#428 – Sean Carroll: General Relativity, Quantum Mechanics, Black Holes & Aliens
2h 44m 40s
Sean Carroll, a leading theoretical physicist and science communicator, discusses key concepts in general relativity and quantum gravity, focusing on the nature of spacetime, black holes, and the information paradox. He explains that gravity arises from the curvature of spacetime, a breakthrough Einstein achieved through self-driven learning of advanced mathematics. Black holes are not solid objects but regions where escape is impossible, with their interiors ending in a future singularity—a moment of spacetime collapse. The central mystery is whether information falling into a black hole is destroyed or preserved, a conflict between classical relativity and quantum mechanics. The holographic principle offers a radical solution: all information about a black hole is encoded on its event horizon, not within its volume, suggesting a deep connection between space, gravity, and information. Carroll highlights that while this idea is theoretically compelling, it remains unproven, with no direct experimental evidence—especially from Hawking radiation, which is too faint to detect. He also touches on neutrino experiments like IceCube, which may one day reveal subtle deviations from quantum field theory, testing the holographic principle in extreme conditions. Ultimately, Carroll emphasizes the limits of human understanding, suggesting that black holes may hold profound revelations about the nature of time, information, and the universe—potentially even challenging quantum mechanics itself. His perspective blends deep physics with philosophical humility, underscoring that many of the most fundamental questions in science remain open and exciting.
The following is a conversation with Sean Carroll, his third time on this podcast.
He is a theoretical physicist at Johns Hopkins, host of the Mindscape podcast that I personally
love and highly recommend, and author of many books, including the most recent book series
called The Biggest Ideas in the Universe. The first book of which is titled Space,
Time, and Motion, and it's on the topic of general relativity. And the second,
coming out on May 14th, so you should definitely pre-order it, is titled Quanta and Fields,
and that one is on the topic of quantum mechanics. Sean is a legit active theoretical physicist,
and at the same time, is one of the greatest communicators of physics ever. I highly
encourage you listen to his podcast, read his books, and pre-order the new book to support
his work. This was, as always, a big honor and a pleasure for me.
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And now, dear friends, here's Sean Carroll.
In book one of the series, The Biggest Ideas in the Universe, called Space-Time-Motion,
you take on classical mechanics, general relativity, by taking on the main equation
of general relativity and making it accessible, easy to understand. So maybe at the high level,
what is general relativity? What's a good way to start to try to explain it?
Probably the best way to start to explain it is to start with the general relativity.
is special relativity, which came first, 1905. It was the culmination, right, of many decades of
people putting things together, but it was Einstein in 1905. In fact, it wasn't even Einstein. I should
give more credit to Minkowski in 1907. So Einstein in 1905 figured out that you could get rid of
the ether, the idea of a rest frame for the universe, and all the equations of physics
would make sense, with the speed of light being a maximum.
But then it was Minkowski, who used to be Einstein's professor in 1907, who realized
the most elegant way of thinking about this idea of Einstein's was to blend space and time together
into space-time, to really imagine that there is no hard and fast division of the four-dimensional
world in which we live into space and time separately. Einstein was at first dismissive
of this. He thought it was just like, oh, the mathematicians are over-formalizing again. But
then he later realized that it was just like, oh, the mathematicians are over-formalizing again.
But then he later realized that if space-time is a thing, it can have properties. And in particular,
it can have a geometry. It can be curved from place to place. And that was what let him solve
the problem of gravity. He had previously been trying to fit in what we knew about gravity from
Newtonian mechanics, the inverse square law of gravity, to his new relativistic theory.
It didn't work. So the final leap was to say gravity is the curvature of space-time,
and that statement is basically general relativity.
And the tension with Minkowski was, he was a mathematician.
Yes.
So there's a tension between physics and mathematics. In fact,
in your lecture about this equation, one of them,
you say that Einstein is a better physicist than he gets credit for.
Yep. I know that's hard. That's a little bit of a joke there, right?
Yeah.
Because we all give Einstein a lot of credit. But then we also
have to be really based on fact, but partly to make ourselves feel better, tell ourselves a story about how later in life Einstein couldn't keep up. There were younger people doing quantum mechanics and quantum field theory and particle physics, and he was just sort of unable to really philosophically get over his objections to that. And I think that that story about the latter part is completely wrong, like almost 180 degrees wrong. I think that Einstein understood quantum mechanics as well as anyone, at least up through the 1930s.
I think that his philosophical objections to it are correct. So he should actually have been taken much more seriously about that. And what he did, what he achieved in trying to think these problems through is to really basically understand the idea of quantum entanglement, which is kind of important these days when it comes to understanding quantum mechanics. Now, it's true that in the 40s and 50s, he placed his efforts in hopes for unifying electricity and quantum mechanics.
But in the 40s and 50s, he placed his efforts in hopes for unifying electricity and quantum mechanics. Brownian motion is another one, which is just, you know, the little vibrations of tiny little dust specks in the air. But who cares about that? What matters is it proves the existence of atoms. He explains Brownian motion by imagining there are molecules in the air and deriving their properties. Brilliant.
And then he basically starts the world on the road to quantum mechanics with his paper on, which again is given a boring label of the photoelectric effect. What it really was is he invented photons.
If the rocket ship were very quiet, you wouldn't be able to know the difference between being in a rocket ship and being on the surface of the Earth. Gravity is sort of not detectable, or at least not distinguishable from acceleration. So number one, that's a pretty clever thing to think. But number two, if you or I had that thought, we would have gone, huh, we're pretty clever. He reasons from there to say, okay, if gravity is not detectable, then it can't be like an ordinary force, right? The electromagnetic force is detectable.
We can put charged particles around, positively charged particles and negatively charged particles respond differently to an electric field or to a magnetic field. He realizes that what his thought experiment showed, or at least suggested, is that gravity isn't like that. Everything responds in the same way to gravity. How could that be the case? And then this other leap he makes is, oh, it's because it's the curvature of spacetime, right? It's a feature of spacetime. It's not a force on top of it. And the feature that it is, is curvature.
And then finally, he says, okay, clearly, I'm going to need the mathematical tools necessary to describe curvature. I don't know them, so I will learn them. And they didn't have MOOCs or AI helpers back in those days. He had to sit down and read the math papers, and he taught himself differential geometry and invented general relativity.
One dimension of space, one dimension of time.
so-called space-time diagram. But, you know, I mean, maybe this is lurking underneath your
question, but even the best physicists will draw, you know, a vertical axis and a horizontal axis,
and they'll go space-time. But deep down, that's wrong, because you're sort of preferring one
direction of space and one direction of time, and it's really the whole two-dimensional thing
that is space-time. The more legitimate thing to draw on that picture are rays of light,
are light cones. From every point, there is a fixed direction at which the speed of light would
represent, and that is actually inherent in the structure. The division into space and time
is something that's easy for us human beings. What is the difference between space and time
from the perspective of general relativity? It's the difference between x and y when you draw
x and y.
On a piece of paper.
So there's really no difference.
There's almost no difference. There's one difference that is kind of important,
which is the following. If you have a curve in space, I'm going to draw it horizontally,
because that's usually what we do in space-time diagrams. If you have a curve in space,
you've heard the motto before that the shortest distance between two points is a straight line.
If you have a curve in time, which is, by the way, literally all of our lives, right? We all
evolve in time. So you can start with one event in space-time,
and then you can start with another event in space-time.
Another event in space-time. What Minkowski points out is that the time you measure along
your trajectory in the universe is precisely analogous to the distance you travel on a curve
through space. And by precisely, I mean it is also true that the actual distance you travel
through depends on your path, right? You can go a straight line, shortest distance, and curvy line
would be longer. The time you measure in space-time, the literal time that takes off on your clock,
also depends on your path. But it depends on it the other way, so that the longest time between
two points is a straight line. And if you zig back and forth in space-time, you take less and less
time to go from point A to point B. How do we make sense of that,
the difference between the observed reality and the objective reality underneath it? Or
is objective reality a silly notion, given general relativity?
I'm a huge believer.
I'm a huge believer in objective reality. I think that objective reality, objectively,
is real. But I do think that people kind of are a little overly casual about the relationship
between what we observe and objective reality in the following sense. Of course,
in order to explain the world, our starting point and our ending point is our observations,
our experimental input, the phenomena we experience and see around us in the world. But in between
there's a theory. There's a mathematical formalization of our ideas about what is going
on. And if a theory fits the data and is very simple and makes sense in its own terms, then we
say that the theory is right. And that means that we should attribute some reality to the entities
that play an important role in that theory, at least provisionally until we come up with a better
theory down the road. I think a nice way to test
the difference between objective reality and the observed reality is what happens at the edge of the
horizon of a black hole. So, technically, as you get closer to that horizon, time stands still.
Yes and no. It depends on exactly how careful we're being. So, here is a bunch of things I
like to point out. One of the things I like to point out is that you treat the whole solution
Einstein's equation and you treat you and me as what we call test particles. So, we don't have
any gravitational fields ourselves. We just move around in the gravitational field. And that's
obviously an approximation, okay? But let's imagine that. And you stand outside the black
hole and I fall in. And as I'm falling in, I'm waving to you, you know, because I'm going into
the black hole. You will see me move more and more slowly. And also, the light from me is red
shift. So, I kind of look embarrassed because I'm falling into a black hole. And there is a limit. There's
a last moment that light will be emitted from me, from your perspective, forever, okay? Now,
you don't literally see it because I'm emitting photons more and more slowly, right? Because from
your point of view. So, it's not like I'm equally bright. I basically fade from view in that
picture, okay? So, that's one approximation. The other approximation is that I'm emitting photons
I do have a gravitational field of my own. And therefore, as I approach the black hole,
the black hole doesn't just sit there and let me pass through. It kind of moves out to eat me up
because its net energy mass is going to be mine plus its. But roughly speaking, yes. I think so.
I don't like to go to the dramatic extremes because that's where the approximations break
down. But if you see something falling into a black hole, you see its clock ticking more and
more slowly. How do we know it fell in? We don't.
I mean, how would we? Because it's always possible that right at the last minute,
it had a change of heart and starts accelerating away, right? If you don't see it pass in,
you don't know. And let's point out that as smart as Einstein was, he never figured out
black holes. And he could have. It's kind of embarrassing. It took decades for people
thinking about general relativity to understand that there are such things as black holes.
Because basically, Einstein comes up with general relativity in 1915.
Years later, Schwarzschild, Karl Schwarzschild, derives the solution to Einstein's equation that
represents a black hole, the Schwarzschild solution. No one recognized it for what it
was until the 50s, David Finkelstein and other people. And that's just one of these examples
of physicists not being as clever as they should have been.
Well, that's the singularity. That's the kind of the edge of the theory, the limit.
So it's understandable that it's difficult to imagine the limit of things.
It is absolutely hard to imagine. And the black hole is very different in many ways
from what we're used to. On the other hand, I mean, the real reason, of course, is that between
1915 and 1955, there's a bunch of other things that are really interesting going on in physics,
all of particle physics and quantum field theory. So many of the greatest minds were
focused on that. But still, if the universe hands you a solution to general relativity
in terms of curved spacetime, and it's kind of mysterious, certain features of it,
I would put some effort into trying to figure it out.
So how does a black hole work? Put yourself in the shoes of Einstein
and take general relativity to its natural conclusion about these massive things.
It's best to think of a black hole as not an object so much as a region of spacetime, okay?
It's a region with the property, at least in classical general relativity. Quantum mechanics
makes everything harder, but let's imagine we're being classical for the moment.
It's a region of spacetime with the property that if you enter, you can't leave. Literally,
the equivalent of escaping a black hole would be moving faster than the speed of light. They're
both precisely equally difficult. You would have to move faster than the speed of light to escape
from the black hole. So once you're in, that's fine. You know, in principle, you don't even
notice when you cross the event horizon, as we call it. The event horizon is that point of no
return, where once you're inside, you can't leave. But meanwhile, the spacetime is sort of
collapsing around you to ultimately a singularity in your future, which means,
that the gravitational forces are so strong, they tear your body apart, and you will die
in a finite amount of time. The time it takes, if the black hole is about the mass of the sun,
to go from the event horizon to the singularity takes about one millionth of a second.
What happens to you if you fall into the black hole? If we think of an object as information,
that information gets destroyed. Well, you've raised a crucially
difficult point. So that's why I keep needing to distinguish between black holes according to
Einstein's theory of general relativity, which is book one of spacetime and geometry, which is
perfectly classical. And then come the 1970s, we start asking about quantum mechanics and what
happens in quantum mechanics. According to classical general relativity, the information
that makes up you when you fall into the black hole is lost to the outside world. It's there.
It's inside the black hole.
But we can't get it anymore. In the 1970s, Stephen Hawking comes along and points out that black holes
radiate. They give off photons and other particles to the universe around them. And as they radiate,
they lose mass, and eventually they evaporate. They disappear. So once that happens, I can no
longer say the information about you or a book that I threw in the black hole or whatever is
still there. It's hidden behind the black hole because the black hole has gone away.
So either that information is destroyed, like you said, or it is somehow transferred to the
radiation that is coming out, to the Hawking radiation. The large majority of people who
think about this believe that the information is somehow transferred to the radiation and
information is conserved. That is a feature both of general relativity by itself and of
quantum mechanics by itself. So when you put them together, that should still be a feature.
We don't know that for sure. There are people who have doubted it, including Stephen Hawking for a long
time. But that's what most people think. And so what we're trying to do now in a topic
which has generated many, many hundreds of papers
called the Black Hole Information Loss Puzzle,
is figure out how to get the information
from you or the book into the radiation
that is escaping the black hole.
Is there any way to observe Hawking radiation
to a degree where you can start getting insight?
Or is this all just in the space of theory right now?
Right now, we are nowhere close
to observing Hawking radiation.
Here's the sad fact.
The larger the black hole is,
the lower its temperature is.
So a small black hole,
like a microscopically small black hole,
might be very visible.
It's given off light.
But something like the black hole
at the center of our galaxy,
three million times the mass of the sun
or something like that, Sagittarius A star,
that is so cold and low temperature
that its radiation will never be observable.
Black holes are hard to make.
We don't have any nearby.
