GZK Neutrinos after the Fermi-LAT Diffuse Photon Flux Measurement
Cosmogenic neutrinos originate from photo-hadronic interactions of cosmic ray protons with the cosmic microwave background (CMB). The neutrino production rate can be constrained through the accompanying electrons, positrons and gamma-rays that quickly cascade on the CMB and intergalactic magnetic fi...
| Main Authors: | , , , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2010
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