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You've (Likely) Been Playing The Game of Life Wrong

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You've (Likely) Been Playing The Game of Life Wrong

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1136 segments

0:00

- Some things are not normal.

0:03

By that I mean if you go out in the world

0:05

and start measuring things like human height, IQ,

0:08

or the size of apples on a tree.

0:10

You will find that for each of these things,

0:12

most of the data clusters around some average value.

0:16

This is so common that we call it the normal distribution,

0:20

but some things in life are not like this.

0:24

- Nature shows power laws all over the place.

0:27

That seems weird.

0:28

Like, is nature tuning itself to criticality?

0:30

- If you make a crude measure of how big is the world war

0:33

by how many people it kills,

0:34

you find that it follows a power law.

0:37

The outcome will vary in size over 10 million, 100 million.

0:42

- It's much more likelihood of really big events

0:45

than you would expect from a normal distribution,

0:47

and they will totally skew the average.

0:49

- The system you're looking at doesn't have

0:52

any inherent physical scale.

0:54

It's really hard to know what's gonna happen next.

0:56

- The more you measure, the bigger the average is,

0:59

which is really weird, it sounds impossible.

1:01

- It's very important to try to understand

1:04

which game you're playing

1:06

and what are the payoffs going to be in the long run.

1:10

- In the late 1800s, Italian engineer Vilfredo Pareto

1:13

stumbled upon something no one had seen before.

1:17

See, he suspected there might be a hidden pattern

1:19

in how much money people make.

1:21

So he gathered income tax records

1:23

from Italy, England, France, and other European countries,

1:26

and for each country he plotted the distribution of income.

1:31

Each country he looked at, he saw the same pattern,

1:34

a pattern which still holds in most countries to this day,

1:38

and it's not a normal distribution.

1:41

If you think about a normal distribution like height,

1:43

there's a clearly defined average

1:45

and extreme outliers basically never happen.

1:48

I mean, you are never going to find someone

1:50

who is, say, five times the average height,

1:53

that would be physically impossible,

1:55

but Pareto's income distributions were different.

1:57

Take this curve for England,

1:59

it shows the number of people

2:00

who earn more than a certain income.

2:03

The curve starts off declining steeply,

2:05

most people earn relatively little,

2:07

but then it falls away gradually,

2:09

much more slowly than a normal distribution would,

2:12

and it spans several orders of magnitude.

2:15

There were people who earned 5 times, 10 times,

2:18

even 100 times more than others.

2:21

That kind of spread just wouldn't happen

2:22

if income were normally distributed.

2:25

Now to shrink this huge spread of data,

2:28

Pareto calculated the logarithms of all the values

2:30

and plotted those instead.

2:32

In other words, he used a log-log plot,

2:35

and when he did that,

2:36

the broad curve transformed into a straight line.

2:39

The gradient was around negative 1.5.

2:42

That means each time you double the income,

2:45

say, from 200 pounds to 400 pounds,

2:47

the number of people earning at least that amount

2:50

drops off by a factor of two to the power of 1.5,

2:53

which is around 2.8.

2:55

And this pattern holds for every doubling of income.

2:58

So Pareto could describe the distribution of incomes

3:01

with one simple equation.

3:02

The number of people who earn an income greater than

3:05

or equal to X is proportional to one over X

3:08

to the power of 1.5.

3:10

Now, that's what Pareto saw for England,

3:13

but he performed the same analysis on data from Italy,

3:16

France, Prussia, and a bunch of other countries,

3:18

and he saw the same thing again and again.

3:22

Each time the data transformed into a straight line

3:26

and the gradients were remarkably similar.

3:28

That meant Pareto could describe the income distribution

3:31

in each country with the same equation,

3:34

one over the income to some power,

3:37

where that power is just the absolute gradient

3:39

of the logarithmic graph.

3:42

This type of relationship is called a power law.

3:45

When you move from the world of normal distributions

3:48

to the world of power laws,

3:49

things change dramatically.

3:51

So to illustrate this,

3:52

let's take a trip to the casino

3:54

to play three different games.

3:57

At table number one, you get 100 tosses of a coin.

4:01

Each time you flip and it lands on heads, you win $1.

4:05

So the question is,

4:06

how much would you be prepared to pay to play this game?

4:09

Well, we need to work out

4:11

how much you'd expect to win in this game

4:12

and then pay less than that expected value.

4:15

So the probability of throwing a head is 1/2.

4:18

Multiply that by $1 and multiply that by 100 tosses,

4:22

that gives you an expected payout of $50.

4:25

So you should be willing to pay

4:26

anything less than $50 to play this game.

4:29

Sure, you might not win every time,

4:31

but if you play the game hundreds of times,

4:33

the small variations either side of the average

4:35

will cancel out and you can expect to turn a profit.

4:39

One of the first people to study this kind of problem

4:41

was Abraham de Moivre in the early 1700s.

4:44

He showed that if you plot the probability of each outcome,

4:46

you get a bell-shaped curve,

4:48

which was later coined the normal distribution.

4:51

- Normal distributions,

4:52

the traditional explanation

4:54

is that when there are a lot of effects that are random

4:56

that are adding up,

4:58

that's when you expect normals.

5:00

So like how tall I am depends on a lot of random things,

5:03

about my nutrition, about my parents' genetics,

5:06

all kinds of things,

5:07

but if these random effects are additive,

5:10

that is what tends to lead to normals.

5:14

- At table number two, there's a slightly different game.

5:17

You still get 100 tosses of the coin,

5:20

but this time,

5:21

instead of potentially winning a dollar on each flip,

5:23

your winnings are multiplied by some factor.

5:26

So you start out with $1,

5:29

and then every time you toss a head,

5:31

you multiply your winnings by 1.1.

5:34

If instead the coin lands on tails,

5:36

you multiply your winnings by 0.9.

5:38

And after 100 tosses,

5:40

you take home the total,

5:41

that is the dollar you started with

5:43

times the string of 1.1s and 0.9s.

