I’ve had the pleasure to attend a talk by Dr. Ian Vega, who works as a theoretical physicist specializing in relativity. The talk was about their most recent paper at the time, which dealt with cosmic censorship.
The whole topic is interesting. Dr. Vega’s work was on extremal Reissner-Nordstrom black holes (black holes with a lot of charge).
The problem was that, if you had a black hole with enough charge, the EM repulsion could overpower the gravitational attraction, like so (excuse my Paint skills):
No matter how close you get to the black hole, charged particles would ALWAYS be repelled. So, there would exist certain charged particles that could get arbitrarily close to the singularity and still be emitted. The singularity could thus be readily seen/measured: a naked singularity.
Thankfully, such a black hole could not form spontaneously; you couldn’t pull that much charged material into such a confined space without them repelling each other and eventually flying off.
BUT, someone thought, what if you had a black hole with just barely enough charge, then throw in a charged particle?
The charged particle could tip the near-critical BH into nakedness: NOT GOOD.
But, as Dr. Ian Vega and his colleagues discovered (through very heavy math I didn’t understand), you couldn’t really throw in any charged particles, because the Lorentz self-force would actually push those particles out.
[details=Spoiler]Lorentz self-force is pretty complicated, but essentially it’s that when a charged particle moves, it causes a change in the electric field around it, which in turn causes a magnetic field to appear around it.
A charged particle moving through a magnetic field experiences a magnetic force. This magnetic force is given this special name, Lorentz self-force, because it looks as if the particle is applying a force on itself.
And as it turns out, in our scenario, this self force can directly oppose the motion of the particle itself.[/details]
So, it turns out we still can’t actually make a naked singularity, even when we try to cheat. Dr. Vega and his colleagues assert that this analysis can also be applied to overspinning Kerr black holes.
[details=Spoiler]Kerr black holes are black holes with a lot of spin angular momentum, as opposed to Reissner-Nordstrom black holes with a lot of charge.
There had also been arguments in which throwing in a spinning particle into a near-extremal Kerr black hole could create a naked singularity, but as Dr. Vega and his colleagues showed, this still wouldn’t be the case (spinning particles also experience a kind of self-force, but with a totally different mechanism from the Lorentz electromagnetic self-force).[/details]