Neutrino Astronomy with the IceCube Observatory
Alexander Kappes (for the IceCube Collaboration)
TL;DR
IceCube is a leading neutrino telescope that detects high-energy neutrinos to explore cosmic sources and fundamental physics, providing key results in neutrino astronomy and related fields.
Contribution
This paper presents the latest results from IceCube, highlighting its capabilities and discoveries in high-energy neutrino detection and astrophysics.
Findings
Detection of high-energy astrophysical neutrinos
Constraints on neutrino sources and fluxes
Insights into neutrino properties and astrophysical phenomena
Abstract
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, 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.
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