# Backflows by AGN jets: Global properties and influence on SMBH accretion

## TL;DR

This study investigates how AGN jet-induced backflows influence the gas dynamics and accretion processes near supermassive black holes, revealing their intermittent nature and potential to significantly modulate jet power.

## Contribution

It provides the first detailed numerical and analytical analysis of AGN jet backflows, linking their properties to jet parameters and their impact on SMBH accretion and jet variability.

## Key findings

- Backflows are spatially coherent and intermittent regardless of jet power.
- Backflows can enhance SMBH accretion rates by up to ten times during episodes.
- Backflows influence the density profile of the circumnuclear disk, creating a flat core.

## Abstract

Jets from Active Galactic Nuclei (AGN) inflate large cavities in the hot gas environment around galaxies and galaxy clusters. The large-scale gas circulation promoted within such cavities by the jet itself gives rise to backflows that propagate back to the center of the jet-cocoon system, spanning all the physical scales relevant for the AGN. Using an Adaptive Mesh Refinement code, we study these backflows through a series of numerical experiments, aiming at understanding how their global properties depend on jet parameters. We are able to characterize their mass flux down to a scale of a few kiloparsecs to about $0.5\,\mathrm{M_\odot/y}$for as long as $15$ or $20$ Myr, depending on jet power. We find that backflows are both spatially coherent and temporally textbf{intermittent}, independently of jet power in the range $10^{43-45}$ erg/s. Using the mass flux thus measured, we model analytically the effect of backflows on the central accretion region, where a Magnetically Arrested Disk lies at the center of a thin circumnuclear disk. Backflow accretion onto the disk modifies its density profile, producing a flat core and tail. We use this analytic model to predict how accretion beyond the BH magnetopause is modified, and thus how the jet power is temporally modulated. Under the assumption that the magnetic flux stays frozen in the accreting matter, and that the jets are always launched via the Blandford-Znajek (1977) mechanism, we find that backflows are capable of boosting the jet power up to tenfold during relatively short time episodes (a few Myr).