Kent State Descending the Gravity Well: An Analysis of the Observer

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According to the Kerr-Newman model of a rotating black hole, there is a region just outside the event horizon where certain space and time vectors switch properties with each other. This is just mathematics, you understand, merely a quirk of the formulas — physically, nothing changes wildly until you get inside the black hole itself, and then who cares what happens? Double-deluxe chocolate-chip cookies could spontaneously spring into being and it wouldn’t matter to the universe outside. Reality may break down inside a black hole, but the effects never percolate back into our familiar space.

Just outside the black hole, however, if it’s rotating, if the model is correct, there is a region called the ergosphere where certain vector fields describing the flow of space and time do a flip-flop. When I was trying to understand what this meant, I told myself that places became moments and moments became places.

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