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High-Energy Neutrinos from Photomeson Processes in Blazars

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abstract

An important radiation field for photomeson neutrino production in blazars is shown to be the radiation field external to the jet. Assuming that protons are accelerated with the same power as electrons and injected with a -2 number spectrum, we predict that km^2 neutrino telescopes will detect about 1-to-several neutrinos per year from flat spectrum radio quasars (FSRQs) such as 3C 279. The escaping high-energy neutron and photon beams transport inner jet energy far from the black-hole engine, and could power synchrotron X-ray jets and FR II hot spots and lobes.

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astro-ph.HE 1

years

2026 1

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UNVERDICTED 1

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TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane

astro-ph.HE · 2026-06-22 · unverdicted · novelty 3.0

Alternative ISRF models produce only modest changes to the LHAASO diffuse gamma-ray fit; the associated pp neutrinos remain consistent with IceCube all-sky data and compatible with ANTARES/KM3NeT limits.

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  • TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane astro-ph.HE · 2026-06-22 · unverdicted · none · ref 26 · internal anchor

    Alternative ISRF models produce only modest changes to the LHAASO diffuse gamma-ray fit; the associated pp neutrinos remain consistent with IceCube all-sky data and compatible with ANTARES/KM3NeT limits.