Are Black Holes Theoretical Phantoms?

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Discussion Overview

The discussion revolves around the nature of black holes, questioning their existence and the implications of event horizons in the context of general relativity and cosmological models. Participants explore theoretical and conceptual aspects, including the measurement of time near black holes and the relationship between particles and singularities.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • Some participants propose that it takes an infinite amount of time for an event horizon to form, raising questions about the implications for the existence of black holes.
  • Others argue that a watch falling into a collapsing star would measure a finite amount of time before reaching the event horizon, while photons emitted would take an infinite amount of time to reach an external observer.
  • A participant questions whether a collapsing star, located outside its Schwarzschild radius, would ever form an event horizon according to local coordinates.
  • There is a suggestion that the concept of existence becomes fuzzy in curved spacetime, particularly regarding black holes and their relation to simultaneity.
  • Some participants express skepticism about the existence of black holes, suggesting that evidence of infalling matter does not necessarily imply their presence.
  • Discussions arise about the properties of particles and their similarities to singularities, with one participant noting the lack of definitive boundaries in particles.
  • There are mentions of the challenges in defining simultaneity and existence in the context of black holes, with references to spacelike and timelike trajectories.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the existence and nature of black holes, with no consensus reached on the fundamental questions posed.

Contextual Notes

Participants highlight limitations in definitions and the ambiguity surrounding the concept of existence in curved spacetime, as well as the challenges in measuring time and trajectories near black holes.

Phrak
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I understand that it takes an infinite amount of time for an event horizon to form. Give this, if there are any black holes, they have been around forever.

Are there good comological models that include 'forever', or is my premise wrong?
 
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Phrak said:
I understand that it takes an infinite amount of time for an event horizon to form.
How are you measuring that?

A watch falling into a collapsing star would measure a finite amount of time before it reaches the event horizon. OTOH the photons emitted from the watch as it passes through would take an "infinite" amount of time to reach an external observer. (According to GR)
 
Hurkyl said:
How are you measuring that?

A watch falling into a collapsing star would measure a finite amount of time before it reaches the event horizon. OTOH the photons emitted from the watch as it passes through would take an "infinite" amount of time to reach an external observer. (According to GR)

Anywhere that is always outside an event horizon. The syntax can get sticky, here, but if there is no event horizon, there is no watch that will ever fall through it. But this is a distraction.

We are on Earth. There may be a collapsing star somewhere, at a distance larger than it's Schwarzschild radius. Would it ever form an event horizon according to our local, normal coordinates?
 
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Phrak said:
We are on Earth. There may be a collapsing star somewhere, at a distance larger than it's Schwarzschild radius. Would it ever form an event horizon according to our local, normal coordinates?
Yes -- an infalling watch measures a finite amount of time before hitting a horizon, and therefore the horizon would be contained in any Riemann normal 'coordinate chart' centered on Earth.

(Assuming, of course, that expansion or other gravitational effects do not prevent geodesic travel from Earth to the star. But, I suppose if that's happened, the star has already fallen off the 'coordinate chart', and so the question would be moot)

(Also making the usual assumptions that there isn't an 'edge of the universe' at which geodesics would vanish before reaching the alledged star and what not)

(I'm putting 'coordinate chart' in quotes, because Riemann normal coordinates do not meet the criteria demanded of coordinate charts in differential geometry -- namely that distinct coordinates always refer to distinct points)
 
Thank you Hurkyl.

Things are stranger than I was prepared for. It appears that seemingly contrary statements such as 'never happened' vs 'happened', or 'will happen' vs 'will not happen' are contectual. I had thought this sort of thing was confined within the domain of quantum mechanics and not relativity.
 
Observationally, black holes are very real. Particles may not be real, but, deceivingly convincing. If you get too near a particle, it has properties that look like a singularity.
 
If you get too near a particle, it has properties that look like a singularity.
what do you mean by this? I'm not very familiar with QM nor GR, but I'm about to start these subjects next semester.. it what sense do you 'approach' a particle? and what are the similiarities with a black hole?
i first agreed with the "particles may not be real" statement, since the atom has no definite boundary (i'm clueless about tinier particles), so it's kinda hard to talk about 'the' particle.. or maybe in the sense that the atoms are made up of even smaller things, and who knows, maybe they're in turn made up of EVEN smaller things..
 
Phrak, when we say 'it exists now' we use some sort on simultanety, usually in our frame. But with a black hole it is not possible to define such simultanety, even theoretically, because our simultanety 'outside' becomes time-like inside the horizon.

As amateur, I think in puctures like
http://www.valdostamuseum.org/hamsmith/DFblackIn.gif
http://nrumiano.free.fr/Images/lightcones_E.gif
http://www.etsu.edu/physics/plntrm/relat/eventho1.gif
 
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I see evidence of infalling matter, Chronos. Not black holes.

Dmitry, Then how can one speak of existence?
 
  • #10
Phrak, the word 'exists' is too fuzzy in the curved spacetime.
when we say 'it exists now' we speak about space-time relation. Or zero-interval in the past, when we talk about distant stars. Or we mean that we can come and touch that object, which means, that there are some timelike trajectories which intersect with that object.

No 'now' surface intersects with an interior of the black hole, so no, black holes do not exist.
But there are some spacelike trajectories which intersect with it (you can fly into the black hole) so yes, black holes do exist :)
 
  • #11
Dmitry67 said:
Phrak, the word 'exists' is too fuzzy in the curved spacetime.
Surely, introducing even fuzzier terms doesn't help clear things up. :-p I have no idea what you mean by a "'now' surface".

And I don't see your problem with "exists" -- either there is such an object in space-time or there is not, there is no mathematical ambiguity there. Phrak's original question, I think, simply boils down to the fact that coordinate charts need not cover all of space-time.

But there are some spacelike trajectories which intersect with it (you can fly into the black hole) so yes, black holes do exist :)
That's a timelike trajectory...
 
  • #12
Hurkyl said:
That's a timelike trajectory...

Yes, sorry, I was drunk :) Sunday...
 
  • #13
Particles have no definitive 'position' in spacetime. Singularities have similarily ill defined positions. We can approximate the position of either object with considerable accuracy.
 

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