First post a question about Black Holes and Gravity

In summary, the conversation touched on the topic of black holes and their mathematical description, which often ends in a singularity. Although black holes are known to exist, their mass is not necessarily infinite, but their density may be. There is also some skepticism towards the danger black holes may pose to our universe, as well as a discussion on the relationship between mass and density in defining a black hole.
  • #36
DrGreg said:
I agree. The theory of general relativity works perfectly well both inside and outside the event horizon. The problem occurs only when we get very close to the centre. General relativity ignores quantum effects, but those effects can't be ignored close to the centre. Until someone successfully combines general relativity with quantum theory we don't really know what happens at the very centre.

To clarify my statement I really meant that we can't know what happens beyond the event horizon so even though GR can be used, we can't test it to be sure. Of course, someone falling into the BH can pride himself on knowing the truth and knowing no one else will know until they join him in eternity.
 
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  • #37
arabianights said:
i'm skeptical about black holes, a couple weeks ago they reported the dicovery of biggest BH yet, a 21 billion solar masses at a distance of 336 million light-years away, and yesterday they found that Milky Way Galactic BH is gulping up near cosmic cloud. these black holes pose clear and present danger to us in the long term (assume we survive in long term of course) according to singularity theory. they might find their theories are totally wrong about BH
Do you mean to say that you doubt the existence of black holes? Because I assure you that they do exist, and in arguing their existence you contradict some of the greatest genius' of the past hundred years; such as Einstein and Hawking.
 
  • #38
As I understand it, any question about the interior of black holes is a question about the future. (And a very special subset of possible futures - see below).

The concept of a universal "now" was dropped with relativity (although frequently people ignore this). What we are left with are the concepts of regions of space-time between which signals can pass in one direction or the other. In addition there are regions between which communication can pass in neither direction.

There is no point on or inside the event horizon of a black hole which can communicate with a point outside this region.

In fact, if I understand the classical view correctly, the region nearer the singularity cannot communicate with an observer falling into the black hole even after it has passed the event horizon (the radius is timelike).

The singularity is thus of relevance to the future of anything that falls into it, concerning precisely what happens when it reaches the region very close to it.

I also understand that all this is compatible with the view that (to outsiders) black holes appear to form and evaporate through Hawking radiation, because this process is indistinguishable from a view where material accumulates just outside the event horizon, becomes practically invisible as it gets very close and the entire energy is radiated from very close to the event horizon. The story looks very different to the observer outside and the one who falls in, but since the one who falls in reaches the singularity, they are not going to compare notes.

I am sure there are subtleties which explain this picture better; if there are inaccuracies, perhaps someone better informed than I am can correct them.

This (classical + Hawking) picture described appears to be very different to the fuzzball picture. In the former, when an observer crosses the event horizon, nothing very special happens; in the latter I read that the observer enters a region of high density, regardless of what material has recently been falling in (presumably). This needs clarification.
 
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