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Sean Carroll: Quantum Mechanics and the Many-Worlds Interpretation

Episode 2019-11-012019-11-01English

Guests: Sean Carroll

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§01Transcript · 00:00–18:41

00:00The following is a conversation with Sean Carroll, part two, the second time we've

00:04spoken on the podcast. You can get the link to the first time in the description.

00:09This time we focus on quantum mechanics and the many worlds interpretation that he details

00:15elegantly in his new book titled Something Deeply Hidden. I own and enjoy both the ebook

00:21and audiobook versions of it. Listening to Sean read about entanglement, complementarity,

00:28and the emergence of space-time reminds me of Bob Ross teaching the world how to paint

00:33on his old television show. If you don't know who Bob Ross is, you're truly missing out. Look him up,

00:40he'll make you fall in love with painting. Sean Carroll is the Bob Ross of theoretical physics.

00:47He's the author of several popular books, a host of a great podcast called Mindscape,

00:53and is a theoretical physicist at Caltech and the Santa Fe Institute, specializing in quantum

00:59mechanics, arrow of time, cosmology, and gravitation. This is the Artificial Intelligence Podcast.

01:06If you enjoy it, subscribe on YouTube, give it five stars on iTunes, support it on Patreon,

01:12or simply connect with me on Twitter @LexFriedman, spelled F-R-I-D-M-A-N.

01:18And now, here's my conversation with Sean Carroll. Isaac Newton developed what we now call

01:25classical mechanics that you describe very nicely in your new book, as you do with a lot of basic

01:30concepts in physics. So, with classical mechanics, I can throw a rock and can predict the trajectory

01:38of that rock's flight. But if we could put ourselves back into Newton's time, his theories

01:45work to predict things, but as I understand, he himself thought that their interpretations

01:52of those predictions were absurd. Perhaps he just said it for religious reasons and so on.

01:58But in particular, sort of a world of interaction without contact, so action at a distance,

02:05it didn't make sense to him on a sort of a human interpretation level. Does it make sense to you

02:11that things can affect other things at a distance?

02:14>> It does, but you know, so that was one of Newton's worries. You're actually right

02:20in a slightly different way about the religious worries. He was smart enough, this is off the

02:26topic but still fascinating, Newton almost invented chaos theory as soon as he invented

02:31classical mechanics. He realized that in the solar system, so he was able to explain how planets move

02:37around the sun, but typically you would describe the orbit of the Earth ignoring the effects of

02:43Jupiter and Saturn and so forth, just doing the Earth and the sun. He kind of knew, even though

02:48he couldn't do the math, that if you included the effects of Jupiter and Saturn, the other planets,

02:52the solar system would be unstable, like the orbits of the planets would get out of whack.

02:56So, he thought that God would intervene occasionally to sort of move the planets

03:00back into orbit, which is the only way you could explain how they were there presumably forever.

03:05But the worries about classical mechanics were a little bit different, the worry about gravity in

03:08particular. It wasn't a worry about classical mechanics, it was a worry about gravity.

03:12How in the world does the Earth know that there's something called the sun 93 million miles away

03:17that is exerting a gravitational force on it? And he literally said, "I leave that for future

03:22generations to think about because I don't know what the answer is." And in fact, people

03:28underemphasized this, but future generations figured it out. Pierre-Simone Laplace in circa

03:331800 showed that you could rewrite Newtonian gravity as a field theory. So, instead of just

03:39talking about the force due to gravity, you can talk about the gravitational field or the

03:44gravitational potential field. And then there's no action at a distance. It's exactly the same

03:48theory empirically, it makes exactly the same predictions. But what's happening is instead of

03:53the sun just reaching out across the void, there is a gravitational field in between the sun and

03:58the Earth that obeys an equation, Laplace's equation, cleverly enough. And that tells us

04:04exactly what the field does. So, even in Newtonian gravity, you don't need action at a distance.

04:09Now, what many people say is that Einstein solved this problem because he invented general relativity.

04:14And in general relativity, there's certainly a field in between the Earth and the sun. But also,

04:19there's the speed of light as a limit. In Laplace's theory, which was exactly Newton's theory, just in

04:24a different mathematical language, there could still be instantaneous action across the universe.

04:29Whereas in general relativity, if you shake something here, its gravitational impulse

04:34radiates out at the speed of light. And we call that a gravitational wave and we can detect those.

04:38It rubs me the wrong way to think that we should presume the answer should look one way or the

04:46other. Like if it turned out that there was action at a distance in physics, and that was the best

04:51way to describe things, then I would do it that way. It's actually a very deep question because

04:57when we don't know what the right laws of physics are, when we're guessing at them,

05:01when we're hypothesizing at what they might be, we are often guided by our intuitions about what

05:06they should be. I mean, Einstein famously was very guided by his intuitions. And he did not

05:11like the idea of action at a distance. We don't know whether he was right or not. It depends on

05:17your interpretation of quantum mechanics and it depends on even how you talk about quantum mechanics

05:22within any one interpretation. - So if you see every force as a field or any other interpretation

05:28of action at a distance, it's just stepping back to sort of caveman thinking. Like, do you really,

05:38can you really sort of understand what it means for a force to be a field that's everywhere?

05:45So if you look at gravity, like what do you think about-- - I think so.

05:48- Is this something that you've been conditioned by society to think that,

05:55to map the fact that science is extremely well predictive of something to believing that you

06:03actually understand it? Like you can intuitively, the degree that human beings can understand

06:11anything that you actually understand it. Are you just trusting the beauty and the power of the

06:16predictive power of science? - That depends on what you mean by this idea of truly understanding

06:24something, right? I mean, can I truly understand Fermat's last theorem? It's easy to state it,

06:30but do I really appreciate what it means for incredibly large numbers? I think yes,

06:37I think I do understand it. But like, if you want to just push people on, well, but your intuition

06:42doesn't go to the places where Andrew Wiles needed to go to prove Fermat's last theorem,

06:47then I can say fine, but I still think I understand the theorem. And likewise,

06:51I think that I do have a pretty good intuitive understanding of fields pervading space-time,

06:56whether it's the gravitational field or the electromagnetic field or whatever, the Higgs

07:00field. Of course, one's intuition gets worse and worse as you get trickier in the quantum field

07:08theory and all sorts of new phenomena that come up in quantum field theory. So our intuitions

07:13aren't perfect, but I think it's also okay to say that our intuitions get trained, right? Like,

07:18you know, I have different intuitions now than I had when I was a baby. That's okay. That's not,

07:22an intuition is not necessarily intrinsic to who we are. We can train it a little bit.

07:27- So that's where I'm gonna bring in Noam Chomsky for a second, who thinks that our

07:33cognitive abilities are sort of evolved through time. And so they're biologically constrained.

07:39And so there's a clear limit as he puts it to our cognitive abilities, and it's a very harsh limit.

07:46But you actually kind of said something interesting in nature versus nurture

07:51thing here is we can train our intuitions to sort of build up the cognitive muscles to be

07:57able to understand some of these tricky concepts. Do you think there's limits to our understanding

08:02that's deeply rooted, hard-coded into our biology that we can't overcome?

08:08- There could be limits to things like our ability to visualize, okay? But when someone

08:16like Ed Witten proves a theorem about, you know, 100 dimensional mathematical spaces,

08:21he's not visualizing it, he's doing the math. That doesn't stop him from understanding the result.

08:26I think, and I would love to understand this better, but my rough feeling,

08:31which is not very educated, is that, you know, there's some threshold that one crosses

08:36in abstraction when one becomes kind of like a Turing machine, right? One has the ability to

08:43contain in one's brain logical, formal, symbolic structures and manipulate them.

08:48And that's a leap that we can make as human beings that dogs and cats haven't made. And

08:55once you get there, I'm not sure that there are any limits to our ability to understand the

09:00scientific world at all. Maybe there are. There's certainly limits on our ability to calculate

09:06things, right? You know, people are not very good at taking cube roots of million digit numbers in

09:10their head, but that's not an element of understanding. It's certainly not a limit

09:14of principle. - So of course, as a human, you would say there doesn't feel to be limits to

09:19our understanding, but sort of, have you thought that the universe is actually a lot simpler than

09:29it appears to us and we just will never be able to, like it's outside of our, okay. So us, our

09:37cognitive abilities combined with our mathematical prowess and whatever kind of experimental

09:44simulation devices we can put together, is there limits to that? Is it possible there's limits to

09:52that? - Well, of course it's possible that there are limits to that. Is there any good reason to

09:58think that we're anywhere close to the limits is a harder question. Look, imagine asking this

10:04question 500 years ago to the world's greatest thinkers, right? Like are we approaching the

10:08limits of our ability to understand the natural world? And by definition, there are questions

10:14about the natural world that are most interesting to us that are the ones we don't quite yet

10:18understand, right? So there's always, we're always faced with these puzzles we don't yet know.

10:23And I don't know what they would have said 500 years ago, but they didn't even know about

10:26classical mechanics, much less quantum mechanics. So we know that they were nowhere close to how

10:31well they could do, right? They could do enormously better than they were doing at the time.

10:36I see no reason why the same thing isn't true for us today. So of all the worries that keep me awake

10:41at night, the human mind's inability to rationally comprehend the world is low on the list.

10:46- Well put. So one interesting philosophical point that quantum mechanics bring up is that

10:54you talk about the distinction between the world as it is and the world as we observe it.

