From our reference frame, how would a black hole ever form?

In summary, a black hole forms when a massive star exhausts its nuclear fuel and can no longer support itself against gravitational collapse. Once the core collapses, it can compress to a point where the gravitational pull becomes so strong that not even light can escape, resulting in a black hole. This process typically occurs at the end of a star's life cycle, often leading to supernova explosions that can also contribute to the creation of black holes.
  • #1
msumm21
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TL;DR Summary
From what I understand, from "our" reference frame a black hole would never form
Looking at Kruskal diagrams, it seems to me we should not be able to see evidence of black holes. Assuming our frame is a hyperbola of roughly constant ##r## in such a diagram, as the black hole's constituent mass comes together time slows (from our POV) to the extent that it never crosses the horizon or forms a black hole.

I realize that, in the frame of a constituent mass, the block hole forms, but my question is from the POV of someone at a roughly constant ##r## outside the black hole.

EDIT: I think my first sentence is mistaken: presumably we could "see evidence" by "watching" the acceleration of an object close to, but outside, the horizon.
 
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  • #2
It depends what you mean but our POV. It's true that some events cannot be directly observed. And that there are systems of coordinates in which no time can be assigned to a given event. That, however, is a deficiency in the coordinate system. You are free to choose another coordinate system that does include the event under discussion.
 
  • #3
PeroK said:
It depends what you mean but our POV. It's true that some events cannot be directly observed. And that there are systems of coordinates in which no time can be assigned to a given be event. That, however, is a deficiency in the coordinate system. You are free to choose another coordinate system that does include the event under discussion.
Copy, thanks. I am thinking in our proper time, so in our proper time the BH never forms, right.

Understand your point with some time coordinates it does form.
 
  • #4
msumm21 said:
I am thinking in our proper time, so in our proper time the BH never forms, right.
"In our proper time" isn't meaningful - better to ask whether an event is or will eventually be in our past light cone, in which case we can reasonably say that "it has happened".

The eternal black hole of the Schwarzschild solution isn't physically realizable, as it describes a black hole that has always existed. A real black hole will have formed by gravitational collapse, and although we cannot directly observe events at the horizon, we can observe that there is a black hole where before there had been some uncollapsed matter..
 
  • #5
msumm21 said:
TL;DR Summary: From what I understand, from "our" reference frame a black hole would never form

Looking at Kruskal diagrams, it seems to me we should not be able to see evidence of black holes.
Note that the Kruskal diagram that you posted is for a Schwarzschild black hole. Indeed, you would never see a Schwarzschild black hole form because it does not form. It is pre-existing.

Instead, what you need is the equivalent of a Kruskal diagram for an Oppenheimer Snyder spacetime. The only one I have found is here: https://jila.colorado.edu/~ajsh/bh/collapse.html

msumm21 said:
in our proper time the BH never forms
Proper time only covers the worldline of the object. So that doesn't make a lot of sense.
 
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FAQ: From our reference frame, how would a black hole ever form?

What is a reference frame in the context of black hole formation?

A reference frame is a perspective from which an observer measures and experiences physical phenomena. In the context of black hole formation, it refers to the viewpoint of an observer who is far away from the gravitational influence of the collapsing object. This observer measures time and space differently compared to someone closer to the black hole.

Why does time appear to slow down near a black hole from our reference frame?

Time appears to slow down near a black hole due to the effects of gravitational time dilation, a consequence of Einstein's theory of General Relativity. As an object approaches the event horizon of a black hole, the intense gravitational field causes time to stretch, making it appear to slow down from the perspective of a distant observer.

Can we ever see an object actually cross the event horizon of a black hole?

No, from our reference frame, we can never see an object actually cross the event horizon of a black hole. Due to gravitational time dilation, the object appears to slow down and asymptotically approach the event horizon, but never quite crosses it. The light emitted or reflected by the object becomes increasingly redshifted and eventually fades away.

How does the formation of a black hole appear to an external observer?

To an external observer, the formation of a black hole appears as a gradual process where the collapsing object becomes increasingly dim and redshifted as it approaches the event horizon. The object seems to freeze at the event horizon and never fully disappears, though it becomes practically invisible over time due to extreme redshifting.

What role does the event horizon play in the perception of black hole formation?

The event horizon is the boundary beyond which nothing, not even light, can escape the gravitational pull of a black hole. To an external observer, the event horizon marks the point where the collapsing object appears to freeze and become infinitely redshifted. It is the critical surface that defines the black hole and influences how we perceive its formation from a distance.

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