Besides that, since a black hole is a singularity, there is no such thing as directly into the singularity (it's infinitismally small), so any light shot "almost" directly at the singularty, and then it'll turn around and go back to the other edge of the event horizon [...]
Except that the inexorability of light falling 'towards' the singularity (see below for an agreement, as opposed to an objection) means that it's not a matter of light 'sloshing around' within the Event Horizon. More like... (well, I suppose intentionally like..., seing as it's supposed to be a model of same) those "gravity wells" that you can send balls into where they can loop around. Down to a certain point, you can engineer an eliptic (give or take loss of energy through air and material resistance) coming back up to the level of release, but after a certain depth you can only really see them going downwards (although, due to intrinsic classical effects its a fast orbital barely downwards rather than dragged mostly 'down').
Or perhaps, to remove the classical effects altogether, don't use the ball and instead painstakingly draw a line on the surface. A straight line (across the constraints of the warped surface). Some lines will merely go 'around' the hole, but some lines you draw will lead down into the funnel and never emerge. The distinct diameter of hole which no line can pass without ending up 'only going downwards' from then on is the event horizon. (Even then, there are flaws in the analogy, but different flaws.)
This realtes to something else I thought of. Generaly, a singularty is assumed to actualy exist. But wouldn't the space-time curving effects of gravity prevent matter from actualy reaching the singularity itself?
Now, this is more or less relevent to a prior reply of mine to someone regarding infinities. In a perfect 'model' gravity well (the 'toy' ones are obviously finite in depth, and are probably designed to asymtotically close to 'just larger than the ball-size' anyway), the slope gets steeper and steeper (close to, but not vertical) and the slice across at that level reveals a smaller and smaller hole (close to, but not, of zero size) but it's an infinitely deep slope which
never quite closes. Thus there is no part of the model that relates to the point of the singularity.
However...
After all, the closer matter (and energy) comes to the singularity, the more time dialatation it's going to experience[...]
Beyond the event horizon, time dilation isn't really applicable any more, in the same manner. A simple (wrong, but indicative) explanation is that v>c, so root(1-(v^2/c^2)) in the various equations is root(1-(
>1)) is root(<0) and thus an imaginary number. Which (given time works like an 'imaginary' dimension in various other formulae encompassing space and time coordinates) lends support to the whole "time becomes space, space becomes time" idea.
It's been said that Hawking radiation would cause a black hole to evaporate long before you reached the singularity, but why is this not true for the matter that is to form a new black hole?
I suspect because it's not a matter of the mass needing to be "at" the future singularity point to create the black hole, but that sufficient mass finds itself within either the event horizon or Schwarzchild radius. (Actually, isn't that the definition of the SR? I forget. Must check Wiki or something at some point.
, there then forms a 'singularity-centred' funnel (where previously there was just a dimple of whatever depth). And (through quantum uncertainty) no actual matter or energy (e.g. baryon, electron, quark, photon, gluon, Higgs boson, graviton, whatever) will be precisely 'at' the virtual point in space that is the 'singularity-centre' to cause complications, and now you just have to worry about whether the energy and matter that form (or later fall into) the black hole loses its identity or not in the warping of space-time.
One would expect the singularity to be virtual, that is there appears to be a singularity, but only from the outside, since in the inside matter hasn't reached the centre yet and never will.
For an external observer, that's definitely the case. You never even see anything pass the event horizon and (assuming an unobstructed view, the ability to handle the doppler issues and of course patience) would see it on the verge of disappearing 'forever' (or until the hole evaporates, when...
). Holding a hypothetical external-to-the-universe POV (which is severaly flawed due to assumptions we must make and the manner of our descriptive language) it would be seen to be either forever 'falling' down the gravity well, beyond the EH level. Perhaps doing so in a form without the original identity and physical limitations (thus allowing the evaporation). But when the well loses efficacy and snaps back into a mere 'dimple', the mass and energy that remains exists smeared out everywhere
except the precise (virtual) point of the singularity.
Of course, there's an issue about the potential discontinuity in the space-time as it converts between dimple and funnel, and vice-versa, but that's a question of cosmological topology that I shall leave unexplained, for want of the descriptive language I want.
Actually, all the above is really poorly described, for which I must apologise.