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Chow Lectures 2025 by Nima Arkani-Hamed: Geometry & Combinatorics of Scattering Amplitudes Part II

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Chow Lectures 2025 by Nima Arkani-Hamed: Geometry & Combinatorics of Scattering Amplitudes Part II

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0:15

So I realized that I hardly said

0:17

anything yesterday uh in two hours. Very

0:20

impressive. Uh that's what tenure is

0:22

for, you know. So um uh but um uh but

0:27

actually I realized that it presents me

0:28

with a with a good opportunity. So um

0:31

yesterday I was planning on after saying

0:33

my very little um to say something uh

0:36

and I was going to first uh as I

0:38

mentioned first talk about the

0:40

motivation that led up to the ample say

0:43

a few things about it and talk about

0:45

some open problems and uh that was to

0:47

sort of piggyback off the beautiful

0:50

lectures that we had yesterday on on uh

0:53

on on related topics. um uh and then for

0:58

my uh second lecture today's lecture I

1:00

was going to tell you about the uh uh

1:02

trace by cube theory and soahedra and so

1:04

on. Now um in fact sort of logically the

1:09

story of trace 5 cubed and the

1:11

sosahhedra and the connection to curves

1:12

on surfaces is simpler is quite a bit

1:15

simpler is somewhat more mathematically

1:18

standard and much better understood by

1:20

now than what what I definitely feel is

1:22

a much deeper and more interesting story

1:24

related to amplitra. Okay. Um but then

1:27

for that for that reason uh and

1:29

especially since we just had Caroline

1:30

this morning I'm just going to reverse

1:31

the order of presentation which now

1:33

makes a lot more logical sense. uh just

1:35

to start with a simpler story where

1:37

things we are can be understood in a

1:38

much more uh straightforward way and

1:40

then tomorrow I'll tell you something

1:42

about the open problems related to the

1:44

ample and then if we get there I'll tell

1:46

you something about the the large end

1:48

story that I uh advertised as well. So

1:51

um so that's what we're going to do uh

1:54

I'm really going to uh begin. So uh so

1:57

so before getting into a really

2:00

systematic exposition of the story, what

2:02

what we're what we're going to try to do

2:04

today is understand this trace 5 cube

2:06

theory. um that uh that's been

2:09

introduced I I'll I'll I'll introduce

2:11

again um and ultimately we'll understand

2:14

it not just at tree level but to all

2:16

orders in perturbation theory because

2:18

there's going to be some way of thinking

2:19

about it uh has nothing to do with

2:21

plarity non-planer everything but the

2:23

color is important but other than that

2:24

to all orders in perturbation theory um

2:27

and uh at least sketch uh for you uh how

2:31

it's related to uh very simple pictures

2:34

of curves on surfaces and some very

2:36

interesting combinatorics associated

2:38

with uh uh uh with these curves on

2:41

surfaces. This is going to connect to uh

2:44

uh field theory trace cubed amplitudes.

2:47

It you can think of it as a bottomup

2:49

discovery of string theory trace cubed

2:51

amplitudes at least in some uh in some

2:55

uh in some limits. In fact, we run into

2:56

a larger collection of objects than than

2:59

standard string theory. Standard string

3:01

theory will be contained in as sort of

3:03

one corner, one special uh sort of

3:06

choice of what this uh uh what this

3:09

object looks like. But you're allowed to

3:10

work with a larger world of ideas. But

3:13

as we'll see, you can sort of get to

3:14

string theory without uh uh six months

3:17

of a uh or a year of a graduate course

3:20

in uh uh in the subject. Okay. So that's

3:23

that's what what what we're going to do.

3:26

But what I want to I want to begin

3:28

before we get into lots of you know

3:30

definitions and for I actually want to

3:31

begin with the uh with the example that

3:34

uh that Carolina talked about uh quite a

3:37

lot of this pentagon. Okay. So here

3:40

we're talking about the uh n equals 5

3:42

point amplitude.

3:45

Um and as uh as Carolina explained it's

3:48

associated with this picture of the uh

3:51

this particular realization

3:54

of the isocahedron. I'll also draw in

3:56

this case the mesh that uh she drew for

4:00

us. Okay. So the amplitude is a function

4:03

of these x variables as she explained.

4:05

So uh this would be x24, x25 and x35.

4:09

And then we also have these meshes uh

4:12

c13, c14

4:14

uh and c2 uh and c24 with the formula

4:17

that she gave that I'll write down again

4:19

uh in a second. Okay. So um uh so we

4:23

have uh we have uh in x13

4:27

uh x14 space we have this picture

4:32

of the socedin where that is here is c13

4:36

this here is 3 c13 plus c14 and this up

4:41

here is c14 plus c24. Okay.

4:45

Okay.

4:47

And so um what what we're going to see

4:49

in in the rest of the lecture for this

4:51

example and many more besides is where

4:52

this all comes from. Okay. So so so

4:55

Carolina motivated it. Um but at some

4:57

points there's a few little you know out

5:00

of somewhat out of the blue steps like

5:02

who told you to draw this mesh? Who told

5:04

you to write the equation x plus x - x -

5:06

x equals constant? All of those things

5:08

sort of seem fairly simple and natural.

5:10

Uh but uh but they're a little bit

5:12

pulled out of apparently nowhere. So um

5:14

so I'm going to talk about an alternate

5:16

point of view for where these things

5:17

come from which is 100% rational. Okay

5:20

is 100% ma rational but will have a

5:22

couple of magical features in it

5:24

nonetheless. Okay so uh but the moves

5:26

that you start making are 100% rational

5:29

but um to give you an idea of uh what it

5:33

will be about uh I just want to

5:35

illustrate some of the things that we'll

5:36

talk about already in this example.

5:38

Okay. So essentially what we're going to

5:40

be talking about is a duel of this

5:42

picture. Uh and um so uh uh uh

5:47

everything that I will say later also

5:49

has an avatar directly in the language

5:50

of the original polytopes. But we're

5:52

sort of going to focus on a on a duel of

5:54

this picture. And if I start here, we're

5:57

going to look at the sort of we're going

5:59

to start by looking at the inward

6:00

pointing normals

6:02

um to the facets of this uh of this

6:05

pentagon. Okay. So that's of course a

6:07

very standard way to see a dual object.

6:09

You have a polytope, the dual polytope,

6:11

the vertices of the dual polytope or the

6:13

facets of the original polytope and so

6:15

on. So it's very reasonable to look at

6:17

those uh inward pointing normals. And if

6:20

you remember this was the face where x13

6:24

goes to zero. This is where x24 goes to

6:27

zero. Uh sorry x1 uh sorry this is where

6:31

x13 goes to x14 goes to zero. This is

6:34

where x24 goes to zero, x25 goes to

6:38

zero,

6:40

x35 goes to zero

6:42

and x14 goes to zero as you also see

6:45

from the uh sorry x13 goes to zero as

6:48

you see from the picture. Okay. So again

6:51

this corner is where both x14 and x13 go

6:55

zero. So you can think of this line as

6:57

associated with this partial

6:59

triangulation of the uh underlying

7:01

pentagon. Just repeating things Carolina

7:03

said, right? This is associated with

7:05

this partial triangulation.

