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Frank Wilczek: Physics of Quarks, Dark Matter, Complexity, Life & Aliens

Episode 1872021-05-29English

Guests: Frank Wilczek

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§01Transcript · 00:00–12:05

00:00The following is a conversation with Frank Wilczek,

00:02a theoretical physicist at MIT who won the Nobel Prize

00:07for the co discovery of asymptotic freedom

00:09in the theory of strong interaction.

00:12Quick mention of our sponsors,

00:14the Information, NetSuite, ExpressVPN, Blinkist,

00:18and Aidsleep.

00:20Check them out in the description to support this podcast.

00:23As a side note, let me say a word about asymptotic freedom.

00:26Protons and neutrons make up the nucleus of an atom.

00:30Strong interaction is responsible

00:31for the strong nuclear force that binds them.

00:34But strong interaction also holds together the quarks

00:37that make up the protons and neutrons.

00:40Frank Wilczek, David Gross, and David Politzer

00:43came up with a theory postulating

00:45that when quarks come really close to one another,

00:48the attraction abates and they behave like free particles.

00:51This is called asymptotic freedom.

00:54This happens at very, very high energies,

00:57which is also where all the fun is.

01:00This is the Lex Friedman Podcast,

01:02and here is my conversation with Frank Wilczek.

01:07What is the most beautiful idea in physics?

01:10The most beautiful idea in physics

01:13is that we can get a compact description of the world

01:19that's very precise and very full

01:22at the level of the operating system of the world.

01:28That's an extraordinary gift.

01:32And we get worried when we find discrepancies

01:38between our description of the world

01:41and what's actually observed

01:43at the level even of a part in a billion.

01:46You actually have this quote from Einstein

01:49that the most incomprehensible thing

01:51about the universe is that it is comprehensible,

01:54something like that.

01:55Yes, so that's the most beautiful surprise

01:58that I think that really was to me the most profound result

02:05of the scientific revolution of the 17th century

02:08with the shining example of Newtonian physics

02:13that you could aspire to completeness, precision,

02:17and a concise description of the world,

02:20of the operating system.

02:21And it's gotten better and better over the years

02:25and that's the continuing miracle.

02:27Now, there are a lot of beautiful sub miracles too.

02:30The form of the equations is governed

02:33by high degrees of symmetry

02:35and they have a very surprising kind

02:39of mind expanding structure,

02:40especially in quantum mechanics.

02:42But if I had to say the single most beautiful revelation

02:47is that, in fact, the world is comprehensible.

02:53Would you say that's a fact or a hope?

02:56It's a fact.

02:58We can do, you can point to things like

03:02the rise of gross national products per capita

03:11around the world as a result of the scientific revolution.

03:14You can see it all around you.

03:15And recent developments with exponential production

03:21of wealth, control of nature at a very profound level

03:27where we do things like sense tiny, tiny, tiny, tiny

03:31vibrations to tell that there are black holes

03:35colliding far away or we test laws as I alluded to

03:40whether it's part in a billion and do things

03:45in what appear on the surface

03:47to be entirely different conceptual universes.

03:49I mean, on the one hand, pencil and paper

03:52are nowadays computers that calculate abstractions

03:55and on the other hand, magnets and accelerators

03:58and detectors that look at the behavior

04:00of fundamental particles and these different universes

04:05have to agree or else we get very upset

04:08and that's an amazing thing if you think about it.

04:12And it's telling us that we do understand a lot

04:18about nature at a very profound level

04:21and there are still things we don't understand of course

04:25but as we get better and better answers

04:28and better and better ability to address difficult questions

04:32we can ask more and more ambitious questions.

04:35Well, I guess the hope part of that is because

04:38we are surrounded by mystery.

04:40So one way to say it, if you look at the growth GDP

04:45over time that we figured out quite a lot

04:47and we're able to improve the quality of life

04:50because of that and we've figured out some fundamental things

04:53about this universe but we still don't know

04:55how much mystery there is and it's also possible

04:58that there's some things that are in fact incomprehensible

05:03to both our minds and the tools of science.

05:07Like the sad thing is we may not know it

05:11because in fact they are incomprehensible

05:14and that's the open question is how much

05:16of the universe is comprehensible?

05:18If we figured out everything what's inside the black hole

05:23and everything that happened at the moment of the Big Bang

05:26does that still give us the key

05:28to understanding the human mind

05:30and the emergence of all the beautiful complexity

05:33we see around us?

05:35That's not like when I see these objects

05:38like I don't know if you've seen them like cellular automata

05:41all these kinds of objects where the from simple rules

05:44emerges complexity, it makes you wonder maybe

05:48it's not reducible to simple beautiful equations

05:52the whole thing only parts of it.

05:54That's the tension I was getting at with the hope.

05:57Well, when we say the universe is comprehensible

06:00we have to kind of draw careful distinctions

06:04about or definitions about what we mean by that.

06:12Both the universe and the kind of and the comprehensive.

06:15Exactly, right so the so in certain areas

06:22of understanding reality we've made extraordinary progress

06:27I would say in understanding fundamental physical processes

06:32and getting very precise equations that really work

06:35and allow us to do the profound sculpting of matter

06:40to make computers and iPhones and everything else

06:43and they really work and they're extraordinary productions

06:48on the other but and that's all based

06:51on the laws of quantum mechanics

06:53and they really work and they give us tremendous control

06:59of nature on the other hand as we get better answers

07:04we can also ask more ambitious questions

07:07and there are certainly things that have been observed

07:11even in what would be usually called the realm of physics

07:15that aren't understood for instance there seems to be

07:19another source of mass in the universe

07:21the so called dark matter that we don't know what it is

07:25and it's a very interesting question what it is then

07:30but also as you were alluding to there's it's one thing

07:34to know the basic equations it's another thing

07:38to be able to solve them in important cases

07:42so we run up against the limits of that

07:45in things like chemistry where we'd like to be able

07:48to design molecules and predict their behavior

07:51from the equations we think the equations could do that

07:54in principle but in practice it's very challenging

07:59to solve them in all but very simple cases

08:04and then there's the other thing which is that a lot

08:07of what we're interested in is historically conditioned

08:11it's not a matter of the fundamental equations

08:15but about what has evolved or come out

08:19of the early universe and formed into people and frogs

08:23and societies and things and the laws of physics

08:27the basic laws of physics only take you so far

08:30in that it kind of provides a foundation

08:32but doesn't really that you need entirely different concepts

08:35to deal with those kind of systems

08:39and one thing I can say about that is that the laws

08:46themselves point out their limitations

08:48that they kind of their laws for dynamical evolution

08:53so they tell you what happens if you have

08:55a certain starting point but they don't tell you

08:57what the starting point should be at least yeah

09:01and the other thing that emerges

09:05from the equations themselves is the phenomena

09:09of chaos and sensitivity to initial conditions

09:14which tells us that you have that there are intrinsic

09:20limitations on how well we can spell out the consequences

09:24of the laws if we try to apply them.

09:26It's the old apple pie if you want to what is it

09:28make an apple pie from scratch you have to build

09:32the universe or something like that.

09:34Well you're much better off starting with apples

09:37than starting with quarks let's put it that way.

09:39In your book A Beautiful Question you ask

09:42does the world embody beautiful ideas?

09:44So the book is centered around this very interesting

09:48question it's like Shakespeare you can like dig in

09:50and read into all the different interpretations

09:52of this question but at the high level what to use

09:56the connection between beauty of the world

09:59and physics of the world.

10:02In a sense we now have a lot of insight into what

10:05the laws are the form they take that allow us

10:09to understand matter in great depth and control it

10:13as we've discussed and it's an extraordinary thing

10:19how mathematically ideal those equations turn out to be.

10:26In the early days of Greek philosophy Plato had this model

10:33of atoms built out of the five perfectly symmetrical

10:37platonic solids so there was somehow the idea

10:39that mathematical symmetry should govern the world

10:44and we've out Platoed Plato by far in modern physics

10:49because we have symmetries that are much more extensive

10:52much more powerful that turn out to be the ingredients

10:56out of which we construct our theory of the world

10:59and it works and so that's certainly beautiful.

11:04So the idea of symmetry which is a driving inspiration

11:13in much of human art especially decorative art

11:18like the Alhambra or wallpaper designs or things

11:22you see around you everywhere also turns out to be

11:26the dominant theme in modern fundamental physics

11:30symmetry and its manifestations the laws turn out

11:33to be very to have these tremendous amounts of symmetry

11:36you can change the symbols and move them around

11:38in different ways and they still have the same consequences.

11:45So that's beautiful that these concepts that humans

11:59find appealing also turn out to be the concepts

12:03that govern how the world actually works.

§02Transcript · 12:07–23:57

12:07I don't think that's an accident.

12:09I think humans were evolved to be able to interact

12:13with the world in ways that are advantageous

12:17and to learn from it and so we are naturally evolved

12:21or designed to enjoy beauty and it's a symmetry

12:24and the world has it and that's why we resonate with it.

12:29Well it's interesting that the ideas of symmetry

12:33emerge at many levels of the hierarchy of the universe.

12:40So you're talking about particles but it also is

12:44at the level of chemistry and biology

12:47and the fact that our cognitive sort of our perception

12:55system and whatever our cognition is also finds

12:59it appealing or somehow our sense of what is beautiful

13:02is grounded in this idea of symmetry

13:05or the breaking of symmetry.

13:06Symmetry is at the core of our conception of beauty

13:09whether it's the breaking or the non breaking

13:11of the symmetry.

13:12It makes you wonder why.

13:17Why?

13:20So I come from Russia and the question of Dostoevsky

13:23he has said that beauty will save the world.

13:27Maybe as a physicist you can tell me

13:29what do you think he meant by that?

13:31I don't know if it saves the world

13:32but it does turn out to be a tremendous source

13:35of insight into the world.

13:37When we investigate kind of the most fundamental

13:42interactions, things that are hard to access

13:46because they occur at very short distances

13:48between very special kinds of particles

13:53whose properties are only revealed at high energies.

14:01We don't have much to go on from everyday life

14:04but so we have when we guess what the,

14:06and the experiments are difficult to do

14:08so you can't really follow a very wholly empirical procedure

14:14to sort of in the Baconian style figure out the laws

14:20kind of step by step just by accumulating a lot of data

14:23what we actually do is guess.

14:25And the guesses are kind of aesthetic really.

14:29What would be a nice description

14:31that's consistent with what we know

14:34and then you try it out and see if it works

14:36and by gosh it does in many profound cases.

14:42So there's that but there's another source of symmetry

14:46which I didn't talk so much about in a beautiful question

14:51but does relate to your comments

14:56and I think very much relates to the source of symmetry

15:02that we find in biology and in our heads, you know,

15:08in our brain which is that, well it is discussed a bit

15:15in a beautiful question and also in fundamentals

15:20is that when you have, symmetry is also a very important

15:28means of construction.

15:30So when you have for instance simple viruses

15:34that need to construct their coat, their protein coat,

15:39the coats often take the form of platonic solids

15:43and the reason is that the viruses are really dumb

15:47and they only know how to do one thing

15:49so they make a pentagon then they make another pentagon

15:51and they make another pentagon

15:52and they all glue together in the same way

15:55and that makes a very symmetrical object sort of.

15:58So the rules of development when you have simple rules

16:02and they work again and again, you get symmetrical patterns.

16:07That's kind of, in fact it's a recipe also

16:09for generating fractals, like the kind of broccoli

16:14that has all this internal structure

16:19and I wish I had a picture to show

16:20but maybe people remember it from the supermarket

16:26and you say how did a vegetable get so intelligent

16:30to make such a beautiful object

16:31with all this fractal structure

16:33and the secret is stupidity.

16:35You just do the same thing over and over again

16:38and in our brains also, you know, we came out,

16:43we start from single cells and they reproduce

16:47and each one does basically roughly the same thing.

16:54The program evolves in time, of course,

16:56different modules get turned on and off,

17:01different regions of the genetic code

17:03get turned on and off but basically,

17:06a lot of the same things are going on

17:08and they're simple things

17:09and so you produce the same patterns over and over again

17:12and that's a recipe for producing symmetry

17:14because you're getting the same thing in many, many places

17:17and if you look at, for instance,

17:20the beautiful drawings of Roman Icahal,

17:24the great neuroanatomist who drew the structure

17:29of different organs like the hippocampus,

17:33you see it's very regular and very intricate

17:37and it's symmetry in that sense

17:43because it's many repeated units

17:46that you can take from one place to the other

17:49and see that they look more or less the same.