5:46

So, how much should you pay to play this game?

5:49

Well, on each flip,

5:51

your payout can either grow or shrink,

5:53

and each is equally likely each time you toss the coin,

5:57

so the expected factor each turn

5:59

is just 1.1 plus 0.9 divided by two, which is one.

6:02

So if you start out with $1,

6:05

then your expected payout is just $1.

6:08

That means you should be willing to pay

6:09

anything less than a dollar to play this game, right?

6:13

Well, if you look at the distribution of payouts,

6:15

you can see that you could win big.

6:17

If you tossed 100 heads,

6:19

you'd win 1.1 to the power of 100.

6:21

That's almost $14,000,

6:24

although the chance of that happening

6:25

is around 1 in 10 to the power of 30.

6:27

You'd be more likely to win the lottery

6:29

three times in a row.

6:30

On the other hand, the median payout is around 61 cents.

6:34

So if you're only playing the game one time

6:36

and you want even odds of turning a profit,

6:39

well, then you should pay less than 61 cents.

6:42

Though either way, if you played the game hundreds of times,

6:45

your payout would average out to $1.

6:48

Now, watch what happens if we switch the x-axis

6:50

from a linear scale to a logarithmic scale.

6:53

Well, then you see the curve transforms

6:54

into a normal distribution.

6:56

That's why this type of distribution

6:58

is called a log normal distribution.

7:01

- When random effects multiply,

7:03

if I have a certain wealth

7:05

and then my wealth goes up by a certain percentage next year

7:08

because of my investments,

7:10

and then the year after that,

7:11

it changes by another random factor,

7:14

as opposed to adding, I'm multiplying year after year.

7:17

If you have a big product of random numbers,

7:19

when you take the log of a product,

7:21

that's the sum of the logs.

7:24

So what was a product of random numbers

7:26

then gets translated into sums of logs of random numbers,

7:31

and that's what leads

7:32

to this so-called log normal distribution.

7:34

And log normal distributions produce big inequalities.

7:38

You don't just see a mean,

7:40

you see a mean with a big long tail.

7:42

It's much more likelihood of really big events,

7:45

in this case, tremendous wealth being obtained,

7:48

than you would expect from a normal distribution.

7:51

- The reason this curve is so asymmetric

7:53

is because the downside is capped at zero,

7:56

so at most, you could lose $1,

7:58

but the upside can keep growing up to nearly $14,000.

8:03

Now let's go on to table three.

8:05

Again, you'll be tossing a coin,

8:07

but this time you start out with a dollar

8:09

and the payout doubles each time you toss the coin

8:12

and you keep tossing until you get a heads,

8:15

then the game ends.

8:17

So if you get heads on your first toss, you get $2.

8:20

If you get a tails first

8:22

and then hit a heads on your second toss, you get $4.

8:25

If you flipped two tails and then a head,

8:27

on your third toss, you'd get $8, and so on.

8:30

If it took you to the nth toss to get a heads,

8:32

you would get two to the n dollars.

8:35

So, how much should you pay to play this game?

8:38

Well, as in our previous example,

8:40

we need to work out the expected value.

8:42

So suppose you throw a head on your first try,

8:45

the payout is $2

8:46

and the probability of that outcome is a half,

8:49

so the expected value of that toss is a dollar.

8:52

If it takes you two tosses to get a heads,

8:54

then the payout is $4

8:56

and the probability of that happening is one over four,

8:59

so again, the expected value is $1.

9:02

We also need to add in the chance

9:03

that you flip heads on your third try,

9:05

in that case, the payout is $8

9:07

and the probability of that happening is one over eight,

9:10

so again, the expected value is $1.

9:13

And we have to keep repeating this calculation

9:15

over all possible outcomes.

9:17

We have to keep adding $1 for each of the different options

9:20

for flipping the coin, say, 10 times until it lands on heads

9:23

or 100 times before you get heads.

9:26

I know it's extremely unlikely,

9:28

but the payout is so huge

9:29

that the expected value of that outcome is still a dollar,

9:33

so it still increases the expected value of the whole game.

9:37

This means that, theoretically,

9:39

the total expected value of this game is infinite.

9:44

This is known as the St. Petersburg paradox.

9:47

If you look at the distribution of payouts,

9:49

you can see it's uncapped,

9:51

it spans across all orders of magnitude.

9:53

You could get a payout of $1,000, $100,000,

9:56

or even a million dollars or more.

9:59

And while a million dollar payout is unlikely,

10:01

it's not that unlikely,

10:03

it's around one in a million.

10:06

Now, if you transform both axes to a log scale,

10:08

you see a straight line with a gradient of negative one.

10:12

The payout of the St. Petersburg paradox

10:14

follows a power law.

10:16

The specific power law in this case

10:18

is that the probability of a payout x

10:20

is equal to x to the power of negative one or one over x.

10:24

In the previous games when you have a normal distribution

10:26

or even a log normal distribution,

10:28

you can measure the width of that distribution,

10:31

its standard deviation.

10:32

And in a normal distribution,

10:34

95% of the data fall within two standard deviations

10:37

from the mean.

10:38

But with a power law, like in the St. Petersburg paradox,

10:41

there is no measurable width,

10:43

the standard deviation is infinite.

10:46

This makes power laws a fundamentally different beast

10:50

with some very weird properties.

10:52

- Imagine you take a bunch of random samples

10:54

and then average them

10:55

and then take more random samples and average them,

10:58

you'll find that the average keeps going up,

11:01

it doesn't converge.

11:03

And the more you measure,

11:04

the bigger the average is,

11:06

which is really weird, it sounds impossible,

11:09

but it's because it has such a heavy tail,

11:12

meaning the probability of really whopping big events

11:15

is so significant that if you keep measuring,

11:18

occasionally you're gonna measure

11:19

one of those extreme outliers

11:21

and they will totally skew the average.

