Multi-Messenger Signatures of PeV-ZeV Cosmic Ray Sources
Abstract
We discuss likely sources of cosmic rays in the eV range and their possible very high energy neutrino and gamma-ray signatures which could serve to identify these sources and constrain their physics. Among these sources we discuss in particular low luminosity gamma-ray bursts, including choked and shock-breakout objects, tidal disruption events and white dwarf mergers. Among efforts aimed at simultaneous secondary multi-messenger detections we discuss the AMON program.
Cite
@article{arxiv.1703.00890,
title = {Multi-Messenger Signatures of PeV-ZeV Cosmic Ray Sources},
author = {Peter Mészáros and Kohta Murase and Katsuaki Asano and Nicholas Senno and Di Xiao},
journal= {arXiv preprint arXiv:1703.00890},
year = {2019}
}
Comments
9 pages; Based on a talk given at the Origin of Cosmic Rays: Beyond the Standard Model 2016 conference in San Vito di Cadore, Dolomites; This is not a comprehensive review; it is weighted towards work the author has been more personally involved with. Fig 3 has been updated to reflect the published work