Origin Of The High Energy Cosmic Neutrino Background
arXiv:1405.5487 · doi:10.1103/PhysRevLett.113.191102
Abstract
The diffuse background of very high energy extra-terrestrial neutrinos recently discovered with IceCube is compatible with that expected from cosmic ray interactions in the Galactic interstellar medium plus that expected from hadronic interactions near source and in the intergalactic medium of the cosmic rays which have been accelerated by the jets that produce gamma ray bursts (GRBs).
Version accepted for publication in PRL
References in corpus (5)
- Cold Dark Clouds: The Initial Conditions for Star Formation
- The Galaxy Population Hosting Gamma-Ray Bursts
- Time-Integrated Searches for Point-like Sources of Neutrinos with the 40-String IceCube Detector
- Ankle-like Feature in the Energy Spectrum of Light Elements of Cosmic Rays Observed with KASCADE-Grande
- A theory of Cosmic Rays
Cited by in corpus (4)
- Spectral analysis of the high-energy IceCube neutrinos
- Diffuse neutrinos from extragalactic supernova remnants: Dominating the 100 TeV IceCube flux
- Probing decaying heavy dark matter with the 4-year IceCube HESE data
- Star-forming galaxies as the origin of IceCube neutrinos: Reconciliation with Fermi-LAT gamma rays