11:24

It's sort of like saying,

11:26

if you're standing in a room with Bill Gates or Elon Musk,

11:30

the average wealth in that room

11:32

is gonna be 100 billion dollars or something (laughs)

11:36

because the average is dominated by one outlier.

11:39

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11:43

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11:45

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11:47

and data centers hold the personal information

11:49

of millions of people,

11:50

so when one of them gets hacked,

11:52

it can have ripple effects across the whole network.

11:56

We've had scammers get a hold of email addresses

11:58

and phone numbers of writers on our team

12:01

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12:04

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12:53

And now, back to power laws.

12:56

So, why do you get a power law

12:58

from the simple St. Petersburg setup?

13:01

If you look at the payout x,

13:03

you can see it grows exponentially

13:05

with each toss of the coin,

13:07

x equals two to the n.

13:09

But if you look at the probability of tossing the coin

13:12

that many times to get a heads,

13:14

you can see that this probability shrinks exponentially.

13:17

So the probability of flipping a coin n times

13:20

is 1/2 to the power of n.

13:22

But we're not really interested in the number of tosses,

13:24

we're interested in the payout.

13:26

Now we know that x equals two to the n,

13:28

so instead of writing two to the n

13:29

in our probability equation,

13:31

we can just write x.

13:32

So we end up with this,

13:34

the probability of a payout of x dollars

13:36

is equal to one over x,

13:38

or in other words, x to the power of negative one.

13:42

- You put them together,

13:44

the exponentials conspire to make a power law.

13:47

And that's a very common thing in nature,

13:49

that a lot of times when we see power laws,

13:51

there are two underlying exponentials

13:53

that are dancing together to make a power law.

13:57

- One example of this is earthquakes.

13:59

If you look at data on earthquakes,

14:01

you find that small earthquakes are very common,

14:03

but earthquakes of increasing magnitudes

14:06

become exponentially rarer.

14:09

But the destruction that earthquakes cause

14:10

is not proportional to their magnitude,

14:12

it's proportional to the energy they release.

14:15

And as earthquakes grow in magnitude,

14:17

that energy grows exponentially.

14:20

- So there's this exponential decay

14:21

in frequency of earthquakes of a given magnitude

14:24

and an exponential increase in the amount of energy released

14:29

by earthquakes of a certain magnitude.

14:31

So when you combine those two exponentials

14:34

to eliminate the magnitude,

14:36

what you find is a power law.

14:38

- But power laws also reveal something deeper

14:40

about the underlying structure of a system.

14:43

To see this in action,

14:44

let's go back to the third coin game

14:46

and the St. Petersburg paradox.

14:48

Now, you can draw all the different outcomes

14:50

as a tree diagram

14:51

where the length of each branch is equal to its probability.

14:54

So starting with a single line of length one

14:56

and then 1/2 for the first two branches,

14:59

1/4 for the next four, and so on.

15:01

Now, when you zoom in,

15:03

you keep seeing the same structure repeating

15:05

at smaller and smaller scales.

15:07

It's self-similar like a fractal,

15:10

and that's no coincidence.

15:12

We see the same fractal-like pattern in the veins on a leaf,

15:15

river networks, the blood vessels in our lungs,

15:18

even lightning,

15:19

and in all of these cases,

15:20

we can describe the pattern with a power law.

15:23

Power laws and fractals are intrinsically linked.

15:26

That's because power laws reveal something fundamental

15:29

about a system's structure.

15:31

- So I've got a magnet and I've got a screw,

15:34

and you'll notice if I bring them close together,

15:36

then the screw gets attracted to the magnet,

15:39

and that's because there's a lot of iron it,

15:40

which is ferromagnetic.

15:42

But watch what happens if I start heating this up.

15:46

Trying to...

15:47

Oh!

15:48

You see that?

15:49

Ah, there it went!

15:50

There it went!

15:50

You see, you heat it up and suddenly it becomes nonmagnetic.

15:54

To find out what happened,

15:55

let's zoom in on this magnet.

15:58

- Inside a magnet,

15:59

each atom has its own magnetic moment,

16:01

which means you can think of it

16:02

like its own little magnet or compass.

16:04

If one atom's moment points up,

16:06

its neighbors tend to point that way too

16:08

since this lowers the system's overall potential energy.

16:11

Therefore at low temperatures,

16:12

you get large regions called domains

16:15

where all the moments align.

16:17

And when many of these domains also align,

16:19

their individual magnetic fields reinforce

16:21

to create an overall field around the magnet.

16:24

But if you heat up the magnet,

16:26

each atom starts vibrating vigorously.

16:29

The moments flip up and down

16:31

and so the alignment can break down.

16:33

And when all the moments cancel out,

16:35

then there's no longer a net magnetic field.

16:38

Now, if you have the right equipment,

16:40

you can balance any magnetic material

16:42

right on that transition point,

16:44

right between magnetic and nonmagnetic.

16:47

This is called the critical point

16:48

and it occurs at a specific temperature

16:51

called the Curie temperature.

16:53

I asked Casper and the team to build a simulation

16:55

to show what's going on inside the magnet

16:58

at this critical point.

17:00

- Each pixel represents the magnetic moment

17:02

of an individual atom.

17:04

Let's say red is up and blue is down.

17:07

Now, when the temperature is low,

17:08

we get these big domains

17:10

where the magnetic moments are all aligned

17:12

and you get an overall magnetic field.

17:15

But if we really crank up the temperature,

17:17

then all of these moments start flipping up and down

17:20

and so they cancel out and the magnet loses its magnetism,

17:23

so that's exactly what happened in our demo.

17:26

But if we tune the temperature just right,

17:29

right to that Curie temperature,

17:31

then the pattern becomes way more interesting.

17:34

- This looks like a map.

17:36

- Like a map?

17:38

- Yeah, it almost looks like the Mediterranean or something.

17:40

It's almost stable,

17:43

like atoms that are pointing one way

17:45

tend to point that way for a while,

17:49

but there is clearly fluctuations as well,

17:53

so domains are constantly coming and going.