The ones we have out there in the universe
are very, very faint.
So there's no immediate hope for detecting
Hawking radiation.
Allegedly, we don't have any nearby.
As far as we know,
we don't have any nearby.
Could tiny ones be hard to detect?
Somewhere at the edges of the solar system, maybe?
So you don't want them to be too tiny
or they're exploding, right?
They're very bright
and then they would be visible.
But there's an absolutely regime
where black holes are large enough
not to be visible
because the larger ones are fainter, right?
Not giving off radiation,
but small enough to not be detected
through their gravitational effect.
Yeah.
Psychologically, just emotionally,
how do you feel about black holes?
Do they scare you?
I love them.
I love black holes.
But the universe, weirdly,
makes it hard to make a black hole, right?
Because you really need to squeeze
an enormous amount of matter and energy
into a very, very small region of space.
So we know how to make stellar black holes.
A supermassive star can collapse
to make a black hole.
We know we also have
these supermassive black holes
at the center of galaxies.
We're a little unclear where they came from.
I mean, maybe stellar black holes
that got together and combined.
But that's, you know,
one of the exciting things about new data
from the James Webb Space Telescope
is that quite large black holes
seem to exist relatively early
in the history of the universe.
So it was already difficult
to figure out where they came from.
Now it's an even tougher puzzle.
So these supermassive black holes
were formed somewhere early on in the universe.
I mean, that's a feature, not a bug, right?
That we don't have too many of them.
Otherwise, we wouldn't have
the time or the space
to form the little pockets of complexity
that we'll call humans.
I think that's fair, yeah.
It's always interesting
when something is difficult
but happens anyway, right?
I mean, the probability of making a black hole
could have been zero.
It could have been one.
But it's this interesting number in between,
which is kind of fun.
Are there more intelligent alien civilizations
than there are supermassive black holes?
Yeah.
I have no idea.
But I think your intuition is right
that it would have been easy
for there to be lots of civilizations
and then we would have noticed them already.
And we haven't.
So absolutely the simplest explanation
for why we haven't is that they're not there.
Yeah.
I just think it's so easy to make them, though.
So there must be. I understand that's the simplest explanation.
But also. How easy is it to make life?
Or eukaryotic life?
Or multicellular life?
It seems like. Life finds a way.
Intelligent alien civilizations, sure.
Maybe there is somewhere along that chain
a really, really hard leap.
But once you start life,
once you get the origin of life,
it seems like life just finds a way.
Everywhere.
In every condition.
It just figures it out.
I mean, I get it.
I get exactly what you're thinking.
I think it's a perfectly reasonable attitude to have
before you confront the data.
I would not have expected Earth to be special in any way.
I would have expected. There'd be plenty of very noticeable
extraterrestrial civilizations out there.
But even if life finds a way,
even if we buy everything you say,
how long does it take for life to find a way?
What if it typically takes 100 billion years?
Then we'd be alone.
So it's a time thing.
So to you, really, there's. Most likely, there's no alien civilizations out there.
I just. I can't see it.
I believe there's a ton of them,
and there's another explanation.
Why we can't see them.
I don't believe that very strongly.
Look, I'm not going to place a lot of bets here.
I would not. I'm both pretty up in the air
about whether or not life itself is all over the place.
It's possible, you know,
when we visit other worlds, other solar systems,
there's very tiny, microscopic life, ubiquitous.
But none of it has reached some complex form.
It's also possible there's just. There isn't any.
It's also possible that there are intelligent civilizations
that have better things to do
than knock on our doors.
So I think, you know,
we should be very humble about these things
we know so little about.
And it's also possible there's a great filter
where there's something fundamental about. Once a civilization develops complex enough technology,
that technology is more statistically likely
to destroy everybody
versus to continue being creative.
That is absolutely possible.
I'm actually putting less credence on that one
just because you need it to happen every single time, right?
Okay.
If even one,
I mean, this goes back to von Neumann pointing out. John von Neumann pointed out that
you don't need to send the aliens around the galaxy.
You can build self-reproducing probes
and send them around the galaxy.
And you might think,
well, the galaxy is very big.
It's really not.
It's some tens of thousands of light years across
and billions of years old.
So you don't need to move
at a high fraction of the speed of light
to fill the galaxy.
So if you were an intelligent alien civilization,
the dictator of one,
you would just send out a lot of probes,
self-replicating probes.
A hundred percent.
And. Just spread out.
Yes.
And what you should do,
this is. So if you want the optimistic spin,
here's the optimistic spin.
People looking for intelligent life elsewhere
often tune in with their radio telescopes, right?
At least we did before Arecibo was decommissioned.
That's not a very promising way
to find intelligent life elsewhere
because why in the world
would a super intelligent alien civilization
waste all of its energy
by beaming it in random directions into the sky?
For one thing,
it just passes you by, right?
So if we're here on Earth,
we've only been listening to radio waves
for a couple hundred years, okay?
So if an intelligent alien civilization
exists for a billion years,
they have to pinpoint exactly the right time
to send us this signal.
It is much, much more efficient
to send probes and to park.
To go to the other solar systems,
just sit there and wait
for an intelligent civilization
to arise in that solar system.
This is kind of the 2001 monolith hypothesis, right?
I would be less surprised
to find a sort of quiescent alien artifact
in our solar system
than I would to catch a radio signal
from an intelligent civilization.
So you're a sucker for in-person conversations
versus remote.
I just want to integrate over time.
A probe can just sit there and wait,
whereas a radio wave goes right by you.
How hard is it for an alien civilization,
again, you're the dictator of one,
to figure out a probe
that is most likely to find a common language
with whatever it finds?
Couldn't I be like the elected leader
of the alien civilization?
Elected leader, democratic leader,
elected leader of a democratic alien civilization, yes.
I think we would figure out
that language thing pretty quickly.
I mean, maybe not as quickly as we do
when different human tribes find each other
because obviously there's a lot of commonalities
in humanity,
but there is logic in math
and there is the physical world.
You can point to a rock and go,
rock, right?
I don't think it would take that long.
I know that Arrival, the movie,
based on a Ted Chiang story,
suggested that the way that aliens communicate
is going to be,
is going to be fundamentally different,
but also they had precognition
in other things I don't believe in.
So I think that if we actually find aliens,
that will not be our long-term problem.
So there's a folks,
one of the places you're affiliated with is Santa Fe
and they approach the question of complexity
in many different ways
and ask the question in many different ways
of what is life,
thinking broadly.
So do you be able to find it?
You'll think you show up,
a probe shows up to a planet,
we'll see a thing and be like,
yeah, that's a living thing.
Well, again,
if it's intelligent and technologically advanced,
the more short-term question of
if we get some spectroscopic data from an exoplanet,
so we know a little bit about what is in its atmosphere,
how can we judge whether or not that atmosphere
is giving us a signature of life existing?
That's a very hard question
that people are debating about.
I mean,
one very simple,
but perhaps interesting approach is to say,
small molecules don't tell you anything
because even if life could make them,
something else could also make them.
But long molecules,
that's the kind of thing that life would produce.
So signs of complexity.
I don't know.
I just have this nervous feeling
that we won't be able to detect.
We'll show up to a planet,
there'll be a bunch of liquid on it.
We like dip,
we take a swim in the liquid.
and we won't be able to see the intelligence in it.
whether that intelligence looks like something like, you know, ants or we'll see movement,
perhaps strange movement, but we won't be able to see the intelligence in it or communicate with
it. I guess if we have nearly infinite amount of time to play with different ideas, we might be
able to, you know, I think, I mean, I'm, I'm in favor of this kind of humility, this intellectual
humility that we won't know because we should be prepared for surprises. But I do always keep
coming back to the idea that we all live in the same physical universe. And if, well, let's put
it this way. The development of our intelligence has certainly been connected to our ability to
manipulate the physical world around us. And so I would guess without a hundred percent credence by
any means, but my guess would be that in any advanced,
advanced kind of life would also have that capability. You know, both dolphins and
octopuses are potential counterexamples to that. But I think in the details, there would be enough
similarities that we would recognize it. I don't know how we got on this topic, but I think it was
from supermassive black holes. So if we return to black holes and talk about the holographic
principle more broadly, you have a recent paper on the topic. You've been thinking about the topic
in terms of rigorous research perspective and just as a popular book writer. So what is the
holographic principle? Well, it goes back to this question that we were talking about with the
information and how it gets out. In quantum mechanics, certainly, arguably even before
quantum mechanics comes along in classical statistical mechanics, there's a relationship
between information and entropy. Entropy is my favorite thing to talk about.
I've written books about and will continue to write books about. So Hawking tells us that black
holes have entropy. And it's a finite amount of entropy. It's not an infinite amount. But the
belief is, and now we're already getting quite speculative, the belief is that the entropy of
a black hole is the largest amount of entropy that you can have in a region of spacetime.
It's sort of the most densely packed that entropy can be. And what that means is there's sort of a
maximum amount of information.
That you can fit into that region of space, and you call it a black hole.
And interestingly, you might expect if I have a box, and I'm going to put information in it,
and I don't tell you how I'm going to put the information in, but I ask,
how does the information I can put in scale with the size of the box? You might think, well,
it goes as the volume of the box, because the information takes up some volume, and I
can only fit in a certain amount. And that is what you might guess for the black hole,
but it's not what the answer is. The answer is that
the black hole is the size of the box. And that's what you might guess for the black hole.
The maximum information as reflected in the black hole entropy scales as the area of the black holes
event horizon, not the volume inside. So people thought about that in both deep and superficial
ways for a long time. And they proposed what we now call the holographic principle, that the way
that spacetime and quantum gravity convey information or hold information is not different
bits. And that's what we now call the holographic principle. And that's what we now call the holographic
or qubits for quantum information at every point in space-time. It is something holographic,
which means it's sort of embedded in or located in or can be thought of as pertaining to one
dimension less of the three dimensions of space that we live in. So in the case of the black hole,
the event horizon is two-dimensional, embedded in a three-dimensional universe. And the holographic
principle would say all of the information contained in the black hole can be thought of
as living on the event horizon rather than in the interior of the black hole. I need to say one
more thing about that, which is that this was an idea. The idea I just told you was the original
holographic principle put forward by people like Gerard de Tuft and Leonard Susskind, super famous
physicist. Leonard Susskind was on my podcast and gave a great talk. He's very good at explaining
these things. Mindscape podcast. That's right. Yes. And you don't just have physicists on.
I don't. I love Mindscape. Oh, thank you very much.
Curiosity-driven. Yeah, ideas. Exploration of ideas.
People, yeah. But anyway, what I was trying to get at was Susskind and also at Tuft were a little
vague. They were a little hand-wavy about holography and what it meant. Where holography,
the idea that information is sort of encoded on a boundary, really came into its own was with
Juan Maldacena in the 1990s and the ADS-CFD correspondence, which we don't have to get into
that into any detail.
But it's a whole full-blown theory. It's two different theories. One theory in n dimensions
of spacetime without gravity, and another theory in n plus 1 dimensions of spacetime with gravity.
And the idea is that this n-dimensional theory is casting a hologram into the n plus 1 dimensional
universe to make it look like it has gravity. And that's holography with a vengeance. And that's
an enormous. It's an enormous source of interest for theoretical physicists these days.
How should we picture what impact that has, the fact that you can store all the information,
you can think of as all the information that goes into a black hole can be stored at the event
horizon?
Yeah, I mean, it's a good question. One of the things that quantum field theory indirectly
suggests is that there's not that much information in you and me compared to the volume of spacetime
we take up.
As far as quantum field theory is concerned, you and I are mostly empty space.
And so we are not information dense, right? The density of information in us or in a book or a CD
or whatever, computer RAM, is indeed encoded by volume. Like there's different bits located at
different points in space, but that density of information is super duper low. So we're just
like the speed of light or just like the Big Bang. For the information in a black hole, we are far
away in our everyday life. And so we're not that dense. We're not that dense. We're not that dense in our everyday experience from the regime where these questions become
relevant. So it's very far away from our intuition. We don't really know how to think about these
things. We can do the math, but we don't feel it in our bones.
So you can just write off that weird stuff happens in a black hole.
Well, we'd like to do better, but we're trying. I mean, that's why we have an information loss
puzzle, because we haven't completely solved it. So here's just one thing to keep in mind.
Once spacetime becomes flexible, which it does according to general relativity,
and you have quantum mechanics, which has fluctuations in virtual particles and things
like that, the very idea of a location in spacetime becomes a little bit fuzzy,
right? Because it's flexible, and quantum mechanics says you can't even pin it down.
So information can propagate in ways that you might not have expected. And that's easy to say,
and it's true, but we haven't yet come up with the right way to talk about it that is perfectly
rigorous.
It's crazy how dense with information,
black hole is. And then plus, like quantum mechanics starts to come into play. So,
you know, you almost want to romanticize the kind of interesting computation type
things that are going on inside the black hole.
You do, you do. But I will, I'll point out one other thing. It's information dense,
but it's also very, very high entropy. So a black hole is kind of like a very, very,
very specific random number, right? It takes a lot of digits to specify it,
but the digits don't tell you.
They don't give you anything useful to work on. So it takes a lot of information,
but it's not of a form that we can learn a lot from.
But hypothetically, I guess, as you mentioned, the information might be preserved,
the information that goes into a black hole, it doesn't get destroyed. So what does that mean
when the entropy is really high?
Well, the black hole, I said that the black hole is the highest density of information,
but it's not the highest amount of information.
Because the black hole can evaporate. And when it evaporates, and people have done the equations
for this, when it evaporates, the entropy that it turns into is actually higher than the entropy of
the black hole was, which is good because entropy is supposed to go up. But it's much more dilute,
right? It's spread across a huge volume of space-time. So in principle, all that you made
the black hole out of, the information that it took is still there, we think, in that information,
but it's scattered to the floor.
We just talked about the event horizon of a black hole. What's on the inside?
What's at the center of it?
No one's been there. So again, this is a theoretical prediction. But I'll say one
super crucial feature of the black holes that we know and love, the kind that Schwarzschild
first invented. There's a singularity, but it's not at the middle of the black hole.
Remember, space and time are parts of one unified space-time. The location
of the singularity in the black hole is not the middle of space, but our future.
