HomeVideos

Biggest Mysteries in Physics: Antimatter, Dark Energy & ToE - Don Lincoln | Lex Fridman Podcast #497

Now Playing

Biggest Mysteries in Physics: Antimatter, Dark Energy & ToE - Don Lincoln | Lex Fridman Podcast #497

Transcript

4235 segments

0:00

The following is a conversation with Don

0:02

Lincoln, a particle physicist at Firmeny

0:05

Lab, who has spent decades working at

0:07

the frontier of high energy physics.

0:10

This was a mind-blowing and inspiring

0:13

conversation. Don turned out to be one

0:16

of my favorite people to talk to about

0:17

physics. truly a unique mind with that

0:21

Richard Fineman ability of taking very

0:23

complicated ideas and explaining them

0:26

simply without losing any of the

0:29

essential brilliant insights at the core

0:31

of those ideas. This is the Lex Freedman

0:35

podcast. To support it, please check out

0:36

our sponsors in the description where

0:39

you can also find ways to contact me,

0:41

ask questions, give feedback, and so on.

0:44

And now dear friends, here's Don

0:47

Lincoln.

0:49

In describing the search for theory of

0:53

everything in physics, you describe the

0:55

history of physics can be told

0:57

effectively as a kind of history of

0:59

unifications.

1:01

There's this centuries long quest to

1:03

show that these distinct phenomena are

1:06

actually linked by some unified

1:11

underlying principles. uh even starting

1:13

with Newton that you can think of the

1:16

effort of physics as one as trying to

1:18

unify the laws of nature. So I was

1:21

wondering if we could talk through the

1:23

history of unification that lens of

1:27

physics. There are of course lots of

1:29

different ways to do physics, but the

1:31

the way that I would say that particle

1:33

physicists, cosmologists do is they are

1:36

trying to to really find basically the

1:41

underlying principles that govern the

1:43

laws of of nature. If we go back say to

1:46

the I don't know 1650s or so, uh you're

1:50

the most brilliant person around and

1:52

you've noticed two things. One you've

1:54

noticed is that when you trip, you fall.

1:57

That is the nature of gravity that that

1:59

we all experience daytoday. But then

2:01

there's sort of astronomy where you look

2:03

out at the heavens and you see the stars

2:06

march across the sky. You see the

2:08

planets move through the stars and there

2:12

that seems to have absolutely nothing to

2:14

do with what happens when you drop your

2:17

sandwich and and the dog grabs it from

2:19

you. So

2:21

>> yeah,

2:21

>> the brilliant thing was when Newton

2:24

looked at that and he thought about

2:26

maybe the moon is falling but it's

2:29

missing the earth. So what we had is

2:30

that in maybe 1650 you had what we might

2:34

call the laws of celestial gravity, the

2:36

gravity that governs the heavens and

2:39

terrestrial gravity, the gravity that is

2:41

here on Earth. Now we don't think of

2:44

that that way anymore. We think of it as

2:46

just gravity. But at that time that

2:48

wasn't at all obvious. And in fact, if

2:51

you look in the books, Newton's theory

2:52

is Newton's law of universal gravity.

2:55

The universal is there. And the reason

2:56

is is because he realized these two

2:59

things that seem to have nothing to do

3:01

with one another were indeed one and the

3:03

same. I mean, this is absolutely

3:05

brilliant. I mean, Newton is arguably

3:08

one of the most brilliant humans I of

3:10

which I'm ever aware. But at any rate,

3:13

it is the first sort of easily to

3:15

describe unification of physics that you

3:19

can state in a way that sort of makes

3:21

sense to to modern humans. I mean, you

3:23

can go back farther than that where

3:25

people are talking about chemistry, the

3:28

nature of atoms. You go back to Democrus

3:30

who was wrong about very many things,

3:32

but the idea that there was a smallest

3:33

particulate form of matter is right. So,

3:36

it's kind of funny. You talk, you read

3:38

the chemistry books and they say that

3:39

the idea of atoms goes back to Democrus

3:41

and you know he his idea was that like

3:44

um there was a smallest atom of oil

3:46

which was smooth and it was smooth of

3:48

course because well oil is smooth. There

3:50

was a smallest atom of vinegar because

3:52

vinegar is tart and it pricks your

3:54

tongue so therefore atoms were little

3:56

sharp pointy things. Um and so he was

3:59

wrong about a lot but he was right about

4:02

the idea that there was a small particle

4:06

and and we now know a very we have a

4:08

very different concept than he did. So

4:11

you can go back farther than that but

4:13

getting to unification there are more

4:15

examples. For instance if you go back to

4:18

say 1830 or so scientists were trying to

4:23

understand electricity for instance and

4:26

there was a lot going on. people really

4:28

understood things. But at the time you

4:30

would have two phenomena that are

4:33

familiar to us now. One is a magnet

4:35

which you know at the time mostly

4:38

magnets were were simply little pieces

4:40

of iron that had been magnetized and

4:42

they could stick to steel. And then you

4:44

had electricity which was at the time

4:46

they were generating little sparks that

4:48

they could play and and have fun with or

4:51

more broadly a uh a lightning bolt

4:53

blazing across the sky. And so when you

4:56

think about this, that lightning bolt

4:58

and that little magnet seemed to be

5:00

really unrelated.

5:02

>> Mhm.

5:02

>> Um but over the 1800s, a number of

5:06

scientists were exploring little aspects

5:09

of it. What happens when you run

5:11

electricity through a wire? It seems to

5:14

make a magnetic field. You know, they

5:16

was a whole bunch of experiments and

5:17

there were a lot of names. But in about

5:19

the 1860s or so, James Clark Maxwell

5:23

took all of those ideas that had been

5:25

percolating around for the previous 50

5:27

years and wrote his laws of

5:30

electromagnetism.

5:31

And they're really fascinating. If you

5:33

look at the laws of electromagnetism,

5:35

they are they're differential equations

5:37

or integral equations. But basically

5:40

what they say is on one side you have a

5:42

bunch of terms that have electricity in

5:45

them and then you have equals on the

5:48

other side a magnetism thing. So

5:51

forgetting all of the mathematical

5:52

symbols you have electricity side equals

5:55

a magnetism side. Electricity equals

5:57

magnetism. And that is a staggering

6:01

concept. The fact that these two things

6:03

a lightning bolt and the magnet that

6:05

holds your kids art to the refrigerator

6:07

are one and the same. And this was

6:09

another case where electricity and

6:11

magnetism became unified into

6:14

electromagnetism. So now we have two

6:15

examples. One, gravity being unified,

6:18

terrestrial and celestial gravity, and

6:20

then electricity and magnetism. So I

6:22

I'll tell you about some more in a

6:24

moment. But one thing that's kind of

6:26

important because the goal is of course

6:28

to to unify everything that if if I

6:31

could do what I want to do, I would have

6:33

some unified theory that would explain

6:35

all the behavior of all energy, matter,

6:37

space and time, which is a grand goal.

6:39

>> And and we should say that maybe one of

6:42

the goals of science more broadly

6:44

outside of physics even is to construct

6:48

uh models

6:49

that can generalize

6:52

the world. So if you look at Darwinian

6:54

evolution that was a very beautiful

6:57

theory that captures another layer of

7:01

reality of like how this particular

7:05

thing that we see here on earth happens

7:07

right

7:07

>> so when we talk about theory of

7:09

everything in physics that's capturing a

7:12

different layer of abstraction about the

7:14

functioning of the universe

7:16

>> right the whole Darwinian evolution the

7:18

fact that our genetics has significant

7:21

overlap with genetics of a banana is is

7:24

pretty staggering is astonishing that

7:26

that works. So that is amazing. Um but

7:30

for at least the class of of scientists

7:33

that I am what we think of is well sure

7:37

biology is interesting and all but when

7:39

you get right down to it it's it's it's

7:42

caused whatever happens in biology is

7:44

caused by the movement of molecules. And

7:47

then you say, "Well, that's great and

7:49

all, but molecules, they do what they do

7:51

because they're made of atoms."

7:53

>> And then the next step is, well, you

7:55

know, atoms, that's great, but atoms

7:56

work the way they do because of the

7:58

nucleus and the electrons. And then the

8:00

nucleus is protons and neutrons. And so

8:03

there are those of us, myself included,

8:05

who want to dig down at to the very very

8:08

bottom and find out what is the smallest

8:11

building block of nature from which all

8:13

of these other far more complex and

8:15

interesting and abstract things are, but

8:18

what is at the very very bottom? And

8:20

also that's great, but if you know um

8:24

what the smallest building blocks are,

8:25

that doesn't tell you the story. That's

8:27

like having a whole bunch of Legos but

8:30

not knowing how to put them together.

8:31

You also need to know how they interact,

8:33

how they work. And so that's what we

8:35

study forces. So there are the various

8:38

subatomic forces of which we're

8:39

familiar. And um for instance,

8:41

electricity and magnetism are components

8:44

of electromagnetism which then governs

8:47

the behavior of things like this is

8:49

amazing. Electric electromagnetism

8:52

explains of course electricity magnetism

8:54

but it explains how light works. It

8:56

explains how much of chemistry works. So

8:59

electromagnetism 1860 or 70 uh the

9:03

wonderful thing about that is if you

9:05

take Maxwell's equations and you apply a

9:07

little bit of calculus it's very easy to

9:10

see that the laws of electricity and the

9:13

laws of magnetism combined together

9:16

make what's called a wave equation which

9:18

that's shows that these electric and

9:21

magnetic fields oscillate. they they

9:24

vary. And if you have a something that's

9:27

varied, that's a wave. And the wave then

9:30

moves. And if you do the math, you find

9:32

out that the speed at which these waves

9:34

move is the speed of light. And so

9:37

people said, "Wow, the speed of light

9:39

comes out of those equations." And that

9:42

had to be, I think, very persuasive. And

9:45

of course, electromagnetism also plays a

9:48

really significant role in chemistry

9:51

because after all, atoms are held

9:52

together by electromagnetic forces.

9:54

There's more to how atoms work. There is

9:57

all the quantum mechanic stuff. But if

10:00

you did not have electromagnetism or if

10:02

electromagnetism was very different,

10:03

then atoms would be very different. So

10:05

it plays a very big role in in holding

10:08

us together. So it it's a a staggering

10:12

advance in science to have a good

10:15

behavior on that. And of course

10:17

being able to to tame electromagnetism

10:22

is why people can hear you when you do

10:25

your podcast because through the

10:27

miracles of the internet just or just

10:29

electricity running the computers. I

10:31

mean, this is a case, if I can get on a

10:34

small soap box, where people back then

10:37

said, "Well, why are you messing around

10:39

with magnets and sparks and who cares?"

10:42

Well, that very

10:46

fundamental digging into the laws of

10:48

nature has spin-offs. And it has

10:50

spin-offs. One of the big spin-offs is

10:52

our entire technological society.

10:55

without being able to govern

10:56

electricity, we'd still be farmers and

10:59

shoemakers in cities, but we certainly

11:01

would not have everything that we do.

11:04

So, off my soap box, but it's really a

11:06

lovely thing to show how this this

11:10

digging into deep fundamental, not

11:13

understood, mysterious things can 100 or

11:17

200 years later transform the world. And

11:21

the type of science I do now, people

11:22

often ask, well, what good is knowing

11:24

about how the inside of atoms work, how

11:26

the inside of quarks work. And I don't

11:29

know the answer to that. Um, but just

11:31

being a little more pragmatic, if I go

11:34

back, say, hundred years, where people

11:36

were trying to understand how the

11:39

protons and neutrons inside atoms held

11:42

together, how they split, how they they

11:45

how you could combine them and so forth.

11:47

This has led to nuclear power. Now,

11:50

whatever you think about nuclear power

11:52

and some people like it and some people

11:53

don't, but it is powerful. It will

11:56

generate uh energy for humanity and and

12:00

it may be that is the path that that we

12:02

take as we move away from digging fossil

12:06

fuels out of the ground. Humanity is

12:08

going to need power no matter what.

12:10

Nobody is going to go back to the way

12:12

things were in the 1700s. And one

12:16

enormous source of energy that is there

12:18

for us to take if we so choose is the

12:21

modification of the nucleus of atoms

12:24

seem to have absolutely nothing to do

12:26

with anything. And yet it provides

12:28

humanity with an opportunity which of

12:31

course requires that we think carefully

12:32

of how we do that and and if we want to

12:35

but it gives us something that we didn't

12:37

have before. Yeah, it's very clear that

12:39

nuclear fusion and nuclear fision will

12:42

unlock huge amount of energy that's

12:45

required for a civilization to flourish.

12:48

But that's almost like near-term.

12:50

>> Mhm.

12:52

>> Longer term, you can think about things

12:54

like we'll talk about dark energy crisis

12:59

and antimatter. Maybe if you figure out

13:04

some of the mysteries around antimatter,

13:06

that too would lead to energy sources,

13:10

how to produce energy, that too might

13:12

lead to counterintuitive propulsion

13:14

systems

13:16

>> for us humans to travel through through

13:18

the universe. Now, right now it seems

13:19

farfetched, too expensive, too

13:21

complicated, too difficult. But

13:24

breakthroughs in the fundamentals

13:26

theoretical physics might lead us to

13:28

unlock some incredible energy sources,

13:31

incredible technologies that uh will uh

13:34

allow humans to explore the universe.

13:36

And of course, we should also mention

13:39

that as always with technology, it's a

13:41

double-edged sword. It will most likely

13:43

lead to the development of more

13:45

dangerous weapons or other sources of

13:47

harm. And then we uh as a civilization

13:51

kind of have to walk that uh line and

13:55

hope we figure out how to do more good

13:57

than bad with the technologies we built.

13:59

>> Right? But but we have to really

14:01

remember while people worry about

14:04

nuclear weapons which are admittedly

14:06

very dangerous and even nuclear power

14:09

which has waste that has to be dealt

14:11

with.

14:12

What science is doing is

14:16

working out finding power that nature

14:19

has presented to us. This is not new.

14:21

Fire is like that too. Fire can burn

14:25

down your house or it can cook your

14:26

steak. Power is like that. And that's

14:29

just something that we have to

14:31

understand as humanity. And that's why

14:33

this needs to be a you know when we talk

14:35

about science it has to be a broad

14:36

conversation by all of society because

14:40

what scientists can do is figure out how

14:43

the world works. Society has to figure

14:45

out how we wish to apply that or not

14:48

apply that.

14:49

>> Also solving the mysteries and the

14:52

puzzles of the universe in itself is

14:55

effing awesome.

14:56

>> It is. It is. So, I mean that that's the

14:59

thing that makes us human in part is

15:02

looking at a thing and saying, "How does

15:04

this work?" And then together, uh, a

15:07

bunch of apes get together like poke the

15:09

thing, kind of shake the thing,

15:11

>> and then over time you have rockets

15:14

going out into space, you build roads

15:16

and bridges, you build the internet.

15:18

Anyway, so we talked about Newton, we

15:21

talked about Maxwell. That takes us in

15:23

the 20th century in terms of

15:25

unification. There's a guy named

15:27

Einstein on whom you wrote a book who

15:29

did quite a lot of progress on the

15:32

effort of unification.

15:33

>> Sure. So Einstein, he's a pretty amazing

15:36

guy. In 1905, he had his miracle year

15:39

where he wrote multiple papers. The one

15:42

that most people know about is special

15:44

relativity where he showed something

15:48

that makes no sense to anybody who's not

15:52

really dug into it very hard. And that

15:55

is that two people experience time

15:58

differently. Time, you know, is a

16:01

fascinating thing. We don't really

16:02

understand what time is, which is weird.

16:04

You think that that'd be something we'd

16:06

understand very well, but we really

16:07

don't. We know a lot about it, but

16:10

really understanding it, not so much.

16:13

But, um, Newton thought that time was

16:15

just universal for everyone. So my time,

16:18

your time, some person's time on Mars or

16:21

on Alpha Centator, everybody experienced

16:24

time the same. What Einstein showed was

16:27

that that wasn't the case. That

16:29

different people moving at different

16:31

speeds with respect to one another

16:32

experience time differently, which is

16:35

absolutely a mindblowing concept. Now,

16:39

most people think that Einstein then

16:41

said, well, he invented spaceime that

16:43

that space and time are the same thing.

16:46

and he was behind that. But that actual

16:48

insight came from one of his teachers, a

16:51

guy by the name of Minowski, who looked

16:54

at Einstein's equations. Mowski was a

16:56

little bit more mathematically inclined

16:57

than Einstein. And he saw that if you

17:00

look at the equations, you have

17:03

basically one person's space and time

17:06

equals some numbers times this person's

17:09

space and time. And so that's kind of a

17:13

a staggering thing. So, so that is where

17:16

Einstein and Manowski really did this

17:20

unbelievable concept that that space and

17:23

time are actually pretty much the same

17:26

thing that runs a foul of our

17:28

understanding of how the world works

17:30

because time just moves. It's

17:33

continuous. We we know what it is at a

17:35

visceral level

17:38

and an experiential level. We might not

17:40

understand it at a formal level, but we

17:42

know what time is. It's what keeps makes

17:44

today today and not yesterday or

17:46

tomorrow. Space is a little different.

17:48

You can walk somewhere, you can walk

17:50

back, you can move around. You have more

17:51

freedom to move in space than you have

17:53

to move in time. You can always move

17:55

forward in time. It's just moving

17:56

backwards. It turns out to be a little

17:58

more difficult. But yeah, Einstein's

18:01

understanding that that is the case, it

18:04

caused everybody to think about the

18:07

world very very differently. And that

18:09

was in 1908 when Minkowski really laid

18:12

it out in the strict spaceime.

18:14

>> Uh and that also led to the work on

18:17

special relativity led to the speed

18:19

limit, the speed of light.

18:21

>> Well, it was a premise. He had two

18:23

premises. One was that the laws of

18:26

nature are the same for everybody. So if

18:28

you're moving at some speed or if I'm

18:30

moving at some speed, I can say I'm not

18:32

moving and saying you're moving at some

18:34

speed. That's not controversial. That is

18:38

what we call Galilean relativity. It's

18:40

from hundreds of years ago. But what

18:42

Einstein said that was controversial was

18:45

that everybody measures that the speed

18:47

of light is the same irrespective of how

18:52

we're moving with respect to each other.

18:54

You'll measure the speed of light to be

18:55

a number. I'll measure the speed of

18:57

light to a number. And that's very very

18:59

different from what Newton would have

19:00

said or Galile or any of the old guys.

19:03

And it was taking those two things

19:05

together that caused all of the

19:08

weirdnesses of special relativity. Now

19:11

you could then very easily say, well

19:14

that second premise that everybody

19:15

measures the speed of light to the same

19:18

is just dumb and that you know you could

19:22

test that. So that's where testing

19:26

relativity comes in and Einstein's

19:27

equations which include those two

19:30

assumptions it predicts the behavior of

19:33

everything perfectly well. Now we've

19:35

actually measured

19:37

uh done experiments where we can say

19:39

that the speed of light is the same for

19:41

everybody. That's not how that's been in

19:44

the beginning. It was really that

19:46

assumption leads to predictions. The

19:48

predictions are true. So the assumption

19:50

is true. Now there is a for for those

19:53

people for your viewers who want to say

19:55

well how do you measure that the speed

19:56

of light is the same for everyone the

19:59

particle physicists do this and the way

20:01

you do this is the following there are

20:04

some subatomic particles that when they

20:07

decay they emit light that's their decay

20:10

product and so you collide two things

20:13

together so you know when the particle

20:15

was created then you have surround your

20:20

collision point by a detector and you

20:24

measure how long it takes for light to

20:27

get to your detector and by God it's the

20:29

speed of light which it should be.

20:32

However, sometimes in these collisions

20:34

some of these subatomic particles you

20:37

make are coming out at very high speed.

20:39

They might be coming out at 95 or 97 or

20:42

very large fraction of the speed of

20:44

light and then they decay into photons.

20:48

And so you measure how long it takes for

20:51

the photon to get to your detector and

20:55

it says it's light travels at the speed

20:57

of light. Now if it were that

21:00

if Einstein's conjecture was incorrect,

21:02

you'd have a particle coming out at near

21:04

the speed of light. It would be decaying

21:05

into a particle traveling at the speed

21:07

of light. Then that particle should have

21:09

traveled at say two times the speed of

21:11

light or something like that. So it

21:12

should have taken half as much time to

21:14

get to the detector. But it doesn't. So

21:17

this is a hard serious measurement that

21:19

shows that something you know we we can

21:22

measure the speed at which light comes

21:25

out of this stationary created particle

21:28

and it's the speed of light then we can

21:30

measure what the speed is of it coming

21:32

out of something that's moving and it's

21:34

still the speed of light. So that is an

21:36

actual measurement but that is not

21:38

something that was possible in

21:40

Einstein's day but it is now. Just to

21:42

take a small tangent. Uh how weird is it

21:46

in the full ranking of weirdness that is

21:48

physics? How weird is it that there's

21:50

that speed limit of this speed of light?

