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The Black Hole Information Paradox Comes to an End (quantamagazine.org)
174 points by daegloe on Oct 30, 2020 | hide | past | favorite | 99 comments


"Trick though it is, it has real physics in it. The gravitational path integral doesn’t distinguish replicas from a real black hole. It takes them literally. This activates some of the latent topologies that the gravitational path integral includes. The result is a new saddle point containing multiple black holes linked by space-time wormholes. It competes for influence with the regular geometry of a single black hole surrounded by a mist of Hawking radiation."

Ah yes, the complex of wormhole interlinked blackholes surrounded by mists of Hawking radiation...

This style of writing, without the actual math, seems to more so obscure true understanding than reveal it for such a complex construct as english words are very likely insufficient for actually capturing the true meaning.

Adding the (partial?) equations of the path integral and/or the matrices would allow for an actual understanding without the confining nature of human words.

In fact just thinking and writing this comment made me more confused, just a few paragraphs prior the path integral could not be fully calculated, but now here it is certain that "the gravitational path integral doesn’t distinguish replicas from a real black hole". Just how powerful is this 'mathematical trick'?


>Adding the (partial?) equations of the path integral and/or the matrices would allow for an actual understanding without the confining nature of human words.

Go read the paper if you want that. Quanta isn't a journal its a popular science mag.


"But in terms of making sense of black holes, this is at most the end of the beginning. Theorists still haven’t mapped the step-by-step process whereby information gets out. “We now can compute the Page curve, and I don’t know why,” said Raphael Bousso at Berkeley."

So it does not seem that the physicists fully understand their calculation results either.

Edit: here's the arxiv link: https://arxiv.org/abs/1911.11977


Thanks for the link. I find it very frustrating when pop science magazines refuse to link to the actual paper. I don't want to read their attempt to put what the paper says into layman's language; their attempts are usually way off. I want to read the actual paper.

Edit: I was finally able to find links to actual papers in the article:

https://arxiv.org/abs/1810.02055

https://arxiv.org/abs/1905.08255

https://arxiv.org/abs/1905.08762

https://arxiv.org/abs/1908.10996

https://arxiv.org/abs/2002.08950

https://arxiv.org/abs/2004.05863

These appear to be the papers giving the various calculations the article discusses. There are also links to some previous work that was built on:

https://arxiv.org/abs/0804.0055

https://arxiv.org/pdf/1304.4926

https://arxiv.org/abs/1408.3203


[flagged]


> If your brain is so big that you find reading Quanta beneath you then why are you reading Quanta at all?

I'm not. I only found out about this through HN, so all I had to start with was the Quanta article since that's all that HN linked to.

> Just read Arxiv or Nature or Physical Review D and shut up

Please save your insults for someone who has asked for them.


I find the criticism had a lot of value because they pointed out all the proper arxiv resources related to the article. I think it should be a top rated comment directly under the article posting.


I'm a layperson. Does this mean there's no firewall but they don't know how?


To someone like me, who believes that the universe is, must be, fundamentally a computer, the actual academic paper is hardly any better. Whatever the paper is doing is not describing any kind of computational process. It's a mille-feuille of semi-rigorous mathematical abstraction that sounds far more like a kind of liturgical incantation than a description of the software our universe is running.

That's not to say it is definitely not useful! It could be that, for some bizarre reason, reading the mathematical tea leaves of our current incomplete (and incoherent) theories might well yield insight into post-quantum physics. I do doubt it though.


I'm not sure what to make of this comment. I'm not going to pretend I understand any of this at anything short of an extremely superficial level but you argument sounds like something a religious fundamentalist might say; just insert their belief system.

"To someone like me, who believes that the universe is, must be, fundamentally a construct of god, the actual academic paper is hardly any better. Whatever the paper is doing is not describing any kind of god process... sounds far more like a kind of liturgical incantation than a description of how god is running our universe."

I might be wrong, my understanding is limited, but you shouldn't dismiss something because it doesn't fit with you beliefs; you beliefs may be wrong g.


Stephen Wolfram takes that view too, but it seems like a fairly narrow lens to peer at the universe through. I suspect it may be true, but that doesn't even mean it's necessarily particularly useful for solving many classes of problems. In fact, are there any actual problems in Physics that have been solved by this approach?

Lots of things are true that aren't much use. Much of science, including physics doesn't describe computational processes. Does that make most of science and physics equally useless?


To someone like me, who believes that the universe is, must be, fundamentally a computer...

Why do you believe that?


In defence of the idea, if all physics is found to have a logical and mathematical basis, then doesn't all physical expression and interaction become computation?


"Computable" is a bit more strict than "logical and mathematical". We can define many perfectly consistent processes with perfectly consistent "observable values", which are inherently uncomputable (as in, there is no algorithm, even an inefficient one, that runs on Turing machines, capable of calculating the observable).

Here is my favorite example: https://en.wikipedia.org/wiki/Chaitin%27s_constant


I guess much of what I'm saying counts on hard determinism, and computation that isn't limited to what can be achieved with boolean logic. I'm talking out my ass here a little, but I picture quantum annealing as a form of computation where quantum physics effects are the actual execution engine.


Quantum effects are still things we can simulate on a Turing machine with a program that halts (just inefficiently slow given our current knowledge of complexity theory). Bringing in quantum effects does not make things uncomputable.