17:51But what you're describing, this kind of beauty

17:54that we're talking about now is a very small sample

17:58in terms of space time in a very big world

18:01in a very short, brief moment in this long history.

18:08In your book, Fundamentals, 10 Keys to Reality,

18:11I'd really recommend people read it.

18:14You say that space and time are pretty big or very big.

18:20How big are we talking about?

18:21Can you tell a brief history of space and time?

18:26It's easy to tell a brief history, but the details get very

18:30involved, of course, but one thing I'd like to say

18:33is that if you take a broad enough view,

18:37the history of the universe is simpler

18:38than the history of Sweden, say,

18:40because your standards are lower.

18:45But just to make it quantitative,

18:49I'll just give a few highlights.

18:51And it's a little bit easier to talk about time,

18:55so let's start with that.

18:57The Big Bang occurred, we think.

19:00The universe was much hotter and denser and more uniform

19:03about 13.8 billion years ago,

19:07and that's what we call the Big Bang.

19:10And it's been expanding and cooling,

19:12the matter in it has been expanding and cooling ever since.

19:16So in a real sense, the universe is 13.8 billion years old.

19:20That's a big number, kind of hard to think about.

19:24A nice way to think about it, though,

19:26is to map it onto one year.

19:29So let's say the universe just linearly mapped

19:32the time intervals from 13.8 billion years onto one year.

19:37So the Big Bang then is on January 1st at 12 a.m.

19:43And you wait for quite a long time

19:49before the dinosaurs emerge.

19:51The dinosaurs emerge on Christmas, it turns out.

19:55And...

19:5512 months, almost 12 months later.

19:57Getting close to the end, yes.

19:59Getting close to the end.

20:01And the extinction event that let the mammals

20:05and ultimately humans inherit the Earth

20:08from the dinosaurs occurred on December 30th.

20:13And all of human history is a small part of the last day.

20:18And so, yes, so we're occupying only,

20:23and a human lifetime is a very, very infinitesimal part

20:26of this interval of these gigantic cosmic reaches of time.

20:35And in space, we can tell a very similar story.

20:39In fact, it's convenient to think that the size

20:44of the universe is the distance that light can travel

20:48in 13.8 billion years.

20:50So it's 13.8 billion light years.

20:54That's how far you can see out.

20:56That's how far signals can reach us.

21:01And that is a big distance.

21:06That is a big distance because compared to that, the Earth

21:14is a fraction of a light second.

21:18So again, it's really, really big.

21:21And so if we wanna think about the universe

21:27as a whole in space and time,

21:30we really need a different kind of imagination.

21:35It's not something you can grasp

21:41in terms of psychological time in a useful way.

21:44You have to think, you have to use exponential notation

21:47and abstract concepts to really get any hold

21:51on these vast times and spaces.

21:56On the other hand, let me hasten to add

21:58that that doesn't make us small

22:00or make the time that we have to us small.

22:06Because again, looking at those pictures

22:10of what our minds are and some of the components

22:15of our minds, these beautiful drawings

22:18of the cellular patterns inside the brain,

22:21you see that there are many, many, many processing units.

22:24And if you analyze how fast they operate,

22:29I tried to estimate how many thoughts

22:31a person can have in a lifetime.

22:33That's kind of a fuzzy question,

22:34but I'm very proud that I was able

22:36to define it pretty precisely.

22:39And it turns out we have time for billions

22:43of meaningful thoughts in a lifetime.

22:46So it's a lot.

22:48We shouldn't think of ourselves as terribly small

22:51either in space or in time,

22:53because although we're small in those dimensions

22:57compared to the universe, we're large compared

23:01to meaningful units of processing information

23:05and being able to conceptualize and understand things.

23:11Yeah, but 99% of those thoughts are probably food,

23:15sex, or internet related.

23:16Well, yeah, well, they're not necessarily, that's right.

23:20Only like point one is Nobel Prize winning ideas.

23:24That's true, but there's more to life

23:26than winning Nobel Prizes.

23:27How did you do that calculate?

23:29Can you maybe break that apart a little bit,

23:31just kind of for fun, sort of an intuition

23:34of how we calculate the number of thoughts?

23:35The number of thoughts, right.

23:37It's necessarily imprecise because a lot of things

23:40are going on in different ways and what is a thought.

23:43But there are several things that point

23:45to more or less the same rate of being able

23:50to have meaningful thoughts.

23:52For instance, the one that I think is maybe

§03Transcript · 23:57–34:44

23:57the most penetrating is how fast

24:01we can process visual images.

24:04How do we do that?

24:07If you've ever watched old movies,

24:11you can see that, well, any movie, in fact,

24:15a motion picture is really not a motion picture.

24:18It's a series of snapshots that are playing

24:20one after the other and it's because our brains

24:25also work that way.

24:26We take snapshots of the world, integrate over a certain time

24:29and then go on to the next one and then by post processing,

24:33create the illusion of continuity and flow,

24:37we can deal with that.

24:38And if the flicker rate is too slow,

24:44then you start to see that it's a series of snapshots

24:48and you can ask, what is the crossover?

24:51When does it change from being something

24:53that is matched to our processing speed versus too fast?

24:57And it turns out about 40 per second.

25:00And then if you take 40 per second as how well,

25:04how fast we can process visual images,

25:06you get to several billions of thoughts.

25:10If you, similarly, if you ask what are some

25:14of the fastest things that people can do?

25:16Well, they can play video games,

25:18they can play the piano very fast if they're skilled at it.

25:22And again, you get to similar units

25:25or how fast can people talk?

25:27You get to similar, you know,

25:28within a couple of orders of magnitude,

25:30you get more or less to the same idea.

25:33So that's how you can say that there's billions

25:38of meaningful, there's room for billions

25:40of meaningful thoughts.

25:42I won't argue for exactly two billion versus 1.8 billion.

25:47It's not that kind of question,

25:49but I think any estimate that's reasonable

25:52will come out within, say, 100 billion and 100 million.

25:58So it's a lot.

26:01It would be interesting to map out

26:04for an individual human being the landscape of thoughts

26:07that they've sort of traveled.

26:09If you think of thoughts as a set of trajectories,

26:14what that landscape looks like.

26:16I mean, I've been recently really thinking

26:19about this Richard Dawkins idea of memes

26:24and just all this ideas and the evolution of ideas

26:27inside of one particular human mind

26:30and how they're then changed and evolved

26:33by interaction with other human beings.

26:36It's interesting to think about.

26:38So if you think the number is billions,

26:41you think there's also social interaction.

26:44So these aren't like there's interaction

26:48in the same way you have interaction with particles.

26:50There's interaction between human thoughts

26:53that perhaps that interaction in itself

26:56is fundamental to the process of thinking.

26:59Like without social interaction,

27:01we would be like stuck, like walking in a circle.

27:04We need the perturbation of other humans

27:07to create change and evolution.

27:09Once you bring in concepts of interactions

27:13and correlations and relations,

27:15then you have what's called a combinatorial explosion

27:20that the number of possibilities expands exponentially

27:24technically with the number of things you're considering.

27:28And it can easily rapidly outstrip these billions

27:34of thoughts that we're talking about.

27:36So we definitely cannot by brute force

27:41master complex situations

27:45or think of all the possibilities in a complex situations.

27:48I mean, even something as relatively simple as chess

27:53is still something that human beings

27:56can't comprehend completely.

27:57Even the best players lose, still sometimes lose

28:00and they consistently lose to computers these days.

28:05And in computer science, there's a concept of NP complete.

28:08So large classes of problems when you scale them up

28:12beyond a few individuals become intractable.

28:16And so that in that sense, the world is inexhaustible.

28:21And that makes it beautiful that we can make any laws

28:25that generalize efficiently and well

28:29can compress all of that combinatorial complexity

28:32just like a simple rule.

28:33That in itself is beautiful.

28:35It's a happy situation.

28:36And I think that we can find general principles

28:43of sort of of the operating system

28:45that are comprehensible, simple, extremely powerful

28:49and let us control things very well

28:52and ask profound questions.

28:55And on the other hand,

28:56that the world is going to be inexhaustible.

28:59That once we start asking about relationships

29:03and how they evolve and social interactions

29:06and we'll never have a theory of everything

29:10in any meaningful sense because that.

29:13Of everything, everything, truly everything is.

29:17Can I ask you about the Big Bang?

29:19So we talked about the space and time are really big.

29:24But then, and we humans give a lot of meaning

29:27to the word space and time in our like daily lives.

29:33But then can we talk about this moment of beginning

29:37and how we're supposed to think about it?

29:40That at the moment of the Big Bang,

29:42everything was what, like infinitely small

29:46and then it just blew up?

29:48We have to be careful here

29:49because there's a common misconception

29:53that the Big Bang is like the explosion of a bomb

29:58in empty space that fills up the surrounding place.

30:02It is space.

30:03It is, yeah.

30:05As we understand it, it's the fact,

30:08it's the fact or the hypothesis,

30:12but well supported up to a point

30:14that everywhere in the whole universe,

30:19early in the history,

30:24matter came together into a very hot, very dense,

30:28if you run it backwards in time,

30:29matter comes together into a very hot, very dense

30:32and yet very homogeneous plasma

30:36of all the different kinds of elementary particles

30:39and quarks and anti quarks and gluons

30:41and photons and electrons and anti electrons,

30:43everything, all of that stuff.

30:45Like really hot.

30:46Really, really, really hot.

30:49We're talking about way, way hotter

30:52than the surface of the sun.

30:56Well, in fact, if you take the equations as they come,

31:00the prediction is that the temperature

31:02just goes to infinity,

31:04but then the equations break down.

31:06We don't really, there are various,

31:10the equations become infinity equals infinity,

31:12so they don't feel that it's called a singularity.

31:15We don't really know.

31:16This is running the equations backwards,

31:19so you can't really get a sensible idea

31:21of what happened before the Big Bang.

31:23So we need different equations

31:25to address the very earliest moments.

31:31But so things were hotter and denser.

31:35We don't really know why things started out that way.

31:40We have a lot of evidence that they did start out that way.

31:43But since most of the,

31:51we don't get to visit there and do controlled experiments.

31:55Most of the record is very, very processed

31:59and we have to use very subtle techniques

32:05and powerful instruments to get information

32:09that has survived.

32:11Get closer and closer to the Big Bang.

32:14Get closer and closer to the beginning of things.

32:16And what's revealed there is that, as I said,

32:22there undoubtedly was a period

32:25when everything in the universe

32:26that we have been able to look at and understand,

32:30and that's consistent with everything,

32:33is in a condition where it was much, much hotter

32:41and much, much denser,

32:44but still obeying the laws of physics

32:46as we know them today.

32:48And then you start with that.

32:51So all the matter is in equilibrium.

32:54And then with small quantum fluctuations

32:57and run it forward,

32:59and then it produces, at least in broad strokes,

33:04the universe we see around us today.

33:06Do you think we'll ever be able to,

33:09with the tools of physics, with the way science is,

33:12with the way the human mind is,

33:14we'll ever be able to get to the moment of the Big Bang

33:17in our understanding or even the moment before the Big Bang?

33:21Can we understand what happened before the Big Bang?

33:24I'm optimistic both that we'll be able to measure more,

33:31so observe more,

33:33and that we'll be able to figure out more.

33:36So they're very, very tangible prospects

33:40for observing the extremely early universe,

33:45so even much earlier than we can observe now

33:49through looking at gravitational waves.

33:52Gravitational waves, since they interact so weakly

33:55with ordinary matter,

33:58sort of send a minimally processed signal from the Big Bang.

34:03It's a very weak signal

34:05because it's traveled a long way

34:07and diffused over long spaces,

34:09but people are gearing up to try to detect

34:13gravitational waves that could have come

34:15from the early universe.

34:16Yeah, LIGO's an incredible engineering project.

34:19It's the most sensitive, precise devices on Earth.

34:24The fact that humans can build something like that

34:27is truly awe inspiring from an engineering perspective.

34:31Right, but these gravitational waves from the early universe

34:34will probably be of a much longer wavelength

34:38than LIGO is capable of sensing,

34:41so there's a beautiful project

§04Transcript · 34:44–46:17

34:44that's contemplated to put lasers

34:51in different locations in the solar system.

34:54We really, really separate it

34:56by solar system scale differences,

34:59like artificial planets or moons in different places

35:03and see the tiny motions of those

35:06relative to one another

35:07as a signal of radiation from the Big Bang.

35:10We can also maybe indirectly see the imprint

35:15of gravitational waves from the early universe

35:18on the photons, the microwave background radiation.

35:23That is our present way of seeing into the earliest universe,

35:27but those photons interact much more strongly with matter.