21:53

>> Well, I have to tell you, when I first

21:54

encountered this, it's pretty freaking

21:56

weird. It's like pegs the weird meter.

21:59

But as you become more familiar with it,

22:03

as you become more more comfortable with

22:06

the idea, the thing to remember is the

22:10

speed of light. It's the speed of light

22:14

through spaceime. Once you embrace that,

22:17

that makes a whole ton of sense. It all

22:19

of a sudden makes everything fall much

22:21

more into place. I think that there is

22:25

an ultimate speed isn't that shocking.

22:28

It just simply says that it's a property

22:30

of space in the same way that there is

22:34

you know space can can transmit a

22:36

certain strength electric field. like

22:38

trans it can support a certain things

22:41

whatever space is and we don't know what

22:43

space is but whatever it is it has the

22:46

capability of of transmitting these

22:49

things at that one speed through space

22:51

or time and everything else comes from

22:54

our insisting that we keep space and

22:57

time different that's that's how I view

22:59

it and at least for me that once I

23:03

accepted that it all became very

23:05

comfortable

23:06

>> so The nature of my question actually

23:09

here that will apply over and over

23:11

>> is trying to empathize, trying to put

23:13

ourselves in the shoes of the people

23:14

before space and time are unified into

23:17

spaceime

23:19

>> and and really experience and think

23:21

through how difficult of a leap is that

23:24

>> huge.

23:25

>> The reason I I sort of say that is we

23:29

are now in the modern day in the 21st

23:31

century and of course we're going to

23:33

have to make leaps like that in our

23:35

future. Mh.

23:36

>> So what are the unifications we're not

23:39

seeing in front of our eyes? So for

23:41

example, there's so many examples

23:42

through through your work, through your

23:44

lectures of um uh Paul Durak taking

23:49

antimatter seriously.

23:50

>> Mhm.

23:51

>> Looking at what the math shows and

23:53

saying, I really think this thing

23:56

exists,

23:57

>> right?

23:57

>> I mean, it just sounds insane.

23:59

>> It does.

24:00

>> And so I think this is a good warm-up.

24:02

The space-time unification is a good

24:05

warm-up as we march through the 20th

24:07

century because it gets uh in my view at

24:10

least weirder and weirder even with

24:12

Einstein himself.

24:13

>> Well, let me give you an even more basic

24:16

example. Sodium and chloride.

24:19

Sodium is an explosive metal. You put it

24:21

in water and and it's kind of neat. You

24:24

put it in water and it just it doesn't

24:26

quite explode, but it gets hot and it

24:27

pops around. Chlorine, it's a gas. It's

24:30

going to kill you. So these two things

24:33

are deadly. They're awful. And yet when

24:36

you mix them, you put it on your food at

24:38

night. Salt, right? And so this is a

24:42

case where where this whole a

24:45

unification and b this deeper

24:47

understanding in this case of chemistry

24:49

of how two things that that are

24:53

dangerous can be brought together and

24:55

turned into something not only innocuous

24:56

but necessary for human life. And so

24:59

this is not unusual that what what

25:02

you're describing. I mean when you think

25:04

about it, forget about everything else.

25:05

Just the fact that you know we tell

25:08

little kids little kids that the world

25:10

is made of atoms. Now that's crazy. Most

25:13

people have never seen atoms and yet

25:15

nobody really doubts it anymore. And I

25:17

think it's just a a case of of

25:19

familiarity and then the culture slowly

25:22

accepts it and it's then it's real even

25:26

without the evidence. In fact, one of

25:27

the courses you described there, um, how

25:29

we know what we know. I think that's a

25:31

valid question. How do we know there are

25:33

atoms? And, and of course, there are

25:34

ways we do. And by the way, on that

25:36

front, I would love to go through how we

25:40

know the building blocks in the universe

25:42

as we march towards quirks. That in the

25:44

course that you mentioned is one of the

25:46

most fascinating things of this

25:48

philosophy of atoms being around for a

25:51

very long time. Then you concretize and

25:54

you actually can prove or have

25:57

strong observations that indicate that

26:00

there is atoms and then there is a

26:02

nucleus, there is electrons, there is

26:03

photons, there is quarks and I mean it

26:06

gets weirder and weirder and now we're

26:08

facing the mystery. Is there building

26:10

blocks even smaller than that? But

26:12

anyway, Einstein turns out didn't just

26:15

do special relativity. By the way, I I

26:18

really think he deserves three Nobel

26:20

prizes. He got it for photoelectric

26:22

effect. The fact that he didn't get it

26:24

for general relativity is a crime

26:26

against humanity. I don't understand.

26:28

Obviously should have gotten it for

26:29

general relativity and and special

26:32

relativity. I mean I think special

26:34

relativity is separate for general

26:36

relativity in ter as far as Nobel prizes

26:38

go. Uh so general relativity is another

26:41

unification.

26:42

>> Yes, that's right. What Einstein

26:44

realized was that if you were in a

26:46

rocket ship and the rocket ship was a

26:50

very quiet rocket ship and it was

26:52

accelerating, it would feel like you're

26:53

experiencing gravity. And so, as as you

26:56

say, it's one of his happiest moments

26:58

when he realized that acceleration and

26:59

gravity feel very much the same. What

27:03

I'm impressed by is that idea, which is

27:06

already a pretty neat idea,

27:09

somehow led him to take his space-time

27:13

idea, take this acceleration gravity

27:16

idea and realize that he could describe

27:20

gravity as the bending of spacetime.

27:24

Spacetime being constant like east,

27:26

west, north, south, that's already hard

27:29

enough. But now he's saying, well, you

27:31

know, take your your map and crinkle it

27:33

and bend it and so forth and that's

27:35

gravity. That is a staggering

27:39

mind-blowing idea.

27:40

>> I guess I wonder if you can comment on

27:43

what do you think is the idea generation

27:46

process that leads to that. So it

27:48

probably in Einstein case has to start

27:50

with what if gravity is itself

27:54

space-time geometry. You you have to

27:57

have a thought like that, right?

27:59

>> Yes, I think so. There's a lot about

28:02

science. There's of course knowing what

28:04

went before. There is knowing the

28:07

mathematics that allows you to figure

28:08

out the implications of your theory.

28:11

There is the discipline to argue with

28:14

yourself and other people because most

28:16

ideas are wrong. But then there's what

28:18

you just described that intuitive spark

28:21

and that is something that is very very

28:23

difficult to to create. There's a reason

28:27

that we venerate these people is because

28:30

it is an unusual

28:32

feature and most people only have that

28:35

aha moment once in their lifetime if

28:38

they have it at all. Mhm.

28:40

>> And then there's a tricky business

28:43

because I'm sure you do and I get a lot

28:45

of letters from from creative thinkers

28:48

who don't have all of the the history

28:51

and the mathematical discipline and the

28:53

the self, you know, self-critique that's

28:56

necessary. Um, and so they come up with

28:58

these ideas and often it's easy to see

29:02

where they just don't play out. Um so in

29:06

order to be that person who changes the

29:08

way we see the world, ideas themselves

29:11

are not enough. These these creative

29:13

ideas that's not enough. You need it

29:15

with the discipline and the critique.

29:18

And it's that amalgam of those things

29:22

that you know make you a genius that

29:24

that history remembers.

29:26

>> But it's hard to know in in a field of

29:28

people you might uh be tempted to call

29:31

crazy, there could be geniuses there.

29:34

And it's hard to know which is which. We

29:36

should mention that Einstein himself

29:40

couldn't see the genius in quantum

29:42

mechanics initially. Couldn't see the

29:45

the correctness, I should say. So he

29:48

could see the the insanity of

29:52

gravity bending spacetime, but quantum

29:55

mechanics was too weird for Einstein.

29:57

>> In all fairness, it's weird for me, too.

29:59

But um

30:01

>> but the thing is even while that is true

30:04

and Einstein maybe spent the last few

30:06

years of his life trying to to blend um

30:10

electricity and magnetism, gravity in a

30:13

a single thing and he was unsuccessful

30:15

but he still was a very very valuable

30:18

critic of quantum mechanics. It's not

30:21

that he didn't understand it because he

30:24

did understand it. He thought about the

30:25

implications and all this quantum

30:27

entanglement business. Well, not all of

30:29

it, but he was responsible for saying,

30:31

well, if you're right, then this. And of

30:34

course, then people went out and found

30:36

out that that Einstein's implication of

30:39

quantum mechanics was real. And so they

30:41

could say, see, quantum mechanics is

30:43

real. So, you know, he was thinking

30:46

deeply about it. And he was doing

30:49

exactly that thing I said. There's that

30:51

spark idea, but there's that critique

30:53

idea. And if you're able to critique an

30:56

idea, you might kill it. And that is

31:00

it's always depressing when I have this

31:02

brilliant idea and it gets killed, but

31:04

it's better to be killed than to keep it

31:06

around and waste time on it. Um, and so

31:10

he was in that case not generating the

31:15

the aha, but he was saying is, "All

31:17

right, let's take your aha. Let's see

31:19

it's right. What does it mean? It means

31:21

this." that allows people to go test it.

31:23

And so he was contributing very

31:28

crucially

31:30

to that other part of scientific

31:32

advancement, which is not just the aha

31:34

moment, but the beat it to death, test

31:37

it, critique it, and make sure it's

31:39

real. And it's only after all of that

31:42

has been done that you really are sure

31:44

you're right. And that's why science is

31:46

such a a powerful tool. It is that that

31:51

combative just downright kind of jerky

31:54

critique that most people don't like.

31:55

They don't like people saying your

31:57

ideas, you know, might be wrong.

32:00

But that is it is crucial. It is crucial

32:03

part of the scientific process.

32:04

>> Plus, there's that quote on the other

32:06

side of it that I've heard you mention

32:09

which is uh you know, I believe your

32:12

idea is crazy, but is it crazy enough?

32:15

Was that

32:17

>> Yes. Yes. We all agree that your idea is

32:19

crazy, but is it crazy enough?

32:20

>> And there is some degree of taking those

32:22

leaps uh of crazy, but it has to be

32:25

backed with rigor,

32:27

>> right?

32:28

>> And the unifications continue that as we

32:31

uh take steps towards the standard

32:32

model, which is such an incredible part

32:35

of of physics in the 20th century. So,

32:37

can you describe that unification?

32:39

>> So, you know, we're sort of jumping

32:40

forward here now to the 1930s or

32:43

thereabout. And at by that time people

32:46

had realized that there are four

32:50

distinct forces that do not seem to be

32:54

connected. One is gravity, two is

32:58

electromagnetism, and those are things

32:59

people are relatively familiar with. But

33:01

there are two other forces that only

33:04

have any real importance inside the

33:06

nucleus of atoms, which is why most

33:08

people have no experience with them. One

33:11

is the strong nuclear force which holds

33:13

the nucleus of the atoms together and

33:16

the other one is what we call the weak

33:17

nuclear force which is responsible for

33:20

some types of of radioactivity. And

33:23

since most people don't play around with

33:25

nuclei and most people don't play around

33:26

with radioactivity, they don't know what

33:28

that is. But um by the 30s scientists

33:33

had done enough experiments, done enough

33:36

theorizing to to say that there were

33:38

these four forces and that was already a

33:42

triumph. I mean we in our goal for a

33:44

theory of everything we'd like to think

33:46

that there is one force which is what

33:48

we're talking about the unification.

33:49

Maybe these four forces are are just

33:52

different ways of looking at a single

33:53

underlying force. But in the 30s that's

33:56

where we were. there were the four

33:58

forces.

34:00

So we move ahead and in the late 50s and

34:06

early 60s some people were thinking that

34:10

maybe the weak nuclear force and

34:14

electromagnetism

34:15

actually were the same. So they were

34:19

working on trying to bring together

34:21

these two forces to show that they're

34:23

connected. And it came true. They were

34:26

able to show that electricity and

34:29

magnetism were actually two different

34:32

facets of a single force that we now

34:35

call the electroeak force. Mhm.

34:37

>> Now, the story that you're told in in

34:41

articles about this about what you

34:44

people have called the Higs Bzon or the

34:45

God particle, the story is very very

34:49

simplified

34:50

because in 1964

34:53

the um there were three groups with six

34:57

individuals who came up with important

35:00

papers talking about what's called the

35:02

Higsfield. I'll get to back get to what

35:04

that is in a minute. But the Higsfield

35:06

is important. But it wasn't until 1967,

35:08

so 3 years later, that Steven Weinberg

35:12

and and some others actually unified

35:16

electromagnetism and the weak force.

35:18

Sheldon Glashau, Abdul Salam and Steven

35:22

Weyberg successfully unified

35:23

electromagnetism and the weak nuclear

35:25

force that uh showing that high energies

35:30

uh these two forces were merged into a

35:32

single electroeak force,

35:34

>> right? And that was in ' 67. All right.

35:37

Um everybody talks about this thing

35:39

happening in ' 64, but it it really

35:41

wasn't. It happened over quite a few

35:43

years actually. But all right. So now

35:46

let's what you said is true. So um uh

35:50

Weinberg, Glacial and Salam showed that

35:53

electromagnetism in the weak force at

35:55

high energies were the same. There was a

35:58

problem however and the problem is that

36:02

electromagnetism has an infinite range.

36:05

Um and we know that because we can see

36:07

stars that are millions of light years

36:09

away. I mean that shows you that the

36:11

range of that force is essentially

36:14

infinite.

36:15

>> The weak force however um basically

36:18

becomes non-existent on distances much

36:22

smaller than the size of a proton.

36:24

>> Mhm.

36:25

>> So that you know to say oh they're the

36:27

same and yet one can reach across the

36:30

universe and one can't reach out of an

36:31

atom. Well that's just dumb. I mean the

36:34

obvious

36:36

thought here is well we just proved that

36:39

that whole idea is stupid so throw it

36:41

away ridiculous. And that is where these

36:45

ideas from 1964 came in and saved the

36:48

day. So how can it be true

36:53

that the electroeak force is real and

36:57

electromagnetism

36:58

and the weak force act so differently?

37:02

The way that could happen is if these

37:06

forces were transmitted by a particle

37:11

moving from one subatomic particle to

37:15

the other. In the case of

37:17

electromagnetism, it's the photon. In

37:20

the case of the weak force, we call them

37:23

now the W and Z particles. So the idea

37:26

is that that Higgs and his colleagues

37:29

came up with is saying all right

37:32

electroeak force is real.

37:35

The way we make it so that there is now

37:38

an electromagnetic force and a weak

37:41

force is the force carrying particle of

37:45

electromagnetism has no mass. The force

37:49

carrying particle of the weak force has

37:52

a mass. And so what was done is a field

37:59

was postulated that there was this

38:02

additional field that was kind of

38:05

distinct from this electroeak field and

38:08

we call it the Higs field. And the Higs

38:10

field permeates all of space.

38:14

And and here's the kicker, some

38:16

particles interact with a field and some

38:19

particles don't interact with a field.

38:21

The ones that interact with the field

38:23

get mass and the ones that don't

38:25

interact with the field don't have mass.

38:28

And so that's the idea is that the Higs

38:31

field gives the weak force particles

38:34

mass. However, the photon laughs at the

38:37

Higs field, doesn't see it, and it has

38:40

no mass. And I should say here, going to

38:42

perplexity, the big picture view, the

38:45

Higs field is a quantum field that fills

38:47

all of space and gives many elementary

38:49

particles. Just as you're saying their

38:51

mass through their interaction with it,

38:54

the Higs Bzon is the particle associated

38:57

with ripples or excitations of this

39:00

field. In modern particle physics, every

39:02

type of particle corresponds to a field

39:04

that exists everywhere. The Higs field

39:07

is one such scalar field, meaning at

39:10

each point in space, it has a single

39:12

numerical value rather than a direction.

39:16

The Higs field differs from most other

39:18

fields because even in empty space,

39:21

empty in quotes by the way, empty space,

39:24

it's uh average value is not zero. This

39:26

nonzero vacuum value is what enable it

39:29

to endow particles with mass.

39:31

>> Right? So let's talk about something a

39:33

little more familiar just to to try and

39:36

hang some some intuition on those words.

39:39

All right? So right in front of us there

39:41

is a gravitational field. Now, you can't

39:43

see it, but right there. Right there.

39:45

Check it out.

39:46

>> Yep.

39:46

>> If I were to take something, a pen or

39:49

whatever, and put it there, it feels a

39:51

force and a falls.

39:53

>> Mhm.

39:53

>> Very insightful. I know. So, we have the

39:56

gravity field and we have the pen that

39:59

has a mass. And the mass and the gravity

40:02

field interact and it drops. Now, if we

40:06

had another

40:07

>> I have uh object for you demonstration

40:11

purposes,

40:11

>> performance art. Here we go. This is

40:13

great.

40:13

>> This thing has mass and we drop it. How

40:17

remarkable. It falls. But when we step

40:20

back and think about what really

40:21

happens, it's the mass of this thing and

40:24

the interaction with this invisible

40:27

field we see here. That's what gives

40:29

this weight.

40:30

>> Now, I have this particle here that you

40:32

can't see, but it's there. It has no

40:34

mass and I leave it there. Well, since

40:38

it has no mass, it doesn't feel gravity.

40:41

It's still floating there.

40:43

And that is really all the Higs field

40:46

is. Some particles have effectively what

40:49

you could call the Higs charge that

40:51

interacts and sees the field and other

40:53

particles don't. And that is really what

40:57

what what you read just basically means.

41:00

Now it's kind of neat because in the

41:02

ordinary day there is a Higs field right

41:05

there and the Higs field is not zero

41:07

just like gravity is not zero and things

41:09

will get mass but at super high energies

41:12

the Higs field the strength of the Higs

41:14

field goes to zero so whether things

41:16

have mass whether they have a Higs

41:18

charge or not they have no char or they

41:20

have the Higs charge Higs field zero

41:23

they don't interact it has no mass so

41:26

that's kind of what uh Weineberg and

41:28

Salam Glass show said is at very high

41:30

energies, the Higs field is zero. Since

41:34

the Higs field is zero, the weak force

41:36

particles don't feel mass and therefore

41:39

they can travel at the speed of light

41:41

just like the photon does and

41:43

everything's happy.

41:44

>> Mhm.

41:45

>> It is when the universe cooled down

41:48

after the big bang. It was very hot,

41:50

very high energy. Nothing had mass. the

41:53

universe cooled and at a certain

41:55

temperature what happened is the Higs

41:57

field turned on and at the moment it

41:59

turned on it gave mass to the weak force

42:03

particles did not give mass to the

42:04

photons. So that's what we call

42:06

electroeak symmetry breaking. So, it's a

42:09

mouthful, but all it says is there was a

42:11

moment in time early in the history of

42:13

the universe at 10 the -12 seconds after

42:16

the big bang, the Higs field turned on

42:20

and particles got mass. So, that's the

42:23

whole idea. So, this is another really

42:26

neat thing. So, the electroeak symmetry

42:29

theory doesn't need Higs because that

42:32

only really applies at very very high

42:35

energies. But in order to make it work

42:38

at low energies, you need to fix the

42:41

theory. And you need to fix the theory

42:43

by effectively putting a band-aid on the

42:46

theory. Higs theory is just a band-aid

42:48

on top of electroeek symmetry theory.

42:51

And that is the band-aid that fixes it

42:53

because it gives mass to particles at

42:56

low energy. Well, how does then Higs

42:59

this band-aid the field and uh the Higs

43:01

Bzon come into play on the experimental

43:05

front on the evidence? Okay.

43:07

>> Discovery front. So, what is this uh

43:09

Higs Bzon?

43:10

>> Okay. Excellent.

43:11

>> So, we have never seen the Higsfield.

43:13

Higsfield is a hypothetical theoretical

43:16

thing.

43:17

>> But that is true of of most of our

43:21

fields. We've never seen the

43:22

electromagnetic field. We've never seen

43:23

the gravity field. We've seen the effect

43:25

of the field. And so all of these

43:27

theories are now what we call quantum

43:30

field theories. And that the whole idea

43:32

of quantum fields if you have a quantum

43:36

field, but that field can vibrate like a

43:39

drum head. And so it doesn't vibrate

43:42

just exactly like a drum head, but it

43:44

vibrates locally. So you can have

43:46

specific localized vibrations. And those

43:49

specific localized vibrations are the

43:51

particles. In the electromagnetic field,

43:53

the vibration is the photon. In the Higs

43:55

field, the vibration is the Higs Bzon.

