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 language | English (US) |
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Pages (from-to) | 291-293 |
Number of pages | 3 |
Journal | Nuclear Physics B - Proceedings Supplements |
Volume | 217 |
Issue number | 1 |
DOIs | |
State | Published - Aug 2011 |
All Science Journal Classification (ASJC) codes
- Atomic and Molecular Physics, and Optics
- Nuclear and High Energy Physics