I now see the distinction you're trying to make about computability, so does this revised claim satisfy you?

> if all calculation of physical effects are found to be reducible to mathematical procedure with definite outcomes, then aren't real-world physical effects execution of computation?

There's probably room for semantic disagreements here. It does seem that the definition is somewhat tautological, but I'd claim that that's because the two are equal.


To an extent, but I think there is still a counter example that gets to why this is such a subtle distinction (computable vs "reducible to a mathematical procedure").

Consider an "analog" computer that is in principle noise-free (i.e. elementary operations like addition on this hardware are performed by adding up two analog quantities, e.g. voltages or currents, and these quantities are infinitely smooth, not discreticized/digital, and not disturbed by hardware imperfections and noise). I can create a model of such a device in theory and if I use only the axioms of classical physics (which we now know are wrong), then such a device will be capable of computing and representing numbers that can not be expressed by a Turing machine (i.e. it would be not just faster than a Turing machine or a quantum computer, it will be capable of things that a Turing machine can not ever do).

This is a device that one can imagine existing, and to quote you it is "reducible to mathematical procedure with definite outcomes". It just happens to be a mathematical procedure we find to be rather unreasonable for our universe (because of unavoidable classical thermal noise and non-classical quantum effects that cause discretization).

Some physicists and computer scientists (me included) like to take this as a starting point, as a reason for why certain theories of physics are probably wrong. I personally find this to be a very elegant, powerful, and subtle approach, up there with Noether's theorem or the second law of thermodynamics. "A theory of physics can not be true if it permits the construction of a computing device that can solve the halting problem" seems pretty much on par with "A theory of physics can not be true if it disobeys conservation laws / causality / locality / entropy considerations". All of this with the caveat that one should not be dogmatic about these vague statements, rather just take them as a general guideline.


I agree with what you're saying (as much as one can as an outsider). But, going back to the original claim, could you say the physical systems that bind our particular universe could be classed as executed 'computation', given that they likely could be computed by a Turing machine?

Side-question: is computation, by definition, strictly limited to that achievable by a Turing machine?


I do not think we have an answer to the first question. At the end it does not really matter whether our universe runs on an actual computer or is simply equivalent to a computable process (as opposed to an uncomputable one). However, for aesthetic reasons some scientists guide their work in theoretical physics by studying specifically only physical laws that are, in principle, computable. Said in other words, some scientist take the "Extended Church-Turing Thesis"[1] as an axiom of physics and work from there.

To the side question, yes, that is a typical definition of "computable" (usually what a CS theorist means by the word). The reason we believe it is a useful practical definition is that (1) such a definition ends up equivalent to a number of other interesting definitions and such a net of equivalences usually ends up being interesting and empowering (2) Turing machines form a "universal" modality of computation because we have proofs that they can "efficiently" simulate other theoretical models of computation (3) We simply do not know of other modalities of computation that can exist in our universe (which is a bit of a circular statement in the context of this conversation) (4) It simply seems to be a useful formalism that enabled us to prove a ton of useful results, so even if it was not as elegant as I claim, it definitely ended up being a productive and practical way of thinking. Side note: Quantum computing muddles the water a bit in terms of what is efficiently computable, but if something is not computable for a Turing machine it is still not computable for a quantum computer (however there are a few things that seem to take exponential time on a Turing machine while taking only polynomial time on quantum computer).

[1]: https://www.scottaaronson.com/papers/npcomplete.pdf


Thanks for your long-form reply. Super informative and entertaining.

For #1, wasn't speaking of the 'universe as simulation' hypothesis specifically, I think an assertion either way is indefensible. It was more about unpacking semantics, i.e., what is the most reductive form of a computation? Does there need to even be an operator that seeks to know an answer? Is computation something that only exists in human context, or can it simply be the unfolding consequences of the 'seed' of the universe? Just rumination on abstract inconsequential ideas :)

#2. I'm familiar with some of the nomenclature is regards to 'computing' complexity, and my question, in retrospect, seems a little silly. Computation is computation. I still only have a lay understanding -- as much as I need to know for perf and the differences between algorithms -- and I'll have a look at that paper and hopefully understand the subject a little deeper.

Thanks again.


I think most of my colleagues that care about such distinctions would say that in the most reductive form one does not need an operator or a goal for the computation. This is the typical assumption I would have when discussing this formalization of the laws of physics.

By the way, if you are fan of SciFi, Greg Egan has very fun stories that play with these ideas (nothing rigorous or seriously scientific, but certainly fun).


Couldn't it be the reverse? Couldn't computation be the closest approximation to pure expression and interaction? Seems to me that this is more natural.

Also, I will bet 500$ that no one will be able to prove that all physics has a logical and mathematical basis within my lifetime :)


I bet the same. I'm not sure that hard determinism could ever be proven, even if it were the case.


Because I don’t think infinite amounts of information, and uncomputable numbers, exist. They are fantasies, and relatively recent ones at that. Unfortunately those fantasies came to dominate 20th century mathematics, and in the guise of string theory obtained a death grip on fundamental physics. Fortunately a new generation of smart people, with intuitions honed on computers, is well placed to capitalize on this arbitrage opportunity.


Thank you for answering. My apologies for not engaging previously with your answer.

