High-energy Neutrinos from Stellar Explosions in Active Galactic Nuclei Accretion Disks

TL;DR

This paper investigates how stellar explosions within active galactic nuclei disks can produce high-energy neutrinos, potentially contributing up to 10% of the diffuse neutrino background, and highlights their importance for multimessenger astronomy.

Contribution

It introduces the idea that AGN stellar explosions are efficient neutrino sources and explores their potential contribution to the diffuse neutrino background.

Findings

High-energy neutrinos can be produced via $pp$-interactions after AGN stellar explosions.

AGN stellar explosions could account for up to 10% of the observed diffuse neutrino background.

AGN stellar explosions are promising targets for joint neutrino and electromagnetic observations.

Abstract

Some catastrophic stellar explosions, such as supernovae (SNe), compact binary coalescences, and micro-tidal disruption events, are believed to be embedded in the accretion disks of active galactic nuclei (AGN). We show high-energy neutrinos can be produced efficiently through $pp$-interactions between shock-accelerated cosmic rays and AGN disk materials shortly after the explosion ejecta shock breaks out of the disk. AGN stellar explosions are ideal targets for joint neutrino and electromagnetic (EM) multimessenger observations. Future EM follow-up observations of neutrino bursts can help us search for yet-discovered AGN stellar explosions. We suggest that AGN stellar explosions could potentially be important astrophysical neutrino sources. The contribution from AGN stellar explosions to the observed diffuse neutrino background depends on the uncertain local event rate densities of these events in AGN disks. By considering thermonuclear SNe, core-collaspe SNe, gamma-ray burst associated SNe, kilonovae, and choked GRBs in AGN disks with known theoretical local event rate densities, we show that these events may contribute to $\lesssim10\%$ of the observed diffuse neutrino background.