11:01So staying at the human level for a second, how big is the gap between what our perception system

11:08allows us to see and the world as it is outside our mind's eye, sort of? Not at the quantum

11:16mechanical level, but as just these particular tools we have, which is the few senses and

11:23cognitive abilities to process those senses. - Well, that last phrase, having the cognitive

11:28abilities to process them, carries a lot, right? I mean, there is our sort of intuitive

11:34understanding of the world. You don't need to teach people about gravity for them to know

11:39that apples fall from trees, right? That's something that we figure out pretty quickly.

11:43Object permanence, things like that. The three-dimensionality of space, even if we don't

11:47have the mathematical language to say that, we kind of know that it's true. On the other hand,

11:53no one opens their eyes and sees atoms, right? Or molecules, or cells for that matter. Forget

11:58about quantum mechanics. But we got there. We got to understanding that there are atoms and cells

12:05using the combination of our senses and our cognitive capacities. So adding the ability

12:12of our cognitive capacities to our senses is adding an enormous amount. And I don't think

12:17it is a hard and fast boundary. If you believe in cells, if you believe that we understand those,

12:23then there's no reason you believe we can't believe in quantum mechanics just as well.

12:27- What to you is the most beautiful idea in physics?

12:32- Conservation of momentum. - Can you elaborate?

12:38- Yeah. If you were Aristotle, when Aristotle wrote his book on physics, he made the following

12:44very obvious point. We're on video here, right? So people can see this. So if I push the bottle,

12:48let me cover this bottle so we do not have a mess, but okay. So I push the bottle, it moves,

12:53and if I stop pushing, it stops moving. And this kind of thing is repeated a large number of times

12:59all over the place. If you don't keep pushing things, they stop moving. This is an indisputably

13:05true fact about our everyday environment, okay? And for Aristotle, this blew up into a whole

13:12picture of the world in which things had natures and teleologies, and they had places they wanted

13:17to be, and when you were pushing them, you were moving them away from where they wanted to be,

13:21and they would return and stuff like that. And it took 1,000 years or 1,500 years for people to

13:27say, "Actually, if it weren't for things like dissipation and air resistance and friction

13:34and so forth, the natural thing is for things to move forever in a straight line,

13:40there's a constant velocity, right? Conservation of momentum." And the reason why I think that's

13:47the most beautiful idea in physics is because it shifts us from a view of natures and teleology

13:55to a view of patterns in the world. So when you were Aristotle, you needed to talk a vocabulary of

14:03why is this happening, what's the purpose of it, what's the cause, et cetera, because it's nature

14:08does or does not want to do that. Whereas once you believe in conservation of momentum, things just

14:12happen. They just follow the pattern. You have Laplace's demon ultimately, right? You give me

14:18the state of the world today, I can predict what it's going to do in the future. I can predict

14:21where it was in the past. It's impersonal, and it's also instantaneous. It's not directed toward

14:27any future goals. It's just doing what it does given the current state of the universe. I think

14:32even more than either classical mechanics or quantum mechanics, that is the profound deep

14:37insight that gets modern science off the ground. You don't need natures and purposes and goals.

14:43You just need some patterns. >> So it's the first moment in our

14:48understanding of the way the universe works where you branch from the intuitive physical space to

14:55kind of the space of ideas. And also the other point you said, which is conveniently,

15:01most of the interesting ideas are acting in the moment. You don't need to know the history

15:07of time or the future. >> And of course, this took a long time to

15:11get there, right? I mean, the conservation of momentum itself took hundreds of years.

15:15It's weird because someone would say something interesting, and then the next interesting thing

15:19would be said like 150 or 200 years later, right? They weren't even talking to each other,

15:23they were just reading each other's books. And probably the first person to directly say that

15:27in outer space, in the vacuum, a projectile would move at a constant velocity was Avicenna,

15:34Ibn Sina in the Persian Golden Age, circa 1000. And he didn't like the idea. He used that,

15:40just like Schrodinger used Schrodinger's cat to say, surely you don't believe that, right?

15:44Ibn Sina was saying, surely you don't believe there really is a vacuum because if there was

15:48a really vacuum, things could keep moving forever, right? But still he got right the idea that there

15:54was this conservation of something, impetus or mile, he would call it. And that's 600 years before

16:01classical mechanics and Isaac Newton. So Galileo played a big role in this, but he didn't exactly

16:06get it right. And so it just takes a long time for this to sink in because it is so

16:11against our everyday experience. >> Do you think it was a big leap,

16:14a brave or a difficult leap of math and science to be able to say that momentum is conserved?

16:25>> I do. I think it's a example of human reason in action. Even Aristotle knew that his theory

16:33had issues because you could fire an arrow and it would go a long way before it stopped.

16:38So if his theory was things just automatically stop, what's going on? And he had this elaborate

16:43story. I don't know if you've heard this story, but the arrow would push the air in front of it

16:48away and the molecules of air would run around to the back of the arrow and push it again.

16:52And anyone reading this is going like, really, that's what you thought? But it was that kind

16:57of thought experiment that ultimately got people to say like, actually, no, if it weren't for the

17:01air molecules at all, the arrow would just go on by itself. And it's always this give and take

17:06between thought and experience back and forth, right? Theory and experiment, we would say today.

17:13>> Another big question that I think comes up certainly with quantum mechanics is what's the

17:20difference between math and physics to you? >> To me, very, very roughly. Math is about

17:28the logical structure of all possible worlds and physics is about our actual world.

17:32>> And it just feels like our actual world is a gray area when you start talking about

17:39interpretations of quantum mechanics or no. >> I'm certainly using the word world in the

17:45broadest sense, all of reality. So I think that reality is specific. I don't think that there's

17:51every possible thing going on in reality. I think that there are rules, whether it's the

17:55Schrodinger equation or whatever. So I think that there's a sensible notion of the set of

18:01all possible worlds and we live in one of them. The world that we're talking about might be a

18:05multiverse, might be many worlds of quantum mechanics, might be much bigger than the world

18:09of our everyday experience, but it's still one physically contiguous world in some sense.

18:13>> So if you look at the overlap of math and physics,

18:19it feels like when physics tries to reach for understanding of our world,

18:26it uses the tools of math to sort of reach beyond the limit of our current understanding.

18:34What do you make of that process of sort of using math to, so you start maybe with intuition or you

18:41might start with the math and then build up an intuition, but this kind of reaching into the

§02Transcript · 18:46–36:30

18:46darkness, into the mystery of the world with math? >> Well, I think I would put it a little

18:51bit differently. I think we have theories, theories of the physical world, which we then

18:57extrapolate and ask, what do we conclude if we take these seriously well beyond where we've

19:02actually tested them? It is separately true that math is really, really useful when we construct

19:08physical theories. And famously, Eugene Wigner asked about the unreasonable success of mathematics

19:13and physics. I think that's a little bit wrong because anything that could happen,

19:19any other theory of physics that wasn't the real world, but some other world,

19:23you could always describe it mathematically. It's just that it might be a mess.

19:28The surprising thing is not that math works, but that the math is so simple and easy that you can

19:33write it down on a t-shirt, right? I mean, that's what is amazing. That's an enormous

19:38compression of information that seems to be valid in the real world. So that's an interesting fact

19:45about our world, which maybe we could hope to explain or just take as a brute fact, I don't know.

19:50But once you have that, there's this indelible relationship between math and physics. But

19:57philosophically, I do want to separate them. We don't extrapolate math because there's a whole

20:02bunch of wrong math that doesn't apply to our world, right? We extrapolate the physical theory

20:07that we best think explains our world. >> Again, an unanswerable question.

20:12Why do you think our world is so easily compressible into beautiful equations?

20:19>> Yeah, I mean, like I just hinted at, I don't know if there's an answer to that question.

20:23There could be. >> What would an answer look like?

20:26>> Well, an answer could look like if you showed that there was something about our world

20:31that maximized something, the mean of the simplicity and the powerfulness of the laws

20:38of physics. Or maybe we're just generic. Maybe in the set of all possible worlds,

20:43this is what the world would look like, right? I don't really know. I tend to think not. I tend

20:48to think that there is something specific and rock bottom about the facts of our world that don't

20:54have further explanation. Like the fact that the world exists at all, and furthermore, the specific

20:59laws of physics that we have. I think that in some sense, we're just going to, at some level,

21:03we're going to say, and that's how it is. And we can't explain anything more. I don't know how,

21:08if we're anywhere close to that right now, but that seems plausible to me.

21:11>> And speaking of rock bottom, one of the things, sort of your book kind of reminded me or revealed

21:16to me is that what's fundamental and what's emergent, it just feels like I don't even know

21:23anymore what's fundamental in physics, if there's anything. It feels like everything, especially

21:30with quantum mechanics is revealing to us is that most interesting things that I would, as a limited

21:37human would think are fundamental, can actually be explained as emergent from the more deeper laws.

21:48>> I mean, we don't know, of course. You had to get that on the table. We don't know what

21:53is fundamental. We do have reason to say that certain things are more fundamental than others.

21:58Atoms and molecules are more fundamental than cells and organs. Quantum fields are more

22:04fundamental than atoms and molecules. We don't know if that ever bottoms out. I do think that

22:11there's sensible ways to think about this. If you describe something like this table as a table,

22:16it has a height and a width, and it's made of a certain material, and it has a certain solidity

22:20and weight and so forth. That's a very useful description as far as it goes. There's a whole

22:25another description of this table in terms of a whole collection of atoms strung together in

22:30certain ways. The language of the atoms is more comprehensive than the language of the table.

22:36You could break apart the table, smash it to pieces, still talk about it as atoms, but you

22:41could no longer talk about it as a table. So I think of this comprehensiveness, the domain of

22:46validity of a theory gets broader and broader as the theory gets more and more fundamental.