It is a moment of time. It is like a big crunch. The Big Bang was an expansion from a singularity
in the past. Big crunch probably doesn't exist, but if it did, it would be a collapse to a
singularity in the future. That's what the interiors of black holes are like. You can be
fine in the interior, but things are becoming more and more crowded. Space-time is becoming
more and more warped, and eventually you hit a limit, and that's the singularity in your future.
Do you know what time is like on the inside of a black hole?
Time always ticks by at one second per second. That's all it can ever do. Time can tick by
for different people. And so you have things like the twin paradox, where two people initially are
the same age, one goes off near the speed of light and comes back. Now they're not. You can
even work out that the one who goes out and comes back will be younger because they did not take the
shortest distance path. But locally, as far as you and your wristwatch are concerned, time is not
funny. Your neurological signals in your brain and your heartbeat and your wristwatch, whatever's
happening to them, is happening to all of them at the same time. So time always seems to be ticking
along at the same rate. Well, if you fall into a black hole and then I'm an observer just watching
it, and then you come out once it evaporates a million years later, I guess you'd be exactly the
same age?
Have you aged at all?
You would be converted into photons. You would not be you anymore.
Right. So it's not at all possible that information is preserved exactly as it went in.
It depends on what you mean by preserved. It's there in the microscopic
configuration of the universe. It's exactly as if I took a regular book,
made a paper, and I burned it. The laws of physics say that all the information in the
book is still there in the heat and light and ashes. You're never going to get it. It's a
matter of practice.
But in principle, it's still there.
But what about the age of things from the observer perspective, from outside the black hole?
From outside the black hole, it doesn't matter because they're inside the black hole.
No. Okay. There's no way to escape the black hole except to let it evaporate.
To let it evaporate.
But also, by the way, just in relativity, special relativity,
forget about general relativity, it's enormously tempting to say, "Okay, here's what's happening
to me right now. I want to know what's happening far away right now." The whole point of relativity
is to say there's no such thing as right now when you're far away. And that is doubly true
for what's inside a black hole. So you're tempted to say, "Well, how fast is their
clock ticking, or how old are they now?" Not allowed to say that according to relativity.
Because space and time are treated the same, and so it doesn't even make sense.
What happens to time in the holographic principle?
As far as we know—
As far as we know, nothing dramatic happens. We're not anywhere close to being confident
that we know what's going on here yet. So there are good unanswered questions about
whether time is fundamental, whether time is emergent, whether it has something to do
with quantum entanglement, whether time really exists at all—different theories, different
proponents of different things. But there's nothing specifically about holography that
would make us change our opinions about time, whatever they happen to be.
Well, holography is fundamentally about—it's a question of space?
It really is, yeah.
Okay, so time is just like a—
Time just goes along for the ride, as far as we know, yeah.
So all the questions about time is just almost like separate questions, whether it's emergent
and all that kind of stuff.
Yeah, I mean, that might be a reflection of our ignorance right now, but yes.
If we figure out a lot, you know, millions of years from now about black holes, how surprised
would you be if they traveled back in time and told you everything you want to know about
black holes? How much—?
How much do you think there is still to know? And how mind-blowing would it be?
It does depend on what they would say. You know, I think that there are colleagues
of mine who think that we're pretty close to figuring out how information gets out of
black holes, how to quantize gravity, things like that. I'm more skeptical that we are
pretty close. I think that there's room for a bunch of surprises to come. So in that sense,
I suspect I would be surprised. The biggest and most interesting surprise to me would
be if quantum mechanics itself were somehow superseded by something better. As far as
I know, there's no empirical evidence-based reason to think that quantum mechanics is
not 100% correct. But it might not be. That's always possible. So—and there are, again,
respectable friends of mine who speculate about it. So that's—that's a good question.
So, that's something I would—that's the first thing I would want to know.
Oh, so like the black hole would be the most clear illustration—
Yeah, that's where it would show up.
—if there's something, it would show up there.
I mean, maybe. The point is that black holes are mysterious for various reasons. So, yeah,
if our best theory of the universe is wrong, that might help explain why.
But do you think it's possible we'll find something interesting like black holes sometimes
create new universes? Or black holes are a kind of portal through which we get to know
the world through space-time to another place or something like this? And then our whole
conception of what is the fabric of space-time changes completely because black holes, it's
like Swiss cheese type of situation.
Yeah, you know, that would be less surprising to me because I've already written papers
about that. We don't have, again, strong reason to think that the interior black hole leads
to another universe. But it is possible, and it's also very possible that that's true for
some black holes and not others.
This is stuff we don't know. It's easy to ask questions we don't know the answer to.
The problem is the questions that are easy to ask that we don't know the answer to are
super hard to answer.
Because these objects are very difficult to test and to explore for us.
The regimes are just very far away. So, either literally far away in space, but also in energy
or mass or time or whatever.
You've published a paper on the holographic principle, or that involves the holographic
principle. Can you explain the details of that?
Yeah, you know, I'm always interested in, since my first published paper, taking these
wild speculative ideas and trying to test them against data. And the problem is, when
you're dealing with wild speculative ideas, they're usually not well-defined enough to
make a prediction, right? Like, it's kind of, I know what's going to happen in some
cases, I don't know what's going to happen in other cases.
So we did the following thing. As I've already mentioned, the holographic principle, which
is meant to reflect the information contained in black holes, seems to be telling us that
information, there's less information, less stuff that can go on than you might naively
expect. So let's upgrade naively expect to predict using quantum field theory. Quantum
field theory is our best theory of fundamental physics right now. Unlike this holographic
black hole stuff, quantum field theory is entirely local. In every point of space, something
can go on.
You can add up all the different points in space, okay? Not holographic at all. So there's
a mismatch between the expectation for what is happening, even in empty space, in quantum
field theory versus what the holographic principle would predict.
How do you reconcile these two things? So there's one way of doing it that had been
suggested previously, which is to say that in the quantum field theory way of talking,
it implies there's a whole bunch more states, a whole bunch more ways the system could be
developed than there really are. I'll do a little bit of math, just because there might
be some people in the audience who like the math. If I draw two axes on a two-dimensional
geometry, like the surface of the table, right? You know that the whole point of it being
two-dimensional is I can draw two vectors that are perpendicular to each other. I can't
draw three vectors that are all perpendicular to each other, right? They need to overlap
a little bit. That's true for any numbers of dimensions. But I can't draw two vectors
that are all perpendicular to each other. I can ask, okay, how much do they have to overlap if I try to put more
vectors into a vector space than the dimensionality of the vector space? Can I make them almost
perpendicular to each other? And the mathematical answer is, as the number of dimensions gets
very, very large, you can fit a huge extra number of vectors in that are almost perpendicular
to each other. So in this case, what we're suggesting is the number of things that are
all perpendicular to each other.
The number of things that can happen in a region of space is correctly described by
holography. It is somewhat overcounted by quantum field theory, but that's because the
quantum field theory states are not exactly perpendicular to each other. I should have
mentioned that in quantum mechanics, states are given by vectors in some huge dimensional
vector space, very, very, very, very large dimensional vector space. So maybe the quantum
field theory states are not quite perpendicular to each other.
If that is true, that's a speculation already, but if that's true, how would you know? What
is the experimental deviation? And it would have been completely respectable if we had
gone through and made some guesses and found that there is no noticeable experimental difference
because, again, these things are in regimes very, very far away.
We stuck our necks out. We made some very, very specific guesses as to how this weird overlap of
neutrinos would show up in the equations of motion for particles like neutrinos. And then we made
predictions on how the neutrinos would behave on the basis of those wild guesses. And then we
compared them with data. And what we found is we're pretty close, but haven't yet reached the
detectability of the effect that we are predicting. In other words, well, basically one way of saying
what we predict is if a neutrino, and there's reasons why it's neutrinos, we can go into if
you want, but it's not that simple. We can go into it if you want, but it's not that simple.
It's not that interesting. The neutrino comes to us from across the universe, from some galaxy
very, very far away. There is a probability as it's traveling that it will dissolve into other
neutrinos because they're not really perpendicular to each other as vectors, as they would
ordinarily be in quantum field theory. And that means that if you look at neutrinos coming from
far enough away with high enough energies, they should disappear. Like if you see a whole bunch
of nearby neutrinos, but then further away, you should see fewer. And there is an experiment
called IceCube, which is this amazing testament to the ingenuity of human beings, where they go
to Antarctica, and they drill holes, and they put photo detectors on a string a mile deep in these
holes. And they basically use all of the ice in a cube. I don't know whether it's a mile or not,
but it's like a kilometer or something like that, some big region. That much ice is their detector.
And they're looking for flashes when a cosmic ray or a neutrino or whatever
hits an ice molecule, water molecule in the ice.
Makes sense.
Flashes in the ice.
Yes, they're looking for flashes in the ice.
But isn't there some crazy, I mean, what does the detector of that look like?
It's a bunch of strings, many, many, many strings with 360 degree photo detectors.
Yeah, that's really cool.
It's extremely cool. And they've done amazing work, and they find neutrinos.
So they're looking for neutrinos.
Yeah, so the whole point is most cosmic rays are protons. Why? Because protons exist,
and they're massive enough that you can accelerate them to very high energies. So high energy
cosmic rays tend to be protons. They also tend to hit the Earth's atmosphere and decay into other
particles. So neutrinos, on the other hand, punch right through, at least usually, right,
to a great extent. So not just Antarctica, but the whole Earth. Occasionally, a neutrino will
interact with a particle here on Earth. And this neutrino is going through your body all the time,
from the sun, from the universe, etc.
And so if you're patient enough, and you have a big enough part of the Antarctic ice sheet to look
at, the nice thing about ice is it's transparent. So you've built yourself, nature has built you a
neutrino detector. Ice cube does.
So why ice? So is it just because of the low noise, and you get to watch this thing, and it's. It's much more dense than air, but it's transparent.
So yeah, much more dense, so higher probability, and then it's transparency, and then it's also,
in the middle of nowhere, so you can, humans are great.
That's all you need. There's not that much ice, right? Yeah. So there's more ice in Antarctica
than anywhere else, right. So anyway, you can go, and you can get a plot from the ice cube
experiment, how many neutrinos there are that they've detected with very high energies. And
we predict, in our weird little holographic guessing game, that there should be a cutoff.
You should see neutrinos as you get to higher and higher energies, and then they should disappear.
If you look at the data, they're. Data gives out exactly where our cutoff is. That doesn't mean that our cutoff is right. It means
they lose the ability to do the experiment exactly where we predict the cutoff should be.
Oh boy. Okay. But why is there a limit?
Oh, just because there are fewer and fewer high-energy neutrinos. So there's a spectrum,
and it goes down, but what we're plotting here is number of neutrinos versus energy.
It's fading away, and they just get very, very few.
And you. We need the high-energy neutrinos for your prediction.
Our effect is a little bit bigger for higher energies. Yeah.
Got it. And that effect has to do with this almost perpendicular thing.
And let me just mention the name of Oliver Friedrich, who was a postdoc who led this.
He deserves the credit for doing this. I was a co-author and a collaborator. I did some work,
but he really gets the lion's share.
Thank you, Oliver. Thank you for pushing this wild science forward.
Just to speak to that, the meta process of it, how do you approach asking these. these big questions and trying to formulate as a paper, as an experiment that could make a prediction,
all that kind of stuff? What's your process?
There's a very interesting thing that happens once you're a theoretical physicist,
once you become trained. You're a graduate student, you've written some papers and whatever.
Suddenly, you are the world's expert in a really infinitesimally tiny area of knowledge, right?
And you know not that much about other areas.
There's an overwhelming temptation to just drill deep, right?
Just keep doing basically the thing.
Just keep doing the thing that you started doing.
But maybe that thing you started doing is not the most interesting thing
to the world or to you or whatever.
So you need to separately develop the capability of stepping back and going,
"Okay, now that I can write papers in that area,
now that I'm sort of trained enough in the general procedure,
what is the best match between my interests, my abilities, and what is actually interesting?"
And honestly, I've not been very good at that.
Over my career.
You know, I have my process traditionally was I was working in this general area of particle physics,
field theory, general relativity, cosmology.
And I would sort of try to take things other people were talking about
and ask myself whether or not it really fit together.
Like my two, so I guess I have three papers that I've ever written that I've done,
you know, I've done a lot of research on.
And I've done a lot of research on, you know, I've done a lot of research on, you know,
So in 1998, observations showed that not only is the universe expanding, but it's expanding
faster and faster.
So that's attributed to either Einstein's cosmological constant or some more complicated
form of dark energy, some mysterious thing that fills the universe.
And people were throwing around ideas about this dark energy stuff.
What could it be?
And so forth.
Most of the people throwing around these ideas were cosmologists.
They work on cosmology.
They think about the universe all at once.
I, you know, since I like to talk to people in different areas, I was sort of more familiar
than average with what a respectable working particle physicist would think about these
things.
And what I immediately thought was, you know, you guys are throwing around these theories.
These theories are wildly unnatural.
They're super finely tuned, like any particle physicist would just be embarrassed to be
talking about this.
But rather than just scoffing at them, I sat down and asked myself, OK, is there a respectable
version?
Is there a way to keep the particle physicists happy but also make the universe accelerate?
and i realized that there is some very specific set of models that is that is relatively natural
and guess what you can make a new experimental prediction on the basis of those and so i did
that people were very happy about that what was the thing that would make physicists happy
that would make sense of this uh fragile thing that people call dark energy so
the fact that dark energy pervades the whole universe and is slowly changing that should
immediately set off alarm bells because particle physics is a story of length scales and time
scales that are generally guess what small right particles are small they vibrate quickly and
you're telling me now i have a new field and its typical rate of change is once every billion years
right? Like that's just not natural. And indeed, you can formalize that and say, you know, look,
even if you wrote down a particle that evolved slowly over billions of years, if you let it
interact with other particles at all, that would make it move faster, its dynamics would be faster,
its mass would be higher, et cetera, et cetera. So there's a whole story. Things need to be robust,
and they all talk to each other in quantum field theory. So how do you stop that from happening?
and the answer is symmetry. You can impose a symmetry that protects your new field from
talking to any other fields. And this is good for two reasons. Number one, it can keep the dynamics
slow. So if you just, you can't tell me why it's slow, you just made that up, but at least it can
protect it from speeding up because it's not talking to any other particles. And the other
is, it makes it harder to detect. Naively, experiments looking for fifth forces or time
changes of fundamental constants of nature, like the charge of the electron, these experiments
should have been able to detect these dark energy fields. And I was able to propose a way to stop
that from happening. The detection. The detection, yeah. Because a symmetry could stop it from
interacting with all these other fields and therefore makes it harder to detect.
