A self-regulated stochastic acceleration model, where fast protons damp the corona's turbulence, reproduces the 30 to 300 TeV proton spectrum inferred from IceCube's NGC 1068 neutrino observations.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Neutrinos from stochastic acceleration in black hole environments
A self-regulated stochastic acceleration model, where fast protons damp the corona's turbulence, reproduces the 30 to 300 TeV proton spectrum inferred from IceCube's NGC 1068 neutrino observations.