The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part II: Properties of the Atmospheric and Astrophysical Neutrino Flux
IceCube Collaboration: M. G. Aartsen, M. Ackermann, J. Adams, J. A., Aguilar, M. Ahlers, M. Ahrens, I. Al Samarai, D. Altmann, K. Andeen, T., Anderson, I. Ansseau, G. Anton, C. Arg\"uelles, J. Auffenberg, S. Axani, H., Bagherpour, X. Bai, J. P. Barron, S. W. Barwick, V. Baum
TL;DR
This paper discusses the properties of atmospheric and astrophysical neutrino fluxes as studied by the IceCube Neutrino Observatory, providing insights into neutrino origins and behaviors relevant to cosmic ray physics.
Contribution
It presents new measurements and analyses of neutrino flux properties from IceCube data, enhancing understanding of neutrino sources and their energy spectra.
Findings
Detection of high-energy astrophysical neutrinos
Characterization of atmospheric neutrino fluxes
Constraints on neutrino source models
Abstract
Papers on the properties of the atmospheric and astrophysical neutrino flux submitted to the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the IceCube Collaboration
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Neutrino Physics Research