Abstract
We discuss likely sources of cosmic rays in the 1015−1020eV 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.
Original language | English (US) |
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Pages (from-to) | 217-225 |
Number of pages | 9 |
Journal | Nuclear and Particle Physics Proceedings |
Volume | 297-299 |
DOIs | |
State | Published - Apr 1 2018 |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics