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3 Pith papers cite this work, alongside 65 external citations. Polarity classification is still indexing.

3 Pith papers citing it
65 external citations · OpenAlex

fields

astro-ph.HE 3

years

2026 3

representative citing papers

Locating the Production Sites of High-Energy Neutrinos in Blazar Jets

astro-ph.HE · 2026-06-01 · conditional · novelty 6.0

Efficient neutrino production in blazar jets requires an external radiation field that strongly dominates the magnetic field (Y>>1), which radio constraints place near the broad-line region and only for uncommon jet acceleration or beaming conditions.

Active Galactic Nuclei as high-energy neutrino sources

astro-ph.HE · 2026-06-29 · accept · novelty 2.5

AGN (jetted and non-jetted) are viable high-energy neutrino sources, with TXS 0506+056 and NGC 1068 as the only statistically significant associations so far, while gamma-ray blazars contribute only a small fraction of the diffuse flux.

citing papers explorer

Showing 3 of 3 citing papers.

  • On the maximum neutrino flux of blazars in the one-zone leptohadronic model astro-ph.HE · 2026-05-22 · unverdicted · none · ref 3

    An analytical derivation of maximum neutrino flux in the one-zone leptohadronic model shows predicted fluxes remain below IceCube levels for neutrino-candidate blazars.

  • Locating the Production Sites of High-Energy Neutrinos in Blazar Jets astro-ph.HE · 2026-06-01 · conditional · none · ref 7

    Efficient neutrino production in blazar jets requires an external radiation field that strongly dominates the magnetic field (Y>>1), which radio constraints place near the broad-line region and only for uncommon jet acceleration or beaming conditions.

  • Active Galactic Nuclei as high-energy neutrino sources astro-ph.HE · 2026-06-29 · accept · none · ref 179

    AGN (jetted and non-jetted) are viable high-energy neutrino sources, with TXS 0506+056 and NGC 1068 as the only statistically significant associations so far, while gamma-ray blazars contribute only a small fraction of the diffuse flux.