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arXiv · 1703.00890

Multi-Messenger Signatures of PeV-ZeV Cosmic Ray Sources

Peter Mészáros·Kohta Murase·Katsuaki Asano·Nicholas Senno·Di Xiao
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Abstract

We discuss likely sources of cosmic rays in the $10^{15}-10^{20}$ 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.

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Peter Mészáros, Kohta Murase, Katsuaki Asano, Nicholas Senno, Di Xiao. 2017-03-02. Multi-Messenger Signatures of PeV-ZeV Cosmic Ray Sources. https://doi.org/10.1016/j.nuclphysbps.2018.07.031

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