7:09

And so this vertex is where the the two

7:12

of them come together. They don't cross

7:13

each other. That's good. So they come

7:15

together there and we get the sort of

7:16

134

7:19

complete triangulation. And the same

7:20

thing happens uh as we go around. Okay.

7:24

So all of the things that meet

7:26

correspond to chords that don't cross

7:28

and the vertices where they meet are the

7:30

complete triangulation that uh goes goes

7:32

along with that. All right.

7:35

So uh we're first going to just draw

7:37

those draw those arrows. And if I draw

7:40

those arrows I get the following

7:41

picture.

7:43

I'm just drawing the normals.

7:46

Okay.

7:48

Now I've chosen to draw the normal so

7:50

they're all like 01 vectors, right? So

7:52

they have zeros or ones. We'll we'll

7:54

we'll come come to that point later. Uh

7:56

I mean when you just draw normals

7:57

there's no meaning to the magnitude of

7:59

the enormal but the but the but these

8:01

mag it's very reasonable thing to do and

8:03

it'll have an explanation later. Okay.

8:06

But here this would be associated I

8:08

won't keep writing X. That will be

8:09

associated with 13. Right? That's this

8:12

inward pointing normal. That's 13. This

8:15

is 1 14

8:17

2 4 25 and 35. Okay.

8:22

And so what we have here is a picture

8:23

where now the kind of plane is divided

8:26

into these cones. Right? The plane is

8:28

divided into these cones.

8:34

And this is the normal fan of the

8:37

corresponding polytope. The dual these

8:40

cones are just associated with the

8:41

vertices of the polytope in the obvious

8:43

way. Okay. So again this cone 1314 is

8:48

associated with this vertex, right? It's

8:50

the two uh it's the it's the two facets

8:53

that meet at that at that vertex that's

8:55

associated with this this this cone. So

8:58

again the point is that this 1314 this

9:01

region is now associated with a vertex

9:03

and that's this vertex right that

9:05

corresponds to this this triangulation

9:08

and the cool thing in this picture is

9:10

that the plane has been divided into

9:12

sort of five regions and each region is

9:14

uniquely associated with a diagram right

9:19

so that's just the dual statement that

9:22

we had an object whose vertices were

9:24

capturing all all of the diagrams okay

9:26

so so far I'm just resetting uh some of

9:29

the things that Carolina told you in

9:31

this uh in the language of this uh uh

9:35

dual uh fan. Okay, so this sometimes

9:37

called the normal fan of the uh of the

9:41

polytope.

9:43

Okay, so again the most basic things are

9:46

that uh uh are that the cones of that

9:49

that we have cones they cover the whole

9:51

space and that each cone can be

9:53

associated with one of the diagrams.

9:56

Okay. Now, something else that Karolina

9:59

told you is that this associally

10:03

presented as a Minkowski sum. Okay,

10:05

that's a remarkable fact. Just to sort

10:07

of pause and back up for a second,

10:10

there's just the zeroth fact that the

10:12

combinatorics of diagrams of

10:13

triangulations of a polygon are captured

10:16

by the faces of an object. Okay, that's

10:19

Stashev's realization. Amazing. That's

10:21

already remarkable, right? If you like

10:23

that's all about fineman diagrams

10:25

related to fineman diagrams

10:27

factorization you know all of those

10:28

words are related to this fact

10:32

the fact that the socied has a

10:34

particular realization not a random one

10:36

you know you can draw it in lots of ways

10:37

I could draw this pentagon with sort of

10:39

sides uh you know tilted with random

10:42

angles and then what I'm saying would

10:44

not be true okay um but the fact that

10:47

there's a particular realization of

10:48

these with parallel sides you see these

10:50

parallel sides mean a lot in this

10:52

picture. Okay. Um uh tells us that uh it

10:57

can also be represented as a sum of

11:00

simple pieces. Okay. The fact that it's

11:03

representable as a sum of simple pieces

11:05

is remarkable is is an extra fact on top

11:09

of the stash effect that that the

11:11

combinatorics is captured by polytope.

11:14

And as Carolina explained in her talk,

11:16

this extra fact has extra implications

11:17

for the amplitude that we didn't know

11:19

about before. Okay, this extra fact

11:21

makes it easy to predict where the

11:22

amplitude vanishes uh and how when you

11:25

go close to the places it vanishes, it

11:27

also factorizes in a way that's uh not

11:29

at all obvious uh if you uh know

11:32

something about fineman diagrams. Okay,

11:34

so this is an extra interesting fact

11:36

that the that the that the association

11:38

is naturally Mowski sum. How is that

11:41

fact reflected in this picture? So let's

11:43

remember what the sum ends look like.

11:45

You know, we had a sum end that looked

11:46

like this. We had a sum end that looked

11:49

like this. and we had a sum end that

11:51

looked like this.

11:53

Okay? And those of you who know about

11:55

Newton polytopes and tropical

11:57

tropicalization and so on are going to

11:58

know exactly what I'm about to do now.

12:01

Okay? But those of you who don't, there

12:03

is something we can obviously do with

12:05

this uh picture as well. I can look at

12:08

the normals to each one of these pieces,

12:11

right? So the normal to this piece looks

12:13

like this

12:15

in the same way. And the normal to these

12:17

piece will look like this. You know,

12:19

look, I guess like this if I'm doing

12:21

inward pointing.

12:26

Okay.

12:29

So, notice that if I just draw these

12:32

guys, well, if I draw uh this one, it

12:35

looks like this.

12:39

Okay. If I draw this one, it just looks

12:43

like this.

12:44

And if I draw the other one, it looks

12:46

like this.

12:48

Okay.

12:50

So the fact that you can uh build the

12:53

associ

12:55

sum in the language of the normal of

12:57

this normal fan is reflected in the

13:00

following cool thing. This has five

13:02

pieces. So I've made kind of a

13:04

complicated space, right? That's uh

13:05

that's divided into five pieces. But I

13:08

can make those five pieces by laying on

13:10

top of each other these three pictures.

13:13

Okay, I have this picture and then I put

13:16

this picture on top of it and I put this

13:18

picture on top of it and putting all the

13:20

pictures on top of each other uh gives

13:22

us this division of the space into the

13:25

five regions each one of which

13:27

corresponds to uh one of these vertices

13:30

uh triangulations

13:32

diagrams all the different ways we could

13:34

we could talk about it right so that's a

13:36

sort of a well-known statement that the

13:38

Minkowski sum at the level of the

13:41

polytope is reflected ed as a common

13:44

refinement of the sums at the level of

13:47

the fan. Okay, if I look at each sort of

13:49

element and I look at the the normal

13:52

vectors for each element, I can build

13:54

the complicated uh fan by just putting

13:56

them stacking them on on top of each

13:58

other. Okay.

14:01

Okay. So that's uh that's and that's

14:03

that's how this fact is represented. And

14:05

now we're going to try to uh uh uh

14:08

understand this this fact better.

