Is the Big Collapse a Black Hole?

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The discussion revolves around the nature of the Big Collapse in the closed Friedmann model and its relationship to black hole singularities. It is established that the Big Collapse is not a black hole but rather a future-spacelike singularity, akin to the Big Bang, which is past-spacelike. The conversation also touches on the implications of quantum mechanics regarding information density in a collapsing universe, suggesting that time might need to reverse as the universe shrinks. Additionally, the collapsing Friedmann model is considered to be symmetric with respect to time reversal, resembling the Big Bang in reverse. Overall, the distinctions between localized black hole singularities and non-localized singularities like the Big Collapse are emphasized.
haael
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In the "closed" Friedmann model, there is a Big Bang in the past and Big Collapse in the future. Big Bang singularity is something different than a Black Hole singularity.

Now my question: is the Big Collapse singularity mathematically equivalent to a Black Hole (localized) singularity, or is it rather a non-localized singularity like a Big Bang one? Or maybe something else?

My another question: in the "closed" collapsing Friedmann model the Universe becomes smaller at some point. From QM we know that we can not stuff infinite information in finite region. Would it mean that time would need to move, uhm, backwards near the end of the collapsing Universe? The information will need to disappear as different states would need to evolve into the same state, since there's no room to hold their information.

My real question is: is the collapsing Friedmann model symmetric with regards to time reversal? Does the Big Collapse look just like the Big Bang played backwards?
 
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haael said:
is the Big Collapse singularity mathematically equivalent to a Black Hole (localized) singularity, or is it rather a non-localized singularity like a Big Bang one?

It's the time reverse of the Big Bang; it is not a black hole.

haael said:
in the "closed" collapsing Friedmann model the Universe becomes smaller at some point. From QM we know that we can not stuff infinite information in finite region.

The closed collapsing FRW model is a classical model, not a quantum model. In a classical model you *can* "stuff infinite information in a finite region".

I'm not sure how much work has been done in trying to construct a quantum model of a closed collapsing universe.

haael said:
is the collapsing Friedmann model symmetric with regards to time reversal? Does the Big Collapse look just like the Big Bang played backwards?

Yes, in the sense given in my first response above.
 
In what sense do you think black hole singularities are "local"? Like the big bang singularity, the Schwarzshchild black hole singularity is a spacelike surface. The difference between these two is simply that the big bang singularity occurred in the past (past-spacelike) while the black hole singularity occurs to the future of worldlines moving across the event horizon (future-spacelike). In these terms, the big crunch singularity is future-spacelike.
 
bapowell said:
the black hole singularity occurs to the future of worldlines moving across the event horizon (future-spacelike). In these terms, the big crunch singularity is future-spacelike.

Yes, but unlike the black hole singularity, the big crunch singularity is in the future of *all* worldlines in the spacetime, not just the ones that pass inside the event horizon. I assumed that that was what the OP meant by the black hole being "local".
 
OK. My concern is that the OP was considering the black hole singularity to be localized in space.
 
bapowell said:
OK. My concern is that the OP was considering the black hole singularity to be localized in space.

Well, it's worth noting the Kerr singularity is timelike rather than spacelike, thus localized, and can be bypassed. It is, of course, unknown whether a more realistic (not perfectly axisymmetric) collapse in classical GR produces a timelike or spacelike singularity (so far as I know, this is one of the remaining open questions in GR).
 
https://en.wikipedia.org/wiki/Recombination_(cosmology) Was a matter density right after the decoupling low enough to consider the vacuum as the actual vacuum, and not the medium through which the light propagates with the speed lower than ##({\epsilon_0\mu_0})^{-1/2}##? I'm asking this in context of the calculation of the observable universe radius, where the time integral of the inverse of the scale factor is multiplied by the constant speed of light ##c##.
The formal paper is here. The Rutgers University news has published a story about an image being closely examined at their New Brunswick campus. Here is an excerpt: Computer modeling of the gravitational lens by Keeton and Eid showed that the four visible foreground galaxies causing the gravitational bending couldn’t explain the details of the five-image pattern. Only with the addition of a large, invisible mass, in this case, a dark matter halo, could the model match the observations...
Why was the Hubble constant assumed to be decreasing and slowing down (decelerating) the expansion rate of the Universe, while at the same time Dark Energy is presumably accelerating the expansion? And to thicken the plot. recent news from NASA indicates that the Hubble constant is now increasing. Can you clarify this enigma? Also., if the Hubble constant eventually decreases, why is there a lower limit to its value?

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