43:59

And so what we can do is not see the

44:03

field, but we can actually excite the

44:06

field, make it vibrate and detect the

44:08

vibrations. So the Higs Bzon idea was

44:14

predicted in ' 64. It became useful in '

44:16

67. And then scientists started looking

44:19

for it. So in the early 2000s,

44:24

people were starting to think that we

44:26

had built part particle accelerators

44:28

more powerful or powerful enough to

44:31

actually to be able to create these

44:33

vibrations and detect them. So the

44:36

accelerator that was working at the time

44:38

was a large particle accelerator outside

44:41

Chicago at Firmeny Lab called the

44:42

Tevatron.

44:44

>> And we were colliding protons and

44:46

antimatter protons at near the speed of

44:48

light at very high energy. And that was

44:51

the accelerator at which the top quark

44:53

was discovered in '95.

44:55

But we had upgraded our apparatus. We

44:58

had 10 times the number of collisions

45:00

per second. We had slightly more energy

45:02

and we were banging the protons and the

45:04

antimatter protons together hoping that

45:07

we would actually find the Higs bzon.

45:09

>> Can you actually back up a little bit

45:10

and look at the bigger picture? So,

45:13

Firmy Lab has this legendary accelerator

45:16

that there's also a personal story with

45:18

you connected to it because I mean

45:20

there's a million questions uh I want to

45:22

ask you and we'll ask you about some

45:24

aspects of that. So, this idea of an

45:26

accelerator, the design and the physics

45:29

of an accelerator, how is that

45:30

productive for understanding

45:33

and discovering uh different aspects of

45:36

particle physics?

45:37

>> Well, I'm so glad you asked.

45:40

I mean, this is fascinating. All right,

45:42

everybody has heard Einstein's equation

45:45

E= MC². Nobody knows what it means.

45:47

Maybe they heard that energy equals mass

45:49

and mass equals energy. I don't know,

45:50

you know, but they've heard the

45:52

equation, the most famous equation in

45:54

all of science.

45:56

But buried inside that equation is a

46:00

really thoroughly fascinating concept

46:03

that energy and matter are equivalent.

46:06

And you can in fact convert movement

46:09

energy into mass. And so this is

46:14

something that we've known for a long

46:16

time. This was predicted back in

46:19

basically 1928. So a long time ago,

46:23

actually almost 100 years ago. And it is

46:26

not in the slightest bit controversial.

46:28

We can do this all the time. So the

46:31

simplest thing is to take two particles

46:34

that have no no structure. So you know

46:38

the closest thing you can have to BB's

46:41

that are just true mathematical BB's. If

46:44

you smash those two things together,

46:46

it's coming in with a huge amount of

46:47

energy from one direction, a huge amount

46:50

of energy from the other direction, the

46:51

directions cancel. So the net momentum,

46:55

the net energy of this has no motion. So

46:57

you have these two things coming in with

46:58

a you know exactly balanced energy and

47:02

if they collide they could stop. Well

47:04

that energy has to go somewhere and that

47:07

energy can literally create mass create

47:11

particles. Now there are special rules

47:13

about what happens if you have two

47:15

things coming together and it creates a

47:17

particle. It has to create an antimatter

47:19

particle to balance it. That's just kind

47:21

of the rules of the laws of nature. Why

47:24

is that the case? Well, we have some

47:26

ideas, but in many respects the answer

47:28

is because those are the laws of the

47:30

universe and that's the things that we

47:32

try to understand. But this is

47:34

absolutely true. So what what particle

47:38

accelerators do among other things is

47:41

simply transform energy into particles.

47:45

And so basically any uh particle that

47:50

doesn't exist in nature we can make in

47:52

this way. You can make the antimatter

47:55

electron by taking two particles,

47:58

smashing them together. The energy sits

48:00

there and it will make an electron and

48:02

an antimatter electron and it just does.

48:04

And we know that the antimatter electron

48:07

was discovered in 1932.

48:10

This is all pretty easy. The antimatter

48:13

proton was discovered in 1955 at the

48:16

Berkeley Bevatron.

48:18

And so this is just what you do. You can

48:20

convert energy into a matter antimatter

48:24

particle. Now the converse goes true and

48:26

that's something we might talk about.

48:27

You can take matter and antimatter and

48:30

bring it together and it'll make energy.

48:31

It's the uh the process can go both

48:36

ways. Energy can make matter and

48:38

antimatter. Matter and antimatter can

48:40

make energy. And this is just true. We

48:42

do it all the time. There's no question

48:44

that this is the case. We should also

48:45

mention that uh this is the reason why

48:48

Firmeny Lab had a nice stash of

48:50

antimatter particles. So as as a side

48:53

effect, you can also collect antimatter

48:55

in this kind of way.

48:56

>> You can produce antimatter, but it's an

48:58

extremely costly

49:00

>> well very very costly. Um in order at

49:03

the Firmeny Lab machine, we would have

49:05

to smash 100,000 protons into something

49:10

to make one antimatter proton. So I mean

49:13

it it took some work. Is there some

49:15

extremely precise recipe of uh of being

49:20

able to produce particular kinds of

49:21

particles and all this kind of stuff

49:23

when you smash two things together? Is

49:26

there like how can you control

49:28

accurately which kind of particles

49:31

you're trying to produce? If you want to

49:32

make antimatter electrons, you smash

49:35

together energy at a certain it's just

49:39

easier with electrons because the

49:42

electrons to the best of our knowledge

49:43

have nothing inside them. So they're

49:45

simple. They have a certain mass and

49:47

that's that. So if you smash particles

49:49

together with the right energy, you can

49:51

make them very very easily because you

49:53

can it's like a old style radio back in

49:56

the day where you had to dial it in. you

49:58

could get right on the station and you

49:59

could hear the the signal and if you

50:01

were off a little it didn't work. The

50:03

problem for things like protons and so

50:05

forth is they're not pointlike

50:07

particles. They're kind of like garbage

50:09

cans full of stuff and so it's very

50:10

difficult to make antimatter protons.

50:14

Now you can get more of them by

50:17

increasing the um energy at which you

50:21

collide two particles together. If

50:22

you're at below a certain energy, the

50:26

and you collide, say you collide two

50:27

protons together at kind of low energy,

50:29

you just don't have enough energy to

50:31

make an anti-roton

50:33

>> and so it doesn't happen. You get to a

50:35

certain energy and you can just barely

50:37

make them. The more energy you collide

50:40

them together, the more you make. So

50:42

that is just sort of how it works. More

50:44

is better. And then uh with with CERN if

50:47

you compare maybe CERN and Firmayab

50:50

going to perplexity here CERN's

50:52

accelerator the large hydron collider

50:54

LHC is the world's highest energy proton

50:57

collider while Firmayab's current and

50:59

plant accelerators focus on intense

51:02

proton beams for neutrino physics rather

51:05

than pushing the absolute energy

51:07

frontier. Absolute energy frontier

51:09

meaning highest possible energy

51:14

smashing of protons together.

51:16

>> Correct. So one we were talking about

51:18

like accumulating antimatter. Yes. All

51:21

right. And so um there that is typically

51:26

making anti-roton as opposed to making

51:28

all particles in general. So let's focus

51:30

on the anti-roton side to begin with.

51:33

All right.

51:33

>> So formula doesn't make anti-rotons

51:35

anymore. We stopped making them in 2011

51:38

and it's because we shut our big

51:40

accelerator down to concentrate on a

51:42

different facet of particle physics.

51:46

However, at the time we would smash um

51:50

protons with a an energy of 120 GEV and

51:55

in that we would make anti-roton. So

51:57

that's a ton of energy.

52:00

It's true that the CERN accelerator, the

52:03

big accelerator, is now much higher

52:05

energy than the Firmenab accelerator

52:07

was. No problem. But that's not how they

52:11

make anti-roton.

52:12

The all of these big beam uh big

52:16

laboratories, it's not one accelerator.

52:18

At Firmay Lab, there were five distinct

52:20

accelerators and it was basically like

52:22

shifting an old standard car cuz you

52:24

couldn't just go zero to super speed in

52:26

one accelerator. you had to go from one

52:28

to another getting higher and higher.

52:30

Well, at CERN, they use one of the

52:34

basically their second gear in their

52:37

very big accelerator complex to make

52:39

antimatter protons. And their

52:41

accelerator is only 26 GEV compared to

52:45

the 120 GV at Firmeny Lab. Firmay Lab's

52:48

not operating, but when it was

52:49

operating, it operated at an energy of

52:52

about four times higher than what CERN

52:54

is doing now. And why is that? Well,

52:56

it's because what CERN needs to do is to

53:00

not make as many anti-rotons as Firmay

53:02

Lab did. They are doing a very different

53:05

current experimental program. They're

53:07

doing a fascinating experimental program

53:09

including trying to figure out does

53:11

anti-gravity fall up or down, which is

53:13

kind of neat and we sort of know the

53:14

answer to that different that's

53:16

separate. But anyways, so getting back

53:18

to the anti-roton business.

53:20

>> Yeah.

53:21

>> Well, Firmay Lab doesn't do it now. It

53:22

was top dog. It's not anymore. Um, the

53:25

only really big anti-roton accelerator

53:28

creator is a small accelerator at CERN.

53:31

Okay, so that's the anti-roton thing.

53:33

And if we get back to antimatter, we

53:35

could talk about that because that is

53:36

way cool.

53:36

>> Yeah. So,

53:38

>> now the other side of your thing about

53:40

making high energergy unknown particles,

53:43

bigger is better. And it is true that

53:46

the LHC is a very high energy machine.

53:48

It is about seven times more powerful in

53:51

terms of energy per collision. It is

53:53

also about a hundred times more

53:56

collisions per second than the Firmeny

53:58

lab machine. So it is true that the LHC

54:03

can make bigger heavier

54:06

uh particles that the old firm lab the

54:09

Tevatron ever couldn't and that is true.

54:12

So if you want to look at high energy

54:13

stuff, yeah, you go to CERN now. Which

54:15

is why many of my colleagues including

54:18

myself once we had

54:21

measured all of the sort of frontier

54:23

measurements we thought we could make

54:26

with the Firmeny Lab accelerator, we saw

54:29

this bigger, more powerful machine with

54:31

seven times the energy and 100 times

54:33

more collisions per second. We said,

54:35

"Heck yeah, let's go work on that." And

54:37

to give you a sense of scale, the top

54:39

quark, which is the heaviest particle

54:42

ever discovered, discovered at Firmeny

54:44

Lab in 1995. There were two discovery

54:46

papers and the one on which I was a

54:48

co-author. We had worked for a good

54:51

chunk of between 6 months and a year of

54:54

collecting collisions and there were a

54:56

lot of collisions and our paper had 38

55:01

top quirk candidates. 38. And we knew

55:05

that half of them were crap because when

55:07

you make a detector like that, there's

55:09

what you call background. So you have

55:10

the background and the good stuff. And

55:11

we know it was about 50/50. So we had

55:13

maybe 19 top quarks after working for

55:17

between 6 months and a year of

55:18

collecting data. But now at the LHC, we

55:23

make a top quark every second.

55:27

And that's what higher energy and more

55:29

collisions per second will do for you.

55:31

That extra energy, you're above

55:33

threshold. You make a ton of them. And

55:35

when you compare the 1995 Firm Firmab

55:39

accelerator to the current CERN

55:41

accelerator, it's probably a thousand

55:42

times of collisions per second. So it

55:45

went from painstaking, pulling teeth to,

55:48

yeah, now top quarks are a background.

55:50

We try to get rid of them. There's just

55:52

too many of them. They get in the way of

55:54

searching for the stuff we really want

55:56

to search. They are like so 30 years

55:58

ago. By the way, is there something to

56:00

be said about the the kind of sort of

56:02

signal processing here? How you remove

56:05

the noise, how you remove the

56:06

background, how you determine which

56:08

particle is which. There's probably some

56:10

like incredible nuance there

56:12

>> even outside of the scope of this

56:14

conversation.

56:14

>> So, let me just throw some numbers out.

56:16

All right. So, at the CERN accelerator

56:19

when it's operating, the collisions

56:21

occur at a prodigious rate. We get about

56:24

a billion with a B collisions per

56:26

second. Now each one of those Yeah.

56:30

Yeah. That's what I said. Wow. Now it

56:31

turns out some of them are happening at

56:33

the same time. So there's about of order

56:36

40 million moments in time per second

56:40

where you would take a shot and inside

56:42

that moment there might be 20

56:45

collisions.

56:46

>> So that's why where we get to the

56:47

billion.

56:48

>> Yeah. But can you individually pinpoint

56:50

the collisions

56:51

>> sort of to a to a degree. So the beams

56:54

are, you know, the when people think of

56:57

beams, they think of like laser beams,

56:58

but that's not really what particle

57:00

beams look like. Particle beams look

57:03

like little tiny sticks of spaghetti,

57:05

except they're much thinner. They're not

57:07

as fat as a stick of spaghetti, and

57:09

they're at the LHC. Different

57:12

accelerators are different. They're

57:13

about this long. And so you have one of

57:15

them going one way full of protons and

57:18

another one going the other way full of

57:20

protons. And they pass through each

57:21

other. And as they pass through of each

57:23

other, you should think of this as like

57:25

a swarm of bees. And this is like a

57:27

swarm of bees. And mostly the bees pass

57:30

through each other and don't do

57:31

anything. But every so often some of the

57:32

bees hit nose on and stripes and and and

57:37

wings and everything everywhere.

57:38

>> That's awesome.

57:39

>> And so as they collide through each

57:41

other, you know, one collisions here and

57:43

one's here and one's here and you can't

57:45

tell too much side to side because the

57:48

beams are really small. They're sort of

57:50

the thickness of a human hair. But you

57:52

can see along the direction and there,

57:54

you know, this is about the right size.

57:56

And so we have detectors around them and

57:59

we can actually see, oh, particles came

58:02

from here and particles came from here.

58:04

And that's amazing. All right. So at any

58:07

one crossing, there's maybe 20

58:09

collisions. Now, most collisions are

58:12

absolutely boring. They're boring

58:14

because they are they they exemplify

58:18

physics that we know a great deal about

58:19

already. We've tested it for for

58:22

decades. We know all about it. We don't

58:24

care. I mean, it's kind of blas that we

58:27

can say, "Oh, yeah, yeah, we're making a

58:28

billion partic subatomic particles every

58:31

second, but who cares?" Because, you

58:33

know, but that's just the way of, you

58:34

know, frontier scientists. So, what you

58:37

need is you need to pick out the cool

58:40

ones, the weird ones, the ones that

58:42

nobody's seen before. And so what

58:44

happens is uh these things these beams

58:49

uh collide and we surround the collision

58:52

point within the enormous detector.

58:55

There are two absolutely ginormous

58:57

detectors at the LHC. One of them called

58:59

CMS which is the one I'm on and the

59:02

other one is called Atlas

59:04

>> which is the other one and we don't

59:06

speak of because well no they're both

59:08

really amazing.

59:09

>> Okay. It's good to know that there's

59:10

friendly competition even inside

59:13

that's awesome.

59:13

>> I mean the fact is they are both amazing

59:16

absolutely amazing detectors

59:17

>> but CMS is just a little cooler than

59:19

>> Oh yeah. Yeah. I mean you know in in in

59:22

particle physics we really absolutely

59:24

want our competitors to do extremely

59:27

well just not quite as well as we do.

59:29

>> Got it. All right. So these two giant

59:31

detectors

59:32

>> right. So but one of them our detector

59:34

the CMS detector it's the small one. It

59:37

is 70 ft long, 50 ft high, 50 ft wide.

59:40

It's 5 stories tall. It weighs 14,000

59:43

tons.

59:44

>> Small

59:45

>> small. Atlas experiment is 150 ft long,

59:48

80 ft across. It weighs only 7,000 tons.

59:51

Just piece of cake.

59:52

>> You could take the Atlas detector and

59:53

you could put four of them on a soccer

59:56

or football field and it would fill the

59:57

field up with just enough room on the

60:00

sidelines for the cheerleaders and the

60:01

water boy and the coaches and stuff.

60:03

That's how big they are. So these are

60:05

absolutely ginormous detectors and

60:07

basically they're cameras and what they

60:09

can do is they can take pictures 40

60:11

million times per second. Now all the

60:14

data comes streaming off that detector

60:16

and we can't record it all. It would

60:18

just fill up all of our tapes and it

60:19

would be full of all these boring things

60:20

we don't care about. So what we do is as

60:23

the beams pass through one another, we

60:27

teach our detectors to say we only want

60:30

one where there are certain

60:32

configurations that might be interesting

60:34

like there's gobs of energy in the

60:36

detector or there's a gob of energy on

60:39

one side and nothing on the other side

60:41

or there's four gobs of energy or

60:43

whatever. These are called triggers. And

60:45

so these what we have is fast

60:47

electronics that take the 40 million

60:50

possible pictures per second and it says

60:55

you know about a 100,000 of those are

60:57

really cool. We should think about them.

61:00

And then it passes not all of the 40

61:03

million but those 100,000 to the next

61:06

level which are commercial processors

61:09

that have uh basically our final uh

61:13

analysis code but optimized to run very

61:15

very quickly. And what they do is they

61:18

do a really quick and dirty analysis to

61:20

say to to further refine what's good and

61:23

what's not. And that that computer form

61:27

then accepts about a thousand collisions

61:30

per second and we record those for

61:33

further analysis. So that's what's

61:35

really happening of the 50 million

61:36

possible collisions per second the fast

61:39

electronics and then the computers pick

61:41

the thousand and then we pass those

61:44

through analysis software and hand them

61:46

to the graduate students and they pick

61:47

through them looking and finding the

61:49

handful that are the next Nobel Prize.

61:52

So that's how that works and that that

61:54

is truly astonishing. I'm hats off to

61:57

the accelerator builders, the detector

61:59

builders, the the the people who make

62:01

the software work, the people who make

62:03

the not not gigabytes, not terabytes,

62:06

but pabytes of data flow around the

62:08

world seamlessly. It's really amazing.

62:10

I'm very grateful.

62:12

>> Uh so take me to uh July 4th, 2012, the

62:16

discovery of Higs Bzon. So this is

62:19

really fun because the people searching

62:23

for the Higs, it's a it's a community

62:25

and the entire community knew that the

62:30

LHC was coming online. So even though

62:32

many of us had been working on the

62:35

Firmenab accelerators, a lot of us were

62:37

transitioning to the CERN uh

62:40

accelerator. So we were in the very

62:43

funny business of wearing our Firmenab

62:46

detector people hats trying desperately

62:48

to find the Higs Bzon at Firmeny Lab

62:52

>> while simultaneously wearing our CERN

62:55

hats knowing that CERN was going to be

62:57

able to find it if existed. And so you

63:00

know we were a little neurotic kind of

63:01

wanted you know our old stuff to work

63:05

and and there was an awful lot of people

63:06

on both experiments. Did you um have a

63:10

sense that one of the two places would

63:12

be able to find the Higs? First, did you

63:14

think the Higs Bzon existed? And second,

63:17

did you think that these accelerators

63:20

have the chance to find them?

63:22

>> So, I was cognizant of the fact that the

63:24

Higs Bzon might not exist, but there was

63:27

a lot of evidence pointing in the

63:29

direction that it might be. I knew that

63:33

both experiments, the Firmeny Lab

63:35

accelerator and the CERN accelerator

63:37

would either find or rule out the Higs

63:41

if it existed.

63:42

>> Rule out?

63:43

>> Well, that's a possibility. I mean,

63:44

maybe the Higs theory was wrong.

63:46

>> Yeah.

63:46

>> Right. Until you until you know it's

63:48

there, it might be wrong. It's like dark

63:49

matter. People talk about dark matter.

63:51

It might not be real.

63:52

>> I mean, I it probably is, but it might

63:54

not be.

63:55

>> So, you knew at these energy levels, you

63:57

would be a you should be able to find

63:58

the Hig boson.

63:59

>> Yes. So that's the nice thing about this

64:02

kind of physics because there was a

64:04

theory that theory made predictions. Now

64:08

there were parameters in the theory we

64:10

didn't know if the mass was this we'd

64:12

get this thing. If the mass was this we

64:13

get this thing. But we could do the the

64:16

calculation for every conceivable Higs

64:19

mass. And so then we could search look

64:22

well let's say the Higs mass is 100 in

64:24

some units. Did we see it there? No.

64:27

then it's not 100. Well, let's look at

64:30

103. Is it there? No. So, we could do

64:33

that. Both accelerators could either

64:36

find it or definitively rule out the

64:39

predictions of simple Higs theory. 100%

64:43

guaranteed.

64:45

>> However, the CERN accelerator had 10

64:49

times the collisions per second and

64:52

three and a half times the energy. So

64:55

remember when I said it with the top

64:56

quirks it was like 6 months for 19

64:59

versus one a second. There's no question

65:02

the writing is on the wall. The h the

65:05

the LHC was going to have an easier time

65:07

of it if it was real.