14:12

Now um

14:14

another two things to say in this uh

14:16

example

14:18

you know if you're given these sumans

14:21

and let me call this direction I'm just

14:22

going to give these directions names

14:24

sort of 13 and 14 okay as we see in in

14:28

this uh picture just associated with the

14:31

the uh the the the normal quadrant here

14:34

um it's of course natural to associate

14:37

polomials with each one of these

14:40

pictures. Okay. So I'm going to

14:42

associate with this picture I'm going to

14:43

associate the polinomial 1 + y14.

14:47

Okay. With this picture I'm going to

14:48

associate the polinomial 1 + y13.

14:52

And with this picture I'm going to

14:54

associate 1 + y14 + y14 y13.

14:59

Okay.

15:01

These are polomials which are a sum of

15:04

monomials and every monomial just

15:06

records the uh the corresponding uh

15:09

vertex of the picture. Okay. So uh this

15:12

vertex is 0 0 this is 01 and this is 1

15:16

comma 1 and so this polomial is 1 for 0

15:20

0 y14 for 01 and y14 y13 for 1 one.

15:24

Okay. So those of you who know about

15:27

Newton polytopes uh will then say that

15:29

the Newton polytope of this polomial is

15:31

back to uh this uh simplex. Okay. The

15:37

Newton polytope of this guy is back to

15:38

this uh of this is back to this one.

15:41

This guy is back to this one. All right.

15:45

Okay.

15:47

um

15:51

something that we can do with these uh

15:53

uh polomials of course none of this is a

15:55

coincidence but I just want to

15:56

illustrate in this example before we say

15:59

everything in general

16:04

and that's the revolution from this

16:05

morning okay so

16:08

erase this

16:18

I'll leave while this is drying.

16:23

Something that we can do with these

16:25

polinomials is we can imagine what what

16:27

would happen if I mean they're all sort

16:29

of plus signs here. So it's very natural

16:30

to imagine that the y's are positive. So

16:32

let's imagine that y13 and y14 are

16:35

positive. Remember I pos I promised you

16:37

positivity is everywhere in this story.

16:40

And here it is at the very at in the

16:42

very most uh basic place.

16:45

Um well for example we could uh do this

16:48

by writing y13 is e to the negative t13.

16:51

This is a pure convention the minus sign

16:53

here. Uh but this convention we like to

16:56

use is e the minus uh t14. So now t13

17:00

and t14 just vary over the entire real

17:03

line. Okay. though.

17:05

Um and so a kind of a natural question

17:08

when when you when you look at these uh

17:10

polomials is to ask in T13 T14 space as

17:15

you go off to infinity in all possible

17:17

ways you know what do these polomials

17:19

look like as you go off to infinity in

17:22

different ways different terms in these

17:24

polomials are going to dominate

17:27

and uh so they will simplify. Of course,

17:29

this is the entire uh this is the

17:31

beginning of thinking about uh tropical

17:33

geometry and tropicalization.

17:36

But uh I just want to do it in this in

17:38

this example. Okay. So, so uh so

17:41

remember the logic is we got these sum

17:42

ends. It's natural to associate these

17:44

polomials with the sum ends and now

17:46

we're going to just ask what they these

17:48

things are not linear but we're going to

17:50

ask what they look like as we

17:51

asmtoically go off to infinity in the

17:53

positive domain where the y's are

17:54

positive. And so for example, what does

17:57

1 + e the minus t14 look like as the t's

18:02

go to infinity? This is going to look

18:04

like e to the max of zero and minus t14.

18:09

Right? That just says either that

18:11

dominates or that dominates. And so

18:13

whoever dominates, we're going to get uh

18:15

we're going to get that guy, right? Um

18:17

let's do the more complicated one. If we

18:19

look at 1 - eus t14 plus eus t14 eus t13

18:25

this is going to go to e to the max

18:29

well either one dominates or if t14 is

18:32

minus t14 is the biggest that will

18:34

dominate or if minus t14us t13 is

18:37

positive that'll dominate.

18:40

Okay. So there's really nothing to do

18:42

here other than just put maxes

18:44

everywhere. All right.

18:49

Okay.

18:51

But now if we

18:55

look at this uh picture, let's let's

18:57

let's do the uh let's do that uh simple

19:00

one first. This uh 1 + uh uh 1 + uh y14.

19:07

If we just ask um where does uh so uh so

19:11

1 + y14

19:13

is going to uh e to the max of zero and

19:18

minus t14.

19:22

And so this in t13 t14 space is not a

19:26

linear function but it's close. It's

19:28

peacewise linear. Sometimes it's going

19:30

to be zero sometimes it's going to be uh

19:32

negative t14. Okay. And so this has a

19:37

domain of linearity in positive T14

19:41

space up here in positive uh uh uh sorry

19:46

I I'll draw it like this.

19:48

[Music]

19:53

In positive T14 space this is zero and

19:57

in negative T14 space it's minus T14.

20:02

Okay,

20:06

so this thing is linear down here is

20:09

negative t14 is linear up here and what

20:12

separates them is exactly the fan that

20:15

we associated with this little factor.

20:18

Okay.

20:24

All right. If we do the more complicated

20:27

example.

20:30

So if we look at 1 + y14 plus y14 y13.

20:36

So again this goes to e to the max

20:40

of 0 minus t13 minus t13 t14 minus t14

20:45

minus uh t13 t14 t14 t13. Okay, same

20:49

thing. Um then it's easy to see that

20:53

this thing is linear but it domains of

20:55

linearity are given by exactly that

20:57

picture.

21:01

Okay. So in this example

21:04

um

21:07

down here

21:10

down here T14 is negative T13 is

21:13

positive. So minus T14 is the biggest of

21:15

all of these guys. Okay. So down here

21:18

this is minus T14.

21:21

Here

21:23

everything is so negative that zero is

21:26

the max and here minus t14 minus t13 is

21:31

the max of everyone.

21:34

Okay.

21:46

Okay. So we have a few now we have a few

21:48

ways of uh we have a few things that we

21:51

can associate with this picture of the

21:52

Minkowski sum. There is the there's the

21:55

uh there's the fan associated with each

21:57

one. There are these polomials

21:59

associated with each sumand and there's

22:02

a tropicalization of the polomials uh

22:05

associated with each sum end. Okay. So

22:07

these are sort of three natural things

22:09

that we can associate with the uh with

22:12

these sums.

22:14

And these last points uh the the

22:17

polomials

22:19

and these tropicalizations

22:22

uh turn out to directly connect

22:25

these pictures to amplitudes.

22:28

Okay. And in fact let me just uh write

22:30

down the amplitudes that they uh that

22:32

they are associated with.

22:35

disguise

22:39

sorry.

22:44

So if I begin with the polomials

22:58

I write down an integral.

23:01

So this is I'm going to call this a5

23:04

going to be a five uh point amplitudes

23:06

but we'll interpret in a second. First I

23:08

write down an integral from 0 to

23:10

infinity with a form that's one of these

23:12

sort of infamous by now dlog forms. Okay

23:16

so our form is going to be a dlog form

23:17

on y13 and y14. Okay so y13 y14 the sort

23:22

of the variables here.