I agree that computation is likely a better model than string theory. However I have the humility to not insist that reality must match any set of concepts that I have.

In particular in this case results like the ones discussed at https://www.scottaaronson.com/blog/?p=3827 and https://www.scottaaronson.com/blog/?p=4372 say that quantum mechanical systems can perform operations in ways that are different from and fundamentally impossible for classical computers. Therefore it seems likely to me that classical computing is going to break down pretty hard as a model for how things really work.


> those fantasies… in the guise of string theory obtained a death grip on fundamental physics

What? The real numbers, with all the uncomputable reals included, are used in every corner of physics, not just in string theory. There is no treatment of calculus (with any semblance of popularity) that does not feature the usual real line.


What? The real numbers, with all the uncomputable reals included, are used in every corner of physics, not just in string theory. There is no treatment of calculus (with any semblance of popularity) that does not feature the usual real line.

First of all, there is no application of physics where uncomputable reals make one bit of difference. Unpopular treatments of Calculus that only deal with computable numbers exist and produce the same results for physics.

Secondly, physicists have a well-known disregard for whether official mathematical constructions support how they are using them. To name but two examples, both the Dirac delta and renormalization were in wide use long before any formalization existed that could justify them.

Given that, there is no way in which the use of mathematics by physics serves as justification for the reality of the obscure mathematical notions that mathematicians have developed.


> Unpopular treatments of Calculus that only deal with computable numbers exist and produce the same results for physics.

I'd really appreciate if you named them. I've seen synthetic differential geometry, which isn't nearly well-developed enough for use in all of physics, and I've seen nonstandard analysis, which obviously doesn't do away with the uncomputable reals at all.

> there is no way in which the use of mathematics by physics serves as justification for the reality

I am not saying the standard reals are real. I am saying that they are more convenient than any existing alternative, and fulfil the current needs of all of physics. I am also saying that the parent's claim that "uncomputable numbers … in the guise of string theory obtained a death grip on fundamental physics" is absurd, since string theory and uncomputable reals are pretty much unrelated.


I was thinking intuitionistic math, such as smooth infinitesmal analysis.

And yes, they are less developed than classical analysis, and harder to work with. But should not produce different results.


As someone who does lots of constructive math, intuitionistic math can't reproduce a large number of results on the reals and this is a kind of well-known thing. Even basic notions of continuity can't be reproduced in the same way and as a result there are multiple competing formalisms. It is possible that there are alternative ways to reproduce results of interest to physics but that's far from obvious.


The world of SIA and SDG is a very, very different world to that of classical analysis. If you think that they "should not produce different results", then

(a) you're either wrong or incredibly optimistic regarding our ability to carefully rephrase the statements of classical analysis in a way that works constructively.

(b) what would be the point of a harder-to-use system that offers exactly the same results, anyway? The whole reason I find SDG interesting is that it will eventually be simpler to use, and because it provides an entirely fresh of the number line.


Nothing in physics has infinite precision. Math is an abstraction - which is to say a stylised representation - and while you can imagine processes and representations with infinite precision, that level of precision is metaphysical.

This confuses Platonists who seem to believe that differential equations really exist - somewhere.

But that's like arguing that you will clock up air miles by zooming around Google Maps.

The set of operations you can perform on representations of reality is in no sense identical to the set of operations you can perform on reality itself.

If this still isn't obvious, try to differentiate a rock.


I'm not disagreeing that the real numbers have no physical basis; that would be silly. I'm disagreeing with the absurd claim that "uncomputable numbers … in the guise of string theory obtained a death grip on fundamental physics". The real numbers are used in every single part of physics, and physicists do not care to distinguish between computable and non-computable reals, because that makes the theory much more complex with no known practical benefit.

I also wish that the person I initially replied to would expand on their vague claim that

> Fortunately a new generation of smart people, with intuitions honed on computers, is well placed to capitalize on this arbitrage opportunity.


I don't know why you’re being downvoted. This is a rather good analogy. And it doesn't mean the initial comment of this thread is not presumptuous. In other words, the why should the expectation be that general authors assume universe be computational in nature, is sorely missing. But it doesn't invalidate an explanation of how analytical and discrete systems are yet unreconciled (and may never be).


Heartening to see that unusual perspectives and opinions are rewarded with downvotes.


I suspect the downvotes are due to (1) the lack of intellectual humility and (2) misrepresentation in your comments. Plenty of physicists agree that uncomputable numbers are unphysical and the idea that infinite information density can not exist is in no way new or controversial (it is pretty much the starting point for the holographic principle, one of our main paths to a theory of everything). They are beautiful ideas worth discussing, but you used your knowledge of them to disparage people and fields which it seems you only have passing familiarity with.


Yes. It is dogmatic, not scientific, to suggest that a paper is worthless because the authors didn’t frame their argument under some set of axioms you just really identify with, conceptually.


It'd be hard for it not to be yet remain consistent with observations and conservation laws.

Depends what you mean though. Define "computer".


See this sibling comment for context https://news.ycombinator.com/item?id=24948188

The definition you are looking for is very well established and intensely studied in physics and theoretical computer science. This is a good place to start a wikipedia exploration of the topic: https://en.wikipedia.org/wiki/Church%E2%80%93Turing_thesis


> Information, they now say with confidence, does escape a black hole. If you jump into one, you will not be gone for good. Particle by particle, the information needed to reconstitute your body will reemerge. Most physicists have long assumed it would; that was the upshot of string theory, their leading candidate for a unified theory of nature.