35:31They're much more strongly processed,

35:32so they don't give us directly such an unprocessed view

35:37of the early universe, of the very early universe,

35:41but if gravitational waves leave some imprint on that

35:45as they move through, we could detect that too,

35:49and people are trying, as we speak,

35:53working very hard towards that goal.

35:56It's so exciting to think about a sensor

35:58the size of the solar system.

36:01That would be a fantastic,

36:03I mean, that would be a pinnacle artifact

36:06of human endeavor to me.

36:08It would be such an inspiring thing

36:11that just we want to know,

36:15and we go to these extraordinary lengths

36:17of making gigantic things that are also very sophisticated

36:20because what you're trying to do,

36:22you have to understand how they move.

36:24You have to understand the properties of light

36:28that are being used, the interference between light,

36:30and you have to be able to make the light with lasers

36:34and understand the quantum theory

36:35and get the timing exactly right.

36:38It's an extraordinary endeavor

36:40involving all kinds of knowledge

36:42from the very small to the very large,

36:45and all in the service of curiosity

36:49and built on a grand scale, so.

36:52Yeah, it would make me proud to be a human if we did that.

36:58I love that you're inspired both by the power of theory

37:01and the power of experiment.

37:02So both, I think, are exceptionally impressive

37:07that the human mind can come up with theories

37:10that give us a peek into how the universe works,

37:13but also construct tools that are way bigger

37:16than the evolutionary origins we came from.

37:20Right, and by the way,

37:22the fact that we can design such things and they work

37:25is an extraordinary demonstration

37:28that we really do understand a lot.

37:30And then in some ways.

37:33And it's our ability to answer questions

37:36that also leads us to be able

37:37to address more ambitious questions.

37:39So you mentioned at the Big Bang in the early days,

37:45things are pretty homogeneous.

37:46Yes.

37:47But here we are, sitting on Earth,

37:51two hairless apes, you could say, with microphones.

37:57In talking about the brief history of things,

37:58you said it's much harder to describe Sweden

38:00than it is the universe.

38:03So there's a lot of complexity.

38:05There was a lot of interesting details here.

38:07So how does this complexity come to be, do you think?

38:11It seems like there's these pockets.

38:13Yeah.

38:14We don't know how rare of like where hairless apes emerge.

38:18Yeah.

38:19And then that came from the initial soup

38:22that was homogeneous.

38:23Was that an accident?

38:26Well, we understand in broad outlines

38:31how it could happen.

38:33We certainly don't understand why it happened exactly

38:36in the way it did.

38:40Or there are certainly open questions

38:42about the origins of life

38:44and how inevitable the emergence of intelligence was

38:47and how that happened.

38:48But in the very broadest terms,

38:52the universe early on was quite homogeneous,

38:58but not completely homogeneous.

39:01There were part in 10,000 fluctuations in density

39:07within this primordial plasma.

39:10And as time goes on, there's an instability

39:16which causes those density contrasts to increase.

39:20There's a gravitational instability

39:21where it's denser, the gravitational attractions

39:24are stronger.

39:25And so that brings in more matter

39:27and it gets even denser and so on and so on.

39:29So there's a natural tendency of matter to clump

39:34because of gravitational interactions.

39:37And then the equation is complicated.

39:39We have lots of things clumping together.

39:43Then we know what the laws are,

39:47but we have to a certain extent wave our hands

39:50about what happens.

39:51But basic understanding of chemistry

39:56says that if things and the physics of radiation

40:00tells us that as things start to clump together,

40:02they can radiate, give off some energy.

40:05So they don't just, they slow down.

40:07As a result, they lose energy.

40:09They can collaborate together, cool down,

40:12form things like stars, form things like planets.

40:16And so in broad terms, there's no mystery.

40:19There's, that's what the scenario,

40:22that's what the equations tell you should happen.

40:25But because it's a process involving

40:30many, many fundamental individual units,

40:37the application of the laws that govern individual units

40:40to these things is very delicate,

40:46computationally very difficult.

40:48And more profoundly, the equations have

40:52this probability of chaos or sensitivity

40:54to initial conditions, which tells you tiny differences

40:57in the initial state can lead to enormous differences

41:00in the subsequent behavior.

41:02So physics, fundamental physics at some point says,

41:08okay, chemists, biologists, this is your problem.

41:11And then again, in broad terms,

41:16we know how it's conceivable that the humans

41:23and things like that, how complex structure can emerge.

41:28It's a matter of having the right kind of temperature

41:34and the right kind of stuff.

41:36So you need to be able to make chemical bonds

41:41that are reasonably stable

41:42and be able to make complex structures.

41:45And we're very fortunate that carbon has this ability

41:48to make backbones and elaborate branchings and things.

41:54So you can get complex things that we call biochemistry.

41:57And yet the bonds can be broken a little bit

42:01with the help of energetic injections from the sun.

42:04So you have to have both the possibility of changing,

42:07but also the useful degree of stability.

42:10And we know at that very, very broad level, physics

42:15can tell you that it's conceivable.

42:17If you want to know what really happened,

42:23what really can happen, then you have to work a bit,

42:26go to chemistry.

42:27If you want to know what actually happened,

42:29then you really have to consult the fossil record

42:32and biologists.

42:33And so these ways of addressing the issue

42:41are complimentary in a sense.

42:43They use different kinds of concepts,

42:49they use different languages

42:52and they address different kinds of questions,

42:54but they're not inconsistent, they're just complimentary.

42:59It's kind of interesting to think about those early fluctuations

43:03as our earliest ancestors.

43:07Yes, that's right.

43:08So it's amazing to think that this is the modern answer

43:15to the, or the modern version of what the Hindu philosophers

43:24had, that art thou.

43:25If you ask what, okay, those little quantum fluctuations

43:30in the early universe are the seeds out of which complexity,

43:36including plausibly humans, really evolve.

43:40You don't need anything else.

43:42That brings up the question of asking for a friend here

43:47if there's other pockets of complexity,

43:52commonly called as alien intelligent civilizations out there.

43:59Well, we don't know for sure,

44:00but I have a strong suspicion that the answer is yes

44:05because the one case we do have at hand to study

44:13here on Earth, we sort of know what the conditions were

44:17that were helpful to life,

44:18the right kind of temperature, the right kind of star

44:21that keeps, maintains that temperature for a long time,

44:24the liquid environment of water.

44:28And once those conditions emerged on Earth,

44:33which was roughly four and a half billion years ago,

44:36it wasn't very long before what we call life

44:39started to leave relics.

44:41So we can find forms of life, primitive forms of life

44:47that are almost as old as the Earth itself

44:49in the sense that once the Earth was turned

44:55from a very hot boiling thing

44:58and cooled off into a solid mass with water,

45:02life emerged very, very quickly.

45:03So it seems that these general conditions for life

45:09are enough to make it happen relatively quickly.

45:13Now, the other lesson I think that one can draw

45:21from this one example, it's dangerous to draw lessons

45:24from one example, but that's all we've got,

45:27and that the emergence of intelligent life

45:32is a different issue altogether.

45:35That took a long time and seems to have been

45:40pretty contingent for a long time.

45:47Well, for most of the history of life,

45:50it was single celled things.

45:55Even multicellular life only rose

45:58about 600 million years ago, so much after.

46:01And then intelligence is kind of a luxury.

46:12Many more kinds of creatures have big stomachs

§05Transcript · 46:18–57:28

46:18than big brains.

46:20In fact, most have no brains at all in any reasonable sense.

46:25And the dinosaurs ruled for a long, long time

46:30and some of them were pretty smart,

46:31but they were at best bird brains

46:35because birds came from the dinosaurs.

46:37And it could have stayed that way.

46:41And then the emergence of humans was very contingent

46:46and kind of a very, very recent development

46:49on evolutionary timescales.

46:51And you can argue about the level of human intelligence,

46:55but I think that's what we're talking about.

46:58It's very impressive and can ask these kinds of questions

47:02and discuss them intelligently.

47:07So I guess my, so this is a long winded answer

47:13or justification of my feeling

47:16is that the conditions for life in some form

47:21are probably satisfied many, many places

47:28around the universe and even within our galaxy.

47:33I'm not so sure about the emergence of intelligent life

47:36or the emergence of technological civilizations.

47:41That seems much more contingent and special.

47:47And we might, it's conceivable to me

47:50that we're the only example in the galaxy.

47:54Although, yeah, I don't know one way or the other.

47:56I have different opinions on different days of the week.

47:59But one of the things that worries me

48:01in the spirit of being humble,

48:04that our particular kind of intelligence

48:09is not very special.

48:10So there's all kinds of different intelligences.

48:13And even more broadly,

48:15there could be many different kinds of life.

48:19So the basic definition, and I just had,

48:22I think somebody that you know, Sarah Walker,

48:24I just had a very long conversation with her

48:27about even just the very basic question

48:29of trying to define what is life from a physics perspective.

48:34Even that question within itself,

48:36I think one of the most fundamental questions

48:38in science and physics and everything

48:41is just trying to get a hold,

48:43trying to get some universal laws

48:45around the ideas of what is life

48:47because that kind of unlocks a bunch of things

48:49around life, intelligence, consciousness,

48:52all those kinds of things.

48:53I agree with you in a sense,

48:55but I think that's a dangerous question

48:56because the answer can't be any more precise

49:01than the question.

49:02And the question, what is life,

49:07kind of assumes that we have a definition of life

49:11and that it's a natural phenomena

49:12that can be distinguished.

49:14But really there are edge cases like viruses

49:17and some people would like to say

49:20that electrons have consciousness.

49:25So you can't, if you really have fuzzy concepts,

49:28it's very hard to reach precise kinds of scientific answers.

49:34But I think there's a very fruitful question

49:37that's adjacent to it,

49:39which has been pursued in different forms

49:42for quite a while

49:44and is now becoming very sophisticated

49:47in reaching in new directions.

49:50And that is, what are the states of matter

49:53that are possible?

49:55So in high school or grade school,

49:58you learn about solids, liquids and gases,

50:01but that really just scratches the surface

50:04of different ways that are distinguishable,

50:07that matter can form into macroscopically different,

50:15meaningful patterns that we call phases.

50:17And then there are precise definitions

50:19of what we mean by phases of matter

50:21and that have been worked out fruitful over the decades.

50:26And we're discovering new states of matter all the time

50:29and kind of having to work at what we mean by matter.

50:33We're discovering the capabilities of matter

50:35to organize in interesting ways.

50:39And some of them, like liquid crystals,

50:46are important ingredients of life.

50:49Our cell membranes are liquid crystals,

50:51and that's very important to the way they work.

50:55Recently, there's been a development

50:57in where we're talking about states of matter

51:01that are not static, but that have dynamics,

51:06that have characteristic patterns,

51:09not only in space, but in time.

51:11These are called time crystals,

51:12and that's been a development

51:14that's just in the last decade or so.

51:17It's just really, really flourishing.

51:20And so is there a state of matter

51:25or a group of states of matter that corresponds to life?

51:31Maybe, but the answer can't be any more definite

51:34than the question.

51:35I mean, I gotta push back on the,

51:38those are just words.

51:39I mean, I disagree with you.

51:41The question points to a direction.

51:45The answer might be able to be more precise

51:49than the question, because just as you're saying,

51:53there is a, we could be discovering

51:56certain characteristics and patterns

51:59that are associated with a certain type of matter,

52:02macroscopically speaking,

52:04and that we can then be able to post facto say,

52:10this is, let's assign the word life to this kind of matter.

52:14I agree with that completely, that's what that's,

52:17but that's, so it's not a disagreement.

52:19It's very frequent in physics that, or in science,

52:23that words that are in common use

52:26get refined and reprocessed into scientific terms

52:31that's happened for things like force and energy.

52:35And so we, in a way, we find out

52:38what the useful definition is, or symmetry, for instance.

52:43And the common usage may be quite different

52:47from the scientific usage,

52:48but the scientific usage is special

52:52and takes on a life of its own,

52:53and we find out what the useful version of it is,

52:59the fruitful version of it is.

53:02So I do think, so in that spirit,

53:05I think if we can identify states of matter

53:10or linked states of matter that can carry on processes

53:18of self reproduction and development

53:23and information processing,

53:28we might be tempted to classify those things as life.

53:34Well, can I ask you about the craziest one,

53:36which is the one we know maybe least about,

53:41which is consciousness.

53:42Is it possible that there are certain kinds of matter

53:44would be able to classify as conscious,

53:50meaning like, so there's the panpsychists, right,

53:54who are the philosophers who kind of try to imply

53:57that all matter has some degree of consciousness,

54:01and you can almost construct like a physics of consciousness.