23:24

UM NOW THIS INTEGRAL BY ITSELF is

23:27

divergent obviously very divergent right

23:29

it's logarithmically divergent at zero

23:30

and infinity so are we going to repair

23:33

this integral to make it finite what

23:36

we're going to do in the neighborhood of

23:37

zero they're going to be factors that

23:39

are powers of y13 so y13 is going to go

23:41

to some power what power could it be

23:43

well the most natural thing is the x

23:45

that goes along with y13 and y14 will be

23:49

raised to the x14

23:51

right we have now successfully repaired

23:54

the singularities near the y's equals z.

23:57

But now these things are going to

23:58

diverge as y goes to infinity. If the

24:00

x's are positive, we fix things near x

24:03

equals z. Now they're going to diverge

24:04

as they go off to infinity. Right?

24:08

So to make them die in infinity, there

24:10

have to be some other factors that are

24:12

going to suppress things at infinity.

24:14

Okay? But in our problem, we now have

24:17

three interesting polomials at our

24:20

disposal. Right? We have these

24:21

polinomials associated with the sum. So

24:24

we're just going to write them down. We

24:26

have the polomial 1 + y14.

24:30

But remember if we go back to the

24:33

picture that uh uh Carolina drew this

24:37

mesh

24:39

this uh this was associated with that

24:42

sum end that was anchored to this mesh

24:45

point. Okay. So we're going to write 1 +

24:48

y14 to the power of the mesh that goes

24:51

along with it to the power of negative

24:53

c24.

24:56

This guy was this one. So we're going to

24:57

write down 1 + y13

25:01

to the minus uh c13.

25:04

And this was the uh triangle. So we're

25:07

going to write down 1 + y14 + y14 y13

25:12

to the c14.

25:15

Okay.

25:17

Now, notice that if the C's are positive

25:19

and the X's are positive, this

25:21

manifestly converges.

25:23

Just mindlessly converges, right?

25:26

Because we've saved it near X equals Z.

25:28

Well, actually, uh, sorry, doesn't so

25:30

mindlessly converge. Um, we've saved it

25:33

near X equals Z. It has a chance to be

25:35

saved near uh Y goes to infinity, but

25:39

obviously these C's can't be, for

25:40

example, you know, 10 the minus 100 if

25:42

the X's are 10. Okay. So, so the X's,

25:46

you know, have to have some positivity

25:47

property relative to the C's in order to

25:49

ensure that this converges everywhere.

25:52

Okay. And you can very easily check in

25:55

this example and it's true on very

25:56

general grounds that it's precisely when

25:59

X lies inside the pentagon as defined by

26:03

these mesh equations that this integral

26:05

is convergent. Okay.

26:09

All right. So, the integral is nicely

26:10

convergent. We have to have the x's are

26:12

positive, the c's are positive. On top

26:13

of that, we have to have x plus x - x

26:16

all of that stuff. Okay, that uh then

26:19

the integral is uh is uh then the

26:21

integral is uh the integral is

26:24

convergent.

26:25

>> Now this object yes

26:27

>> is the statement that if you move

26:29

anywhere slightly away it will diverge

26:31

or that this is a good this is one

26:33

positive

26:34

>> no no it'll diverge. I mean these

26:36

integrals will diverge if you're outside

26:37

the polytope they'll just diverge. So,

26:39

so the sort of polytope is literally the

26:41

the same as a domain of convergence of

26:42

the integrals. Okay.

26:45

Okay. Now, this is a slightly fancy

26:47

looking object. Okay. This is a slightly

26:49

fancy looking object. In fact, the x's

26:51

have units. They're momentum squared.

26:53

So, to make this a unitless statement, I

26:54

need to put something here that has

26:56

units of one over momentum squared or

26:58

length squared. So, these things uh

27:01

typically are called alpha prime.

27:04

Uh so alpha prime is just something

27:06

there to to to make this have correct

27:08

units

27:10

but um and we'll we'll talk about it in

27:12

a little bit more detail later but this

27:14

is in fact the five particle string

27:16

theory amplitude

27:22

right

27:24

[Music]

27:25

so it has this interesting extra

27:26

parameter alpha prime in it this is a

27:28

very interesting function of the x's is

27:30

a quite complicated function of the x's

27:32

that's meamorphic uh Uh so there's a lot

27:34

to say about string amplitudes we'll not

27:36

be talking about in uh uh in this

27:39

lecture but what I just wanted you to

27:41

see very quickly right away is that

27:44

starting from the picture of the

27:45

association of the Minowski sum the

27:47

Minowski sum is about string theory.

27:51

Okay, it's a Minowski sum picture that

27:53

immediately tells you how to write down

27:54

a string amplitude. You just take the

27:56

sum ends and shove them to the power of

28:00

what what appears in front of them. All

28:02

right. And this is something that is

28:04

going to give you uh uh string

28:07

amplitudes. Okay.

28:10

Now we can ask what happens uh to these

28:14

functions uh in the limit where the x's

28:16

where this combination alpha prime x is

28:18

tiny. Okay. So alpha prime has units of

28:21

a length. So saying that alpha prime x

28:24

length squared. So saying that alpha

28:26

prime x is tiny is the same as saying

28:28

the momenta are very small. Okay. So

28:30

this would be a low energy limit. Uh if

28:33

you're a string theorist, you would say

28:34

that in street theory, we have the

28:36

particles that we see and then there's

28:37

massive cousins, string excitations of

28:41

these particles whose mass is set by

28:42

that parameter alpha prime. If you go to

28:45

very high energies, you'll see all of

28:46

them. Uh uh very short distances, you'll

28:49

see the little wiggling strings. But at

28:52

very low energies and very long

28:53

distances, you're not going to see them,

28:54

and you're just going to go back to

28:56

seeing the good oldfashioned particles.

28:59

Okay,

29:01

so how can we study the very low energy

29:04

limit of this uh amplitude? Well,

29:07

clearly as alpha prime goes to zero,

29:10

this amplitude IS ACTUALLY GOING TO BLOW

29:12

UP. IT'S GOING TO blow up with some

29:14

power of 1 over alpha prime. After all,

29:16

the whole point of those exponents was

29:17

to regulate these integrals. Okay,

29:21

in fact, if we look at this integral,

29:22

NAIVELY GO LIKE ONE OVER ALPHA prime

29:24

squared, right? because there's going to

29:26

be a sort of a one over alpha prime from

29:27

every one of these uh uh integrations.

29:30

Conventionally, for that reason,

29:31

sometimes people multiply this by an

29:33

alpha prime squared out in front just so

29:35

we have something which is well defined

29:37

as uh uh as alpha prime goes to zero.

29:40

But regardless of that cosmetic thing,

29:42

um it's going to be dominated when alpha

29:45

prime is small. This is going to be

29:46

dominated by the extreme regions in this

29:49

y space either when the y's go to zero

29:51

or the y's go to infinity precisely

29:53

because we're barely regulating it.

29:55

Okay. So that's why as alpha prime goes

29:58

to zero.

30:00

Um

30:02

so this is a string of alpha prime.

30:10

But as alpha prime goes to zero

30:16

uh a string of alpha prime is going to

30:21

descend to a field theory or particle

30:24

theory which doesn't have an alpha prime

30:28

in it. Okay.

