pith. sign in

arxiv: astro-ph/0607515 · v3 · submitted 2006-07-24 · 🌌 astro-ph

Ultra high energy neutrinos: the key to ultra high energy cosmic rays

classification 🌌 astro-ph
keywords energyhighultracosmicneutrinossourcesaccelerationcosmogenic
0
0 comments X
read the original abstract

We discuss the relation between the acceleration spectra of extragalactic cosmic ray protons and the luminosity and cosmological evolution of their sources and the production of ultra high energy cosmogenic neutrinos in their propagation from the sources to us.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.