I do a fair bit of blogging about the technological Singularity, but this post is about one the better known scientific singularities — in this case the singularity that lies at the heart of a black hole and how to go about getting a glimpse of one in all its glory. All that would take is to destroy the black hole that hides the singularity. This physics arXiv blog post is something of an instructional guide on how to go about snuffing out a black hole. Pretty simple in theory, but you know the rest.
From the last link:
In general relativity, the mathematical condition for the existence of a black hole with an event horizon is simple. It is given by the following inequality: M^2 > (J/M)^2 + Q^2, where M is the mass of the black hole, J is its angular momentum and Q is its charge.
Getting rid of the event horizon is simply a question of increasing the angular momentum and/or charge of this object until the inequality is reversed. When that happens the event horizon disappears and the exotic object beneath emerges.
At first sight, that seems straightforward. The inequality suggests that to destroy a black hole, all you need to do is to feed it angular momentum and charge.
To any ordinary physicist, a singularity is an indication that a theory has broken down and some new theory is needed to describe what is going on. It is a matter of principle that singularities are mathematical objects, not physical ones and that any ‘hole’ they suggest exists not in the fabric of the Universe but in our understanding of it.
Astrophysicists are different. They have such extraordinary faith in their theories that they believe singularities actually exist inside black holes. The likes of Roger Penrose and Stephen Hawking have even proved that singularities are inevitable in gravitational collapse.
For them, removing the event horizon around a black hole raises the exciting prospect of revealing a singularity in all its naked glory. When that happens, we will be able to gaze at infinity.