30:30

And what does that descion look like?

30:33

Well, I mean, if I go back to this

30:34

integral

30:36

and I use these variables where y13 is

30:38

eus t13, y14 is e minus t14,

30:43

then uh

30:48

then this is the integral over all t.

30:50

So, integral dt13 dt14. Okay, the y13 to

30:56

the minus x13 is going to look like e to

30:59

the minus uh I'm going to now put alpha

31:01

prime to one now since uh um uh it's

31:05

going to look like e the minus t13 x13

31:09

e to the minus t14 x14

31:12

and then e the minus c13 max of 0 and

31:17

minus t13

31:20

e to the minus uh uh c24 4 max of 0 and

31:25

minus t14 and then our favorite big guy

31:28

e to the max c14 0 - t14 minus t14 - t13

31:35

sorry for the small writing here right

31:38

so this is what this is what the uh

31:40

field theory amplitude becomes I mean

31:42

what's sorry this is this is the full

31:43

amplitude I haven't taken any limit here

31:45

right this is the uh full amplitude I

31:47

apologize but this is just the full

31:49

amplitude but now the point is that that

31:53

in the limit that we're talking about

31:54

this integral will be dominated by the

31:56

t's going to infinity. Okay. Oh, I'm

31:59

sorry. This is the limit. Sorry. Uh so

32:01

so what what uh in in taking the limit

32:04

the integral is dominated by where t's

32:06

go to infinity and where the t's go to

32:07

infinity we precisely replace the

32:09

polomials by these e to their

32:11

tropicalizations.

32:13

All right. So this is a different

32:15

expression than the expression that I

32:17

wrote down to begin with. The string

32:18

amplitude is some sort of fancy curvy

32:20

integral, right? With polomials and so

32:22

on in it. This is a simpler integral,

32:25

right? Again, now what's inside the

32:27

exponential is peacewise linear. Is not

32:29

linear, but is peacewise linear. Okay,

32:32

is this clear so far? Any any questions

32:34

about this? So, this is what the low

32:35

energy field theory limit looks like.

32:38

>> I think before you integrated from 0 to

32:40

infinity, now it's minus infinity.

32:42

>> Oh, because this was in the language of

32:43

the y's. So, the y's are from 0 to

32:45

infinity. So, the t's are from minus

32:46

infinity to infinity. Okay. So the t's

32:48

are from minus infinity to infinity.

32:50

Okay.

32:51

And now this integral actually has a

32:53

very beautiful uh interpretation

32:57

because exactly what we said before

33:00

remember what we said before is that

33:02

each one of those factors

33:05

you know so let's let's let's try to do

33:08

this integral. Well, obviously the

33:10

integral should be easy in some sort of

33:13

in some local region in tsp space

33:15

because each one of these factors is

33:16

just going to turn into something

33:17

linear. Okay, so let's just see where

33:21

each one of them is is is linear, right?

33:23

So where was this guy linear? So this

33:26

part of the that part of the uh

33:29

exponential looks like this.

33:32

That part is going to look like

33:35

uh what we figured out before. So, it's

33:36

going to look like C14 * minus T14 here,

33:41

right?

33:43

It's going to look like um uh C14 * -

33:48

T14 minus T13 here. And is going to look

33:52

like zero here. C14 * 0.

33:56

Okay,

33:58

so that's that factor.

34:01

What about this factor?

34:05

Well, that's peacewise linear in another

34:07

region. In fact, to see it, well, it by

34:09

alone, oops, that red thing

34:12

disintegrated. So, let's use this. So,

34:16

remember this factor alone

34:19

was uh

34:22

uh peacewise linear like in this region.

34:28

And obviously when P13 is is positive,

34:32

so I would add to this plus c13 * 0 and

34:38

when t13 is negative on this side I

34:40

would add to it plus uh c13 * negative

34:44

t13

34:48

and similarly

34:50

for the last guy well I'll draw it the

34:52

same same color here right

34:55

for the last guy then down here I would

34:58

have plus uh c24 * t24 T14 sorry and up

35:05

here I have plus C24

35:08

time zero

35:10

okay

35:12

oh sorry and I didn't write uh I didn't

35:14

write uh I should have written things

35:16

here so uh so um uh no sorry yeah this

35:20

is this is uh uh this is this is okay so

35:24

but I but but I should have uh uh

35:27

remember this C14 minus T14 minus T13

35:31

was valid in this whole region Okay. So

35:34

in this little corner uh I'm sorry I did

35:37

it precisely wrong. Uh uh so uh so uh so

35:41

from uh from C13 I have zero on this

35:44

side but I have negative uh C13 T13 on

35:47

this side. So here I'm going to get C14

35:51

* T14 and negative T13

35:54

and then plus C13 * negative T13.

35:58

Okay. And so on. Okay. So uh so um uh

36:03

okay so now now I have now I have the

36:06

whole plane is divided up into these

36:09

five regions that we get by putting all

36:11

the fans on top of each other and in

36:13

each one of these regions the integral

36:15

is linear. Okay so we can do the

36:18

integral.

36:19

Now the integral is easiest to do in

36:21

this region. Okay.

36:26

Um,

36:30

and I may have screwed something up

36:32

here.

36:34

Um,

36:42

[Music]

36:45

sorry.

36:49

[Music]

36:54

Oh, sorry. I precisely screwed up. I

36:56

screwed up at the very beginning.

36:57

Someone should have stopped me. Sorry. I

37:00

screwed up in writing this expression.

37:02

Okay.

37:04

Okay. So, if we have this guy,

37:08

okay, here is negative t14.

37:11

Okay. But here is zero. Okay. Because it

37:14

was max of zero. This was max of zero

37:17

and negative t13 and negative t13.

37:20

Negative t14 negative t13. Okay. So

37:25

that's zero here and here it's negative

37:27

t14 negative t13. Okay. Sorry. Okay. So

37:33

um so very good. So we erase that here.

37:37

But now we have to concmplyantly uh uh

37:41

erase it here. And here is where I

37:43

should have this uh negative t14 and

37:45

negative t13. Okay.

37:55

Okay. Anyway, so uh so so you see you

37:59

have an expression that's peacewise

38:00

linear in each one of these cones. And

38:03

now let's look at what it looks like for

38:04

example in this cone. This is the

38:05

simplest one in which we can do it.

38:07

Right? So in that cone what are we

38:10

getting

38:17

in that cone? We're getting the integral

38:19

0 to infinity.

38:28

We're getting the integral 0 to infinity

38:30

from this cone

38:33

of just dt13 dt14

38:37

eus x13 t13 eus x14 t14. All the c's go

38:43

away. And this is just equal to 1 /x13

38:46

1x14.

38:49

Right? And that's precisely the fineman

38:52

diagram that you'd associate

38:54

with the having these two chords x13 and

38:58

x14. Right? That's exactly the fineman

39:00

rule that we'd associate with that.

39:02

>> Sorry, why did all the C's go away?

39:04

>> Uh because in this region

39:08

the contribution from the C's was zero.

39:10

>> Okay. And so we always have the t x13

39:13

t13 x14 t14 on top of what I added. I

39:16

should have added that even there. But

39:18

that'll just be common linear factor

39:19

everywhere.