17:56

It's both got some elements of stability

18:00

and some persistence over time,

18:02

some features which are consistent,

18:04

but it's also not locked in place

18:08

because you notice changes over time.

18:12

- [Casper] If you zoom in,

18:12

you find that the same kinds of patterns

18:14

repeat at all scales.

18:16

You've got domains of tens of atoms,

18:17

hundreds, thousands, even millions.

18:20

There's just no inherent scale to the system,

18:22

that is, it's scale-free,

18:24

it's just like a fractal.

18:26

And if you plot the size distribution of the domains,

18:28

you get a power law.

18:31

- The underlying geometry suddenly shows a fractal character

18:34

that it doesn't have on either side of the phase transition.

18:38

Right at the phase transition,

18:39

you get fractal behavior

18:41

and that pops out as a power law.

18:43

- In fact, whenever you find a power law,

18:45

that indicates you're dealing with a system

18:47

that has no intrinsic scale,

18:49

and that is a signature of a system in a critical state,

18:53

which turns out has huge consequences.

18:56

- See, normally in a magnet below the Curie temperature,

18:59

each atom influences only its neighbors.

19:01

If one atom's magnetic moment flips up,

19:04

then that means that its neighbors are slightly more likely

19:06

to point up too.

19:07

But that influence is local,

19:09

it dies out just a few atoms away.

19:11

But as the magnet approaches its critical temperature,

19:13

those local influences start to chain together.

19:16

One spin nudges its neighbor

19:17

and that neighbor nudges the next and so on,

19:20

like a rumor spreading through a crowd.

19:22

And the result is that the effective range of influence

19:25

keeps expanding,

19:26

and right at the critical point,

19:28

it becomes effectively infinite.

19:30

A flip on one side can cascade

19:32

throughout the entire material.

19:35

So you get these small causes, just a single flip,

19:38

to reverberate throughout the entire system.

19:41

- And it gets right into that point

19:44

where the system is maximally unstable,

19:47

anything can happen.

19:48

It's also maximally interesting in a way.

19:51

It means the system is most unpredictable,

19:55

most uncertain,

19:56

it's really hard to know what's gonna happen next,

19:58

and that seems to be a natural procedure

20:00

that happens in many different systems in the world.

20:03

- One such system is forest fires.

20:06

In June, 1988,

20:08

a lightning strike started a small fire

20:10

near Yellowstone National Park.

20:12

This was nothing out of the ordinary.

20:14

Each year, Yellowstone experiences thousands

20:16

of lightning strikes.

20:17

Most don't cause fires

20:19

and those that do tend to burn a few trees,

20:21

maybe even a few acres before they fizzle out.

20:24

3/4 of fires burn less than 1/4 of an acre.

20:28

The largest fire in the park's recent history

20:30

occurred in 1931.

20:32

That burned through 18,000 acres,

20:34

an area slightly larger than Manhattan.

20:37

But the 1988 fire was different,

20:39

that initial spark spread slowly at first

20:42

covering several thousand acres.

20:44

Then over the next couple of months,

20:46

it merged with other small fires

20:47

to create an enormous complex of megafires

20:50

that blazed across 1.4 million acres of land.

20:54

That's around the size of the entire state of Delaware.

20:58

That's 70 times bigger than the previous record,

21:01

and 50 times the area of all the fires

21:03

over the previous 15 years combined.

21:07

So, what was so special about the 1988 fires?

21:10

Well, to find out, we made a forest fire simulator.

21:13

- We've got a grid of squares,

21:16

and on each square,

21:17

either a tree could be there, it could grow,

21:20

or it could not be there.

21:21

There's gonna be some probability for lightning strikes.

21:24

So the higher that probability,

21:26

the more fires we're gonna have.

21:27

We can run this.

21:29

- So trees are growing.

21:30

- [Casper] Trees are growing,

21:32

- Forest is filling in.

21:35

Nice.

21:36

Getting pretty dense.

21:38

- What do you expect is gonna happen?

21:39

- I expect to see some fires.

21:43

Probably, you know, now that...

21:45

Oh!

21:46

That was good,

21:47

that was a good little fire.

21:49

Whoa!

21:52

Whoa!

21:54

No way!

21:57

Well, that's crazy.

21:59

You haven't adjusted the parameters, right?

22:00

It's just like- - Not yet, not yet.

22:02

- This seems like a very critical situation just by itself.

22:07

I say that because of how big that fire was.

22:09

- This sort of system will tune itself to criticality,

22:14

and you can see it start to happen.

22:16

So right now,

22:16

I think it's a good moment where you have basically domains

22:19

of a lot of different sizes.

22:21

And then one way to think about it

22:23

is if some of these domains become too big,

22:26

then you get a single fire like that one, perfectly timed.

22:30

- Burns them all out. - It's just gonna propagate

22:31

throughout the whole thing and burn it back down a little.

22:34

But then if it goes too hard,

22:36

then now you've got all these domains

22:37

where there are no trees

22:38

and so it's gonna grow again

22:40

to bring it back to that critical state.

22:42

- I can see how it's the feedback mechanism, right,

22:45

that the fire gets rid of all the trees

22:47

and there's nothing left to burn,

22:49

and then that has to fill in again.

22:51

- [Casper] Yeah. - Yeah.

22:52

But if there hasn't been a fire,

22:54

then the forest gets too thick

22:55

and then it's ripe for this sort of massive fire.

23:00

- For a magnet,

23:01

you have to painstakingly tune it to the critical point,

23:03

but the forest naturally drives itself there.

23:06

This phenomenon is called self-organized criticality.

23:10

Yeah, and if you let it run,

23:11

what you get is, again, a power law distribution.

23:15

So this is log-log,

23:16

so it should be a straight line.

23:18

- That kind of stuff seems so totally random

23:22

and unpredictable,

23:23

and it is in one way,

23:25

and yet it follows a pattern.

