
Adam Brown – How Future Civilizations Could Change The Laws of Physics
Adam Brown is a founder and lead of BlueShift with is cracking maths and reasoning at Google DeepMind and a theoretical physicist at Stanford.
We discuss: destroying the light cone with vacuum decay, holographic principle, mining black holes, & what it would take to train LLMs that can make Einstein level conceptual breakthroughs.
Stupefying, entertaining, & terrifying.
Enjoy!
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Timestamps
(00:00:00) - Changing the laws of physics
(00:26:05) - Why is our universe the way it is
(00:37:30) - Making Einstein level AGI
(01:00:31) - Physics stagnation and particle colliders
(01:11:10) - Hitchhiking
(01:29:00) - Nagasaki
(01:36:19) - Adam’s career
(01:43:25) - Mining black holes
(01:59:42) - The holographic principle
(02:23:25) - Philosophy of infinities
(02:31:42) - Engineering constraints for future civilizations
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Full Transcript
Today, I'm chatting with Adam Brown, who is a founder and lead of the Blue Ship team, which is cracking math and reasoning at Google DeepMind, and a theoretical physicist at Stanford. Adam, welcome.
Delighted to be here. Let's do this.
Okay, we'll talk about AI in a second, but first, let's talk about physics. Okay.
First question, what is going to be the ultimate fate of the universe? And how much confidence should we have? The ultimate fate is a really long time in the future, so you probably shouldn't be that confident about the answer to that question. In fact, our idea of the answer to what the ultimate fate is has changed a lot in the last hundred years.
About a hundred years ago, we thought that the universe was just static, wasn't growing or shrinking, was just sitting there statically. And then in the late 20s, Hubble and friends looked up at massive telescopes in the sky and noticed that distant galaxies were moving away from us and the universe is expanding.
So that's like big discovery number one. There was then a learned debate for many years about the universe is expanding, but is it expanding sufficiently slowly that it'll then re-collapse in a big crunch, like a time reverse of the Big Bang, and that'll be super bad for us? Or is it going to keep expanding forever, but just sort of ever more slowly as, you know, gravity pulls it back, but it keeps, it's fast enough that it keeps expanding? And there was a big debate around this question, and it turns out the answer to that question is neither.
Neither of them is correct. In possibly the worst day in human history, sometime in the 1990s, we discovered that in fact not only is the universe expanding, it's expanding faster and faster and faster.
It's what we call dark energy or the cosmological constant. It's just a word for uncertainty.
It's making the universe expand at an ever faster rate, accelerated expansion as the universe grows. So that's a radical change in our understanding of the fate of the universe.
And if true is super duper bad news. It's really bad news because the accelerated expansion of the universe is dragging away from us lots of distant galaxies.
And we really want to use those galaxies. We have big plans to go and grab them and turn them into vacation destinations or computronium or in any other ways extract utility from them.
And we can't if the cosmological constant is really constant, if this picture is correct, because anything close enough, we can go out and grab it, obviously. But if it's further away than about a dozen billion light years the expansion of the universe is dragging it away sufficiently rapidly that even if we send probes out at almost the speed of light they will never make it they will never make it there and make it back they'll never even make it there if it's sufficiently far away and that means that there's a finite amount of free energy in our future and that's bad i mean that means we we're doomed to a heat death if that's true um but is it true is it i mean that was the second ask for your question and you know first of all we keep changing our minds about these things over the last century or so so on first principles grounds you may be somewhat suspicious that we'll change our minds again and none of this is settled physics and indeed it may be that the cosmological constant is not constant and you should you should hope with all your heart that it's not it may be that it naturally bleeds away it may be in fact that our fate is in our hands and that our distant descendants will go and bleed the cosmological constant away will force it to go to zero they will be strongly incentivized to do it if if they can because otherwise we're doomed to a heat death.
How would they breathe this away? Oh, okay. This obviously depends on physics that we're not totally sure about yet.
But it seems pretty consistent with the known laws of physics that the cosmonautical constant, what we perceive it as being a constant, this dark energy quantity that's pushing the universe apart from each other. In many very natural extensions of the known laws of physics, that is something that we have the ability to change.
In fact, it can change, can take different values. It is not just totally fixed once and for all.
That in fact, you have what's called different vacuum, different regions of parameter space that you you can transition between in which the cosmological constant can take different values and if that's true then well you could either sort of wait around and hope to get lucky hope that the universe just sort of spontaneously moves from one of these vacuums to another one with a lower cosmological constant tending towards zero asymptotically. Or you could take matters into your own hand.
Or you could imagine our descendants deciding that they're not going to just suffer the heat death, that they're going to try and trigger a vacuum decay event to get us from one vacuum we're in to another vacuum with a lower cosmoversial constant. And our distance descendants will be forced, basically, to do that
if they don't want to suffer a heat death.
Proceed with caution.
But definitely proceed with caution.
In these theories where there's lots and lots of vacuums out there,
and most of those vacuums are incredibly inhospitable to life as we know it.
In fact, seemingly they're just completely inhospitable to all forms of intelligence.
So you really, really don't want to end up in them.
How do you feel? incredibly inhospitable to life as we know it. In fact, seemingly, they're just completely inhospitable to all forms of intelligence.
So you really, really don't want to end up in them. However, again, if our best theories are correct, it seems as though there should be some of them that are much like our own in many ways, but have a lower value of the cosmological constant.
And so what we'd want to do is engineer that we end up in one of those vacuums. Sorry, what is a vacuum? Ah, great question.
A vacuum is like a possible, well, what we would perceive as a possible set of laws of physics as we see them. So it's what it really is, is a minima in higher dimensional uh abstract laws of physics space uh in which you can find yourself in a minima but these minima may just be local minima in fact according to our understanding are the minima which we live today is that gives us all the laws of physics that we see around us is in fact just a local minimum and there's a lower minimum in fact there's many lower minima out there to which we can transition spontaneously or because of our own deliberate action.
Okay, I'm just going to throw all my confusion at you and you figure out which one is worth dealing with first. What is the nature of the loss function that makes one value a minimum and one higher up? You know, what is exactly the ball rolling up on when it gets out or into a valley here um and then you're hinting at the possibility that there are other other places in i'm not sure if you're suggesting in the physical universe or in some hypothetical universe where the vacuum could be different as in in, in reality, there are other pockets with different vacuums or that hypothetically they could exist or that our universe kind of factually could have been one of these.
I don't know. This is the kind of thing I'd like throw into like, you know, just like put everything I can into like a clot prompt and see what comes out the other end.
Good. Well, I'm happy to be your clot.
The loss function is the energy density. And so maybe a good analogy would be water.
Water can exist in many phases. It can be steam.
It can be water. It can be ice.
And even if it's in a cloud, let's say it would rather rather be water than be water vapor but it's having a tough time getting there because in in the middle there's a there's a barrier and so you know that's just spontaneously it can eventually due to a sort of thermal process turn from steam into to water these will be like the two minima in this in this landscape. And or you can go and do cloud seeding to turn it from water, from water vapor into water.
And so those would be the equivalent of the minima here. The existence of different minima in general is a very well-established part of physics.
The possibility that we could engineer going from one minima to another in a controlled way is a more speculative branch of physics speculation, but it seems totally consistent with everything we know that our distance attendants would try to attempt it. What would it take to do this? Probably you'd want something that would look a bit like a particle accelerator, but it would be considerably more controlled.
You'd need a very controlled way to collapse a field and make a bubble of this new vacuum that was big enough that it would continue to expand, rather than just reclapse under its own surface tension. You'd have to do that in a very careful way, both to make sure that you didn't, you know, accidentally make a black hole instead by the time you concentrated all those energies, and also, you know, worse than making a black hole would be ending up in a vacuum that you didn't want to end up in, would be ending up in a vacuum in which you had not only bled off the cosmological constant in some way, but that you had changed, let's say, the electromagnetic constant, the strong nuclear force or any of those other forces,
which would be seriously bad news.
Because if you did that,
your life as you know it is extremely well attuned
to the value of the electromagnetic constant
in your evolutionary environment.
It would be very, very bad indeed
if we changed those constants as well.
We'd really just try and target
the cosmological constant and nothing else.
And that would require a lot of engineering prowess.
So sorry, it sounds like you're saying that changing the laws of physics is like, it's not like some crazy, it's not even like Dyson sphere level crazy. It's like somebody could do it on like some planet in the middle of...
I'd say it's definitely substantially harder than Dyson Spheres, as far as the tech tree goes. But it's not...
Yeah. What do we mean by changing the laws of physics? Like, that just sounds like magic.
We're not actually changing the laws of physics. We're just changing the laws of physics, the sort of low energy laws of physics, as they present to us.
In this scenario, again, this is speculative, but it's not like super duper crazy. It's a natural consequence of our best theories of, or at least some of our best theories of quantum gravity, that they allow for this possibility.
And there is a meta law of physics, the true laws of physics, be it string theory or whatever else, that you're not changing. That's just the rules of the game.
What I'm describing is changing the way that the universe looks around you, changing the cosmological constant. So I think, again, changing water vapor into water is a great analogy here.
There's nothing actually, the laws of physics are still the laws of physics, but the way it feels to live in that universe, you know, the value of the electromagnetic constant is perhaps not an absolute fixed value. It can vary in different places.
And one, similarly, the density of water around you, the viscosity would change. It'll be an environmental variable like that.
Yeah. So one question you might have is if this is the thing that could sort of, I don't know if organic is the right way to describe it, but maybe spontaneous.
If this is the thing that can just like kind of happen. there's something really interesting where like if a thing can happen
you kind of see
examples if this is the thing that can just like kind of happen. There's something really interesting where like, if a thing can happen, you kind of see examples of it happening before.
So even with nuclear weapons, I don't remember the exact phrase. I'm sure you actually probably know what it is.
But wasn't it the case that early in Earth's history, when there was a higher fraction of 238 isotopes, that there were spontaneous nuclear explosions? There probably was spontaneous nuclear reactors, not nuclear. They've discovered a seam in Africa where it looks like there was a fission reaction that naturally happened.
It didn't explode, but it did do the same thing that happens in our nuclear power plants. You know, one way you can look at like nukes is like, oh my gosh, this is like, this thing just would not have been possible if some intelligent beings hadn't tried to make it happen.
But, you know, like something like this happened before because the laws of physics allow it. Is there any story you can tell here where this vacuum decay is like, in one sense, maybe it takes like a super intelligent species to coordinate to make it happen.
But also because it is a thing that the laws of physics can manufacture or can allow for, it has happened before or is happening or something. Yeah, I mean, absolutely.
Almost certainly. Anything that humans can do can happen without humans.
It's interesting to reflect on what aspects of human behavior nature has a tough time doing without us and what it just does on its own for example we we make colder things in our laboratories than really exist naturally in the universe but the universe suddenly could make anything colder just by chance but yeah yeah vacuum decay is something that if it is possible will in our future definitely happen that's just like a feature of the world that eventually due in in our distant future if it's possible at all it will happen due to a quantum fluctuation our descendants may not wish to wait around for a quantum fluctuation to happen they may wish to take the fate into their own hands since the quantum fluctuations can take exponentially long times to happen and if they even happened you'd end up in a unfavorable vacuum not hospitable for life rather than trying to steer the cosmological constant in a happy direction but they certainly can happen and in our future, and indeed definitely will happen if they're permitted. According to our understanding of quantum mechanics, if they're permitted, they must eventually happen.
Furthermore, there are, again, speculative but not wild theories of the early universe in which this happened in our past, in which we transitioned far, far in the past, maybe into what's called a bubble universe. So we started off in some other much higher vacuum long in the past.
And then what we see as the Big Bang was, in fact, just a sort of local vacuum decay that then gave rise to the bubble in which we live, everything we see around us. Who would be in a position to seed these bubbles? Usually people are thinking that something just spontaneously happens, you know, like in the same way that rain spontaneously happens in a cloud, that somebody didn't go and seed it deliberately to make it happen.
But you could, more than free to speculate, that somebody seeded it to make it happen as well. How does this respect the conservation of energy or the conservation of that? Energy is not conserved in general relativity.
Energy is not conserved. It's conserved locally at things you can do at a local level.
But in an expanding universe, energy is not conserved globally. This is one of the big surprises.
This is not some, that is not a speculative statement. That is a statement that goes all the way back to Einstein and general relativity, is energy is simply not conserved at the global level.
It's conserved at the local level. You can't do something in your lab that will generate free energy.
But if you can participate in the expansion of the entire universe, then energy is not conserved. So if you were to spawn a bubble universe in your lab, you've theoretically created a lot more matter and energy.
And what would be the thing that offsets this or that makes this viable? Energy is conserved in a universe that's not expanding. Okay.
A static universe. Yeah.
A universe that is expanding, energy is not conserved. It can just sort of appear.
And general relativity is quite clear on that. General activity, Einstein's theory of space and time, one of our most beautiful and best-tested theories, is quite clear on that point.
Energy is not conserved. To ask what happened to the energy, you can ask at a local level what happened to the energy density, but at a global level, energy is simply not conserved.
Then do our future descendants have any constraints in terms of, because earlier we were mentioning, it was a catastrophe we found out about the cosmological constant because it limits our cosmic horizon and thus limits the free energy that our descendants would have access to. But if you can just make entire universes.
Yeah, this is a matter of extreme interest, I interest, I would say to us. It won't be relevant for tens of billions of years, probably, because that's the timescale on which the cosmological constant operates.
But if the cosmological constant is truly constant, and we've only known about it for 25 years, and there are, you know, astronomical observations that seem to be in tension with that. But like if it is truly constant, then there is a finite amount of free energy in our universe.
If it's not constant, if we can manipulate it, or even if it naturally decays on its own, then there is the possibility of an unbounded amount of free energy in our future and we would avoid a heat death scenario. The situation you mentioned earlier where somebody seeded our universe they've created a bunch of energy um correct it would be extremely and that's related to them having something equivalent to a positive a positive cosmological constant in there yes in any of these scenarios in which our universe is a bubble uh yeah formed in a sort of bigger, what's called a multiverse, or that's a loaded term, but a sort of larger universe in which our universe is just one bubble.
The higher, the meta universe also has a cosmological constant and it is higher than the value in our universe. That is the one sense in which there's some version of energy conservation is that you can go down from high from high to low it is considerably harder to go from low to high so the idea is that you would recursively have universes in which the bottom most one would immediately implode because of a negative cosmological constant and the biggest one is like exponentially increasing? Correct.