54:04Do you, again, we're in such early days of this,

54:09but nevertheless, it seems useful to talk about it.

54:13Is there some sense from a physics perspective

54:15to make sense of consciousness?

54:18Is there some hope?

54:19Well, again, consciousness is a very imprecise word

54:24and loaded with connotations that I think we should,

54:28we don't wanna start a scientific analysis with that,

54:31I don't think.

54:34It's often been important in science

54:38to start with simple cases and work up.

54:43Consciousness, I think what most people think of

54:45when you talk about consciousness is,

54:47okay, what am I doing in the world?

54:52This is my experience.

54:53I have a rich inner life and experience,

54:57and where is that in the equations?

54:59And I think that's a great question,

55:02a great, great question,

55:03and actually, I think I'm gearing up to spend part of,

55:07I mean, to try to address that in coming years.

55:10One version of asking that question,

55:12just as you said now,

55:14is what is the simplest formulation of that to study?

55:19I think I'm much more comfortable

55:20with the idea of studying self awareness

55:23as opposed to consciousness,

55:25because that sort of gets rid of the mystical aura of the thing.

55:30And self awareness is in simple,

55:33you know, I think contiguous at least

55:38with ideas about feedback.

55:41So if you have a system that looks at its own state

55:45and responds to it, that's a kind of self awareness.

55:50And more sophisticated versions

55:54could be like in information processing things,

55:57computers that look into their own internal state

56:00and do something about it.

56:03And I think that could also be done in neural nets.

56:08This is called recurrent neural nets,

56:10which are hard to understand and kind of a frontier.

56:15So I think understanding those

56:18and gradually building up a kind of profound ability

56:26to conceptualize different levels of self awareness.

56:32What do you have to not know?

56:33And what do you have to know?

56:34And when do you know that you don't know it?

56:36Or when do you, what do you think you know

56:38that you don't really know?

56:39And these, I think clarifying those issues,

56:44when we clarify those issues

56:47and get a rich theory around self awareness,

56:51I think that will illuminate the questions

56:55about consciousness in a way that, you know,

56:58scratching your chin and talking about qualia

57:00and blah, blah, blah, blah is never gonna do.

57:04Well, I also have a different approach to the whole thing.

57:06So there's, from a robotics perspective,

57:09you can engineer things that exhibit qualities

57:13of consciousness without understanding how things work.

57:19And from that perspective, you, it's like a back door,

57:25like enter through the psychology door.

§06Transcript · 57:28–1:08:33

57:28Precisely, I think we're on the same wavelength here.

57:32I think that, and let me just add one comment,

57:35which is I think we should try to understand consciousness

57:40as we experience it as, in evolutionary terms,

57:48and ask ourselves, why, why does it happen?

57:53This thing seems useful.

57:54Why is it useful?

57:55Why is it useful?

57:56Interesting question.

57:57I think we've got a conscious eyewatch here.

58:01Interesting question.

58:02Thank you, Siri.

58:03Okay.

58:08I'll get back to you later.

58:09The, and I think what we're gonna,

58:14I'm morally certain that what's gonna emerge

58:18from analyzing recurrent neural nets

58:21and robotic design and advanced computer design

58:26is that having this kind of looking at the internal state

58:33in a structured way that doesn't look at everything,

58:38this guy's has, it's encapsulated,

58:40looks at highly processed information,

58:42is very selective and makes choices

58:44without knowing how they're made.

58:45There's, there'll also be an unconscious.

58:47I think that that is gonna be,

58:49turn out to be really essential

58:51to doing efficient information processing.

58:55And that's why it evolved,

58:59because it's, it's, it's, it's helpful in,

59:03because brains come at a high cost.

59:06So there has to be, there has to be a good why.

59:09And there's a reason, yeah.

59:10They're rare in evolution and big brains

59:16are rare in evolution and they, they come at a big cost.

59:19You mean, if you, you, they, they,

59:22they have high metabolic demands.

59:27They require, you know, very active lifestyle,

59:30warm bloodedness and take, take away from the ability

59:36to support metabolism of digestion.

59:39And so, so it's, it's, it comes at a high cost.

59:42It has to, it has to pay back.

59:44Yeah, I think it has a lot of value in social interaction.

59:47So I actually am spending the rest of the day today

59:49and with our friends that are,

59:54our legged friends in robotic form at Boston Dynamics.

59:58And I think, so my probably biggest passion

60:03is human robot interaction.

60:05And it seems that consciousness from the perspective

60:09of the robot is very useful to improve

60:12the human robot interaction experience.

60:16The first, the display of consciousness,

60:18but then to me, there's a gray area

60:20between the display of consciousness and consciousness itself.

60:23If you think of consciousness

60:24from an evolutionary perspective,

60:26it seems like a useful tool in human communication, so.

60:29Yes, it's certainly, well,

60:32whatever consciousness is will turn out to be.

60:35I think addressing it through its use

60:39and working up from simple cases

60:42and also working up from engineering experience

60:45in trying to do efficient computation,

60:48including efficient management of social interactions

60:53is going to really shed light on these questions.

60:56As I said, in a way that sort of musing abstractly

60:59about consciousness never would.

61:01So as I mentioned, I talked to Sarah Walker

61:04and first of all, she says, hi, spoke very highly of you.

61:07One of her concerns about physics and physicists and humans

61:12is that we may not fully understand the system

61:16that we're inside of.

61:18Meaning like, there may be limits

61:22to the kind of physics we do

61:24in trying to understand the system of which we're part of.

61:28So like, the observer is also the observed.

61:33In that sense, it seems like

61:39our tools of understanding the world,

61:42I mean, this is mostly centered around the questions

61:44of what is life, trying to understand the patterns

61:47that are characteristic of life and intelligence,

61:51all those kinds of things.

61:53We're not using the right tools because we're in the system.

61:57Is there something that resonates with you there?

62:01Almost like...

62:02Well, yes, we have limitations, of course,

62:08in the amount of information we can process.

62:12On the other hand, we can get help from our Silicon friends

62:16and we can get help from all kinds of instruments

62:21that make up for our perceptual deficits.

62:25And we can use, at a conceptual level,

62:30we can use different kinds of concepts

62:32to address different kinds of questions.

62:35So I'm not sure exactly what problem she's talking about.

62:40It's a problem akin to an organism living in a 2D plane

62:45trying to understand a three dimensional world.

62:47Well, we can do that.

62:48I mean, in fact, for practical purposes,

62:53most of our experience is two dimensional.

62:55It's hard to move vertically.

62:57And yet we've produced conceptually

63:00a three dimensional symmetry

63:01and in fact, four dimensional space time.

63:05So by thinking in appropriate ways and using instruments

63:10and getting consistent accounts and rich accounts,

63:14we find out what concepts are necessary.

63:22And I don't see any end in sight of the process

63:25or any showstoppers because, let me give you an example.

63:32I mean, for instance, QCD,

63:35our theory of the strong interaction,

63:37has nice equations, which I helped to discover.

63:40What's QCD?

63:41Quantum chromodynamics.

63:42So it's our theory of the strong interaction,

63:47the interaction that is responsible for nuclear physics.

63:51So it's the interaction that governs

63:53how quarks and gluons interact with each other

63:55and make protons and neutrons

63:59and all the strong, the related particles

64:03and many things in physics.

64:05It's one of the four basic forces of nature

64:07as we presently understand it.

64:09And so we have beautiful equations,

64:15which we can test in very special circumstances

64:22using at high energies, at accelerators.

64:25So we're certain that these equations are correct.

64:28Prizes are given for it and so on.

64:30And people try to knock it down and they can't.

64:32Yeah, but the situations in which we can calculate

64:43the consequences of these equations are very limited.

64:46So for instance, no one has been able to demonstrate

64:52that this theory, which is built on quarks and gluons,

64:58which no one, which you don't observe,

65:01actually produces protons and neutrons

65:03and the things you do observe.

65:04This is called the problem of confinement.

65:07So no one's been able to prove that analytically

65:11in a way that a human can understand.

65:13On the other hand, we can take these equations

65:16to a computer, to gigantic computers and compute.

65:20And by God, you get the world from it.

65:25So these equations in a way that we don't understand

65:32in terms of human concepts, we can't do the calculations,

65:36but our machines can do them.

65:39So with the help of what I like to call our silicon friends

65:43and their descendants in the future,

65:46we can understand in a different way

65:50that allows us to understand more.

65:53But I don't think we'll ever, no human is ever going

65:56to be able to solve those equations in the same way.

66:00So, but I think that's, you know,

66:04when we find limitations to our natural abilities,

66:09we can try to find workarounds.

66:12And sometimes that's appropriate concepts.

66:15Sometimes it's appropriate instruments.

66:17Sometimes it's a combination of the two.

66:19But I think it's premature to get defeatist about it.

66:26I don't see any logical contradiction

66:32or paradox or limitation

66:35that will bring this process to a halt.

66:38Well, I think the idea is to continue thinking

66:40outside the box in different directions,

66:42meaning just like how the math allows us

66:45to think in multiple dimensions

66:47outside of our perception system, sort of thinking,

66:54you know, coming up with new tools

66:55of mathematics or computation or all those kinds of things

66:58to take different perspectives on our universe.

67:04Well, I'm all for that.

67:05You know, and I kind of have even elevated into a principle

67:08which is of complementarity following Bohr

67:11that you need different ways of thinking

67:16even about the same things

67:18in order to do justice to their reality

67:21and answer different kinds of questions about them.

67:23I mean, we've several times alluded to the fact

67:27that human beings are hard to understand

67:30and the concepts that you use to understand human beings

67:34if you wanna prescribe drugs for them

67:37or see what's gonna happen if they move very fast

67:42or are exposed to radiation.

67:45And so that requires one kind of thinking

67:47that's very physical based on the fact

67:52that the materials that were made out of.

67:55On the other hand, if you want to understand

67:57how a person's going to behave

67:59in a different kind of situation,

68:02you need entirely different concepts from psychology

68:06and there's nothing wrong with that.

68:08You can have very different ways

68:09of addressing the same material

68:11that are useful for different purposes, right?

68:14Can you describe this idea

68:16which is fascinating of complementarity a little bit?

68:18Sort of first of all, what state is the principle?

68:25What is it?

68:26And second of all, what are good examples

68:29starting from quantum mechanics?

68:30You used to mention psychology.

68:32Let's talk about this more.

§07Transcript · 1:08:33–1:20:42

68:33It's like in your new book

68:34one of the most fascinating ideas actually.

68:38I think it's a wonderful, yeah.

68:40To me it's, well, it's the culminating chapter of the book

68:43and I think since the whole book is about the big lessons

68:48or big takeaways from profound understanding

68:52of the physical world that we've achieved,

68:56including that it's mysterious in some ways,

69:01this was the final overarching lesson, complementarity.

69:06Lesson, complementarity and it's a approach.

69:16So unlike some of these other things

69:18which are just facts about the world,

69:20like the world is both big and small

69:22and different sizes and is big but we're not small,

69:26things we talked about earlier

69:28and the fact that the universe is comprehensible

69:30and how complexity could emerge from simplicity

69:33and so those things are in the broad sense

69:37facts about the world.

69:39Complementarity is more an attitude towards the world

69:42than encouraged by the facts about the world.

69:46And it's the concept or the approach

69:54or the realization that it can be appropriate

69:59and useful and inevitable and unavoidable

70:02to use very different descriptions of the same object

70:08or the same system or the same situation

70:12to answer different kinds of questions

70:15that may be very different

70:17and even mutually uninterpretable,

70:22immutually incomprehensible.

70:27But both correct somehow.

70:28But both correct and sources of different kinds of insight

70:32which is so weird.

70:34But it seems to work in so many cases.

70:36It works in many cases and I think it's a deep fact

70:41about the world and how we should approach it.

70:44It's most rigorous form where it's actually a theorem

70:50if quantum mechanics is correct,

70:53occurs in quantum mechanics

70:55where the primary description of the world

71:00is in terms of wave functions.

71:03But let's not talk about the world.

71:04Let's just talk about a particle, an electron.

71:09The primary description of that electron

71:12is its wave function.

71:14And the wave function can be used to predict

71:19where it's gonna be.

71:21If you observe, it'll be in different places

71:24with different probabilities or how fast it's moving.

71:27And it'll also be moving in different ways

71:31with different probabilities.

71:32That's what quantum mechanics says.

71:35And you can predict either set of probabilities

71:38if you know what's gonna happen

71:40if I make an observation of the position or the velocity.

71:48So the wave function gives you ways of doing both of those.

