- #1
arusse02
- 24
- 0
I saw a fascinating video from PBS space time about dissolving an event horizon. See here for reference:
The video addresses rotating kerr black holes and charged black holes, but doesn't talk about the combination of rotation and charge. So what happens when you spin up the black hole as much as possible so that its an extremel black hole, and then on top of that you start adding electrons with such a trajectory that it still contributes angular momentum? Does the outward pressure of the black hole rotation and the charge combine, thus letting us easily produce a naked singularity? Or is there some effect such that adding electrons to a rotating kerr black hole would somehow expand the event horizon just enough to prevent a naked singularity? Thanks.
The video addresses rotating kerr black holes and charged black holes, but doesn't talk about the combination of rotation and charge. So what happens when you spin up the black hole as much as possible so that its an extremel black hole, and then on top of that you start adding electrons with such a trajectory that it still contributes angular momentum? Does the outward pressure of the black hole rotation and the charge combine, thus letting us easily produce a naked singularity? Or is there some effect such that adding electrons to a rotating kerr black hole would somehow expand the event horizon just enough to prevent a naked singularity? Thanks.