A two-zone model for blazar emission: implications for TXS 0506+056 and the neutrino event IceCube-170922A

TL;DR

This paper proposes a two-zone model for blazar TXS 0506+056 that better explains neutrino and gamma-ray emissions, predicting higher neutrino fluxes and aiding future observational differentiation.

Contribution

It introduces a two-zone emission model separated by the broad line region, improving neutrino flux estimates over traditional one-zone models.

Findings

Two-zone model predicts higher neutrino flux (~10^{-11} erg cm^{-2} s^{-1})

Different zones suppress X-ray electromagnetic cascades

Next-generation neutrino telescopes can distinguish models

Abstract

A high-energy muon neutrino event, IceCube-170922A, was recently discovered in both spatial and temporal coincidence with a gamma-ray flare of the blazar TXS 0506+056. It has been shown, with standard one-zone models, that neutrinos can be produced in the blazar jet via hadronic interactions, but with a flux which is mostly limited by the X-ray data. In this work, we explore the neutrino production from TXS 0506+056 by invoking two physically distinct emission zones in the jet, separated by the broad line region (BLR). Using the Doppler-boosted radiation of the BLR as the target photon field, the inner zone accounts for the neutrino and gamma-ray emission via $p\gamma$ interactions and inverse Compton scattering respectively, while the outer zone produces the optical and X-ray emission via synchrotron and synchrotron self-Compton processes. The different conditions of the two zones allow us to suppress the X-ray emission from the electromagnetic cascade, and set a much higher upper limit on the muon neutrino flux (i.e., $\sim 10^{-11}\rm erg~cm^{-2}s^{-1}$) than in one-zone models. We compare, in detail, our scenario with one-zone models discussed in the literature, and argue that differentiating between such scenarios will become possible with next generation neutrino telescopes, such as IceCube-Gen2.