22:50>> So what do you think Newton would say, maybe right in a book review, if you read your latest

23:00book on quantum mechanics, something deeply hidden? >> It would take a long time for him to

23:05think that any of this was making any sense. >> You catch him up pretty quick in the beginning.

23:09>> Yeah. >> You give him a shout out in the beginning.

23:12>> That's right. I mean, he is the man. I'm happy to say that Newton was the greatest scientist who

23:17ever lived. I mean, he invented calculus in his spare time, which would have made him the greatest

23:21mathematician just all by himself, right? All by that one thing. But of course, it's funny because

23:28Newton was in some sense still a pre-modern thinker. Rocky Kolb, who is a cosmologist at

23:35the University of Chicago said that Galileo, even though he came before Newton, was a more modern

23:41thinker than Newton was. If you got Galileo and brought him to the present day, it would take him

23:46six months to catch up and then he'd be in your office telling you why your most recent paper was

23:49wrong. Whereas Newton just thought in this kind of more mystical way. He wrote a lot more about

23:57the Bible and alchemy than he ever did about physics. But he's also more brilliant than

24:02anybody else and way more mathematically astute than Galileo. So I really don't know. He might

24:09just, yeah, say like, give me the textbooks, leave me alone for a few months and then be caught up.

24:13Or he might have had mental blocks against seeing the world in this way. I really don't know.

24:20- Or perhaps find an interesting mystical interpretation of quantum mechanics.

24:24- Very possible, yeah.

24:25- Is there any other scientists or philosophers through history

24:29that you would like to know their opinion of your book?

24:33- That's a good question. I mean, Einstein is the obvious one, right? I mean,

24:38he was not that long ago, but I even speculate at the end of my book about what his opinion would be.

24:43I am curious as to what about older philosophers like Hume or Kant, right? What would they have

24:50thought? Or Aristotle, what would they have thought about modern physics? Because they do

24:56in philosophy, your predilections end up playing a much bigger role in your ultimate conclusions

25:02because you're not as tied down by what the data is. In physics, physics is lucky because we can't

25:08stray too far off the reservation as long as we're trying to explain the world that we actually see

25:13in our telescopes and microscopes. But it's just not fair to play that game because the people we're

25:19thinking about didn't know a whole bunch of things that we know, right? We lived through a lot that

25:25they didn't live through. So by the time we got them caught up, they'd be different people.

25:32- So let me ask a bunch of basic questions. I think it would be interesting, useful for people

25:38who are not familiar, but even for people who are extremely well familiar. Let's start with,

25:43what is quantum mechanics? - Quantum mechanics is the paradigm of physics that came into being in

25:51the early part of the 20th century that replaced classical mechanics. And it replaced classical

25:57mechanics in a weird way that we're still coming to terms with. So in classical mechanics,

26:01you have an object, it has a location, it has a velocity. And if you know the location and velocity

26:06of everything in the world, you can say what everything's going to do. Quantum mechanics

26:10has an aspect of it that is kind of on the same lines. There's something called the quantum state

26:16or the wave function. And there's an equation governing what the quantum state does. So it's

26:22very much like classical mechanics. The wave function is different. It's sort of a wave.

26:26It's a vector in a huge dimensional vector space rather than a position and a velocity. But okay,

26:31that's a detail. And the equation is the Schrodinger equation, not Newton's laws, but okay,

26:35again, a detail. Where quantum mechanics really becomes weird and different is that there's a

26:40whole nother set of rules in our textbook formulation of quantum mechanics, in addition

26:46to saying that there's a quantum state and it evolves in time. And all these new rules have

26:50to do with what happens when you look at the system, when you observe it, when you measure it.

26:54In classical mechanics, there were no rules about observing. You just look at it and you see what's

26:59going on. That was it, right? In quantum mechanics, the way we teach it, there's something profoundly

27:05fundamental about the act of measurement or observation. And the system dramatically changes

27:11its state, even though it has a wave function, like the electron in an atom is not orbiting in

27:16a circle, it's sort of spread out in a cloud. When you look at it, you don't see that cloud.

27:21When you look at it, it looks like a particle with a location. So it dramatically changes its

27:26state right away. And the effects of that change can be instantly seen in what the electron does

27:30next. So that's the, again, we need to be careful because we don't agree on what quantum mechanics

27:38says. So that's why I need to say like in the textbook view, et cetera, right? But in the

27:41textbook view, quantum mechanics, unlike any other theory of physics, gives a fundamental role to the

27:49act of measurement. >> So maybe even more basic, what is an atom and what is an electron?

27:56>> Sure. This all came together in a few years around the turn of the last century,

28:01right? Around the year 1900. Atoms predated then, of course, the word atom goes back to

28:07the ancient Greeks, but it was the chemists in the 1800s that really first got experimental

28:13evidence for atoms. They realized that there were two different types of tin oxide. And in these two

28:21different types of tin oxide, there was exactly twice as much oxygen in one type as the other.

28:26And like, why is that? Why is it never 1.5 times as much, right? And so Dalton said, well, it's

28:33because there are tin atoms and oxygen atoms. And one form of tin oxide is one atom of tin and one

28:40atom of oxygen, and the other is one atom of tin and two atoms of oxygen. And on the basis of this,

28:45so this is a speculation, a theory, right? A hypothesis. But then on the basis of that,

28:49you make other predictions. And the chemists became quickly convinced that atoms were real.

28:53The physicists took a lot longer to catch on, but eventually they did. And I mean, Boltzmann,

28:59who believed in atoms, had a really tough time his whole life because he worked in Germany,

29:05where atoms were not popular. They were popular in England, but not in Germany.

29:09- And there, in general, the idea of atoms is it's the smallest building block of the universe

29:16for them. That's the kind of how they thought of it.

29:18- That was the Greek idea, but the chemists in the 1800s jumped the gun a little bit. So these days,

29:23an atom is the smallest building block of a chemical element, right? Hydrogen, tin, oxygen,

29:29carbon, whatever. But we know that atoms can be broken up further than that. And that's what

29:34physicists discovered in the early 1900s, Rutherford especially, and his colleagues. So

29:41the atom that we think about now, the cartoon, is that picture you've always seen of a little nucleus

29:47and then electrons orbiting it like a little solar system. And we now know the nucleus is made of

29:51protons and neutrons. So the weight of the atom, the mass, is almost all in its nucleus. Protons

29:58and neutrons are something like 1800 times as heavy as electrons are. Electrons are much lighter,

30:04but because they're lighter, they give all the life to the atoms. So when atoms get together,

30:10combine chemically, when electricity flows through a system, it's all the electrons that are doing

30:14all the work. - And where quantum mechanics steps in,

30:18as you mentioned, with the position of velocity, with classical mechanics, and quantum mechanics

30:23is modeling the behavior of the electron. I mean, you can model the behavior of anything,

30:28but the electron, because that's where the fun is. - The electron was the biggest challenge,

30:33right from the start, yeah. - So what's the wave function? You said

30:36it's an interesting detail, but in any interpretation, what is the wave function

30:43in quantum mechanics? - Well, we had this idea from Rutherford

30:47that atoms look like little solar systems. But people very quickly realized that can't possibly

30:52be right, because if an electron is orbiting in a circle, it will give off light. All the light that

30:58we have in this room comes from electrons zooming up and down and wiggling, and that's what

31:01electromagnetic waves are. And you can calculate how long would it take for the electron just to

31:06spiral into the nucleus, and the answer is 10 to the minus 11 seconds, okay? 100 billionth of a

31:11second. So that's not right. Meanwhile, people had realized that light, which we understood from the

31:181800s was a wave, had properties that were similar to that of particles, right? This is Einstein and

31:24Planck and stuff like that. So if something that we agree was a wave had particle-like properties,

31:32then maybe something we think is a particle, the electron, has wave-like properties, right?

31:37And so a bunch of people eventually came to the conclusion, don't think about the electron as a

31:42little point particle orbiting like a solar system. Think of it as a wave that is spread out.

31:49They cleverly gave this the name the wave function, which is the dopiest name in the world

31:53for one of the most profound things in the universe. There's literally a number at every

31:59point in space, which is the value of the electron's wave function at that point.

32:04>>ANDREW: And there's only one wave function. >>BD: Yeah, they eventually figured that out.

32:09That took longer. But when you have two electrons, you do not have a wave function for electron one

32:15and a wave function for electron two. You have one combined wave function for both of them. And

32:20indeed, as you say, there's only one wave function for the entire universe at once.

32:24>>ANDREW: And that's where this beautiful dance, can you say what is entanglement?

32:31It seems one of the most fundamental ideas of quantum mechanics.

32:35>>BD: Well, let's temporarily buy into the textbook interpretation of quantum mechanics.

32:39And what that says is that this wave function, so it's very small outside the atom, very big

32:44in the atom. Basically the wave function, you take it and you square it, you square the number,

32:49that gives you the probability of observing the system at that location. So if you say that for

32:55two electrons, there's only one wave function, and that wave function gives you the probability

32:59of observing both electrons at once doing something. So maybe the electron can be here

33:04or here, here or here, and the other electron can also be there. But we have a wave function

33:09set up where we don't know where either electron is going to be seen, but we know they'll both be

33:14seen in the same place. So we don't know exactly what we're going to see for either electron,

33:20but there's entanglement between the two of them. There's a conditional statement. If we see one in

33:26one location, then we know the other one's going to be doing a certain thing. So that's a feature

33:30of quantum mechanics that is nowhere to be found in classical mechanics. In classical mechanics,

33:35there's no way I can say, "Well, I don't know where either one of these particles is, but if I

33:39find out where this one is, then I know where the other one is." That just never happens. They're

33:42truly separate. >> And in general, it feels like if you think of a wave function like as a dance floor,

33:47it seems like entanglement is strongest between things that are dancing together closest. So

33:53there's a closeness that's important. >> Well, that's another step. We have to be

33:58careful here because in principle, if you're talking about the entanglement of two electrons,

34:03for example, they can be totally entangled or totally unentangled no matter where they are in

34:09the universe. There's no relationship between the amount of entanglement and the distance between

34:14two electrons. But we now know that the reality of our best way of understanding the world is

34:20through quantum fields, not through particles. So even the electron, not just gravity and

34:25electromagnetism, but even the electron and the quarks and so forth are really vibrations in

34:31quantum fields. So even empty space is full of vibrating quantum fields. And those quantum

34:39fields in empty space are entangled with each other in exactly the way you just said. If they're

34:43nearby, if you have two vibrating quantum fields that are nearby, then they will be highly entangled.