Does this mean string theory produced a prediction? I thought it had no predictive power and that's why people didn't like it.


Maybe not. From the article: "But the new calculations, though inspired by string theory, stand on their own, with nary a string in sight. Information gets out through the workings of gravity itself — just ordinary gravity with a single layer of quantum effects...Over the past two years, physicists have shown that the entanglement entropy of black holes really does follow the Page curve, indicating that information gets out. They did the analysis in stages. First, they showed how it would work using insights from string theory. Then, in papers published last fall, researchers cut the tether to string theory altogether."

Sounds like there is no dependency on string theory.


I took that to mean that they don't use string theory to prove anything per se. But it sounds like they got "insights" from string theory, which seems like it was useful for once? IANAP.


I am a mathematician with some physics background and have been skimming this article: they took mathematical inspiration from string theory in terms of how they formulated the path integrals, but the physical concept of a string doesn’t actually appear. So string theory provided analytic tools but didn’t actually provide physics.


I'm a former string theorist and no, it didn't produce a prediction here.

The problem with getting predictions out of ST is that you need to find a vacuum (ground state) with 3 macroscopic space dimensions and no scalar fields (except for a Higgs). It is historically done by keeping some supersymmetry (for instance using Calaby Yau Manifolds) to keep the problem mathematically tractable. It is then a problem because no supersymmetry was found at CERN where it should have been (in some models) with this particular Higgs mass.

This however doesn't mean that the theory has nothing to say. For instance AdS/CFT from which this paper uses inspiration was discovered using ST, but is believed to be more general.

Also, i can tell you after working 4 years in the field: I think string theory (theories is more exact, there are at least 6) is incomplete: the part we understand is just a sector of a bigger theory where things are nice and geometric. For instance: many people say you cannot get flat vacuum in ST, this is incorrect some perfectly sound ST's have Minkowskian vacuum.

Now for the hatred of some people against it (including many on this forum): some physicists in the field had big promises that were not kept, and that was a big mistake of them exposing their half-baked models to the public as it was The Solution. ST on Calaby Yau is indeed not the solution. On the other hand people like Lee Smolin and Sabine have overreacted (many times with bad arguments, and i respect their work and some of their criticism but it's not like they have perfect models themselves..) to this and the result ugly: An open war and a beautiful field of physics which is now destroyed by personal egos, collapsing funding and no hope for permanent postions.

Let's be honest, no one understands a thing at this organised mess we call Nature. Not even Witten.

In the end, be it MOND, ST, LQG, etc, etc they are just models, some models have no implementation in the real world but might be useful to improve our understanding of the world, this is how Physics works. It is very sad that people now think of ST vs LQG like one should choose her/his religion, i find them both beautiful theories personally. It's for a reason i left the field i can tell you.

Anyway: Nice result <3


Really appreciate this no-nonsense explainer.


Not in a useful sense, it just matched with another theory. The problem with string theory remains that we can't actually measure any of its predictions.


I’m glad Quanta changed the title (it should be changed here too). The research is interesting, but the paradox is in the same place it’s been in for years, ie “locality probably doesn’t survive the paradox”.


"To astronauts who ask whether they can get out of a black hole, physicists can answer, “Sure!” But if the astronauts ask how to do it, the disquieting reply will be: “No clue.”"

My intuition is that these astronauts would exit the black hole the way a candle exits a flame, i.e., at the atomic or subatomic level, correct?


They would exit as a stream of extremely small and infrequent particles over billions or even trillions of years, depending on the size of the black hole, in most cases ending once all the stars have died and universal expansion has emptied out almost all of the accessible universe.


The title is incorrectly copied. The original says "Nears Its End"


The title probably changed. The URL slug still has "comes-to-an-end".


It seems like every few weeks there are these huge, complicated and profound discoveries in physics. I feel like i missed the boat on this, as if I chose the wrong profession or am missing out on something. I should have pursued math further but I probably would not have been smart enough anyway. Wikipedia has no mention of the page curve, so this is pretty cutting-edge and theoretical even by the standards of theoretical physics.


If it makes you feel better, I studied physics (although only at the undergraduate level) and I still can’t really follow articles like this. If you really want to understand this stuff you basically have to dedicate your life to it, genius or not.


Sean Carrol's Mindscape podcast does a pretty good job explaining things to where an average Hacker News reader would understand things. Highest recommendation. He had someone on recently talking about this paradox, the CFT-ADST correspondance and holographic theory and it was reasonably understandable.


Thanks for the recommendation. We used his textbook in my relativity class and he's definitely a good teacher.


Discussed on Sean Carroll's podcast, Mindscape:

https://www.preposterousuniverse.com/podcast/2020/09/21/115-...

He seems a little non-committal if not skeptical.