And just by luck, I realized, because it was actually based on my first ever paper,
there's one loophole. If you impose these symmetries, so you protect the dark energy
field from interacting with any other fields, there's one interaction that is still allowed,
that you can't rule out. And it is a very specific interaction between your dark energy
field and photons, which are very common. And it has the following effect. As a photon travels
through the dark energy, the photon has a polarization, up, down, left, right, whatever
it happens to be. And as it travels through the dark energy, that photon will rotate its
polarization. This is called birefringence. And you can kind of run the numbers and say,
because we're just making up this model.
But if you want to roughly fit the data,
you can predict how much polarization rotation
there should be, a couple of degrees, okay?
Not that much.
So that's very hard to detect.
People have been trying to do it.
Right now, literally, we're on the edge.
of either being able to detect it or rule it out
using the cosmic microwave background.
And there is just, you know, truth in advertising.
There is a claim on the market that it's been detected,
that it's there.
It's not very statistically significant.
If I were to bet, I think it would probably go away.
It's a very hard thing to observe.
But maybe as you get better and better data,
cleaner and cleaner analysis, it will persist
and we will have directly detected the dark energy.
So if we just take this tangent of dark energy,
people will sometimes bring up dark energy and dark matter
as an example of why physicists have lost it,
lost their mind.
We're just going to say that there is this field
that permeates everything.
It's unlike any other field and it's invisible.
And it helps us work out some of the math.
How do you respond to that kind of suggestion?
Well, two ways.
One way is those people would have had to say the same thing
when we discovered the planet Neptune.
Because it's exactly analogous.
Where we have a very good theory,
in that case, Newtonian gravity in the solar system.
We made predictions.
The predictions were slightly off
for the motion of the outer planets.
You found that you could explain that motion
by positing something very simple.
One more planet in a very, very particular place.
And you went and looked for it and there it was.
That was the first successful example
of finding dark matter in the universe.
It's a matter that we can't see.
Neptune was dark.
Yeah.
There's a difference between dark matter and dark energy, right?
Dark matter, as far as we are hypothesizing it,
is a particle of some sort.
It's just a particle that interacts with us very weakly.
So we know how much of it there is.
We know more or less where it is.
We know some of its properties.
We don't know specifically what it is.
But it's not. It's not anything fundamentally mysterious.
It's a particle.
Dark energy is a different story.
So dark energy is indeed uniformly spread throughout space
and has this very weird property
that it doesn't seem to evolve as far as we can tell.
It's the same amount of energy
in every cubic centimeter of space
from moment to moment in time.
That's why far and away,
the leading candidate for dark energy
is Einstein's cosmological constant.
The cosmological constant is strictly constant,
100% constant,
the data say it had better be 98% constant or better.
So 100% constant works, right?
And it's also very robust.
It's just there.
It's not doing anything.
It doesn't interact with any other particles.
It makes perfect sense.
Probably the dark energy is the cosmological constant.
The dark matter,
super important to emphasize here,
you know, it was hypothesized
at first in the 70s and 80s,
mostly to explain the rotation of galaxies.
Today, the evidence for dark matter
is both much better than it was in the 1980s
and from different sources.
It is mostly from observations
of the cosmic background radiation
or of large-scale structure.
So we have multiple independent lines of evidence,
also gravitational lensing and things like that,
many, many pieces of evidence
that say that dark matter is there.
And also that say that the effects of dark matter
are different than if we,
you know, modified gravity.
So that was my first answer to your question is
dark matter, we have a lot of evidence for.
But the other one is,
of course, we would love it
if it weren't dark matter.
Our vested interest is 100% aligned
with it being something more cool and interesting
than dark matter
because dark matter is just a particle.
That's the most boring thing in the world.
And it's non-uniformly distributed to space, dark matter?
Absolutely, yeah.
You can even see maps of it
that we've constructed from gravitational,
gravitational lensing.
So verifiable sort of clumps of dark matter
in the galaxy that explains stuff.
Bigger than the galaxy, sadly.
Like we think that in the galaxy,
dark matter is lumpy,
but it's just, it's weaker.
Its effects are weaker.
But on the scale of large-scale structure
and clusters of galaxies and things like that,
yes, we can show you where the dark matter is.
Could there be a super cool explanation
for dark matter that would be interesting
as opposed to just another particle
that sits there in clumps?
The super cool explanation,
would be modifying gravity
rather than inventing a new particle.
Sadly, that doesn't really work.
We've tried.
I've tried.
That's my third paper that was very successful.
I tried to unify dark matter and dark energy together.
That was my idea.
That was my aspiration, not even idea.
I tried to do it.
It failed even before we wrote the paper.
I realized that my idea did not help.
It helps.
It could possibly explain away the dark energy,
but it would not explain
the way of the dark matter.
And so I thought it was not that interesting, actually.
And then two different collaborators of mine said,
has anyone thought of this idea?
Like, they thought of exactly the same idea
completely independently of me.
I said, well, if three different people
found the same idea, maybe it is interesting.
And so we wrote the paper.
And yeah, it was very interesting.
People are very interested.
Can you describe this paper a little bit?
Like, it's just, it's fascinating
how much of a thing there is,
dark energy and dark matter,
and we don't quite understand it.
So what was your dive into exploring it?
How do you unify the two?
So here is what we know
about dark matter and dark energy.
They become important in regimes
where gravity is very, very, very weak.
That's kind of the opposite
from what you would expect
if you actually were modifying gravity.
Like, there's a rule of thumb
in quantum field theory, et cetera,
that new effects show up
when the effects are strong, right?
We understand weak fields.
We don't understand strong.
We don't understand strong fields.
But okay, maybe this is different, right?
So what do I mean by when gravity is weak?
The dark energy shows up
late in the history of the universe.
Early in the history of the universe,
the dark energy is irrelevant.
But remember, the density of dark energy
stays constant.
The density of matter and radiation go down.
So at early times,
the dark energy was completely irrelevant
compared to matter and radiation.
At late times, it becomes important.
That's also when the universe is dilute
and gravity is relatively weak.
Now think about galaxies, okay?
A galaxy is more dense in the middle,
less dense on the outside.
And there is a phenomenological fact about galaxies
that in the interior of galaxies,
you don't need dark matter.
That's not so surprising
because the density of stars and gas
is very high there
and the dark matter is just subdominant.
But there's generally a radius
inside of which you don't need dark matter
to fit the data,
outside of which you do need dark matter
to fit the data.
So that's, again, when gravity is weak, right?
So I asked myself,
of course we know in field theory,
new effects should show up
when fields are strong, not weak,
but let's throw that out of the window.
Can I write down a theory
where gravity alters when it is weak?
And we've already said what gravity is.
What is gravity?
It's the curvature of space-time.
So there are mathematical quantities
that measure the curvature of space-time.
And generally, you would say,
like I have an understanding,
Einstein's equation,
which I explain to the readers in the book,
relates the curvature of space-time
to matter and energy.
The more matter and energy,
the more curvature.
So I'm saying,
what if you add a new term in there
that says the less matter and energy,
the more curvature?
No reason to do that
except to fit the data, right?
So I tried to unify
the need for dark matter
and the need for dark energy.
That would be really cool
if that was the case.
Super cool, right?
It'd be the best.
It'd be great.
It didn't work.
It'd be really interesting
if gravity did something funky
when there's not much of it.
Almost like at the edges of it,
it gets noisy.
That was exactly the hope.
But the great thing about physics is
there are equations, right?
I mean, you can come up with the words
and you can wave your hands,
but then you've got to write down
the equations, and I did.
And I figured out that
it could help with the equations,
but if it helps with the dark energy,
the acceleration of the universe,
it doesn't help with dark matter at all.
Yeah.
It just sucks that at the scale of galaxies
and scale of solar systems,
the physics is kind of boring.
Yeah, it does.
I agree.
And again, that's why it is a little bit,
I tear my hair out
when people who are not physicists
accuse physicists, like you say,
of sort of losing the plot
because they need dark matter
and dark energy.
I don't want dark matter
and dark energy.
I want something much cooler than that.
I've tried.
But you've got to listen
to the equations and to the data.
You mentioned three papers.
Your first ever,
your first awesome paper ever,
and your second awesome paper ever.
Of course, you wrote many papers,
so you're being very harsh
on the others.
Well, by the way,
this is not awesomeness.
This is impact.
Impact.
Right?
There's no correlation
between awesomeness and impact.
Right.
Some of my best papers
fell without a speck.
The first paper was called
Limits on a Lorentz and Parity
Violating Modification
of Electromagnetism
or Electrodynamics.
So we figured out
how to violate Lorentz invariance,
which is the symmetry
underlying relativity.
And the important thing is
we figured out a way to do it
that didn't violate anything else
and was experimentally testable.
So people love that.
The second paper was called
Quintessence and the Rest of the World.
So quintessence is this dynamic
ENEMICAL DARK ENEMIES.
energy field. The rest of the world is because I was talking about how the quintessence field
would interact with other particles and fields and how to avoid the interactions you don't want.
And the third paper was called, is cosmic speed up due to gravitational physics,
something like that. So you see the common theme. I'm taking, you know, what we know,
the standard model of particle physics, general relativity, tweaking them in some way,
and then trying to fit the data. And trying to make it so it's experimentally validated.
Ideally, yes, that's right. That's the goal. You wrote the book, Something Deeply Hidden
on the Mysteries of Quantum Mechanics, and a new book coming out soon, part of that
Biggest Ideas in the Universe series we mentioned called Quanta and Fields. So that's focusing on
quantum mechanics. Big question first, biggest ideas in the universe. What to you is most beautiful?
Or perhaps most mysterious about quantum mechanics?
Quantum mechanics is a harder one. You know, I wrote a textbook on general relativity,
and I started it by saying general relativity is the most beautiful physical theory ever invented.
I will stand by that. It is less fundamental than quantum mechanics, but quantum mechanics
is a little more mysterious. So it's a little bit kludgy right now. You know, if you think about
how we teach quantum mechanics to our students, the Copenhagen interpretation, it's a,
god-awful mess. Like, no one's going to accuse that of being very beautiful. I'm a fan of the
many worlds interpretation of quantum mechanics, and that is very beautiful in the sense that
fewer ingredients, just one equation, and it could cover everything in the world.
It depends what you mean by beauty, but I think that the answer to your question is
quantum mechanics can start with extraordinarily austere, tiny ingredients, and in principle,
lead to the world, right?
That boggles my mind. It's much more comprehensive. General relativity is about
gravity, and that's great. Quantum mechanics is about everything and seems to be up to the task.
And so I don't know, is that beauty or not? But it's certainly impressive.
So both for the theory, the predictive power of the theory, and the fact that the theory
describes tiny things creating everything we see around us.
It's a monist theory. In classical mechanics, I have a particle here, a particle there,
and I describe them separately. I can tell you what this particle is doing, what that particle is
doing. In quantum mechanics, we have entanglement, right? As Einstein pointed out to us in 1935.
And what that means is there is a single state for these two particles. There's not one state
for this particle, one state for the other particle. And indeed, there's a single state
for the whole universe, called the wave function of the universe, if you want to call it that.
And it obeys one equation, and it is our job then to sort of
change the way we think about it. And so I think that's a great question. And I think that's a great
question. And I think
it's a great question. To carve it up, to figure out how to get tables and chairs and things like that out of it.
You mentioned the many worlds interpretation, and it is in fact beautiful. But it's one of your
more controversial things you stand behind. You've probably gotten a bunch of flack for it.
I'm a big boy. I can take it.
Well, can you first explain it, and then maybe speak to the flack you may have gotten?
Sure. You know, the classic experiment to explain quantum mechanics to people
is called the Stern-Gerlach experiment. You're measuring the spin of a particle,
okay? And in quantum mechanics, the spin is, you know, it's just a spin. It's the rate at which
something is rotating around in a very down-to-earth sense. The difference being is that
it's quantized. So for something like a single electron or a single neutron, it's either spinning
clockwise or counterclockwise. Those are the only two, let's put it this way, those are the only two
measurement outcomes you will ever get. There's no it's spinning faster or slower. It's either spinning
one direction or the other. That's it. Two choices, okay? According to the rules of quantum mechanics,
I can set up an electron, let's say, in a state where it is neither purely clockwise or
counterclockwise, but a superposition of both. And that's not just because we don't know the answer.
It's because it truly is both until we measure it. And then when we measure it,
we see one or the other. So this is the fundamental mystery of quantum mechanics,
is that how we describe the system when we're not looking at it is different from
what we see when we look at it. So what we teach our students in the Copenhagen way of thinking
is that the act of measuring the spin of the electron causes a radical change in the physical
state. It spontaneously collapses from being a superposition of clockwise and counterclockwise
to being one or the other. And you can tell me the probability that that happens, but that's all
you can tell me. And I can't be very specific about when it happens, what caused it to happen,
why it's happening, none of that. That's all called the measurement problem of quantum mechanics.
So many worlds just says, look, I just told you a minute ago that there's only one way
function for the whole universe. And that means that you can't take too seriously just describing
the electron. You have to include everything else in the universe. In particular, you clearly have
to interact with the electron in order to measure it. So whatever is interacting with the electron
should be included. And that's the problem. Include it in the wave function that you're describing. And look, maybe it's just you. Maybe
your eyeballs are able to perceive it, but okay, I'm going to include you in the wave function.
And if you do that, let's be, you know, since you have a very sophisticated listenership,
I'll be a little bit more careful than average. What does it mean to measure the spin of the
electron? We don't need to go into details, but we want the following thing to be true.