34:48If they're far away, they will not be entangled. >> So what do quantum fields in a vacuum look like,

34:52empty space? >> Just like empty space,

34:54it's as empty as it can be. >> But there's still a field.

34:57What does nothing look like? >> Just like right here,

35:03this location in space, there's a gravitational field which I can detect by dropping something.

35:07I don't see it, but there it is. >> So we got a little bit of an idea of

35:15entanglement. Now, what is Hilbert space and Euclidean space?

35:23>> Yeah, I think that people are very welcome to go through their lives not knowing what Hilbert

35:28space is, but if you want to dig into a little bit more into quantum mechanics, it becomes necessary.

35:33You know, the English language was invented long before quantum mechanics or various forms of

35:39higher mathematics were invented. So we use the word space to mean different things. Of course,

35:45most of us think of space as this three-dimensional world in which we live, right? I mean, some of us

35:49just think of it as outer space. But space around us, it gives us the three-dimensional location of

35:55things and objects. But mathematicians use any generic abstract collection of elements as a

36:04space, a space of possibilities, momentum space, et cetera. So Hilbert space is the space of all

36:11possible quantum wave functions, either for the universe or for some specific system. And it could

36:16be an infinite dimensional space, or it could be just really, really large dimensional but finite.

36:21We don't know because we don't know the final theory of everything. But this abstract Hilbert

36:25space is really, really, really big and has no immediate connection to the three-dimensional

36:30space in which we live. >> What do dimensions in Hilbert space mean?

§03Transcript · 36:34–55:13

36:34>> You know, it's just a way of mathematically representing how much information is contained

36:39in the state of the system. How many numbers do you have to give me to specify what the thing is

36:45doing? So in classical mechanics, I give you the location of something by giving you three numbers,

36:51right? Up, down, left, X, Y, Z coordinates. But then I might want to give you its entire

36:57state, physical state, which means both its position and also its velocity.

37:02The velocity also has three components. So its state lives in something called phase space,

37:07which is six-dimensional, three dimensions of position, three dimensions of velocity.

37:11And then if it also has an orientation in space, that's another three dimensions and so forth. So

37:16as you describe more and more information about the system, you have an abstract mathematical space

37:23that has more and more numbers that you need to give. And each one of those numbers corresponds

37:27to a dimension in that space. >> So in terms of the amount of

37:31information, what is entropy? This mystical word that's overused in math and physics,

37:38but has a very specific meaning in this context. >> Sadly, it has more than one very specific

37:43meaning. This is the reason why it is hard. Entropy means different things even to different

37:48physicists. But one way of thinking about it is a measure of how much we don't know

37:53about the state of a system, right? So if I have a bottle of water molecules, and I know that,

37:59okay, there's a certain number of water molecules, I could weigh it, right, and figure out, I know

38:03the volume of it, and I know the temperature and pressure and things like that. I certainly don't

38:07know the exact position and velocity of every water molecule, right? So there's a certain amount

38:12of information I know, certain amount that I don't know that is part of the complete state of the

38:17system. And that's what the entropy characterizes, how much unknown information there is, the

38:23difference between what I do know about the system and its full exact microscopic state.

38:27>> So when we try to describe a quantum mechanical system, is it infinite or finite but very large?

38:36>> Yeah, we don't know. That depends on the system. You know, it's easy to mathematically

38:41write down a system that would have a potentially infinite entropy, an infinite dimensional Hilbert

38:46space. So let's go back a little bit. We said that the Hilbert space was the space in which

38:52quantum wave functions lived. For different systems, that will be different sizes. They

38:57could be infinite or finite. So that's the number of numbers, the number of pieces of information

39:02you could potentially give me about the system. So the bigger Hilbert space is, the bigger the

39:07entropy of that system could be, depending on what I know about it. If I don't know anything

39:12about it, then, you know, it has a huge entropy, right? But only up to the size of its Hilbert

39:17space. So we don't know in the real physical world whether or not, you know, this region of space

39:23that contains that water bottle has potentially an infinite entropy or just a finite entropy. We have

39:29different arguments on different sides. >> So if it's infinite, how do you think about

39:34infinity? Is this something you can, your cognitive abilities are able to process,

39:41or is it just a mathematical tool? >> It's somewhere in between, right? I mean,

39:45we can say things about it. We can use mathematical tools to manipulate infinity very,

39:50very accurately. We can define what we mean. You know, for any number n, there's a number bigger

39:55than it. So there's no biggest number, right? So there's something called the total number of all

39:59numbers, and it's infinite. But it is hard to wrap your brain around that. And I think that gives

40:04people pause because we talk about infinity as if it's a number, but it has plenty of properties

40:10that real numbers don't have. You know, if you multiply infinity by two, you get infinity again,

40:15right? That's a little bit different than what we're used to.

40:17>> Okay, but are you comfortable with the idea that in thinking of what the real world actually

40:25is, that infinity could be part of that world? Are you comfortable that a world in some dimension--

40:30>> I'm comfortable with lots of things. I mean, you know, I don't want my level of comfort to

40:37affect what I think about the world. You know, I'm pretty open-minded about what the world could

40:42be at a fundamental level. >> Yeah, but infinity is a tricky one. It's

40:47not almost a question of comfort. It's a question of is it an overreach of our intuition? Sort of,

40:57it could be a convenient, almost like when you add a constant to an equation just because it'll help.

41:03It just feels like it's useful to at least be able to imagine a concept, not directly,

41:08but in some kind of way that this feels like it's a description of the real world.

41:14>> Think of it this way. There's only three numbers that are simple. There's zero,

41:20there's one, and there's infinity. A number like 318 is just bizarre. You need a lot of bits to

41:30give me what that number is. But zero and one and infinity, like once you have 300 things,

41:35you might as well have infinity things, right? Otherwise, you have to say when to stop making

41:38the things, right? So there's a sense in which infinity is a very natural number of things to

41:44exist. >> I was never comfortable with infinity because it's just such a-- It was too good to be

41:49true because in math, it just helps make things work out. When things get very large, close to

41:59infinity, things seem to work out nicely. It's kind of like, because my deepest passion is

42:05probably psychology. And I'm uncomfortable how in the average, the beauty of how much we vary

42:17is lost. In that same kind of sense, infinity seems like a convenient way to erase the details.

42:23>> But the thing about infinity is it seems to pop up whether we like it or not, right? Like

42:29you're trying to be a computer scientist. You ask yourself, well, how long will it take this

42:33program to run? And you realize, well, for some of them, the answer is infinitely long. It's not

42:37because you tried to get there. You wrote a five-line computer program. It doesn't halt.

42:42>> So coming back to the textbook definition of quantum mechanics, this idea that I don't think

42:48we talked about, can you-- This one of the most interesting philosophical points we talked at

42:55the human level, but at the physics level, that at least the textbook definition of quantum mechanics

43:03separates what is observed and what is real. One, how does that make you feel? And two,

43:13what does it then mean to observe something, and why is it different than what is real?

43:19>> Yeah. My personal feeling, such as it is, is that things like measurement and observers and

43:28stuff like that are not going to play a fundamental role in the ultimate laws of physics. But my

43:33feeling that way is because so far, that's where all the evidence has been pointing. I could be

43:39wrong, and there's certainly a sense in which it would be infinitely cool if somehow observation

43:45or mental cogitation did play a fundamental role in the nature of reality. But I don't think so,

43:52and again, I don't see any evidence for it, so I'm not spending a lot of time worrying about

43:56that possibility. So what do you do about the fact that in the textbook interpretation of quantum

44:01mechanics, this idea of measurement or looking at things seems to play an important role?

44:07Well, you come up with better interpretations of quantum mechanics, and there are several

44:11alternatives. My favorite is the many worlds interpretation, which says two things. Number one,

44:17you, the observer, are just a quantum system like anything else. There's nothing special about you.

44:23Don't get so proud of yourself. You're just a bunch of atoms. You have a wave function. You

44:28obey the Schrodinger equation like everything else. And number two, when you think you're

44:33measuring something or observing something, what's really happening is you're becoming entangled

44:38with that thing. So when you think there's a wave function for the electron, it's all spread out,

44:43but you look at it and you only see it in one location. What's really happening is that there's

44:48still the wave function for the electron in all those locations, but now it's entangled

44:52with the wave function of you in the following way. There's part of the wave function that says

44:57the electron was here and you think you saw it there. The electron was there and you think you

45:01saw it there. The electron was over there and you think you saw it there, et cetera.

45:06And all of those different parts of the wave function, once they come into being,

45:09no longer talk to each other. They no longer interact or influence each other. It's as if

45:14they are separate worlds. So this was the invention of Hugh Everett III, who was a

45:19graduate student at Princeton in the 1950s. And he said, basically, look, you don't need all these

45:25extra rules about looking at things. Just listen to what the Schrodinger equation is telling you.

