PoS - Proceedings of Science
Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Neutrino. NU-astrophysical neutrinos
Solar atmospheric neutrino search with IceCube
S. In, M. Jeong*  on behalf of the IceCube Collaboration
Full text: pdf
Pre-published on: August 16, 2017
Published on: August 03, 2018
Cosmic rays interacting in the solar atmosphere can produce high energy neutrinos, which could be detected with IceCube. Neutrinos are produced through the decay of pions and kaons, similar to cosmic ray air showers in the Earth’s atmosphere. Due to the lower solar atmospheric density, the neutrino spectrum from the Sun is expected to be harder as mesons tend to decay before they can interact or encounter any significant energy loss. The solar disk neutrino flux could be visible over the atmospheric backgrounds at energies above a few hundred GeV. We present IceCube’s sensitivity as determined by a dedicated analysis for solar atmospheric neutrinos.
DOI: https://doi.org/10.22323/1.301.0965
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.