High-energy Neutrino Emission from NGC 1068 by Outflow-cloud Interactions
Yong-Han Huang, Kai Wang, Zhi-Peng Ma

TL;DR
This paper proposes an outflow-cloud interaction model in NGC 1068's AGN core to explain its high-energy neutrino emission, suggesting neutrinos originate from shock-accelerated protons interacting with surrounding matter and photons.
Contribution
The study introduces a novel outflow-cloud interaction model that accounts for neutrino production in NGC 1068, aligning theoretical predictions with IceCube observations.
Findings
Neutrino flux matches IceCube data in the 1-30 TeV range.
Predicted gamma-ray emission is suppressed due to photon absorption.
Model explains the high-energy neutrino emission without corresponding gamma-ray signals.
Abstract
As the hottest high-energy neutrino spot, NGC 1068 has received much attention in recent years. Here we focus on the central region of the active galactic nuclei (AGN) and propose an outflow-cloud interaction model that could probably explain the observed neutrino data. Considering the accretion process adjacent to the central supermassive black hole (SMBH) of NGC 1068, strong outflows will be generated, which will likely interact with surrounding clouds floating in the corona region. Particles carried by the outflow will be accelerated to very high energy by the shocks forming during the outflow-cloud interactions. For the accelerated high-energy protons, interactions with the background photon field of the corona and disk and interaction with the surrounding gas will produce considerable high-energy -rays and neutrino. However, because of the extremely dense…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae · Astronomy and Astrophysical Research