71:51But to do it, to get those predictions,

71:54you have to process the wave function in different ways.

71:57You process it one way for position

71:59and in a different way for momentum.

72:01And those ways are mathematically incompatible.

72:05It's like you have a stone

72:08and you can sculpt it into a Venus de Milo

72:11or you can sculpt it into David, but you can't do both.

72:18And that's an example of complementarity.

72:20To answer different kinds of questions,

72:22you have to analyze the system in different ways

72:25that are mutually incompatible,

72:29but both valid to answer different kinds of questions.

72:32So in that case, it's a theorem,

72:34but I think it's a much more widespread phenomena

72:38that applies to many cases

72:40where we can't prove it as a theorem,

72:42but it's a piece of wisdom, if you like,

72:46and appears to be a very important insight.

72:53And if you ignore it,

72:53you can get very confused and misguided.

73:02Do you think this is a useful hack

73:06for ideas that we don't fully understand?

73:10Or is this somehow a fundamental property

73:13of all or many ideas,

73:16that you can take multiple perspectives

73:19and they're both true?

73:20Well, I think it's both.

73:24So it's both the answer to all questions.

73:26Yes, that's right.

73:27It's not either or, it's both.

73:28It's paralyzing to think that we live in a world

73:32that's fundamentally surrounded by complementary ideas.

73:39Because we somehow want to attach ourselves

73:44to absolute truths,

73:45and absolute truths certainly don't like the idea

73:48of complementarity.

73:50Yes, Einstein was very uncomfortable with complementarity.

73:53And in a broad sense,

73:55the famous Bohr Einstein debates

73:59revolved around this question

74:00of whether the complementarity

74:03that is a foundational feature of quantum mechanics,

74:08as we have it,

74:10is a permanent feature of the universe

74:16and our description of nature.

74:19And so far, quantum mechanics wins.

74:22And it's gone from triumph to triumph.

74:26Whether complementarity is rock bottom,

74:28I guess, you can never be sure.

74:31I mean, but it looks awfully good

74:34and it's been very successful.

74:35And certainly, complementarity has been extremely useful

74:40and fruitful in that domain,

74:43including some of Einstein's attempts to challenge it

74:50with the famous Einstein Podolsky Rosen experiment

74:55turned out to be confirmations

74:57that have been useful in themselves.

75:03But so thinking about these things was fruitful,

75:05but not in the way that Einstein hoped.

75:07Yeah, so as I said, in the case of quantum mechanics

75:19and this dilemma or dichotomy

75:26between processing the wave function in different ways,

75:29it's a theorem.

75:30They're mutually incompatible

75:31and the physical correlate of that

75:32is the Heisenberg uncertainty principle

75:35you can't have position and momentum determined at once.

75:41But in other cases, like one that I like to think about

75:48or like to point out as an example

75:50is free will and determinism.

75:52It's much less of a theorem

75:57and more a kind of way of thinking about things

76:06that I think is reassuring

76:10and avoids a lot of unnecessary quarreling and confusion.

76:16The quarreling I'm okay with

76:17and the confusion I'm okay with,

76:18I mean, people debate about difficult ideas,

76:21but the question is whether it could be

76:24almost a fundamental truth.

76:26I think it is a fundamental truth.

76:28That free will is both an illusion and not.

76:32Yes, I think that's correct.

76:35There's a reason why people say quantum mechanics is weird

76:39and complementarity is a big part of that.

76:45To say that our actual whole world is weird,

76:48the whole hierarchy of the universe is weird

76:52in this kind of particular way,

76:54and it's quite profound, but it's also humbling

77:03because it's like we're never going to be on sturdy ground

77:06in the way that humans like to be.

77:09It's like you have to embrace that this whole thing

77:13is like unsteady mess.

77:18It's one of many lessons in humility

77:21that we run into in profound understanding of the world.

77:28The Copernican revolution was one,

77:30that the earth is not the center of the universe.

77:35Darwinian evolution is another,

77:36that humans are not the pinnacle of God's creation and the apparent result

77:53of deep understanding of physical reality,

77:57that mind emerges from matter and there's no call

78:05on special life forces or souls.

78:09These are all lessons in humility,

78:11and I actually find complementarity a liberating concept.

78:19It's, okay, you know, we...

78:21Yeah, it is in a way.

78:22That is what I remember.

78:28There's a story about Dr. Johnson,

78:30and he's talking with Boswell,

78:32and Boswell was, they were discussing a sermon

78:36that they'd both heard,

78:37and the sort of culmination of the sermon was the speaker saying,

78:43I accept the universe.

78:45And Dr. Johnson said, well, damn well better.

78:50And there's a certain joy in accepting the universe

78:55because it's mind expanding.

78:57And to me, complementarity also suggests tolerance,

79:10suggests opportunities for understanding things

79:15in different ways that add to rather than detract

79:22from understanding.

79:25So I think it's an opportunity for mind expansion

79:29and demanding that there's only one way

79:33to think about things can be very limiting.

79:36On the free will one, that's a trippy one, though.

79:38To think like I am the decider of my own actions

79:43and at the same time I'm not is tricky to think about,

79:49but there does seem to be some kind of profound truth in that.

79:53I get, well, I think it is tied up.

79:56It will turn out to be tied up when we understand things better

80:00with these issues of self awareness and where we get,

80:04what we perceive as making choices,

80:06what does that really mean and what's going on under the hood.

80:12But I'm speculating about a future understanding

80:15that's not in place at present.

80:17Your sense there will always be,

80:19like as you dig into the self awareness thing,

80:22there'll always be some places

80:24where complementarity is gonna show up.

80:26Oh, definitely, yeah.

80:28I mean, there will be, how should I say?

80:31There'll be kind of a God's eye view

80:33which sees everything that's going on

80:37in the computer or the brain.

80:40And then there's the brain's own view

§08Transcript · 1:20:42–1:32:34

80:42or the central processor or whatever it is,

80:46what we call the self, the consciousness,

80:50that's only aware of a very small part of it.

80:53And those are very different.

80:54Those are, so the God's eye view can be deterministic

80:59while the self view sees free will.

81:07I'm pretty sure that's how it's gonna work out actually.

81:11But as it stands, free will is a concept

81:15that we definitely, at least I feel I definitely experience,

81:19I can choose to do one thing then another.

81:21And other people I think are sufficiently similar to me

81:24that I trust that they feel the same way.

81:30And it's an essential concept in psychology

81:33and law and so forth.

81:35But at the same time, I think that mind emerges from matter

81:42and that there's an alternative description of matter

81:47that's up to subtleties about quantum mechanics,

81:51which I don't think are relevant here,

81:53really is deterministic.

81:56Let me ask you about some particles.

81:57Okay.

81:59First the absurd question,

82:00almost like a question that like Plato would ask.

82:04What is the smallest thing in the universe?

82:08As far as we know, the fundamental particles

82:13out of which we build our most successful description

82:17of nature are points.

82:20They don't have any internal structure.

82:27So that's as small as can be.

82:31So what does that mean operationally?

82:34That means that they obey equations that describe entities

82:39that are singular concentrations of energy,

82:46momentum, angular momentum,

82:47the things that particles have,

82:50but localized at individual points.

82:53Now that mathematical structure

82:57is only revealed partially in the world

83:01because to process the wave function

83:04in a way that accesses information about the precise

83:09position of things, you have to apply a lot of energy

83:12and that's an idealization

83:14and you can apply infinite amount of energy

83:16to determine a precise position.

83:19But at the mathematical level,

83:23we build the world out of particles that are points.

83:26So do they actually exist and what are we talking about?

83:29Oh, they exist.

83:30So let me ask sort of do quarks exist?

83:33Yes, do electrons exist?

83:36Yes, do photons exist?

83:37Yes.

83:38But what does it mean for them to exist?

83:39Okay, so well, the hard answer to that,

83:43the precise answer is that we construct the world

83:49out of equations that contain entities

83:51that are reproducible,

83:56that exist in vast numbers throughout the universe,

84:00that have definite properties of mass,

84:05spin and a few others that we call electrons

84:13and what an electron is is defined by the equations

84:17that it satisfies theoretically

84:19and we find that there are many, many exemplars

84:24of that entity in the physical world.

84:28So in the case of electrons,

84:31we can isolate them and study them

84:34and individual ones in great detail

84:36and we can check that they all actually are identical

84:42and that's why chemistry works and yes.

84:45So in that case, it's very tangible.

84:49Similarly with photons,

84:51you can study them individually, the units of light

84:55and nowadays, it's very practical

84:59to study individual photons

85:01and determine their spin and their other basic properties

85:05and check out the equations in great detail.

85:11For quarks and gluons,

85:13which are the other two main ingredients

85:16of our model of matter that's so successful,

85:22it's a little more complicated

85:23because the quarks and gluons that appear in our equations

85:29don't appear directly as particles you can isolate

85:33and study individually.

85:35They always occur within what are called bound states

85:41or structures like protons.

85:43A proton, roughly speaking, is composed of three quarks

85:48and a lot of gluons but we can detect them

85:50in a remarkably direct way actually nowadays,

85:54whereas at relatively low energies,

85:58the behavior of quarks is complicated.

86:00At high energies, they can propagate through space

86:05relatively freely for a while and we can see their tracks.

86:11So ultimately, they get recaptured into protons

86:14and other mesons and funny things

86:17but for a short time, they propagate freely

86:21and while that happens, we can take snapshots

86:25and see their manifestations.

86:29Actually, this kind of thing is exactly

86:31what I got the Nobel Prize for,

86:33predicting that this would work.

86:35And similarly for gluons,

86:36although you can't isolate them as individual particles

86:41and study them in the same way that we study electrons,

86:43say, you can use them theoretically as entities

86:51out of which you build tangible things

86:57that we actually do observe

86:59but also you can, at accelerators at high energy,

87:03you can liberate them for brief periods of time

87:06and study and get convincing evidence

87:10that they leave tracks and you can get convincing evidence

87:15that they were there and have the properties

87:17that we wanted them to have.

87:19Can we talk about asymptotic freedom,

87:21this very idea that you won the Nobel Prize for?

87:24Yeah.

87:25So it describes a very weird effect to me,

87:30the weird in the following way.

87:33So the way I think of most forces or interactions,

87:38the closer you are, the stronger the effect,

87:43the stronger the force, right?

87:46With quarks, the close they are,

87:50the less so the strong interaction.

87:53And in fact, they're basically act like free particles

87:58when they're very close.

88:00That's right, yes.

88:01But this requires a huge amount of energy.

88:04Like can you describe me why, how does this even work?

88:11How weird it is?

88:12A proper description must bring in quantum mechanics

88:18and relativity and it's,

88:21so a proper description and equations,

88:25so a proper description really is probably more

88:29than we have time for and require quite a bit of patience

88:34on your part, but.

88:35How does relativity come into play?

88:37Wait, wait a minute.

88:39Relativity is important because when we talk about

88:48trying to think about short distances,

88:51we have to think about very large momenta

88:55and very large momenta are connected

88:56to very large energy in relativity.

88:59And so the connection between how things behave

89:02at short distances and how things behave at high energy

89:06really is connected through relativity

89:09in sort of a slightly backhanded way.

89:13Quantum mechanics indicates that short,

89:16to get to analyze short distances,

89:20you need to bring in probes that carry a lot of momentum.

89:26This again is related to uncertainty

89:29because it's the fact that you have to bring in

89:31a lot of momentum that interferes with the possibility

89:36of determining position and momentum at the same time.

89:40If you want to determine position,

89:41you have to use instruments that bring in a lot of momentum.

89:45And because of that, those same instruments

89:48can't also measure momentum

89:50because they're disturbing the momentum that,

89:53and then the momentum brings in energy and yeah.

89:56So that there's also the effect that asymptotic freedom

89:59comes from the possibility of spontaneously making

90:08quarks and gluons for short amounts of time

90:12that fluctuate into existence and out of existence.

90:16And the fact that that can be done

90:21with a very little amount of energy

90:23and uncertainty and energy translates

90:26into uncertainty and time.

90:27So if you do that for a short time, you can do that.

90:31Well, it's all comes in a package.

90:35So I told you it would take a while to really explain,

90:39but the results can be understood.

90:44I mean, we can state the results pretty simply, I think.

90:48So in everyday life, we do encounter some forces

90:53that increase with distance

90:56and kind of turn off at short distances.

90:59That's the way rubber bands work, if you think about it,

91:02or if you pull them hard, they resist,

91:06but they get flabby if the rubber band is not pulled.

91:12And so there are, that can happen in the physical world,

91:17but what's really difficult is to see

91:19how that could be a fundamental force

91:21that's consistent with everything else we know.