One telling exchange near the end regarding the gravitational path integral they used:

* * *

"1:18:41 SC: And there is this trick that you can introduce, ’cause what you’re supposed to do is say, well, integrate up all of the spacetimes that match on to this particular wave function you’re looking at. But the trick is, instead of integrating all the four-dimensional spacetimes that match on to this condition you’re looking at, you can just say, well, I’m going to integrate over all four dimensional spaces, so I’m going to forget about spacetime. I’m just going to do what we call the Euclidean path integral because Euclid just talked about space, not time. And…

1:19:13 NE: Oh, you went there. [laughter]

1:19:15 SC: I did, I did. This is where I’m going. And so it was sort of like you could justify… It’s a trick. It’s a mathematical trick. And it’s very rigorously justifiable in certain simple cases in quantum mechanics, and it certainly has the smell of being correct in certain more subtle cases in quantum field theory. In quantum gravity, what they were doing with it, it just seemed to be a trick so they could get a finite answer at the end of the day, and it was very unclear why it had anything to do with the real world, but they suggested it did. Maybe they were right. And since then, I think we’ve become a little more comfortable with the idea that we can use this trick of calculating quantum gravity wave functions by integrating over the Euclidean path integral, the set of all the spaces that end up looking like what we want, instead of all the spacetimes that look like what we want.

1:20:05 NE: Yes.

1:20:05 SC: And that’s what you’re doing, isn’t it? That’s the kind of wormholes that you’re invoking.

1:20:09 NE: Yes, right. That’s what I was trying to sweep under the rug.

1:20:11 SC: I know. [laughter] And you were right to do so, but I just like to live dangerously here.

[chuckle]

1:20:18 SC: So Lenny and Juan have wormholes that are literally good old in spacetime wormholes, and you have wormholes that are in these fake Euclidean spaces that you used to calculate the entropy.

1:20:29 NE: That’s exactly right. Yeah, that’s exactly right. And these fake Euclidean spacetimes have more boundaries. There are more edges than our original spacetime, which means that these wormholes are connecting these… More edges than we have in our original spacetime, and therefore, it’s difficult to make sense of them in terms of the original spacetime that we’ve started with."

* *


"Muted at first, these effects come to dominate when the black hole gets to be extremely old. The hole transforms from a hermit kingdom to a vigorously open system. Not only does information spill out, anything new that falls in is regurgitated almost immediately."


> extremely old

Completely OT, but this gives an indication of 'old' in this context: https://m.youtube.com/watch?v=uD4izuDMUQA


So if enough matter feel into a black hole, we'd get an entangled parallel universe?

Big question then it's what is the entanglement "key" and its properties. Or how to even brute force it.


Blind leading blind:

My impression was that parallel universes do not feature.

Rather, it was that, contrary to appearances, Hawking radiation contains all the same information that went into the black hole.

However, this information appears only in the joint distribution over those photons rather than in any of the marginal distributions.

Broken metaphor: You throw a coin into a black hole. Was it heads or tails? Two photons escape the black hole, both spin-up* with 50% probability -- they each appear to carry no information about the coin. But suppose that if they are the /same/ spin, then the coin was heads, and if they are /different/ spin then the coin was tails. In this way the coin's information is not destroyed, but is also not carried by any individual photon.

* I have no idea if spin is actually the property of the radiation that carries the information.

I also get the impression that it is later photons that must somehow be entangled with earlier ones. That -- referring to that V-shaped curve -- the black hole is storing up information about what went in up to about the halfway point in time, which it later radiates away during the second half.

Waiting for an actual physisict to chime in, as, disclaimer, I don't actually know anything about this.


There's a Royal Institute video featuring Sean Carroll and Jen Ouelette[1] that more fully explains the problem, but as I understand it it comes down to a quantum mechanical principle called monogamy of entanglement---there's only so much entanglement to go around, and if two particles (e.g. the pair of Hawking radiation particles) are fully entangled then they cannot have any amount of entanglement with anything else (e.g. information about the black hole). The result in TFA breaks the entanglement between the Hawking pair, allowing the outgoing particles to encode the black hole's information.

[1] https://www.youtube.com/watch?v=_8bhtEgB8Mo


I read it as "every photon emitted carries information about everything that fell into the hole up until that point, but you don't get complete information about everything until the very last photon is emitted".


>You throw a coin into a black hole. Was it heads or tails?

being heads or tails is a property of landing with all of one side of the coin facing down. This does not seem possible in the situation described.


Of course, but it doesn't matter. Any bit of information can do the trick here.


To which my wife says, "Well, we've always said information wants to be free." I (heart) my wife.


It would make more sense to me if black holes had no internals, so the matter exists on the surface of the horizon. No infinities, and the matter can slowly escape over time. Maybe something in the nature of gravity which prevents more than a certain density to exist in any place and time.


Right, except (my lay understanding is) that would require something special to happen to infalling matter at the event horizon, though we don't have a plausible theory for what that thing is--the prevailing interpretation is that passing through the event horizon is a non-event for the observer.

On the other hand, the holographic principle says that the event horizon surface is big enough to contain all the information, so in a way of speaking we seem to be free to model black hole information as though it is "on the event horizon".


The holographic principle combined with "infinity means the theory fails" is what brought me to post my -3 voted comment. Interestingly, none of the commenters have been negative only the casual down-voters. Where's PBS Space Time when you need them?


>It would make more sense to me if black holes had no internals, so the matter exists on the surface of the horizon.

That may still be the case, but for that we need a theory of quantum gravity.


To an external observer, new material takes an infinite amount of time to cross the event horizon. So your intuition is kind of right there. But there is matter that starts out inside the horizon, and there needs to be something going on in there because otherwise the gravity would keep pulling it tighter and tighter to infinite density in an infinitely small spot (the original meaning of "singularity").


