Abstract
IceCube is the first representative of the km3 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, but it is also an excellent detector for the investigation of a variety of other highly topical astrophysics and particle physics topics like supernovae, dark matter and neutrino oscillations. After an introduction to neutrino astronomy and neutrino telescopes, this article presents a selection of latest results from the IceCube neutrino detector with respect to searches for cosmic high-energy neutrino sources.
Cite
CITATION STYLE
Kappes, A. (2013). Neutrino astronomy with the IceCube observatory. In Journal of Physics: Conference Series (Vol. 409). Institute of Physics Publishing. https://doi.org/10.1088/1742-6596/409/1/012014
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