91:24And that's what asymptotic freedom is.

91:28It says that there's a very particular kind

91:33of fundamental force that involves special particles

91:37called gluons with very special properties

91:40that enables that kind of behavior.

91:43So there were experiment, at the time we did our work,

91:47there were experimental indications

91:49that quarks and gluons did have this kind of property,

91:54but there were no equations

91:56that were capable of capturing it.

91:59And we found the equations and showed how they work

92:02and showed how they, that they were basically unique.

92:06And this led to a complete theory

92:08of how the strong interaction works,

92:09which is the quantum chromodynamics we mentioned earlier.

92:14And so that's the phenomenon that quarks and gluons

92:23interact very, very weakly when they're close together.

92:26That's connected through relativity

92:29with the fact that they also interact very, very weakly

92:32at high energies.

§09Transcript · 1:32:34–1:42:51

92:34So if you have, so at high energies,

92:37the simplicity of the fundamental interaction gets revealed.

92:42At the time we did our work,

92:43the clues were very subtle,

92:46but nowadays at what are now high energy accelerators,

92:50it's all obvious.

92:51So we would have had a much,

92:52well, somebody would have had a much easier time

92:5520 years later, looking at the data,

92:57you can sort of see the quarks and gluons.

92:59As I mentioned, they leave these short tracks

93:02that would have been much, much easier,

93:04but from fundamental, from indirect clues,

93:08we were able to piece together enough

93:10to make that behavior a prediction

93:13rather than a post diction, right?

93:15So it becomes obvious at high energies.

93:17It becomes very obvious.

93:19When we first did this work,

93:21it was frontiers of high energy physics

93:24and at big international conferences,

93:27there would always be sessions on testing QCD

93:30and whether this proposed description

93:34of the strong interaction was in fact correct and so forth.

93:37And it was very exciting.

93:39But nowadays the same kind of work,

93:44but much more precise with calculations

93:48to more accuracy and experiments

93:50that are much more precise

93:54and comparisons that are very precise.

93:57Now it's called calculating backgrounds

93:59because people take this for granted

94:03and wanna see deviations from the theory,

94:06which would be the new discoveries.

94:09Yeah, the cutting edge becomes a foundation

94:11and the foundation becomes boring.

94:13Yes.

94:15Is there some, for basic explanation purposes,

94:19is there something to be said about strong interactions

94:23in the context of the strong nuclear force

94:26for the attraction between protons and neutrons

94:30versus the interaction between quarks within protons?

94:35Well, quarks and gluons have the same relation

94:40basically to nuclear physics

94:43as electrons and photons have

94:46to atomic and molecular physics.

94:49So atoms and photons are the dynamic entities

94:56that really come into play in chemistry and atomic physics.

95:01Of course, you have to have the atomic nuclei,

95:03but those are small and relatively inert,

95:07really the dynamical part.

95:09And for most purposes of chemistry,

95:12you just say that you have this tiny little nucleus,

95:14which QCD gives you.

95:17Don't worry about it.

95:17It just, it's there.

95:19The real action is the electrons moving around

95:22and exchanging and things like that.

95:26Okay, but we want it to understand the nucleus too.

95:29And so atoms are sort of quantum mechanical clouds

95:36of electrons held together by electrical forces,

95:38which is photons.

95:39And then this radiation,

95:40which is another aspect of photons.

95:43That's where all the fun happens

95:44is the electrons and the photons.

95:45Yeah, that's right.

95:47And the nucleus are kind of the,

95:51well, they give the positive charge

95:53and most of the mass of matter,

95:55but they don't, since they're so heavy,

96:01they don't move very much in chemistry.

96:03And I'm oversimplifying drastically.

96:07They're not contributing much to the interaction in chemistry.

96:12For most purposes in chemistry,

96:13you can just idealize them as concentrations

96:16of positive mass and charge that are,

96:20you don't have to look inside,

96:22but people are curious what's inside.

96:24And that was a big thing on the agenda

96:29of 20th century physics starting in the 19,

96:32well, starting with the 20th century

96:34and unfolding throughout of trying to understand

96:38what forces held the atomic nucleus together,

96:41what it was and so.

96:44Anyway, the story that emerges from QCD

96:49is that very similar to the way that,

96:55well, broadly similar to the way

96:57that clouds of electrons held together

97:01by electrical forces give you atoms

97:04and ultimately molecules.

97:08Protons and neutrons are like atoms

97:13made now out of quarks, quark clouds held together

97:17by gluons, which are like the photons

97:20that give the electric forces,

97:23but this is giving a different force, the strong force.

97:26And the residual forces between protons and neutrons

97:31that are leftover from the basic binding

97:37are like the residual forces between atoms

97:40that give molecules, but in the case of protons and neutrons,

97:43it gives you atomic nuclei.

97:45So again, for definitional purposes,

97:48QCD, quantum chromodynamics,

97:51is basically the physics of strong interaction.

97:54Yeah, we understand, we now would understand,

97:56I think most physicists would say

97:58it's the theory of quarks and gluons

98:02and how they interact.

98:04But it's a very precise, and I think it's fair to say,

98:07very beautiful theory based on mathematical symmetry

98:11of a high order, and another thing that's beautiful

98:16about it is that it's kind of

98:22in the same family as electrodynamics.

98:26The conceptual structure of the equations are very similar.

98:31They're based on having particles that respond to charge

98:34in a very symmetric way.

98:37In the case of electrodynamics,

98:39it's photons that respond to electric charge.

98:42In the case of quantum chromodynamics,

98:44there are three kinds of charge that we call colors,

98:47but they're nothing like colors.

98:49They really are like different kinds of charge.

98:51But they rhyme with the same kind of,

98:54like it's similar kind of dynamics.

98:56Similar kind of dynamics.

98:57I'd like to say that QCD is like QED on steroids.

99:02And instead of one photon, you have eight gluons.

99:05Instead of one charge, you have three color charges.

99:09But there's a strong family resemblance between them.

99:13But the context in which QCD does this thing

99:16is it's much higher energies.

99:19Like that's where it comes to life.

99:20Well, it's a stronger force,

99:22so that to access how it works and kind of pry things apart,

99:28you have to inject more energy.

99:30And so that gives us, in some sense,

99:35a hint of how things were in the earlier universe.

99:39Yeah, well, in that regard,

99:41asymptotic freedom is a tremendous blessing

99:43because it means things get simpler at high energy.

99:48The universe was born free.

99:50Born free.

99:50That's very good, yes.

99:52Universe was born.

99:53So in atomic physics,

99:56a similar thing happens in the theory of stars.

99:59Stars are hot enough that the interactions

100:03between electrons and photons, they're liberated.

100:07They don't form atoms anymore.

100:08They make a plasma,

100:09which in some ways is simpler to understand.

100:12You don't have complicated chemistry.

100:14And in the early universe, according to QCD,

100:18similarly atomic nuclei dissolved

100:20and take the constituent quarks and gluons,

100:22which are moving around very fast

100:24and interacting in relatively simple ways.

100:27And so this opened up the early universe

100:30to scientific calculation.

100:33Can I ask you about some other weird particles

100:35that make up our universe?

100:37What are axions?

100:39And what is the strong CP problem?

100:42Okay, so let me start with what the strong CP problem is.

100:49First of all, well, C is charge conjugation,

100:53which is the transformation,

100:57the notional transformation, if you like,

100:59that changes all particles into their antiparticles.

101:03And the concept of C symmetry,

101:09charge conjugation symmetry, is that if you do that,

101:13you find the same laws that would work.

101:16So the laws are symmetric if the behavior

101:20that particles exhibit is the same

101:22as the behavior you get with all their antiparticles.

101:27And then P is parity,

101:31which is also called spatial inversion.

101:35It's basically looking at a mirror universe

101:39and saying that the laws that are obeyed

101:41in a mirror universe, when you look,

101:44that the mirror images obey the same laws

101:46as the sources of their images.

101:50There's no way of telling left from right, for instance,

101:52that the laws don't distinguish between left and right.

101:55Now, in the mid 20th century,

102:00people discovered that both of those are not quite true.

102:05Really, the equation that the mirror universe,

102:08the universe that you see in a mirror

102:15is not gonna obey the same laws

102:18as the universe that we actually interpret.

102:23You would be able to tell

102:26if you did the right kind of experiments,

102:28which was the mirror and which was the real thing.

102:33Anyway, that.

102:34That's the parity and they show

102:36that the parity doesn't necessarily hold.

102:37It doesn't quite hold.

102:41Examining what the exceptions are turned out to be,

102:45to lead to all kinds of insight

102:47about the nature of fundamental interactions,

102:49especially properties of neutrinos

§10Transcript · 1:42:51–1:52:42

102:51and the weak interaction, it's a long story.

102:53But it's a very, it's a.

102:55So you just define the C and the P,

102:57the conjugation, the charge conjugation.

102:59Now that I've done that, I wanna.

103:00What's the problem?

103:01Shove them off.

103:02Okay, great.

103:04Because it's easier to talk about T,

103:06which is time reversal symmetry.

103:08We have very good reasons to think CPT

103:13is an accurate symmetry of nature.

103:17It's on the same level as relativity

103:19and quantum mechanics, basically.

103:20So that better be true.

103:23Or else we.

103:24So it's symmetric when you.

103:26When you do.

103:26When you do conjugation parity and time.

103:28And time and space reversal.

103:30If you do all three,

103:32then you get the same physical consequences.

103:35Now, so, but that means that CP is equivalent to T.

103:39But what's observed in the world

103:41is that T is not quite an accurate symmetry of nature,

103:45either.

103:46So most phenomena of, at the fundamental level.

103:52So interactions among elementary particles

103:54and the basic gravitational interaction.

103:59If you ran them backwards in time,

104:03you'd get the same laws.

104:05So if, again, going back.

104:08This time we don't talk about a mirror,

104:11but we talk about a movie.

104:13If you take a movie and then run it backwards,

104:18that's the time reversal.

104:21It's good to think about a mirror in time.

104:23Yeah, it's like a mirror in time.

104:25If you run the movie backwards,

104:29it would look very strange

104:30if you were looking at complicated objects

104:32and a Charlie Chaplin movie or whatever.

104:37It would look very strange if you ran it backwards in time.

104:40But at the level of basic interactions,

104:43if you were able to look at the atoms

104:46and the quarks involved, they would obey the same laws.

104:49They do a very good approximation, but not exactly.

104:53So this is not exactly, that means you could tell.

104:55You could tell, but you'd have to do very, very

104:59subtle experiments with at high energy accelerators

105:04to take a movie that looked different

105:06when you ran it backwards.

105:08This was a discovery by two great physicists

105:13named Jim Cronin and Val Fitch in the mid 1960s.

105:20Previous to that, over all the centuries

105:22of development of physics with all its precise laws,

105:25they did seem to have this gratuitous property

105:30that they look the same if you run the equations backwards.

105:33It's kind of an embarrassing property actually

105:35because life isn't like that.

105:38So empirical reality does not have this imagery

105:41in any obvious way.

105:42And yet the laws did.

105:44It's almost like the laws of physics

105:46are missing something fundamental about life

105:48if it holds that property, right?

105:51Well, that's the embarrassing nature of it.

105:54Yeah, it's embarrassing.

105:55Well, people worked hard at what's,

106:01this is a problem that's thought to belong

106:04to the foundations of statistical mechanics

106:07or the foundations of thermodynamics

106:10to understand how behavior,

106:14which is grossly not symmetric

106:18with respect to reversing the direction of time

106:21in large objects, how that can emerge from equations

106:24which are symmetric with respect to changing

106:28the direction of time to a very good approximation.

106:31And that's still an interesting endeavor.

106:33That's interesting.

106:35And actually it's an exciting frontier of physics now

106:38to sort of explore the boundary

106:40between when that's true and when it's not true.

106:42When you get to smaller objects

106:44and exceptions like time crystals.

106:47I definitely have to ask you about time crystals

106:49in a second here.

106:50But so the CP problem and T,

106:53so there's all of these.

106:55We're in danger of infinite regress,

106:57but we have to convert soon.

106:59So.

107:00Can't possibly be turtles all the way down.

107:02We're gonna get to the bottom turtle.

107:03So it became,

107:06so it got to be a real,

107:08I mean, it's a really puzzling thing

107:11why the laws should have this very odd property

107:15that we don't need.

107:16And in fact, it's kind of an embarrassment

107:20in addressing empirical reality.

107:22But it seemed to be almost,

107:24it seemed to be exactly true for a long time.

107:26And then almost true.

