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Astrophysical neutrinos and cosmic rays observed by IceCube
Univ Adelaide, Dept Phys, Adelaide, SA 5005, Australia.
DESY, D-15735 Zeuthen, Germany.
Univ Canterbury, Dept Phys & Astron, Private Bag 4800, Christchurch, New Zealand.
Univ Libre Bruxelles, Sci Fac, CP230, B-1050 Brussels, Belgium.
Vise andre og tillknytning
2018 (engelsk)Inngår i: Advances in Space Research, ISSN 0273-1177, E-ISSN 1879-1948, Vol. 62, nr 10, s. 2902-2930Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

The core mission of the IceCube neutrino observatory is to study the origin and propagation of cosmic rays. IceCube, with its surface component IceTop, observes multiple signatures to accomplish this mission. Most important are the astrophysical neutrinos that are produced in interactions of cosmic rays, close to their sources and in interstellar space. IceCube is the first instrument that measures the properties of this astrophysical neutrino flux and constrains its origin. In addition, the spectrum, composition, and anisotropy of the local cosmic-ray flux are obtained from measurements of atmospheric muons and showers. Here we provide an overview of recent findings from the analysis of IceCube data, and their implications to our understanding of cosmic rays.

sted, utgiver, år, opplag, sider
2018. Vol. 62, nr 10, s. 2902-2930
Emneord [en]
IceCube, Neutrinos, Cosmic rays
HSV kategori
Identifikatorer
URN: urn:nbn:se:uu:diva-371533DOI: 10.1016/j.asr.2017.05.030ISI: 000449448700012OAI: oai:DiVA.org:uu-371533DiVA, id: diva2:1273498
Forskningsfinansiär
Swedish Research CouncilSwedish National Infrastructure for Computing (SNIC)Knut and Alice Wallenberg FoundationAustralian Research CouncilTilgjengelig fra: 2018-12-21 Laget: 2018-12-21 Sist oppdatert: 2019-05-21bibliografisk kontrollert

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Botner, OlgaBurgman, AlexanderEuler, SebastianHallgren, Allande los Heros, CarlosStröm, RickardTaavola, HenricUnger, Elisabeth

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