So we know that if you have enough mass in a small enough radius you get a black hole. This radius being r= 2Gm/c^2. This all assumes that the total mass m is within that radius r.
Keep that in the back of your head for a minute. Lets jump over to special relativity. We know that the length of an object decreases as speed increases.
Using the Lorentz contraction L'= l * sqrt(1-(v^2/c^2))
It would seem that eventually you would be able to create a black hole if you gave an object enough speed that an outside observer would see the current object shrink past it's Schwartzchild Radius. Yes I realize that it is only the length that is in question not the width and height, but the same question still applies as sqrt(1-(v^2/c^2)) approaches 0 as v approaches c. Basically flattening the object.
So the questions:
1: If an object gains enough speed to appear to be a black hole and then loses momentum will it return to normal (not be a black hole), or is this a one way trip once you hit that point (will the gravitational forces take over and sustain the black hole)? Or will it even be considered a back hole?
2: Is it possible that the time dilation seen in particle accelerators really just a side effect of this relativistic density change and therefore essentially equivalent to gravitational time dilation?
I will admit I have only looked at this from the side of special relativity. I assume this gets a little more complicated in General Relativity.