# Cosmic neutrinos from the sources of galactic and extragalactic cosmic rays

@article{Halzen2007CosmicNF,
title={Cosmic neutrinos from the sources of galactic and extragalactic cosmic rays},
author={Francis Halzen},
journal={Astrophysics and Space Science},
year={2007},
volume={309},
pages={407-414}
}
• F. Halzen
• Published 29 November 2006
• Physics
• Astrophysics and Space Science
Abstract Although kilometer-scale neutrino detectors such as IceCube are discovery instruments, their conceptual design is very much anchored to the observational fact that Nature produces protons and photons with energies in excess of 1020 eV and 1013 eV, respectively. The puzzle of where and how Nature accelerates the highest energy cosmic particles is unresolved almost a century after their discovery. From energetics considerations we anticipate on the order of 10–100 neutrino events per…
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## References

SHOWING 1-10 OF 70 REFERENCES
Observation of high-energy atmospheric neutrinos with the Antarctic Muon and Neutrino Detector Array
• Physics
• 2002
The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from
Possible High-Energy Neutrinos from the Cosmic Accelerator RX J1713.7–3946
• Physics
• 2002
The observation of TeV γ-rays of π0 origin from the supernova remnant RX J1713.7-3946 might have revealed the first specific site where protons are accelerated to energies typical of the main
Neutrinos from propagation of ultrahigh-energy protons
• Physics
• 2001
We present a calculation of the production of neutrinos during propagation of ultra-high energy cosmic rays from their astrophysical sources to us. Photoproduction interactions are modeled with the
HIGH-ENERGY NEUTRINO ASTROPHYSICS
• Physics
• 2003
▪ Abstract High-energy (>100 MeV) neutrino astrophysics enters an era of opportunity and discovery as the sensitivity of detectors approaches astrophysically relevant flux levels. We review the major
Ultra-high energy neutrino fluxes: new constraints and implications
• Physics
• 2003
We apply new upper limits on neutrino fluxes and the diffuse extragalactic component of the GeV γ-ray flux to various scenarios for ultra-high energy cosmic rays and neutrinos. As a result we find
Observation of high-energy neutrinos using Čerenkov detectors embedded deep in Antarctic ice
• Physics
Nature
• 2001
The detection of upwardly propagating atmospheric neutrinos by the ice-based Antarctic muon and neutrino detector array (AMANDA) is reported, establishing a technology with which to build a kilometre-scale neutrini observatory necessary for astrophysical observations.
Cosmic rays and particle physics
The study of high energy cosmic rays is a diversified field of observational and phenomenological physics addressing questions ranging from shock acceleration of charged particles in various
Discovery of very-high-energy γ-rays from the Galactic Centre ridge
• Physics
Nature
• 2006
The source of Galactic cosmic rays (with energies up to 1015 eV) remains unclear, although it is widely believed that they originate in the shock waves of expanding supernova remnants. At present the