Could time move inside a black hole?

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Discussion Overview

The discussion revolves around the nature of time within and around black holes, particularly focusing on the behavior of time as objects approach the event horizon and the implications of singularities. Participants explore theoretical aspects, assumptions about density, and the effects of time dilation in the context of black hole physics.

Discussion Character

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

Main Points Raised

  • Some participants propose that time continues to move below the event horizon, suggesting that objects falling in experience time normally.
  • Others argue that the rate at which time passes for an observer falling into a black hole appears to slow down from the perspective of an outside observer, leading to questions about the formation of the event horizon.
  • A participant raises the issue of whether an object can actually fall past the event horizon, suggesting that the black hole might cease to exist due to Hawking radiation before the infalling object crosses it.
  • Another participant challenges the idea that the mass of a collapsing object reduces proportionally to the radius, asserting that the mass remains constant during collapse.
  • Some participants express skepticism about the physical existence of singularities, suggesting that the concept of time may vanish at the singularity.
  • There is a contention regarding the perception of time for infalling observers versus static observers, with differing views on whether time appears to speed up or slow down for those crossing the event horizon.

Areas of Agreement / Disagreement

Participants do not reach a consensus; multiple competing views remain regarding the behavior of time near and within black holes, the nature of singularities, and the implications of time dilation.

Contextual Notes

Limitations include assumptions about consistent density during collapse, the idealization of mass remaining constant, and the unresolved nature of how time behaves at the singularity.

whatdoctor
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At the event horizon for a black hole is R=2GM/C^2
This means that, as a star collapses, it gets more dense until this limit is reached. Assuming a consistent density (just an approximation as I know this will not really be the case), the Mass will reduce proportionally to the cube of R, but the event horizon goes down proportional to M - so the event horizon radius reduces faster than the mass that would create it. This means that, below the event horizon, time is still moving.
Assuming the minimum size of a naturally occurring black hole is about 2 stellar masses - this gives us a radius of about 6km inside every black hole where time still moves.
Or does the star instantaneously collapse to a singularity? If so, how can it continue to collapse once time has stopped?
 
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whatdoctor said:
Assuming a consistent density (just an approximation as I know this will not really be the case), the Mass will reduce proportionally to the cube of R, but the event horizon goes down proportional to M - so the event horizon radius reduces faster than the mass that would create it. This means that, below the event horizon, time is still moving.

Time would pass normally for any observer who passes the event horizon. It's the rate that the observer's time passes as viewed from someone well outside the event horizon that goes to zero. That is, to an observer standing far away from the black hole, the rate at which an infalling observer's clock ticks approaches zero as they approach the event horizon. The problem with black holes is that thing become unpredictable when an observer reaches the singularity.

whatdoctor said:
Or does the star instantaneously collapse to a singularity? If so, how can it continue to collapse once time has stopped?

I believe there is an issue with how an event horizon can form if the infalling material slows down under time dilation. As the density during collapse increases, the amount of time dilation increases, so to an far away observer the material should appear to "freeze" before an event horizon forms. I'm not sure if this is a real issue or if there is a way around it. Perhaps someone else can answer that.
 
Given it is presumed that space collapses to zero volume at the singularity, it is perfectly reasonable to expect the very concept of time itself also vanishes at the singularity. Nonsensical situations like this is what leads most scientists to reject the notion of the physical existence of singularities
 
whatdoctor said:
Assuming a consistent density (just an approximation as I know this will not really be the case), the Mass will reduce proportionally to the cube of R

No, it won't. The mass of the collapsing object is constant (assuming it doesn't give off radiation or eject matter--any real collapse will do both of those things, but we can idealize them away for this discussion).

whatdoctor said:
so the event horizon radius reduces faster than the mass that would create it

No, this is not correct. Assuming an idealized collapse that does not emit radiation or eject matter, the horizon radius is known at the start of the collapse--it's the radius corresponding to the original mass of the collapsing object.

whatdoctor said:
This means that, below the event horizon, time is still moving.

It is true that "time is still moving" below the horizon, in the sense that objects that fall in (or objects in the collapsing matter) continue to experience time normally. So you have the right conclusion here, but your method of getting to it is incorrect. See above.
 
I would say that an object cannot fall past the event horizon. My reasoning is this: From the perspective of the object falling, time moves normally for it - but time outside the event horizon would appear to speed up. So as the next second passes for the falling object, billions (or even trillions) of years pass outside the event horizon. By this time the black hole would cease to exist (by Hawking radiation). So as soon as the object hits the event horizon, the black hole vanishes.
 
whatdoctor said:
I would say that an object cannot fall past the event horizon. My reasoning is this: From the perspective of the object falling, time moves normally for it - but time outside the event horizon would appear to speed up. So as the next second passes for the falling object, billions (or even trillions) of years pass outside the event horizon. By this time the black hole would cease to exist (by Hawking radiation). So as soon as the object hits the event horizon, the black hole vanishes.
Totally incorrect. Have you been reading this thread? The infaller doesn't even notice the EH.
 
whatdoctor said:
From the perspective of the object falling, time moves normally for it - but time outside the event horizon would appear to speed up

No, it doesn't. Don't confuse the infaller with a static observer. A static observer, one who "hovers" at a constant altitude close to the horizon, will see the rest of the universe speeded up, yes. But an infalling observer will not. In fact, as the infalling observer crosses the horizon, he will see the rest of the universe slowed down.
 

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