45:30It's telling you that you have a wave function, that you become entangled, and that the different

45:35versions of you no longer talk to each other. So just accept it. He did therapy more than anything

45:40else. He said, it's okay. You don't need all these extra rules. All you need to do is believe

45:45the Schrodinger equation. The cost is there's a whole bunch of extra worlds out there.

45:49>> So the world's being created whether there's an observer or not.

45:56>> The world's created anytime a quantum system that's in a superposition becomes

46:00entangled with the outside world. >> What's the outside world?

46:04>> It depends. Let's back up. Whatever it really says, what his theory is, is there's a wave

46:11function of the universe, and it obeys the Schrodinger equation all the time. That's it.

46:17That's the full theory right there. The question, all of the work is how in the world do you map

46:24that theory onto reality, onto what we observe? So part of it is carving up the wave function

46:31into these separate worlds, saying, look, it describes a whole bunch of things that don't

46:35interact with each other. Let's call them separate worlds. Another part is distinguishing between

46:39systems and their environments. And the environment is basically all the degrees of freedom, all the

46:44things going on in the world that you don't keep track of. So again, in the bottle of water,

46:50I might keep track of the total amount of water and the volume. I don't keep track of the individual

46:55positions and velocities. I don't keep track of all the photons or the air molecules in this room.

47:00So that's the outside world. The outside world is all the parts of the universe that you're not

47:05keeping track of when you're asking about the behavior of some subsystem of it.

47:08So how many worlds are there?

47:13Yeah, we don't know that one either. There could be an infinite number. There could be only a

47:19finite number, but it's a big number one way or the other.

47:21It's just a very, very big number. In one of the talks, somebody asked, well, if it's finite,

47:31so actually I'm not sure exactly the logic you used to derive this, but is there going to be

47:38overlap, a duplicate world that you return to? So you've mentioned, and I'd love if you can

47:49elaborate on sort of idea that it's possible that there's some kind of equilibrium that these

47:54splitting worlds arrive at. And then maybe over time, maybe somehow connected to entropy,

48:00you get a large number of worlds that are very similar to each other.

48:04Yeah. So this question of whether or not Hilbert space is finite or infinite dimensional is

48:11actually secretly connected to gravity and cosmology. This is the part that we're still

48:17struggling to understand right now, but we discovered back in 1998 that our universe is

48:21accelerating. And what that means if it continues, which we think it probably will,

48:25but we're not sure, but if it does, that means there's a horizon around us. Because the universe

48:31not only expanding, but expanding faster and faster, things can get so far away from us

48:36that from our perspective, it looks like they're moving away faster than the speed of light.

48:40We will never see them again. So there's literally a horizon around us and that horizon

48:45approaches some fixed distance away from us. And you can then argue that within that horizon,

48:51there's only a finite number of things that can possibly happen, the finite dimensional

48:55Hilbert space. In fact, we even have a guess for what the dimensionality is. It's 10 to the power

49:01of 10 to the power of 122. That's a very large number. Just to compare it, the age of the

49:07universe is something like 10 to the 14 seconds, 10 to the 17 or 18 seconds maybe. The number of

49:13particles in the universe is 10 to the 88th, but the number of dimensions of Hilbert space is 10

49:18to the 10 to the 122. So that's just crazy big. If that story is right, that in our observable

49:26horizon, there's only a finite dimensional Hilbert space, then this idea of branching

49:31of the wave function of the universe into multiple distinct separate branches has to reach a limit

49:36at some time. Once you branch that many times, you've run out of room in Hilbert space.

49:41And roughly speaking, that corresponds to the universe just expanding and emptying out and

49:46cooling off and entering a phase where it's just empty space literally forever.

49:51>> What's the difference between splitting and copying, do you think? A lot of this is

50:00an interpretation that helps us sort of model the world. So perhaps shouldn't be

50:10thought of as like, philosophically or metaphysically, but even at the physics level,

50:19do you see a difference between sort of generating new copies of the world or splitting?

50:26>> I think it's better to think of in quantum mechanics in many worlds, the universe splits

50:31rather than new copies because people otherwise worry about things like energy conservation.

50:35And no one who understands quantum mechanics worries about energy conservation because the

50:40equation is perfectly clear. But if all you know is that someone told you the universe duplicates,

50:44then you have a reasonable worry about where all the energy for that came from. So a pre-existing

50:50universe splitting into two skinnier universes is a better way of thinking about it. And

50:54mathematically, it's just like, if you draw an X and Y axis and you draw a vector of length one,

50:59a 45 degree angle, you know that you can write that vector of length one as the sum of two vectors

51:07pointing along X and Y of length one over the square root of two. So I write one arrow as the

51:13sum of two arrows, but there's a conservation of arrow-ness, right? Like there's now two arrows,

51:18but the length is the same. I just am describing it in a different way. And that's exactly what

51:22happens when the universe branches. The wave function of the universe is a big old vector.

51:26>> So to somebody who brings up a question of saying, doesn't this violate the conservation

51:33of energy? Can you give further elaboration? >> Right. So let's just be super duper perfectly

51:41clear. There's zero question about whether or not many worlds violate conservation of energy.

51:46It does not. And I say this definitively because there are other questions that I think there's

51:51answers to, but they're legitimate questions, right? About where does probability come from

51:55and things like that. This conservation of energy question, we know the answer to it. And the answer

52:00to it is that energy is conserved. All of the effort goes into how best to translate what the

52:06equation unambiguously says into plain English, right? So this idea that the universe comes

52:14equipped with a thickness and it sort of divides up into thinner pieces, but the total amount of

52:18universe is conserved over time is a reasonably good way of putting English words to the underlying

52:25mathematics. >> So one of my favorite things about many worlds is, I mean, I love that there's

52:32something controversial in science. And for some reason it makes people actually not like upset,

52:40but just get excited. Why do you think it is a controversial idea? So there's a lot of,

52:47it's actually one of the cleanest ways to think about quantum mechanics. So why do you think

52:53there's a discomfort a little bit amongst certain people? >> Well, I draw the distinction in my book

52:59between two different kinds of simplicity in a physical theory. There's simplicity

53:04in the theory itself, right? How we describe what's going on according to the theory by its own

53:09rights. But then, you know, theory is just some sort of abstract mathematical formalism. You have

53:13to map it onto the world somehow, right? And sometimes like for Newtonian physics, it's pretty

53:20obvious, like, okay, here is a bottle and it has a center of mass and things like that. Sometimes

53:26it's a little bit harder with general relativity, curvature of space-time is a little bit harder to

53:31grasp. Quantum mechanics is very hard to map what the language you're talking in of wave functions

53:38and things like that onto reality. And many worlds is the version of quantum mechanics where it is

53:43hardest to map on the underlying formalism to reality. So that's where the lack of simplicity

53:50comes in, not in the theory, but in how we use the theory to map onto reality. And in fact,

53:55all of the work in sort of elaborating many worlds quantum mechanics is in this effort to map it on

54:02to the world that we see. So it's perfectly legitimate to be bugged by that, right? To say,

54:08like, well, no, that's just too far away from my experience. I am therefore intrinsically skeptical

54:15of it. Of course, you should give up on that skepticism if there are no alternatives and this

54:19theory always keeps working, then eventually you should overcome your skepticism. But right now,

54:23there are alternatives that are, that, you know, people work to make alternatives that are by their

54:29nature closer to what we observe directly. - Can you describe the alternatives? I don't

54:33think we touched on it. So the Copenhagen interpretation and the many worlds, maybe

54:40there's a difference between the Everettian many worlds and many worlds as it is now, like has the

54:47idea sort of developed and so on. And just in general, what is the space of promising contenders?

54:54We have democratic debates now, there's a bunch of candidates. - 12 candidates.

54:57- 12 candidates on stage. What are the quantum mechanical candidates on stage for the debate?

55:02- So if you had a debate between quantum mechanical contenders, there'd be no problem

55:08getting 12 people up there on stage, but there would still be only three front runners.

55:13And right now the front runners would be Everett. Hidden variable theories are another one. So the

§04Transcript · 55:19–1:12:22

55:19hidden variable theories say that the wave function is real, but there's something in

55:24addition to the wave function. The wave function is not everything, it's part of reality, but it's

55:28not everything. What else is there? We're not sure, but in the simplest version of the theory,

55:34there are literally particles. So many worlds says that quantum systems are sometimes are

55:40wave-like in some ways and particle-like in another because they really, really are waves,

55:45but under certain observational circumstances, they look like particles. Whereas hidden variable

55:51says they look like waves and particles because there are both waves and particles involved in

55:56the dynamics. And that's easy to do if your particles are just non-relativistic Newtonian

56:03particles moving around, they get pushed around by the wave function roughly. It becomes much

56:08harder when you take quantum field theory or quantum gravity into account. The other big

56:13contender are spontaneous collapse theories. So in the conventional textbook interpretation, we say

56:20when you look at a quantum system, its wave function collapses and you see it in one location.