107:29And in way, almost true is even,

107:33is more disturbing than exactly true

107:35because exactly true,

107:37it could have been just a fundamental feature of the world.

107:39And at some level you just have to take it as it is.

107:42And if it's a beautiful, easily articulatable regularity,

107:47you could say that, okay,

107:48that's fine as a fundamental law of nature.

107:51But to say that it's approximately true,

107:53but not exactly, that's weird.

107:56So, and then, so there was great progress

108:00in the late part of the 20th century

108:06in getting to an understanding

108:09of fundamental interactions in general

108:11that shed light on this issue.

108:14It turns out that the basic principles of relativity

108:20and quantum mechanics,

108:22plus the kind of high degree of symmetry that we found,

108:27the so called gauge symmetry

108:28that characterizes the fundamental interactions,

108:31when you put all that together,

108:33it's a very, very constraining framework.

108:37And it has some indirect consequences

108:42because the possible interactions are so constrained.

108:45And one of the indirect consequences

108:48is that the possibilities for violating the symmetry

108:54between forwards and backwards in time are very limited.

108:57They're basically only two.

109:01And one of them occurs and leads to a very rich theory

109:05that explains the Cronin Fish experiment

109:07and a lot of things that have been done subsequently

109:09has been used to make all kinds of successful predictions.

109:13So that's turned out to be a very rich interaction.

109:19It's esoteric and the effects only show up at accelerators

109:23and are small and so on,

109:24but they might've been very important in the early universe

109:26and lead to them be connected to the asymmetry

109:29between matter and antimatter in the present universe.

109:32And so, but that's another digression.

109:36The point is that that was fine.

109:40That was a triumph to say

109:41that there was one possible kind of interaction

109:44that would violate time reversal symmetry.

109:47And sure enough, there it is.

109:49But the other kind doesn't occur.

109:54So we still got a problem.

109:55Why doesn't it occur?

109:59So we're close to really finally understanding

110:01this profound gratuitous feature of the world

110:04that is almost but not quite symmetric

110:08under reversing the direction of time, but not quite there.

110:12And to understand that last bit

110:18is a challenging frontier of physics today.

110:22And we have a promising proposal for how it works,

110:27which is a kind of theory of evolution.

110:31So there's this possible interaction,

110:35which we call a coupling,

110:37and there's a numerical quantity

110:39that tells us how strong that is.

110:41And traditionally in physics,

110:43we think of these kinds of numerical quantities

110:46as constants of nature that you just have to put them in.

110:54From experiment, they have a certain value and that's it.

110:57And who am I to question what God doing?

111:01They're just constant.

111:02Well, they seem to be just constants.

111:04I'm just wondering.

111:06But in this case,

111:10it's been fruitful to think and work out a theory

111:15where that strength of interaction

111:22is actually not a constant.

111:23It's a fun, it's a field.

111:27It's a, fields are the fundamental ingredients

111:31of modern physics.

111:32Like there's an electron field,

111:34there's a photon field,

111:35which is also called the electromagnetic field.

111:37And so all of these particles

111:39are manifestations of different fields.

111:41And there could be a field,

111:45something that depends on space and time.

111:47So a dynamical entity instead of just a constant here.

111:53And if you do things in a nice way,

111:57that's very symmetric,

111:58very much suggested aesthetically by the theory.

112:02But the theory we do have,

112:05then you find that you get a field

112:11which as it evolves from the early universe,

112:17settles down to a value

112:22that's just right to make the laws

112:27very nearly exact, invariant or symmetric

112:32with respect to reversal of time.

112:33It might appear as a constant,

112:34but it's actually a field that evolved over time.

112:36It evolved over time, okay.

112:38But when you examine this proposal in detail,

§11Transcript · 1:52:42–2:02:44

112:42you find that it hasn't quite settled down to exactly zero.

112:47There it's still,

112:48the field is still moving around a little bit.

112:52And because the motion is so,

112:55the motion is so difficult.

112:59The material is so rigid.

113:00And this material,

113:01the field that fills all space is so rigid.

113:03Even small amounts of motion can involve lots of energy.

113:08And that energy takes the form of particles,

113:14fields that are in motion

113:16are always associated with particles.

113:18And those are the axioms.

113:20And if you calculate how much energy

113:23is in these residual oscillations,

113:26this axiom gas that fills all the universe,

113:30if this fundamental theory is correct,

113:32you get just the right amount

113:36to make the dark matter that astronomers want.

113:39And it has just the right properties.

113:41So I'd love to believe that.

113:44So that might be a thing that unlocks,

113:47might be the key to understanding dark matter.

113:50Yeah, I'd like to think so.

113:51And many, many physicists are coming around

113:53to this point of view,

113:54which I've been a voice in the wilderness.

113:58I was a voice in the wilderness for a long time,

114:00but now it's become very popular, maybe even dominant.

114:04So almost like,

114:05so this axion particle slash field

114:10would be the thing that explains dark matter.

114:13It explains, yeah,

114:14would solve this fundamental question of finally,

114:17of why the laws are almost, but not quite exactly the same

114:24if you run them backwards in time.

114:26And then seemingly in a totally different

114:30conceptual universe,

114:32it would also provide,

114:35give us an understanding of the dark matter.

114:38That's not what it was designed for.

114:41And the theory wasn't proposed with that in mind,

114:45but when you work out the equations, that's what you get.

114:47That's always a good sign.

114:49Yes.

114:51I think I vaguely read somewhere

114:53that there may be early experimental validation of axion.

114:59Is that, am I reading the wrong?

115:03Well, there've been quite a few false alarms

115:05and I think there are some of them still,

115:08people desperately wanna find this thing.

115:10And, but I don't think any of them are convincing

115:15at this point,

115:16but there are very ambitious experiments

115:20and kind of new,

115:23you have to design new kinds of antennas

115:24that are capable of detecting these predicted particles.

115:28And it's very difficult.

115:29They interact very, very weakly.

115:31If it were easy, it would have been done already.

115:33But I think there's good hope

115:37that we can get down to the required sensitivity

115:40and actually test whether these ideas are right

115:44in coming years or maybe decades.

115:47And then understand one of the big mysteries,

115:50like literally big in terms of its fraction

115:53of the universe is dark matter.

115:55Yes.

115:56Let me ask you about, you mentioned a few times,

115:59time crystals.

116:01What are they?

116:02These things are, it's a very beautiful idea

116:05when we start to treat space and time

116:10as similar frameworks.

116:13Yes, right.

116:14Physical phenomena.

116:15Right, that's what motivated it.

116:17First of all, what are crystals?

116:19Yeah.

116:20And what are time crystals?

116:20Okay, so crystals are orderly arrangements

116:24of atoms in space.

116:27And many materials,

116:30if you cool them down gently, will form crystals.

116:38And so we say that that's a state of matter

116:43that forms spontaneously.

116:45And an important feature of that state of matter

116:50is that the end result, the crystal,

116:53has less symmetry than the equations

117:01that give rise to the crystal.

117:03So the equations, the basic equations of physics

117:09are the same if you move a little bit.

117:12So you can move, they're homogeneous,

117:15but crystals aren't.

117:16The atoms are in particular place,

117:18so they have less symmetry.

117:20And time crystals are the same thing in time, basically.

117:27But of course, so it's not positions of atoms,

117:30but it's orderly behavior that certain states of matter

117:38will arrange themselves into spontaneously

117:41if you treat them gently

117:44and let them do what they want to do.

117:46But repeat in that same way indefinitely.

117:50That's the crystalline form.

117:51You can also have time liquids,

117:54or you can have all kinds of other states of matter.

117:57You can also have space time crystals

117:58where the pattern only repeats if with each step of time,

118:03you also move at a certain direction in space.

118:07So yeah, basically it's states of matter

118:12that displace structure in time spontaneously.

118:17So here's the difference.

118:21When it happens in time,

118:24it sure looks a lot like it's motion,

118:27and if it repeats indefinitely,

118:29it sure looks a lot like perpetual motion.

118:32Yeah.

118:32Like looks like free lunch.

118:35And I was told that there's no such thing as free lunch.

118:39Does this violate laws of thermodynamics?

118:42No, but it requires a critical examination

118:45of the laws of thermodynamics.

118:47I mean, let me say on background

118:49that the laws of thermodynamics

118:51are not fundamental laws of physics.

118:55There are things we prove

118:58under certain circumstances emerge

119:01from the fundamental laws of physics.

119:03They're not, we don't posit them separately.

119:06They're meant to be deduced,

119:08and they can be deduced under limited circumstances,

119:10but not necessarily universally.

119:12And we're finding some of the subtleties

119:15and sort of accept edge cases

119:18where they don't apply in a straightforward way.

119:22And this is one.

119:25So time crystals do obey,

119:27do have this structure in time,

119:30but it's not a free lunch

119:31because although in a sense, things are moving,

119:36they're already doing what they want to do.

119:39They're in the,

119:40so if you want to extract energy from it,

119:44you're gonna be foiled

119:44because there's no spare energy there.

119:50So you can add energy to it and kind of disturb it,

119:53but you can't extract energy from this motion

119:58because it's gonna, it wants to do,

120:00that's the lowest energy configuration that there is,

120:03so you can't get further energy out of it.

120:06So in theory, I guess perpetual motion,

120:10you would be able to extract energy from it

120:13if such a thing was to be created,

120:15you can then milk it for energy.

120:17Well, what's usually meant

120:20in the literature of perpetual motion

120:23is a kind of macroscopic motion

120:27that you could extract energy from

120:29and somehow it would crank back up.

120:33That's not the case here.

120:35If you want to extract energy,

120:38this motion is not something you can extract energy from.

120:42If you intervene in the behavior,

120:45you can change it, but only by injecting energy,

120:48not by taking away energy.

120:51You mentioned that a theory of everything

120:54may be quite difficult to come by.

120:56A theory of everything broadly defined

120:58meaning like truly a theory of everything,

121:00but let's look at a more narrow theory of everything,

121:03which is the way it's used often in physics

121:07is a theory that unifies our current laws of physics,

121:16general relativity, quantum field theory.

121:19Do you have thoughts on this dream

121:22of a theory of everything in physics?

121:25How close are we?

121:26Is there any promising ideas out there in your view?

121:29Well, it would be nice to have.

121:32It would be aesthetically pleasing.

121:35Will it be useful?

121:36No, probably not.

121:38Well, I shouldn't, it's dangerous to say that,

121:43but probably not.

121:45I think we, certainly not in the foreseeable future.

121:52Maybe to understand black holes.

121:54Yeah, but that's, yes, maybe to understand black holes,

121:57but that's not useful.

122:00That's my book.

122:02And well, not only, I mean,

122:04to understand it's worse,

122:08it's not useful in the sense

122:09that we're not gonna be basing any technology anytime soon

122:12on black holes, but it's more severe than that,

122:16I would say it's that the kinds of questions

122:19about black holes that we can't answer

122:24within the framework of existing theory

122:28are ones that are not going to be susceptible

122:33to astronomical observation in the foreseeable future.

122:37They're questions about very, very small black holes

122:41when quantum effects come into play

§12Transcript · 2:02:46–2:14:08

122:46so that black holes are,

122:50not black holes, they're emitting this discovery

122:54of Hawking called Hawking radiation,

122:57which for astronomical black holes is a tiny, tiny effect

123:01that no one has ever observed, it's a prediction

123:03that's never been checked.

123:04So like supermassive black holes, that doesn't apply?

123:06No, no, the predicted rate of radiation

123:11from those black holes is so tiny

123:13that it's absolutely unobservable

123:15and is overwhelmed by all kinds of other effects.

123:21So it's not practical in the sense of technology,

123:24it's not even practical in the sense

123:26of application to astronomy, our existing theory

123:33of general relativity and quantum theory

123:37and our theory of the different fundamental forces

123:41is perfectly adequate to all problems of technology,

123:46of technology, for sure, and almost all problems

123:58of astrophysics and cosmology that appear

124:03except with the notable exception

124:06of the extremely early universe, if you want to ask,

124:09what happened before the Big Bang

124:11or what happened right at the Big Bang,

124:13which would be a great thing to understand, of course.

124:17Yes. We don't, but.

124:19But what about the engineering question?

124:21So if we look at space travel,

124:23so I think you've spoken with him, Eric Weinstein.

124:28Oh, yeah. Really, you know,

124:31he says things like we want to get off this planet.

124:36His intuition is almost motivated

124:39for the engineering project of space exploration

124:42in order for us to crack this problem

124:44of becoming a multi planetary species,

124:47we have to solve the physics problem.