65:09

>> However, so but you know I'm a Firmay

65:11

Lab scientist and we wanted Firmen Lab

65:14

you know come on we want Firm Lab to win

65:16

not you know. So we were busting our

65:18

butt and we had done what I said. We had

65:20

ruled out this region. And we had

65:22

certain R mass ranges. We knew it wasn't

65:25

there. And we finally said if there was

65:29

a Higs Bzon, if it existed, which we

65:31

didn't know at the time, its mass was

65:34

somewhere between, if I recall, between

65:36

like 120 and 145. All right, we'd ruled

65:39

out all the other stuff. And so, wearing

65:43

our our CERN hat, we said, "Okay, we're

65:45

going to find that." But we were really,

65:47

really, really trying to do it. Now, if

65:49

we had had another 2 years or maybe 3

65:53

years of running the Fermy accelerator,

65:57

Fermy Lab would have discovered or ruled

66:00

out or in this case turning out

66:01

discovered the Higs boson because it's a

66:03

real thing. We would have found it

66:04

without a question, but we didn't have

66:07

enough data in July of 2012. We needed a

66:12

couple more years. Unfortunately,

66:15

in 2008, or fortunately, the LHC had

66:18

turned on. It broke. They had to fix it.

66:20

Turned on again in 2010. It ran poorly

66:23

in 2011. In 2012, they pushed up their

66:26

sleeves and said, "Let's do this." And

66:29

it turned on. And so, you know, there

66:32

was this the Firmy Lab knew if it didn't

66:35

have it now, it wasn't it was too late.

66:38

Anyways, come 2012 rolls around and um

66:44

like two days before

66:46

uh the announcement at CERN was July

66:48

4th. So two days before that, Firmayab

66:50

made a measurement and said we can rule

66:53

out certain regions but certain regions

66:57

we can't rule out but what we know and

67:00

this is important. If the Higs Bzon

67:02

exists, it must be in this region for

67:05

which we are not capable yet of ruling

67:08

out. So that's where we were 2 days

67:12

before the LHC said we got it. That was

67:17

uh July 4th, 2012. So detecting the Higs

67:21

Bzon confirmed the existence of the Higs

67:24

field, the mechanism through which

67:27

fundamental particles like electrons and

67:28

quarks acquire mass in the standard

67:30

model. Correct? Although let's be very

67:34

specific of what we did then we found a

67:38

particle consistent with the existence

67:41

of the Higs boson. There were

67:43

alternative theories at the time that

67:45

predicted not one but multiple Higs

67:48

bosons. So there's a theory called super

67:51

symmetry which said that there was not

67:52

one but five Higs bosons. The standard

67:56

original 1964 Higs theory says there

67:58

were one. And so all we really knew at

68:01

the time was we found a theory. We did

68:04

not necessarily confirm that Higs was

68:06

right. We found data that said that it

68:09

looked like Higs was right. But until we

68:12

ran for longer, we were unable to rule

68:15

out other alternative theories. So

68:18

that's the the deal. Now in the fullness

68:21

of time, it is after all uh what 14

68:25

years now later, we have been able to

68:27

basically rule out some of those other

68:28

things. And by now we have validated a

68:32

things. We found the mass of the

68:33

particle. We know the spin of the Higs

68:36

Bzon. It has a spin of zero. We have

68:39

discovered Hig Bzon decays. It

68:42

preferentially decays into the heaviest

68:45

particles. It can through energy

68:47

conservation can't decay into top

68:50

quarks. It's too light to decay into top

68:52

quarks, but it can decay into bottom

68:54

quirs. It can decay into W and Z

68:56

particles. Can decay into a weird way

68:58

into photons. And we have looked for all

69:02

of the hypothesized decays of the

69:06

original Higs theory. And we have

69:08

validated that it decays in those ways

69:11

at the rates that theory predicted. And

69:15

so now in the fullness of time, I'm

69:17

pretty comfortable saying Peter Higgs

69:20

and Robert Brout and Franco and his

69:22

colleagues, they were right back in the

69:24

60s. But we weren't sure on July 4th.

69:27

All we knew is we found a particle

69:29

consistent. But the thing is with these

69:32

discoveries, they're often just barely

69:34

discoveries. it takes a while to go and

69:36

do the more complex detailed

69:38

measurements and that's what we've done.

69:40

>> So at the time I remember being called

69:43

referred to as the god particle.

69:46

>> Uh you also uh had a minor in theology.

69:51

So throwing that all together. So

69:54

calling it the god particle is speaking

69:57

to the importance the potential

69:58

importance of discovering this particle.

70:00

Do you think uh that is in some degree

70:03

justified like if we look at the big

70:04

impact of it on the the history of

70:07

physics? How important was it to find

70:09

and show that the the the Higs fields is

70:13

real?

70:14

>> Well, I don't think it is as important

70:16

as for instance some of Einstein's

70:17

stuff. I mean it was it's an important

70:20

prediction like the prediction of quirks

70:22

was very important and interesting in

70:24

validating this. The Higs was kind of

70:26

like um validating that quirks existed.

70:30

it it's an important stepping stone and

70:33

I I do not wish to to denigrate it in

70:36

any way but there's ones that change the

70:38

way we thought about the world like

70:40

Einstein did it wasn't that sort of

70:43

thing and there is a funny story so the

70:44

reason they call it the God particles

70:46

this book by Leon Letterman and um and

70:50

if you read his book he uh he says well

70:54

you know we we call it the god particle

70:56

but but we should call it the godamn

70:58

particle because it's been causing us so

71:00

much trouble trying to find it.

71:03

>> And Leon ran Firmy Lab. So, and he wrote

71:05

a a forward for one of my books. And you

71:07

know, I talked to him. He's he was a

71:08

really funny guy.

71:10

>> And the real truth was the book was

71:13

called The God Particle because his

71:15

publisher thought it would sell more

71:16

copies.

71:18

>> But but you know, then that got into the

71:20

mindset of the reporters and so forth

71:21

and we called it the God Particle. Leon

71:23

never really thought of it as anything

71:26

to do with a religious or even I mean he

71:28

was an incredible jokester. the goddamn

71:30

particle.

71:30

>> It is a really important part of our

71:32

model of the universe. It is that

71:34

there's this field that it gives mass to

71:36

some particles and not others. That's

71:38

>> right. It it's a huge thing but it was

71:41

part of the standard model. The standard

71:43

model had known forces. It had known

71:45

particles. It had all that. The the Higs

71:48

Bzon the one thing that is true is it

71:50

was the last

71:52

unvalidated

71:54

piece of the standard model. The

71:56

standard model does not answer all

71:58

questions which is why we have

72:00

unanswered questions in physics. But it

72:03

was a punctuation point end of about 50

72:05

years of discovery and searching where

72:07

we finally were able to say the standard

72:10

model while while incomplete, it's

72:13

mostly right as far as it goes. Quick

72:17

10-second thank you to our sponsors.

72:19

Check them out in the description. It

72:20

really is the best way to support this

72:22

podcast. Go to lexreman.com/sponsors.

72:26

And now, dear friends, back to my

72:28

conversation with Don Lincoln. We did a

72:32

whirlwind tour of the history of physics

72:36

and took a little tangent on this

72:39

incredible discovery of the Higs boson.

72:42

Uh, but we didn't go all the way yet.

72:44

There's this dream of the grand unified

72:47

theory, the gut that uh is a step

72:51

towards the toe theory of everything. So

72:53

can we talk about the gut first? So what

72:55

what's what's entailed in the gut? So

72:58

the gut is short for grand unified

73:01

theory. We talked about that there were

73:03

four known subatomic forces. the um

73:06

electromagnetic force, gravity, the

73:08

strong force and the weak force and

73:10

electroeak symmetry unification merged

73:13

the weak force and electromagnetism into

73:16

the electroeak force. So what gut hopes

73:19

to do is to merge the electroeak force

73:23

and the strong force into one grand

73:25

unified force. Now that leaves gravity

73:27

outside because gravity is seemingly

73:30

fundamentally significantly different.

73:32

Then subsequently it is hoped that a

73:35

higher energy we will be able to blend

73:38

the theory of everything together with

73:40

all of the known subatomic forces the

73:42

strong weak and electromagnetic forces

73:44

and then gravity but so as you say gut

73:46

is sort of a a way station along the way

73:49

that's the goal and uh at this point I

73:53

would have to say that I do not see a

73:58

fast progress in the immediate future. I

74:00

think we're a ways away from that at

74:02

this point.

74:02

>> You mean on the gravity front?

74:04

>> Maybe we'll come up with something

74:05

really cool. We certainly had some ideas

74:08

back in the early 80s that we tested and

74:10

they didn't pan out.

74:12

>> Uh speaking of which, string theory is

74:14

the thing you're referring to.

74:16

>> Uh so string theory posits that

74:20

particles are tiny vibrating strings and

74:22

by tiny we mean extremely tiny at the

74:25

scale of a plank length. Uh then there's

74:28

there's other leading candidates like

74:30

loop quantum gravity. Uh maybe there's

74:33

some alternate theories in the works. So

74:36

can you uh linger on that a little bit

74:38

more? Do you think a theory of

74:41

everything exists? So I hold personally

74:44

that there are rules that govern matter

74:46

and energy space time and they probably

74:49

are rules that I don't know. There are

74:51

probably phenomena I'm not aware of. But

74:54

I do believe that something there are is

74:57

a rule that governs reality. And so in

75:01

that sense once we understand the rules

75:04

that govern reality, the fundamental

75:06

rules that would be a theory of

75:07

everything. You know there are things

75:09

that are unknowable like for instance

75:11

inside black holes we don't know what's

75:13

inside there but that doesn't mean that

75:14

there's not something inside there. So

75:16

there's a distinction between what we

75:18

can know and truth. So I I do believe

75:22

that there are the rules and I do

75:26

believe that with sufficient time,

75:28

technology, effort, we will be able to

75:30

figure this all out. Now, this isn't a

75:32

thing in my lifetime. It's not a thing

75:34

in my grandchildren's lifetime or even

75:36

their grandchildren's lifetime.

75:38

>> Whoa, whoa, whoa. That's a pretty strong

75:39

statement, right? That's a pretty strong

75:41

statement saying we're

75:44

>> we're 50 to 100 years out from finding a

75:47

theory of of everything. It took 200

75:49

years to go from unifying gravity to

75:52

unifying electromagnetism. It took a

75:54

hundred years to go from unifying

75:56

electromagnetism to unifying the

75:58

electroeak force. Now you could say,

76:00

well, gee, that's went from 200 to 100.

76:03

So it's getting faster, but it's also

76:05

getting harder because the unification

76:07

scale is of order 10 the 15, which we

76:12

can do the math. That's a quadrillion

76:14

times higher than the highest energy

76:17

accelerator we can build today.

76:19

>> And it was one thing to, you know, we

76:22

are reaching diminishing returns. We get

76:24

something like a factor of seven

76:27

increase in particle accelerator energy

76:30

every 20 years. And so we have to get to

76:34

a quadrillion times. Now, you know, if

76:38

you really did believe uh a factor of

76:41

seven every 20 years, then that's we're

76:43

talking like 500 years, but you know,

76:45

this is like Mo's law that it doesn't

76:47

continue forever. We're not going to

76:49

every seven year. I mean, every 20 years

76:51

get another factor of seven. So, yes, I

76:53

I think it's a very long time. That's my

76:55

prediction. Um, you know, some people

76:57

are far more optimistic and we can talk

77:00

about that. We should also actually

77:01

mention

77:03

that I guess your intuition behind that

77:05

is not just the part where you come up

77:08

with a theory that's beautiful and seems

77:11

to be internally consistent, but you

77:14

have to have a theory that's making

77:16

falsifiable testable predictions.

77:19

>> Correct? And you have to have a a

77:23

feasible

77:24

engineering construction a methodology

77:27

for creating an experiment that tests

77:29

that prediction. So I think a lot of

77:32

your this is 50 100 200 years from now.

77:35

Intuition is maybe about the second part

77:38

of that which is like you need to have

77:40

an experiment. Yeah. Yes. Yes. But you

77:44

know let's say I mean you alluded to

77:47

super strings. I haven't answered that

77:48

question. And I'll table that for a

77:49

moment. Super strings is a fascinating

77:51

idea. I don't believe it. Um but I love

77:54

it. I hope it's true. And there's a

77:56

real, you know, apherism and it says you

77:59

should absolutely never believe what you

78:01

think. So even if you think Superstrings

78:03

is true, you shouldn't believe it

78:04

because it hasn't been tested.

78:06

>> Now let's say super string is correct.

78:11

I mean hypothesis it's correct. 100%

78:13

correct. I don't know it's correct. So I

78:16

don't care. I mean, you know, it could

78:18

be correct, but I don't, you know, until

78:20

it's validated, it's just a wild ass

78:23

guess, you know. So, I we have to have a

78:26

way of validating it. So, yes, the the

78:28

the empirical side of it is important. I

78:31

mean, you could wake up tomorrow and

78:33

have the theory that is the perfect

78:35

theory, but if I can't prove it, I don't

78:38

care. If we were to think, this is going

78:40

back to the great courses on the

78:42

evidence for modern physics,

78:45

>> we're talking about energy levels and

78:49

tiny particles

78:51

to the degree where the kind of

78:53

prediction we would be making is not

78:55

accelerator type predictions. So,

79:00

it's probably going to be impossible to

79:01

build an accelerator that detects

79:03

something like a string.

79:06

So you have to make predictions

79:09

about macrocale behaviors.

79:13

>> That's another alternative.

79:15

>> It's a different kind of prediction.

79:17

>> Sure.

79:18

>> Do we even have intuitions about what

79:20

kind of predictions they would be? So

79:22

one one of course one of the lines of

79:23

intuitions has to do with black holes

79:26

where in the singularity

79:28

the physics of black holes combine

79:30

certain elements of general relativity

79:32

and quantum mechanics. So there

79:34

>> you could see some kind of predictions

79:37

you can make.

79:38

>> Uh but you can't really mess with a

79:40

black hole. It's not like you can create

79:42

a black hole in the lab.

79:43

>> And the energies that you were talking

79:45

about, the sizes we're talking about are

79:47

inside a black hole, which you can

79:48

intrinsically never see.

79:50

>> Yeah.

79:51

>> So you know, you can only see the

79:52

outside of a black hole, not the inside

79:54

of a black hole. So what you said, you

79:56

did say something that was incredibly

79:58

important and incredibly correct and

80:00

probably won't happen, but that's still

80:02

good. Okay. So we have two choices when

80:06

you talk about super strings. Either

80:08

super strings are correct and they're

80:09

making predictions up at the plank

80:11

energy scale at which point we have to

80:14

somehow build facilities that can

80:16

generate plank plank energies. That's

80:18

possibility one. Possibility too is this

80:22

theory which is currently only

80:25

applicable at plank energy scales.

80:28

Someone figures out a way to take those

80:31

equations and solve them in a way that

80:35

say predicts the mass of the electron.

80:37

>> Mhm.

80:38

>> Right. And that is a tricky business.

80:41

Um, I am not a string theorist, so I

80:43

can't tell you that that's likely, but I

80:46

can tell you that they've been working

80:47

on it since the 80s, and they haven't

80:49

gotten very far. Furthermore, if I uh I

80:53

think it's fair to characterize that

80:55

string theory is still a a vague idea,

80:59

and that's unfair. But let me tell you

81:01

why I say that. Because what they have

81:04

are approximate solutions to approximate

81:07

equations.

81:10

And that is already saying that we're a

81:14

ways away from really getting a handle

81:16

on that. So yes, if there could be some

81:20

bright young ladder lass out there,

81:21

someone listening to this podcast right

81:23

now who figures out a way to take super

81:25

string theory and solve them in

81:28

tractable ways that makes predictions

81:29

from the scale at which they currently

81:31

apply down to measurable scale today.

81:34

And if that happens, well, then I might

81:36

retract my my question or my my concept.

81:41

There's a reason why I think that

81:42

probably isn't true. That's probably not

81:46

valid. So, let let me I I love this. All

81:49

right, so let's back up. I'm going to

81:51

pitch. I wrote this book for Oxford,

81:53

Einstein's Unfinished Dream. And

81:54

Einstein's unfinished dream was to come

81:56

up with a theory of everything. It was

81:57

unfinished because, well, it's

81:59

unfinished. And so the the second part

82:02

the tagline of that book is practical

82:04

progress towards a theory of everything

82:05

with the emphasis on practical. Because

82:08

when you read books about theories of

82:12

everything, when you see podcasts, when

82:14

you listen to YouTube videos or

82:15

whatever, they are often written by

82:18

theorists. And theorists are they're big

82:22

idea people. They're very very smart.

82:25

But but there's a pragmatism that is

82:28

often missing in the sense that they say

82:31

well super strings look you know have

82:33

these little vibrating things and

82:34

wouldn't it be cool and you know but you

82:36

got to get to the do you know it. So

82:40

let's pretend super string theory or

82:41

something like it is correct. The energy

82:44

scale at which um that should occur is

82:48

of order um 10 to the 15 times higher 10

82:52

to the 19 Gev. We can currently do

82:55

things at 10 the 4th GEV give or take.

82:58

So that is 10 the 15 that's a

83:00

quadrillion times higher energy.

83:03

So what we are doing now is we are

83:05

looking at the world with our very best

83:07

measurements and we are trying to

83:09

project out a quadrillion times higher

83:13

and figure out a theory that explains

83:15

everything. Now I I have this I have a

83:19

couple of analogies but I like this.

83:20

Suppose that you were some, you know,

83:22

Joe oustralopythecus 2 million years ago

83:25

or something in Africa wandering around

83:28

somewhere in Kenya.

83:29

>> Mhm.

83:30

>> All right. You're about a meter in size.

83:32

So you can walk a meter meter scale is

83:34

like your scale.

83:36

>> Mhm.

83:36

>> You can walk 10 meters in every

83:37

direction. That's 30 ft. No problem. You

83:39

can work 100 meters, 300 feet. You can

83:42

work a thousand meters, that's half a

83:43

mile. You can work 10,000 meters, that's

83:47

60 miles. 100,000 meters is 10 to the

83:49

5th. And that that's unlikely. But the

83:53

distance that we need to go from what we

83:55

can see to the plank scale, it's not 10

83:57

to the 5th, it's 10 to the 15th. So that

84:00

means in my analogy, think about this

84:03

guy who's walking around Africa. Now, if

84:06

he walks, you know, 100 ft or something,

84:08

it looks a lot like what it is now. He

84:10

can make a prediction about what he

84:11

sees, and when he goes to that new

84:13

place, it's probably going to be okay.

84:15

But if he starts walking 500 miles east,

84:18

well, he walking around the center of

84:21

Africa has no concept of, for instance,

84:23

the Indian Ocean, he would never predict

84:26

sperm whales or Kraken. He would never

84:29

predict what it's like the bottom of the

84:31

ocean is going north. He's he's in

84:34

Africa. He would never ever have a clue

84:36

about the Alps or Antarctica. Going even

84:40

smaller distances, going a mile up,

84:43

things wouldn't be very different. But

84:44

if he goes 10 miles up, he wouldn't

84:46

breathe and he'd freeze. If he goes 100

84:48

miles up, he would die. If he goes two

84:50

miles down, he would roast. The point

84:53

being is

84:56

we are like that oropycus. We have a

85:00

realm that we can study and we can even

85:04

predict to some validity what would

85:06

happen if we go some distance away. But

85:09

the farther away we go, the less and

85:12

less our local prediction really

85:15

represents the reality of those more

85:17

distant times. And so basically his

85:21

theory about the the world would be

85:23

totally bogus. So even if he had the

85:25

best theory, his theory would not have

85:27

anticipated the elps. It would not have

85:30

anticipated penguins,

85:33

>> right? Flamingos not there, you know,

85:36

>> and that is just the case. So now that's

85:39

what we're doing. We are taking

85:41

something and we have reason to

85:43

understand what we know and we can

85:45

predict a factor of 10 or 100. But I

85:48

think it is the absolute

85:51

the pinnacle of arrogance to think that

85:52

what we can do given the understanding

85:55

that we have from what we've measured

85:57

now and predict it out a quadrillion

86:00

times higher than we can see now. So my

86:04

opinion and this is partly because I'm

86:05

an experimentalist. The correct way to

86:08

make progress, practical progress

86:10

towards a theory of everything, is to

86:12

look around at the things that we don't

86:15

have answers to right now. For instance,

86:18

are there something smaller than quarks?

86:20

I don't know. Is dark matter real? I

86:24

don't know. If it's real, what is it? I

86:27

don't know. Is dark energy real? Yes,

86:29

probably. But I don't know. What is the

86:32

nature of space and time? I don't know.

86:35

But these are questions we can explore.

86:37

And I would expect, and this is my

86:39

prediction, that all right, we're going

86:41

to figure things out at a factor of 10

86:43

or 100 times better than we can do now.

86:45

And we might be able to do that in my

86:46

kids' lifetime or something like that.