56:25A spontaneous collapse theory says that every particle has a chance per second of having its

56:34wave function spontaneously collapse. The chance is very small for a typical particle will take

56:38hundreds of millions of years before it happens even once, but in a table or some macroscopic

56:43object, there are way more than a hundred million particles and they're all entangled with each

56:47other. So when one of them collapses, it brings everything else along with it. There's a slight

56:53variation of this. That's a spontaneous collapse theory. There are also induced collapse theories

56:57like Roger Penrose thinks that when the gravitational difference between two parts of the

57:01wave function becomes too large, the wave function collapses automatically. So those are basically,

57:08in my mind, the three big alternatives. Many worlds, which is just there's a wave function

57:12and always obeys the Schrodinger equation. Hidden variables, there's a wave function that always

57:16obeys the Schrodinger equation, but there are also new variables. Or collapse theories, which

57:21the wave function sometimes obeys the Schrodinger equation and sometimes it collapses. So you can

57:26see that the alternatives are more complicated in their formalism than many worlds is, but they are

57:32closer to our experience. - So just this moment of collapse, do you think of it as a wave function,

57:40fundamentally, sort of a probabilistic description of the world? And is collapse sort of reducing

57:48that part of the world into something deterministic? Where again, you can now describe the position and

57:53the velocity in this simple classical model? Is that how you think about collapse?

57:58- There is a fourth category, there's a fourth contender, there's a Mayor Pete of

58:02quantum mechanical interpretations, which are called epistemic interpretations. And what they

58:08say is all the wave function is, is a way of making predictions for experimental outcomes. It's not

58:14mapping onto an element of reality in any real sense. And in fact, two different people might

58:20have two different wave functions for the same physical system because they know different things

58:24about it, right? The wave function is really just a prediction mechanism. And then the problem with

58:28those epistemic interpretations is if you say, okay, but it's predicting about what? Like what

58:35is the thing that is being predicted? And they say, no, no, no, that's not what we're here for.

58:41We're just here to tell you what the observational outcomes are going to be.

58:44- But the other interpretations kind of think that the wave function is real.

58:47- Yes, that's right. So that's an ontic interpretation of the wave function,

58:54ontology being the study of what is real, what exists, as opposed to an epistemic

58:58interpretation of the wave function, epistemology being the study of what we know.

59:01- I would actually just love to see that debate on stage.

59:05- There was a version of it on stage at the World Science Festival a few years ago

59:09that you can look up online.

59:11- On YouTube?

59:11- Yep, it's on YouTube.

59:12- Okay, awesome. I'll link it and watch it. Who won?

59:16- I won. I don't know, there was no vote. There was no vote. But Brian Green was the moderator,

59:25and David Albert stood up for spontaneous collapse, and Shelley Goldstein was there for

59:30hidden variables, and Rüdiger Schock was there for epistemic approaches.

59:33- Why do you, I think you mentioned it, but just to elaborate,

59:37why do you find many worlds so compelling?

59:40- Well, there's two reasons, actually. One is, like I said, it is the simplest, right? It's

59:45like the most bare-bones, austere, pure version of quantum mechanics. And I am someone who is very

59:52willing to put a lot of work into mapping the formalism onto reality. I'm less willing to

59:56complicate the formalism itself. But the other big reason is that there's something called modern

60:01physics, with quantum fields and quantum gravity and holography and space-time, doing things like

60:08that. And when you take any of the other versions of quantum theory, they bring along classical

60:14baggage. All of the other versions of quantum mechanics prejudice or privilege some version

60:21of classical reality, like locations in space, okay? And I think that that's a barrier to doing

60:29better at understanding the theory of everything, understanding quantum gravity and the emergence

60:32of space-time. Whenever, if you change your theory from, you know, here's a harmonic oscillator,

60:38oh, there's a spin, here's an electromagnetic field, in hidden variable theories or dynamical

60:43collapse theories, you have to start from scratch. You have to say like, well, what are the hidden

60:46variables for this theory or how does it collapse or whatever? Whereas many worlds is plug and play.

60:50You tell me the theory and I can give you as many worlds version. So when we have a situation like

60:55we have with gravity and space-time, where the classical description seems to break down in a

61:00dramatic way, then I think you should start from the most quantum theory that you have,

61:05which is really many worlds. >> So start with the quantum theory and try to

61:10build up a model of space-time, the emergence of space-time.

61:15>> That's right. >> Okay, so I thought space-time was

61:20fundamental. >> Yeah, I know.

61:22>> So this sort of dream that Einstein had, that everybody had and everybody has of, you know,

61:28the theory of everything. So how do we build up from many worlds, from quantum mechanics,

61:34a model of space-time, a model of gravity? >> Well, yeah, I mean, let me first mention

61:40very quickly why we think it's necessary. You know, we've had gravity in the form that Einstein

61:45bequeathed it to us for over a hundred years now, like 1915 or 1916, he put general relativity in

61:51the final form. So gravity is the curvature of space-time and there's a field that pervades

61:56all the universe that tells us how curved space-time is.

61:59>> And that's a fundamentally classical. >> That's totally classical, right, exactly.

62:03But we also have a formalism, an algorithm for taking a classical theory and quantizing it.

62:10>> This is how we get quantum electrodynamics, for example. And it could be tricky. I mean,

62:14you think you're quantizing something, so that means taking a classical theory and promoting

62:19it to a quantum mechanical theory, but you can run into problems. So they ran into problems and

62:24they did that with electromagnetism, namely that certain quantities were infinity and you don't

62:29like infinity, right? So Feynman and Tomonaga and Schwinger won the Nobel Prize for teaching us how

62:34to deal with the infinities. And then Ken Wilson won another Nobel Prize for saying you shouldn't

62:38have been worried about those infinities after all. But still, it's always the thought that that's

62:44how you will make a good quantum theory. You'll start with a classical theory and quantize it.

62:47So if we have a classical theory of general relativity, we can quantize it or we can try to,

62:52but we run into even bigger problems with gravity than we ran into with electromagnetism. And so

62:57far those problems are insurmountable. We have not been able to get a successful theory of

63:02quantum gravity by starting with classical general relativity and quantizing it.

63:07And there's evidence that there's a good reason why this is true that whatever the quantum theory

63:13of gravity is, it's not a field theory. It's something that has weird non-local features

63:19built into it somehow that we don't understand. And we get this idea from black holes and Hawking

63:25radiation and information conservation and a whole bunch of other ideas I talk about in the book.

63:29So if that's true, if the fundamental theory isn't even local in the sense that an ordinary

63:34quantum field theory would be, then we just don't know where to start in terms of getting a classical

63:40precursor and quantizing it. So the only sensible thing, or at least the next obvious sensible thing

63:45to me would be to say, okay, let's just start intrinsically quantum and work backwards. See

63:49if we can find a classical limit. So the idea of locality, the fact that locality is not fundamental

63:58to the nature of our existence, I guess in that sense, modeling everything as a field makes sense

64:06to me. Stuff that's close by interacts, stuff that's far away doesn't. So what's locality and

64:13why is it not fundamental? And how is that even possible? - Yeah, I mean, locality is the answer

64:18to the question that Isaac Newton was worried about back at the beginning of our conversation,

64:22right? I mean, how can the earth know what the gravitational field of the sun is? And the answer

64:28as spelled out by Laplace and Einstein and others is that there's a field in between.

64:32And the way a field works is that what's happening to the field at this point in space

64:37only depends directly on what's happening at points right next to it. But what's happening

64:42at those points depends on what's happening right next to those, right? And so you can build up an

64:46influence across space through only local interactions. That's what locality means.

64:51What happens here is only affected by what's happening right next to it. That's locality.

64:56The idea of locality is built into every field theory, including general relativity as a

65:01classical theory. It seems to break down when we talk about black holes. And Hawking taught us in

65:07the 1970s that black holes radiate, they give off, they will eventually evaporate away. They're not

65:12completely black once we take quantum mechanics into account. And we think, we don't know for

65:18sure, but most of us think that if you make a black hole out of certain stuff, then like Laplace's

65:26demon taught us, you should be able to predict what that black hole will turn into if it's just

65:30obeying the Schrodinger equation. And if that's true, there are good arguments that can't happen

65:36while preserving locality at the same time. It's just that the information seems to be spread out

65:41non-locally in interesting ways. >> And people should, you talk about holography

65:46with Leonard Susskind on your Mindscape podcast. >> Oh yes, I have a podcast. I didn't even mention

65:51that. This is terrible. >> No, I'm going to ask you questions about

65:55that too. And I've been not shutting up about it. It's my favorite science podcast. Or not,

66:00it's not even a science podcast. It's like a scientist doing a podcast.

66:05>> That's right. That's what it is. Absolutely, yes.

66:07>> Yeah. Anyway. >> Yeah, so holography is this idea when

66:11you have a black hole. And black hole is a region of space inside of which gravity is so strong that

66:16you can't escape. And there's this weird feature of black holes that, again, is totally a thought

66:21experiment feature because we haven't gone and probed any yet. But there seems to be one way

66:26of thinking about what happens inside a black hole as seen by an observer who's falling in,

66:32which is actually pretty normal. Everything looks pretty normal until you hit the singularity and

66:35you die. But from the point of view of the outside observer, it seems like all the information that

66:41fell in is actually smeared over the horizon in a non-local way. And that's puzzling.

66:48And that's so holography because that's a two-dimensional surface that is encapsulating

66:52the whole three-dimensional thing inside, right? Still trying to deal with that, still trying to

66:56figure out how to get there. But it's an indication that we need to think a little bit more subtly

67:00when we quantize gravity. >> So because you can describe

67:03everything that's going on in three-dimensional space by looking at the two-dimensional

67:08projection of it, it means that locality is not necessary.

67:14>> Well, it means that somehow it's only a good approximation. It's not really what's going on.

67:19>> How are we supposed to feel about that? >> You're supposed to feel liberated.

67:23You know, space is just a good approximation. And this was always going to be true once you

67:29started quantizing gravity. So we're just beginning now to face up to the dramatic

67:36implications of quantizing gravity. >> Is there other weird stuff that

67:40happens to quantum mechanics in black hole? >> I don't think that anything weird has happened

67:46with quantum mechanics. I think weird things happen with space-time. I mean, that's what it is.