> To an external observer, new material takes an infinite amount of time to cross the event horizon.

While this is a common pop science statement, it is not correct. The correct statement is that the external observer never sees the material cross the event horizon, because, heuristically, it would take an infinite time for light emitted exactly on the event horizon to get out to the external observer. However, this does not equate to the external observer being able to assign an "infinite time" to the material crossing the horizon. The notion of "time" the external observer would have to use to do that is mathematically undefined on the horizon.

> there is matter that starts out inside the horizon

No, there isn't. When an ordinary object like a star collapses to a black hole, there is no horizon at all to start with, and there is no matter starting out inside any horizon.


It's that "keep pulling it tighter and tighter" that I'm wondering about. What if there's a separate force, or an aspect of gravity itself, which prevents a certain amount of gravitational density?


In my mental model the internal structure of the black hole, composed of all the material that fell into it, is always preserved from some frame of reference.

As you fall into a black hole the event horizon shrinks away below you and from your own POV you never cross it. Thats true of every particle or photon it traps. Of course they get twisted and distorted by the extreme gravitational forces, but in principle there is always structure. I suppose from the internal perspective, Hawking Radiation manifests as a rain of negative energy.

I'm sure I'm wildly off the mark, but it's the best I can do.


>As you fall into a black hole the event horizon shrinks away below you and from your own POV you never cross it.

You have it backwards. From the POV of an external observer you never cross the event horizon, because that's a function time dilation, and light that you emit being more and more red-shifted as you get closer to the event horizon. From the falling observer POV, nothing really changes - or rather, what happens close to the event horizon or just past the event horizon depends on what the theory of quantum gravity says.


I didn't address the POV of an external observer but I'm sure you're right. But what you describe for the POV of someone falling in seems consistent with what I suggested. I don't understand what you think is backwards about it.


You said that from the perspective of a falling observer, they never see themselves cross the event horizon. That's not right. The falling observer certainly will see themselves cross the event horizon. In their frame of reference, time flows normally. For smaller black holes, they may get spaghettified, but for larger ones, crossing event horizon will be an unremarkable occurrence.


There will always be an event horizon below them beyond which light cannot reach them, and they will always be able to observe the external universe. So how will they see themselves crossing the event horizon?


> There will always be an event horizon below them beyond which light cannot reach them

Wrong. See my other response upthread.

> they will always be able to observe the external universe

But the light coming to them from the external universe will be more and more redshifted, and they can calculate from the observed redshift when they have crossed the horizon.

Also, they will only see a limited portion of the future of the universe; anything that happens later than a fairly short time after they cross the horizon, they will never see, because they will hit the singularity inside the hole before light from such events can reach them.


The usual definition of event horizon is from the perspective of the external observer—the falling astronaut can calculate the threshold at which no amount of thrust can ever move them away from the singularity (in fact, this is what is meant that a time and space coordinate switch places—you can now only move 'down' in space, just like you can only move forward in time).


> The usual definition of event horizon is from the perspective of the external observer

Strictly speaking, no, the usual definition of event horizon is completely observer independent: the event horizon is the boundary of the region of spacetime that cannot send light signals to infinity. That region, and its boundary, are invariant geometric properties of the spacetime, independent of any observer.

> time and space coordinate switch places

This is a common pop science statement, but it can be very misleading. It would be better to say that, inside the horizon, moving "down in space" (meaning, decreasing the surface area of the 2-spheres you pass through, since the radial coordinate that you are using is defined in terms of those areas) is moving forward in time: the "forward in time" direction in spacetime is also the "decreasing areal radius" direction in spacetime.

Even that, however, depends on a particular choice of coordinates. There are other choices of coordinates where it is not true (at least not in the simple form in which I have just stated it).


> no amount of thrust

Are you sure that's right? Thrust implies acceleration, not just velocity.

Suppose you're just inside the event horizon, from the perspective of an external observer. You're traveling outward at a velocity of .95c. That's lower than the escape velocity (which is > c), so you're going to fall back in before you actually get to the external observer. But if you were close to the event horizon you might cross back over it before you fall back in, right? At which point the external observer could see you again.

And once you're outside the event horizon, e.g. to the place where escape velocity is .9c, you might by then have slowed to .8c, but if you still have the capacity to accelerate back above .9c again, you could still get out, couldn't you?


> Are you sure that's right? Thrust implies acceleration, not just velocity.

Yes. The simpler answer is that even if you shoot a laser straight up the light can't get out, and the corollary is that you can't get out yourself even with arbitrarily high thrust.

No matter how much thrust you have to fight against gravity, light will always beat you, because light cannot be slowed down by gravity. If light is trapped then you are trapped.

> You're traveling outward at a velocity of .95c.

Let's make it simpler, and calculate what it takes for the outside observer sees you moving away from the black hole at all, even 1mph.

The closer you get to the black hole, the higher your local speed has to be. If you're 10 meters outside the event horizon, you have to get up to 99.999etc. percent of light speed (locally measured) just to slowly inch away from it (as measured by the outside observer), or even just to stay still. Once you fall inside the event horizon, you would have to go faster then light locally for the outside observer to measure you as moving upward.


> Are you sure that's right?