The rate at which the universe is exponentially increasing is set by the cosmological constant in which the volume of the universe is exponentially increasing. So you can imagine a scenario in which there was a high cosmological constant that you have a bubble universe that has a lower value of the cosmological constant it continues to expand you could make new bubble universes or you know new regions in that universe that have a lower cosmological constant either naturally and spontaneously or or due to action that we might take and as long as that cosmological constant is non-negative is zero positive, that universe will not implode.
If it goes negative, that universe will eventually implode. So you could imagine a cascade in which you go to lower and lower values of the cosmological constant.
There are a lot of engineering details to be worked out, but what I'm describing is a scenario that is not inconsistent with the known laws of physics. How likely do you think this is if the laws of physics are as we believe them to be and if we do not blow ourselves up uh in some other way this is a issue that our distant descendants will eventually have to confront no no as in like how the the whole like the there's like other bubbles not about something our descendants might do, but the fact that the Big Bang was the result of a bubble within some other metastable state.
That's a tricky question. But since you asked it, I'd say probably 50%.
There's a lot we don't understand about any of these questions. They're all like super speculative.
It's an active area of research, how to combine quantum mechanics and expanding universes. On the other hand, it seems pretty natural when you do combine quantum mechanics and gravity and try and fit them all together in a consistent picture.
If universes can expand a lot, then at all, according to the gravitational theory, then quantum mechanics will naturally populate those bits that can expand a lot. And so you'll naturally end up with an expanding universe.
So I would say probably in my heart, slightly higher than 50%, but I'm going to round it down to 50 out of epistemic humility. It's funny because this is often the way people talk about their AI timelines of like, you know, if I like i think it's like 2027 but if i'm like taking the outside of you i'm gonna say 2030 um okay and is there any way uh given our current understanding of using bubble universes to do useful work for the people outside of it so to have do some computation within it or to get some sort of actual energy out of it.
For the people outside of the bubble. Yeah.
So the thing about these bubbles is that they tend to expand at the speed of light. So even if you start off outside, you're probably going to end up inside them in short order unless you run away very quickly.
Yeah. So this isn't something that we make in the lab and then just remains in a box in the lab and then we use to do things.
This would be something that we would do or maybe would just happen to us because of spontaneous vacuum decay and it would engulf all of our future light cone. And so we wouldn't, it's not a box that you're using to do things.
It's a new place that you live. You better hope that you've engineered stuff so that that new place is still hospitable for life.
So look, if it's the case that you can set up some apparatus, not now, but not in this room, but eventually that if some individual wants to change the constants of nature, they can not only do this, but then the repercussions will extend literally
as far as light can expand.
You might have some hope
that future civilizations,
individuals or AIs
have tons of freedoms
and they can do
all kinds of cool things.
You can have your own
galactic cluster over there
and if you want to,
you know,
go do whatever you want, right?
Go live your life
and there's going to be
some libertarian utopia. But if you can literally destroy the universe, maybe it's a different story.
That is a big negative externality, destroying your future light cone. And in a world with big negative externalities, libertarian fantasies can't really happen.
It has pretty good big governance implications is that if it is possible for people just to wipe out their entire future light cone, not only themselves, but everybody else who wishes to participate in that future light cone, then we're going to need a government structure that prevents them from doing so. I mean, the worst case scenario is even worse than that.
Not just that they could do it, but that they in some sense be incentivized to do it you could imagine really adverse laws of physics in which maybe you could speculatively build some power plant that just is like really uh you know makes use of just sort of sitting on that edge of instability and and then each person individually might say oh i'm quite happy to bear one in a trillion chance that I wipe out the future light cone because I get so much benefit from this power plant.
But obviously the negative X-fidelity means that people really shouldn't do that.
So I hope the laws of physics don't turn out that way.
Otherwise, we're going to have to have some super arching control.
I've done a couple of these interviews, actually.
These end up being my favorite interviews where a normal person who's just had great school education can think like, of course I understand this, right? Or if you've just seen enough YouTube videos about like PopSci. Give you a concrete example.
When I interviewed David Reich, the geneticist of ancient DNA, I feel like we have a sense that we understand the basics of how humans came to be. What is the story of human evolution? And just like the episode revealed to me that the main questions we might have about like how humans came to be, where did it happen? When did it happen? Who did it happen with? In fact, it's like totally the last few decades of insights have totally revolutionized our understanding.
We have a sense that we understand what basically cosmology implies, but this idea that in fact there's this underlying field which not only implies very interesting things about the distant past, about the Big Bang, but also what our future descendants, what kinds of civilizations they'll be able to set up both from a governance and a practical like energy perspective it's like totally changes your understanding yeah it just keeps changing i mean not not just your idea our idea everybody's idea has changed a lot in my lifetime and may continue to change and in some sense it's because you have the lever the long lever arm of asking about the very, very distant future that makes even small uncertainties today pan out to absolutely ginormous distances in the distant future. I think you earlier said, I wouldn't be that crazy, but also it's not as easy as a Dyson spear.
Like, what are we talking about here? How much energy would it take to... The energy requirements are probably pretty pretty small much more than we can currently make in our particle colitis but much smaller just in terms of mc squared than the you know the energy in your body for example um the energy is not going to be the heartbeat the heartbeat is going to be concentrating it together in a really small little bubble that's shaped exactly right in order that it doesn't form a black hole uh expands in just the way that you want it to expand and lands in the vacuum that you're aiming for so it's more going to be a control issue than just a pure energy issue but you think this is just table stakes for distant descendants who are colonizing the stars?
It's not inconsistent with the known laws of physics, which means that it's just engineering.
I feel like the most sort of a turdy phrase that a physicist is going to show how to occur is,
your proposition is not inconsistent with the known laws of physics.
Not this.
If we lived in a world of intelligent design, and these were the laws we found ourselves with, at a high level, what is the creator trying to maximize? Like, what is the, I mean, other than maybe us existing, does there seem like something that is being optimized for? What's going on here um if you just throw a dart in laws of physics space in some sense uh you would not there are some properties of our universe that would be somewhat surprising um including the fact that our life seems to be incredibly hospitable for complexity and interesting interestingness and the possibility of intelligent life which is an interesting fact you know everything is just tuned just so that chemistry is possible and perhaps in most places you would throw the dart in possibility space chemistry would be impossible the. The universe, as we look around us, is incredibly rich.
There's structure at the scale of viruses all the way to structure at the scale of galaxies. There's interesting structure at all levels.
This is a very interesting fact. Now, some people think that actually interesting structure is a very generic property.
And if we threw a dart somewhere in possibility space, there would be interesting structure, no matter where it hit. Maybe it wouldn't look like ours, but there'd be some different structure.
But really, if you look at the laws of physics, it does seem like they're very well attuned for life. So in your scenario, where there's an intelligent creator, then they would probably be, you'd have to say they'd optimized for that.
It's also the case that you can imagine explanations for why it's so well-tuned for life that don't involve an intelligent creator. Is there any explanation other than the anthropic principle for why we find ourselves in such a universe? Well, you suggested one with an intelligent creator, but yeah, the usual one that people like to talk about is the anthropic principle.
So is it like 99% that basically the reason we find ourselves in a universe like this is the anthropic principle like what probability is pretty high well what probability do you put on like anthropic principle is a key to explaining why we find ourselves in the kind of universe we find ourselves in i think it's going to depend on what quantity you're asking me about yeah so if you ask me you know 99 of the matter in the solar system lives in the sun or on jupiter and yet we seem to live in this like really weird corner of the solar system why is that i'm pretty confident that the answer to that is anthropic that if we lived in the center of the sun would be dead and so one should expect intelligent life to like live in this weird place in parameter space yeah so that's that's perhaps my most confident answer to that question. Why do we live where we live? Then if we start talking about different constants of nature, we start getting different answers to that question.
Why is the universe tuned such that the proton is just a tiny bit more stable than the neutron? That seems like that's begging for an anthropic answer. Of course, if that's true, that demands that there be different places somewhere in the multiverse where, in fact, the neutron is slightly heavier than the protons decay to neutrons rather than vice versa, and people just don't live there.
So that, if you want to go down that road, you end up being naturally drawn to the existence of these variables scanning over space. Is there some way for the anthropological principle to exist that doesn't involve these bubble universes? Yes.
All you need is that there is different places in some larger possibility space where these quantities scan, where they take different different values bubble universe is just one way to do that we could just be different experiments uh simulations in some meta universe somewhere um what part of this is the least sort of logically inevitable right like some some theories seem to have this uh feeling of like it had to be this way and then some are just like why are there these like 16 fields and hundreds of particles and so forth what part of the the our understanding of physics yeah i would say that there's three categories there's things like quantum mechanics and general relativity that are not logically inevitable but do seem to be attractors in in some sense um then there are things like the standard model has 20 fields and it has a mass of the neutrino. Why do those masses of the neutrino have the values that they have? That seems the standard model was just fine before we discovered that the neutrinos have mass in the 1990s.
And those just seem to be just totally kind of out of nowhere. Who ordered that was a famous Nobel Prize winning physicist said about the muon, in fact, longer ago than that.
They just seem to be there, but without any particular reason. And then there are these quantities that are somewhere in the middle that are not logically necessary, but do seem to be necessary for life as we know it to exist.
How confident are we that these different properties of different universes would actually be inconsistent with intelligent life? Yeah, I think that's a great question. And this line of thought is a skeptical response to the anthropic principle.
Yeah. An example that sometimes people use is a puddle that's sitting in some depression
in the ground reflects on how wonderful the universe is, that this puddle seemed, this depression in the ground seemed to have maybe made the perfect shape for the puddle to exist. And our view would have said, no, the reason the puddle has that shape is because it is self-adapted to the hole in the ground.
So maybe no matter what the laws of physics, there would be something that emerged there and certainly if you go to you know there's all these weird bacteria at the bottom of the sea or in nuclear reactors or in various other places this kind of life will find a way philosophy seems to be adapted at least there where it's very different from the surface of the earth where we find ourselves and yet there are able to be certain life is able to live in undersea vents and is able to adapt itself to those environments. I think I basically buy that life is quite adaptable but whether life is adaptable enough that a universe with a cosmological constant that ripped it apart every microsecond, that seems implausible to me.
Or even closer to home, the center of the sun. It's not clear exactly whether we can get intelligent life living at the center of the sun.
Even though it has the same laws of physics as us, it just has different environmental variables. What is the most underappreciated discovery in cosmology in our lifetime? We have, in the 2000s and before, very carefully studied the cosmic microwave background, what's sometimes called the echo of the Big Bang and the inhomogeneities in it, the fact that it's not quite the same in every direction.
And doing that discovered a super interesting fact that was definitely not known in my lifetime anyway, which is the quantum origin of all of the structure we see in the universe. So if you look out in the universe, the density is not the same everywhere.
The density on Earth is much more than an interplanetary space, which is itself much more than an intergalactic space. And the center of the sun is all the more denser.
It is inhomogeneous. It is not the same.
And if you look back to the early universe,
it was considerably more homogeneous.
It was homogeneous to one part in 10 to the 5 or 10 to the 6.
Super almost everywhere, every point,
had almost exactly the same density.
And so then there's kind of an easy part and a hard part.
The easy part is understanding how if you have very small inhomogeneities, how they grow into large inhomogeneities. That's already quite well understood by classical physics.
Basically, the idea is this. If you have a place that's denser and a place that's less dense, then the gravitational force pulls stuff towards the high density stuff.
So if you have a small inhomogeneity, they naturally under that effect where they where they just gravitationally fall towards the denser thing that that'll if you start seeded with small inhomogeneities that will grow large inhomogeneities um and that's that's well understood the thing that we now understand much better than we did uh is where those small inhomogeneities come from like why just after just after the Big Bang, was the universe not perfectly homogeneous? Because if it was perfectly homogeneous, there's no opportunity for anything to grow. And we now understand with a high degree of confidence, something that we didn't understand, which is that those inhomogeneities were seeded by quantum fluctuations.
That when the universe, just after the Big Bang, was considerably smaller than it is today, the effects of quantum mechanics were correspondingly more important. And those quantum fluctuations produced tiny little fluctuations in the density of matter in the universe.
And all of those tiny little, you know, one part in a million fluctuations grew into all of the structures you see in the universe and all of those tiny little one part in a million fluctuations grew into all of the structures here in the universe all the galaxies you me everything else is there is it a meaningful question to ask what level of structure the each individual uh discrepancy corresponds to each individual one and ten to the five part is it is it a gal supercluster? Is it a galaxy? Is it? It depends. So there were, I mean, we believe that these were generated during the period we call inflation, very poorly understood, very early in the universe.
And there were fluctuations made not just at one scale in those days, but at all scales or many, many scales. So there were fluctuations made at a scale that nowadays corresponds to 10% of the distance across the visible universe, all the way down to structures that were in homogeneities that were at much, much smaller scale that correspond to a galaxy today, all the way down to, now this is speculation, but in some models of inflation, there were tiny in homogeneities, very small scale inhomogeneities that would give rise to primordial black holes, like tiny little black holes left over from the Big Bang.
There's no actual evidence in terms of observational evidence, no strong observational evidence for those, but those are a possibility that's allowed by our theory and people think about them and look for them. Super excited to announce our new partner, Scale AI.
Adam is, of course, a lead of BlueShift, which is cracking maths and reasoning at Google DeepMind. DeepMind, along with all the other major AI labs like Meta, Anthropic, and OpenAI, partner with Scale.
For many of them, Scale supplies high quality data to fuel post-training, including advanced reasoning capabilities. Publicly available data is running out.
To keep developing smarter and smarter models, labs will need to rely on Scales Data Foundry, which combines subject matter experts with AI models to generate fresh data and break through the data wall. Scales Research Lab, SEAL, is focused on human-centric AI alignment.
SEAL's mission is to develop practical ai safety frameworks evaluate frontier ai system safety via public leaderboards and create foundations for integrating advanced ai into society while ensuring alignment and human control so if you're an ai researcher or engineer and you want to learn more about how scales data foundry can help you go beyond the current frontier of capabilities, go to scale.com slash Thwarkesh. All right, back to Adam.
What makes general relativity so beautiful? I think general relativity is really an extraordinary story. It's pretty unusual in the history of physics that you, to first approximation, just have one guy who sits down and thinks really, really hard with lots of thought experiments about jumping up and down in elevators and beetles moving on the surface of planets and all the rest of it.
And at the end of that time, writes down a theory that completely reconceptualizes nature's most familiar force and also speaks not just to that, but speaks to the origin and fate of the universe and almost immediately achieves decisive experimental confirmation in the orbits of astronomical observations or the orbits of planets and the deflections of lights during and eclipses and stuff like that. It's a pretty beautiful theory.