67:49>> That's right. >> Like quantum mechanics is still just

67:50quantum mechanics. But our ordinary notions of space-time don't really quite work. And

67:57there's a principle that goes hand-in-hand with holography called complementarity,

68:03which says that there's no one unique way to describe what's going on inside a black hole.

68:10Different observers will have different descriptions, both of which are accurate,

68:14but sound completely incompatible with each other. So it depends on how you look at it.

68:20The word complementarity in this context is borrowed from Niels Bohr, who points out you

68:24can measure the position or you can measure the momentum. You can't measure both at the same time

68:29in quantum mechanics. >> So a couple of questions on many worlds.

68:33How does many worlds help us understand our particular branch of reality? So, okay,

68:41that's fine and good, that everything is splitting, but we're just traveling down a

68:45single branch of it. So how does it help us understand our little unique branch?

68:50>> Yeah, I mean, that's a great question. But that's the point, is that we didn't invent many

68:55worlds because we thought it was cool to have a whole bunch of worlds, right? We invented it

68:58because we were trying to account for what we observe here in our world. And what we observe

69:04here in our world are wave functions collapsing, okay? We do have a situation where the electron

69:10seems to be spread out, but then when we look at it, we don't see it spread out. We see it located

69:14somewhere. So what's going on? That's the measurement problem of quantum mechanics.

69:17That's what we have to face up to. So many worlds is just a proposed solution to that problem. And

69:22the answer is nothing special is happening. It's still just the Schrodinger equation, but you have

69:28a wave function too. And that's a different answer than would be given in hidden variables

69:33or dynamical collapse theories or whatever. So the entire point of many worlds is to explain

69:39what we observe, but it tries to explain what we already have observed, right? It's not trying to

69:44be different from what we've observed because that would be something other than quantum mechanics.

69:49>> But the idea that there's worlds that we didn't observe that keep branching off is kind of,

69:55it's stimulating to the imagination. So is it possible to hop from, you mentioned the branches

70:05are independent. Is it possible to hop from one to the other? So it's a physical limit.

70:12The theory says it's impossible. >> There's already a copy of you in

70:17the other world, don't worry. >> Yes.

70:18>> Then leave them alone. >> No, but there's a fear of missing out,

70:24FOMO. >> Yes.

70:25>> That I feel like immediately start to wonder if that other copy is having more or less fun.

70:32>> Yeah, well, the downside to many worlds is that you're missing out on an enormous amount.

70:36And that's always what it's going to be like. >> And I mean, there's a certain stage of

70:42acceptance in that. >> Yes.

70:43>> In terms of rewinding, you think we can rewind the system back. The nice thing about many worlds,

70:51I guess, is it really emphasizes the, maybe you can correct me, but the deterministic

70:58nature of a branch. And it feels like it could be rewound back. Do you see as something that

71:07could be perfectly rewinded back? >> If you're at a fancy French restaurant,

71:14and there's a nice linen white tablecloth, and you have your glass of Bordeaux, and you knock it over,

71:19and the wine spills across the tablecloth. If the world were classical, okay, it would be possible

71:26that if you just lifted the wine glass up, you'd be lucky enough that every molecule of wine would

71:31hop back into the glass, right? But guess what? It's not going to happen in the real world.

71:35And the quantum wave function is exactly the same way. It is possible in principle to rewind

71:42everything if you start from perfect knowledge of the entire wave function of the universe.

71:46In practice, it's never going to happen. >> So time travel, not possible?

71:52>> Nope. At least quantum mechanics has no help. >> What about memory? Does the universe have a

72:01memory of itself where we could, so not time travel, but peek back in time and do a little

72:10like replay? >> Well, it's exactly the same in quantum mechanics as classical mechanics. So

72:18whatever you want to say about that. The fundamental laws of physics in either many

72:22worlds, quantum mechanics or Newtonian physics, conserve information. So if you have all the

§05Transcript · 1:12:29–1:29:44

72:29information about the quantum state of the world right now, your Laplace's demon-like in your

72:34knowledge and calculational capacity, you can wind the clock backward. But none of us is, right? And

72:40so in practice, you can never do that. You can do experiments over and over again, starting from the

72:44same initial conditions for small systems. But once things get to be large, Avogadro's number

72:50of particles, right? Bigger than a cell, no chance. >> We talked a little bit about error of time last

72:57time, but in many worlds that there is a kind of implied error of time, right? So you've talked

73:08about the error of time that has to do with the second law of thermodynamics. That's the error

73:14of time that's emergent or fundamental. We don't know, I guess. >> No, it's emergent. >> Does

73:22everyone agree on that? Well, nobody agrees with everything. >> They should. >> They should.

73:28So that error of time, is that different than the error of time that's implied by many worlds?

73:33>> It's not different, actually, no. In both cases, you have fundamental laws of physics that

73:39are completely reversible. If you give me the state of the universe at one moment in time,

73:43I can run the clock forward or backward equally well. There's no arrow of time built into the

73:48laws of physics at the most fundamental level. But what we do have are special initial conditions

73:5514 billion years ago near the Big Bang. In thermodynamics, those special initial conditions

74:00take the form of things were low entropy, and entropy has been increasing ever since,

74:05making the universe more disorganized and chaotic, and that's the arrow of time.

74:09In quantum mechanics, these special initial conditions take the form of there was only

74:15one branch of the wave function, and the universe has been branching more and more ever since.

74:19>> Okay, so if time is emergent, so it seems like our human cognitive capacity likes to take things

74:28that are emergent and assume and feel like they're fundamental. So if time is emergent,

74:36and locality, is space emergent? >> Yes.

74:42>> Okay. >> But I didn't say time was emergent,

74:44I said the arrow of time was emergent. Those are different.

74:47>> What's the difference between the arrow of time and time? Are you using arrow of time to

74:54simply mean they're synonymous with the second law of thermodynamics?

74:57>> No, but the arrow of time is the difference between the past and future. So there's space,

75:03but there's no arrow of space. You don't feel that space has to have an arrow, right? You could live

75:07in thermodynamic equilibrium. There'd be no arrow of time, but there'd still be time. There'd still

75:11be a difference between now and the future or whatever. >> Oh, so okay. So if nothing changes,

75:16there's still time. >> Well, things could even change.

75:20If the whole universe consisted of the Earth going around the Sun, it would just go in circles,

75:27or ellipses, right? >> That's another reason.

75:28>> Things would change, but it's not increasing entropy. There's no arrow. If you took a movie

75:33of that and I played you the movie backward, you would never know.

75:36>> So the arrow of time can theoretically point in the other direction for brief, briefly.

75:45>> To the extent that it points in different directions, it's not a very good arrow. I mean,

75:49the arrow of time in the macroscopic world is so powerful that there's just no chance of going

75:54back. When you get down to tiny systems with only three or four moving parts, then entropy can

75:58fluctuate up and down. >> What does it mean for space

76:01to be an emergent phenomena? >> It means that the fundamental

76:04description of the world does not include the word space. It'll be something like a vector

76:08in Hilbert space, right? And you have to say, well, why is there a good approximate description

76:13which involves three-dimensional space and stuff inside it?

76:16>> Okay. So time and space are emergent. We kind of mentioned in the beginning,

76:23can you elaborate, what do you feel hope is fundamental in our universe?

76:29>> A wave function living in Hilbert space. >> A wave function in Hilbert space that we

76:34can't intellectualize or visualize really. >> We can't visualize it. We can intellectualize

76:38it very easily. >> Like, well, how do you think about?

76:41>> It's a vector in a 10 to the 10 to the 122-dimensional vector space. It's a complex

76:46vector, unit norm. It evolves according to the Schrodinger equation.

76:49>> Got it. When you put it that way. >> What's so hard, really?

76:54>> It's like, yep. Quantum computers. There's some excitement, actually a lot of excitement

77:04with people that it will allow us to simulate quantum mechanical systems.

77:08What kind of questions do you, about quantum mechanics, about the things we've been talking

77:14about, do you think, do you hope we can answer through quantum simulation?

77:19>> Well, I think that there's a whole fascinating frontier of things you can do with quantum

77:26computers, both sort of practical things with cryptography or money, privacy eavesdropping,

77:33sorting things, simulating quantum systems, right?

77:39>> So, it's a broader question, maybe even outside of quantum computers. Some of the

77:45theories that we've been talking about, what's your hope? What's most promising to test these

77:50theories? What are kind of experiments we can conduct, whether in simulation or in the

77:56physical world, that would validate or disprove or expand these theories?

78:02>> Well, I think for, there's two parts of that question. One is many worlds and the

78:07other one is sort of emergent space time. For many worlds, there are experiments ongoing

78:12to test whether or not wave functions spontaneously collapse. And if they do, then that rules

78:18out many worlds and that would be falsified. If there are hidden variables, there's a theorem

78:24that seems to indicate that the predictions will always be the same as many worlds. I'm

78:29a little skeptical of this theorem. I'm not completely, I haven't internalized it. I haven't

78:32made it in part of my intuitive view of the world yet. So, there might be loopholes to

78:36that theorem. I'm not sure about that. Part of me thinks that there should be different

78:40experimental predictions if there are hidden variables, but I'm not sure.

78:43But otherwise, it's just quantum mechanics all the way down. And so, there's this

78:48cottage industry in science journalism of writing breathless articles that say,

78:54quantum mechanics shown to be more astonishing than ever before thought. And really, it's the

78:58same quantum mechanics we've been doing since 1926. Whereas with the emergent space time stuff,

79:03we know a lot less about what the theory is. It's in a very primitive state. We don't even

79:08really have a safely written down, respectable, honest theory yet. So, there could very well be

79:15experimental predictions we just don't know about yet. That is one of the things that we're trying

79:18to figure out. But for emergent space time, you need really big stuff, right?

