Disk magnetic fields in magnetically arrested AGN disks can confine the jet cocoon, sharpen jet collimation, and slightly speed up jet heads, boosting breakout emission for low-power jets.
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Impact of disk magnetic fields on the propagation of stellar-scale jets in the magnetically arrested accretion disks of active galactic nuclei
Disk magnetic fields in magnetically arrested AGN disks can confine the jet cocoon, sharpen jet collimation, and slightly speed up jet heads, boosting breakout emission for low-power jets.