39:20

>> Okay.

39:21

>> Change the boundaries from minus

39:22

infinity to zero

39:24

>> because here this is only in this cone.

39:27

So now I'm going to do the integral. I

39:28

want to do the integral over all t's.

39:30

But now I've simplified my life to see

39:31

that in this cone it's linear. In this

39:33

cone it's linear. In each one of these

39:35

five cones it is linear. And so I'm just

39:37

going to do the integral over each cone

39:39

at once. Okay, in every cone it's

39:42

linear. And this is the easiest cone in

39:43

which I can do it. And what I get is 1

39:45

/x13 x14.

39:48

Now physicists call this trick for

39:50

representing 1 /x equals the integral 0

39:53

to infinity dt eus tx. This is called

39:57

swinger parameterization.

39:59

Okay, there's various nice physics words

40:02

associated with it. You can sort of

40:04

think about t uh as a as a length of a

40:08

propagator in position space. Okay. So

40:10

there's various nice words associated

40:12

with it. But it's just a way of

40:14

representing uh these uh these

40:16

propagators. So what we've seen is that

40:19

in this cone I get something that looks

40:22

like the swinger parameterization for

40:25

that diagram. Right? So the cone goes

40:29

with that cone is associated with that

40:31

diagram. And when we do this integral,

40:34

what we're getting is the Schwinger

40:35

parameterization for that diagram. And

40:38

the contribution from that cone is

40:39

precisely giving me the finding diagram

40:41

associated with that uh uh with the

40:44

corresponding uh

40:47

the integration over the cone is giving

40:48

me the amplitude uh that I'll get from

40:51

the the contribution of the amplitude

40:52

from the corresponding finding diagram.

40:55

You can easily check that the same thing

40:57

is true for all of the other cones.

41:00

Okay, it's maybe slightly interesting

41:02

like these cones don't look like the

41:05

standard positive cone for that formula

41:07

to be valid. But of course, you can

41:08

always do a linear transformation. You

41:10

know, the integral over this cone, I can

41:11

just do a linear transformation to bring

41:13

it to the standard form, which is the

41:15

positive uh uh the positive quadrant.

41:18

The integral over this little triangle,

41:19

I can do a linear transformation to

41:21

bring it to a positive quadrant. And

41:23

every one of those uh contributions ends

41:25

up being 1 /x 1 /x from the

41:28

corresponding diagrams.

41:30

Okay.

41:34

Okay. So let's just just pause and say

41:37

what what has happened. We have this

41:39

picture of the associ. We haven't I mean

41:41

well Carolina gave you a picture of

41:43

where it came from. We're now going to

41:44

we're now going to talk about where it

41:45

comes from in a more sort of primitive

41:48

uh principled way. But imagine you got

41:50

the uh the picture. The really magical

41:53

things that is presented as a Minowski

41:55

sum um uh in the language of the

41:57

polytope or in the language of the fan

42:00

that we have a fan that has cones that

42:02

cover all of space. Okay. All every cone

42:06

is associated with a particular

42:07

triangulation, a particular diagram.

42:10

Now that's already interesting. That's

42:12

already interesting that there's some

42:13

way to divide all of space naturally so

42:16

that into columns where each column

42:17

corresponds to a diagram. That already

42:19

sounds like progress. Okay. But uh

42:22

having done that, if someone told you,

42:24

well then go add up the shringer

42:27

parameterizations from every diagram,

42:29

you'd be this still sucks because I

42:30

still have to go cone by cone by cone

42:33

shringer parameterize for each one and

42:35

add them all up. That's basically doing

42:37

finding diagrams again.

42:39

But the fact that this sort of

42:41

complicated set of cones is secretly a

42:44

simple set of individual fans put on top

42:47

of each other tells you that there is a

42:50

simple peace-wise linear tropical

42:53

function that produces all this

42:55

complicated mass of refinement diagrams.

42:57

Okay. Now this small example was uh

43:01

maybe not small is maybe too small to

43:03

impress but it already illustrates the

43:05

point. There are five diagrams.

43:08

we have three tropical functions.

43:11

Okay, we did not have one function for

43:13

every diagram. Instead, it's the magic

43:15

of the Mowski sum picture, right? That

43:17

uh that was uh it was presented with

43:19

these sort of three uh simple fans on

43:22

top of each other. So, three tropical

43:24

functions were all you needed to produce

43:26

the five diagrams.

43:28

[Music]

43:30

Now what's going to happen in general

43:32

and that's what we're now going to see

43:34

is that not just at tree level but when

43:36

we generalize to all loop orders all

43:38

surfaces etc these two bits of magic

43:41

always happen. So first there's a way of

43:45

uh uh getting into the the space of the

43:48

appropriate dimension and seeing that

43:50

it's naturally divided up into cones and

43:53

each cone corresponds to a diagram but

43:56

you don't manually have to sort of you

43:58

know make them it's it's just going to

44:00

come out of the box. We're going to make

44:01

we're going to figure out how to hand

44:02

you a bunch of vectors such that the

44:04

cones made out of them are automatically

44:06

going to correspond to diagrams. That's

44:07

going to be small miracle one.

44:10

Bigger miracle too is that there are

44:13

some functions associated uh to these

44:16

pictures as well. There are polomials as

44:19

we saw here and there are

44:21

tropicalizations. Okay. So there they

44:23

both have an interesting role to play.

44:27

These are going to be few of these

44:29

polomials. So just give you a just so

44:32

you have an example in mind. If we're

44:34

talking about tree amplitudes

44:36

asmtoically the number of finding

44:37

diagrams the number of triangulations

44:39

are given by cataline numbers and

44:42

cataline numbers grow like four to the n

44:44

if you have an n going okay so the

44:46

number of fineman diagrams are growing

44:48

exponentially

44:50

however we're going to give about n squ

44:53

tropical functions we're going to give

44:55

about n^ squ polomials there's going to

44:57

be a polomial associated essentially

44:59

with every point in that mesh right or

45:02

there's going to be a polinomial

45:03

associated with every every uh one of

45:05

these xigs at every one of these igs

45:08

there's going to be a polomial and the

45:09

polinomial will have at most n terms in

45:11

it okay so I'm going to hand you around

45:14

n squ polomials each one having at most

45:16

n terms all right

45:20

no four to the n here so clearly I'm not

45:23

summing over all diagrams right the sort

45:24

of magic is I'm going to give you n squ

45:26

polinomials with about n terms each

45:28

first of all if you shove those

45:30

polomials in to the integral d y y y y y

45:32

y y y y y y y y y y y y y y y y y y y y

45:32

y y y y y y y y y y y y y y y y to the X

45:33

product of all the polinomials so

45:35

they're minus C that will define string

45:36

amplitude

45:38

okay without your string theory of

45:40

course

45:42

uh and secondly if you tropicalize those

45:45

expressions in just the way that we

45:46

talked about that will give YOU A GLOBAL

45:49

SWINGER PARAMETERIZATION FOR ALL THE

45:51

diagrams together at once. Okay, but

45:53

again the magic is there will be order n

45:56

square tropical functions each one of

45:58

which has a max of order at most n

46:00

things

46:02

very small number but if you put them

46:04

all on top of each other the domains of

46:06

linearity of all of these guys

46:08

exponentiate right and generate this

46:10

humongous complexity of all the diagrams

46:12

together right this is a second magical

46:14

fact a more magical fact both the

46:17

existence of the polomials and the

46:20

existence of uh and the fact that Well

46:23

anyway the the existence of the

46:24

polinomials is the essential fact and

46:26

the tropicalization is this sort of as

46:27

this very beautiful interpretation as

46:29

giving you cone by cone the shringer

46:32

parameterizations for each diagram but

46:33

in a global way that combines them all

46:35

together. Okay. The point is that these

46:37

peace-wise linear functions morph into

46:40

the swinger parameterization for every

46:42

diagram as you move around the cones

46:44

without doing any manual work. Right?