23:26

There's a consistent mathematical pattern

23:28

to all these kind of disasters.

23:31

It's shocking.

23:33

- Is there something fractal about this?

23:36

- Mostly in terms of the, I guess, domains of the trees

23:39

when you're at that critical state.

23:42

So you get very dense areas, you get non-dense areas.

23:45

And as a result, when a single lightning bolt strikes,

23:48

you can get fires of all sizes.

23:50

Most often you get small fires of 10 or fewer trees burning.

23:54

A little less frequently,

23:55

you get fires of less than 100 trees.

23:57

And then every once in a while,

23:59

you get these massive fires

24:01

that reverberate throughout the entire system.

24:04

Now, you might expect that because the fire is so large,

24:06

there has to be a significant event causing it,

24:09

but that's not the case

24:11

because the cause for each fire is the exact same,

24:13

it's a single lightning strike.

24:16

The only difference is where it strikes

24:18

and the exact makeup of the forest at that time.

24:21

So in some very real way,

24:23

the large fires are nothing more

24:24

than magnified versions of the small ones,

24:27

and even worse, they're inevitable.

24:29

So what we've learned

24:30

is that for systems in a critical state,

24:32

there are no special events causing the massive fires.

24:35

There was nothing special about the Yellowstone fire.

24:39

- In 1935, the US Forest Service established

24:41

the so-called 10:00 AM policy.

24:44

The plan was to suppress every single fire

24:46

by 10:00 AM on the day following its initial report.

24:49

Now, naively, this strategy makes sense.

24:52

I mean, if you keep all fires under strict control,

24:54

then none can ever get out of hand.

24:57

But it turns out this strategy is extremely risky.

25:01

- So let's say we're gonna bring down

25:04

the lightning probability,

25:05

so it's very small,

25:06

only one in a million right now,

25:08

and we're also gonna crank up the tree growth a little bit.

25:12

Now what do you think is gonna happen?

25:14

- We're gonna get some big fires, I would imagine,

25:17

like a lot of not fire and then some huge fires.

25:21

Yeah.

25:22

(Derek laughs)

25:25

- [Casper] Yep.

25:26

- Oh boy.

25:27

- [Casper] So nowadays,

25:28

the fire service has a very different approach.

25:30

They acknowledge that some fires are essential

25:32

to make the megafires less likely.

25:34

So they let most small fires burn

25:36

and only intervene when necessary.

25:39

In some cases, they even intentionally create small fires

25:42

to burn through some of the buildup,

25:44

though it could take years

25:45

to return the forest to its natural state

25:47

after a century of fire suppression.

25:49

But it's more than just the Earth's forests

25:51

that are balanced in this critical state.

25:54

Every day, the Earth's crust is moving

25:56

and rearranging itself.

25:58

Stresses build up slowly

25:59

as tectonic plates rub against each other.

26:02

Most of the time, you get a few rocks crumbling,

26:04

the ground might move just a fraction of a millimeter,

26:07

but the stresses dissipate in many earthquakes

26:09

that you wouldn't even feel.

26:11

- There are really tiny earthquakes

26:13

that are happening right now beneath your feet,

26:16

you just can't feel 'em because they're very small.

26:19

But they are earthquakes,

26:20

they're driven by small slipping movements

26:23

in the Earth's crust.

26:25

- [Casper] But sometimes those random movements

26:27

can trigger a powerful chain reaction.

26:30

- [Derek] In Kobe, Japan,

26:31

the morning of January 17, 1995 seemed just like any other.

26:35

This was a peaceful city,

26:36

and although Japan as a country

26:38

is no stranger to earthquakes,

26:39

Kobe hadn't suffered a major quake for centuries.

26:42

Generations grew up

26:43

believing the ground beneath them was stable,

26:46

but that morning, deep underground,

26:48

a stress released nearby the Nojima fault line.

26:51

The stress propagated to the next section of the fault

26:54

and the next.

26:55

Within seconds,

26:56

the ruptured cascaded along 40 kilometers of crust,

26:59

shifting the ground by up to two meters

27:01

and releasing the energy equivalent

27:03

of numerous atomic bombs.

27:05

The resulting quake destroyed thousands of homes

27:07

along with most major roads

27:09

and railways leading into the city.

27:10

It killed over 6,000 people

27:12

and forced 300,000 from their homes.

27:16

- How far it goes depends a lot on chance

27:19

and the organization of all that stress field

27:22

in the Earth's crust.

27:23

And it just seems to be organized in such a way

27:26

that it is possible oftentimes

27:28

for the earthquake to trickle along an avalanche

27:31

along a long way

27:32

and produce a very large unusual earthquake.

27:35

But if you look at the process behind that earthquake,

27:37

it is exactly the same physical process.

27:40

It's just that the earthquake-generating process

27:43

naturally produces events

27:45

that range over an enormous range of scale,

27:47

and we're not really used to thinking about that.

27:50

- We have this ingrained assumption

27:51

that we can use the past to predict the future,

27:54

but when it comes to earthquakes

27:56

or any system that's in a critical state,

27:58

that assumption can be catastrophic

28:00

because they're famously unpredictable.

28:02

So, how can you even begin to model something

28:05

like the behavior of earthquakes?

28:07

- [Derek] In 1987, Danish physicist Per Bak

28:09

and his colleagues considered a simple thought experiment.

28:12

Take a grain of sand and drop it on a grid,

28:15

then keep dropping grains on top

28:17

until at some point the sandpile gets so steep

28:20

that the grains tumble down onto different squares.

28:23

- What they looked at was the size of these,

28:27

what they were calling avalanches,

28:28

these reorganizations of numbers of grains of sand.

28:32

They asked for how often do you see avalanches

28:34

of a certain size.

28:36

- This is the most simple version of a sandpile simulator

28:40

that you could almost imagine.

28:41

We're gonna drop a little grain of sand

28:43

at first always in the center,

28:45

and then it's just gonna keep going up.