86:49

But in order for us to predict a

86:52

quadrillion times higher, I'm pretty

86:54

sure super string theory is wrong. Not

86:56

because people aren't smart, but because

86:58

something new is going to happen. I

87:00

mean, if you were talking about

87:02

chemistry, you would have never

87:04

predicted nuclear physics. And that's a

87:06

small increase in energy, right? The

87:09

idea that there is something in the

87:10

nucleus of atoms that causes the sun to

87:12

burn. There's a reason why people didn't

87:15

believe, you know, they they calculated

87:17

how old the sun should be and it should

87:19

only be 10 million years old because

87:20

otherwise it would burn out. Well,

87:22

that's clearly wrong. And it's wrong

87:24

because of nuclear physics. That is why

87:27

I feel fairly confident to say while

87:31

someone could think well super string

87:32

might be right or something and maybe

87:34

it's right and I hope it's right. It

87:35

would be awesome if it's right but what

87:37

are the odds when you making something

87:40

with that tiny lever arm predicting it

87:43

out a quadrillion away and say oh yeah

87:45

we got it right. What are the odds? And

87:48

my answer is you got to be kidding me.

87:50

Now I could be wrong and I admit that I

87:53

could be wrong but that's why I I think

87:55

the real issue is not the brilliance of

87:58

humanity. It's the stuff we haven't

88:00

found. We don't know. I mean the simple

88:03

one and I'm say simple and it's not but

88:07

what is dark matter.

88:09

>> We don't have a bleeping clue. Not a

88:12

clue. We know a lot of what it isn't but

88:14

we don't know what it is. And so you

88:16

know talk about super strings. All

88:17

right. Well, maybe dark matter fits in

88:19

superstrings. Or maybe dark matter is

88:22

governed by a physics that is completely

88:24

diametrically opposed to the super

88:25

string concept.

88:26

>> And allow me a bit of a thought

88:28

experiment here. A brief thought. My

88:31

intuition says that when you propose a

88:34

theory of everything, the kind of

88:36

prediction you want to make involves a

88:40

kind of leap of conceptual understanding

88:42

that Einstein did. So for example, you

88:44

want to come up with something like

88:47

spacetime and then gravity bends space

88:51

time.

88:53

>> So it's not merely that you have this

88:54

beautiful mathematical framework,

88:58

but that framework allows you to rethink

89:03

how you see reality enough to make a

89:07

prediction that's about the macro world.

89:10

I mean to come up with something like

89:13

spacetime you know there's one idea for

89:16

instance to say that space and time

89:17

aren't real they they emerge from from

89:20

entropy yeah that's a way of a new way

89:22

of thinking and maybe there's some

89:24

validity and I want people to think

89:25

about it but in the end it's just an

89:29

idea and that's the real key thing and

89:32

and as you say it has to tie to a macro

89:34

world you have to validate if you don't

89:36

validate it's a crazy idea theorists are

89:41

incredibly creative, smart, wonderfully

89:45

interesting people. But I don't care. I

89:48

want a measurement that validates the

89:50

idea because there are so many I mean if

89:53

you read the the journals, there are so

89:55

many theoretical papers with all these

89:57

nifty ideas that die. you know, uh, one

90:00

that was recently I liked and and might

90:03

still be true was, um, that dark matter

90:07

that, you know, our simple model of dark

90:09

matter is that there's a subatomic

90:11

particle out there that's heavy and it's

90:12

floating around and it's causing

90:13

gravity. But someone said, well, you

90:15

know, maybe there's complex dark matter,

90:17

which means there's a whole dark sector.

90:19

So, there are dark atoms and they

90:20

interact with one another. And that is a

90:22

nifty idea and I love it. And that was

90:26

all the rage for a while. and we looked

90:27

at it and it may still be true but the

90:30

simple ideas have been mostly

90:32

invalidated

90:33

because we've tested it and it doesn't

90:35

work. Same thing there was a talk about

90:38

um large extra dimensions. The reason

90:40

that gravity is so much weaker than the

90:42

other forces was well maybe gravity can

90:44

sneak into more dimensions than the

90:46

other forces.

90:47

>> It leaks into those dimensions.

90:49

>> That was a cool idea. I mean but that's

90:50

the point is you have these lovely cool

90:53

interesting ideas that constantly die.

90:56

Mhm.

90:57

>> And so,

90:59

you know, I I would love for a new nifty

91:02

idea to be the idea, but I don't know

91:04

how to pick it out of the the hurricane

91:07

of wrong ideas.

91:08

>> I mean, that's the real beauty of

91:10

science. It really is. I mean, the

91:13

theories kind of get some of the glory

91:15

sometimes, but the real beauty emerges

91:18

from the experiment and the

91:20

demonstration that the theory is is

91:22

correct.

91:22

>> And there are two directions. You're

91:23

talking a top down. someone comes up

91:25

with this big idea that's testable. But

91:27

you also have the other way that science

91:30

advances and it's not with a theory that

91:33

is then tested. It's with the huh that's

91:37

weird. For instance, either in in the

91:41

1930s with Fritz Wiki or in the 1970s

91:44

with Vera Rubin, she did a simple thing.

91:46

She said, "How fast are galaxies

91:48

rotating?" Cuz it's an easy thing to

91:50

calculate. You can literally calculate

91:52

that with high school physics and you

91:54

get an answer and then you measure it

91:56

and it's wrong. And so all that that's

91:58

the wow. Huh. I don't know what that is.

92:01

And that led to the hypothesis of of

92:04

dark matter. Now dark matter is not a

92:05

theory of everything, but it's a clue.

92:07

It's a powerful clue. We should pull tug

92:09

at that thread. Maybe our entire

92:12

theoretical edifice unravels. Or maybe

92:14

it doesn't. Maybe it's just a snag and

92:16

we can fix what we have now. I'm not

92:18

sure. So that's another option is to

92:20

simply look at many measurements that

92:23

are very precise and find ones where the

92:26

outcome and the prediction with

92:28

established theory disagree and that is

92:31

a clue. Before we leave the topic, we

92:35

got to talk about string theory. In your

92:37

view, is it basically dead? as I

92:41

understand uh one of the primary flaws

92:44

of string theory outside of the testable

92:47

experiments that we were talking about

92:49

is uh because it's relies on these

92:52

unobserved extra dimensions. There was a

92:55

hope that it uh it uniquely could

92:58

explain our universe, but it turns out

92:59

this quote landscape, there's an

93:02

enormous so-called landscape of

93:04

possibilities that it'll lead to. And so

93:07

it renders the theory basically

93:09

unpredictive because you can describe

93:12

all kinds of universes and therefore you

93:14

can just select

93:16

>> uh tune it to describe ours. I I agree

93:20

to a degree,

93:21

>> but I bring it back to my prior

93:25

objection. It is absolutely true that

93:29

super string theory um in its current

93:32

manifestation

93:34

aside from the extra dimensions which

93:36

are at some level small potatoes, it

93:40

allows for an extremely large number of

93:45

possible universes.

93:47

What if we were able to take those

93:52

predictions and somehow connect it to a

93:56

physical measurement? Then what we would

93:58

do is we'd lop off those alternatives.

94:01

We'd throw them away as saying, well,

94:03

you know, those are like an equation,

94:07

you know, x + 5. I can put in any number

94:09

I want in there. It doesn't matter. But

94:11

if x + 5 equals 9, then I've ruled out a

94:14

whole bunch of pe numbers except four.

94:17

And so this is a case of string theory

94:20

does allow for many predictions. But if

94:23

we could rule them out by connection to

94:25

a measurement, then it would no longer

94:27

do it. We would modify string theory and

94:30

we would retain the vibrating string

94:32

concept, which I really really like. I

94:34

mean, I really like it. But until we can

94:38

can validate this, it's it's I we can't.

94:42

So now you ask is it dead or not? In my

94:46

opinion, it is very difficult to kill

94:48

such a theory. I mean really truly kill

94:50

it cuz kill it means make a prediction

94:52

and it fails. But what can happen and

94:55

what is happening is people have been

94:57

working on it since the 70s. So we're

95:00

talking of order 50 years. people have

95:03

been working on it and it has not solved

95:07

the problem. And so I think what's

95:09

happening is people are looking at that

95:12

and saying

95:14

I do I want to spend my life working in

95:17

this direction with a very likely

95:19

possibility that 30 years from now we'll

95:22

be not much farther along than we are

95:23

now. It's a lot like back in the 1940s

95:27

when people started thinking about the

95:29

meaning of quantum mechanics. And I

95:32

wanted to do that when I was a kid in in

95:34

the 70s. But then when I went to grad

95:37

school, I realized that people very

95:38

smart people smarter than me had been

95:40

working on that for most of their lives

95:43

and made no definitive progress. And so

95:45

you have to decide as a scientist who

95:48

wants to answer questions. Do I really

95:50

want to take on a question that is so

95:52

hard that it will not be answered in my

95:54

lifetime? And I think that's what's

95:56

happening with a lot of super string

95:57

theory is people are saying it's really

95:59

neat. It might be right, but I don't

96:02

want to devote my life to something that

96:04

I might not see progress

96:07

forward in my lifetime.

96:08

>> What do you think about the alternate

96:10

theories? Do you think there's anything

96:12

interesting in those?

96:14

>> You know, many of those theories are

96:15

espoused by passionate people. They have

96:18

fans,

96:20

people love them, but they don't do what

96:23

science needs to do, which is make

96:25

predictions. Now, loop quantum gravity

96:27

is a little different. That one is

96:29

better developed. And that one is not a

96:32

theory of everything. So, we should be

96:33

make that clear. Loop quantum gravity is

96:35

not a theory of everything. It is simply

96:38

a theory of quantum gravity. Period. It

96:41

does not aspire to include all of the

96:44

known forces. It simply tries to take

96:47

gravity which is currently intrinsically

96:51

it treats space as smooth and

96:53

continuous. For those of your viewers

96:55

who are mathematically inclined in

96:58

Einstein's theory of general relativity,

97:01

gravity is infinitely divisible. There

97:05

is no smallest bit. And so essentially

97:08

the laws of calculus apply.

97:10

>> Mhm. However, it is possible that at a

97:13

small enough scale

97:16

um space is no longer divisible in the

97:19

same way that you can, you know, take a

97:21

cup of water out of a swimming pool and

97:23

then a/4 a cup and so forth, but

97:25

eventually once you've taken out a

97:26

single molecule of water, you can no

97:28

longer take out a smaller thing. So,

97:31

loop quantum gravity attempts to

97:34

quantize gravity. So, that's what it

97:36

does. And so this is unlike string

97:39

theory which attempts to bring gravity

97:43

in with the other forces. And in fact

97:45

the reason the fundamental the one

97:47

reason why string theory became so um

97:52

interesting to the theoretical community

97:55

is string theory was not

97:59

being developed as a theory of

98:00

everything. It was being developed as a

98:02

theory of the strong force. And it was

98:06

in competition with QCD, which is the

98:08

currently accepted theory of the strong

98:10

force. And it turned out the the two

98:13

groups, the string theory groups and the

98:16

um QCD groups competed for a while. And

98:19

string theory basically failed the race

98:22

and people paid attention to to quantum

98:25

chromodnamics, QCD. But then somebody

98:28

noticed in string theory that one of the

98:30

things it predicted was a zero mass spin

98:35

2 particle. And you can prove that any

98:38

zero mass spin 2 particle is the

98:40

graviton. And so if you see a theory

98:43

that has a zero mass spin 2 particle,

98:46

you are now have a candidate for

98:47

dragging gravity in. And then oh my

98:50

gosh, people got terribly excited

98:51

because now this theory which was um

98:54

working in the direction of the other

98:56

quantum forces brought in gravity and

98:58

now it was a candidate theory for

98:59

everything.

99:01

But um but that's not what loop quantum

99:03

gravity is. Loop quantum gravity is

99:05

simply trying to understand the nature

99:07

of space itself which is already a

99:09

fantastic thing. And you I talk to Ralli

99:12

every so often. I write about his theory

99:16

um and I point out some of the issues

99:18

with the theory but I'm usually about

99:20

like two months behind as he and his

99:23

colleagues are developing and so forth

99:25

because one of the things is originally

99:27

loop quantum gravity predicted that the

99:30

speed of light would not be universal.

99:33

The speed of light would depend on the

99:35

frequency of the light. So high

99:37

frequency would travel at one speed and

99:39

low frequency would travel at a

99:41

different speed. didn't it had to do

99:42

with the wavelength of light basically

99:44

interacting with the structure of space

99:47

if you know and so that was an issue

99:50

with loop quantum gravity and so if you

99:52

look at gammaray bursters which are you

99:54

know super explosions of astronomical

99:57

events that are a billion lightyears

99:59

away or more and they spit out light in

100:02

all wavelengths and if that loop quantum

100:04

gravity prediction were correct when you

100:07

saw a um one of these gammaray bursters

100:10

you would see the wavelength of one

100:12

light appearing on Earth at a different

100:14

time than another wavelength because of

100:16

the different speeds. And that wasn't

100:18

the case. They appear at the same time.

100:20

And so I went on to say, well, let's

100:24

pretty much kill loop quantum gravity

100:26

only to get a prickly note from Mr. or

100:29

Dr. Ralli saying, you know, we've

100:32

disproved that. We've changed the

100:33

theory. That's no longer true. And now

100:35

that that prediction, that old

100:37

prediction of loop quantum gravity is no

100:39

longer valid. And so that observation of

100:43

the the uniformity of the speed of light

100:46

no longer kills the new loot quantity.

100:49

It would have killed the old one, but it

100:51

didn't kill the new one.

100:51

>> By the way, that example of uh different

100:54

uh speeds of light uh based on

100:57

wavelength, that's a beautiful thing

100:59

that a theory that's a testable thing.

101:02

>> It is.

101:03

>> Right. So like those kinds of things and

101:05

if it in fact did explain a phenomena of

101:07

that sort that's a good sign for the

101:09

theory right

101:10

>> if it correctly predicted. There was

101:12

another brilliant observation recently.

101:15

I love it. Um the observation of uh

101:18

gravity waves.

101:19

>> Mhm.

101:20

>> And it was from two neutron stars

101:24

orbiting and coalescing. And so they

101:27

made gravitational waves. Fantastic. But

101:30

they also because they were not black

101:31

holes, they were neutron stars. They hit

101:34

and exploded. Gave off a tremendous

101:36

bright flash of light. And so

101:39

astronomers saw the flash.

101:41

>> Mhm.

101:42

>> Gravitational wave astronomers saw the

101:44

ripples of spaceime. It was 140 million

101:49

lighty years away, which means light

101:50

would have traveled 140 million years to

101:54

get here. And the two incidents, light

101:56

and gravity, both arrived within 1.7

101:59

seconds of one another. And that tells

102:01

you that gravity travels at the speed of

102:04

light. That was a brilliant, fantastic

102:07

measurement. Now we thought gravity

102:09

traveled at the speed of light, but now

102:10

we have a measurement. We proved it and

102:12

damn it, I am impressed. Our universe is

102:15

so fascinating. Speaking of which, since

102:17

we brought up antimatter,

102:20

we have to talk about it. Uh you've

102:23

talked about in several of your lectures

102:24

from different angles, including uh the

102:28

dark energy crisis and including uh

102:30

empty space and vacuum and so on. So

102:32

let's look at the empty space angle. So

102:35

uh you know it turns out the empty space

102:38

is not empty.

102:40

>> It's true which is kind of bizarre.

102:42

>> Can you can you speak about what do we

102:44

know about what makes up empty space?

102:47

>> That's a hard hard question because we

102:49

don't know what space is. But let's

102:51

start out

102:52

>> let's just start out with something

102:54

simple. We'll assume that space is not

102:58

quantized. Okay. Now it probably is. I

103:01

don't know. But you know, we got to

103:03

start with somewhere. So, let's start

103:04

out with sort of the space of calculus,

103:06

the space that you can divide forever.

103:09

The modern version of quantum mechanics

103:12

is called quantum field theory. And it

103:15

postulates that a space exists. Then it

103:19

postulates that within space there exist

103:23

fields for every known subatomic

103:26

particle. So there is a photon field,

103:28

there's an electron field, there's an up

103:30

quark field, there's a down quark field,

103:32

there's a all the fields

103:35

and those fields can vibrate and when

103:38

they vibrate those are the subatomic

103:41

particles. So an electron field

103:44

vibrating in a characteristic way is an

103:47

electron. Now, it's also possible for

103:50

the electron field to vibrate not in the

103:53

characteristic way, but in a way that's

103:56

still vibrating, but it's not an exact

103:58

electron. So, this is what we call

104:01

virtual particles. Now, virtual

104:04

particles, there are lots of ways to

104:06

talk about them, and the way I'm talking

104:08

about now is the most correct and the

104:12

most sophisticated way that we can talk

104:16

about them. I will talk about them

104:18

briefly in a in a simpler way to help

104:21

but right now that's the important thing

104:24

is that there are these fields specific

104:26

vibrations are the known particles

104:29

vibrations that are a little different

104:30

are

104:32

are these virtual particles they're

104:34

particles that don't truly exist and so

104:37

that is what

104:40

we think space is. There is all of these

104:44

these these fields. They are all

104:46

vibrating a little. If you insert the

104:49

right amount of energy, you can get it

104:50

to vibrate in the characteristic way and

104:53

make that subatomic particle. But even

104:55

when you don't there is um the particles

104:59

I mean the fields are there and they are

105:01

vibrating. So those vibrating vibrations

105:03

are what we called virtual particles.

105:05

Now your viewers may have heard of

105:07

virtual particles in other ways in which

105:09

case it says that space is just empty

105:12

and what happens is matter and

105:13

antimatter particles briefly appear for

105:16

a very short period of time before they

105:18

coalesce back again and disappear and

105:21

and reemerge back into the field. And so

105:26

that these are both correct. So what

105:28

happens is is that's what quantum field

105:30

theory says is it says that these

105:31

ripples are hearing or these particles

105:33

are appearing and disappearing. And so

105:36

that just sounds nuts. You look at empty

105:39

space, you're not seeing anything

105:41

happening, but they're happening fast

105:43

enough that they can't be seen. But they

105:45

do have consequences. And there are two

105:49

experimental measurements that I can

105:51

think of that validate that this thing

105:54

that sounds crazy is really happening.

105:57

And one is called the casemir effect. So

105:59

in the casemir effect you take two metal

106:03

plates that parallel plates and you put

106:05

them near one another very very close.

106:08

Now if this is the case if if these

106:12

virtual particles exist then in between

106:15

the plates these particles appearing and

106:17

disappearing and outside the plates the

106:19

particles are disappear appearing and

106:21

disappearing. However, because these

106:24

plates are close to one another, this

106:26

puts a constraint on the wavelength of

106:29

the particles that can occur between the

106:32

two plates because they the particles

106:34

cannot extend outside the plates. So the

106:38

short wavelength particles can exist

106:40

inside the between the plates, but the

106:42

longer ones cannot. However, outside the

106:46

plates there is no constraint. So short

106:48

wavelength and long wavelength particles

106:50

can exist there. And the net effect is

106:53

there are more particle virtual

106:55

particles outside and less particles

106:57

inside. And therefore you have a net

107:00

pressure which would then push those two

107:02

plates together. That is a prediction

107:04

we've been talking about. And guess

107:05

what? It happens. Those plates push

107:08

together. So that is a validation for

107:11

the existence of these particles in

107:13

empty space. Now there is another

107:15

measurement and this changes the

107:18

magnetic properties of particles like

107:20

the electron the muon and and so forth

107:23

and so this was uh discovered in 1948.

107:28

So if you take old school standard

107:31

quantum mechanics um you know the spin

107:33

of an electron you know its charge you

107:35

can calculate its magnetic moment and it

107:38

comes out to a number. If you do the

107:40

measurement, what you find is the

107:44

measurement disagrees with the quantum

107:47

mechanics, the 1930s quantum mechanical

107:49

prediction by 0.1%. And that was

107:52

measured in 1948.

107:54

And people went, huh? So this happened

107:58

at the Shelter Island conference in New

108:01

York. And on the way home, someone who

108:04

saw the this measurement thought about

108:07

it and they invented what we now call

108:10

quantum electronamics. So old quantum

108:13

mechanics quantizes matter. The second

108:15

quantization quantizes both matter and

108:19

the fields. In this case, quantized the

108:22

electric fields. And so in this

108:25

quantized um field, it predicts that

108:30

surrounding a bare say electron which is

108:33

spinning and has a has a charge, there

108:36

is this this bath of particles, virtual

108:40

particles appearing and disappearing all

108:41

around it. And the ensemble of all of

108:44

those particles appearing and

108:46

disappearing will alter the magnetic

108:49

properties that you can measure for the

108:51

subatomic particle. and it changes it by

108:54

0.1%. And we have measured this and we

108:57

have not measured this imprecisely. We

109:00

have measured the magnetic properties of

109:03

both the electron and the muon to 12

109:07

count them 12 significant figures. And

109:11

the theory and the data agree number for

109:14

number for 10 places. And then once you

109:18

get out to the very end where both the

109:20

theory and the data have some

109:23

imprecision, they then disagree. And so

109:25

maybe there's some interesting stuff

109:27

going on there. But 10 figures, it's

109:30

just staggering. So virtual particles

109:32

refer to

109:34

matter and antimatter particles coming

109:36

to life.

