TY - JOUR
T1 - Multi-Messenger Signatures of PeV-ZeV Cosmic Ray Sources
AU - Mészáros, Peter
AU - Murase, Kohta
AU - Asano, Katsuaki
AU - Senno, Nicholas
AU - Xiao, Di
N1 - Funding Information:
In summary, while cosmic rays and neutrinos are notoriously elusive preys, new observations throughout the next decade can be expected to lead to signifi- cant advances in our understanding of both UHECRs and their multi-messenger secondaries, as well as in the implications they bear for the physical nature of their sources. Acknowledgments: P.M. is grateful to the organizers of the 2nd “Cosmic Ray Origin - Beyond the Standard Models” conference in San Vito di Cadore, Dolomites, Italy (2016); and to NASA NNX 13AH50G for partial support.
Publisher Copyright:
© 2018 Elsevier B.V.
PY - 2018/4/1
Y1 - 2018/4/1
N2 - 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.
AB - 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.
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U2 - 10.1016/j.nuclphysbps.2018.07.031
DO - 10.1016/j.nuclphysbps.2018.07.031
M3 - Article
AN - SCOPUS:85055325161
SN - 2405-6014
VL - 297-299
SP - 217
EP - 225
JO - Nuclear and Particle Physics Proceedings
JF - Nuclear and Particle Physics Proceedings
ER -