28:47

For one grain, it'll be fine.

28:49

For two grains, it'll be fine.

28:50

Three grains, it'll be fine,

28:51

but it's on the edge of toppling.

28:53

And then when it reaches four or more,

28:55

it's gonna basically go.

28:58

It feels a bit like a, I don't know, pulsing thing,

29:01

like something's trying to escape or something,

29:03

very video game-like.

29:05

That seemed pretty crazy.

29:06

And it is symmetrical.

29:08

- Yeah, nice geometric features.

29:11

- So this might be interesting

29:12

because right now we passed it at a point

29:14

where this middle one is gonna go,

29:17

and then you look around it and you see,

29:19

essentially you can think of these brown

29:25

or these three tall grain stacks

29:29

as being maximally unstable.

29:30

They're about to go,

29:31

and so you could think of them

29:33

as these fingers of instability.

29:35

If anything touches them,

29:37

like, they're just gonna go.

29:40

(lively music)

29:42

- I see it propagating out.

29:45

- It's cool seeing it slower.

29:46

I feel like you can see several waves

29:50

propagating at the same time.

29:52

- Some people have reasoned that the Earth's crust

29:54

becomes riddled with similar fingers of instability

29:57

where you get stresses building up,

29:59

and then when one rock crumbles,

30:01

it can propagate along these fingers,

30:03

potentially triggering massive earthquakes.

30:06

If you look at the data,

30:07

there's some even more compelling evidence

30:09

that links the sandpile simulation to earthquakes.

30:13

- Let's say instead of dropping it at the center,

30:15

pretty unrealistic to have it drop in the center,

30:18

I'm gonna drop at random.

30:23

- Hah!

30:25

That's crazy.

30:26

- You can actually see it tune itself

30:28

to the critical state.

30:30

Like at the start,

30:31

you only see these super tiny avalanches

30:35

and then now it's everything.

30:36

- It has to build up.

30:38

- We can slow down a little.

30:42

Oh, and that's a super clean power law.

30:45

There are events of all sizes.

30:47

One grain of sand might knock over just a few others

30:50

or it could trigger an avalanche of millions of grains

30:53

that cascade throughout the entire system.

30:56

And if you look at the power law

30:58

you get from the sandpile simulation,

31:00

it closely resembles the power law

31:02

of the energy released by real earthquakes.

31:05

But if you look at the sandpile experiment more closely,

31:08

it doesn't just resemble earthquakes.

31:10

What does it remind you of?

31:12

- Forest fires. - [Casper] Right?

31:14

It feels like it's the exact same behavior.

31:16

- That's the really surprising thing,

31:18

and that's why this little paper with a sandpile

31:20

was published in the world's top journal

31:23

because it did something

31:24

that people just didn't really think was possible.

31:27

- Now, what's ironic is if you look at real sandpiles,

31:31

they don't behave like this.

31:33

- Okay, you said sand,

31:35

I'm gonna do an experiment on a real sandpile.

31:37

And of course, it doesn't follow a power law distribution

31:39

of avalanches at all.

31:41

It's totally wrong.

31:43

(Steven and Derek laugh)

31:44

Per Bak, naturally, gets a chance to reply to the criticism,

31:49

and he says, I'm pretty close to quoting,

31:52

he says, "Self-organized criticality

31:54

only applies to the systems it applies to."

31:57

(Steven laughs)

31:58

So he doesn't care,

32:00

the fact that his theory is not relevant to real sandpiles.

32:03

So what?

32:04

Get out of my face.

32:05

He's interested in bigger fish to fry than sandpiles.

32:10

It's like, you're taking me too literally.

32:12

I'm talking about a universal mechanism

32:14

for generating power laws.

32:15

And the fact that it doesn't work in real sand

32:18

is uninteresting to him.

32:20

I thought that took some real nerve.

32:22

- You could think about the Earth

32:26

and the Earth going around the Sun.

32:28

That's a very complex system.

32:31

You've got the molten core,

32:32

everything sloshing around,

32:33

and you've got oceans,

32:34

and you've even got the moon going around the Earth,

32:36

which in theory, you know,

32:38

all should affect the exact motion

32:40

of the Earth around the Sun.

32:42

But Newton ignored all of that,

32:44

all he looked at was just a single parameter, essentially,

32:48

the mass of the Earth.

32:50

And with that, he could correctly, for the most part,

32:52

predict how the Earth was gonna go around the Sun.

32:54

Similarly here,

32:56

there are people that have looked at these phenomena

32:58

that go to the critical state,

33:00

in this case it's self-organized criticality,

33:03

is it brings itself there,

33:05

and what they find is that there's this universal behavior

33:07

where it doesn't even really matter what the subparts are,

33:11

you just get the behavior that's the exact same.

33:14

- At that critical point

33:16

when all the forces are poised

33:18

and the system is right on that delicate balance

33:21

between being organized, highly organized,

33:24

or being totally disorganized,

33:26

it turns out that almost none of the physical details

33:29

about that system matter to how it behaves.

33:33

There's just a universal behavior that is irrespective

33:37

of what physical system you're talking about.

33:39

The term that was used is called universality,

33:42

and it's kind of a miracle,

33:44

it means you can make extremely powerful theories

33:47

without involving any technical details,

33:49

any real details of the material.

33:52

- What this means is that you could have these systems

33:54

that on the surface seem totally different,

33:57

but when you get to the critical point,

33:58

they all behave in the exact same way.

34:01

The other thing you could do is instead of this being trees,

34:05

you could imagine it being people

34:07

and the thing that's spreading-

34:08

- Is disease.

34:09

- Is disease, yeah.

34:12

- You almost get something for nothing

34:15

at these critical points.

34:16

- See, many of these systems fall into what's known

34:18

as universality classes.

34:20

Some of them you need to tune to get there,

34:22

like magnets at their Curie temperature

34:24

or fluids like water or carbon dioxide

34:27

at their critical point,

34:28

but some other systems

34:29

seem to organize themselves to criticality,

34:32

like the forest fires or sandpiles or earthquakes.