109:37

>> Correct.

109:38

>> Can we just talk about the the

109:39

antimatter part of that? So it's

109:41

starting with Paul Durac, one of the

109:43

most legendary examples of math leading

109:46

to physics. So the math suggesting that

109:50

so something like an antimatter should

109:53

exist and Paul Direct taking it

109:55

seriously and then eventually showing

109:58

that it does exist. So what evidence do

110:00

we have for antimatter? So antimatter

110:03

was predicted in 1928. Paul Durac was

110:06

trying to merge quantum mechanics and

110:08

relativity because the original

110:10

Schroinger equation did not was not

110:12

relativistic and in doing so he

110:14

basically the equations were complex but

110:17

in the end it came down to something

110:19

like equation squar= 1. You take the

110:22

square root of both sides you get

110:24

equation equals +1 or minus1. + one was

110:27

the electron minus one was something you

110:29

didn't know what it was. Um there was

110:31

some conversation for a while thought

110:33

maybe it might be the proton but that

110:35

didn't seem to work out and so he

110:36

insisted that his equations were right

110:38

and that there was an antimatter he

110:41

didn't call it an antimatter but a

110:44

positively charged uh sibling of the

110:48

electron what we now call the posetron

110:50

the antimatter electron so it was

110:52

predicted it was discovered in 1932 by

110:56

Carl Anderson and his student Seth

110:58

Nettoer they saw saw an antimatter

111:02

electron

111:04

and that was pretty cool. So that right

111:06

there they knew it was real. Antimatter

111:09

was predicted. It was observed. That's

111:10

that. In 1956 the antimatter proton was

111:14

created and that required a large

111:16

particle accelerator high enough energy

111:19

um to to to make it and that was done at

111:22

Berkeley and a year later the antimatter

111:24

neutron was discovered. So at this point

111:27

and now jumping ahead to now we can make

111:31

using uh energy by smashing particles

111:34

together we can make antimatter protons.

111:37

We can make antimatter electrons. We

111:40

have gone so far to make anti-atter

111:44

helium nuclei. So we have made two anti-

111:47

protons and two anti- neutrons. Combine

111:51

them together to make an anti-atter

111:53

helium nuclei. This has been done, been

111:55

observed. No question. At CERN, they

111:59

have gone so far as to make antimatter

112:01

hydrogen. They take a beam off one of

112:04

their lower energy accelerators. They

112:07

make antimatter protons. They collect

112:10

them. They slow them down. They cool

112:11

them to almost absolute zero. They take

112:15

um sodium 22, which makes antimatter

112:18

electrons. They slow them down. They

112:20

bring them together. They coalesce them

112:22

and they make literal antimatter

112:25

hydrogen atoms with an antimatter proton

112:29

surrounded by an antimatter electron and

112:31

they have done incredible measurements.

112:34

They have agitated the atoms and caused

112:38

it to emit light. They have looked at

112:39

the light that comes out of antimatter

112:42

atoms. And the question is is does the

112:44

light coming out of antimatter hydrogen

112:46

atoms have exactly the same spectral

112:49

characteristics as ordinary hydrogen

112:51

which we predict that it does

112:53

and the answer is it does. So the tests

112:56

have been staggering. We now know a

112:59

great deal about antimatter hydrogen.

113:01

recently recently like 2023 I believe it

113:04

was one of the experiments called alpha

113:06

at CERN made antimatter hydrogen put it

113:11

in a bottle and released it and watched

113:15

which way it would go did it fall up or

113:18

did it fall down because um while it

113:21

kind of makes sense maybe to think that

113:24

maybe antimatter falls up in the same

113:26

way that we have Kulum's law you've got

113:28

electric charges and they might attract

113:30

or repel Well, um, however, there was

113:34

lots of ample theoretical reasons to

113:36

believe that antimatter also would fall

113:39

down. So they did this fantastic

113:41

measurement and they first they put in

113:44

hydrogen and they calculated that some

113:46

if they did this something like 80% of

113:49

the hydrogen atoms would fall through

113:51

the bottom of the bottle and 20% would

113:54

go through the top just because um

113:57

gravity is very weak and the atoms will

114:00

escape wherever they do but there will

114:01

be a bias pulling hydrogen atoms down.

114:04

So they did the exactly the same thing

114:06

and what did they find? They find that

114:09

antimatter falls down. Now they do not

114:12

have a good enough measurement at this

114:15

time to say that the gravity that

114:18

antimatter experiences is 100% that of

114:23

matter. What they have measured is that

114:26

antimatter fell down with 75%

114:30

the strength of regular matter. But

114:33

there were big uncertainties. There was

114:36

plus or minus.13

114:38

due to the experiment which was good but

114:42

imperfect and plus or minus.16 due to

114:46

their um their theoretical model. So

114:48

it's like 75 plus or minus something

114:51

like 29 and that means there's a good

114:54

chance it's between.5 and one which

114:57

means it's consistent with one. So they

115:00

are improving their measurements. Well,

115:03

if I can, I would love to take a bit of

115:05

a tangent on that topic because I went

115:08

down a rabbit hole watching some of your

115:09

v videos on antimatter and I mean Firmmy

115:12

Lab was the hub for the production of

115:15

antimatter for quite a while.

115:17

>> It was

115:18

>> I saw that NASA said that the global

115:21

estimate for the current rate of

115:23

production of antimatter is 1 nanog per

115:26

year. Can you speak to how hard was it

115:29

to make antimatter? And also you did

115:32

mention in a video that you know if

115:34

matter and antimatter meet they produce

115:36

a lot of energy.

115:38

>> I think 20 grams of antimatter is

115:41

equivalent to a 1 megaton nuclear

115:44

warhead in terms of explosive energy.

115:47

Yeah. So all those questions together.

115:49

So how hard is it to produce antimatter?

115:52

>> It's freaking hard. Okay. All right. So

115:55

here's the deal. So at the time until

115:58

2011, Firmay Lab was the most powerful

116:02

anti-roton production facility on the

116:04

planet. Every 2.3 seconds, we would

116:08

smash 10^ the 13 protons into a target

116:13

and we would get out 10 to the 8th

116:16

anti-roton. So basically in order to get

116:19

a single anti-roton we needed to smash

116:22

100,000 protons into material. So every

116:27

2.3 seconds we would get of order 10 to

116:31

the 8th antiprotons. And what we would

116:34

do is we would collect them over the

116:36

course of 12 hours or so. And we would

116:39

get in the end we would have to collect

116:41

them and cool them down and so forth of

116:43

order 10 the 12th antirotons every 12 to

116:47

24 hours. So 10 the 12th sounds like a

116:51

lot. It really does. That is a trillion.

116:54

But you need to remember that a gram of

116:57

antimatter is 10^ the 23 antirotons. So

117:01

that means over the course of a day we

117:04

were able to create something like 100

117:09

billionth of a gram.

117:12

And so if we did that for a year then

117:16

that would be about a nanogram. So about

117:18

a nanogram a year give or take. That's

117:20

that's a reasonable estimate. So a nanog

117:25

one billionth of a gram. So that means

117:27

at that rate with that facility it would

117:30

take a billion years running with very

117:32

little downtime to make a single gram of

117:35

antimatter. If you combine 1 g of

117:38

antimatter and 1 g of matter together,

117:43

the energy release is equivalent to the

117:46

combined Hiroshima and Nagasaki

117:48

explosions. So that tells you if you

117:51

wanted a megat ton, you need about 25

117:54

times more. So you would have to run for

117:57

25 billion years to get a megat ton of

117:59

explosive power.

118:00

>> Let me uh lay it all out because I think

118:02

it's pretty interesting actually. This

118:04

is a NASA estimate of how much it cost

118:07

to produce antimatter. So looking at all

118:11

the the cost of the accelerator, all

118:14

everything combined together to do

118:17

enough for a one megaton antimatter bomb

118:19

of such a thing would be even possible

118:22

on the order of 25 grams like we

118:23

mentioned will cost about based on the

118:26

NASA estimate

118:28

>> uh 1.5 quadrillion.

118:30

By the way, uh NASA wasn't talking about

118:32

Obama. It's just me adding NASA was

118:35

talking about the estimate the cost of

118:38

62 to63 trillion per gram of

118:41

anti-hydrogen

118:43

actually is what they're referring to.

118:45

Uh so compared I was looking at

118:48

estimates the current best estimates how

118:50

much it takes to produce a 1 megaton

118:53

nuclear warhead

118:55

everything combined is about 10 to 50

118:57

million in the United States. So you're

119:00

talking about difference in terms of a

119:02

weapon with equal power $50 million

119:04

versus $1.5 quadrillion.

119:08

To me what's interesting weapons is just

119:11

one uh indication of this. One other

119:14

possibility and NASA also writes about

119:16

this is the use of antimatter and

119:18

propulsion systems.

119:19

>> Right?

119:20

>> Uh just like you can use uh nuclear

119:23

fision and maybe even nuclear fusion

119:25

down the line in propulsion systems. I

119:29

saw that one gram can help get us to

119:31

Alpha Centauri star system. If we can

119:34

get to 02 times the speed of light in 20

119:39

years. Uh meaning it would take us 20

119:41

years to get to Alpha Centauri. Is any

119:44

of this a possible future? The use of

119:46

antimatter for generation of energy

119:49

because we should mention that it's

119:50

extremely compact. It has the obvious

119:53

downsides that it's extremely costly to

119:55

produce. who don't know how to do that

119:57

kind of scale.

119:59

>> The upside is it's compact. It's

120:01

>> very powerful.

120:02

>> So the short answer is it is not a

120:05

physics problem. It's an engineering

120:06

problem. So I have people for that.

120:08

Okay. Um okay. But no no um the truth is

120:13

that antimatter

120:15

if you are able to uh assemble it and

120:18

store it. Sure. It would be able to take

120:20

that antimatter, heat up matter and

120:24

shoot it out the back of a rocket and it

120:26

would, you know, do what rockets do and

120:29

it would make us go quick and that would

120:31

be fine.

120:31

>> And we should mention the thing that you

120:33

just mentioned is is correct. One of the

120:35

hugest challenges is the containment.

120:37

>> Oh, because antimatter when it comes in

120:40

contact with matter

120:42

>> uh is a is a problem,

120:43

>> right? So if you were unable to uh to

120:46

contain your trip to Alpha Centuri for

120:49

even a millionth of a second, boom. And

120:52

that would not be good.

120:53

>> Yeah.

120:54

>> Um you know, it reminds me of the uh the

120:57

Star Trek where Scotty's saying,

120:58

"Captain, you know, the antimatter pods

121:00

are about look, we're losing containment

121:03

going to blow." And that's exactly what

121:04

would happen.

121:06

So the short answer is yes. antimatter

121:10

as in principle we could make and use as

121:13

a a source of energy, but there are

121:16

probably far less expensive sources of

121:18

energy. Um,

121:21

you know, it depends on what you need to

121:24

do. The Voyager probes are still

121:25

chugging along with plutonium now.

121:27

They're running out of energy at this

121:28

point, but we could, you know,

121:30

presumably do a somewhat better job if

121:32

we needed to. So, I I like the idea of

121:35

antimatter, you know, but the reality is

121:38

the danger, not the obvious danger of

121:40

weapons, but the danger of if you wanted

121:42

to be in a ship run by antimatter, if it

121:45

ever got loose, well, you you would

121:48

never know it. That would be that.

121:51

>> The reason I I find this kind of

121:53

inspiring

121:55

is antimatter in this space of physics

121:58

that has a lot of mysteries. There's a

122:01

lot of exploration to be done. And so

122:04

this kind of connection to energy means

122:06

that

122:08

uh if we have a bunch of breakthroughs

122:09

on the antimatter side that might lead

122:13

to a better propulsion system, better

122:15

energy generation systems

122:16

>> in principle.

122:17

>> There's some combination of engineering

122:19

here, but there's some combination of

122:21

understanding the fundamental physics.

122:22

>> I mean, we know how to do this.

122:25

You know, we we know you take energy,

122:28

you make antimatter. You have to contain

122:30

it, you have to store it, you have to do

122:32

all the hard things. But I I would be

122:35

shocked if there was some like new

122:38

addition to the theory that made

122:39

antimatter production easier.

122:42

>> Interesting. So, we know how to produce

122:44

antimatter with accelerators. You're

122:46

saying there's not

122:49

breakthroughs in physics that could lead

122:51

to different mechanisms for the

122:53

generation of antimatter.

122:54

>> You have to concentrate energy. That's

122:56

it. If there's another way to

122:58

concentrate energy, that would work too.

123:00

>> And our best knowledge of how to

123:02

concentrate energy is the accelerator.

123:04

>> And remember, we're talking

123:05

concentrating it into um volumes the

123:08

size of a proton. I mean, if you

123:10

concentrated to the size of your thumb,

123:12

well then, you know, it's really the

123:14

density that matters, the local density.

123:17

And so, when you smash two protons

123:19

together, all of that's occurring in a

123:20

tiny tiny volume. So, it's the local

123:22

density of energy that matters. If you

123:24

had a lot of energy in a thimble or

123:27

something,

123:29

>> it's probably not dense enough. You

123:32

know, it really has to be in close

123:33

proximity for that to happen. And then

123:36

when it does it, it's it's okay. So So

123:40

if there's another way, we know how to

123:42

do it to to make that that density thing

123:44

with with accelerators. If someone has a

123:47

bright idea on how to make highly dense

123:51

energy then yeah uh making antimatter is

123:54

a piece of cake but that's the crux

123:57

concentrated energy.

123:59

>> Yeah. How to do so in a cost efficient

124:02

manner not trillions of dollars.

124:05

>> Well yeah.

124:05

>> So one of the big mysteries with

124:07

antimatter is the bigger why.

124:11

Where is the antimatter that should kind

124:14

of be there? If the whole idea is that

124:17

anytime you generate matter, you

124:19

generate the same amount of antimatter.

124:21

And yet when we look out into the

124:22

observable universe, it seems like

124:24

there's not antimatter for the most part

124:26

there.

124:27

>> So what do we understand about this

124:29

mystery? What are the possible

124:30

explanations as to why? So there's this

124:33

thing called um

124:35

biogenesis and and as you say so

124:39

reiterating a little bit what you just

124:41

said um these are both Einstein things.

124:44

Einstein says that when you take energy

124:45

you make matter and antimatter in equal

124:47

quantities and Einstein says after the

124:49

big bang there was a lot of energy in

124:51

the universe which should have made

124:52

matter and antimatter. We only see

124:54

matter. Where' the antimatter go? And

124:56

the answer is we don't know.

124:59

However, there are some ideas and

125:02

there's a lot of thinking on it and um

125:04

in fact for me it's doing an experiment

125:06

right now with nutrinos trying to to

125:11

better understand what it was that made

125:15

the matter and antimatter not be the

125:19

same. Now, we do have a measurement of

125:21

how much different it should be. And

125:23

it's kind of neat. We can do this by

125:25

counting the number of protons in the

125:29

universe just looking at galaxies and so

125:31

forth. And then we can look at the

125:33

cosmic microwave background which is

125:35

sort of the aftermath of the big bang.

125:37

And we can count the number of photons

125:40

from the cosmic microwave background.

125:42

And with a little bit of math, what we

125:45

can do is we can then say that somehow

125:50

in the early universe, something made a

125:53

very very tiny asymmetry.

125:57

So that for every billion billion with a

126:00

B antimatter particles that existed in

126:04

the universe, there were a billion and

126:06

one matter particles. Mhm.

126:09

>> The billions canled, annihilated,

126:11

destroyed each other, and that extra one

126:14

that's left over is us.

126:16

>> Mhm.

126:17

>> And so what physics mechanism made that

126:23

ever so slight

126:25

asymmetry is not understood. There are

126:28

some thoughts. One thought is uh that

126:32

well, it's just how it was when the

126:34

universe was formed. There was an

126:36

asymmetry. it was not made by matter and

126:38

antimatter.

126:40

Another possibility is um there are

126:44

various numbers of theories all under

126:46

the word beriogenesis and berio um

126:49

coming from word beron which basically

126:51

means protons and genesis meaning the

126:53

creation of and we'd say that simply

126:55

because the protons are the heaviest

126:58

particles and so biogenesis is just the

127:01

creation of matter and there are just a

127:04

number of theories in quantum mechanics

127:06

that say that matter and antimatter can

127:09

can oscillate back and forth into one

127:11

another. And there is a slate slate

127:15

asymmetry in how that happens. And we

127:18

know that this is true to a degree. Um

127:21

we've measured it in the 1960s with a a

127:24

different form of matter. I mean, you

127:27

know, not protons, but a a a type of

127:31

ephemeral matter that only exists in

127:32

particle accelerators. And so we know

127:34

that there is a slight difference

127:36

between matter and antimatter, but it's

127:38

not enough. If it doesn't explain that,

127:40

we're not sure. So, at Firmeny Lab, we

127:42

have this idea which kind of turns

127:45

things on its head and it it's not

127:47

beriogenesis, it's leptogenesis. So,

127:49

lepttons are the electrons.

127:52

And because Fermy Lab is currently the

127:58

world's most powerful nutrino

128:00

accelerator and nutrinos are leptons,

128:03

there is this idea. Now leptogenesis is

128:05

incredibly complicated but the idea is

128:10

that it is possible. We we know that

128:12

nutrinos actually change their identity.

128:15

There are three different types of

128:16

nutrinos like uh I don't know cats and

128:19

jaguars and tigers. And if you have a

128:21

beam of just cats if you go along a

128:23

little while you find there's cats and

128:25

jaguars and then tigers and then they'll

128:27

be back to all cats again. And so this

128:29

oscillation thing is called nutrino

128:31

oscillation. We've known it's been true

128:32

since 1998.

128:34

And what we are studying is we're going

128:38

to make a beam of nutrinos and another

128:41

beam of antimatter nutrinos. And we're

128:43

going to study the oscillation behavior

128:46

of the two of them. And it is possible,

128:48

it is unlikely, but it is possible that

128:51

the two of them will oscillate at

128:53

slightly different rates.

128:54

>> Mhm. And if the nutrinos oscillate at

128:58

slightly different rates, then that

129:00

along with several other highly

129:03

improbable things can tie together and

129:06

might explain why there is more matter

129:09

in the universe. So if I was going to

129:12

bet the farm, I'll bet that they

129:14

oscillate at the same rate. But I don't

129:16

know, and you don't know till you do the

129:18

measurement. So that's what we're doing.

129:20

There are some other uh experiments

129:22

trying to measure it right now. So

129:23

there's a big race between the Firmeny

129:25

Lab group and another group in Japan to

129:28

see who gets there first and make this

129:30

measurement and we will find out. If it

129:33

turns out though that there is a

129:34

difference in this oscillation rate

129:36

between matter and antimatter, it will

129:38

be a huge clue in this very very

129:41

difficult puzzle. I wish I could tell

129:43

you I knew what the answer is, but but

129:46

literally nobody knows. I mean, and

129:49

that's the thing of being a research

129:50

scientist like me is if you're not

129:52

confused,

129:54

you're not doing your job.

129:55

>> So, there is this desperate or not

129:57

desperate, exciting search for this tiny

130:00

asymmetry.

130:01

>> Yes.

130:02

>> It's so so crazy to think that

130:05

everything we see around us

130:08

is a result of this tiny asymmetry that

130:10

there was this gigantic annihilation of

130:13

matter and antimatter in the early

130:15

universe.

130:16

>> And this is just some little

130:18

accident.

130:19

>> Yeah. Yeah. That's crazy.

130:21

>> It's a happy accident.

130:22

>> That is just I mean it's totally crazy.

130:25

>> This is one of the areas of physics

130:27

where there's a lot of mystery.

130:29

>> Mhm.

130:31

>> Okay. So, uh can we pull at that thread

130:35

a little further? Let's talk about our

130:37

intuition of what is uh dark energy as

130:40

it connects to empty space and

130:41

everything we've been talking about. Uh

130:44

what's what's the cleanest definition of

130:45

dark energy? So dark energy is either

130:50

energy of space or energy in space. The

130:55

most common statement is the energy of

130:58

space.

130:59

And it is essentially a repulsive form

131:03

of gravity.