If the electron were in a state that was a hundred percent spinning clockwise,
then we want the measurement to tell us it was spinning clockwise. We want your brain to go,
yes, the electron was spinning clockwise, right? Likewise, if it was a hundred percent
counterclockwise, we want to see that, to measure that. The rules of quantum mechanics,
the Schrodinger equation of quantum mechanics is a hundred percent clear that if you want to
measure it clockwise when it's clockwise and measure it counterclockwise when it's
counterclockwise, what will happen is that you and the electron will entangle with each other.
And by that, I mean that the state of the universe evolves into part saying the electron was spinning
clockwise and I saw it clockwise. And part of the state is it's in a superposition with
the part that says the electron was spinning counterclockwise and I saw it counterclockwise.
Everyone agrees with this entirely uncontroversial, straightforward consequence of the
Schrodinger equation.
And then Niels Bohr would say, and then part of that wave function disappears
and we're in the other part. And you can't predict which part it will be, only the probability.
Hugh Everett, who was a graduate student in the 1950s, was thinking about this,
says, I have a better idea. Part of the wave function does not magically disappear. It
stays there. The reason why that idea, Everett's idea that the whole wave function always sticks
around and just obeys the Schrodinger equation was not thought of years before.
Is because naively, you look at it and you go, okay, this is predicting that I will be in a
superposition. That I will be in a superposition of having seen the electron be clockwise and
having seen it be counterclockwise. No experimenter has ever felt like they were in a superposition.
You always see an outcome, okay? Everett's move, which was kind of genius, was to say,
the problem is not the Schrodinger equation. The problem is you,
have misidentified yourself in the Schrodinger equation. You have said, oh, look, there's a
person who saw counterclockwise. There's a person who saw clockwise. I should be that superposition
of both. And Everett says, no, no, no, you're not. Because the part of the wave function
in which the spin was clockwise, once that exists, it is completely unaffected
by the part of the wave function that says the spin was counterclockwise. They are,
apart from each other, they are uninteracting. They have no influence. What happens in one part
has no influence in the other part. So Everett says the simple resolution is to identify yourself as
either the one who saw spin clockwise or the one who saw spin counterclockwise. There are now two
people. Once you've done that experiment, the Schrodinger equation doesn't have to be messed
with. All you have to do is locate yourself correctly in the wave function. That's many
worlds. The number of
worlds is very, very, very, very big. Where do those worlds fit? Where do they go?
The short answer is the worlds don't exist in space. Space exists separately in each world.
So, I mean, there's a technical answer to your question, which is Hilbert space,
the space of all possible quantum mechanical states. But physically, you know, we want
to put these worlds somewhere. That's just a wrong intuition that we have. There is no such thing as
the physical spatial location of the worlds, because space is inside the worlds.
One of the properties of this interpretation is that you can't travel from one world to the other.
That's right.
Which kind of makes you feel that they're existing separately.
They are existing separately and simultaneously.
And simultaneously.
Without locations in space.
Is it possible to visualize them existing without a location in space?
The real answer to that, the honest answer is the equation's predicted.
Yeah, yeah.
If you can't visualize it, so much worse for you.
The equations are crystal clear about what they're predicting.
Is there a way to get closer to understanding and visualizing the weirdness of the implications of this?
You know, I don't think it's that hard.
It wasn't that hard for me.
I don't mind the idea that when I make a quantum mechanical measurement, there is later on in the universe multiple descendants of my present self who got different answers for that measurement.
I can't interact with them.
Hilbert space, the space of all quantum wave functions was always big enough to include all of them.
I'm going to worry about the parts of the universe I can observe.
So let's put it this way.
Many worlds comes about by taking the Schrodinger equation seriously.
The Schrodinger equation was invented to fit the data, to fit the spectrum of different atoms and different, you know, emission and absorption experiments.
And it's perfectly legitimate to say, well, okay, you're taking the Schrodinger equation, you're extrapolating it.
You're trusting it, believing it beyond what we can observe.
I don't want to do that, right?
That's perfectly legit.
Except, okay, then what do you believe?
Come up with a better theory.
You're saying you don't believe the Schrodinger equation.
Tell me the equation that you believe in.
Turns out, and people have done that.
Turns out it's super hard to do that in a legitimate way that fits the data.
And many worlds is a really clean.
Absolutely.
The most austere, clean, no extra baggage theory of quantum mechanics.
So if it, in fact, is correct.
Isn't it the weirdest thing of anything we know?
Yes.
In fact, let me put it this way.
The single best reason, in my mind, to be skeptical about many worlds is not because it doesn't make sense or it doesn't fit the data or I don't know where the worlds are going or whatever.
It's because to make that extrapolation, to take seriously the equation that we know is correct in other regimes.
It requires new philosophy.
It requires a new way of thinking about identity, about probability, about prediction, a whole bunch of things.
And it's work to do that philosophy, and I've been doing it, and others have done it, and I think it's very, very doable.
But it's not straightforward.
It's not a simple extrapolation from what we already know.
It's a grand extrapolation very far away.
And if you just wanted to be sort of methodologically conservative.
And say, that's a step too far.
I don't want to buy it.
I'm sympathetic to that.
I think that you're just wimping out.
I think that you should have more courage.
But I get the impulse.
And there is, under many worlds, an arrow of time where if you rewind it back, there's going to be one initial state.
That's right.
All of quantum mechanics, all different versions require a kind of arrow of time.
It might be different in every context.
It might be different in every kind, but the quantum measurement process is irreversible.
You can measure something, it collapses.
You can't go backwards.
If someone tells you the outcome, if I say, I've measured an electron, its spin is clockwise, and they say, what was it before I measured it?
You know, there was some part of it that was clockwise, but you don't know how much, right?
And many worlds is no different.
But the nice thing is that the kind of arrow of time you need in many worlds is exactly the kind of arrow of time you need anyway.
For entropy and thermodynamics and so forth, you need a simple, low-entropy initial state.
That's what you need in both cases.
So if you actually look at, under many worlds, into the entire history of the universe, correct me if I'm wrong, but it looks very deterministic.
Yes.
In each moment, does the moment contain the memory of the entire history of the universe?
To you, does the moment contain the memory of everything that preceded it?
As far as we know.
So according to many worlds, the wave function of the universe, all the branches of the universe at once, all the worlds, does contain all the information.
Calling it a memory is a little bit dangerous, because it's not the same kind of memory that you and I have in our brains, because our memories rely on the arrow of time.
And the whole point of the Schrodinger equation or Newton's laws is they don't have an arrow of time built in.
They're reversible.
The state of the universe not only remembers where it came from, but also determines where it's going to go in a way that our memories don't do that.
But our memories, we can do a replay.
Can you do this?
We can, but the act of forming a memory increases the entropy of the universe.
It is an irreversible process also, right?
You can walk on a beach and leave your footprints there.
That's a record of your passing.
It will eventually be erased by the ever-increasing entropy of the universe.
But you can. Imperfectly replay it.
I guess, can we return, travel back in time imperfectly?
Oh, it depends on the level of precision you're trying to ask that question.
You know, the universe contains the information about where the universe was, but you and I don't.
We're nowhere close.
And it's, what, computationally very costly to try to consult the universe.
Well, it depends on, again, exactly what you're asking.
Like, there are some. There are some simple questions.
Like, what was the temperature of the universe 30 seconds after the Big Bang?
We can answer that, right?
That's kind of amazing that we can answer that to pretty high precision.
But if you want to know where every atom was, then no.
What to you is the Big Bang?
Why did it. Why?
Why did it happen?
We have no idea.
I think that that's a super important question that I can imagine making progress on.
But right now, I'm more or less maximally uncertain about what the answer is.
You think black holes will help?
No.
Potentially?
Not that much.
Quantum gravity will help, and maybe black holes will help us figure out quantum gravity, so indirectly, yes.
But we have the situation where general relativity, Einstein's theory, unambiguously predicts there was a singularity in the past.
There was a moment of time when the universe had infinite curvature, infinite energy, infinite acceleration.
There was an expansion rate, the whole bit.
That's just a fancy way of saying the theory has broken down, and classical general relativity is not up to the task of saying what really happened at that moment.
So it is completely possible there was, in some sense, a moment of time before which there were no other moments.
And that would be the Big Bang.
Even if it's not a classical general relativity kind of thing, even if quantum mechanics is involved, maybe that's what happened.
It's also completely possible there was time before that.
Space and time, and they evolved into our hot Big Bang by some procedure that we don't really understand.
And if time and space are emergent, then the before even starts getting real weird.
Well, I think that if there is a first moment of time, that would be very good evidence, or that would fit hand in glove with the idea that time is emergent.
If time is fundamental, then it tends to go forever, because it's fundamental.
Well, yeah.
I mean, the general formulation of this question is what's outside of it.
Well, what's outside of our universe?
So in time and in space.
I know it's a pothead question, Sean.
I understand.
I apologize.
Look, that's my life.
My life is asking pothead questions.
Some of them, the answer is, that's not the right way to think about it.
Okay.
But is it possible to think at all about what's outside our universe?
It's absolutely legit to ask questions, but you have to be comfortable with the possibility that the answer is there's no such thing as outside our universe.
That's absolutely on the table.
In fact, that is the simplest, most likely to be correct answer that we know of.
But it's the only thing in the universe that wouldn't have an outside.
Yeah.
If the universe is the totality of everything, it would not have an outside.
That's so weird to think that there's not an outside.
We want there to be.
We want there to be sort of a creator, a creative force that led to this.
And an outside, like this is our time.
We want there to be a town, and then there's a bigger world, and there's always a bigger world.
Because that is our experience.
That's the world we grew up in, right?
The universe doesn't need to obey those rules.
Such a weird thing.
When I was a kid, that used to keep me up at night.
Like, what if the universe had not existed?
Right.
It feels like a lot of pressure that if this is the only universe, and we're here, one of the few intelligent civilizations,
maybe the only one, it's the old theories that we're at the center of everything.
It just feels suspicious.
That's why Many Worlds is kind of exciting to me, because it's humbling in all the right kinds of ways.
It feels like infinity is the way this whole thing runs.
There's one pitfall that I'll just mention, because there's a move that is made in these theoretical edges of cosmology
that I think is a little bit mistaken, which is to say,
think about the universe on the basis
of imagining that I am a typical observer. This is called the principle of typicality or the
principle of mediocrity or even the Copernican principle. Nothing special about me. I'm just
typical in the universe. But then you draw some conclusions from this. And what you end up
realizing is you've been hilariously presumptuous because by saying I'm a typical observer in the
universe, you're saying typical observers in the universe are like me. And that is completely
unjustified by anything. So I'm not telling you what the right way to do it is, but these kinds
of questions that are not quite grounded in experimental verification or falsification are
ones you have to be very careful about. That to me is one of the most interesting questions.
It's in different ways to approach it, but like what's outside of this? How did the big mess
start? How do we get something from nothing? That's always the thing you're sneaking up to.
When you're studying all of these questions, you're always sneaking. That's where the black
hole and the unifying getting quantum gravity, all this kind of stuff. You're always sneaking
up to that question. Where did all of this come from? And I think that's probably an answerable
question. Right? No. It doesn't have to be. So you think there could be a turtle at the bottom
of this that refuses to reveal its identity? Yes.
I think that. Specifically the question, "Why is there something rather than nothing?"
does not have the kind of answer that we would ordinarily attribute to why questions.
Because the typical why questions are embedded in the universe. And when we answer them,
we take advantage of the features of the universe that we know and love. But the universe itself,
as far as we know, is not embedded in anything bigger or stronger, and therefore it can just be.
Do you think it's possible that the universe itself is not embedded in anything bigger or stronger, and therefore it can just be?
Do you think it's possible this whole place is simulated?
Sure.
It's a really interesting, dark, twisted video game we're all existing in.
You know, my own podcast listeners, Mindscape listeners,
tease me because they know from my AMA episodes that if you ever
start a question by asking, "Do you think it's possible that?" the answer's going to be yes.
That might not be the answer that you care about, but it's possible, sure, as long as you're not
you know, adding two even numbers together and getting an odd number.
When you say it's possible, there's a mathematically yes,
and then there's more of like intuitive?
Yeah. You want to know whether it's plausible. You want to know is there a
reasonable non-zero credence to attach to this. I don't think that there's any
philosophical knockout objection to the simulation hypothesis. I also think
that there's absolutely no reason to take it seriously.
Do you think humans will try to create one?
I guess that's how I always think about it. I've spent quite a bit of time
over the past few years, and a lot more recently, in virtual worlds,
and just am always captivated by the possibility of creating
higher and higher resolution worlds. As we'll talk a little bit about artificial intelligence,
sort of the advancement on the SORA front, you can automatically generate those worlds
and the possibility of existing in those automatically generated worlds is pretty
exciting. As long as there's a consistent physics quantum mechanics and general relativity that
governs the generation of those worlds. So it just seems like humans will for sure try to create this.
Yeah, I think they will create better and better simulations. I think
the philosopher David Chalmers has done what I consider to be a good job of
arguing that we should treat things that happen in virtual reality and in simulated realities as just
as real as the reality that we experience. I also think that as a practical matter,
people will realize how much harder it is to simulate a realistic world than we
naively believe. So this is not a my lifetime kind of worry.
Yeah, the practical matter of going from a sort of a prototype that's impressive
to a thing that governs everything. Similar question on this front is in AGI. Yeah, you said
that we're very far away from AGI. Yeah.
I want to eliminate the phrase AGI.
So basically, when you're analyzing large language models and seeing how far are they from whatever
AGI is, and we could talk about different notions of intelligence that we're not as close as kind of
some people in public view are talking about. So what's your intuition behind that?
My intuition is basically that artificial intelligence is different than human intelligence.
And so the mistake that is being made by focusing on AGI among those who do
is an artificial agent that as we can make them now or in the near future might be
way better than human beings at some things, way worse than human beings at other things.
And rather than trying to ask how close is it to being a human-like intelligence,
we should appreciate it for what its capabilities are. And that will both be more accurate and help
put it to work and protect us from the dangers better rather than always anthropomorphizing it.
I think the underlying idea there under the definition of AGI is that
the capabilities are extremely impressive. That's not a precise statement, but meaning-
No, I get that. I completely agree.