And it completely changed our idea of gravity from being a force to just being an artifact of the curvature of space-time. Actually, so this is actually a good point to chat about your actual day job.
So there's these open debates about the kind of reasoning that these LLMs do. Does it correspond to quote unquote true reasoning or is it something more procedural? And it sometimes gets into a definition game.
But this is maybe a good way to test our intuitions here. The kind of thing that Einstein was doing where you start off with some thought experiments, you start off with some seeming conceptual inconsistencies in existing models, and you trace them through to some beautiful unified theory at the end, and you make incredibly productive use of these intuition intuition pumps that kind of reasoning how far are our ai's from that i have heard it said and i kind of agree with this that maybe the very last thing that these systems will be able to do these llms will be able to do is given the laws of physics as we understood them at the turn of the last century invent general relativity from that so i think that's probably the terminal step and then once once it can do that if it can do that then there won't be much else to do as far as humans are concerned it's pretty extraordinary i mean particularly coming from a physics background in which progress is pretty slow to come to the AI field and see progress being so extraordinarily rapid day by day, week by week, year by year.
Looking at it, it certainly looks like these LLMs and these AI systems in some sense are just interpolators. But the level of abstraction at which they're interpolating keeps going up and up and up.
And we keep sort of riding up that chain of abstractions. And then presumably, from a sufficiently elevated point of view, the invention of generativity from Newtonian physics is just interpolation at some sufficiently grandiose level of abstraction that perhaps tells us something about the nature of intelligence, human intelligence, as well as about these large language models.
If you ask me how many years until we can do that, that is not totally clear. But in some sense general relativity was the greatest leap that humanity ever made and once we can do that perhaps in 10 years uh then then we will have fully encompassed human intelligence will it have the same will it be of the same character as what einstein did clearly there's some there are many disanalogies between human intelligence and these large language models but i think at the right level of abstraction it may be the same do you see early examples of the kind of thing it was obviously not a little difficulty but you just start off with like hey here's here's something funny uh go think about it for a while um what like what's is there is there something especially impressive you see when you kind of run that kind of experiment at the moment these tend to be you know the systems tend to be doing uh more elementary material than that they tend to be doing undergraduate level material um yes i haven't seen anything that jumps out to me like inventing generative TV or even a toy version of that.
But there is, in some sense, creativity or interpolation required to answer any of these problems where you start with some science problem, you need to recognize that it's analogous to some other thing that you know, and then sort of combine them and then make a mathematical problem out of it and solve that problem. Do you think AI mathematicians, AI physicists will have advantages over humans just because they can, by default, think in terms of weird dimensions and manifolds in a way that doesn't natively come to humans?
Ah. You know, I think maybe we need to back up to in what sense the humans do or don't think natively in higher dimensions.
Obviously, it's not our natural space. There was a technology that was invented to think about these things, which was, you know, notation, tensor notation, various other things that allows you to much
using just even writing as Einstein did 100 years ago, allows you to sort of naturally
move between dimensions.
And then you're thinking more about manipulating these mathematical objects than you are about
thinking in higher dimensions.
I don't think there's any sense, I mean, in which large language models naturally think
in higher dimensions more than humans do. You could say, well, this large language models have billions of parameters.
That's like a billion dimensional space. But you could say the same about the human brain, that it has all of these billions of parameters and is therefore billion dimensional.
Whether that fact translates into thinking in billions of spatial dimensions, I don't really see that in the human. and I don't think that applies to an element either.
Yeah, I guess you could imagine that, you know, if you're just seeing like a million different problems that rely on doing this weird tensor math, then in the same way that maybe even a human gets trained up through that to build better intuitions, same thing would happen to the ai just sees more problems can develop better representations of these kinds of weird geometries or something i think that's certainly true that you know it is definitely seeing more examples than any of us will ever see in our life and it is perhaps going to build more sophisticated representations than we have yeah often in the history of physics, a breakthrough is just how you think about it, what representation you do. It is sometimes jokingly said that Einstein's greatest contribution to physics was a certain notation he invented called the Einstein Summation Convention, which allowed you to more easily express and think about these things in a more compact way that strips away some of the other things.
Penrose, one of his great contributions was just inventing a new notation for thinking about some of these space times and how they work that made certain other things clear. So clearly, coming up with the right representation has been an incredibly powerful tool in the history of physics and many incredibly large developments.
somewhat analogous to coming up with a new experimental technique in some of the more applied scientific domains. And yeah, one would hope that as these large language models get better, they come up with better representations, at least better representations for them that may not be the same as a good representation for us.
We'll be getting somewhere when you ask Gemini a question and it says, ah, good question. You know, in order to better think about this, let me come up with this new notation.
So we've been talking about what AI physicists could do. What could physicists with AI do? That is to say, are your physicist colleagues now starting to use LLMs? Are you yourself using LLMs to help you with your physics research? What are they especially good at? What are they especially bad at? Yeah.
So what physicists don't do is, or don't productively do, is just say, LLM, please quantize gravity for me. Go.
That doesn't get you anywhere. But physicists are starting to use them in a big way, but just not for that.
More of an assistant rather than agent. Three years ago, there was totally useless.
Like, no value whatsoever in them um like low-hanging fruit fruit uses include doing literature search so if you just say you know i have this idea what are some relevant papers they're great at that and it's semantically greater than any other kind of search the other thing that they're extremely useful for now that they were useless for is just as a tutor um if there is a huge amount of physics that a physicist would be expected to that has already been done and no human has ever read the whole literature or understands everything or maybe there isn't even something that you feel you should understand or you once understood uh that you don't understand and i think the very best thing in the world for that would be to phone up a colleague and say, if you knew exactly who to phone, they'd probably be able to answer your question the best. But it's certainly, if you just ask a large language model, you get great answers, probably better than all but the very best person you could phone.
and they know about a huge amount. They're non-judgmental.
They will not only tell you what the right answer is, but debug your understanding on the wrong answer. So I think a lot of physics professors are using them just as personal tutors.
And it fills a hole because there are personal, if you want to know how to do something basic, there is typically very well documented.
If you want to know quite advanced topics, there are not often good resources for them. And talking to these language models will often help you debug and understand your understanding.
And it'll explain to you not only why, what the right answer is, but why what you thought was wrong. and I think it'll be a pretty big deal,
sort of analogous to the way that chess players today are much better, even when they're playing across the board without the benefit of a computer, just having been able to be tutored by chess machines off the board. And this is the same.
You want to understand this thing about group theory, go and ask the machine and it'll explain it to you and it won't it won't judge you while it's doing it so there's a there's an interesting question here clearly these models know a lot and that's evidenced by the fact that even professional physicists can ask and learn about fields that they're less familiar with but this um doesn't this raise the question of we think these things are smart and getting smarter. If a human that is reasonably smart had memorized basically every single field and knew about the open problems, knew about the open problems in other fields and how they might connect to this field, knew about potential discrepancies and connections, what you might expect them to be able to do is not like Einstein-level conceptual leaps, but there are a lot of things where just like, hey, magnesium correlates with this kind of phenomenon of the brain, this kind of phenomenon correlates with headaches, therefore maybe magnesium supplements cure headaches.
These kinds of like basic connections, you would... Anyways, does this suggest that LLMs are, as far as intelligence goes, even weaker than we might expect, given the fact that, given their overwhelming advantages in terms of knowledge, they're not able to already translate that into new discoveries? Yes, they definitely have different strengths and weaknesses than humans.
And obviously, one of their strengths is that they have read way more than any human will ever read in their entire life um i think maybe again the analogy with chess programs is is a good one here they will often consider way more possible positions there's a monte carlish research than any human chess player ever would and yet they're of even at human human level strength, if you fix human level strength, they're still doing way more search. So their ability to evaluate is maybe not quite as natural as a human.
So the same, I think, would be true of physics. If you had a human who had read as much and retained as much as they had, you might expect them to be even stronger.
Do you remember what the last physics query that you asked an LLM was? The last physics query, well, a recent one was I asked it to explain to me the use of squeezed light at LIGO, which is a topic that I always felt like I should understand. And then try to explain it to somebody else and realize that I didn't understand it and went and asked the LLM,
that blew me away,
that it was able to exactly explain to me
why what I was thinking was incorrect.
So why do we use this particular form of quantum light
in interferometer used to discover gravitational waves?
The reason that's a good topic
is perhaps because it's an advanced topic. Not many people know that, but it's not a super advanced topic.
There are, out of a physics literature of millions of papers, there have got to be at least a thousand on that topic. If there was just a handful of papers on a topic, it's typically not that strong at it it do you reckon that there's a um among those thousand papers is one that explains why the um initial understanding or thought you had about it was wrong because if it just intuited that that is actually quite like that's that's pretty fucking cool i yeah i don't know uh the answer that is an interesting question i think it might be able to debug even without that.
If you do much simpler things like give these language models code, it will successfully debug your code, even though presumably no one has made that exact bug in your code before. This is at a higher level of abstraction than that, but it wouldn't surprise me if it's able to debug what you say in that way.
It does falsify a of stories about uh they're just fuzzy search or whatever scott aronson recently or it was a year or so ago he posted about the fact that the uh gpd4 got like a b or an a minus or something on his intro to quantum computing class which is definitely a higher grade than i got and so i'm already below the waterline um But yeah, you know, you teach a bunch of subjects, including GR at Stanford. I assume you've been querying these models with questions from these exams.
How has their performance changed over time? Yeah, I take an exam I gave years ago in my graduate generativity class at Stanford and give it to these models. And it's pretty extraordinary.
Three years ago, zero. A year ago, they were doing pretty well.
Maybe a weak student, but in the distribution. And now they essentially ace the test.
In fact, I'm retiring that. That's just my own little private eval.
It's not published anywhere, but I just give them this thing just to follow along how they're doing, and it's pretty strong. They may be easy by the standard of graduate courses, but a graduate course in general relativity, and they get pretty much everything right on the final exam.
That's just in the last couple of months that these have been doing that. What is required to ace a test? Obviously, they probably have read about all the general relativity textbooks, but I assume to ace a test, you need something beyond that? Is there something you'd characterize? Physics problems compared to math problems tend to have two components.
One is to sort of take this word question and like turn it using your physics knowledge into a maths question. Yeah.
And then solve the maths question. That tends to be the typical structure of these problems.
So you need to be able to do both. The bit that's maybe, you know, only LLMs can do and wouldn't be so easy for other things is step one of that is like turning into a maths problem.
I think if you ask them hard research problems, you certainly can come up with problems that they can't solve. That's for sure.
But it's pretty noticeable as we have tried to develop evaluations for these models that as recently as a couple of years ago, certainly three years ago, you just scrape from the internet any number of problems that are standard, totally standard high school math problems that they couldn't do. And now we need to hire PhDs in whatever field and, you know, they come up with one great problem a day or something, you know, the difficulty as these LLMs have got stronger stronger the difficulty of evaluating their performance has has increased how much do they generalize from these difficult problems to not only that domain of physics but just generally becoming a better reasoner overall like if you just see like a super hard gr problem are they like better coding now generally you see positive transfer between domains so if you make them better at one thing they become better at another thing uh across across all domains it is possible to make a model that is like really really really good at one very particular thing that you care about and then at some stage there is some Pareto frontier and you start degrading performance on other metrics.
But generally speaking, there's positive transfer between abilities across all domains. We've got these literally exabytes of data that we collected from satellites and telescopes and other kinds of astronomical observations.
Typically in AI, when you have lots of data and you have lots of compute something something large model great discoveries is there any hope of using these exabytes of astronomical data to do something cool yeah great question people are trying that um there's an effort you know shir Ho and Flatiron, which is basically that exact plan, is they take the pipeline of all of the data that comes out of these astronomical observatories. They plug them into a transformer and see what happens.
You can come up with all sorts of reasons in advance why that might not be something that will work. But you could also come up with reasons in advance why large language models wouldn't work, and they do.
So I'm very curious to see what happens. I mean, the dream there would be that, you know, there's lots of things hidden in the data that no human would ever be able to tease out.
And that by doing this, you could just revolutionize the of these astronomical observatories are incredibly expensive if we can just have a computer better parse all of the data from them in a way that no human ever come could that would be a tremendous improvement these things are very good at finding patterns and maybe they'll find patterns that are not particularly interesting to a human um okay so going on the g-art thread again maybe one advantage these models have is obviously you can run a lot of them in parallel and they don't get fatigued or dazed and you could imagine again naively you would imagine some sort of setup i assume you're doing many much more sophisticated things but naively you could imagine a setup where um uh look it seems like what uh uh special relativity which is something that like maybe is easy to understand, is just like you start off with, let's just like randomly select a couple of observations. Obviously, they were randomly selected, but, you know, and like, let's just think about what's going on here for a while.
You know, like, let's just do a bunch of chain of thought for a year or so. And you can just imagine doing this and doing some sort of best event across like a thousand different randomly selected parts of the current model of the universe.
And just seeing like at the end of it, which one comes up with some especially productive line of thought. Yeah, I mean, I think that could be productive.
One challenge in in that would be how do you evaluate whether you had a good theory yeah at the end um that's going to be the tricky bit for things that are most easily paralyzed are things in which if you get the right answer it's clear you got the right answer you know perhaps things in np one might say. Whereas in this case, is special relativity, how would your computer know if it generated special relativity that it was onto a winner? There are various ways in which it could know.
It could check that it was mathematically self-consistent and various other facts. But the evaluation is going to be a tricky part of this pipeline that you might wish to set up.
Is there no experimental way that you could detect time dilation or something? There is an experimental way that you could detect time dilation. Yeah.
But that would involve sending out probes or doing something in the real world. Whereas I thought you were just trying to run this in a data center.
But now today we have these exabytes of information. So you could just have some sort of, like, ability to search or query.
Like, ah, I've come up with this theory. I think maybe this is a philosophical difference, where you maybe think that the way that a theory is good is that it best matches the, you know, best predicts the data with some loss minimization.
That's not always how new theories, particularly revolutionary theories, come up. There's this famous fact, even when they were moving from a geocentric worldview to a heliocentric worldview that that it was so beautiful the theory by the time they were finished with the epicycles i mean not beautiful it was so ornate uh by the time where these planets were moving around the sun but moving on epicycles that actually the data didn't any better fit the heliocentric worldview than the geocentric worldview, especially since they didn't properly understand the ellipticity of the Earth's orbit around the sun.
So it wasn't. Why does one theory replace another? One reason is obviously that it's more consistent with the data, but that's by no means the only theory.
