Developments in High Energy Neutrino Astronomy
Astrophysics
2016-08-30 v1
Abstract
Nature produces cosmic ray particles, probably protons, with energies well above eV -- how are they produced? Where do they come from? Gamma rays with energies above eV are produced in jets of active galaxies -- are these produced by energetic electrons or protons? What is the correct model of Gamma Ray Bursts? These are just some of the fundamental questions in high energy astrophysics to be answered by observations made with large area neutrino telescopes.
Cite
@article{arxiv.astro-ph/9907374,
title = {Developments in High Energy Neutrino Astronomy},
author = {R. J. Protheroe},
journal= {arXiv preprint arXiv:astro-ph/9907374},
year = {2016}
}
Comments
Short invited article to appear in Europhysics News (1 page, 1 figure)