And then the underlying question where a lot of the debate is, is how impressive is it?
What are the limits of large language models? Can they really,
do things like common sense reasoning, how much do they really understand about the world?
Or are they just fancy mimicry machines? And where do you fall on that as to the limits
of large language models?
I don't think that there are many limits in principle. I'm a physicalist about consciousness
and awareness and things like that. I see no obstacle to, in principle, building an artificial
machine-
That is indistinguishable in thought and cognition from a human being.
But we're not trying to do that, right? What a large language model is trying to do
is to predict text. That's what it does. And it is leveraging the fact that we human beings,
for very good evolutionary biology reasons, attribute intentionality
and intelligence and agency to things that act like human beings. As I was driving here to get
to this podcast space, I was using Google Maps. And Google Maps was talking to me,
but I wanted to stop to get a cup of coffee. So I didn't do what Google Maps told me to do.
I went around a block that it didn't like. And so it gets annoyed, right? It says like,
"No, why are you doing?" It doesn't say exactly in this, but you know what I mean. It's like,
"No, turn left, turn left, and you turn right." It is impossible as a human being
not to feel a little bit sad that Google Maps is getting mad at you.
It's not. It's not even trying to. It's not a large language model. There's
no aspirations to intentionality, but we attribute that all the time. Dan Dennett,
the philosopher, wrote a very influential paper on the intentional stance, the fact that it's the
most natural thing in the world for we human beings to attribute more intentionality to
artificial things than are really there, which is not to say it can't be really there. But if you're
trying to be rational,
and clear thinking about this, the first step is to recognize our huge bias towards attributing
things below the surface to systems that are able to, at the surface level, act human.
So if that huge bias of intentionality is there in the data, in the human data, in the vast
landscape of human data that AI models, large language models, and video models in the future
are trained on,
don't you think that that intentionality will emerge
as fundamental to the behavior of these systems naturally?
Well, I don't think it will happen naturally. I think it could happen.
Again, I'm not against the principle, but again, the way that large language models came to be
and what they're optimized for is wildly different than the way that human beings
came to be and what they're optimized for. So I think we're missing
a chance to be much more clear-headed about what large language models
are by judging them against human beings, again, both in positive ways and negative ways.
Well, I think, sort of to push back on what they're optimized for,
it's different to describe how they're trained versus what they're optimized for.
So they're trained in this very trivial way of predicting text tokens. But you can describe what
they're optimized for and what the actual task in hand is, is to construct a world model, meaning an
understanding of the world. And that's where it starts getting closer to what humans are kind of
doing. We're just, in the case of large language models, know how the sausage is made, and we don't
know how it's made for us humans. But they're not optimized for that. They're optimized to
sound human. That's the fine-tuning. But the actual training is optimized for understanding,
creating a compressed representation of all the stuff that humans have created on the internet.
And the hope is,
that that gives you a deep understanding of the world.
Yeah. So that's why
I think that there's a set of hugely interesting questions to be asked about the ways in which
large language models actually do represent the world, because what is clear is that they're very
good at acting human. The open question in my mind is, is the easiest, most efficient, best way to
act human to do the same things that human beings do, or are there other ways? And I think that's
an open question. I just heard a talk by Melanie Mitchell at Santa Fe Institute, an artificial
intelligence researcher, and she told two stories about two different papers, one that someone else
wrote and one that her group is following up on, and they were modeling Othello. Othello, the game
with a little rectangular board, white and black squares. So the experiment was the following. They
fed a neural network the moves that were being made in the most symbolic form, like E5, just
means that, okay, you put a token down E5. So it gives a long string. It does this for millions of
games, right? Real legitimate games. And then it asks the question, the paper asks the question,
okay, you've trained it to tell what would be a legitimate next move from not a legitimate next
move. Did it in its brain, in its little large language model brain, I don't even know if it's
technically a large language model, but a deep learning network, did it come up with a representation
of the Othello board? Well,
how do you know? And so they construct a little probe network that they insert and ask it,
what is it doing right at this moment, right? And the answer is that the little probe network can
ask, would this be legitimate or is this token white or black or whatever? Things that in practice
would amount to it's invented the Othello board. And it found that the probe got the right answer,
not 100% of the time, but more than by chance.
Substantially more than by chance. So they said, there's some tentative evidence that this neural
network has discovered the Othello board just out of data, raw data, right? But then Melanie's group
asked the question, okay, are you sure that that understanding of the Othello board wasn't built
into your probe? And what they found was at least half of the improvement was built into the probe,
not all of it, right? And then they found that at least half of the improvement was built into the
probe, not all of it, right? And then they found that at least half of the improvement was built
And look, a Othello board is way simpler than the world. So that's why I just think it's an open
question whether or not the, I mean, it would be remarkable either way to learn that large language
models that are good at doing what we train them to do are good because they've built the same kind
of model of the world that we have in our minds, or that they're good despite not having that model.
Either one of these is an imagination.
I think I have some sort of intellectual humility about the whole thing because I was humbled by several stages in the machine learning development over the past 20 years. And I just would never have predicted that LLMs, the way they're trained, on the scale of data they're trained, would be as impressive as they are. And there, that's where intellectual humility steps in, where my
intuition would say something like with Melanie, where you need to be able to have very sort of concrete common sense reasoning, symbolic reasoning type things in a system in order for it to be very intelligent. But here, I'm so impressed by what it's capable to do, train on next token prediction, essentially. That's, I just, my conception of the nature of intelligence is just completely, not completely, but
humbled, I should say.
That's, I just, my conception of the nature of intelligence is just completely, not completely, but
could be then it's the scale of computation will keep increasing but perhaps it's a race between
efficiency and and uh scale there are constraints right you know there's a certain amount of energy
a certain amount of damage we can do to the environment before it does not worth it anymore
so yeah i think that's a new question in fact it's it's kind of frustrating because we get better and
better at doing things efficiently but we invent more things we want to do faster than we get good
at doing them efficiently so we're continuing to make things worse in various ways i mean that's
that's the dance of humanity where we're constantly creating better and better and better technologies
that are potentially causing a lot more harm and that includes for weapons includes ai used as
weapons that includes nuclear weapons of course which is surprising to me that we haven't destroyed
human civilization yet given how many nuclear warheads are out there look i'm with you between
nuclear and bio weapons uh it is a little bit surprising that we haven't caused enormous
devastation of course we did drop two atomic bombs on japan but compared to what could have happened
or could happen tomorrow it could be much worse yeah it does seem like there's a underlying
speaking of quantum fields there's like a like a like a field of goodness within the
the human heart that like in some kind of game theoretic way,
we create really powerful things that could destroy each other.
And there's greed and ego and all this kind of power hungry dictators that are
at play here in all the geopolitical landscape.
But we somehow always like don't go too far.
Yeah.
But that's exactly what you would say right before we went too far.
Right before we went too far.
And that's why we don't see aliens.
So you're,
like I mentioned,
associated with Santa Fe Institute.
I just would love to take a stroll down
the landscape of ideas explored there.
So they look at complexity in all kinds of ways.
What do you think about the emergence of complexity
from simple things interacting simply?
I think it's a fascinating topic.
I mean, that's why I'm thinking about these things these days
rather than the papers that I was describing to you before.
All of those papers I described to you before are guesses.
like, what if the laws of physics are different in the following way? And then you can work out
the consequences. At some point in my life, I said, like, what is the chance I'm going to guess
right? You know, Einstein guessed right, Steven Weinberg guessed right, but there's a very small
number of times that people guessed right. Whereas with this emergence of complexity from
simplicity, I really do think that we haven't understood the basics yet. I think we're still
kind of pre-paradigmatic. There've been some spectacular discoveries, people like Jeffrey
West at Santa Fe and others have really given us true insights into important systems, but still
there's a lot of the basics I think are not understood. And so searching for the general
principles is what I like to do. And I think it's absolutely possible that, I mean, to be a
think this is kind of a cliche i think the key is information and i think that what we see through
the history of the universe as you go from simple to more and more complex is really subsystems of
the universe figuring out how to use information to do whatever to survive or to to thrive or to
reproduce i mean that's that's the sort of fuel the leverage the resource that we have
for a while anyway until the heat death but uh that's where the complexity is really driven by
yeah but the mechanism of it what i mean you mentioned jeffrey west what what are interesting
inklings of progress in this realm and what are systems that interest you in terms of information
so i mean for me just as a as a fan of complexity uh just even looking at simple cellular automata
is always just a fascinating way to illustrate the emergence of complexity so for those of
the listeners who don't know viewers cellular automata come from in imagining a very simple
complex system and it's a very simple complex system and it's a very simple complex system
configuration for example a set of ones and zeros along a line and then you invent a rule that says
okay i'm going to evolve this in time and generally the simplest ones start with just
each block of three ones and zeros have a rule that they will determinously go to either one or
a zero and you can actually classify all the different possibilities a small number of possible
cellular automata of that form and what was discovered by various people including steven
some of these cellular automata have the feature that you start from almost nothing like zero zero
zero zero one zero zero zero zero and you let it rip and it becomes wildly complex okay so this is
very provocative very interesting it's also not how physics works at all because as we said
physics conserves information you can go forward or backwards these cellular automata do not
they're not reversible in any sense you've built in an arrow of
time you have a starting point and then you evolve so what i'm interested in is seeing how
in the real world with the real laws of physics and underlying reversibility but macroscopic
irreversibility from entropy in the arrow time etc how does that lead to complexity i think that
that's an answerable question i don't think that cellular automata are really helping us in that
one so what is in that what is the landscape of entropy in the universe look like well entropy is
you localize it's a property of systems not of parts of systems right um having said that we can
do approximate uh answers to the question the answer is black holes are huge in entropy most
of let's put it this way the whole observable universe that we're in had a certain amount of
entropy before stars and planets and black holes started to form 10 to the 88th i can even tell you
the number okay the single most observable universe in the universe is the black hole
the center of our galaxy has entropy 10 to the 90. single black hole center of our galaxy has more
entropy than the whole universe used to have not too long ago so most of the entropy in the universe
today is in the form of black holes okay that's fascinating first of all uh but second of all if
we take black holes away what are the different interesting perturbations and entropy across
space what what is uh would where do we earthlings fit into that the interesting thing to me is that
if you start with a system that is isolated from the rest of the universe and you start it
at low entropy there's almost a theorem that says if you're very very very low entropy
then you the system looks pretty simple because there's low entropy means there's only a small
number of ways that you can rearrange the parts to look like that so if there's not that many ways
the answer is going to look simple but it's also almost a theorem that says when you're at maximum
entropy the system is going to look simple because it's all smeared out if it had like
interesting structure then it would be complicated right so entropy in this isolated system only goes
up that's the second law of thermodynamics but complexity starts low goes up and then goes down
again sometimes people mistakenly think that complexity or life or whatever is fighting
against the second law of thermodynamics fighting against the increase of entropy that is
precisely the wrong way to think about it we are surfers riding the wave of increasing entropy we
rely on increasing entropy to survive that is part of what makes us special this table
maintains its stability mechanically by which i mean there's molecules there have forces on each
other and it holds up you and i aren't like that we maintain our stability dynamically by ingesting
fuel right food and water and air and so forth burning it increasing its entropy we are non-equilibrium
quasi-steady state systems we are using the fuel the universe gives us in the form of low entropy
energy to maintain our stability i just wonder what that mechanism of surfing looks like i mean
that's where first of all i mean one question to ask do you think it's possible to have a kind of
precise ways or clearly defined ways of measuring complexity i think it is and i think we don't
it's possible to have it i don't think we yet have it because you know in part because
complexity is not a univalent thing there's different ideas that go under the rubric of
complexity one version is just comal girl of complexity right if you have a configuration
or a string of numbers or whatever can you compress it so that you have a small program
that will output that that's comal growth complexity but that's the complexity of a string
of numbers okay it's not like the complexity of a problem right computational complexity the traveling
salesman problem or factoring large numbers that's a whole different kind of question that is also
about complexity so we don't have a sort of unified view of it do you think it's possible to have a
complexity of a physical system yeah in the same way we do entropy yeah you think that's a Sean
Carroll paper or what
we're working on various things my the the glib thing that i'm trying to work on right now with
with a student is complexogenesis how does complexity come to be if all the universe is
doing is moving from low entropy to high entropy it's a sexy name it's a good name yeah i like the
name i just gotta write the paper sometimes a name yeah arose by any other name uh what which
which uh in which context uh the the the birth of complexity are you most
interested well i think it comes in stages right so i think that if you go from the i'm a again a
physicist so biologists studying evolution will talk about you know how complexity evolves all
the time the complexity of the genome the complexity of our physiology right but they
take for granted that life already existed you know and and entropy is increasing and so forth
I want to go back to the beginning and say the early universe was simple and low entropy and
uh entropy increases with time and the universe sort of differentiates and becomes more complex
but that that statement which is indisputably true has different meanings because complexity
has different meanings so sort of the most basic primal version of complexity is is what you might
think of as configurational complexity that's what come all grow up gets at how much information do
you need to specify the configuration of the system then there's a whole nother step where
subsystems of the universe start burning fuel right so in many ways a planet and a star are
not that different in configurational complexity they're both spheres with density high at the
middle and getting less as you go out but there's something fundamentally different because the star
only survives as long as it has fuel right I mean then it turns into a brown door for a white door
for whatever but as a star as a main sequence star it is an out of equilibrium system but it's more
static right like if I spill the coffee mug and it falls in the process of falling it's out of
equilibrium but it's also changing all the time a specific kind of system is where it's looks sort
of macroscopically stationary like a star but underneath the hood it's burning fuel to beat
the band in order to maintain that stability so as stars form that that's a different kind
of complexity that comes to be then there's another kind of complexity that comes to be
roughly speaking at the origin of life because that's where you have information really being
gathered and utilized by subsystems of the universe and then arguably there's any number
of stages past that I mean one of the most obvious ones to me is we talk about simulation theory but