And if you just optimize for being consistent with the data you're going to end up with if you optimize only for being consistent with the data you're going to end up with epicycles you're not going to end up with some beautiful new conceptual thing part of the reason people like these new theories is that even though they're maybe not better at matching the data they are more beautiful and we'd have to teach and that's been a reliable guide in the history of science, and we'd have to teach these LLMs beauty. So this actually raises an interesting question, which is, look, in some sense, we have the same problem with human scientists, right? And so there's all these people who claim to have a new theory of everything.
And I guess there's not an easy verifier that everybody agrees to because some people call them cranks, other people think they're geniuses. But somehow we've solved this problem, right? Well, we've sort of solved it.
I mean, we haven't solved it in the same way that if you have some new sort algorithm that you claim is faster than everybody else's sort algorithm, there doesn't need to be any dispute about that. You can just run it and see.
Physics is not the the same way it is definitely the case that there's a number of people who think they have great theories and uh there are even perfectly respectable you know people who are professors at prestigious universities who have very different opinions about what is and isn't a worthwhile uh direction to be exploring eventually you hope that this gets grounded in experiment and various other things. But the distance between starting the research program and the community reaching consensus based on data and other considerations can be a long time.
So yeah, we definitely don't have a good verifier in physics. Even if we did someday get superhuman intelligence that could try to find all the remaining sort of like high-level conceptual breakthroughs, how much more room is there for that? Basically, was it just like 50 years of like, here's all the really advanced, great physics, and now we just bogged through like additions to the standard model? You know, if you look at Nobel Prizes year after year, they get less and less, at least in physics, they tend to get less and less significant.
And in fact, this year, the Nobel Prize in Physics was awarded to Hotfield and Hinton for their work in AI. So apparently...
A taste of things to come. I don't think there's reason.
I don't think we should be pessimistic about that. I think there could easily be room for completely new conceptualizations that change things.
I don't think it's just turning the crank going forward. I think new ways to think about things have always been extremely powerful.
Sometimes they're fundamental breakthroughs. Sometimes they are breakthroughs in which you even take regular physics this is a story to do with renormalization that maybe is a little too technical to get into but there was a sort of amazing understanding in the 1970s about the nature of theories that have been around for forever or for for years at that stage that allowed us to sort of better understand and conceptualize them um so i think there's good reason to think that there's still room for new ideas and completely new ways of understanding understanding the universe do you have some hot take about why the current physics community hasn't i mean the cosmology is maybe a very notable exception where like it does seem like the expected value of the light co-q slits switching back and forth.
Well, if you take particle physics, I think it's because we were a victim of our own success. Is that we wrote down theories in the 1970s and those theories were, it's called the standard model.
And those theories were too good in the sense that we won. In the sense that we could predict everything that would come out of a particle accelerator and every particle accelerator that's ever been built and every particle accelerator that's likely to be built given our current budgeting constraints.
So particle physics, I mean, there were some questions around the edges, but this model that we wrote down in the 70s and into the 80s basically completely cleaned up that field.
We wish to build bigger, more powerful particle accelerators to find stuff that goes beyond that. but basically we we won and uh that makes it difficult to immediately you know to to immediately
uh if you if you get too good then it's hard to know nowhere to push from there that's as far as particle physics is concerned is there some so it sounds like the problem with these colliders is that the end like the expected entropy is like not that high of like yeah we because the reason it's not that useful is because like we kind of have some sense of what we'd get on the other side is there some experimental apparatus that we should build where we in fact do have great uncertainty about what would happen and so we would learn a lot by what the result ends up being well the problem with particle colliders is in some sense that they got too expensive um and cern is is tens of billions of dollars a small number of tens of billions of dollars to to run this thing um they'll build agi with that money right yeah i mean it's super interesting how everybody talks about how academics can't possibly compete with the big labs yeah but the cost of cern is is larger than the cost of uh big model training runs so by by lot so that's just academics pooling their money. So that's an interesting fact.
But yeah, they got so expensive that it's difficult to persuade people to buy a new one for us that's even bigger. It's a very natural thing to do, to build an atom smasher that just smashes things together to higher energy.
It's a very natural thing to see what comes out. People were perhaps somewhat disappointed with the output of the LHC, where it made the Higgs, which was great, and we found it, but we also expected it to be there.
And it didn't make anything else, any of these more fanciful scenarios, or anything basically unexpected. But people had spec speculated we see supersymmetry there or we see extra dimensions.
And basically that was a null result. We didn't see anything like that.
I would say we should definitely build another one if it was cheap to do so. And we should build another one once AGI has made us all so rich that it's cheap to do so.
But it's not the obvious place to spend $50 billion if you had $50 billion to spend on science. Often it's these smaller experiments that can look for things in unexpected places.
A decade ago, there was BICEP, which is a reasonably cheap tens of millions of dollars experiment at the South Pole that thought it had seen some hints in the cosmic microwave background of gravitational waves. That would have been revolutionary, if true.
Not worth doing BICEP if it costs $10 billion. Definitely worth doing BICEP if it costs $10 million.
So there's all sorts of experiments like that, often observational. What is the value of seeing these primordial gravitational waves? Oh, it gives you hints.
You're just examining the night sky very closely and seeing hints of what happened at the Big Bang. Right.
So yeah, this is a sort of different approach to doing high energy physics, which is, why do you want to build a big collider? You want to build a big collider because the bigger the collider, the more high energy you can smash this together with.
And Heisenberg's uncertainty principle says that high energy means short resolution. You can see things on very small scales.
That's great, except the cost to build them is there's some scaling laws and those scaling laws are not particularly friendly. there is another sort of approach that one might say, which is, you know, there was a ginormous explosion that happened, which was the Big Bang.
You know, if you imagine, if we look at out in the universe, it's expanding. If you sort of play the tape backwards, it's contracting.
Eventually it all contracts at 13.8 billion years ago in the Big Bang. And so that's a very big particle collider indeed.
And so by just examining very closely the Big Bang and its aftermath, we're able to hopefully probe some of these quantities that are very difficult to probe with particle colliders. The disadvantage is that you can't keep running it and adjust the parameters as you see fit.
It's just like one thing that happened once, and now we're having to peer backwards with our telescopes to see what happened. But it can give us hints about things that would be inaccessible with any future glider.
Is there any information about the distant past that is in principle principle and accessible? Probably not in principle. So something happened to the universe in its evolution, which is that the very early universe, just after the Big Bang, was opaque to light.
We can only see light past about 300,000 years after the futureter bit of Big Bang. Before that, everything's so dense, it's like just a dense plasma that light just gets absorbed by.
It's like trying to look through the sun. And so we cannot see directly anything from before 300,000 years.
Nevertheless, we can infer lots of stuff that happened from before 300,000 years. In fact, looking at that light, what's called the cosmic microwave background that was emitted at that time, we infer lots of stuff about just due to the patterns of anisotropies that we see in the sky, we can infer a great deal about what was happening earlier.
And most of our confidence about modern cosmology comes from a number of experiments that starting in the 80s but accelerating in the 2000s really very carefully measured that anisotropy and allowed us to infer stuff before that. At the information theoretic level, there's nothing inaccessible.
I guess that makes sense. The conservation of information.
Maybe you'll tell me that that also isn't true. Well, that's a great question.
I mean, there's been a lot of debate in the black hole context about whether information is conserved by black holes, but the modern consensus is that it is. Look, if you're enjoying this conversation, you should consider working for my sponsor, Jane Street.
They're a very successful quantitative trading firm. Physicists do particularly well in trading because they can combine hard applied mathematics with a bunch of empirical and theoretical considerations.
In fact, Adam once filed for a patent using quantum entanglement and violation of Bell's inequality to do relativistic arbitrage. I don't understand what that means.
Maybe I should have asked Adam, but if you do, you should go work for Jane Street. Jane Street is keen to hire smart, curious, and rigorous people who want to work on interesting technical problems.
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And there's also a really interesting video there about their ML work that you should check out. All right, back to Adam.
All right, Adam, what are your tips for hitchhiking? Oh, good question. So I hitchiked uh a bunch around around america and europe i've done you know oxy to morocco uh when i moved from princeton out of sanford i hitchhiked a bunch of other times down to new orleans various other places um i think the probably the biggest tip for hitchhiking is to stand in a good place some counterparty modeling modeling, imagine the person who's picking you up, they need time to see you, to evaluate you, and to decide they're going to pick you up, and then to safely stop, and that all needs to happen.
So stand somewhere where people can see you, possibly at a stoplight, and where there's a place for them to safely pull over. How do you model the motivations of people who pick you up?
What are they getting out of this?
I think it's different for different people.
I think about 20% of people
will just always pick up hitchhikers
no matter what.
Even if I was dressed very differently
and presented very different,
I think some people would just
pick people up no matter what.
I basically fall into that category now.
I'll just hard-coded into my brain that I will 100% pick up hitchhikers always under all circumstances, just because enough people have generously picked me up down the years that I just feel as though it's my duty and sort of not subject to a cost-benefit analysis. Just it's in there.
Many other people are evaluating you and just, you know, trying to decide what what you're in for some people are lonely and want somebody to talk to some people have a just a spirit of adventure and find it exciting to pick pick people up certainly it's not a representative cross section of people i would say there's definitely a selection bias and who picks you up they tend to be more open and more risk tolerant and what was your motivation for did you were you just in need of a car or what was going on no i um enjoy meeting people and it's i enjoy the experience of meeting people and weird episodic uh sense of which just you never know what's going to happen i think i have a a very tolerance for ambiguity and I enjoy that. What was the percentage of we just had a normal conversation, they went in the general direction I was going and that was that versus I've got a crazy story to tell about X incident.
What percentage is each? I think some people are just totally normal people, families moving their child to college, and you get there and you help them move some stuff into the dorm room just to thank you, all the way through to absolutely wild cases. Probably 20%, just like this is one of the craziest things that ever happened in one way or another.
Yeah, any particular examples of the wild things? Oh, yeah. Huge.
I mean, it's just absolutely fire hose of wild things happening. I could tell so many stories.
Like, I remember once there was a trucker who picked me up in the desert outside Salt Lake City and who drove me to Battle Station, Nevada, and who, as we were talking, the truckers are always, in fact, the most interesting of all. It's typically illegal or in any way in violation of their employment contract for them to pick people up.
So those guys are really, and it's always guys, are really pushing the envelope in terms of picking you up. The truckers often will say, you're the first person I've had in my cab in 20 years of trucking or something.
And then they tell you about 20 years worth of things that have been on their mind. So I'd say that those are often the really interesting ones.
as I said there was this one in Utah who was just just talked from the moment I got into the cab
um until Those are often the really interesting ones. As I said, there was this one in Utah who was just talked from the moment I got into the cab until we got to Nevada.
And I kind of got the feeling that he had sort of excess mental capacity and that this was his, you know, he was now just going to dump it on me. And he was telling me all about his life.
And I remember this very well, how his brother-in-law thought he was a loser, his sister's husband. But like now we had the hot fiancé, so who was the loser.
And then just sort of gradually over the course of the six hours, it just suddenly occurred to me that his fiancé was doing advanced fee fraud on him. And the whole thing was some ginormous – and he was being scammed by his fiance.
And very unfortunately for them, they tried to execute the scam while he had me in the cab and he never had anyone in his cab. So now he had me in his cab and they were trying to do some fraud on him.
And I was able to, they had some wheat factory in Wales, United Kingdom, that they had some British high court
document saying that he was entitled to if he paid off the lien on it. There was some long, complicated story that was totally flagrantly false.
And I kind of felt like I had a moral obligation to him to break the news to him. On the other hand, we were in the middle of nowhere in Nevada, and it was clearly a very important part of his personality that this was so.
So I kind of waited until we got close and said, is it possible that your fiance is being scammed by these people? And, you know, sort of raised the notion of scamming. And he was willing to intellectually entertain the possibility.
And then we got a bit closer. Is it possible that that you were yourself being scammed by your fiancé? And then he was like, no, no, no, it can't be.
And he had all these documents to show that it was all legit. And they were just sort of, to somebody from a British legal background, sort of transparent forgeries.
And he did eventually accept it and was just crying on my shoulder in some truck stop. It was quite, you know, a high pathos moment.
And then said, this happened before, and it turned out he'd previously been scammed in the same way, or a similar way, through somebody he'd met through the same Match.com profile. That was his lucky profile, because, you know, people kept messaging him through it.
So um so we you know we talked through that and worked through that and like i felt in some ways i'd been his his guardian angel and uh but he'll you know he'd also be my guardian angel and picked me up in the middle of the desert so there was some there was some great exchange there that's that's crazy um i i hope you closed down that profile i hope so i mean we you know i did chat to him about that that possibility and he wasn't fully bought in on it but uh yeah well uh what's the uh what's the longest you've been stranded somewhere oh uh that would probably be one time in richmond virginia uh in some not particularly good neighborhood trying to hitch out of there um i think that was about a day, which is really bad. That's really bad.
Like sometimes if you get a good spot, that's worth a thousand miles. Just don't give it up just for a short hop anywhere.
If you get a bad spot, get out of there on any means necessary because there's probably a thousand X variants in how high quality hitchhiking spots are, I would say. How did you find the time to get stranded for a day at an end? In terms of intensity, it doesn't really take that much wall clock time, as we say.
Coast to coast is like a week or so. It's pretty fast because you're not yourself driving.
In that sense, it's easier. You do have to wait.
And there is definitely high variance how long you can be. But in terms of sort of instance per minute, it's a pretty good way to see the world.
And you see such a cross-section of people who I might never otherwise meet. And such a sort of high-variance cross-section.
Everything from sort of idle millionaires cruising around the country looking for adventure to people who just got out of prison to uh in one memorable incident well it eventually transpired as we were going along that they were uh they had they were actually just teenagers and i didn't somehow didn't clock that when getting in the car and they they had stolen the family car and were were driving west without a plan. And yeah, there I gave him a talk of talking to.
And... They had stolen the family car and were driving west without a plan.
And there I gave them a talk, talking to, and bought them dinner and some life advice. So that was some stuff I got.
Did you make them call their parents? I did make them call their parents, yes. Heavily encouraged them to call their parents.
Is there a log to get a professor? Yeah. None of these people typically realize that, you know, your academic background never really comes up in conversation typically.
I mean, sometimes it does, but typically that's not the nature of the conversations. Was there any time you felt particularly unsafe? I have definitely felt more unsafe picking up hitchhikers than I have hitchhiking maybe i just got lucky but picking up hitchhikers there it tends to be um you know no one really picked picks up hitchhikers uh anymore and there's definitely a selection effect on who's hitchhiking right um i have definitely felt more in risk of my life with hitchhikers i picked up than i ever did hitchhiking.
But, you know, it's possible I just got lucky. You don't see the other branches of the way function.
