Is Causality Relative in Black Holes?

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Discussion Overview

The discussion revolves around the nature of causality in the context of black holes, particularly focusing on the perspectives of different observers (one falling into the black hole and another far away). It explores concepts from general relativity (GR) regarding event horizons, the behavior of time and space near black holes, and implications for conservation laws.

Discussion Character

  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • Some participants propose that an observer far away (B) would never see another observer (A) cross the event horizon due to time dilation and length contraction effects, leading to questions about the nature of causality.
  • Others argue that while B cannot see A cross the horizon, this does not imply that A never crossed it; B can still calculate A's experiences using the laws of physics.
  • There is a discussion about whether the inability of B to detect A's fall is due to increasing redshift and the nature of light signals near the event horizon.
  • Some participants express concerns about conservation of mass and energy, questioning if a black hole can be considered massless if matter crosses the event horizon and converges to a singularity.
  • Others clarify that the mass/energy is still present in the curvature of spacetime, and that a black hole is a vacuum in terms of stress-energy but not in terms of mass/energy.
  • There is a debate about whether the properties of spacetime can change and how this relates to the concept of mass being a property of the entire spacetime geometry rather than a specific point.
  • One participant draws an analogy between the disappearance of the sun and the behavior of mass entering a black hole, questioning the implications for the propagation of curvature in spacetime.

Areas of Agreement / Disagreement

Participants express differing views on the implications of black holes for causality and conservation laws. There is no consensus on whether causality is relative or how to interpret the properties of mass and energy in relation to black holes.

Contextual Notes

Participants highlight limitations in understanding the nature of spacetime and stress-energy, as well as the complexities involved in discussing the effects of black holes on causality and conservation principles.

FallenApple
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So in GR, for a classical black hole, if A is approaching the event horizon, to an observer far away, let say B, B would never observe A crossing the event horizon as B would observe A's time slow down in the limit to 0 and A's length contract in the limit to 0. In fact, according to B, A never crossed the event horizon.

But A in it's own reference frame crossed the event horizon.

So then in this case, would A and B disagree on causality since both A and B completely disagree on what even happened? Then would that mean that causality is relative?
 
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FallenApple said:
B would observe A's time slow down in the limit to 0

B would see A's clock appear to slow down. But that is a distortion because of the curvature of spacetime between A and B. It is not because of anything happening to A's clock.

FallenApple said:
and A's length contract in the limit to 0

This is not correct.

FallenApple said:
according to B, A never crossed the event horizon

No. B cannot see A cross the horizon, but that does not mean B can say that A never crossed the horizon. All B can say is that he does not see A crossing the horizon. It's no different than an object going below your horizon when you're standing somewhere on Earth; the object doesn't cease to exist just because you can no longer see it.

FallenApple said:
would A and B disagree on causality since both A and B completely disagree on what even happened?

No. A and B don't disagree on what happened. B cannot see everything that A can see; but B is perfectly capable of calculating what A sees using the laws of physics.
 
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PeterDonis said:
B would see A's clock appear to slow down. But that is a distortion because of the curvature of spacetime between A and B. It is not because of anything happening to A's clock.
This is not correct.
No. B cannot see A cross the horizon, but that does not mean B can say that A never crossed the horizon. All B can say is that he does not see A crossing the horizon. It's no different than an object going below your horizon when you're standing somewhere on Earth; the object doesn't cease to exist just because you can no longer see it.
No. A and B don't disagree on what happened. B cannot see everything that A can see; but B is perfectly capable of calculating what A sees using the laws of physics.
Ok got it. So B simply cannot detect A falling experimentally with observation? This is due to increasing redshift?

This leads me to a followup question. It's actually based on what you posed. I found it when searching for info on black holes.

You stated: "The classical (GR) model says (not "assumes"--it's derived from the Einstein Field Equation) that the black hole is vacuum inside. The mass that originally collapsed to form the hole reaches the singularity and disappears."

from this thread. https://www.physicsforums.com/threa...nd-quantum-physics-agree.891177/#post-5609778

So according to your earlier post in this thread, and your statement in the linked thread I just posted, an observer can conclude that the matter from a stellar collapse would cross the event horizon and then converge to nothingness in finite time.

Then would that not violate conservation of mass and energy? I mean, the black hole would be massless. Also, as an aside, spacetime is still curved, inside and outside the event horizon, which should not be possible since the presence of mass and energy is required to explain curved spacetime. Unless, the black hole became unstable and dissapears in finite time, due to lacking mass.
 
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FallenApple said:
So B simply cannot detect A falling experimentally with observation?

Yes.

FallenApple said:
This is due to increasing redshift?

It's because the region at and beneath the event horizon cannot send light signals to anywhere outside the horizon.

FallenApple said:
would that not violate conservation of mass and energy?

No. The mass/energy is still there, stored in the curvature of spacetime, and the black hole still acts as a source of gravity the same way the original object did.

It is true that the black hole is a vacuum, but that does not mean "zero mass/energy". It means "zero stress-energy". See below.

FallenApple said:
the black hole would be massless

No, it wouldn't.

FallenApple said:
the presence of mass and energy is required to explain curved spacetime.

The correct term is "stress-energy". But there is stress-energy in the spacetime; the object that originally collapsed to form the black hole has it. A curved spacetime does not have to have stress-energy at every single event where there is curvature. It just has to have stress-energy somewhere in the past light cone of an event where there is curvature.
 
PeterDonis said:
No. The mass/energy is still there, stored in the curvature of spacetime, and the black hole still acts as a source of gravity the same way the original object did.

It is true that the black hole is a vacuum, but that does not mean "zero mass/energy". It means "zero stress-energy". See below.

So the substance that possesses the stress energy disappears but leaves behind the stress energy inside the curved spacetime. Makes sense since conservation must be preserved.

So the center spatial point can be said to possesses mass even if there is no substance there?
PeterDonis said:
The correct term is "stress-energy". But there is stress-energy in the spacetime; the object that originally collapsed to form the black hole has it. A curved spacetime does not have to have stress-energy at every single event where there is curvature. It just has to have stress-energy somewhere in the past light cone of an event where there is curvature.

Is this similar as the following situation?

If I waved a magic wand and made the sun disappear, we would only feel the effects 8 min later because of the speed limit of causality.

the instant the sun disappears, the spatial warping seems to propagate outwards and becomes more dilute.

For the black hole, it's similar since the mass going into the event horizon is like a magic wand( the horizon shields the universe from the inner mass.) But is it different from the disappearing Sun situation since the curvature does not change and propagate outwards? What causes this?
 
FallenApple said:
So the substance that possesses the stress energy disappears but leaves behind the stress energy inside the curved spacetime.

No. Remember we are talking about spacetime. Spacetime doesn't "change"; it just is. And there is a portion of it that contains stress-energy, and a portion that does not. Nothing "disappears"; it's just different regions of spacetime with different properties.

FallenApple said:
So the center spatial point can be said to possesses mass even if there is no substance there?

As I have already said, "mass" is a property of the spacetime geometry as a whole. It isn't a property of any particular point.

FallenApple said:
If I waved a magic wand and made the sun disappear

Then you would be violating the conservation of energy and the laws of GR. So this is a meaningless hypothesis.

FallenApple said:
For the black hole, it's similar since the mass going into the event horizon is like a magic wand( the horizon shields the universe from the inner mass.)

No, it isn't. Once more: the mass is a property of the spacetime geometry as a whole. It is not "located" inside the horizon.
 

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