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Spinning supermassive black holes (BHs) in active galactic nuclei (AGN)magnetically launch relativistic collimated outflows, or jets. Without angularmomentum supply, such jets are thought to perish within $3$ orders of magnitudein distance from the BH, well before reaching kpc-scales. We study the survivalof such jets at the largest scale separation to date, via 3D generalrelativistic magnetohydrodynamic simulations of rapidly spinning BHs immersedinto uniform zero-angular-momentum gas threaded by weak vertical magneticfield. We place the gas outside the BH sphere of influence, or the Bondiradius, chosen much larger than the BH gravitational radius,$R_\text{B}=10^3R_\text{g}$. The BH develops dynamically-important large-scalemagnetic fields, forms a magnetically-arrested disk (MAD), and launchesrelativistic jets that propagate well outside $R_\text{B}$ and suppress BHaccretion to $1.5\%$ of the Bondi rate, $\dot{M}_\text{B}$. Thus,low-angular-momentum accretion in the MAD state can form large-scale jets inFanaroff-Riley (FR) type I and II galaxies. Subsequently, the disk shrinks andexits the MAD state: barely a disk (BAD), it rapidly precesses, whips the jetsaround, globally destroys them, and lets $5-10\%$ of $\dot{M}_\text{B}$ reachthe BH. Thereafter, the disk starts rocking back and forth by angles$90-180^\circ$: the rocking accretion disk (RAD) launches weak intermittentjets that spread their energy over a large area and suppress BH accretion to$\lesssim 2 \% ~ \dot{M}_\text{B}$. Because BAD and RAD states tangle up thejets and destroy them well inside $R_\text{B}$, they are promising candidatesfor the more abundant, but less luminous, class of FR0 galaxies.

Jets with a Twist: Emergence of FR0 Jets in 3D GRMHD Simulation of Zero Angular Momentum Black Hole Accretion