What are the other interesting insights from just getting this random cross-section? Yeah, all sorts of facts. A lot of people just like to talk.
There's a lot of people out there, and I like to talk too. So it's mutually beneficial.
Well, the truckers, I imagine, are especially key. Yeah, those guys, they those those guys interesting um yeah they're all they're all cheating their logs they have certain logs about how long they can travel for at least every single one who's ever picked me up maybe maybe it's correlated with their willingness to pick up hitchhikers has all been in some way or another gaming the system of of their their logs about how long they're allowed to drive for and and playing games with time zones and stuff like that.
And they typically, yeah, they're smart people and they just have a lot to say and don't really have anybody to say it to. So they're very grateful.
What are they especially insightful about? They tend to have listened to a huge number of audiobooks. They have an enormous amount of information stored in their brain but nobody to tell it to um also many of them tend to have had unlucky romances at some stage in their past that they've never really got over or spoken to and i really feel as though many of them would do well to speak to a therapist but you are the therapist in that case so you know in many ways people will tell you things that frequently people will say things like i've never told anybody else this in my life before that's common not just the truckers other people as well i mean sometimes it's you know families picking you up and so they're not going to say that but often it's just um often it's just you know single people picking you up and they'll they'll say i've never said this before to anyone else in my life and you know they'll tell you some story of their life and i do think it's obviously i'm very grateful to them for driving me down the road but i think also it's an exchange and they're also getting quite lot out of the conversation um i remember one case going to new orleans somebody just meant to only only take us you know my i think it was just there's some state trooper come along in in south carolina and was going to arrest us because it's illegal in some states to uh hitchhike and north carolina and so i was like i could just take the next ride and it was just 10 miles down the road and he ended up getting sort of so into it that we ended up driving you know maybe a thousand miles out of his way by the time we'd gone and he'd had this uh you know we having great conversations just absolutely sort of wonderful time and he just wanted to keep going and going and drive us uh through the night and then we ended up going through the deep south in the middle of the night and arriving near New Orleans around dawn.
And he'd had a father who had been in the military, but he'd kind of had a difficult relationship with and ended up going and visiting his father's grave in Baton Rouge, never having done that in the 20 years since his father died. But just as this sort of turned, I mean, he just was driving along, expecting to go home, and then it just turned into this sort of spiritual quest for him.
So, you know, stuff like that can be pretty gratifying. It's also sort of cheating.
You're not, in my way of thinking about it, meant to be taking people out of their way. Like, they're meant to be going where they're going, and you go with them, and they take you no further.
But in this case, I think he needed to go there. So that was good for him.
Did you stay in contact with any of the people you were checked with? Typically, no. And I would almost consider it poor form to do so.
But actually, there was one lady who came to stay in New York later. And she was going down to Haiti to sort of be a doctor there.
She was a doctor, and so I stayed in contact with her a bit. But typically, it's just the nature of the interaction is that you have this sort of beautiful moment in time together, and then that's it.
Yeah. Any other tips that somebody should know? I mean, should they do this anymore given that it's largely uncommon and so uncommon types of people might pick you up? I think it used to be very common in the United States.
It's still reasonably common in Europe. It used to be very common in the United States and then there were some mass murderers who drove the popularity down by targeting hitchhikers.
Maybe this is just pure cope. In my mind, you need to worry about that less because if you are a mass murderer, it's really a serial killer.
It's not really a high expected value strategy to cruise around looking for hitchhikers since there's so few of them. But that just might be pure cope in my head.
I've never refused a ride for safety grounds, but I would.
I hope I would if if necessary sometimes you would refuse a ride because somebody's only going a short distance and you're at a good hitchhiking spot it's kind of bad karma to refuse a ride but sometimes sometimes you should do that other tips don't um don't write your exact destination on your sign. Write the sort of direction in which you're going.
The reason is maybe twofold. One, a lot of people, if they're heading towards that place but not going to that place, will not stop because they think, oh, I'm not going to wherever it is.
I better not, you know, I'm not going there, so I won't pick you up, even though you'd very much appreciate a partial ride there. The other reason is if you do want to decline a ride, it's certainly a lot easier to do so if the person says, oh, I'm going to that city.
That's hard. If they say they're going to that city and you've written something more vague on your sign, then it's maybe easier to decline a ride.
If you want to get out of the car, the classic, and there is to say that you, you know, you get in and you feel unsafe, is to say that you're car sick. Because, you know, even serial killers don't want vomit in their car.
So that's a good reason to get out. And then you just say, okay, I'll just stay here.
That's another trick. trick i've never had to deploy that oh i was just about as you know i never had to deploy that typically it's pretty like there's a moment of like anxiety in the first minute um but then after a minute it's clear that everybody is and they're also i mean they're also anxious about you and you know many ways you can tell that they're quite nervous about you um uh and then after a minute it's clear that everybody is uh if not a sensible human being then at least a safe human being and uh everything's super relaxed for the rest of the ride typically any other strange people who picked you up that come to mind oh that's really strange but just like uh memorable so many different kinds of people um yeah i remember um there was one like seemingly very successful cowboy but you know a cowboy some driving some fancy truck in wyoming and had a big herd of cattle and all the rest of it and was just asking me actually somewhat unusually sort of asking me what i do and so you know that time i was doing cosmology so I sort of trying to explain to him and just had no totally disconnecting with anything just didn't understand a word I was saying all the way through and eventually we landed on the fact that the stars in the sky are just like the sun only much further away and this was a fact that in his life up to that stage he just never encountered and it that was extremely gratifying because he um he was blown away by that fact like he wasn't he was totally intellectually capable understanding it he just never in his 50 years of existence up to that moment ever um ever heard that fact and his mind was just totally racing uh this this was reorienting his picture of his place in the universe.
It must be so big. There's stars out there.
And he phoned his wife, who I think was somewhat less excited, and then took me to a gun store and brought me lunch. And, you know, it was a good time.
He was a rancher. He was seemingly a very successful rancher based on everything about him.
But he had some prize high quality bulls that were uh that were some rare kind of uh high quality bulls i can't exactly remember the details but yeah he just never really contemplated what the night sky meant for him there's uh there's a sherlock holmes story where uh holmes runs that learns that actually the sun is the center of the solar system oh interesting and interesting. And then the logic is Watson tells him this and Holmes is like, fuck, why did you tell me this? I try to like reserve mental space for things that are actually relevant to my work.
Now I got to like forget this. Yeah, the hitchhiker's going to the galaxy.
Yeah. What did you learn from studying the firsthand accounts of the accounts of the nagasaki bombers oh yeah that was okay so during the pandemic um my my landlord has a big library and i just started reading uh you know during deep lockdown some books in the library and i was just some so where do you stay that you're a landlord oh i um you've got an apartment complex library i live in a house that was uh used to belong to the chair of the english department to some stanford and then it's hered by grandson who rents it to me and it was um he has a very extensive library it's very interesting and i was like you know going through it during during first lockdown and came across this like super enigmatic statement in some book about the history of Japan and was like super fascinated by it and started for reasons that I'll explain in a moment then just became obsessed for a few months on reading absolutely everything I could about the bombing of Nagasaki which is the most recent nuclear weapon ever to be set off during wartime.
And was reasonably controversial because people question whether we should have done it or not. And that wasn't the question I was looking at, the question I was looking at wasn't should they have ordered it to be done, but were the people who did it even following orders? And it's a pretty wild story that I didn't know, certainly before any of this happened, which is it was never meant to be a mission to Nagasaki.
It was meant to be a mission to bomb Kokura, a different Japanese city, but they got there and it was clouded over and they had like very strict instructions do not bomb if unless you can see the target uh and that was that was the order do not bomb unless you can see the target and they got to this other city and they passed over a bunch of times and they couldn't see the target it was covered in clouds so then they went to their secondary target nagasaki and it was again covered in clouds and they did a whole bunch of passes um and they'd made various mess ups the bomber crew had beforehand including getting lost and they'd made a number of mistakes uh personal flying mistakes on their part that meant that they didn't have enough fuel once they got to nagasaki to carry the bomb uh back back to base. And they probably have ended up in the ocean had they tried.
So they were extremely motivated. At the time, this was the only nuclear weapon that existed in the world.
We'd had two, and then it went down to one, and now there was one, and they were just about to drop it in the ocean and lose it. So according to the official account, after having done all this, on the third and final pass over Nagasaki, there was a miraculous hole in the cloud that suddenly opened up, and then they dropped it.
And that story is a bit sus. If for no other reason than that they actually missed, little known fact, they missed Nagasaki.
They were aiming for one point and they hit another point that was on the other side of the hill, such that the original thing they were aiming for was reasonably untouched by comparison for the fact that a nuclear weapon had been dropped. They missed by much more than you would miss if you were doing visual bombing and they would have been told to do visual bombing.
So this kind of suspicion is that they were doing a little bit of radar bombing against direct orders. So is it possible that 50% of all of the nuclear weapons ever dropped in combat were in fact dropped against direct orders? Which is, you know, if true, that's a pretty uh fact about nuclear war since people are somewhat worried with nuclear war that someone will launch nuclear weapons uh without being ordered to do so and it does kind of look like 50 percent of all the nuclear weapons ever dropped in combat were dropped against direct orders and when they got back um curtis lemay was going to feel was going to court-martial them uh and was like super mad but then the war ended and they didn't want to do it for pr reasons so i just ordered and found every account ever written by every person super fascinating to do that because uh all these different people had completely non-overappling lives.
You know, some of them were, you know, were on the Manhattan Project and were there observers and waited later win Nobel Prizes for physics. And some of them were just people who were just, you know, there for one moment.
So, no, like Louis Alvarez. Physicists themselves were on the plane? There was, yeah, in every, there was typically a physicist, a representative of the Manhattan Project on the plane, just in case.
So Louis Alvarez was someone there. He actually wasn't on the Nagasaki mission.
He was on the Hiroshima mission. But in his biography, he's like, they said they saw a hole in the clouds.
I don't think I believe them. So, like, I think, one of the hints.
It was maybe reading his, at some stage, reading his autobiography that was one of the big hints. The other people insist there was.
But what's super clear is that whether or not there was a hole in the clouds, and probably there was a hole in the clouds just because of some of the technical things to do with their discussion, though it's's definitely not obvious what's clear is that whether or not there was a hole in the clouds they certainly you know had decided in the cockpit on that final run that no matter what they were going to drop it so even if there wasn't a hole in the cloud was a hole in the clouds wasn't a hole in the clouds they had decided to drop the nuclear weapons against direct orders and as they had written like basically like oh we totally saw a hole in the clouds but even if we hadn't we would have dropped it that basically is yeah so different people write different things how do you were on the plane there's about 10 people on these planes did any of them say not all of them were um you know some of them are some ways away from where the action is happening there's the bombardier who says that uh that he saw a hole in the clouds there's the pilot who says something but everyone has their own different perspective and some of the perspectives are just totally this is something that i guess i'd always been told by my history teachers but never really appreciated until i'd done this 360 view of history that people can describe the same events and just they have flatly inconsistent uh memories of each other nobody who was on the plane said that they faked the hole in the story. But some people who were on the plane said they were determined to drop the bomb no matter what.
And they were highly incentivized to do this because if they had not done it, they'd have probably, as it was, they only barely made it back to their emergency landing spot in Okinawa. They would have definitely ended up in the drink and certainly the bomb would have ended up in the drink had they not done it.
So I don't know. I mean, I'm not a professional historian, and maybe there'll be difference of opinions, but it's clear there was something highly sus about at least 50% of all the nuclear weapons dropped in combat.
I mean, the interesting thing is that the reason nuclear war was averted in other cases is also because they refused to follow direct orders, right? So in this case, or in the case of Petrov, he didn't report the seeming sighting of nukes from America, and that obviously contradicts orders. Yeah, there's nuclear insubordination in both directions.
That's right. There's like the good kind, where they sort of maybe should drop the bomb according to their orders and refuse to.
And then there's the other kind. Yeah.
I also want to ask, so you've had not only one remarkable career, but two remarkable careers. So in physics, you're a close collaborator with people like Leonard Susskind, and you've done all this interesting research.
Now you're helping do the reasoning work that Google DeepMind's working on in AI. Is there some chronology you have in your head about how your career has transpired? Oh, I don't impose narratives on it like that.
It's certainly a big, very big contrast between doing physics and writing retail papers, as it were. Retail? You know, doing one by one, writing physics papers, and then doing AI, which moves just tremendously faster, and doing, you know, trying to contribute to the wholesale production of knowledge in that way.
Yeah, and they have very different impacts in terms of counterfactual impact. Physics, like you write some papers and you're like, had I not written that paper? No one written that paper for years or ever, perhaps.
Computer science doesn't feel like that. It feels like if you didn't do it, someone else would do it pretty soon thereafter.
On the other hand, the impact, even a few days of impact in computer science, these things are going to change the world, hopefully for the better, to such a large degree that that's much bigger than potentially all the physics papers you ever wrote. That's interesting you say that about you feel that uh physics is physicists are not fungible in the same way the story about why physics has slowed down is usually that in fact there isn't any low-hanging fruit and the idea that you would discover something that somebody wouldn't have written about for many years to come um i had a couple of double negatives there but basically like you're not gonna um you know we've like found all the things that are you can just like write a paper about and you're not just gonna like think about something and find something that somebody else wouldn't have written about otherwise um but here you're saying the the field that's moving way faster which is computer science that's the one where like all these people are gonna you know, come up with your algorithms if you hadn't come up with them yourself.
And it's physics where if you had more Leonard Susskinds and Adam Browns, you would have a much faster progress potentially. Well, partly there's just so many more people working on the problems in computer science than there are in physics.
There's just the number of people is part of what makes the counterfactualfactual impact i mean like how many theoretical physicists are there versus how many people are working on like uh ai research ai research around the world there's you know i don't know how many people are in the matter thousands and thousands and thousands but in physics it's 100 200 300 really well in the narrow domain of you know high energy physics. I mean, there's many more physicists than that if you include people more generally, but they're sufficiently specialized.
I mean, that's partly part of the reason is that it's much more specialized field. So in a very specialized field, the number of people who would actually write that paper is a much smaller number.
How much do you ascribe the slowness of physics to these kinds of things that are just intrinsic to any field that is as specialized and as mature versus to uh uh any any particular dysfunctions of physics as a field yeah we look back on the golden era of physics you know in uh you know from the 1900 through 1970s or something you know as a as a when things happened. I do think there is a low-hanging fruit aspect to it.
I mean, we already talked about how the standard model is so successful in terms of particle colliders that it's just hard to make rapid progress thereafter. So I don't really see it as a dysfunction of the field so much as being a victim of our own success.
