High-Energy neutrinos from extragalactic cosmic-ray sources

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

High-energy neutrinos, which can uniquely identify the production of hadronic cosmic rays and especially probe dense sources, are detectable by the nearly-completed IceCube and the planned KM3Net. We discuss high-energy neutrino emission from powerful extragalactic cosmic-ray accelerators such as active galaxies, gamma-ray bursts, clusters of galaxies and magnetars. We take a view of future prospects for those potential neutrino sources.

Original languageEnglish (US)
Pages (from-to)291-293
Number of pages3
JournalNuclear Physics B - Proceedings Supplements
Volume217
Issue number1
DOIs
StatePublished - Aug 1 2011

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cosmic rays
neutrinos
magnetars
active galaxies
gamma ray bursts
energy
accelerators
galaxies
probes

All Science Journal Classification (ASJC) codes

  • Atomic and Molecular Physics, and Optics
  • Nuclear and High Energy Physics

Cite this

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abstract = "High-energy neutrinos, which can uniquely identify the production of hadronic cosmic rays and especially probe dense sources, are detectable by the nearly-completed IceCube and the planned KM3Net. We discuss high-energy neutrino emission from powerful extragalactic cosmic-ray accelerators such as active galaxies, gamma-ray bursts, clusters of galaxies and magnetars. We take a view of future prospects for those potential neutrino sources.",
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High-Energy neutrinos from extragalactic cosmic-ray sources. / Murase, Kohta.

In: Nuclear Physics B - Proceedings Supplements, Vol. 217, No. 1, 01.08.2011, p. 291-293.

Research output: Contribution to journalArticle

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