It's right.

> Suppose you're just inside the event horizon, from the perspective of an external observer.

Whether or not you are inside the event horizon is not a matter of perspective. All observers will agree on it.

> You're traveling outward at a velocity of .95c.

Relative to what?

Outside the horizon, velocities, such as the escape velocity you mention, are usually meant as velocities relative to static observers--observers who are maintaining the same altitude above the horizon.

But below the horizon, there are no static observers. It is impossible to maintain a constant "altitude" (which here just means the surface area of the 2-sphere at your location, centered on the hole) even for an instant. So "velocity" relative to a static observer has no meaning inside the horizon.

> That's lower than the escape velocity (which is > c), so you're going to fall back in before you actually get to the external observer.

No, that's not what happens. Relativity is not Newtonian physics.

The event horizon is not a place in space. It is an outgoing null surface: a surface formed by radially outgoing light rays. Spacetime around the black hole is curved in such a way that this particular outgoing null surface has a constant surface area: in other words, even though there is a full 2-sphere's worth of radially outgoing light rays at the horizon, the surface area of the 2-sphere formed by those light rays is constant--the 2-sphere does not expand, as you would expect a radially outgoing spherical wave front to do, because of the curvature of spacetime.

If you are just a little bit inside the horizon, you are on a slightly smaller 2-sphere, and on that 2-sphere, even radially outgoing light rays cannot stay in the same place, much less expand; they contract--that spherical wave front, even though it is radially outgoing, decreases in area with time, i.e., it is falling. So you, having to move slower than light, will fall even more. You can't move outward at all; you can't even stop moving inward. (The fact that there are no static observers inside the horizon is a consequence of this.) That is true no matter how hard you accelerate, since no amount of acceleration will let you move faster than light.


I suppose they could calculate the theoretical event horizon from infinity, but they won't observe it, however they will observe one below them.


> they will observe one below them

No, they won't. This is simply wrong. See my other responses upthread.


> From the POV of an external observer you never cross the event horizon

More precisely, the external observer never sees you cross the horizon. But he can still deduce that you did from other data. So the external observer does not say "you never cross the horizon", period. He just can't see it happen.


This still isn't quite right. In the coordinate system of an observer at a constant distance from the horizon, the path of a free-falling object takes an infinite amount of coordinate time.

In this coordinate system, the time coordinate becomes space-like passed the event horizon and the radial coordinate becomes timelike. There is a coordinate singularity around this switch, which is where the infinite coordinate time comes from.

An observer fammiliar with relativity could compute the proper time of a path traversing the event horizon, which they would find to be finite.


> In the coordinate system of an observer at a constant distance from the horizon, the path of a free-falling object takes an infinite amount of coordinate time

No: the path of the free-falling observer at and beneath the horizon is not covered at all by the coordinate system of the external observer. That coordinate system simply becomes mathematically undefined, which means you can't use it to make any claims about what happens.

> In this coordinate system, the time coordinate becomes space-like passed the event horizon and the radial coordinate becomes timelike.

No: there is a separate coordinate patch that covers the region inside the horizon (but not the horizon itself--the horizon is not covered by either patch), in which the "areal radius" coordinate is timelike, and in which the coordinate corresponding to the extra Killing vector field is spacelike. Calling the former coordinate "radial" is at least justifiable, since it still is the "areal radius" coordinate even though it's timelike. But calling the latter coordinate "the time coordinate" is simply wrong; the fact that the letter t is commonly used for it does not mean it's a "time" coordinate in any meaningful sense.

> There is a coordinate singularity around this switch

Yes.

> which is where the infinite coordinate time comes from.

No, which is what makes statements like "infinite coordinate time" incorrect; the correct statement is that neither coordinate patch covers the horizon at all.

> An observer fammiliar with relativity could compute the proper time of a path traversing the event horizon

Yes. The easiest way to do that is to switch to some other coordinate chart which covers the entire path, above, at, and below the horizon. In such a coordinate chart, the "areal radius" coordinate will not be timelike below the horizon. (In at least one chart commonly used for this, Painleve coordinates, all four coordinates are spacelike below the horizon.)


I'm not sure what you mean by coordinate "patch" in a format sense; although I think I informally get what you are going for. Since we seem to agree that an external observer sees a coordinate singularity at the horizon [0], it is not clear to me that there is an objective answer to what "their" coordinate system looks like on the interior. I tend to use a hyperbolic coordinate system. In the region on the outside of the horizon, it matches the natural coordinate system for an observer maintaining constant acceleration away from the black hole. From a purely geometric perspective, it is also defined on the region inside the horizon.

By "time coordinate" I mean the hyperbolic angle. This corresponds to the proper time of our constantly accelerating observer. This remains a well defined coordinate on the interior of the black hole. As you identify, in the language of relativity, this is a spatial coordinate on the interior of the horizon. I specifically refer to this as "coordinate time" because it is the coordinate that our observer is using for time; not because it is actually a time coordinate in all regions of space-time.

> No, which is what makes statements like "infinite coordinate time" incorrect; the correct statement is that neither coordinate patch covers the horizon at all.

You do not need to consider the horizon itself. Consider just portion of the path that occurs before the horizon. This path crosses infinite coordinate time. Put another way, the singularity in this coordinate system is precisely that coordinate time diverges towards infinity as you approach the horizon. Put another way, if you pick any finite amount of coordinate time, you can find a portion of free-falling path from before the horizon that crosses that amount of coordinate time .

