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I'm sorry but I don't understand what you wrote here. Please rephrase for clarification for me. Thank you.
However one can look at a black hole as a collapsed star whose matter never makes it into the event horizon because it gets frozen just at or outside the event horizon, as the link I providewd above suggests.
Assuming a rotating black hole has an accretion disk from which matter spirals down, 'spiral inflow, to the horizon, my question…If your saying matter never makes it into the event horizon and is ‘frozen’ at/outside the event horizon, then are we allowed to think any future or later matter that spirals down from the accretion disk will never be seen to reach the horizon but is accumulating at the end point of the spiral inflow near the horizon?
Thus, I suggested wouldn’t this make the shape of the black hole non-symmetrical?