Uh, having said that, does physics have fads? Does physics have fashions? Does physics have any of these other things? Uh, absolutely it does. But quite how much counterfactual progress we'd make if that weren't true, I don't know.
How well calibrated are the best physicists? It doesn't necessarily pay to be well calibrated. Uh, and that incentive structure is perhaps structure is perhaps reflected in the poor calibration of many of the best physicists.
First of all, because physics is a sufficiently mature field, all the good ideas that look like good ideas have already been had, or many of them. Where we're at now is the good ideas that look like bad ideas uh so in order to motivate yourself to you know get over the hump uh of uh get through the get over the barrier and actually explore them you need a little bit of irrational optimism uh to sort of ride out uh the uh the initial discouraging things that you'll discover as you go along.
So I would say that typically theoretical physicists are not particularly well calibrated and tend to be in love with all their own theories and make highly confident predictions about their own theories. Before the LHC turned on, there were certainly a lot of high-energy theorists making extremely confident predictions about what we'd see at the LHC.
And it was typically their own favorite particle that we'd see. And while I'd love to have found supersymmetry, it would in some sense felt somewhat unjust to reward the hubris of people making overconfident and poorly calibrated predictions.
So yeah, that's definitely a thing that happens. But I wonder if poor calibration on the individual level is somehow optimal on the collective level.
Yeah, I think that's basically right. I mean, the same is kind of true in other domains of life as well, of course.
You know, startups, if you were properly calibrated about how likely your startup to succeed would be, maybe you wouldn't do it. But it's good for the ecosystem that certain people are willing to give it a go.
yeah I think it's good for the ecosystem and perhaps bad for the individual to be well calibrated. Yeah.
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Another topic I know you study a lot is how one might mine a black hole. Oh yeah, right.
I read a paper about that. Very good.
Tell me about it. Okay, so what do we mean by mine black hole? Mine black hole means take the energy out of a black hole that used to be in a black hole obviously if our distant descendants have used up all of the energy and stars and everything else uh the black hole might be the last thing they turn their eye to um yeah so can you get energy out of black holes at all uh the old story pre-1970s is no like it's just a black hole is one way.
Matter falls in, it never comes out, it's stuck. The thing that Hawking and Bekenstein discovered in the 70s is that once quantum mechanics is involved, that's not true anymore.
Once quantum mechanics is involved, in fact, energy, even without you doing anything, starts to leave black holes. The problem, as far as our distant descendants will be concerned, is that it leaves black holes extremely slowly.
So if you took a solar mass black hole, same mass as the sun, just collapsed to form a black hole, there'll be this little quantum, what's called a Hawking radiation nowadays, little quantum Hawking radiation in which the energy will leach out again very, very slowly. And the temperature of a solar mass black hole is measured in nanokelvins, so very low temperature.
So the energy leaches out when something like cold, you know, so cold you couldn't even see it in the cosmic microwave background. It leaches out incredibly slowly back into the universe.
And that's bad news because it means the energy comes out super duper slowly. So the mining question is, can you speed that up?
Solar mass black hole, if you don't help it,
will take about 10 to the 55 times the current age
of the universe to have given out all its energy
back into the universe.
Can you make that faster?
And there were these proposals stretching back
a few decades that you could.
You could do what's called mining black holes,
where we see the Hawking radiation that escapes when we're a very long way away from the black hole but actually mathematically it's known that much of the hawking radiation doesn't escape it just sort of makes it a little bit out of the black hole and then falls back in again and there was this proposal that you could kind of reach in with a mechanical claw obviously not crossing the horizon because otherwise you've lost the claw and you're somewhat counterproductive but like just just outside the horizon just grab some of that hawking radiation and just drag it a long way away from the black hole and then and then feast on it or do whatever it is you want to do with it and in that way you could what's called mine a black hole you could speed up the evaporation of a black hole by a huge factor so in fact that the lifetime would no longer go like the mass cubed, like it does with just unaided Hawking radiation, but would scale like just the mass, so considerably faster for a large black hole. And so this was these proposals.
And what I had a somewhat sort of pessimistic contribution to the story, which is that the existing proposals did not work. They didn't work to speed it up.
And in fact, you can't speed it up. You can't get down that m cubed down to m.
You can't, in fact, get anything less than m cubed. It still scales like the mass cubed.
The length of time you need to wait to get all the energy out of a black hole still scales like the mass cubed. And what goes wrong is ultimately a material science problem.
So this scoop that comes down really close to the horizon. Now, from one point of view, that's just like a space elevator, albeit a very high-performance space elevator.
Space elevators, you'll remember, are these ideas for how we might get things off the surface of the Earth without using rockets. And the idea is that you have some massive orbiting object, sort of very long way away beyond geostationary orbit, and then you dangle off that rope down to the surface of the Earth, and then you can essentially just climb up the rope to get out.
That's the space elevator idea. And already around Earth, it's hitting pretty hard material science constraints.
So if you want to make a space elevator, the trouble with making a space elevator isn't so much supporting the payload that you're trying to have climb up. It is merely just the rope supporting its own weight.
Because each bit of the rope needs to support not only its own weight, but also the weight of all of the rope beneath it. So the tension that you require keeps getting more and more and more as you go up.
At the bottom, there is no tension effect it doesn't even touch the earth it's not like a compression structure that's like a skyscraper that's pushed up from below it's a tension structure that's held up from above but as you go up because the tent you need more and more tension you also need to make the rope thicker and thicker and thicker and if you try and on earth or around earth build a space elevator out of steel say it just doesn't Steel is not strong enough. You need to keep doubling the thickness until by the time you get to geostationary orbit, the thickness of the steel rope is more than the size of the Earth.
Like the whole thing just doesn't work at all. But carbon nanotubes are this material that we discovered that are much stronger than steel.
So in fact, around Earth, carbon nanototubes will just about work if we can make them long enough and pure enough and then they will be strong enough that we will be able to build a space elevator around earth in you know maybe sometime in the next next century that you only need a couple of doublings of the thickness of the carbon nanotubes along its entire length. So carbon nanotubes work great around Earth, but they are totally inadequate for black holes.
For black holes, the critical material science property you need for this rope is the tensile strength to mass per unit length ratio. It needs to be strong, high tensile strength, but low weight, like light, low mass per unit length.
And that's the critical ratio. And carbon nanotubes is 10 to the minus 12 or something on that scale.
And that is simply not strong enough at all. In fact, what I showed in my paper is that you need a tensile strength to weight ratio that is as strong as is consistent with the laws of nature.
So in fact, the laws of nature bound this quantity. The finiteness of the speed of light means you cannot have an arbitrarily strong rope with a given mass per unit length.
There is a bound set by the C squared in some units that bounds the maximum possible tensile strength that any rope can have. Any rope, in fact, that has that, an example of a rope that has that is a string.
So a string is, I mean, a fundamental string from string theory is an example of a hypothetical rope that is just strong enough to saturate that bound, that strength bound. And then the problem is the
following. The problem is that if you have a rope that saturates the bound, as strong as any rope
can be, it is just strong enough to support all of its own weight exactly on the edge there,
with exactly no strength left over to support any payload it might wish to carry. And that's ultimately what dooms these mining black holes, you know, these rapid mining black hole proposals.
And what happens if you try to make the rope stronger? Well, you can't. One example of a thing that goes wrong is the speed of sound in a rope goes up with the tension and down with the mass point at length.
and if you try and use a rope that's stronger than this or some hypothetical rope you would find that the speed of sound is greater than the speed of light and that's a pretty good indication what is the speed of sound so if you just take a rope you know stretch between you and me and ping it there will be uh little right vibrations that that head over towards you and those vibrations are subluminal if's just a normal rope, are move at the speed of light for a string or something that saturates the nullity condition and would be faster than the speed of light. That would be an example of why you know there's something wrong with that proposal.
So it just happens to be the case that the rope cannot mine black holes um i think we've mentioned a couple other bounds like this where there's no uh in principle reason you might have anticipated x ante why there would be such a bound that prevents something that just kind of gets in our way um but it just so happens to be this way um is it does this suggest that there's some sort of like deeper conservation principle we'd be violating and then like the universe conspires to create these engineering difficulties which uh limit that yes nothing is ever a coincidence so usually um you know from the perspective of the story i just told to do with mining black holes it's not clear what exactly will be broken about the universe if you could mine black holes somewhat faster than we can. There are other symmetry.
There are other ways of thinking about it in which if you could make a string that was strong enough to actually do it, if you could make a rope that was stronger than this bound, that various things would go wrong there are various symmetry arguments that that can't happen um but yeah usually uh often it turns out if we have these bounds that there's something that that sort of saturates the bound or gets very close to the bound and that's a sign that you're that you're on the right lines with some of these bounds on the right lines in what sense as in uh if you have a bound but you can't can't think how to get close to the bound that's usually an indication that you need to think closer because often these bounds are uh often these bounds if you're clever enough there's a way to get to the bound there's no rule that has to be so but that's that's often that's often the case that someone will come up with a bound, someone will come up with, and there'll be a gap between the bound and how close we can get. And usually more ingenuity will take you up to the bound.
I guess the thing I'm curious about is why it would be the case that such a bound would exist in the first place? And how often do you run into these things where, basically, are you expecting to discover something in the future about like why it had to be this way that you can't mine black holes? Like something would be violated about, like that tells us something important about black holes that they can't be mined. And it's deeper than the tensile strength of the string that would be required to mine it.
Yeah, good question. I started these investigations because it offended my intuition
for various information theoretic reasons.
The idea that black holes could be mined,
you know, with parametric speeds ups.
When I thought harder about it,
the reasons why I thought that couldn't happen
didn't really make sense.
So in this particular case,
maybe someone will come up with a reason.
I don't actually have a particularly strong reason
why they can't be mined anymore,
except that they can't.
Okay, so we can't get the material out of the black hole
at a pace that would make it reasonably useful to us.
What can we do with black holes?
What are they good for?
If you have a small black hole,
you can get stuff out of them more rapidly. The temperature of a black hole is in person proportionate of size.
So one thing that people have talked about with black holes is using them to extract all of the energy from matter. So as you know, most chemical reactions are pretty inefficient.
You burn gasoline and you extract, as a function of the rest mass of the gasoline that you started with, you extract one part in 10 billion of energy from the gasoline that you started with. So that's bad from the point of view, you know, you have MC squared worth in a gallon gallon of gasoline, you've got a full mc squared worth of energy in there, and you can only get out one part in 10 to the 10.
That's a pretty unsatisfactory situation. Roughly speaking, the reason that all chemical processes are so inefficient is that they only address the electromagnetic energy in the electrons, and a very small fraction of the electromagnetic energy in atoms is stored in the electromagnetic interaction between the electrons and between the nucleus and the electrons.
Most of it is stored in the nucleus itself, in the strong nuclear forces, and particularly in the rest mass of the protons and neutrons that constitute it. So you can do much better if instead of doing electromagnetic interactions, you use nuclear interactions that can probe the energy in turning protons into neutrons.
That's why nuclear power plants are so much more efficient on a per-mass basis than chemical power plants like coal plants or gas plants, because you're getting a much higher fraction
you know best case scenario you're getting one part in 10 to the three or 10 to the four of the rest mass of the uranium that you start with you're extracting as energy but even there in even in that process it's still only you know absolute best one part in a thousand the rest. And the reason is that you are using where much more of the energy is stored, which is the strong and weak interactions between the protons and the neutrons.
So much more is available to you. But still, at the end of whatever the process you finish with there, there's a number that will be conserved.
And that is what's called the baryon number. So it's the total number of protons plus the total number of neutrons.
You can transmute protons into neutrons or vice versa in nuclear processes, which is part of the reason they're using much more better energy than things that just affect the chemistry. But still, most of the energy is stored in the rest mass of the protons and the neutrons.
And you want to get that, and nuclear processes conserve that. Beta decay will maybe turn a proton into a neutron or vice versa, but the total number of protons plus neutrons is not changing.
And so therefore, 99.9% of the energy is inaccessible to you. So what you need to do to get that energy and try and get most of the MC squared out of the matter that you have, what you need to do is use a process that eats barium number in which you can start off with a proton and a neutron and end up with no proton or neutron and instead all of that energy unleashed in high energy radiation that you can use for any purposes.
So electromagnetic interactions won't do that. Strong interactions also won't do that.
Weak interactions won't do that. The only force of nature that will do that, with a small caveat, the only force of nature that we know that will do that is the gravitational interaction.
And so it is a property of black holes that you can stand outside the black hole and throw protons and neutrons into the black holes. And then it'll process it and then spit out photons at the end in Hawking radiation and gravitons, which is going to be slightly annoying to have to capture and neutrinos.
But like they're there in principle. And in principle, you could capture them.
So one thing that black holes might be technologically useful for in the future is you start off with a much smaller black hole than what I've just done, the size of the sun. Be very careful about making sure it doesn't grow and yeah you can be super
careful um and throw in protons and neutrons uh and then get out photons and in principle if you could capture the everything that's emitted from the black hole including the gravitons and in the neutrinos that gets rid of the barrier number conservation problem and allows you to build power plants that approach 100% efficiency. And by 100%, I mean not the way we measure gas turbine efficiency, where we talk about the total available chemical energy in the gas.
I mean 100% of the MC squared of the entire gas you're putting in. Yeah.
Although if you consider our cosmic endowment, we're not exactly lacking for mass. We have a lot of mass.
On the other hand, you know, we also have plans for our future that involves exponential growth. And eventually we will run low on that mass and, you know, not that many doublings before using up the whole galaxy.
So you want to use it carefully. Okay.
Let's actually talk about black holes. Yeah.
Yeah, maybe just ask, like, how much information can a black hole store? Ah, okay. Well, as much information, that's a great question.
That has been a very productive line of thought. And the answer to that question goes back to Hawking and Penrose.
So you could even ask another question, which is, how much information can anything store? So actually So can we back up? Why do we like it is actually notable that this is a question we ask of black holes in particular like how often do we ask like how much information can the sun store? Like why in particular are we interested in how much information a black hole can store? Well that it turns out that that's been an incredibly productive line of thought a and b it also turns out that that is the the main fact that we're most confident about about quantum gravity so the two great theories of 20th century physics gravity einstein's theory of the curvature of space-time and gravity and all the rest of it, the very, tends to make itself felt at the very large scale. And on the other hand, quantum mechanics, a theory of the very small, to do with Heisenberg's uncertainty principles and atom and atomic spectra, tends to make itself seen at the very small scale.
