. F. Cowen , R. Cross , C. Day , M. Day , J. P. A. M. de André , C. De Clercq , E. del Pino Rosendo , H. Dembinski , S. De Ridder , F. Descamps , P. Desiati , K. D. de Vries , G. de Wasseige , M. de With , T. DeYoung , J. C. Díaz-Vélez , V. di Lorenzo , H. Dujmovic , J. P. Dumm , M. Dunkman , B. Eberhardt , W. R. Edwards , T. Ehrhardt , B. Eichmann , P. Eller , S. Euler , P. A. Evenson , S. Fahey , A. R. Fazely , J. Feintzeig , J. Felde , K. Filimonov , C. Finley , S. Flis , C. -C. Fösig , A. Franckowiak , M. Frère , E. Friedman , T. Fuchs , T. K. Gaisser , J. Gallagher , L. Gerhardt , K. Ghorbani , W. Giang , L. Gladstone , T. Glauch , D. Glowacki , T. Glüsenkamp , A. Goldschmidt , J. G. Gonzalez , D. Grant , Z. Griffith , L. Gustafsson , C. Haack , A. Hallgren , F. Halzen , E. Hansen , T. Hansmann , K. Hanson , J. Haugen , D. Hebecker , D. Heereman , K. Helbing , R. Hellauer , R. Heller , S. Hickford , J. Hignight , G. C. Hill , K. D. Hoffman , R. Hoffmann , K. Hoshina , F. Huang , M. Huber , P. O. Hulth , K. Hultqvist , S. In , M. Inaba , A. Ishihara , E. Jacobi , J. Jacobsen , G. S. Japaridze , M. Jeong , K. Jero , A. Jones , B. J. P. Jones , J. Joseph , W. Kang , A. Kappes , T. Karg , A. Karle , U. Katz , M. Kauer , A. Keivani , J. L. Kelley , J. Kemp , A. Kheirandish , J. Kim , M. Kim , T. Kintscher , J. Kiryluk , N. Kitamura , T. Kittler , S. R. Klein , S. Kleinfelder , M. Kleist , G. Kohnen , R. Koirala , H. Kolanoski , R. Konietz , L. Köpke , C. Kopper , S. Kopper , D. J. Koskinen , M. Kowalski , M. Krasberg , K. Krings , M. Kroll , G. Krückl , C. Krüger , J. Kunnen , S. Kunwar , N. Kurahashi , T. Kuwabara , M. Labare , K. Laihem , H. Landsman , J. L. Lanfranchi , M. J. Larson , F. Lauber , A. Laundrie , D. Lennarz , H. Leich , M. Lesiak-Bzdak , M. Leuermann , L. Lu , J. Ludwig , J. Lünemann , C. Mackenzie , J. Madsen , G. Maggi , K. B. M. Mahn , S. Mancina , M. Mandelartz , R. Maruyama , K. Mase , H. Matis , R. Maunu , F. McNally , C. P. McParland , P. Meade , K. Meagher , M. Medici , M. Meier , A. Meli , T. Menne , G. Merino , T. Meures , S. Miarecki , R. H. Minor , T. Montaruli , M. Moulai , T. Murray , R. Nahnhauer , U. Naumann , G. Neer , M. Newcomb , H. Niederhausen , S. C. Nowicki , D. R. Nygren , A. Obertacke Pollmann , A. Olivas , A. O'Murchadha , T. Palczewski , H. Pandya , D. V. Pankova , S. Patton , P. Peiffer , Ö. Penek , J. A. Pepper , C. Pérez de los Heros , C. Pettersen , D. Pieloth , E. Pinat , P. B. Price , G. T. Przybylski , M. Quinnan , C. Raab , L. Rädel , M. Rameez , K. Rawlins , R. Reimann , B. Relethford , M. Relich , E. Resconi , W. Rhode , M. Richman , B. Riedel , S. Robertson , M. Rongen , C. Roucelle , C. Rott , T. Ruhe , D. Ryckbosch , D. Rysewyk , L. Sabbatini , S. E. Sanchez Herrera , A. Sandrock , J. Sandroos , P. Sandstrom , S. Sarkar , K. Satalecka , P. Schlunder , T. Schmidt , S. Schoenen , S. Schöneberg , A. Schukraft , L. Schumacher , D. Seckel , S. Seunarine , M. Solarz , D. Soldin , M. Song , G. M. Spiczak , C. Spiering , T. Stanev , A. Stasik , J. Stettner , A. Steuer , T. Stezelberger , R. G. Stokstad , A. Stößl , R. Ström , N. L. Strotjohann , K. -H. Sulanke , G. W. Sullivan , M. Sutherland , H. Taavola , I. Taboada , J. Tatar , F. Tenholt , S. Ter-Antonyan , A. Terliuk , G. Tešić , L. Thollander , S. Tilav , P. A. Toale , M. N. Tobin , S. Toscano , D. Tosi , M. Tselengidou , A. Turcati , E. Unger , M. Usner , J. Vandenbroucke , N. van Eijndhoven , S. Vanheule , M. van Rossem , J. van Santen , M. Vehring , M. Voge , E. Vogel , M. Vraeghe , D. Wahl , C. Walck , A. Wallace , M. Wallraff , N. Wandkowsky , Ch. Weaver , M. J. Weiss , C. Wendt , S. Westerhoff , D. Wharton , B. J. Whelan , S. Wickmann , K. Wiebe , C. H. Wiebusch , L. Wille , D. R. Williams , L. Wills , P. Wisniewski , M. Wolf , T. R. Wood , E. Woolsey , K. Woschnagg , D. L. Xu , X. W. Xu , Y. Xu , J. P. Yanez , G. Yodh , S. Yoshida , M. Zoll

The IceCube Collaboration is currently building the world's largest neutrino telescope at the South Pole to observe high energy neutrinos from a variety of astrophysical sources. In this paper we review the current status of the IceCube…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Anthony M Brown

Weakly interacting neutrinos are ideal astronomical messengers because they travel through space without deflection by magnetic fields and, essentially, without absorption. Their weak interaction also makes them notoriously difficult to…

High Energy Astrophysical Phenomena · Physics 2018-08-01 Markus Ahlers , Francis Halzen

The IceCube Neutrino Observatory is a Cherenkov detector located at the South Pole. Its main component consists of an in-ice array of optical modules instrumenting one cubic kilometer of deep Glacial ice. The DeepCore sub-detector is a…

High Energy Astrophysical Phenomena · Physics 2023-06-29 Shiqi Yu

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

IceCube is a cubic kilometer neutrino detector array in the Antarctic ice that was designed to search for astrophysical, high-energy neutrinos. It has detected a diffuse flux of astrophysical neutrinos that appears to be of extragalactic…

High Energy Astrophysical Phenomena · Physics 2021-07-21 Jannis Necker

The IceCube detector, which is embedded in the glacial ice at the geographic South Pole, is the first neutrino telescope to comprise a volume of one cubic kilometer. The search for neutrinos of astrophysical origin is among the primary…

High Energy Astrophysical Phenomena · Physics 2019-08-13 A. Franckowiak