Chronos said:
The Swarzschild radius gives you the basic relationship.
To expand on this response (to make it even vaguely useful), the event horizon, photon sphere, and other interesting surfaces can all be easily calculated in GR for any type of black hole---with the different surfaces generally expressed in terms of the Schwarzschild radius (and other fundamental parameters, i.e. spin and charge).
Chalnoth said:
I don't think we can realistically trust General Relativity to give the correct answer to the behavior of a black hole inside the event horizon, unfortunately.
Just to clarify, GR Is well behaved within the event horizon, its only near the singularity that it breaks down. In the case of a rotating or charged black hole, it can be a little worse.
bill alsept said:
The fact that its g has an escape velocity of c doesn’t necessarily mean the body of the black hole has to be a point.
According to GR, the central mass
does need to be a point. Not only is the escape velocity equal to 'c'; but also, space-time is so distorted inside the event horizon that the only direction a particle can move is inward (i.e. its 'impossible' to even stay still--like on a hard surface).
bill alsept said:
Why is pressure required to keep the matter collapsing? Did you mean keep the matter FROM collapsing? If something becomes 100% dense (as I believe the singularity to be) and cannot get any denser then how can it collapse any farther? And why would it need pressure to keep it from collapsing?
He did mean "keep the matter 'from' collapsing". Pressure is always required to keep material from collapsing. The reason the Earth doesn't collapse, or the air in the room, or the table your typing on---are because of pressure. Once inside the event horizon there
is no pressure strong enough to resist collapse (according to general relativity). There is no such thing as '100%' dense---something can become arbitrarily dense because it can become arbitrarily small.
People think that a new
quantum theory of gravity might be able to explain what actually happens at the singularity. Most string theorists, for example, think that at some point the matter
will reach a maximum density (and minimum size), at about the Planck scale---\sim 10^{-35} m; but no one really knows.
An additional thing to note is that charged and rotating black-holes have singularities that aren't points. A rotating black hole (called a "Kerr black hole") actually has a torus-shaped singularity (again, according to GR) with a finite, calculable size.