131:05

And we believe this is real. And the

131:08

reason we believe this is real is from

131:11

observation. And this is one of those

131:12

things where we talked about a while ago

131:15

where I said that, you know, you can

131:16

think about things up this theoretical

131:18

stuff and try to come up with a

131:19

measurement or you can make measurements

131:21

and see where they disagree with

131:24

predictions and lead that in a

131:26

direction. So back in the late 1990s,

131:30

some astronomers were looking at the

131:31

expansion rate of the universe. So the

131:33

the big bang occurred, the universe is

131:35

expanding. The universe is full of

131:37

matter. Matter attracts. So the gravity

131:41

due to the matter of the universe should

131:43

slow the expansion of the universe. And

131:45

the only question was how much? There

131:48

were three possibilities. The

131:50

possibilities were there was so much

131:52

gravitational force that the expansion

131:55

of the universe would slow and be pulled

131:58

back together in a big crunch. Number

132:00

two was that the universe would continue

132:03

expanding, slowing down, but never

132:06

really stopping. And then the third

132:09

possibility was the exact critical case

132:11

where expansion would slow forever and

132:13

approach zero only at infinity never

132:16

quite stopping or reversing. So those

132:18

were the possibilities. Door number one,

132:20

two or three. So they did the

132:22

measurement and what did they found? It

132:24

was door number four. The universe was

132:27

not only expanding but the expansion was

132:29

speeding up. And the only way that could

132:30

happen given that gravity slows it down

132:32

is there was a repulsive force. And the

132:35

name we give to that repulsive force is

132:38

dark energy. This is something that

132:40

Einstein postulated early on in his um

132:45

his development of of general

132:48

relativity. But then because at the time

132:52

he knew that his theory predicted that

132:54

the universe would collapse. Um but he

132:56

believed the universe was eternal and

132:58

not unchanging. And so he needed

133:00

something to counterbalance the uh that

133:04

uh collapse. And so he invented dark

133:06

energy. He didn't call it that. Call it

133:08

the cosmological constant. Um but then a

133:11

few years later, Edwin Hubble discovered

133:13

that the universe was indeed expanding.

133:16

And so since the universe was no longer

133:18

static, Einstein said no need for

133:21

cosmological constant, took it back out.

133:23

>> Thought it was a dumb idea that he put

133:25

it in and was embarrassed. Um, however,

133:28

in 1998, it became clear that his

133:30

original idea that there should be some

133:31

sort of repulsive form of gravity was

133:34

real and it's put back in the theory.

133:38

>> And so that's what it is. We are pretty

133:40

confident at this point that the

133:41

expansion of the universe is speeding up

133:44

and the thing driving it is dark energy.

133:48

Now, what is dark energy? I don't know.

133:50

Um, as I said, the most common thought

133:54

is that it is the energy of space

133:56

itself.

133:58

But it is at least conceivable that

134:01

there is a field in space where space

134:03

exists

134:05

>> and that field is pushing space apart.

134:08

That's another conceivability that I'm

134:11

not sure that we have the the

134:13

instrumentation to distinguish, but

134:15

that's not what normally people think.

134:16

People think it is literally a property

134:18

of space.

134:19

>> But but there is the

134:23

what you call the worst prediction in

134:25

physics which is a

134:26

>> oh yeah that's another one

134:27

>> a nice little insight about the

134:30

complicated nature of dark energy. So

134:33

the observations

134:35

as you described say that empty space

134:37

has a tiny energy density that

134:39

accelerates expansion of the universe.

134:42

But

134:43

quantum field theory's prediction for

134:46

what vacuum energy should be when

134:49

coupled with gravity is much larger.

134:51

>> Mhm.

134:52

>> Uh so this is what makes for the uh

134:54

quote you have a video on this worst

134:56

prediction in physics.

134:58

>> Can you can you explain this crisis?

135:00

>> Well the there's a measurement and you

135:02

can measure how fast the universe is

135:04

expanding and from that you get a

135:05

measurement of dark energy. However, if

135:09

you then say, well, suppose the dark

135:12

energy is due to fields in space. So

135:17

that's quantum field theory. Hey, I know

135:19

a lot about quantum field theory.

135:21

>> And so we can take the quantum field

135:22

theory and we can calculate what the

135:25

density of energy is due to quantum

135:28

field theory. And basically what you do

135:32

is you take within a volume the uh all

135:36

of the wavelengths, the the longer

135:38

wavelength, the shorter wavelengths, the

135:40

shorter shorter and shorter. And you can

135:41

add them all up.

135:43

And each wavelength adds a certain

135:46

amount of energy. And if you add that

135:49

all up, then you get a number. And that

135:52

number is the rather embarrassing

135:56

10 to the 120 power times that's a one

136:02

with 120 zeros after it bigger than the

136:06

measurement of dark energy.

136:07

>> Yeah.

136:08

>> So you go yuck that is not fun at all.

136:13

And that is because the equation comes

136:16

to the highest energy or the smallest

136:20

wavelength particle that you can imagine

136:23

to the fourth power since anything to

136:25

the fourth power is a big deal. So

136:29

that's where you get that awful number.

136:31

Now if it turns out that there is some

136:34

new physics that's just about at the

136:36

energy scale we can measure using our

136:38

biggest particle accelerators. Remember

136:40

I told you that that was a factor the

136:44

maximum energy scale plank scale is 10

136:46

the 15 times bigger than what we can

136:49

measure now. So let's say that we don't

136:52

have to calculate up to the plank scale

136:55

because something happens something

136:57

changes at the energy that we know right

136:59

now. Well then that means we don't have

137:02

to integrate to plank scale. We

137:04

integrate to 10 the 15th less of the

137:06

plank scale. And this thing is to the

137:08

4th power. So 10^ the 15 to the 4th

137:10

power is 60. So now

137:14

even if we say you know Don he's

137:16

brilliant he's going to find something

137:18

at the LHC tomorrow is going to solve

137:19

all this problem. Now we've solved it.

137:22

It's much better. It's only different by

137:24

10 to the 60 power which is still pretty

137:27

bleeding big. So the short answer is

137:31

there is very clearly something going

137:33

on, something wrong, very badly wrong in

137:36

the quantum field theory. You know, we

137:39

have to have maybe there's another field

137:41

that balances out the energy that

137:43

cancels it down. And even that, you

137:46

know, that that's not so so outrageous.

137:49

You know, you could imagine that there's

137:51

another, you know, like we have matter

137:53

and antimatter. They balance pretty

137:54

well. Okay, maybe there's something

137:56

going on. And you could cancel that out.

137:58

That'd be perfect. But cancelelling

138:01

something to zero is easy cuz you know

138:04

plus one and minus one 0 + 2 - 2 0. But

138:07

we still have dark energy. Dark energy

138:09

is a little bit. So if it cancels, it

138:11

doesn't cancel exactly because it left

138:14

over that little bit of dark energy. So

138:17

that is its own curiosity. Perfect

138:20

cancellation pretty easy. Theorists do

138:22

that, you know, eight times before

138:24

breakfast. imperfect cancellation much

138:27

harder.

138:27

>> Just to elaborate that a little bit,

138:29

what do you think solving in quotes

138:31

solving dark energy would look like?

138:33

>> Well, you could what you would do is you

138:35

would hypothesize that there existed

138:36

some other field that had the the the

138:40

reverse uh effect of existing quantum

138:43

fields,

138:44

>> but not to zero.

138:45

>> But not to zero. So, but if you had it

138:46

to go to zero, you know, uh, sure, maybe

138:49

there's a field that that exists at

138:52

really high energies that we haven't

138:54

seen yet. I don't know, but it cancel

138:56

things out and we're cool.

138:58

>> How would we then demonstrate the

138:59

existence of that field?

139:00

>> Uh, well, that would depend on the

139:02

prediction.

139:03

>> How do you even come up with a new field

139:05

>> like all theorists do? Well, let's add

139:07

something to my equation and see what

139:09

happens. I mean, and and that's okay. I

139:11

mean, I I'm being glib about that, but

139:13

that is precisely what you do. You say

139:16

what change? We we have this thing that

139:18

works quite beautifully except it fails

139:20

here. What is the addition that we need

139:23

to make that changes very little in the

139:27

realm that we measured and yet fixes

139:30

this hard thing? And so you literally

139:32

just go da da da. Okay, what do I need

139:35

plus six or something and as long as it

139:39

makes no changes where it would hurt our

139:42

measurements and fixes the big thing,

139:44

then that is at least a candidate

139:46

theory. Now, that doesn't mean it's

139:48

right, but it at least gives you an

139:52

understanding

139:54

of what the right answer should look

139:58

like. M

139:59

>> and so that's the first step is what

140:00

should the real answer look like or what

140:02

is a possible real answer and then once

140:06

you kind of know that then other people

140:08

can look and say well let me think about

140:10

a theory that kind of has the required

140:13

properties

140:15

to do what we need it to do. So, it's

140:17

it's a multi-step process, but the first

140:19

step is how do we tame this problem

140:24

without coming up with really terrible

140:27

predictions that we've already ruled

140:29

out.

140:31

>> And and so that's what you do. And and

140:33

you know that that is literally a a

140:37

sensible, viable theoretical thing, you

140:39

know, cuz you have to explore cool

140:41

ideas. I mean one of the reasons dark

140:43

energy is super interesting is it kind

140:46

of gives us a mechanism by which we can

140:49

talk about the deep future of the

140:51

universe. I it's making we have

140:53

observations about the expansion of the

140:55

universe

140:57

but it's also giving us the mechanism of

141:00

that right so we can talk about

141:03

uh any weirdness any good model we have

141:06

that that captures some of the weirdness

141:08

of dark energy

141:09

>> might give us insights about how this

141:12

thing ends how the universe

141:14

>> about the deep future of the universe

141:15

right

141:16

>> absolutely as it stands right now if

141:18

dark energy is real and who knows you

141:20

know if it's a real exact exactly as

141:22

we've measured it. Then as the um

141:25

universe gets uh bigger and bigger, dark

141:29

energy becomes a bigger and bigger

141:32

component of the energy balance of the

141:34

universe and it takes over and it drives

141:36

the continued accelerated expansion of

141:39

the universe.

141:40

>> And if dark energy gets lower, you know,

141:43

for some reason that we don't

141:44

understand, maybe it changes over time,

141:46

gets smaller, that could change things.

141:48

If it gets bigger, it could change

141:49

things. That is one of the big open

141:51

questions whether it's constant over

141:52

time or not.

141:53

>> Right? And there has been a recent

141:55

measurement that suggests that dark

141:56

energy is getting smaller. Um however

141:59

that is a new measurement not confirmed

142:02

blah blah blah blah blah. Nobody should

142:04

believe it but it's a hint that maybe

142:06

it's changing which is kind of cool in

142:09

itself because the current bias until

142:12

recently is that dark energy is

142:15

constant. Now I want to be super careful

142:17

because it's misleading. People say dark

142:21

energy is constant. Dark energy is a

142:23

density.

142:24

>> Mhm.

142:25

>> Now that think about that. You have a

142:27

certain density. Let's start with that.

142:30

>> Then the universe expands. So energy is

142:34

volume times density. If the universe

142:36

gets bigger and the density is constant,

142:38

that means dark energy

142:40

>> is increasing. It's not just increasing

142:43

as a fraction and overwhelming ordinary

142:46

matter. But ordinary matter as the

142:49

universe expands its density decreases

142:52

because it's constant and the volume

142:54

gets bigger, the density drops. Dark

142:56

energy until recently is thought to be

143:00

constant density.

143:02

>> So that's what's implied when you say

143:03

constant. You say constant density which

143:05

means it's actually increasing because

143:06

space is increasing. The size of space

143:08

is increasing. Interesting. And so

143:10

that's a a weirdness. And that then ties

143:13

into the nature of space. Why does that

143:16

tie into the nature of space? Well,

143:18

because if dark energy is a field in

143:21

space, if you increase the volume, you

143:23

would think the energy density would

143:25

drop.

143:26

>> Mhm.

143:26

>> But if space is increasing and space is

143:29

quantized, and I don't know if it is,

143:31

then maybe what's happening is space

143:34

isn't stretching, but like little space

143:36

particles are appearing as the space You

143:39

know, there's like bubbles of space

143:41

appearing and each bubble contains a

143:43

certain amount of dark energy. And so

143:45

therefore, that would give you a sense

143:47

that dark energy is a property of space

143:50

rather than a field in space. But that's

143:54

all very handwavy, guessworky stuff. So

143:58

if you had bet all your money, is dark

144:00

energy like a real physical what does

144:05

that even mean thing that exists versus

144:08

is this just an a renaming of the

144:11

cosmological constant?

144:13

>> Unfortunately, I think it's both. I

144:14

mean,

144:16

>> well, I mean, it is it's describing a

144:19

reality, but it's also maybe telling us

144:22

something about space,

144:24

>> literally a property of space. Yeah,

144:26

it's I mean that's kind of what it looks

144:28

like given that it seems to be constant

144:31

density. That seems to me now this is

144:34

not something anybody should believe.

144:36

Please, nobody believe this. But it

144:39

seems to me that this is leaning towards

144:42

the idea that A it's a property of

144:47

space, B, space is quantized. C as space

144:51

is expanding little quantum of space are

144:54

appearing and D each one of those quanta

144:57

has a certain amount of energy

144:58

associated with it and that would kind

145:00

of explain the constant density. Now,

145:04

please, that's not anybody should,

145:06

nobody accepts that. This is just

145:08

nonsense.

145:09

>> But a lot of the stuff that you just

145:11

said is experimentally

145:13

probably experimentally testable. You

145:15

can probably construct them

145:17

>> experiment the bubbles of

145:19

>> Well, finding out the bubbles of space,

145:21

but those quanta conceivably are

145:23

planksiz bubbles.

145:25

>> Yeah, the quanta.

145:26

>> Well, they'd be quantum of space. I mean

145:28

the idea is you know you look at a sand

145:30

dune and it looks smooth and continuous

145:32

but you can see individual grains of

145:34

sand right and so what this is saying is

145:37

as this dune expands new grains of sand

145:40

are appearing and each one of them is a

145:42

quantum of space.

145:43

>> So what kind of experiments can we do in

145:46

the coming decades or centuries to

145:49

understand dark energy better? I mean

145:51

people have been talking about quantum

145:53

entanglement of gravity.

145:56

In standard quantum mechanics a particle

145:58

can be in two places at the same time.

146:00

All right? So now you have two

146:02

particles. So this particle can be in

146:04

two places in the same time. This

146:06

particle be be two places at the same

146:07

time. If you put them near one another,

146:09

well if they're close to each other,

146:11

there's a certain gravitational force.

146:12

If they're far apart, they're certain.

146:14

And if they one is close and one is far,

146:16

you have another one. You can calculate

146:18

the effects of gravity having to do with

146:23

quantum entangled particles being in two

146:25

places. And people are talking about

146:29

doing this and trying to see if in doing

146:34

such a measurement they might be able to

146:36

definitively determine whether gravity

146:40

is a quantum phenomena

146:42

or a continuous phenomena. And that is

146:47

potentially a measurement that could be

146:49

done

146:51

soonish because the technologies of

146:55

inherent in all of this recent work on

146:58

quantum mechanics is allowing people to

147:01

be able to make

147:04

instrumentation that might be precise

147:06

enough to do this measurement. Now this

147:09

will not tell us what quantum gravity

147:11

is. It will not tell us anything. But it

147:13

will tell us that gravity is quantized.

147:17

And just knowing that, well, for one

147:20

thing, it shuts out a whole realm of of

147:22

continuous gravity. And the theoretical

147:24

community will then turn its attention,

147:26

forget this stuff, and and think over

147:29

here. Now, that doesn't tell you that

147:30

space is quantized, but it tells you

147:32

that gravity is quantized if it bears

147:36

out. So, and if gravity is quantized,

147:39

then people will start thinking more

147:40

about space being quantized.

147:42

>> I have to ask because you mentioned dark

147:43

matter is perhaps even more mysterious

147:46

than dark energy.

147:47

>> Okay.

147:48

>> Can you can you can you uh build up the

147:51

intuition why it's more mysterious. What

147:52

is dark matter?

147:53

>> Oh gosh. What is dark matter? A, I don't

147:56

know. B, it's terribly fascinating.

147:59

>> Yeah.

147:59

>> All right. So, first thing and the most

148:01

important thing cuz I'm an

148:02

experimentalist by God. The first thing

148:05

is why do we believe there's dark

148:06

matter? And the reason is that

148:09

astronomical measurements do not agree

148:11

with predictions by Newtonian or

148:14

relativity theory. Galaxies spin too

148:17

fast. Clusters of galaxies move too

148:19

quickly. And the distortion of very

148:23

distant galaxies due to the

148:25

gravitational field of near galaxies

148:28

disagrees with the prediction from what

148:30

we see from the observed matter. So

148:33

there are three very distinct reasons

148:36

why we are predicting that that

148:39

something is wrong in our understanding

148:41

of either the laws of physics or the

148:46

matter budget of the universe. The

148:48

easiest one to talk about is the

148:50

spinning galaxies. Now this is what I'm

148:53

saying is not unique to spinning

148:55

galaxies just easiest to talk about. So,

148:58

galaxies are observed to spin more

149:01

quickly than they should if we add up

149:05

the gravity we see. By all rights,

149:07

galaxies spinning that fast should blow

149:08

themselves apart and they don't. So,

149:12

what can be the answer? Well, you have

149:15

the force required for a star to orbit

149:18

to move in a circle and you have the

149:20

force due to gravity and they're

149:22

connected by an equal sign and the

149:24

prediction is wrong. So either the force

149:27

due to gravity is wrong, the force

149:30

needed to move in a circle is wrong or

149:32

the equal sign is wrong. I mean this is

149:34

really simple. One of those things is

149:36

wrong.

149:38

So one possibility is simply that

149:41

Newton's law of gravity mass time the

149:43

mass over r 2 time a constant that's

149:46

just wrong. Another possibility is

149:48

Newton's F= ma that we are taught in

149:51

introductory physics is wrong. Both of

149:54

those are eminently possible over here.

149:56

Maybe we don't understand gravity

149:59

or maybe there's more mass than we can

150:03

see. So these, you know, I mean, it's

150:05

nice that that you can look at this

150:07

really simply and come up with a list,

150:09

you know, cookbook things we can test.

150:12

And um and so we've done that. We've

150:15

gone and said, what are the

150:17

possibilities? Well, the most obvious

150:19

possibility is that there is more mass

150:22

than we can see. there's black holes,

150:24

there's uh um hydrogen gas that we can't

150:27

see, whatever. There's something out

150:29

there. So, that was the first thing. So,

150:30

you go and you look and there's no

150:32

hydrogen gas because we can see that

150:34

with radio waves. That's not it. Um in

150:37

the '9s, we went looking for black

150:38

holes, rogue planets, things like that.

150:41

Those exist, but not enough of them.

150:43

That's not it. And so now we're left

150:47

with there's some sort of matter that we

150:49

can't see or we don't understand gravity

150:52

or we don't understand inertia.

150:54

Now I personally if you asked me this oh

150:58

I don't know 25 years ago I would have

151:01

said the most likely uh answer is that

151:05

we don't understand inertia or gravity.

151:09

You know I if 20 years ago 25 years ago

151:11

that's what I would have said. No

151:12

problem. However, there have been a

151:14

couple of observations

151:16

that um

151:19

that have caused me to change my

151:20

thinking and I think that dark matter is

151:23

more likely. One of them is called the

151:25

bullet cluster. So, the bullet cluster

151:27

there are two large clusters of

151:29

galaxies.

151:31

In these large clusters of galaxies,

151:33

well, any galaxy consists of a couple of

151:37

components. There are the galaxies

151:39

themselves. There is the hydrogen gas

151:41

that surrounds the galaxies. And maybe

151:43

there is dark matter.

151:46

And if dark matter is real or dark

151:49

matter is not real, you will get

151:51

different answers if those two galaxies

151:53

pass through one another. The galaxies

151:55

themselves should pass through one

151:56

another basically not interacting. But

151:58

the big thing is the gas clouds. So if

152:00

there's big clouds of gas, as the

152:02

galaxies pass through one another, the

152:04

clouds should interact and the gas cloud

152:06

should stop in the middle and be really

152:08

really hot. So then you would see if

152:10

there were no dark matter, you would see

152:13

a cluster of galaxies, a cluster of

152:15

galaxies, a big gas cloud in the middle.

152:18

And because the big gas cloud in the

152:21

middle is much more massive than the

152:24

galaxies themselves, you would expect to

152:26

see distortions that we call dark matter

152:28

distortions in the middle. If however,

152:31

dark matter is real, the galaxies pass

152:34

through one another. The cloud stops.

152:35

dark matter doesn't interact with the

152:37

clouds so it passes through. In that

152:39

case, you would expect to see the

152:40

distortions where the galaxies are

152:43

>> and that's what we see. So that is a

152:46

strong evidence in my mind. The bullet

152:48

cluster is strong evidence that dark

152:49

matter is a real thing. And there is

152:51

another example which is much more

152:53

recent. Dark bullet cluster was a while

152:54

ago called the dragonfly galaxies.

