Astrophysical origin of high-energy cosmic neutrinos

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The origin of high-energy cosmic neutrinos is a new interesting mystery in astroparticle physics. The present data suggest interesting connection to cosmic-ray and/or gamma-ray sources. We review various scenarios for the cosmic neutrinos, and emphasize the importance of multimessenger approaches to reveal the sources.

Original languageEnglish (US)
Title of host publicationISVHECRI 2014 - 18th International Symposium on Very High Energy Cosmic Ray Interactions
EditorsAlbert de Roeck, Michelangelo Mangano, David Berge, Bryan Pattison
PublisherEDP Sciences
ISBN (Electronic)9782759817221
DOIs
StatePublished - Aug 4 2015
Event18th International Symposium on Very High Energy Cosmic Ray Interactions, ISVHECRI 2014 - Geneva, Switzerland
Duration: Aug 18 2014Aug 22 2014

Publication series

NameEPJ Web of Conferences
Volume99
ISSN (Print)2101-6275
ISSN (Electronic)2100-014X

Other

Other18th International Symposium on Very High Energy Cosmic Ray Interactions, ISVHECRI 2014
CountrySwitzerland
CityGeneva
Period8/18/148/22/14

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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  • Cite this

    Murase, K. (2015). Astrophysical origin of high-energy cosmic neutrinos. In A. de Roeck, M. Mangano, D. Berge, & B. Pattison (Eds.), ISVHECRI 2014 - 18th International Symposium on Very High Energy Cosmic Ray Interactions [05001] (EPJ Web of Conferences; Vol. 99). EDP Sciences. https://doi.org/10.1051/epjconf/20159905001