These are the two most beautiful theories of 20th century physics, the two things that we should be most proud about that we discovered in the early 20th century. And it was noticed pretty early on that these two theories seem to be inconsistent with each other, that the most obvious ways to try and reconcile quantum mechanics and gravity break.
They don't, you can't really shove them together. And this is a problem if you think that the world should be comprehensible, that there should be some theory that in fact is consistent that describes the world.
So this has been a big project in theoretical physics over the last few decades, is trying to understand how we can take Einstein's general relativity and quantum mechanics and make them meld together in a mathematically and physically consistent manner. It's tricky in part because there's very little experimental guidance because general relativity tends to make itself at large scales, quantum mechanics at small scales.
And so trying to find a place where they meet in the middle, and it must be that they do meet, but that trying to drag that out with experiment is very tricky. But this has been a big project, is trying to figure out how to do this.
Einstein spent some years unsuccessfully doing this in the later less productive part of his career. And this project of trying to unite these is something that a lot of people have thought a lot about.
The string theory comes out of this project, a number of other lines of thought. There is, however, one fact about that merger that we are most confident about, about anything about the merger.
And that exactly returns to this question of how much information can you store in a given region of space-time. And in fact, how much region, and the answer to that involves black holes.
So the answer is how much, if you have a region of a certain area, maybe a sphere of a certain area, and you said how much information can you store in that region, the amount of information you can store measured in bits, the entropy of that region, is given by the area of that region divided by G, Newton's constant, and H-bar, Planck's constant. So that's how you know that this is something to do with quantum gravity because it it involves both G and h-bar.
Is that the only situation in physics where both of those constants end up being in the same place? That is not the only situation, no. Anytime you have quantum gravity, they'll tend to be in the same place.
And sometimes, even when you don't have quantum gravity, but you have the interplay of gravitational forces and quantum degeneracy pressures, those will also, that'll end up in those. But it's in some sense the simplest situation in which it occurs, which is why so much time has been thinking, spent thinking about thought experiments to do with black holes.
So there was a physicist called Bekenstein who figured out that that should be the answer, the area divided by g h bar. And then Hawking's great contribution to physics was figuring out that it was the area divided by g h bar, but he also got the pre-factor, and the pre-factor was a quarter.
So this is, Hawking figured out that it's a quarter at the area divided by 4 g h bar. And this is a super interesting answer um how much information can you store in a given region is given by the area.
And in fact, black holes maximize that. Black holes store that amount of information in a given area.
But specifically area meaning surface area. Meaning surface area, exactly.
So the reason that that's such a wild answer answer and an answer that's led to all sorts of thought experiments to do with quantum gravity ever since then is that you might naively think that the amount of information you can store in a region is given not by its surface area, but by its volume. So if I have a hard drive and I take another hard drive and another hard drive and another hard drive and I keep piling them up, the amount of information I can store on those hard drives scales like the number of those hard drives.
And that means it scales like the volume of the region in which I'm storing the hard drives. That everything we know about classical, you know, classic thermodynamics tells us that the amount of information should scale like the volume.
Everything we know about non-gravitational physics tends to tell us to point in the direction of the amount of information you can store goes, like, the volume. And yet, this is, like, the most surprising fact that is incredibly generative, is that in, once you combine, once you add gravity to the picture, once you combine quantum mechanics and gravity, the amount of information you can store in a given region, a given sphere, goes like the surface area of that region, not like the volume in that region.
And you might think that that's, you might think that that possibly be right. And you might give the following argument.
Okay, so there's some region and I'm just gonna keep adding more and more hard drives to that region. And as I make that region bigger and bigger and bigger, the amount of information on those hard drives goes like the number of those hard drives, which goes like the radius of that region cubed.
And the thing about the radius of the region cubed is it grows faster at large radius than the radius of that region squared So I just told you that the amount of information you can store in a region is given by the surface area And yet I also gave you a way to make it scale like the volume So eventually if I make the region big enough the amount of information in that In that volume will break will be bigger than the bound that I just said. It's therefore I've ruled out Hawking's
and Penrose and Bekenstein's bound.
What goes wrong with that thought experiment
is that eventually if I make a big enough pile of hard drives,
the whole pile of hard drives
will undergo gravitational collapse
and form a black hole.
Actually, but then there has to be sort of an experiment,
not experimental, but a sort of, do you have
to crunch the numbers then to determine that just before the pile of hard drives would collapse into a black hole, the amount of information stored in that cubic pile of hard drives is less than the amount of information that then gets turned into the surface area of the black hole. Because theoretically, it's possible.
I don't know if I'm getting my math intuitions right, right? It's theoretically possible that even though the black hole is smaller because it's only the surface area, the cubic ends up being bigger. Yeah, you have to run that calculation.
But if you do run the calculation, it turns out that it's nowhere near. It wasn't close.
Isn't that one of those things where they just balance each other out? Yeah, they don't just balance each other out. If I take an online shopping website and I buy a bunch of Wiss and digital hard drives and I calculate the information storage capacity of those and compare it to the area of a black hole, I figure out when the pressure in the hard drive would be enough to stop it collapsing to form a black hole.
It is nowhere close. It will make a black hole way, way, way before it comes close to violating Bekenstein or King pound.
Got it. Okay.
Sorry. And then you...
Oh, yeah. So that's the information storage in black holes.
The reason you know that that's also the information storage bound for anything, not just black holes, is that if you had something that wasn't a black hole that had more information than that in a given region, and you just added matter, eventually that thing itself would collapse to form a black hole. And so it couldn't be the case, just logically, that that had more information than the black hole it'll tend to.
You just hinted at the idea that somehow this is like the most productive line of thought that physics has come up with in the last few decades. Why is that? Why is the fact that the area is proportional to the information of a black hole? Tell us so much about the universe.
It's been extremely important for our understanding of quantum gravity. It's perhaps the central fact that we know about quantum gravity is that the information scales with the area.
And that is a hint. That fact that was known since the 70s was a big hint that became very influential later on.
As understood by Beck and Stephen Hawking, it's just a weird fact about black holes perhaps, but we now understand it as a strong indication of what we call the holographic principle. The holographic principle has been a sort of powerful idea in quantum gravity, and it's the following.
So if you took a non-gravitational system,
you know, in which you ignored gravity, like the pile of hard drives, the information storage would scale like the volume, as we discussed, whereas in fact it scales like the area. So, or another way to say that is if you take a three-dimensional, three plus one-dimensional theory in which you have both quantum mechanics and gravity, the information score scales like R squared rather than R cubed, i.e.
it scales as though you had a non-gravitational system in one fewer dimension. So if you had a two-dimensional theory in which there was no gravity, the information stored in a given region would also scale like r squared, because the information would be just the two-dimensional volume, as in the area.
So in other words, it's at least as far as information density, the information capacity is concerned. A gravitational theory in three dimensions is like a non-gravitational theory in two dimensions.
Or more generally, a gravitational theory in n dimensions is like a non-gravitational theory in n minus one dimensions. So that is a big hint that forms the basis of the holographic principle.
It's like gravity eats information. There's less information than you thought there was, than you naively thought there was, if you didn't include information.
And so the holographic principle says that maybe that's not just a neat observation. Maybe it in fact is the case that for some quantum gravitational theories, there is another theory that is exactly equivalent to it in one fewer dimension.
And so this led to Maldusena's ADS-CFT correspondence, the gate-gravity duality, which was the most cited paper in Hengi theoretical physics ever, I think, maybe, at this stage. And in the late 90s, he wrote down, he took that as a hint and it wrote down an exact we believe an exact duality between a particular theory of quantum gravity some particular flavor of string theory and a non-gravitational theory that lives on lives on the boundary of that space um and what problem does it solve if you can model the world in a fewer dimension that doesn't involve gravity? Well, this was a very influential paper, as I said, and really becomes a tremendous theoretical laboratory for trying to understand the connection between gravity and quantum mechanics.
One problem it solves is gravity is mysterious, particularly once we improve quantum mechanics in various ways that we could go into. You know, this is why it's hard to quantize gravity.
But if you can say that this theory that involves both quantum mechanics and gravity is exactly Joule, is in some sense the same theory, is just an alternative description of a theory in one fewer dimensions that doesn't involve gravity, well, that's great because we have much better grasp on how to understand theories that don't have gravity than we do on theories that do have gravity. So it puts everything on a much clearer footing to have this non-gravitational description because then you can just use the standard tools of non-gravitational quantum field theory in order to define it and understand it.
So at one level, I understand that if the information in an area is limited by the information that would be on the surface of a black hole in that region, then yeah, you can model the surface area as a two-dimensional object um on the other hand if I just think about like real world they're just like you're over there and I'm over here and if I like do something here it's not interacting with you and in order to model that fact I need to model the dimension in which the third dimension in which we're separated um which I guess if I'm like actually looking at you through a window pane i maybe wouldn't have access to so and i so how interdimensions how do you model how like that there's a reason we have the third dimension right and how is that how is that modeled if you reduce that dimension yeah so i maybe i should just lead with some disappointing news which is that ads cft was a tremendous conceptual breakthrough in our understanding of quantum gravity and embodied the holographic principle. But at the same time, it doesn't describe our universe.
In particular, in ADS-CFT, there is a negative cosmological constant in the gravitational theory. And our universe, as we discussed before, has a positive cosmological constant.
So it's great because it provides an existence proof of a well-defined theory of quantum gravity, not alas in the universe in which we live in. Okay, but having said that, yeah, it's extremely confusing and was a very impressive result, precisely because you might think, how could it possibly be the case that two different theories in two different dimensions could turn out to be equivalent.
And the answer to your question is, if you have two people who are living in this negatively curved space and talking to each other, what does that look like in this other theory? I say that there's this process going on in the gravitational theory. That's Joule, which is exactly isomorphic to some process going on in the non-gravitational theory in one fewer dimensions but what what maybe looks very simple in one theory like you and i chatting back and forth to each other would look like some complicated plasma physics in in the lower dimensional boundary theory and so that the sort of complexity of how it looks like,
which is a better description,
does not need to be conserved across the isomorphism.
So in fact, that's often what we use it for.
We use it to do arbitrage
between things that look simple in one theory
and things that look simple in the alternative description.
And we use the fact that things look simple in one
to understand the sort of complicated version in the other.
In fact, it flows in both directions.
You might naively expect
that because gravity is so complicated,
we would always be using the non-gravitational theory
to understand the gravitational theory.
That's not always true.
There are these,
plasma physics is itself extremely complicated,
and there are these big collisions
that we do at Rick and Brookhaven where we smash two gold atoms together and make big fireballs of quark-luon plasma. And it's extremely challenging to calculate what would happen there.
And yet people use this duality in the opposite direction to say, even though it looks super complicated with this weird plasma physics, in the non-gravitational theory, it actually can simply be understood as some simple black hole property in the gravitational theory. Maybe not ADS-CFT itself, but would some theory which relies on the holographic principle ever be able to account for a world like ours where, unlike the surface of a black hole,
there isn't a boundary because of the positive cosmological constant and it's constantly expanding. Is there some hope that there in fact is a way to have some sort of
dual theory to this that somehow describes a boundary? Yeah, people are working on that.
That is an open area of research. Ever since the original ADS-CFT was written down, people have
been trying to formulate versions of it in which have a positive cosmological constant. It's difficult, and part of the difficulty goes all the way back to Archimedes.
It is easiest to formulate a theory if you have a fixed point on which to stand and observe things from a distance. in a universe with a positive cosmological constant that you don't have that you don't have that you're necessarily mixed up with the system because you live in a universe that has only a finite amount of entropy finite amount of free energy there is inherent limitation to the precision of the experiments you can do that just makes things way trickier so.
So for that and related reasons, it's a much harder project, but for sure people are working on that. What is the correct conceptual way to think about this? Because one version is the boundary is one way to simplify the processes that are actually four-dimensional.
Another is, I don't know how we think about this in the context of black holes, but maybe in the context of black holes, no, the information actually is on the horizon. The analogous thing here would be like, no, somehow we are on the boundary of the universe somehow.
Is there a sense in which one of these interpretations is correct? Ah, yeah, okay, that's a good good question so this duality idea where you have two different descriptions of the same thing is not the ADS-CFT was not the first such example in physics it's a common trope in physics that you can have two different descriptions of the same thing some of which are more useful in one scenario some of which are more useful in the other scenario but but which are both exactly correct and there are non-gravitational examples in physics that go back a long way you may then ask you know which one is right yeah and which one is not right uh is is it actually a cft that's pretending to be you know that has this weird alternative description as a as a gravitational theory or is the gravitational theory correct and the other one's not correct i think this is more of a philosophical question. My answer would be is if the isomorphism was just an approximation, like it was really one thing and you were just pretending it was the other thing and that approximation worked in some region of validity and not others, then I would say that one was right and the other one was just an alternative fanciful description.
That is not our understanding of ADS-CFT as we understand it today. Our understanding is that this is a precise isomorphism.
It's not an analogy. It's not a metaphor.
It is not an approximation that is valid in some domain and not another. It really is the case that these two theories are exactly equivalent to each other.
And if that's correct, then as a matter of philosophy, I would say those are both equi-real. So it's not the case that one is more real than the other.
They're perfect simulations of each other. Yeah.
Are you an ADS dreaming you're a CFT or a CFT dreaming you're an ADS? I think these are just two completely different, inequivalent descriptions of the same identical physics. Tell me if this is just like a question that just doesn't make sense because look, when I was like, if you try to ask somebody about like the quantum many worlds, where are the other worlds, right? And they're just like, they're in Hilbert space.
Like, where is Hilbert space? They're just like, no, dude, it's just like a conceptual, like just like a conceptual like you don't you know just like stop asking questions um intuitively it feels like there should be a sense in which like there's some physical existence and either that existence is in this four-dimensional space or it's in some space that exists on the boundary um is this just again just going to lead us into philosophical loops or is there something that can be said more about it and also in a decider in a world like ours um what exactly would the boundary mean yeah so there are two components to that question you have an intuition that if something is real it needs to be spatially and things that are delocalized in space somehow can't be real. I would say that that's not my intuition.
My intuition is that there can be two completely different descriptions of the same physics. And if it's precise, neither of those is any more real than the other.
Things do not need to be spatially localized. You separately asked, what would it look like? What would a version of, where is the boundary theory in the sort of space since there's no boundary? That is a great question that people who are trying to generalize ADS CFT to a universe like ours that has a positive squash model constant that they wrestle with.
And there's more than one proposal, some of which is that the place, one example of a proposal is that the Joule theory should live on the cosmic horizon. So there's a, if you go five billion light years, you can send information to that point and have it returned to you.