46:47

And it's literally this this difference

46:49

between polomial versus exponential

46:51

complexity. sort of polinomial uh

46:53

complexity in exponential uh complexity

46:56

out. All right. So those are the things

46:58

that I now want to explain where these

47:00

things uh where these things come from.

47:02

Before doing that, let me mention a

47:04

final thing that we can see in this

47:06

example. Okay. Final thing we can see in

47:08

uh in this uh uh example

47:12

that's also going to uh also going to

47:15

play a sort of starring role.

47:18

Um

47:35

and this is the existence of something

47:36

that I'll give some whimsical names to

47:38

and then an official name to.

47:44

But let me start with the more uh

47:46

whimsical name. Remember, part of the

47:48

part of what the esocahedron does

47:52

is if we drew this picture,

47:55

of course, it captures all of the uh it

47:58

captures all of the

48:03

all the compatible uh uh chords and so

48:06

on. But a sort of very minimal thing uh

48:09

that it does is it keeps apart things

48:12

that cannot cross. Right? That's the

48:15

point that that that we can't have 1 13

48:18

and 25. They cannot occur together,

48:21

right? The chords cross. The chords 1

48:23

three and 25 cross. And so part of the

48:25

job of the association is to keep them

48:26

apart, right? So 1 13 and 25 do not

48:29

meet. Okay? 35 and 1 cross. So 35 and 1

48:33

do not meet. Okay? Of course, it does

48:36

more. The the things that do meet have

48:38

the correct combinator. They all meet

48:39

the way they should and so on. But but

48:41

the most zero order thing that it does

48:43

is keep things apart. That's very

48:46

beautiful that we can do that in this

48:48

sort of polytopal way. But you'll also

48:50

notice that it's kind of uh it's not

48:52

entirely rigid, right? I mean, of

48:54

course, I can move these faces around

48:56

parallel to each other in various ways.

48:58

So it's not entirely god-given. Okay,

49:02

there is a more god-given object which

49:05

does exactly the same thing that you can

49:07

call these are the whimsical words you

49:09

can call a curvy associ

49:14

we sometimes call binary geometry

49:21

and okay it's also positive coordinates

49:24

for tech space but I get I fall asleep

49:27

by the middle of that sentence okay so

49:29

uh okay so um uh so it's related to

49:32

compactifications of technular space in

49:35

some way but if you don't know what what

49:37

that is uh that's more than fine by me

49:39

okay so um okay so um so what is this

49:44

doing so there is something uh there is

49:46

something uh interesting here remember

49:48

what the conventional sort of flat

49:50

associed this is polytopal this is cut

49:52

out by linear equations what the

49:54

conventional flat associed is doing

49:57

amongst other things is keeping things

49:58

apart

50:00

And so we do that by well we associate

50:02

these variables x's with them and so on

50:05

right so the flat associed

50:07

then on on this side

50:10

the flat associated for every so our you

50:13

know we have chords we have some chords

50:16

I j

50:18

chords kl they want to be kept apart

50:20

from each other when they cross and so

50:22

on in the flat association we associate

50:25

these things with variables xig and then

50:27

there's some there's the association as

50:29

a polytope

50:31

that's cut out by equations involving

50:33

these X's. So this is the flat associed

50:36

world.

50:40

In the curvy world

50:43

or non nonlinear world,

50:46

every one of these chords is associated

50:48

with another variable we call UIJ.

50:52

Okay?

50:56

But we're not going to write down

50:57

inequalities and things like that for

50:59

them. Instead, these UIJs are going to

51:01

satisfy the following set of very

51:03

interesting nonlinear equations.

51:06

UIJ plus the product over all chords KL.

51:20

Right

51:22

now I'm just writing these equations

51:23

down. Okay. again we'll understand

51:25

better where these things come from.

51:27

Okay.

51:28

But let's say just out of the box I

51:30

handed you uh an equation that looks

51:32

looks like this. Well, what's your first

51:35

reaction to this uh uh equation? Let's

51:38

try writing it down at five points.

51:41

Okay. So at five points

51:46

very simple

51:53

at five points we have that uh so let's

51:56

draw our our our our five gone. So I

52:00

have like the equation for U13. So U13

52:04

plus the product of all the chords

52:06

across 13. So who are the chords across

52:08

13? There's 2 4 and 2 5. Those are the

52:12

only ones that cross 13. So U13 plus U24

52:15

U25 is equal to 1. Okay.

52:20

And then we have the cyclic friends of

52:22

this guy, right? So we have plus uh uh

52:24

U24 plus U 35 U13 = 1 and so on. Okay.

52:30

So we have a total of five equations.

52:36

Okay.

52:38

So without thinking, YOU THINK YOU HAVE

52:39

FIVE EQUATIONS, FIVE UNKNOWNS. This has

52:42

some solutions and points. Okay,

52:46

the interesting thing is it doesn't have

52:47

solutions and points. It has a full

52:49

two-dimensional space of solutions.

52:51

Okay, these equations have a full

52:53

interesting two-dimensional space of

52:55

solutions. For example, a natural thing

52:58

you could do this does this turns out

53:00

not to generalize very easily. Okay, but

53:02

one thing you could do in this example

53:04

is to just choose two of the U's and

53:06

solve for the rest of the U's in terms

53:08

of them. For example, you can find that

53:10

uh U25

53:12

is uh is 1 - U13 U14. If you just solve

53:17

these equations, u35

53:20

is uh

53:22

1 - U14 over 1us U13 U14. and u uh

53:29

24 is 1 - u13 over 1 - u13 u14. Okay, so

53:35

this is one way you could solve the uh

53:37

equations. All right, you can just check

53:38

that that's uh you can just check that

53:40

that's true. All right,

53:43

but what's interesting about these

53:45

nonlinear equations? Uh why do we call

53:48

it a curvy association or binary

53:50

geometries? What's that word binary?

53:54

Again, it has to do with the word

53:55

positivity

53:57

because we ask for real positive

54:00

solutions of these equations. Okay? So,

54:02

I'm going to ask for the what happens

54:04

when the uj are greater than or equal to

54:07

zero. What happens if the uj are greater

54:09

than or equal to zero?

