Visualization of simulations with and without BH feedback physics, each from a snapshot when a BH is undergoing rapid growth. Left two zoom-in plots: Gas morphology for the 10⁶ M_⊙ GMCs without (top) or with (bottom) BH feedback. From left to right, we zoom into a BH undergoing hyper-Eddington accretion. As the smallest scale, each panel shows the velocity field near the BH, with the circular velocity ($\sqrt{G{M}_{\mathrm{cl}}/R_{\mathrm{cl}}}$) presented as a gauge. Right two zoom-in plots: Same as the left plots, but for the 10⁸ M_⊙ GMC.