But on the other hand, there are things that are a hundred billion light years away years away that we'll never be able to communicate with. And there's a boundary between those two, between some things that we could in principle communicate with and things that we couldn't in principle communicate with.
That is the cosmological horizon. And some people who are trying to do a version of holography that works in universes of the positive cosmological constant like to put the second theory there.
Other people like to put it in the distant future, in the sort of infinitely distant future. And that's part of the problem, is that where do we even put that theory? It's not like in our universe where you can just put it spatially infinitely far away and be done with it.
If it's spatially finite, then we are currently at the boundary of infinite many other universes that are located, or whose center is located elsewhere. Absolutely.
So a cosmological horizon is very different from a black hole horizon in this regard. A black hole horizon, there is a point of no return.
And if you get closer than that, you fall into the black hole and you're never getting out again. And everybody can agree where that is.
For cosmology, there is a point of no return, but the point of no return is return to a given person. And so for each person, there is a different point of no return.
And as you say, we live on the boundary just as much as we live on the boundary of those people live on our cosmological horizon we may live on on this okay another uh philosophical question there's seems to be many theories which imply that um there's some sort of infinity or approximate infinity that exists um where uh in quantum many worlds you know there's just like constantly these um constantly these different branches of the wave function spawning off where things are slightly different. And so everything that can possibly happen has happened, including basically the same exact thing.
I guess if this bubble universe stuff is correct, it implies a similar picture. Philosophically, should it have some implication on our worldview uh it would be surprising that we would learn this much about the universe then it has like no implications whatsoever right good question i think i'm going to say yes and no i mean it's so clearly i mean if correct let's just take the quantum case which is perhaps even more secure than the cosmological multiverse case the quantum case, it really does look like the default expectation, given everything we understand about quantum mechanics, should be the many worlds interpretation in which the universe
keeps branching off and there'd be more and more branches. And every time, or almost every time,
you come to a point of quantum measurement, we might colloquially say, is made that the universe
branches and then there's every possibility is represented still in the in the way in the grander way function that's a pretty profound thing to learn about the ontology of the world if if correct it seems like it should be the default expectation um and you might say you know maybe i don't care about uh existential risk uh in our universe because, you know, we blow each other up or turn into goo or whatever. Okay, that's sad for us.
Maybe our world has vacuum decay, but there are some other branches of the wave function where it's not. And so I'm kind of, you know, some other branches would have made different choices in the past and they're sort of guaranteed to somewhere in the branches of the of the wave function to be a flourishing world and so i'm not so bothered um i would say that that's i'm not not going to tell you you know what what uh what utility function you should place on the wave function but uh but born is uh you know that's the born rule in quantum mechanics and And that tells you that you shouldn't just say, if it's there in one branch, that's just as good as anything else.
Born's rule, which is one of the foundational rules in quantum mechanics, tells you how much to care about each branch. You don't care about them equally.
and it says that the correct way to calculate the expectation value of anything
is to calculate its value in each branch and weight those branches by the square of the amplitude of the wave function, which is some particular quantity, and then add together all of those different answers. So that's a linear answer, which is to say that the total utility of the universe is the sum of the utility in each of these branches, appropriately weighted by Born's rule.
So if that's true, you know, you should hope to make our branch as good as possible, just because whatever is going on in the other branch, the total utility is just the sum of what's going on in that branch and what's going on in our branch. And so you should try as hard as you can to make our branches as great as possible.
Nevertheless, I do kind of understand that you might have a portfolio theory that seems to be inconsistent with Born's rule, but is somehow intuitive in which somehow it's not just a linear function on these universes. Yeah, I mean, this would only be like, if you are a total utilitarian, Who then there's a sort of very straightforward way in which you can dismiss this.
Yeah. And be like, it's one of these like it seems like in physics, there's always these kinds of things where like, oh, we think we discover something new.
But would you look at that? Like that is the speed of light. It is still conserved.
And similarly here, like, oh, infinite universe is. But like like would you look at that like it has
implications on our decisions but most people are not totally utilitarians and if you have some very simple thought experiments to illustrate a couple suppose that there's two universes and sorry two worlds in two different cosmic horizons who will never interact with each other causally but each one has intelligent life
and civilization and beauty and everything we might care about. If one of the two gets extinguished, I'm like pretty sad.
And this is, I suppose both of these make up the entire universe. If both of them get extinguished, I'm more than twice as sad.
There's something to that sort of finality, which makes existential risk salient in the first place. And if you agree with that intuition, then I think you should be inclined to think that like, oh, there's something significant about the fact that in some base reality, like genuinely the story carries forward.
On the other end, you're somebody who cares about minimizing uh the uh downside of like people talking about like suffering risk or something right like the idea that if it's physically possible to have a universe full of torture it's actually in fact happening or will happen again is like uh you could just be like ah but the amplitude on that is like so small or or the squarely amplitude is so small, you know, like, and the weighted average ends up close to nothing. But I'm like, that really sucks.
You know, that's like actually happening. Yeah, I think there's a number of ways to think about this.
I think in part, people's intuition is maybe formed in cases like extinction, where if you have an animal that's going extinct, you know, if half of the animals get wiped out, that's somehow less bad than if both halves of the animals gets wiped out. But that's because they really are going to interact in the future.
And there's the possibility of the... Those don't have non-overlapping future light cones, the two populations of some possibly extinct animal.
It's also the case that this is a pretty... Like Bour's Rule, narrowly defined, does not really have anything to say about this, how one should calculate the total utility.
It's just more of a sort of the natural utility measure that would come out of this. Particularly when you get to the cosmological multiverse, I think that these are very difficult questions to answer.
Your intuition that two, you know, maybe perhaps two different universes in which, like, how we calculate those, do we just add together the utility in both or is there some non-linearity to do with it? Basically, for the cosmological multiverse, there isn't a particularly good way to decide what the weighting factor should be. We don't have the same equivalent of Born's rule in quantum mechanics.
And I think it's at least open for opinions like yours to be, you know, to be in fact, there should be some better way in which we calculate it that's not just a linear function. Of these different kinds of infinities, is there some sense in which some are more fundamental than others.
That is, maybe the bubbles are artifacts
of what's actually happening on the wave function or vice versa.
You're talking about the two kinds of multiverse,
the sort of cosmological multiverse
and the quantum mechanical multiverse.
Yeah, they get very bound up
if you try and write down a theory that has both of them.
Because whether there's a bubble there,
you're trying to make bubble universes. But what gives rise to bubble universes is often quantum processes.
So often you end up in superpositions over there being a bubble universe and there not being a bubble universe there. And that means that these two kinds of multiverse, the sort of quantum mechanical multiverse and the cosmological multiverse end up getting totally intermeshed with each other.
But it sounds like the base reality is like still like the wave function over all the bubbles and the entire inflaton field or whatever. Yeah.
So again, we only really properly know how to do quantum gravity and do the counting in when there's a negative cosmological constant, as we discussed with ADS-CFT. In these bubble universes where there's a positive cosmological constant, it's still somewhat an open question how to do the accounting of what happens and where and how much it should count.
Which is to say we don't know the answer to that question and your opinion is not ruled out. You know, it's a little bit confusing because uh in one context we're laying out sort of very practical i don't know if you can call uh black hole batteries practical but um very like sort of like tangible um uh uh limitations on the uh what future or like very distant future descendants could do with all the matter in the galaxy and so forth.
On the other hand, we're like, bubble universes as big as our own made somewhere in somebody's lab? Maybe. So basically, yeah, how confident are we in the practical limitations we think we know about will actually constrain our future descendants?
Yeah, I think that's a good question.
Certainly, some of the possibilities we've discussed so far have different epistemic statuses about how confident we are or not confident.
And as we also discussed, some of these bounds are somewhat fragile um can you communicate faster than the speed of light for example let's just take that as an example bound um we think you can't according to the laws of science as we understand it most physicists will be pretty surprised if it turned out that you could even though probability if like a million years from now we are able to communicate faster than light? How surprised are you? That is a tricky one. That is a really tricky one.
We've only thought, it's only a century that we thought you can't communicate faster than the speed of light. A million years is such a radical time that maybe we've sort of dissolved the question into some greater question and we understand it doesn't even really make sense.
I would be pretty surprised. If you make me make a number, I think that there is a greater than 90% chance that in 100 years we are still limited by the speed point.
There's a 98% chance, if you make me make me be precise okay so then what are the other
constraints on a future civilization uh that are that they might care about right so if uh
we've got the superhuman intelligences and they're colonizing the galaxy
uh what are uh what are the things they might want to do that they can't do
um they probably care about energy they care care about computation. So energy limits.
We've talked about the efficiency of batteries and extracting energy. MC squared is the – I'm highly confident that the most energy you can extract from a given piece of matter is MC squared, at least until you start getting cosmology involved.
Other limits will be Landau's limit, or in other words, you know, with a given amount of energy, how much, how useful is a given amount of energy to you? You know, if you, we wouldn't care about having as huge amounts of energy if you could get an arbitrary amount of value out of a fixed unit of energy. We think that that's not true.
We think that the, in particular, if we're going to do computations with it, for example, that there's going to, and that computation makes errors, that there is a fixed cost of a bit, basically a bit of free energy, in order to correct those errors. And we're confident that there's no way to make computers that don't make errors? It is a very interesting question what the fundamental limits on errors are in a computer.
How far down can they be pushed? In terms of never making errors, I think that's very unlikely. If for no other reason than that there is a minimum background temperature caused by the expansion of our universe, by, again, it all coming back to the cosmological constant, that gives a very small but non-zero temperature to our universe that I think will inevitably mean that we make errors.
You might imagine we could just set up some kind of perpetual motion machine that's just like thinking happy thoughts over and over again in a quantum computer that never tires and never stops. I think that inevitably there would be, the universe would leak in and there will be errors.
Yeah, but what the the minimum error rate is is not i think a clear i don't have a clear answer to that question and physics doesn't have a clear answer to that question so one question you might have is how like what will be the nature of uh not only the things that our descendants might care about but like um what will they be able to produce quote-unquote domestically? What will they want to trade for? And if something like Alchemy is just like super, you know, just like equals MC squared is all you care about, then it's just like, look, your star system, your galaxy has a certain amount of mass and you can convert that to energy. And there's fundamentally no reason to trade if there's like not that high transaction cost to um uh make it into whatever you want on the other hand if there are some limits like in fact you had to make like galaxy wide factories or um you had to do these np hard calculations that you can even with a galaxy you can only trace down certain segments of um uh the search space or something there might be reasons to trade um extremely sort of like uh uh pines question but how much can be into it about these kinds of constraints i mean so in economics the theory of comparative advantage yeah only applies if not all resources can be transported.
Like if you can just go in and just disassemble whoever you're doing the comparative advantage with, you might as well just apply it all to the party with the absolute advantage. So maybe the same thing would be true in the universe.
I think there are a number of questions in there. For starters, not all energy is equally useful in different places in the universe.
If there's a galaxy over there and a galaxy here on this side of the universe, because of the expansion of the universe, if I beamed the energy, if I disassembled that galaxy and tried to send it back here either by you know literally sending it on starships or converting it to light and beaming the light back in a laser and then having a big you know photo photos here uh pv here so collected or for whatever mechanism by the time it reached me there would be a massive redshift And so keeping it in place is maybe better than just disassembling it and all and bringing it back home. But there's another question, which is, you know, what is the, is the plan to, these are all unknowns to do with both physics and the nature of technology.
Is the most important thing that all of the value will be created here on Earth and we just need to get as many resources back here on earth and it's you know the the there are super linear returns to scale of having accumulated resources in one place so we just want to make earth an absolute paradise or do we want to spread is in fact sublinear and we want to spread civilization all the way throughout all of these galaxies um i think questions like that are going to be important in addressing your question of what the returns to scale are and returns to trade as well. If like the galaxy in a billion years from now has a certain GDP, what percentage of that GDP do you think is just like the end result of computations or confirmation that a computation has been made? Maybe it's like simulating hedonium that the other side of the galaxy cares about or something.
Just because it may prove to be so much more efficient to do things in simulation than to do them in the real world, my guess would be a high percentage of that. But maybe that's wrong.
If compute is the main thing you care about, what is going to be the, physically, how will the full ops in a galaxy be organized? Will it be as like a planet-wide computers, as like a huge blob the size of a star system? Do we have some sense of? Yeah, I think this is a super interesting question. So it returns to the question we were asking before.
With quantum computers, we know, for example, that the amount of quantum computation you can do in terms of the equivalent amount of classical computation in trying to do some factoring algorithm or something grows super linearly with the number of qubits. In fact, it grows almost exponentially with the number of qubits.
So a 200 qubit quantum computer is much more than twice as good as a 100 qubit quantum computer. For certain tasks, but for the tasks that we try and use quantum computers for, that's true.
So that line of reasoning might lead you to believe that in the distant future we will just try and you know even paying the cost of the redshift and all these other questions we'll feed all of the energy and free energy back into one central quantum computer and it'll all be about making that central quantum computer as big as we possibly can even at the cost of inefficiency On the other hand, there are other kinds of tasks for which actually having a twice as big computer is not that much better or certainly not more than twice as better as having two smaller computers. In that scenario, it'll be a more distributed setup.
I guess in this quantum computer system, you would need to have coherence across this like huge, which might not be a practical engineering difficulty for future civilizations, but that seemed like. Yeah, either it would need to be co-located or you need to send the quantum coherence out.
That's actually not that hard to do. It's a property of photons that they do tend to maintain when they're propagating in the vacuum.
They basically maintain their coherence for a very long way. In fiber optic cables, you reach trouble because they start getting absorbed by the fiber optics after tens of miles.
But in the vacuum, you could, in principle, share quantum entanglement across the universe if you did you did it right then wouldn't you wouldn't you expect um when you say like a central computer physically wouldn't just be like a huge like contiguous uh well it might be because you know the sort of analog of the classical fact that flops are not the only thing you care about you also care about bandwidth and interconnects and things like that. So perhaps the same would be true.
I mean, here we're getting into a pretty speculative area, but you could imagine either configuration, either on which you have a huge number of different quantum computers that are talking to each other via entanglement networks or in which you just have one big central computer. Yeah.
Final question. Timeline to when you are automated as a physicist.
Oh, good question. Many of the tasks that I might have performed in the past, I think, are already automated at some level until I am totally out of the picture and no longer necessary.
That's probably pretty close to ASI complete. So whatever your timeline for ASI is.
Well, I guess the question is what is yours? Yeah, I'm squirming somewhat uncomfortably in answer to that question because I'm not totally sure. I could certainly imagine a scenario in which it's five years.
All right.
I think that's a great place to close.
Adam, thanks so much.
Thank you.
Great to be here.