A population of AGN coronae with magnetization parameters spanning up to σ ~ 10 can reproduce the entire observed diffuse neutrino flux from TeV to PeV energies.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
Bayesian calibration of neutrino-hard X-ray luminosity relation on six AGN shows seven blazars are consistent, with joint permutation test indicating non-random association at 3.23 sigma.
citing papers explorer
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Turbulent AGN coronae as the origin of diffuse neutrinos up to PeV energies
A population of AGN coronae with magnetization parameters spanning up to σ ~ 10 can reproduce the entire observed diffuse neutrino flux from TeV to PeV energies.
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Correlation Between X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars
Bayesian calibration of neutrino-hard X-ray luminosity relation on six AGN shows seven blazars are consistent, with joint permutation test indicating non-random association at 3.23 sigma.