34:36

But what's crazy is that if you succeed

34:38

in understanding just one system from a class,

34:41

then you know how all the systems in that class behave,

34:44

and that includes even the crudest simplest toy models,

34:48

like the simulations we've looked at.

34:50

So you can model incredibly complex systems

34:53

with the most basic of models.

34:55

And some people think this critical thinking

34:57

applies even further.

34:59

When we look around the world,

35:00

there are lots of systems

35:01

that show the same power law behavior

35:03

that we see in this critical systems.

35:05

It's in everything from DNA sequencing

35:08

to the distribution of species in an ecosystem

35:10

to the size of mass extinctions throughout history.

35:13

We even see the same behavior in human systems,

35:16

like the populations of cities,

35:18

fluctuations in stock prices,

35:20

citations of scientific papers,

35:22

and even the number of deaths in wars.

35:25

So some people argue that these systems

35:27

and perhaps many parts of our world also organize themselves

35:31

to this critical point.

35:33

- So the fact that all these natural hazards,

35:35

as they call them,

35:36

floods, wildfires, and earthquakes,

35:38

they all follow power law distributions

35:40

means that these extreme events are much more common

35:45

than you would think based on normal distribution thinking.

35:48

- If you find yourself in a situation

35:50

or an environment that is sort of governed by a power law,

35:54

how should you change your behavior?

35:56

- If you have events with one of these power distributions,

36:01

what you're seeing most of the time is small events.

36:04

And this can lull you into a false sense of security,

36:08

you think you understand how things are going.

36:10

You know, floods for example,

36:11

there are a lot of small floods,

36:12

and then every once in a while, there's a huge one.

36:15

One response to this is insurance,

36:18

that insurance is designed precisely

36:21

to protect you against the large rare events

36:24

that would otherwise be very bad.

36:25

But then there's the other side of that picture,

36:29

which is you are the insurance company

36:31

that needs to insure people

36:33

and they have a particularly difficult job

36:35

because they have to be able to say how much to charge

36:39

so that they have enough money to pay out

36:41

when the big bad thing comes along.

36:44

- [Derek] In 2018,

36:44

a forest fire tore through Paradise, California,

36:47

it became the deadliest

36:48

and most destructive fire in the state's history,

36:51

but the insurance company, Merced Property & Casualty,

36:54

hadn't planned for something that huge,

36:57

and when the claims came in,

36:58

they just didn't have the reserves to pay out.

37:01

So just like that, the company went bust.

37:04

- But while extreme events can cripple some companies,

37:07

there are entire industries

37:09

that are built on power law distributions.

37:12

Between 1985 and 2014,

37:15

private equity firm Horsley Bridge

37:17

invested in 7,000 different startups

37:20

and over half of their investments actually lost money,

37:23

but the top 6% more than 10xed in value

37:26

and generated 60% of the firm's overall profit.

37:29

In fact, the best venture capital firms

37:31

often have more investments that lose money,

37:34

they just have a few crazy outliers

37:36

that show extraordinary growth,

37:38

a few outliers that carry the entire performance.

37:41

In 2012, Y Combinator calculated that 75% of their returns

37:46

came from just two out of the 280 startups they invested in.

37:50

So venture capital is a world that depends on taking risks

37:53

in the hope that you'll get a few of these extreme outliers

37:57

which outperform all of the rest

37:58

of the investments combined.

38:00

- [Derek] Book publishers operate in a similar fashion,

38:03

most titles flop,

38:05

but in 1997,

38:06

a small independent UK publisher called Bloomsbury

38:09

took a chance on a story about a boy wizard.

38:12

The boy's name, of course, was Harry Potter,

38:14

and now Bloomsbury is a globally recognized brand.

38:18

We see a similar pattern play out on streaming platforms.

38:21

On Netflix, the top 6% of shows account for over half

38:24

of all viewing hours on the platform.

38:26

On YouTube,

38:27

less than 4% of videos ever reach 10,000 views,

38:30

but those videos account for over 93% of all views.

38:35

- All these domains follow the same principle

38:37

that Pareto identified over 100 years ago

38:39

where the majority of the wealth goes to the richest few.

38:43

The entire game is defined by the rare runaway hits.

38:47

- But not every industry can play this game.

38:50

Like if you're running a restaurant,

38:51

you need to fill tables night after night.

38:54

You can't have one particularly busy summer evening

38:56

that brings in millions of customers

38:57

to make up for a bunch of quiet nights.

39:00

Over a year, the busy nights and quiet ones balance out

39:02

and you're left with the average.

39:04

Airlines are similar,

39:05

an airline needs to fill seats on each flight.

39:08

You can't squeeze a million passengers onto one plane,

39:11

so it's the average number of passengers over the year

39:13

that defines an airline's success.

39:16

- We're used to living in this world

39:17

of normal distributions and you act a certain way,

39:20

but as soon as you switch to this realm

39:22

that is governed by a power law,

39:24

you need to start acting vastly different.

39:26

It really pays to know what kind of world

39:28

or what kind of game you're playing.

39:30

- That is good.

39:31

That's good, yes.

39:32

You should come on camera and just say that just like that.

39:35

You were on camera, you just did do it.

39:37

(Steven laughs) - If you are in a world

39:40

where random additive variations cancel out over time,

39:42

then you get a normal distribution.

39:44

And in this case, it's the average performance,

39:47

so consistency, which is important.

39:50

But if you are in a world that's governed by a power law

39:52

where your returns can multiply

39:54

and they can grow over many orders of magnitude,

39:57

then it might make sense to take some riskier bets

39:59

in the hope that one of them pays off huge.

40:02

In other words,

40:03

it becomes more important to be persistent than consistent.

40:07

- [Derek] Though as we saw in the second coin game,

40:08

totally random multiplicative returns

40:10

give you a log normal distribution, not a power law.

