Regular black holes

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Discussion Overview

The discussion revolves around the concept of regular black holes as proposed in a recent paper, which suggests that these black holes do not contain singularities. Participants are exploring the theoretical implications of this work, its relation to general relativity, and the nature of black holes in modified theories of gravity.

Discussion Character

  • Exploratory, Technical explanation, Debate/contested

Main Points Raised

  • Some participants highlight that the paper proposes regular black holes as endpoints of gravitational collapse in a theory with higher-curvature corrections, suggesting a resolution to singularities.
  • Others note that there are known solutions in standard general relativity, such as Bardeen black holes, which do not have event horizons but can appear black hole-like for extended periods.
  • A participant expresses a desire to understand specific claims from the paper, particularly regarding the transition of these regular black holes to a new universe through a bounce.
  • There is a discussion about the lack of experimental evidence for the claims made in the paper, with some participants emphasizing that opinions on the work remain speculative.
  • Some participants question the clarity of the paper regarding the transition to a white hole and the implications of such a transition.
  • One participant mentions that the model described in the paper exhibits properties that are unusual and not typically associated with real astrophysical objects, raising concerns about its physical reasonableness.

Areas of Agreement / Disagreement

Participants generally do not reach a consensus on the validity of the claims made in the paper. Multiple competing views remain regarding the implications of the proposed model and its relationship to established theories.

Contextual Notes

Participants note that the discussion is limited by the speculative nature of the claims and the absence of experimental validation. The paper's reliance on higher-curvature corrections and its implications for singularity resolution are also points of contention.

javisot
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TL;DR
Regular black holes by infinite corrections
A work published some time ago by several of my compatriots, on regular black holes, without singularity.

https://arxiv.org/abs/2412.02742

I would like to ask some questions but first I want to hear expert opinions on this work.

Sabine has uploaded a video about it,
 
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javisot said:
I would like to ask some questions
Then you should ask them.

javisot said:
first I want to hear expert opinions on this work
Any such opinion will be just that, an opinion. Meaning, there is no experimental evidence involved, and without any experimental evidence, no one's opinion carries any real weight anyway.
 
Btw, there is at least one known class of solutions in standard GR (i.e., without the modifications described in the paper referenced in the OP) that, while it has no actual event horizon, looks like a black hole from the outside for a very, very long time, on the order of the Hawking evaporation time. The term "Bardeen black hole" is used to describe this class of solutions, although since they have no event horizons, the term "black hole" is actually a misnomer.

See this post and the paper it references:

https://www.physicsforums.com/threa...n-evaporating-black-hole.1062617/post-7086255

Note, btw, that the paper uses the term "regular black hole" to describe the Bardeen black hole class of solutions--not solutions in a modified theory which has different dynamics from standard GR, as in the paper referenced in the OP.
 
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PeterDonis said:
Any such opinion will be just that, an opinion. Meaning, there is no experimental evidence involved, and without any experimental evidence, no one's opinion carries any real weight anyway.
Sorry, I explained myself poorly. I'd like to hear expert opinions on whether this work is theoretically correct and make sense. Assuming it's incorrect, then I wouldn't have any questions.
 
I extract 3 parts of the work that I try to understand:

1-"We have shown that regular black
holes are the endpoint of gravitational collapse in a purely gravitational theory. This is a generic consequence of a theory containing an infinite tower of higher-curvature corrections with only very mild and qualitative conditions on the couplings. This provides a mechanism for the resolution of singularities and the formation of regular black holes in any di-mension D ≥ 5. We believe this is the first time results of such generality have been achieved. Our model affords considerable opportunity to address important problems in the theory of regular
black holes and singularity resolution."

2- "These effects will likely play an
important role in the final stages of regular black hole evaporation. Whether or not the mechanism we have identified is the one responsible for singularity resolution in Nature remains to be seen. What is clear is that it provides a robust mechanism where many long-thought impossible questions can be finally addressed."

3- "We analytically solve the collapse of a thin shell of dust and show that it inevitably experiences a bounce at small radius and that its motion can be extended to arbitrary proper time. The collapse of the shell always gives rise to a singularity-free, geodesically complete spacetime that contains horizons if the total mass is above a critical value. In that case, the shell bounces into a new universe through a white hole explosion. Our construction provides, to the best of our knowledge, the first fully dynamical description of formation of regular black holes, and it suggests that higher-derivative corrections may be the most natural way to resolve the singularities of Einstein’s theory."
 
javisot said:
I'd like to hear expert opinions on whether this work is theoretically correct and make sense.
It's probably too early for experts to have an opinion on that, since the paper is proposing a modified theory of gravity.
 
javisot said:
I extract 3 parts of the work that I try to understand:
Ok, so what questions do you have about them?
 
PeterDonis said:
Ok, so what questions do you have about them?
I want to understand part 3.

So, these regular black holes, as described in this paper, have an event horizon, no singularity, and they transition to white? (I'm not clear about this last part, since the authors dedicate little to it)
 
javisot said:
So, these regular black holes, as described in this paper, have an event horizon, no singularity, and they transition to white?
"Transition to white" in the sense that they "bounce into a new universe", as what you quoted from the paper says. Fig. 2 of the paper shows the Penrose diagram that describes this.
 
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  • #10
PeterDonis said:
"Transition to white" in the sense that they "bounce into a new universe", as what you quoted from the paper says. Fig. 2 of the paper shows the Penrose diagram that describes this.
I see it. I also see that the only part where they discuss it is practically at the end, and they stop explaining what appears to be the description of the white hole after the bounce. It feels like they don't want to talk about it.

"One of these contains the shell, inside of which the spacetime is flat, while the other region corresponds to a “de Sitter core” in which the line r = 0 is fully regular.[77] Ultimately, the shell starts climbing the potential and reaches a turning point at which R˙ = 0 and R = Rmin — this always happens in region III. At that point, a bounce occurs. The shell begins increasing its size, crossing the inner and outer horizons and emerging in a new universe from a white hole. The shell will grow up to r = R0, at which point the process of collapse restarts. If the total mass is below the critical threshold, the shell experiences a bounce as well, but horizons never form."
 
  • #11
So they start from GR black hole, apply an infinite tower of higher-curvature corrections, hey get a black hole without singularity, and then a bounce (similar to LQC)?

I just noticed that this white hole part isn't mentioned by Sabine in her video either.
 
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  • #12
javisot said:
they stop explaining what appears to be the description of the white hole after the bounce. It feels like they don't want to talk about it.
I can imagine they don't, because of the "new universe" part.
 
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  • #13
javisot said:
they start from GR black hole, apply an infinite tower of higher-curvature corrections
More precisely, they apply "an infinite tower of higher-curvature corrections" to the Einstein-Hilbert action (and hence to the Einstein Field Equation), and then examine the properties of what corresponds to something like the Schwarzschild solution in this modified theory.

javisot said:
they get a black hole without singularity, and then a bounce (similar to LQC)?
That's more or less how they describe it, but what their model actually shows is something a lot weirder: it's like the maximal extension of Reissner-Nordstrom or Kerr, even though their model is spherically symmetric (no rotation) and vacuum (no electric charge). And that maximal extension has some very strange properties, which aren't normally talked about much since nobody believes that actual objects in our universe have those properties, they're just properties of an idealized, physically unreasonable model. But this paper appears to be relying on those same properties and claiming that they are physically reasonable.
 
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