124:49His intuition is like, if we figure out this,

124:51what he calls the source code, which is like,

124:55like a theory of everything might give us clues

125:00on how to start hacking the fabric of reality,

125:04like getting shortcuts, right?

125:06It might. I can't say that, you know,

125:08I can't say that it won't,

125:10but I can say that in the 1970s and early 1980s,

125:16we achieved huge steps in understanding matter.

125:23QCD, much better understanding of the weak interaction,

125:28much better understanding of quantum mechanics in general.

125:32And it's had minimal impact on technology.

125:36On rocket design, on propulsion.

125:38On rocket design, on anything, any technology whatsoever.

125:42And now we're talking about much more esoteric things.

125:46And since I don't know what they are,

125:48I can't say for sure that they won't affect technology,

125:51but I'm very, very skeptical

125:52that they would affect technology.

125:57Because, you know, to access them,

125:59you need very exotic circumstances

126:02to make new kinds of particles with high energy.

126:04You need accelerators that are very expensive

126:07and you don't produce many of them, and so forth.

126:09You know, it's just, it's a pipe dream, I think.

126:13Yeah, about space exploration.

126:15I'm not sure exactly what he has in mind,

126:18but to me, it's more a problem of,

126:26I don't know, something between biology and...

126:29And information processing.

126:34Processing, what you mean, how should I...

126:37I think human bodies are not well adapted to space.

126:43Even Mars, which is the closest thing

126:46to a kind of human environment

126:49that we're gonna find anywhere close by.

126:52Very, very difficult to maintain humans on Mars.

126:57And it's gonna be very expensive and very unstable.

127:02But I think, however, if we take a broader view

127:09of what it means to bring human civilization

127:17outside of the Earth, if we're satisfied

127:20with sending mines out there that we can converse with

127:25and actuators that we can manipulate

127:29and sensors that we can get feedback from,

127:33I think that's where it's at.

127:37And I think that's so much more realistic.

127:41And I think that's the long term future

127:45of space exploration.

127:48It's not hauling human bodies all over the place.

127:50That's just silly.

127:54It's possible that human bodies...

127:56So like you said, it's a biology problem.

127:59What's possible is that we extend human life span

128:03in some way, we have to look at a bigger picture.

128:07It could be just like you're saying,

128:09by sending robots with actuators

128:12and kind of extending our limbs.

128:16But it could also be extending some aspect of our minds,

128:19some information, all those kinds of things.

128:20And it could be cyborgs, it could be, it could be...

128:23No, we're talking, not getting the fun.

128:26It could be, you know, it could be human brains

128:32or cells that realize something

128:34like human brain architecture

128:36within artificial environments,

128:42you know, shells, if you like,

128:44that are more adapted to the conditions of space.

128:47And that, yeah, so that's entirely man machine hybrids,

128:52as well as sort of remote outposts

128:57that we can communicate with.

128:59I think those will happen.

129:02Yeah, to me, there's some sense in which,

129:05as opposed to understanding the physics

129:07of the fundamental fabric of the universe,

129:15I think getting to the physics of life,

129:17the physics of intelligence,

129:18the physics of consciousness will,

129:20the physics of information that brings,

129:27from which life emerges,

129:29that will allow us to do space exploration.

129:32Yeah, well, I think physics in the larger sense

129:34has a lot to contribute here.

129:36Not the physics of finding fundamental new laws

129:39in the sense of another quark or axions even.

129:44But physics in the sense of,

129:51physics has a lot of experience

129:53in analyzing complex situations

129:56and analyzing new states of matter

129:58and devising new kinds of instruments

130:00that do clever things.

130:01Physics in that sense has enormous amounts

130:05to contribute to this kind of endeavor.

130:09But I don't think that looking

130:13for a so called theory of everything

130:16has much to do with it at all.

130:19What advice would you give to a young person today

130:24with a bit of fire in their eyes,

130:26high school student, college student,

130:28thinking about what to do with their life,

130:30maybe advice about career or bigger advice

130:35about life in general?

130:37Well, first read fundamentals

130:38because there I've tried to give some coherent deep advice.

130:45That's fundamentals, 10 keys to reality by Frank Kulczyk.

130:50So that's a good place to start.

130:50Available everywhere.

130:52If you wanna learn what I can tell you.

130:56Is there an audio book?

130:57I read that ebook.

130:58Yes, there is an audio book.

130:59There's an audio book, that's awesome.

131:00I think it's, I can give three pieces of wise advice

131:05that I think are generally applicable.

131:08One is to cast a wide net,

131:13to really look around and see what looks promising,

131:19what catches your imagination and promising.

131:25Yeah, and those, you have to balance those two things.

131:28You could have things that catch your imagination,

131:30but don't look promising in the sense

131:32that the questions aren't ripe or,

131:34and things that you,

131:37and part of what makes things attractive is that,

131:42whether you thought you liked them or not,

131:43is if you can see that there's ferment

131:45and new ideas coming up that become,

131:47that's attractive in itself.

131:49So when I started out, I thought I was,

131:52and when I was an undergraduate,

131:53I intended to study philosophy

131:55or questions of how mind emerges from matter.

131:57But I thought that that wasn't really right.

132:00Timing isn't right yet.

132:01The right, the timing wasn't right

132:03for the kind of mathematical thinking

132:05and conceptualization that I really enjoy and am good at.

132:12But, so that's one thing, cast a wide net, look around.

132:18And that's a pretty easy thing to do today

132:25because of the internet.

132:27You can look at all kinds of things.

132:30You have to be careful though

132:30because there's a lot of crap also.

132:33But you can sort of tell the difference

132:36if you do a little digging.

132:42So don't settle on just,

132:44what your thesis advisor tells you to do

132:46or what your teacher tells you to do.

132:49Look for yourself and get a sense of what seems promising,

132:54not what seemed promising 10 years ago or, so that's one.

133:03Another thing is to, is kind of complimentary to that.

133:09Well, they're all complimentary.

133:12Complimentary to that is to read history

133:18and read the masters,

133:19the history of ideas and masters of ideas.

133:22I'd benefited enormously from, as early in my career,

133:28from reading in physics, Einstein in the original

133:34and Feynman's lectures as they were coming out and Darwin.

133:39You know, these, you can learn what it, and Galileo,

133:43you can learn what it is to wrestle with difficult ideas

133:46and how great minds did that.

133:48You can learn a lot about style,

133:51how to write your ideas up and express them in clear ways.

133:57And also just a couple of that with,

134:00I also enjoy reading biographies.

134:02And biographies, yes, similarly, right, yeah.

134:04So it gives you the context of the human being

134:08that created those ideas.

§13Transcript · 2:14:08–2:22:31

134:08Right, and brings it down to earth in the sense that,

134:11you know, it was really human beings who did this.

134:14It's not, and they made mistakes.

134:17And yeah, I also got inspiration from Bertrand Russell

134:22who was a big hero and H.G. Wells and yeah.

134:25So read the masters, make contact with great minds.

134:31And when you are sort of narrowing down on a subject,

134:33learn about the history of the subject

134:35because that really puts in context

134:38what you're trying to do and also gives a sense of community

134:43and grandeur to the whole enterprise.

134:46And then the third piece of advice

134:48is complimentary to both those,

134:51which is sort of to get the basics under control

134:58as soon as possible.

135:00So if you wanna do theoretical work in science,

135:04you know, you have to learn calculus,

135:08multivariable calculus, complex variables, group theory.

135:11Nowadays, you have to be highly computer literate

135:15if you want to do experimental work.

135:16You also have to be computer literate

135:17and you have to learn about electronics

135:19and optics and instruments.

135:22So get that under control as soon as possible

135:26because it's like learning a language to produce great works

135:32and express yourself fluently and with confidence.

135:37It should be your native language.

135:39These things should be like your native language.

135:41So you're not wondering what is the derivative?

135:44This is just part of your, it's in your bones,

135:50so to speak, and the sooner that you can do that,

135:53then the better.

135:55So all those things can be done in parallel and should be.

136:01You've accomplished some incredible things in your life,

136:04but the sad thing about this thing we have is it ends.

136:09Do you think about your mortality?

136:15Are you afraid of death?

136:19Well, afraid is the wrong word.

136:20I mean, I wish it weren't going to happen

136:23and I'd like to, but.

136:27Do you think about it?

136:28I, you know, occasionally I think about,

136:30well, I think about it very operationally

136:32in the sense that there's always a trade off

136:35between exploration and exploitation.

136:39This is a classic subject in computer science,

136:42actually in machine learning that when you're

136:46in an unusual circumstance, you want to explore

136:50to see what the landscape is and what, and gather data.

136:54But then at some point you want to use that,

136:57make, decide, make choices and say,

137:00this is what I'm going to do and exploit the knowledge

137:02you've accumulated.

137:03And the longer the period of exploitation you anticipate,

137:10the more exploration you should do in new directions.

137:14And so for me, I've had to sort of adjust the balance

137:18of exploration and exploitation and.

137:25That's it, you've explored quite a lot.

137:28Yeah, well, I haven't shut off the exploitation at all.

137:31I'm still hoping for. The exploration.

137:34The exploration, right.

137:35I'm still hoping for 10 or 15 years

137:38of top flight performance.

137:39But the, several years ago now when I was 50 years old,

137:47I was at the Institute for Advanced Study

137:49and my office was right under Freeman Dyson's office

137:52and we were kind of friendly.

137:53And, you know, he found out it was my 50th birthday

137:58and said, congratulations.

138:00And you should feel liberated because no one expects much

138:05of a 50 year old theoretical physicist.

138:07And he, and he obviously had felt liberated

138:10by reaching a certain age.

138:13And yeah, there is something to that.

138:15I feel, you know, I feel I don't have to catch,

138:19I don't have to keep in touch

138:21with the latest hypertechnical developments

138:25in particle physics or string theory or something.

138:27I, because I'm not gonna, I'm really not gonna

138:31be exploiting that.

138:33But I, but where I am exploring in these directions

138:37of machine learning and things like that.

138:40And, but then, but I'm also concentrating

138:43within physics on exploiting directions

138:46that I've already established

138:48and the laws that we already have

138:50and doing things like,

138:52I'm very actively involved in trying to design,

138:58helping people, experimentalists and engineers even

139:02to design antennas that are capable of detecting axions.

139:08So there, and that's, there we're deep

139:10in the exploitation stage.

139:13It's not a matter of finding the new laws,

139:14but of really, you know, using the laws we have

139:17to kind of finish the story off.

139:20So it's complicated, but I'm, you know,

139:25I'm very happy with my life right now

139:27and I'm enjoying it and I don't wanna cloud that

139:31by thinking too much that it's gonna come to an end.

139:39You know, it's a gift I didn't earn.

139:42Is there a good thing to say about

139:45why this gift that you've gotten

139:50and didn't deserve is so damn enjoyable?

139:53So like, what's the meaning of this thing, of life?

139:57To me, interacting with people I love, my family,

140:01and I have a very wide circle of friends now

140:04and I'm trying to produce some institutions

140:08that will survive me as well as my work

140:12and it's just, it's, how should I say?

140:18It's a positive feedback loop when you do something

140:24and people appreciate it and then you wanna do more

140:28and you get rewarded and it's just, how should I say?

140:32This is another gift that I didn't earn

140:34and don't understand, but I have a dopamine system

140:37and yeah, I'm happy to use it.

140:42It seems to get energized by the creative process,

140:47by the process of exploration.

140:48Very much so.

140:49And all of that started from the little fluctuations

140:56shortly after the Big Bang.

140:58Frank, well, whatever those initial conditions

141:01and fluctuations did that created you, I'm glad they did.

141:04This is, thank you for all the work you've done,

141:07for the many people you've inspired,

141:09for the many, of the billion, most of your ideas

141:12were pretty useless of the several billions,

141:16as it is for all humans, but you had quite a few

141:20truly special ideas and thank you for bringing those

141:23to the world and thank you for wasting your valuable time

141:25with me today, it's truly an honor.

141:27It's been a joy and I hope people enjoy it

141:31and I think the kind of mind expansion that I've enjoyed

141:37by interacting with physical reality at this deep level,

141:41I think can be conveyed to and enjoyed by many, many people

141:45and that's one of my missions in life, to share it.

141:48Beautiful.

141:49Thanks for listening to this conversation

141:50with Frank Wilczek and thank you to The Information,

141:54NatSuite, ExpressVPN, Blinkist and 8sleep.

141:58Check them out in the description to support this podcast

142:01and now let me leave you with some words

142:03from Albert Einstein, nothing happens until something moves.

142:08Thanks for listening and hope to see you next time.

— A LITTLE MORE TO THINK ABOUT. —