[0] Although I think we need to be a bit more careful about what we mean by external observer for this to be formally true. A free falling observer is "external" until they cross the horizon, but they don't see a coordinate singularity there.


> I'm not sure what you mean by coordinate "patch"

I mean that there are two separate, disjoint regions of spacetime (one outside the horizon and one inside the horizon), and each one is covered by a separate coordinate chart. Informally people often talk as though those two charts are "the same", but they're not. They're two separate coordinate charts, that just happen to be described using the same symbols.

> we seem to agree that an external observer sees a coordinate singularity at the horizon

No, we don't agree about that. The coordinate singularity is only there for the particular coordinates we are talking about (which cannot cover the horizon). There are plenty of other possible choices of coordinates that do not have a coordinate singularity at the horizon, so a single coordinate patch covers the entire region of spacetime of interest.

There is a certain sense in which the coordinates we have been using (Schwarzschild coordinates) are the "natural" ones for an observer who is at rest relative to the hole. But one has to be very careful not to put too much weight on that; it can easily lead to errors if taken too far.

> I tend to use a hyperbolic coordinate system.

Can you give a reference for this? What you are describing in your next paragraph (about "hyperbolic angle" and so forth) does not seem like any of the coordinate charts I am aware of for Schwarzschild spacetime (Schwarzschild, Painleve, Eddington-Finkelstein, Kruskal-Szekeres, or Penrose).

> In the region on the outside of the horizon, it matches the natural coordinate system for an observer maintaining constant acceleration away from the black hole.

This is just Schwarzschild coordinates; any observer who is at rest relative to the hole (a static observer) has to maintain constant outward proper acceleration to stay that way. Close enough to the horizon, these coordinates can be approximated by Rindler coordinates on flat spacetime, which are a commonly used coordinate chart in special relativity for treating observers with constant proper acceleration.

However, if Schwarzschild coordinates are what you have in mind, first, your next paragraph doesn't seem to be describing them at all, and second, the key property you give here does not hold on the patch inside the horizon, since there are no static observers there.

> Consider just portion of the path that occurs before the horizon. This path crosses infinite coordinate time

No, it doesn't. Every event on the path that is outside the horizon has a finite value of Schwarzschild coordinate time. You even say so later in this paragraph, so you appear to be contradicting yourself.

It is true that, for some cases, you can take limits as Schwarzschild coordinate time increases without bound to compute quantities that are finite on the horizon. In fact, the proper time experienced by an infalling observer from some altitude above the horizon, to the horizon itself, is one of them. But you cannot use this limiting process to justify saying that the Schwarzschild coordinate time itself "is infinite" at the horizon.

> A free falling observer is "external" until they cross the horizon, but they don't see a coordinate singularity there.

Any observer can choose any coordinates, regardless of their state of motion. Whether any observer "sees a coordinate singularity" at the horizon is purely a matter of which coordinates they choose, and has no physical meaning.


> As you fall into a black hole the event horizon shrinks away below you and from your own POV you never cross it.

No, this is not correct. To the extent that the horizon is something that can be "seen" at all, you see it when you cross it. It doesn't shrink away below you.

> I suppose from the internal perspective, Hawking Radiation manifests as a rain of negative energy.

This is a common heuristic picture, but it is very limited. No real particles fall into the hole as a result of Hawking radiation. An observer already inside the horizon might be able to deduce that Hawking radiation was being emitted from local observations on, say, the tidal forces in his vicinity, but I'm not sure even that would be true: the models I am familiar with for evaporating black holes do not require any causal connection at all between the emission of Hawking radiation and any particular observer inside the horizon (in more technical language, the two remain spacelike separated for the entire trajectory of the observer inside the horizon).


Does that mean the finite duration of a black hole to an outside observer prior to its evaporation corresponds to an infinite duration of an observer within the black hole?


No. An observer who falls into the hole only experiences a finite duration before he hits the singularity and is destroyed.



I think you might be a bit reversed; an outside observer will never see you fall past the event horizon (because it would be impossible for light from you to reach them), but unless you happen to fall into a black hole with a "fire wall", you won't experience anything special when passing through the event horizon, aside from the already high tidal forces.


>already high tidal forces.

Tidal forces are low for supermassive black holes, right?

https://en.wikipedia.org/wiki/Supermassive_black_hole#Descri...


At least to me, it's pretty obvious that the shadow follows the form. Gravity is like an echo for mass. It seems that we are now realizing it was wrong to assume that the echo was homogenous. The electron movement process in atoms is emitting gravitational waves. The movement of any type of energy causes gravitational waves. Gravity won't be homogenous if the pattern of mass-energy emitting it, isn't homogenous. We know most mass comes from cyclic processes, ie. the inner processes of hadrons. So it stands to reason that those processes should have a unique and animated gravitational field.


one hydrogen atom doesn't have enough mass to produce a graviton.


General Relativity has no quantization, so all minor changes are infinitely perturbated. Now if you choose to go with some kind of quantum gravity, the energy of a graviton wouldn't be fixed, it would vary depending on the frequency of it.

https://en.wikipedia.org/wiki/Graviton#Energy_and_wavelength




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