152:57

There's dragonfly 2 and dragonfly 4.

153:00

These are galaxies

153:02

that rotate exactly according to

153:06

Newton's laws.

153:08

And so the fact that they rotate exactly

153:11

according to Newton's laws

153:13

says that whatever is causing galaxies

153:16

to rotate too fast is not a property of

153:18

matter. But if you had a galaxy where

153:22

there was no dark matter, for whatever

153:24

reason, it got stripped off or

153:25

something, this is one of those lovely

153:27

ironies that the existence of a galaxy

153:30

with no dark matter is very strong

153:32

evidence that dark matter is real

153:34

because you can take the dark matter

153:35

out. So the DF2 and DF4 also suggests to

153:40

me that dark matter is real. So now

153:43

while it remains possible that um we

153:46

need to modify the laws of inertia or we

153:48

need to modify the laws of gravity those

153:50

are possible still in my opinion and now

153:53

this is Dawn's opinion but it's probably

153:55

the opinion of most of the the

153:58

scientific community.

154:00

Dark matter is likely a real thing. Now

154:04

that's great. I've taken you all the way

154:06

to dark matter. So now you're going to

154:07

ask me. You're going to say, "Don, what

154:09

is dark matter?" I'm going to I don't

154:10

know.

154:12

But I know what it isn't. Okay? I know

154:16

that it is not black holes. I know that

154:18

it is not rogue planets. I know that

154:21

we've done the measurements. We've

154:22

looked across nearly every mass range

154:24

for compact objects and ruled them out.

154:27

So if dark matter is real, it can't be

154:29

made of those.

154:31

So then you're left with the idea that

154:32

dark matter is a particle. And that's

154:34

what we've thought about. The name for

154:36

the the dark matter particle that we've

154:38

called for a long time is a wimp for a

154:40

weekly interacting massive particle. And

154:42

we have spent the last god 30 years

154:45

looking for them in the various ways.

154:47

There are three ways that we might see

154:49

dark matter. The direct way which says

154:52

that dark matter exists literally

154:54

everywhere in this room in our

154:56

laboratory and the dark matter is

154:58

passing through the earth like a wind

155:00

and we put up detectors trying to see

155:02

those. We have done that and we've seen

155:05

nothing.

155:06

>> So we should say we have done that for

155:07

nutrinos.

155:08

>> We've done that for many different types

155:10

of dark matter. We just simply put

155:12

detectors in labs deep underground and

155:16

we can see nutrinos in them. It's true.

155:18

But dark matter would have especially

155:20

heavy dark matter what these these wimps

155:23

um they have a different signature and

155:25

we've seen no evidence of dark matter

155:27

interaction in these detectors. So

155:29

nutrinos are also weakly interacting and

155:32

also have mass they are

155:34

>> but not enough ma. So wimps are

155:37

>> heavy on the um

155:38

>> right? Nutrinos are indeed wimps of a

155:41

sort. Now we have to be careful what we

155:43

mean by wimps. They are weakly

155:44

interacting massive particles but we can

155:47

calculate and there's just not enough

155:48

mass in them. It's not it.

155:50

>> Got it. So we need another form and we

155:54

have seen zero evidence of this wind of

155:56

dark matter through the uh the earth.

156:00

Another possibility is you look where

156:01

you think dark matter might be

156:04

concentrated at the center of galaxies

156:06

and if dark matter exists and there's

156:09

antimatter dark matter maybe they

156:11

annihilate and make photons. And so we

156:13

look for gamma rays and various other

156:15

signatures of annihilating dark matter.

156:18

And there are always constantly

156:22

announcements of oh we saw it oh we

156:24

didn't oh you know the problem is that

156:26

way of looking for dark matter is hard

156:28

because there are other ways of making

156:31

for instance gamma rays like neutron

156:33

stars and stuff and you really need to

156:35

understand the details of galaxies

156:37

really really well to believe that and

156:40

then the final option is what I do where

156:42

we smash particles together at high ma

156:45

or high energy we try to make dark

156:46

matter particles If you make dark matter

156:49

particles because they don't interact

156:51

except via gravity, they escape with

156:53

your detector. So what you're seeing,

156:55

what you hope to see is an event where

156:57

you collide particles, a dark matter

156:59

particle escapes and you don't see it,

157:01

but the recoil you see on the other side

157:04

because momentum is conserved. So you

157:05

see a blob of energy on this side,

157:07

nothing on the other side. Maybe that's

157:09

dark matter. And that also happens with

157:12

nutrinos. So you need to understand

157:14

everything about nutrinos and calculate

157:15

how many of those you see and then hope

157:17

you see more and then that might be dark

157:19

matter again that hasn't worked. So

157:22

we've ruled out some dark matter

157:24

particles but the problem is the range

157:26

of space of possible mass if dark matter

157:30

is of a particulate form. The range of

157:34

viable dark matter ranges from something

157:38

like the mass of an asteroid to far

157:40

lighter than an electron and everywhere

157:43

in between.

157:45

And we have looked, we've ruled out some

157:46

little spots in that phase space, but

157:48

that's a big range.

157:50

>> Is it really possible to miss a particle

157:52

the size of an asteroid? the

157:54

astronomical searches were not sensitive

157:56

to that level of of dark matter, but you

158:01

know, then you would expect that there

158:02

would be some of those in the solar

158:05

system. And if they're what we think

158:07

like asteroids or something, then we'd

158:09

heat them up and we'd eventually see

158:11

them. But if they're really like truly

158:13

dark matter doesn't interact with

158:16

matter, which means they wouldn't absorb

158:18

energy from the sun, so they'd be really

158:20

dark. I don't know, maybe they're out

158:21

there. But the only way we have we

158:24

searched for them was um a thing called

158:27

microl lensing. So if a massive object

158:31

you have a distant star and a massive

158:34

object pass between that star and your

158:37

eye that star will momentarily brighten.

158:41

>> Mhm. And so you just look for these what

158:44

they call microl lensing events and you

158:46

count them and you see some and we did

158:49

see some you know black holes pass in

158:51

front of stars and and we've seen them

158:53

but we just haven't seen enough. And for

158:56

very low mass particles like asteroids

159:00

they um they just wouldn't make enough

159:03

brightening effect to see. So there's

159:06

like a minimum sensitivity of

159:07

brightening and that about a third the

159:10

mass of a moon. Our moon is about the

159:14

sensitivity that we had. So you know

159:17

that nobody I think really thought that

159:19

these low mass guys were likely. What

159:21

they thought was more likely they were

159:23

just unseen black holes which I thought

159:25

you know I think is completely

159:26

reasonable. Then when that got ruled out

159:28

I thought okay modified gravity or uh

159:32

>> or inertia. Well, now that you know,

159:34

bullet cluster and dragonfly seems to

159:36

ruled that out. So, I'm stuck in my head

159:38

with dark matter seems to be real and it

159:42

we don't know what it is

159:43

>> and it makes up a giant percentage of

159:45

matter in the universe.

159:46

>> It is five times more prevalent than

159:48

ordinary matter.

159:50

>> This is incredible. It is so fascinating

159:52

and that's why it's cool. So, if someone

159:54

out there is, you know, a young person

159:57

wants to get into this, understanding

159:59

dark matter is a big deal. I mean, it's

160:01

five times more prevalent. The problem

160:03

is is, as I told you, if the mass is

160:06

ranging from an asteroid to far lighter

160:08

than an electron, if you get on an

160:10

experiment that looks at one little

160:12

range of mass, maybe you weren't the

160:15

lucky guy that measured the right place,

160:17

you know, and that's one of the reasons

160:20

why, as fascinating as I think it is,

160:22

I'm not doing dark matter experiments,

160:24

because,

160:25

you know, if you make an experiment that

160:28

searches one mass range, it'll be blind

160:30

to another mass range. So what you need

160:32

is you need many groups doing all sorts

160:35

of radically different experiments

160:37

exploring all sorts of parameter space.

160:41

And with all that said, until you see

160:44

it, there still is the possibility that

160:46

maybe we don't understand gravity or

160:48

inertia, right? You know, you can't rule

160:50

that out.

160:51

>> If there is dark matter out there,

160:53

you're hoping it's actually somehow

160:55

detectable.

160:56

>> I mean, I don't know what it is. I think

160:58

it's cool. It's very, very fascinating.

161:00

That is one thing I really do hope in my

161:03

lifetime is is understood because I' I'd

161:06

like to know the answer to that.

161:07

>> And that that's the thing that you could

161:09

there legitimately you can see a

161:11

discovery of.

161:12

>> You got to get lucky though. I mean you

161:13

got to look in the right place whatever

161:15

it is.

161:16

>> Just imagine or you have to come up with

161:18

that really cool theoretical idea that

161:20

everybody's overlooked which is another

161:22

possibility. And there are people who

161:24

are really really religiously hating

161:27

dark matter largely because we've looked

161:30

so hard for so many years and the

161:32

experiments in today's world are a

161:34

million times more sensitive than when I

161:36

was a a starting student and they still

161:39

haven't seen anything and that's why

161:41

people really hate dark matter. I mean

161:43

some of them because they think we

161:45

should have seen it by now but

161:46

>> you know uh I don't know. I mean, I'm a

161:49

sucker for direct observation. Not

161:51

indirect is obviously also really great,

161:53

but direct. Just imagine pointing your

161:56

telescope in a certain direction and

161:58

because of some artifact of cosmology

162:01

being able to directly detect a giant

162:04

amount of of a thing that you could say

162:06

is dark matter.

162:07

>> Yeah. You would see it orbit things

162:09

orbit it or it would eclipse things in

162:12

front of it or

162:13

>> Yeah. like in an obvious way cuz uh some

162:15

of the stuff you mentioned with DF2 and

162:17

DF4 those are like brilliant indirect

162:21

um deductions that there should be

162:25

something like dark matter but some

162:27

obvious yeah blocking oluding this kind

162:31

of thing we did that in the 90s with

162:33

experiments called macho ogle and some

162:36

others they looked for a black hole that

162:39

you just can't see you know black hole

162:41

you can't see it's perfect it's a

162:42

perfect candidate for dark matter. And

162:45

if there's enough of them out there,

162:47

remember there's five times the number

162:49

of stars, which means there's a whole

162:51

lot of freaking black holes out there.

162:53

We should have seen them and we didn't.

162:57

>> What a grand mystery. We covered so many

162:59

of them. I could talk to you for a

163:01

thousand more hours. Don, let me if I

163:03

can uh ask you about a little bit more

163:06

of a on the personal side. Um, you have

163:10

a really inspiring life story. Your

163:13

folks didn't uh go to college. Can you

163:16

just tell me about your childhood and

163:18

where you found the love for physics and

163:21

science and maybe how you found your

163:24

journey to to to become a physicist

163:27

given the the context of where you came

163:30

from?

163:31

Well, uh, you know, I grew up a poor kid

163:35

in the Boondocks. Great parents, but not

163:39

ones that could guide me terribly

163:41

academically, but very, uh, very

163:43

nurturing. You know, my mom would laugh

163:45

that she could stop helping me math

163:47

after like sixth or seventh grade, you

163:49

know. Um, but they were supportive. And

163:53

there were a couple of things that

163:56

couple three things I think that folded

163:58

into it. One is I was a voracious reader

164:00

as a kid. I loved science fiction. I

164:03

would read a book a day. It drove my

164:04

mother nuts cuz she would try to be

164:06

nice. She'd buy me a book and I'd say

164:08

thank you and the next day it'd be done.

164:09

You know, it just drove her completely

164:11

nuts. But anyways, but science fiction

164:13

is good for

164:16

fostering imagination. And so that's

164:19

precisely what it did. In addition, um,

164:22

and this is where the more serious

164:24

science came along, there were lovely

164:30

science communicators that were popular

164:32

in the 1970s. Isaac Azimoff, Carl Sean,

164:36

guy by the name of George Gamma. They

164:38

wrote books about science aimed at a lay

164:41

person. I was a kid. I surely couldn't

164:43

read a a textbook and understand it, but

164:47

I could read and and you know, get a a

164:50

hint of what science was. And on top of

164:53

that, you know, I was, as most

164:56

scientist, people who became scientists,

164:58

irrepressibly curious about everything.

165:02

Um, and I had sort of a quasi

165:04

philosophical

165:06

mind. I mean, I was interested in things

165:08

that questions that have in the past

165:10

been theological and then philosophical

165:12

and now are more scientific. Questions

165:14

about how did the universe come into

165:17

existence? Um, why is the universe the

165:20

way it is? Why are the laws of the

165:22

universe what we see them to be? How

165:24

will the universe was it created? How

165:26

will it be destroyed? These are, you

165:28

know, big questions that have bothered

165:30

humanity for, well, thousands of years.

165:33

And so, you know, I did you you said I

165:35

had uh um you know, philosophy and

165:38

religion minors in college, and I did

165:40

because I was curious about that. Um I

165:42

was hoping that learning that history

165:46

might help me understand these

165:48

questions. Um and it was in college

165:50

where I came to realize that the answers

165:52

that I were searching for were not to be

165:55

found in those directions, but I still

165:57

learned about how those questions have

165:59

been asked in the past.

166:01

Um, and so I became a a scientist and

166:05

the only question was was I going to be

166:07

uh a cosmologist/astrophysicist

166:10

or a particle physicist. And when I had

166:13

to make that decision, it was the

166:15

mid80s. And at the time, there were a

166:19

lot fewer cosmology measurements. There

166:22

was an awful lot of thinking about the

166:24

universe and not enough measuring.

166:27

Whereas with uh particle physics, by

166:30

God, you could do experiments. And so

166:32

the what attracted me was the ability to

166:35

actually get an answer and not just mull

166:37

over what an answer might be. And so I

166:40

became a particle physicist. Um it was

166:44

difficult without having you know uh

166:48

family mentors or anything like that but

166:50

but you know I managed and that actually

166:54

is why well I'm here and why I have

166:56

spent a fair bit of my time writing

167:00

books and so forth because I figure that

167:02

there has to be some other kid out there

167:05

in Iowa, Kansas, Montana somewhere out

167:08

in some little town without a lot of

167:11

access to the kinds of thing that

167:14

people, you know, who have highly

167:17

educated parents do. And I'm hoping

167:20

that, you know, some of them will have

167:22

read some of the things I've written and

167:24

will find their own path forward because

167:27

I found it very rewarding over the

167:29

years. And um, you know, I've been doing

167:32

this long enough that I'm I'm sure this

167:34

is true. I've had kids come up to me at

167:37

the lab and say, "Hey, I'm a summer

167:39

intern because I saw your video or read

167:41

your book or you know, whatever." Um, so

167:43

I know that at least I've made a small

167:46

impact. I mean, always would like to do

167:48

more and, you know, I appreciate the uh

167:51

opportunity that your uh audience

167:55

affords me um cuz I I think it's

167:57

important to talk about these things.

167:58

These are really cool, fascinating

168:01

questions. They are unanswered and they

168:04

are just waiting for youngsters to come

168:07

and spend some time thinking about them

168:09

because one of your viewers might be one

168:12

of the people who answer these questions

168:14

that have stymied very smart people for

168:17

decades.

168:18

>> And we should also say that you're a

168:20

legit scientist. So we we'll mention

168:23

Sean Carol who's a legit scientist,

168:26

legit physicist, but is also a good

168:29

science communicator. Anyway, I did want

168:31

to mention, I don't know if this is

168:33

true, but I I kind of heard you talk

168:35

about this, that when you first showed

168:37

up to Firmeny Lab, you were like working

168:39

crazy hours, working extremely hard,

168:41

>> 8:00 a.m. to midnight.

168:43

>> I did.

168:44

>> Uh, first of all, I love that.

168:47

>> Uh, can you speak to what drove you and

168:50

maybe the value of hard work in those

168:54

context in your in the early career when

168:57

you discover a thing you're passionate

168:59

about?

169:00

Well, yeah. I mean, obviously being

169:03

smart, you know, if you're Einstein,

169:05

then maybe you can slack, I guess.

169:06

Although even he didn't do that, but I'm

169:09

not Einstein. But the fact is when I was

169:11

young and I was unencumbered, no no

169:14

family, no kids or something. I couldn't

169:17

imagine anything I wanted to do more. I

169:19

mean, some people they want to go out to

169:21

the club, they want to, I don't know,

169:22

play soccer or something, but I wanted

169:24

to make measurements and I wanted to

169:27

understand and and and learn, and that

169:29

was fantastic. And so, as a graduate

169:32

student, and this isn't for everybody,

169:33

but I worked outrageously. I would from

169:37

Monday through Saturday, I would be at

169:39

the lab voluntarily because I wanted to

169:41

be from 8:00 a.m. to midnight. And on

169:45

Sunday, I would work from 8 until about

169:47

5:00. And that's because from 5 to

169:49

midnight I had to wash clothes and buy

169:51

groceries and things like that. And I

169:54

loved it, you know, uh, and I still love

169:57

it. I can't do that anymore. Um, but but

170:02

that's simply because I have other

170:03

obligations, but had I been rich, I

170:08

would have done the same thing. You

170:10

know, it's it's something I truly truly

170:12

loved. And the I mean there is

170:17

absolutely nothing more fascinating to

170:19

me than having a hard problem and

170:22

figuring it out. And that you know that

170:24

work ethic. Well, there's a couple of

170:25

things that separate

170:28

smart people from no kidding scientists

170:30

cuz all scientists are smart. But the

170:32

thing that that separates that that that

170:35

many scientists have is a a drive and a

170:40

real grit. the um

170:44

for me and for so many scientists that I

170:46

know

170:49

trying to measure something and having

170:50

it not work just kind of ticks me off

170:53

and I am not going to let the universe

170:55

in my lab or whatever

170:58

beat me. And you know some people they

171:01

you know if the thing breaks it's like

171:02

oh man that didn't work and a lot of

171:04

people well I'm going to go home I'm fed

171:07

up. No, it would just kind of make me

171:09

mad and I'd put more effort into it. And

171:12

you know, not every I mean, okay, I was

171:14

crazy. I worked long hours, but but I

171:16

think the people who are really good at

171:18

this will do maybe not that much. You

171:21

know, some people have to have a better

171:22

life than that, but but a lot because it

171:25

it's just you can't imagine not knowing

171:28

the answer. Mhm.

171:30

>> And that if when when you see that as an

171:33

older guy, you don't maybe not to that

171:35

degree, but when you see that kind of

171:36

drive, that that that

171:40

intensity of trying to get the answers,

171:43

you know that person's a winner. And and

171:45

so if you know some student out there,

171:48

if it doesn't, you know, bring you joy,

171:51

as uh what's her name? The Japanese girl

171:54

says, if it doesn't bring you joy, then

171:55

it might not be for you. And then you

171:57

could be a person who reads about it and

171:59

you know is involved. But if you want to

172:01

be a real scientist, it it has to be

172:04

just part of what you are here.

172:06

>> And by the way,

172:08

it is a hard life, but it is also a very

172:11

fulfilling one. So working hard towards

172:14

the thing you love is a really

172:16

fulfilling way to to be. I think that's

172:19

true for an artist or something, you

172:21

know, anybody, a musician, you know,

172:23

musician, they just keep practicing

172:26

because it is who they are.

172:28

>> Well, I'm glad there's people like you

172:30

at a place I admire like Fermy Lab, uh,

172:35

one of the many places in the United

172:36

States, in the world that, uh, is

172:39

carrying the beacon of great science and

172:42

great engineering

172:43

forward. Uh, Don, thank you so much for

172:47

everything you do, for all the teaching

172:50

you do uh, online, for all the

172:53

incredible physics work that you do at

172:55

Firmay Lab, and uh, thank you so much

172:58

for talking today.

172:59

>> Thank you for having me.

173:01

>> Thanks for listening to this

173:02

conversation with Don Lincoln. To

173:04

support this podcast, please check out

173:05

our sponsors in the description where

173:07

you can also find links to contact me,

173:10

ask questions, give feedback, and so on.

173:13

And now, let me leave you with some

173:14

words from Marie Kuri, a twotime Nobel

173:18

Prize winner. First in physics, second

173:21

in chemistry. Nothing in life is to be

173:24

feared. It is only to be understood.

173:28

Thank you for listening. I hope to see

173:30

you next time.

Interactive Summary

Don Lincoln, a particle physicist at Fermilab, provides an insightful overview of the history of unification in physics, from Newton's celestial and terrestrial gravity to modern efforts like the Standard Model and the search for a Theory of Everything. He explains complex concepts such as space-time, the Higgs field, dark energy, and antimatter, while emphasizing the importance of both theoretical brilliance and experimental verification. Lincoln also shares his personal journey and emphasizes the passion and hard work required to push the frontiers of science.

Suggested questions

3 ready-made prompts