40:14

To get a power law,

40:15

there must be some other mechanism at play.

40:18

In the early 2000s,

40:19

Albert-László Barabási was studying the internet,

40:22

and to his surprise,

40:23

he found that there was no normal webpage

40:26

with some average number of links.

40:28

Instead, the distribution followed a power law.

40:30

A few sites like Yahoo

40:32

had thousands of times more connections

40:34

than most of the others.

40:36

Barabasi wondered what could be causing

40:38

this power law of the internet,

40:39

so he made a simple prediction.

40:41

As new sites were added to the internet,

40:43

they were more likely to link to well-known pages.

40:46

To test this prediction,

40:48

he and his colleague Réka Albert ran a simulation.

40:51

They started with a network of just a few nodes

40:53

and gradually they added new nodes to the network

40:56

with each new node more likely to connect to those

40:59

with the most links.

41:00

As the network grew, a power law emerged.

41:03

The power was around negative two,

41:05

which almost exactly matched the real data of the internet.

41:08

- [Casper] Look at that. - [Derek] That's fun.

41:11

- It's still so satisfying.

41:12

This will basically also distribute a power law.

41:15

One of the ideas here is that this could be individuals

41:18

or even companies,

41:19

and so if you're more likely

41:21

to become more successful or more well known

41:25

or successful you already are,

41:26

you're gonna get this sort of runaway effect

41:28

where you get a few that sort of dominate the distributions.

41:33

I wonder if part of the takeaway

41:34

is like if you're playing some sort of game

41:37

that is dominated by a power law,

41:39

then you better do the work as much of it

41:41

as early as possible

41:42

so you get to benefit from the snowball effect, essentially.

41:46

- Yeah, I guess that's a good idea.

41:48

I'm not sure whether you can control it, though.

41:50

Human beings like to think of ourselves

41:52

as being a bit special,

41:54

and that maybe somehow because we're intelligent

41:56

and have free will.

41:59

We will escape the provenance of the laws of physics

42:05

in order and organization,

42:06

but I think that's probably not the case.

42:09

So if you look at the number of world wars,

42:12

and if you make a crude measure of how big is the world war

42:15

by how many people it kills,

42:18

which is a bit macabre, but still,

42:21

you find that, again, it follows a power law

42:23

virtually identical to the power law you find

42:25

in stock market crashes.

42:27

- So if the world is shaped by power laws,

42:30

then it feels like we're poised

42:32

in this kind of critical state

42:33

where two identical grains of sand,

42:36

two identical actions can have wildly different effects.

42:40

Most things barely move the needle,

42:42

but a few rare events totally dwarf the rest,

42:44

and that, I think, is the most important lesson.

42:47

If you choose to pursue areas

42:49

governed by the normal distribution,

42:51

you can pretty much guarantee average results.

42:54

But if you select pursuits ruled by power laws,

42:56

the goal isn't to avoid risk,

42:58

it's to make repeated intelligent bets.

43:00

Most of them will fail,

43:02

but you only need one wild success to pay for all the rest.

43:06

- And the thing is that beforehand you cannot know

43:08

which bet is going to be

43:10

because the system is maximally unpredictable.

43:12

It could be that your next bet does nothing,

43:14

it could do a little bit,

43:15

or it could change your entire life.

43:18

In fact, around three years ago,

43:19

I was reading this little book,

43:21

and in the book there was this little line

43:23

saying something like,

43:24

"One idea could transform your entire life."

43:27

So right underneath that, I wrote,

43:29

"Send an email to Veritasium."

43:32

A couple days later, I wrote an email to Derek, saying,

43:34

"Hey, Derek, I'm Casper.

43:36

I study physics and I can help you research videos."

43:39

I didn't hear back for four weeks,

43:41

so I was getting pretty sad

43:42

and just wanted to forget about it and move on,

43:46

but then a couple days later I got an email back saying,

43:49

"Hey, Casper, we can't do an internship right now,

43:52

but how would you like to research, write,

43:54

and produce a video as a freelancer?"

43:57

So I did,

43:58

and that's how I get started at Veritasium.

44:04

Hey, just a few quick final things.

44:06

All the simulations that we used in this video

44:09

we'll make available for free for you to use

44:11

in the link in the description.

44:14

And the other thing is that we just launched

44:16

the official Veritasium game.

44:18

It's called Elements of Truth

44:19

and it's a tabletop game with over 800 questions.

44:22

It's the perfect way to challenge your friends

44:25

and see who comes out on top.

44:27

Now, at Veritasium, we're all quite competitive,

44:30

so every time we play, things get a little bit heated,

44:32

but that's honestly a big part of the fun.

44:35

Now, when we launched on Kickstarter,

44:37

we got a lot of questions asking

44:39

if we could ship to specific countries.

44:42

And originally we didn't enable this,

44:44

and this is our mistake,

44:45

this is on us and we totally hear you,

44:48

but I'm glad to say

44:49

that right now we have enabled worldwide shipping.

44:52

So no matter where you are in the world,

44:54

you can get your very own copy.

44:55

To reserve your copy and get involved,

44:58

scan this QR code or click the link in the description.

45:02

I wanna thank you for all your support,

45:03

and most of all, thank you for watching.

Interactive Summary

The video explores the concept of power laws, contrasting them with normal distributions. While normal distributions describe phenomena where data clusters around an average (like human height), power laws describe systems with extreme outliers and a wide range of outcomes, where small causes can have massive effects. Examples of power laws include income distribution (Pareto's law), the size of world wars, earthquakes, forest fires, and even internet link structures. The concept of self-organized criticality explains how some systems naturally evolve to a state where they are maximally sensitive to change, exhibiting power law behavior. This critical state is characterized by a lack of intrinsic scale, fractal-like patterns, and unpredictable outcomes. Understanding whether a system follows a normal distribution or a power law is crucial for decision-making, as it dictates whether consistency or persistent, risk-taking strategies are more effective.

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