79:24Well, or really fast stuff or really energetic stuff. We don't know. That's the thing. So,

79:29there could be violations of the speed of light if you have emergent space time. Not going faster

79:36than the speed of light, but the speed of light could be different for light of different

79:39wavelengths, right? That would be a dramatic violation of physics as we know it, but it could

79:45be possible. Or not. I mean, it's not an absolute prediction. That's the problem. The theories are

79:50just not well-developed enough yet to say. >> Is there anything that quantum mechanics

79:57can teach us about human nature or the human mind? Do you think about sort of consciousness

80:03and these kinds of topics? It's certainly excessively used, as you point out. The word

80:10quantum is used for everything besides quantum mechanics. But in more seriousness, is there

80:17something that goes to the human level and can help us understand our mind?

80:25>> Not really, is the short answer. Minds are pretty classical, I don't think. We don't know

80:33this for sure, but I don't think that phenomena like entanglement are crucial to how the human

80:37mind works. >> What about consciousness? So, you mentioned, I think, early on in the conversation,

80:42you said it would be unlikely but incredible if sort of the observer is somehow a fundamental part.

80:53So, observer, not to romanticize the notion, but seems interlinked to the idea of consciousness.

81:01So, if consciousness is, as the panpsychics believe, is fundamental to the universe,

81:07is that possible? Is that weight? I mean, everything's possible.

81:11>> Just like Joe Rogan likes to say, it's entirely possible. But, okay, but is it

81:18on a spectrum of crazy out there? Statistically speaking, how often do you ponder the possibility

81:27that consciousness is fundamental or the observer is fundamental to-

81:31>> I personally don't at all. There are people who do. I'm a thorough physicalist when it comes

81:36to consciousness. I do not think that there are any separate mental states or mental properties.

81:41I think they're all emergent, just like space-time is. And space-time is hard enough to understand.

81:45So, the fact that we don't yet understand consciousness is not at all surprising to me.

81:50>> You, as we mentioned, have an amazing podcast called Mindscape. It's, as I said,

81:56one of my favorite podcasts, sort of both for your explanation of physics, which a lot of people love,

82:05and when you venture out into things that are beyond your expertise. But it's just a really

82:11smart person exploring even questions like morality, for example. It's very interesting.

82:19I think you did a solo episode and so on. I mean, there's a lot of really interesting

82:23conversations that you have. What are some, from memory, amazing conversations that pop to mind

82:32that you've had? What did you learn from them? Something that maybe changed your mind or just

82:38inspired you? Or just, through this whole experience of having conversations, what stands out to you?

82:43>> It's an unfair question. >> It's totally unfair, but that's okay.

82:47That's all right. It's often the ones, I feel like the ones I do on physics and closely related

82:54science, or even philosophy ones, are like, I know this stuff and I'm helping people learn about it.

83:01But I learn more from the ones that have nothing to do with physics or philosophy, right? So,

83:06talking to Wynton Marsalis about jazz, or talking to Master Sommelier about wine,

83:11talking to Will Wilkinson about partisan polarization and the urban-rural divide,

83:16talking to psychologists like Harold Tavris about cognitive dissonance and how those things work.

83:24Scott Derrickson, who is the director of the movie Doctor Strange, I had a wonderful conversation

83:31with him where we went through the mechanics of making a blockbuster superhero movie, right?

83:36And he's also not a naturalist, he's an evangelical Christian, so we talked about

83:40the nature of reality there. I want to have a couple more discussions with

83:46highly educated theists who know the theology really well, but I haven't quite arranged those

83:55yet. >> I would love to hear that. I mean,

83:57how comfortable are you venturing into questions of religion?

84:02>> Oh, I'm totally comfortable doing it. I did talk with Alan Lightman, who is also

84:06an atheist, but he is trying to rescue the sort of spiritual side of things for atheism. And I did

84:16talk to very vocal atheists like Alex Rosenberg. So, I've talked to some religious believers,

84:23but I need to talk to more. >> How have you changed

84:27through having all these conversations? >> You know, part of the motivation was I had

84:33a long stack of books that I hadn't read and I couldn't find time to read them, and I figured

84:36if I interviewed their authors, it forced me to read them, right? And that has totally worked,

84:41by the way. Now I'm annoyed that people write such long books. I think I'm still very much

84:47learning how to be a good interviewer. I think that's a skill that I think I have good questions,

84:53but there's the give and take that is still, I think, I can be better at. I want to offer

84:59something to the conversation, but not too much, right? I've had conversations where I barely

85:04talked at all, and I've had conversations where I talked half the time, and I think there's a

85:07happy medium in between there. >> So, I think I remember listening to,

85:10without mentioning names, some of your conversations where I wish you would have

85:14disagreed more. As a listener, it's more fun sometimes. >> Well, that's a very good question,

85:22because everyone has an attitude toward that. Some people are really there to basically give

85:29their point of view, and their guest is supposed to respond accordingly. I want to get my view on

85:37the record, but I don't want to dwell on it when I'm talking to someone like David Chalmers, who I

85:42disagree with a lot. I want to say, "Here's why I disagree with you, but we're here to listen to

85:49you." I have an episode every week, and you're only on once a week, right? So, I have an upcoming

85:54podcast episode with Philip Goff, who is a much more dedicated panpsychist. So, there we really

86:02get into it. I think that I probably have disagreed with him more on that episode than I ever have

86:06with another podcast guest, but that's what he wanted, so it worked very well.

86:09>> Yeah, yeah. That kind of debate structure is beautiful when it's done right. When you can

86:17detect that the intent is that you have fundamental respect for the person.

86:21For some reason, it's super fun to listen to when two really smart people are just arguing,

86:30and sometimes lose their shit a little bit, if I may say so.

86:32>> Well, there's a fine line, because I have zero interest in bringing... I mean, maybe you

86:39implied this. I have zero interest in bringing on people for whom I don't have any intellectual

86:43respect. I constantly get requests like, "Bring on a flat earther or whatever, and really slap

86:49them down," or a creationist. I have zero interest. I'm happy to bring on a religious person,

86:55a believer, but I want someone who's smart and can act in good faith and can talk, not a

87:00charlatan or a lunatic, right? So, I will happily bring on people with whom I disagree,

87:06but only people from whom I think the audience can learn something interesting.

87:10>> So, let me ask. The idea of charlatan is an interesting idea. You might be more educated on

87:17this topic than me, but there's folks, for example, who argue various aspects of evolution,

87:26sort of try to approach and say that evolution, sort of our current theory of evolution,

87:34has many holes in it, has many flaws. And they argue that, I think, like Cambrian explosion,

87:42which is like a huge added variability of species, doesn't make sense under our current description

87:51of evolution, theory of evolution. Sort of, if you were to have the conversation with people

87:57like that, how do you know that they're... the difference between outside the box thinkers

88:04and people who are fundamentally unscientific and even bordering on charlatans?

88:12>> That's a great question. And the further you get away from my expertise, the harder it is for

88:17me to really judge exactly those things. And I don't have a satisfying answer for that one,

88:23because I think the example you use of someone who believes in the basic structure of natural

88:29selection, but thinks that this particular thing cannot be understood in terms of our current

88:35understanding of Darwinism, that's a perfect edge case where it's hard to tell, right? And I would

88:42try to talk to people who I do respect and who do know things. And I would have to, given that I'm

88:47a physicist, I know that physicists will sometimes be too dismissive of alternative points of view.

88:53I have to take into account that biologists can also be too dismissive of alternative points of

88:56view. So yeah, that's a tricky one. >> Have you gotten heat yet?

89:01>> I get heat all the time. There's always something... I mean, it's hilarious because

89:05I try very hard not to have the same topic several times in a row. I did have two climate change

89:14episodes, but they were from very different perspectives. But I like to mix it up. That's

89:17the whole point. That's why I'm having fun. And every time I do an episode, someone says, "Oh,

89:21the person you should really get on to talk about exactly that is this other person." I'm like,

89:24"Well, I don't... But I did that now. I don't want to do that anymore."

89:26>> Well, I hope you keep doing it. You're inspiring millions of people with your books,

89:33your podcast. Sean, it's an honor to talk to you. Thank you so much.

89:36>> Thanks very much, Lex.

89:38[END]

89:38>> Thanks, Lex.

89:39[END]

89:39>> Thanks, Lex.

89:40[END]

89:41>> Thanks, Lex.

89:41[END]

89:42>> Thanks, Lex.

89:43[END]

89:43>> Thanks, Lex.

89:43[END]

89:43>> Thanks, Lex.

89:44[END]

89:44>> Thanks, Lex.

§06Transcript · 1:29:44–1:29:52

89:44[END]

89:44>> Thanks, Lex.

89:45[END]

89:45>> Thanks, Lex.

89:45[END]

89:45>> Thanks, Lex.

89:46[END]

89:46>> Thanks, Lex.

89:46[END]

89:46>> Thanks, Lex.

89:47[END]

89:47>> Thanks, Lex.

89:47[END]

89:47>> Thanks, Lex.

89:48[END]

89:48>> Thanks, Lex.

89:48[END]

89:49>> Thanks, Lex.

89:49[END]

89:49>> Thanks, Lex.

89:50[END]

89:50>> Thanks, Lex.

89:50[END]

89:51>> Thanks, Lex.

89:51[END]

89:51>> Thanks, Lex.

89:52[END]

89:52>> Thanks, Lex.

89:52[END]

— A LITTLE MORE TO THINK ABOUT. —