Ultra-high Energy Cosmic Rays and Neutrinos from Gamma-Ray Bursts, Hypernovae and Galactic Shocks
arXiv:1407.5671 · doi:10.1016/j.nuclphysbps.2014.10.028
Abstract
I review gamma-ray burst models (GRBs) and observations, and discuss the possible production of ultra-high energy cosmic rays and neutrinos in both the standard internal shock models and the newer generation of photospheric and hadronic GRB models, in the light of current constraints imposed by IceCube, Auger and TA observations. I then discuss models that have been proposed to explain the recent astrophysical PeV neutrino observations, including star-forming and star-burst galaxies, hypernovae and galaxy accretion and merger shocks.
13 pages, 10 figures. Based on a talk given at the "Cosmic Ray Origins: Beyond the Standard Models" international conference in San Vito di Cadore, Dolomites, Italy, 16-22 March 2014. To be published in the conference proceedings, in Nucl. Phys. B; Editors: O. Tibolla, L. Drury, M. Persic, S. Kaufmann, H. Voelk, K. Mannheim and A. de Angelis
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Cited by in corpus (8)
- Constraining High-Energy Cosmic Neutrino Sources: Implications and Prospects
- Extragalactic star-forming galaxies with hypernovae and supernovae as high-energy neutrino and gamma-ray sources: the case of the 10 TeV neutrino data
- Identifying Ultrahigh-Energy Cosmic-Ray Accelerators with Future Ultrahigh-Energy Neutrino Detectors
- High-Energy Neutrino Emission from White Dwarf Mergers
- Hadronic origin of multi-TeV gamma rays and neutrinos from low-luminosity active galactic nuclei: implications of past activities of the Galactic center
- Constraints to a Galactic Component of the Ice Cube cosmic neutrino flux from ANTARES
- Search for Blazar Flux-Correlated TeV Neutrinos in IceCube 40-String Data
- Obscured flat spectrum radio AGN as sources of high-energy neutrinos