Dissolving Event Horizon w/Charged & Rotating BH

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SUMMARY

The discussion centers on the interaction between rotation and charge in Kerr black holes, specifically regarding the formation of naked singularities. It concludes that adding electrons to a near-extremal rotating black hole requires sufficient mass and energy to prevent the black hole from becoming super-extremal, which is necessary for a naked singularity to form. The combination of rotation and charge does not introduce new qualitative effects, as the mass of the electrons and their kinetic energy counterbalance the angular momentum contributed to the black hole.

PREREQUISITES
  • Understanding of Kerr black holes and their properties
  • Knowledge of general relativity and singularity theories
  • Familiarity with concepts of angular momentum and charge in astrophysics
  • Basic principles of particle physics, specifically electron behavior in gravitational fields
NEXT STEPS
  • Research the properties of near-extremal Kerr black holes
  • Study the implications of charged black holes in general relativity
  • Explore the concept of naked singularities and their theoretical foundations
  • Investigate the role of mass and energy in black hole dynamics
USEFUL FOR

Astronomers, theoretical physicists, and students of astrophysics interested in black hole dynamics and the implications of charge and rotation on singularity formation.

arusse02
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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.
 
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arusse02 said:
I saw a fascinating video from PBS space time

This is a pop science video and is not a good source for learning the actual physics.

arusse02 said:
The video addresses rotating kerr black holes and charged black holes, but doesn't talk about the combination of rotation and charge.

Combining rotation and charge doesn't add anything qualitatively new.

arusse02 said:
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?

Yes. When you work out the details, it turns out that however you try to add angular momentum or charge to a near-extremal hole, you have to add enough mass along with it to keep the hole from becoming super-extremal (which is what would be required to form a naked singularity).
 
arusse02 said:
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?
The electrons have mass, and need kinetic energy if they are going to contribute angular momentum. That mass and energy contribute to the mass of the hole at least as much as is necessary to keep it from becoming super-extremal. And as you add electrons and the black hole becomes charged you have to give the electrons more energy to get them to the event horizon, since like charges repel.
 

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