you and I run simulations in our heads they're just not that good but we imagine different
hypothetical Futures right bacteria don't do that so that's the kind of information processing that is
a form of complexity so I would like to understand all these stages and how they fit together yeah
imagination yeah mental time travel yeah the the things going on in my head when I'm imagining
worlds are are super compressed representations of those worlds but they get to the essence of them
and maybe it's possible with non-human computing type devices to do those kinds of simulations in
more and more compressed ways there's an argument to be made that literally what separates human
beings from other
species on Earth is our ability to imagine counterfactual hypothetical
futures yeah i mean that's one of the big features i don't know if everyone has their own favorite
little feature but that that's why i said there's an argument to be made i did a podcast episode on
it with adam bully it developed slowly i did different podcasts sorry to keep mentioning
podcast episodes i did but malcolm mciver who is an engineer at northwestern has a theory about
one of the major stages in evolution is when fish first climbed on the land and i mean of course
that is a major stage of evolution but in particular there's a cognitive shift because
when you're a fish swimming under the water the attenuation length of light in water is not that
long you can't see kilometers away you can see meters away and you're moving at meters per second
so all of the evolutionary optimization is make all of your decisions on a time scale of less
than a second when you see something new you have to make a rapid fire decision what to do about it
as soon as you climb onto land you can essentially see forever right you can see stars in the sky
so now a whole new mode of reasoning opens up where you see something far away and rather than
saying look up table i see this i react you can say okay i see that thing what if i did this what
if i did that what if i did something different and and that's you know the birth of imagination
eventually you've been critical on panpsychism yes you've been critical on panpsychism
you've noticed that right can you make the case for panpsychism and against it so panpsychism is
the idea that consciousness permeates all matter it's maybe it's uh the fundamental force or
a physics of the way of the fabric of the universe panpsychism thought everywhere consciousness
everywhere right it is what it's to a point of entertainment the idea frustrates you which sort
of is a fan of panpsychism
is wonderful to watch and you've had uh great episodes with with uh panpsychists that's your
podcast where you go at it i had david chalmers who's you know one of the world's great philosophers
and he is he is panpsychism curious yeah oh he's not he doesn't commit to anything but he's
certainly willing to entertain it philip goff who i've had and who's a great guy but he is devoted
to panpsychism in fact he is almost single-handedly responsible for the upsurge of interest in panpsychism
in the popular imagination and the argument for it is supposed to be that there is something
fundamentally uncapturable about conscious awareness by physical behavior of atoms and
molecules so the panpsychist will say look you can tell me maybe someday through advances of
neuroscience and what have you exactly what happens in your brain and how that translates
into thought and speech and action what you can't tell me
is what it is like to be me you can't tell me what i am experiencing when i see something that
is red or they taste something that is sweet you can tell me what neurons fire but you can't tell
me what i'm experiencing that first person inner subjective experience is simply not capturable
by physics and therefore this is an old argument of course but then therefore is supposed to be
something that is not contained within physics to account for that and i'm just going to call it
mind we don't know what it is yet we're going to call it mind and it has to be separate from
physics and then there's two ways to go if you if you if you buy that much you can either say
okay i'm going to be a dualist i'm going to believe that there's matter and mind and they
are separate from each other and they are interacting somehow or that's a little bit
complicated and sketchy as far as physics is going to go so i'm going to believe in mind but i'm going
to believe prior to matter i'm going to believe that mind comes first and that consciousness is
the fundamental aspect of reality and everything else including matter and physics comes from it
that would be at least as simple as physics comes first right now the physicalist such as myself
will say i don't have any problem explaining what it's like to be you or what you experience when
you see red it's a certain way of talking
about the atoms and the neurons etc that make up you just like the hardness or the brownness of
this table these are words that we attach to certain underlying configurations of ordinary
physical matter likewise sadness and redness or whatever are words that we attach to you to
describe what you're doing and when it comes to consciousness in general i'm very quick to say i
do not claim
to have any special insight on how consciousness works other than i see no reason to change the
laws of physics to account for it if you don't have to change the laws of physics where do you
think it emerges from is consciousness an illusion that's almost like a shorthand that we humans use
to describe a certain kind of feeling we have when interacting with the world or is there some
big leap that happens at some stage i almost never use the word illusion illusion means that there's
something that you're perceiving that is actually not there like an oasis in the desert is an illusion
it has no causal efficacy if you walk up to where the oasis is supposed to be you'll say you were
wrong about it being there that's different than something being emergent or non-fundamental but
also real like this table is real even though i know it's made of atoms that doesn't remove the
realness from the table i think the consciousness and free will and things like that are just as
real in tables and chairs oasis in the desert does have causal efficacy
in that in your thirst causal efficacy well it leads you to draw incorrect conclusions about
the world sure but imagining a thing can sometimes bring it to reality as we've seen and that has a
kind of a causal efficacy sure but your understanding of the world in a way that
gives you power over it and influence over it is decreased rather than increased by believing in
that oasis that is not true about consciousness or this table
you don't think you can uh increase the chance of a thing existing by imagining imagining it existing
unless you build it or make it no that's what i mean like imagining humans can fly if you're
imagining that humans are flying right in terms of counterfactuals in the future absolutely
imagination is crucially important but that's not an illusion that's just a oh okay so the
possibility of the future versus what reality is i mean the future is a concept so you can
time time time is just a concept so you can play with that but yes reality um so to you so for
example i have to love asking this so donald hoffman um thinks that
the entire idea of the conversation we've been having about spacetime is an illusion is it possible
for you to steel man the case for that can you make the case for and against reality as i think
uh he writes that um the laws of physics as we know them with spacetime is a kind of interface
to a much deeper thing that we don't at all understand and that we're fooling ourselves
by constructing this world well i think there's like part of that idea that is perfectly respectable and
part of it that is perfectly nonsensical and i'm not even going to try to steel man the nonsensical
part the real part to me is is what is called structural realism so we don't know what the
world is at a deep fundamental level right let's put ourselves in the in the minds of people living
200 years ago like they didn't know about quantum mechanics they didn't know about relativity
that doesn't mean they were wrong about the universe that they understood they had newton's
laws right they could predict what time the sun was going to rise perfectly well in the progress
of science the words that would be used to give the most fundamental description
of how you were predicting the sun would rise changed because you now you have curved spacetime
and things like that right and you didn't have any of those words 200 years ago but the prediction
is the same why because that prediction independent of what we thought the fundamental ontology
was the prediction pointed to something true about our understanding of reality to call it
an illusion is just wrong i think we might not know what the best most comprehensive way of
stating it is but it's still true is it true in the way for example belief in god is true
because for most of human history people have believed in a god or multiple gods and that
seemed very true to them uh as an explanation for the way the world is uh some of the deeper
questions about life itself with the human condition and why certain things happen that
was a good explainer um so do you that's not an illusion no i think that was completely an illusion
i think it's a very very reasonable illusion to be under there are illusions there are you know
substantive claims about the world and i think that's a very very reasonable illusion to be
the world, that go beyond. predictions that we can make and verify, which later turned out to be wrong. And the existence
of God was one of them. If those people at that time had abandoned their belief in God and replaced
it with a mechanistic universe, they would have done just as well at understanding things, right?
Again, because there are so many things they didn't understand, it was very reasonable for
them to have that belief. It wasn't that they were dummies or anything like that.
But that is, as we understand the universe better and better, some things stick with us,
some things get replaced. So like you said, you're a believer of the mechanistic universe.
You're a naturalist, and as you've described, a poetic naturalist. That's right. What's the word
poetic? What is naturalism and what is poetic naturalism? Naturalism is just the idea that
all that exists is the natural world. There's no supernatural world. You can have artificial
arguments about what that means, but I would claim that the argument should be about what
the word supernatural means, not the word natural. The natural world is the world that we learn about
by doing science. The poetic part means that you shouldn't be too, I want to say, fundamentalist
about what the natural world is. As we went from Newtonian space-time to Einsteinian space-time,
something is maintained there. There is a difference.
There is a different story that we can tell about the world. And that story in the Newtonian regime,
if you want to fly a rocket to the moon, you don't use general relativity. You use Newtonian
mechanics. That story works perfectly well. The poetic aspect of the story is that there are many
ways of talking about the natural world. And as long as those ways latch on to something real and
causally efficacious about the functioning of the world, then we attribute some reality and truth
to them. So the poetic really looks at the
pothead questions at the edge of science. It's more open to them.
It's doing double duty a little bit. So that's why it's confusing. The more obvious respectable
duty it's doing is that tables are real. Even though you know that it's really a quantum field
theory wave function, right? Tables are still real. They're a different way of talking about
the underlying deeper reality of it. The other duty it's doing is that we move beyond purely
descriptive vocabulary. We move beyond purely descriptive vocabulary. We move beyond purely
tabularities for discussing the universe onto normative and prescriptive and judgmental ways of
talking about the universe. This painting is beautiful. That one is ugly. This action is
morally right. That one is morally wrong. These are also ways of talking about the universe. They
are not fixed by the phenomena. They are not determined by our observations. They cannot be
ruled out by a crucial experiment, but they're still valid. They might not be universal. They
might be subjective, but they're not arbitrary.
And they do have a role in describing how the world works.
So you don't think it's possible to construct experiments that explore
the realms of morality and even meaning? So those are just, those are subjective?
Yeah. They're human. They're personal.
But do you think that's just because we don't have a, the tools of science have not expanded
enough to incorporate the human experience? No, I don't think that's what it is. I think that
what we mean by,
or morality are, we're attaching categories, properties to things that happen in the
physical world. And there is always going to be some subjectivity to our attachment and how we
do that. And that's okay. And the faster we recognize that and deal with it, the better off
we'll be. But if we deeply and fully understand the functioning of the human mind, won't be able
to incorporate that? No. That will absolutely be helpful in explaining why certain people have
certain moral beliefs. It won't justify those beliefs. That's right or wrong.
Do you think it's possible to have a kind of general relativity, but that includes the observer
effect where the human mind is the observer? Sort of like how we morph in the same way gravity
morphs space-time, how does the human mind morph reality and have a very thorough theory
of how that morphing actually happens? That's a very pothead question, Lex.
I'm sorry.
We know you think it's possible.
The answer is yes. I think that we're part of the physical world and the natural world.
Physicalism would have been just as good a word to use as naturalism, maybe even a more accurate
word, but it's a little bit more off-putting. So I do want a snappier, more attractive label
than physicalism.
Are there limits to science?
Sure. We just talked about one, right? Science can't tell you right from wrong.
You need science to implement your ideas about right and wrong. If you are functioning on the
basis of an incorrect view of how the world works, you might very well think you're doing right,
but actually be doing wrong. But all the science in the world won't tell you which action is right
and which action is wrong. Dictators and people in power will sometimes use science as an authority
to convince you what's right and wrong. Studying Nazi science is fascinating.
Yeah.
But there's an instrumentalist view here. You have to first decide what your goals are,
and then science can help you achieve those goals. If your goals are horrible,
science has no problem helping you achieve them. Science is happy to help out.
Let me ask you about the method behind the madness on several aspects of your life.
So you mentioned your approach to writing for research and writing popular books.
How do you find the time of the day? Like, what's a day in the life of Sean Carroll?
Very unclear how I find the time.
So you don't have a thing where in the morning you're like, you try to fight for two hours
somewhere.
I don't. I'm really terrible at that. My strategy for finding time is just to ignore
interruptions in emails. But it's a different time every day. Some days it never happens.
Some weeks it never happens.
Well, you're able to pull it off because you're extremely prolific. So you're able to have days
where you don't write and still write the next day.
Right.
Oh, wow. That's a rare thing, right? A lot of prolific.
Prolific writers will carve out two hours because otherwise it just disappears.
Right. No, I get that. Yeah, I do. And yeah, it's just like, everyone has their foibles or whatever.
So I'm not able to do that. Therefore, I have to just figure it out on the fly.
And what's the actual process look like when you're writing popular stuff? You get behind
a computer?
Yeah, get behind a computer. And my way of doing it,
so my wife, Jennifer, is a science writer. But it's interesting because our techniques are
entirely different. She will think about something, but then she will free write.
She'll just sit at a computer and write. Like, I think this, I think this. And then that will be
vastly compressed, edited, rewritten or whatever until the final thing happens.
I will just sit there silently thinking for a very long time. And then I will write what is
almost the final draft. So a lot of it happens. There might be some scribbles for an outline or
something like that. But a lot of it is in my brain before it's on the page.
So that's the case for the biggest ideas in the universe,
the quanta book and the space-time motion book?
Yeah, quanta and fields, which is actually mostly about quantum field theory and particle physics.
That's coming out in May. And that is, I'm letting people in on things that no other book lets them
in on. So I hope it's worth it. It's a challenge because there's a lot of equations.
I mean, you did the same thing with space-time motion. You did something quite interesting,
which is-
It's like you made the equation the centerpiece of a book.
Right. There's a lot of equations. Book two goes further in those directions than book one did.
So it's more cool stuff. It's also more mind-bending. It's more of a challenge.
Book three that I'm writing right now is called Complexity and Emergence.
Oh, wow.
And that'll be the final part of the trilogy.
Oh, that's fascinating. So there's a lot of probably-
There's a lot of ideas there. I mean, that's a real cutting edge.
Well, but you know, I'm not trying to be cutting edge. In other words, I'm not trying to speculate
in these books. Obviously, in other books, I've been very free about speculating. But
the point of these books is to say things that 500 years from now will still be true.
And so there are some things we know about complexity and emergence, and I want to focus
on those. And I will mention, I'm happy to say, this is something that needs to be speculated
about, but I won't pretend to be telling you what one is the right one.
Yeah.
But you somehow found the balance between the rigor of mathematics and still accessible,
which is interesting.
I try. I mean, look, these three books, the Biggest Ideas books, are absolutely an experiment.
They're going to appeal to a smaller audience than other books will. But that audience should
love them. Like, my 16-year-old self would have been so happy to get these books, I can't tell you.
Yeah, in terms of looking back in history, those are books,
the trilogy would be truly special in that way.
Worked for Lord of the Rings.
So I figured, why not me?
You and Tolkien are just. Yeah.
Different styles, different topics.
Same ultimate reality.
Like we mentioned, Mindscape podcast, I love it. You interview a huge variety of experts
from all kinds of fields. So just several questions I want to ask. How do you prepare?
How do you prepare to have a good conversation? How do you prepare in a way that satisfies,
makes your own curious?
