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Ice Cube: Physics, status, and future
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).
2011 (English)In: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, ISSN 0168-9002, E-ISSN 1872-9576, Vol. 626, s6-S12 p.Article in journal (Refereed) Published
Abstract [en]

The IceCube observatory is the first cubic kilometre scale instrument in the field of high-energy neutrino astronomy and cosmic rays. In 2009, following five successful deployment seasons, IceCube consisted of 59 strings of optical modules in the South Pole ice, together with 118 air shower detectors in the IceTop surface array. The range of physics topics includes neutrino signals from astrophysical sources, dark matter, exotic particle physics, cosmic rays, and atmospheric neutrinos. The current IceCube status and selected results are described. Anticipated future developments are also discussed, in particular the Deep Core low energy subarray which was recently deployed.

Place, publisher, year, edition, pages
2011. Vol. 626, s6-S12 p.
Keyword [en]
IceCube, Neutrino astronomy, Cosmic rays, South pole, Dark matter
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:su:diva-67330DOI: 10.1016/j.nima.2010.05.014ISI: 000286446800003OAI: oai:DiVA.org:su-67330DiVA: diva2:470321
Note
authorCount :1Available from: 2011-12-28 Created: 2011-12-28 Last updated: 2017-12-08Bibliographically approved

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Hultqvist, Klas
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