Diffuse PeV neutrinos from EeV cosmic ray sources: Semirelativistic hypernova remnants in star-forming galaxies
- Phys.Rev.D 89 (2014) 8, 083004
- Published: Apr 8, 2014
- 1310.1263 [astro-ph.HE]
Citations per year
We argue that the excess of sub-PeV/PeV neutrinos recently reported by IceCube could plausibly originate through pion-production processes in the same sources responsible for cosmic rays (CRs) with energy above the second knee around
- 9 pages, 2 figures; large amount of content added; PRD accepted
- 95.85.Ry
- 98.58.Mj
- 98.70.Sa
- p: target
- gamma ray: background
- gamma ray: flux
- target: density
- cosmic radiation
- hypernova
- IceCube
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