Makes your mind happy? All that kind of stuff.
Yeah, no, these are great questions. And I've sort of struggled and changed my techniques.
over the years. It's an over five-year-old podcast. It might be approaching six years old now.
I started out over-preparing when I first started. I had a journey that I was going to go down.
Many of the people I talked to are academics or thinkers who write books, so they have a story
to tell. I could just say, "Okay, give me your lecture," and then an hour later, stop.
The mistake is to anticipate what the lecture would be and to ask the leading questions that
would pull it out of them. What I do now is much more, "Here are the points. Here are the
big questions that I'm interested in," and so I have a much sketchier outline to start and then
try to make it more of a real conversation. I'm helped by the fact that it is not my day job,
so I strictly limit myself to one day of my life per podcast episode on average. Some days take more
time. That includes not just doing the research but inviting the guest, recording it, editing it,
publishing it. I need to be very, very efficient at that.
You enforce constraints for yourself in which creativity can emerge.
That's right. That's right. Look, sometimes if I'm interviewing a theoretical physicist,
I can just go in. When I'm interviewing an economist or a historian, I have to do a lot of
work. Do you ever find yourself
getting lost in rabbit holes that serve no purpose?
No purpose except satisfying your own curiosity and then potentially expanding
the range of things you know that can help your actual work and research and writing?
Yes, on both counts. Some people have so many things to talk about
that you don't know where to start or finish. Others have a message. One thing I discovered
over the course of these years is the correlation with age. There are brilliant people, and I try
very hard on the podcast to get all sorts of people, different ages and things like that,
and bless their hearts, the most brilliant young people are not as practiced at wandering past
their literal research. They have less mastery over the field as a whole,
much less how to talk about it, whereas certain older people just have their patent answers,
and that's kind of boring. So you want somewhere in between the ideal person who
is -- who has a lot of experience, has a lot of experience, has a lot of experience, has a lot of
experience, has a broad enough scope that they can wander outside their specific papers they've
written, but they're not overly practiced, so they're just giving you their canned answers.
I feel like there's like a connection to the metaphor of entropy and complexity, as you said
there.
Edge of chaos.
You also do incredible AMAs, and people should sign up to your Patreon
because you can get to ask questions, Sean Carroll. Well, for several hours, you just answer
in fascinating ways.
Yeah.
Yeah.
I think that's a good point.
I think that's a really interesting question. Is there something you could
say about the process of finding the answers to those?
That's a great one. Again, it's evolved over time. So the Ask Me Anything episodes were first,
when I started doing them, they were only for Patreon subscribers to both listen to and to ask
the questions. But then I actually asked my Patreon subscribers, "Would you like me to release
them publicly?" And they overwhelmingly voted yes. So I do that. So the Patreon supporters ask the
questions.
Everyone can listen. And also at some point, I really used to try to answer every question,
but now there's just too many. So I have to pick, and that's fraught with peril. And my personal
standard for picking questions to answer is what are the ones I think I have interesting answers
to give for, right? So that both means if it's kind of the same old question about special
relativity that I've gotten 100 times before, I'm not going to answer it because you can just Google
that. It's easier.
Yeah.
There are some very clear attempts to ask an interesting question that honestly,
just I don't have an answer to. Like, "I read this science fiction novel. What do you think
about it?" I'm like, "Well, I haven't read it, so I can't help you there." "What's your favorite
color?" I could tell you what it is, but it's not that interesting. And so I try to make it a mix.
I try to like, it's not all physics questions, not all philosophy questions. I will talk about
food or movies or politics or religion, if that's what people want. I keep suggesting that people
ask me for relationship advice, but they never do.
Yeah. I don't think I've heard one.
Yeah. I'm willing to do it, but I'm a little reluctant because I don't actually like giving
advice, but I'm happy to talk about those topics. I want to give several hours of talking, and I
want to try to say things that I haven't said before and keep it interesting, keep it rolling.
If you don't like this question,
wait for the next one.
What are some of the harder questions you've gotten? Do you remember? What kinds of
questions are difficult for you?
Rarely, but occasionally, people will ask me a super insightful philosophy question.
I hadn't thought of things in exactly that way, and I try to recognize that.
A lot of times, it's the opposite, where it's like, "Okay, you're clearly confused, and I'm going to
try to explain how the question is."
The question you should have asked.
Oh, I love those. Yeah, why that's the wrong question or that kind of stuff.
That's great.
Right.
That's great.
But the hard questions, I don't know. I don't actually answer personal questions very much.
The most personal I will get are questions like, "What do you think of Baltimore?" That much I can
talk about are, "How are your cats doing?" Happy to talk about the cats in infinite detail, but very
personal questions I don't get into.
But you even touch politics and stuff like this.
Yeah, no, very happy to talk about politics. I try to be clear on, "What is professional expertise? What is just me
babbling? What is my level of credence in different things? Where you're allowed to disagree, whether if you
disagree, you're just wrong?" And people can disagree with that also, but I do think, and I'm happy to go out on a
limb a little bit. I'm happy to say, "Look, I don't know, but here's my guess." I just did a whole solo podcast,
which was exactly that.
Yeah.
And it's interesting. Some people are like, "Oh, this was great." And there's a whole bunch of people are like,
"Why are you talking about this thing that you are not the world's expert in?"
Well, I love the actual dance between humility and having a strong opinion on stuff. It's a fascinating dance to pull off.
And I guess the way to do that is to just expand into all kinds of topics and play with ideas and then change your mind and all that kind of stuff.
Yeah, it's interesting because when people. react against you by saying you are being arrogant about this. 99.999% of the time,
all they mean is I disagree. That's all they really mean, right? You know, like at a very
basic level, people will accuse atheists of being arrogant. And I'm like, you think God exists and
loves you and you're telling me that I'm arrogant. I think that all of this is to say, just advice.
When you disagree with somebody, try to specify the substantive disagreement. Try not to
psychologize them, right? You know, try to say, oh, you're saying this because of this. Maybe it's
true. Maybe you're right. But if you had an actual response to what they were saying, that would be
much more interesting. Yeah, I think, I wonder why it's difficult for people to say or to imply
that they're arrogant. I mean, I think it's true. I think it's true. I think it's true. I think it's
true. I respect you. I like you. But I disagree on this. And here's why I disagree. Like, I wonder
why they go to this place of like, well, you're an idiot or you're egotistical or you're confused
or you're naive or you're, you know, all the kinds of words, as opposed to like, I respect you as a
and I disagree. I will complicate the question even more because there's some people I don't
respect or like. And I once wrote a blog post. I think it was called The Grid of Disputation.
And I had a two by two grid. And it's, are you someone I agree with or disagree with?
Are you someone who I respect or don't? Right? And all four quadrants are very populated. And
that, so what that means is there are people who I like,
and I disagree with. And there are people who agree with me. And I have no respect for it all.
The embarrassing allies quadrant. That was everyone's favorite. So, and I just think
being honest, right? Like trying to be honest about where people are. But if you actually
want to move a conversation forward, forget about whether you like or don't like somebody.
Explain the disagreement. Explain the agreement. But you're absolutely right. I completely agree.
As a society, we are not very good at disagreeing. We instantly go to the insults.
And I mean, even on the deeper level, I think at some deep level, I respect and love
the humanity in the other person.
Yep.
You said that general relativity is the most beautiful theory ever?
So far.
What do you find beautiful about it?
Let's put it this way. When I teach courses, there's no more satisfying,
subject to teach than general relativity. And the reason why is because it starts
from very clear, precisely articulated assumptions. And it goes so far, right? And when I give my talk,
you can find it online. I'm probably not going to give it again. The book, one of the biggest ideas
talk, right, was building up from you don't know any math or physics. An hour later, you know
Einstein's equation for general relativity. And the punchline is the equation is much smarter than
Albert Einstein. Because Albert Einstein did not know about the Big Bang. He didn't know about
gravitational waves. He didn't know about black holes, but his equation did. And that's, I mean,
that's a miraculous aspect of science more generally, but general relativity is where
it manifests itself in the most absolutely obvious way. A human question. What do you
think of the fact that Einstein didn't get the Nobel Prize for general relativity?
Tragedy. He should have gotten maybe four Nobel Prizes.
Honestly, that certainly should have got the photoelectric effect was 100% worth the Nobel
Prize because, and people don't quite get this. Who cares about the photoelectric effect? That's
like this very minor effect. The point is his explanation for the photoelectric effect
invented something called the photon. That's worth the Nobel Prize. Max Planck gets credit for this
in 1900, explaining blackbody radiation by saying that when a little electron is
jiggling in a object at some temperature, gives off radiation in discrete chunks rather than
continuously. He didn't quite say that's because radiation is discrete chunks, right? It's like
having a coffee maker that makes one cup of coffee at a time. It doesn't mean that liquid comes in
one cup quanta, right? It's just that you are dispensing it like that. It was Einstein in 1905
who said light is quanta, and that was a radical thing.
So that clearly, that was not a mistake. But also special relativity clearly deserved the Nobel
Prize, and general relativity clearly deserved the Nobel Prize. Not only were they brilliant,
but they were experimentally verified, like everything you want.
So separately, you think?
Yeah. Yeah, absolutely.
Oh, humans.
Yeah.
Whatever the explanation there.
Edwin Hubble never won the Nobel Prize for finding these universes was expanding.
Yeah. But even the fact that we give prizes is almost kind of silly,
and we limit the number.
The number of people that get the prize and all that.
I think the Nobel Prize has enormous problems. I think it's probably a net good for the world
because it brings attention to good science. I think it's probably a net negative for science
because it makes people want to win the Nobel Prize.
Yeah, there's a lot of fascinating human stories underneath it all. Science is its own thing,
but it's also a collection of humans, and it's a beautiful collection. There's tension,
there's competition.
There's jealousy. But there's also great collaborations and all that kind of stuff.
Daniel Kahneman, who recently passed, is one of the great stories of collaboration in science.
So all of it, all of it, that's what humans do. And Sean, thank you for being the person that makes
us celebrate science and fall in love with all of these beautiful ideas in science for writing
amazing books.
For being legit and still pushing forward the research science side of it. And for allowing me
and these pothead questions. And also for educating everybody through your own podcast.
Everybody should stop everything and subscribe and listen to every single episode of Mindscape.
So thank you. I've been a huge fan forever. I'm really honored that you would speak with me in
the early days when I was still starting this podcast. I'm really honored that you
early days when I was still starting this podcast in the world. I appreciate it. Thanks very much
for having me on now that you're a big deal, still having me on. Thank you, Sean.
Thanks for listening to this conversation with Sean Carroll. To support this podcast,
please check out our sponsors in the description. And now let me leave you with some words from
Richard Feynman. Study hard what interests you the most in the most undisciplined, irreverent,
and original manner possible. Thank you for listening and hope to see you next time.
Podcast Summary
Key Points:
Sean Carroll explains general relativity as gravity being the curvature of spacetime, building on Einstein’s insights and Minkowski’s space-time unification.
Einstein self-taught himself differential geometry to develop general relativity, demonstrating deep physical intuition despite lacking modern tools.
Black holes are regions of spacetime where escape is impossible, and their interiors contain singularities in time, not space, leading to a "big crunch" in the future.
The black hole information paradox remains unresolved
The holographic principle proposes that all information in a black hole is encoded on its event horizon, not in its interior, challenging traditional views of space and information.
Neutrino behavior in distant cosmic sources may reveal deviations from quantum field theory predictions, testing the holographic principle empirically.
Current observations of Hawking radiation are impossible due to black holes’ extreme coldness, making direct experimental validation unfeasible.
Sean emphasizes intellectual humility, noting that the true nature of time, information, and quantum gravity may still surprise us, especially in black hole physics.
Summary:
Sean Carroll, a leading theoretical physicist and science communicator, discusses key concepts in general relativity and quantum gravity, focusing on the nature of spacetime, black holes, and the information paradox. He explains that gravity arises from the curvature of spacetime, a breakthrough Einstein achieved through self-driven learning of advanced mathematics. Black holes are not solid objects but regions where escape is impossible, with their interiors ending in a future singularity—a moment of spacetime collapse.
The central mystery is whether information falling into a black hole is destroyed or preserved, a conflict between classical relativity and quantum mechanics. The holographic principle offers a radical solution: all information about a black hole is encoded on its event horizon, not within its volume, suggesting a deep connection between space, gravity, and information. Carroll highlights that while this idea is theoretically compelling, it remains unproven, with no direct experimental evidence—especially from Hawking radiation, which is too faint to detect.
He also touches on neutrino experiments like IceCube, which may one day reveal subtle deviations from quantum field theory, testing the holographic principle in extreme conditions. Ultimately, Carroll emphasizes the limits of human understanding, suggesting that black holes may hold profound revelations about the nature of time, information, and the universe—potentially even challenging quantum mechanics itself. His perspective blends deep physics with philosophical humility, underscoring that many of the most fundamental questions in science remain open and exciting.
FAQs
General relativity explains gravity as the curvature of spacetime caused by mass and energy. Instead of being a force acting at a distance, gravity is the result of objects moving along curved paths in spacetime, which appears as gravitational attraction.
The holographic principle suggests that all information within a black hole is encoded on its event horizon, a two-dimensional surface, rather than being stored in the three-dimensional interior. This implies that the maximum information capacity of a region of space scales with its surface area, not its volume.
Locally, time always ticks at one second per second, regardless of location. However, inside a black hole, time and space swap roles, and all future paths lead to the singularity. From an outside observer's view, time appears to slow down infinitely as an object approaches the event horizon.
According to the current understanding, information is not destroyed. While classical general relativity suggests it's lost, quantum mechanics implies it's preserved. The information is believed to be encoded in the Hawking radiation emitted by the black hole as it evaporates.
Currently, we cannot observe Hawking radiation directly. It is extremely weak and only detectable from tiny black holes, which are not known to exist nearby. Larger black holes, like those in our galaxy, emit radiation so faintly it is beyond current observational capabilities.
In general relativity, the singularity is not a point in space but a moment in time — a future endpoint. It represents a point where spacetime curves infinitely, and it lies in the future of any object falling into the black hole, not at a spatial center.
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