Multi-Messenger Signatures of PeV-ZeV Cosmic Ray Sources

Peter Mészáros, Kohta Murase, Katsuaki Asano, Nicholas Senno, Di Xiao

Research output: Contribution to journalArticle

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 languageEnglish (US)
Pages (from-to)217-225
Number of pages9
JournalNuclear and Particle Physics Proceedings
Volume297-299
DOIs
StatePublished - Apr 1 2018

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cosmic rays
signatures
gamma ray bursts
neutrinos
shock
luminosity
gamma rays
physics
energy

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics

Cite this

Mészáros, Peter ; Murase, Kohta ; Asano, Katsuaki ; Senno, Nicholas ; Xiao, Di. / Multi-Messenger Signatures of PeV-ZeV Cosmic Ray Sources. In: Nuclear and Particle Physics Proceedings. 2018 ; Vol. 297-299. pp. 217-225.
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Multi-Messenger Signatures of PeV-ZeV Cosmic Ray Sources. / Mészáros, Peter; Murase, Kohta; Asano, Katsuaki; Senno, Nicholas; Xiao, Di.

In: Nuclear and Particle Physics Proceedings, Vol. 297-299, 01.04.2018, p. 217-225.

Research output: Contribution to journalArticle

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