54:12

These equations then tell us not just

54:15

these but but in general remember in

54:17

general we're writing down uj plus the

54:20

product over kl of u kl is equal to one

54:24

right so these equations are telling us

54:29

uh that if the 's are positive if the

54:32

sum of two positive numbers adds up to

54:34

one they all also have to be less than

54:35

one

54:37

right all right so all these 's have

54:40

also got to be less than with the one.

54:43

Okay,

54:44

that's where the word binary comes in.

54:47

And now they have an interesting

54:49

property. Suppose a given u like a given

54:52

ui star jar some ui star jar. Let's say

54:55

this heads to a boundary of the space

54:57

where this goes to zero.

55:00

By the dent of these equations,

55:03

all of the u's that cross it must go to

55:05

one.

55:07

Okay. So the U KL for KL crossing

55:15

I star J star

55:18

have to go to one.

55:21

Okay.

55:24

That's remarkable. If you think about

55:25

hitting the boundaries of the space

55:26

corresponding to U's go to zero. You see

55:29

THIS IS DOING EXACTLY what the is

55:30

associed is doing. It's keeping apart

55:33

things that cross,

55:36

but it's keeping them apart in an

55:38

entirely rigid way. There isn't any

55:40

parameters that you can move around.

55:42

These variables are from 0 to one. And

55:44

when you go to a boundary uh for one

55:47

chord, all of the chords that cross it

55:49

just go to one. Okay.

55:54

All right.

55:57

Okay. So now this turns out to exist. uh

56:01

these variables exist uh uh at at tree

56:05

level for the case that we're talking

56:07

about. Again, all of this generalizes to

56:08

all all all surfaces in interesting

56:11

ways. You draw any surface, there is a

56:14

chord uh there's a variable associated

56:16

with any open curve on the surface and

56:19

you write down in general if you have a

56:21

uh a curve x on the surface, you write

56:24

down this formula, the product over all

56:25

other curves of the u for the y and it's

56:28

raised in general to the number of times

56:30

the curves x and y intersect each other.

56:33

Okay, so that's just a sneak peek.

56:35

That's the that's the equation. It's a

56:37

sneak peek because uh I I like to say if

56:39

I if I had to hand someone, you know,

56:41

one fact and tell them to go to a desert

56:43

island and work out what I did for the

56:45

last 5 years of my life, that would be

56:46

what I would do. Just hand them that

56:47

that equation, say go, right? And then

56:50

then just studying that equation would

56:51

lead to all the things that we're about

56:53

to talk about. All of it is in

56:55

understanding uh how that equation can

56:57

be true and and how to solve it. Okay?

56:59

Uh we'll see how much we we get to this

57:01

uh uh in uh later in this lecture, but

57:05

okay. Okay. But so so it's true not just

57:07

at tree level, it's true for all all

57:09

surfaces.

57:12

But what's especially interesting about

57:13

it is we know how to solve them. Okay.

57:15

There's a way of solving these uh these

57:18

equations and the U's are given as

57:20

ratios of polomials. Right? So let me

57:22

tell you what this ratio of polinomials

57:24

looks like for our uh pentagon example.

57:40

For instance, uh we find that uh that

57:43

that u's are parameterized in terms of

57:45

some positive coordinates y. Okay. And

57:50

the formulas are that u13 is y13 over 1

57:53

+ y13

57:56

u14.

58:37

Okay. And I just invite you as a little

58:38

exercise to check that these satisfy U

58:41

plus UU equals 1. Okay. So for instance

58:45

if we take u13

58:47

plus u24 u25

58:50

okay this is u13 is y13 over 1 + y13

58:56

but u24 u25 there's a nice telescopic

59:00

cancellation of that factor and this

59:02

factor and we're left with 1 over 1 +

59:04

y13

59:06

and this is dutifully equal to one.

59:09

Okay.

59:11

So you see we're solving these U

59:13

equations. We're solving these U

59:15

equations in terms of these interesting

59:17

polomials.

59:18

Now notice those are exactly the

59:20

polomials that showed up in our previous

59:22

picture. Okay?

59:25

They're precisely the polinomials that

59:27

showed up in our uh Mikowski summaries.

59:30

So let's summarize what we saw in this

59:32

example that we're now going to give a

59:34

rational uh uh uh explanation for. Okay.

59:38

We started with the socedin.

59:40

The simple case there was a pentagon. We

59:42

drew the dual fan associated with it.

59:45

The fan has the feature that it divides

59:48

the space up into cones. Every cone

59:49

corresponds to a triangulation or a

59:51

diagram. Okay. The fact that the

59:55

association has a main sum decomposition

59:57

is reflected in the fact that the fan

60:00

even though it has five pieces is

60:02

naturally thought of as sort of putting

60:03

three simple pieces simpler pieces on

60:05

top of each other. And that three versus

60:07

five distinction gets much more dramatic

60:09

at at higher points. Okay, there is a

60:11

small number of pieces each one of which

60:13

looks like the fan of a simplex which

60:16

when you put them on top of each other

60:17

order n squared pieces where you put

60:19

them on top of each other generates the

60:21

horrendous complexity of all the 4 to

60:23

the n uh fineman diagrams.

60:27

Okay. uh there is this simple integral

60:30

that you write down just integrating

60:32

with the dlog form in the uh uh uh so if

60:36

we can then associate polomials with

60:38

each one of these uh sumands there's a

60:41

simple integral that we we can write

60:42

down with the dlog form uh y to the x

60:46

and all the polomials raised to the

60:48

power of their coefficients in the

60:49

sumand that gives us the string

60:50

amplitude. If we take the low energy

60:54

limit of this, we simply tropicalize

60:55

this integral and that's interpreted as

60:58

the global shinger parameterization a

61:00

way of combining all the finding

61:02

diagrams together in a uh single object

61:05

so that cone by cone we get the

61:07

contribution from the diagram but

61:08

without having to invent the diagrams

61:10

right they all sort of come out

61:12

and these polomials themselves are

61:16

associated with this interesting notion

61:17

of a binary geometry this much more

61:20

rigid way of associating creating a

61:22

geometric object with the combinotaurics

61:24

of triangulations of an engon. Okay,

61:27

there's a sort of curvy version of the

61:29

ocosahedron where there's no moduli,

61:31

there's no parameters, it's just zeros

61:33

and ones, right? But with every variable

61:35

you associate a u this interesting u

61:38

equations um which have the feature that

61:41

uh when when when you approach

61:43

boundaries um

61:45

uh when you approach boundaries uh the

61:48

um

61:49

uh 's go uh uh when 's go to zero all

61:53

the crossing chords uh go to one. In

61:55

fact, I'll mention one last thing here

61:58

to just close this example.

62:01

I'm going to go back and write the

62:02

string amplitude again. You remember the

62:05

string amplitude was written in terms of

62:06

these polomials and but the 's are some

62:09

interesting uh you know uh just

62:12

combinations of these polomials upstairs

62:14

and downstairs.

62:16

So I'm going to go back and I'm going to

62:17

write the string amplitude directly in

62:20

terms of these u's where they look much

62:22

more elegant.

62:24

So that string amplitude again is still

62:26

this dlog form. It's still the integral

62:28

0 to infinity. d y13 over y13

62:32

d y14 over y14.

62:36

Okay. But all of the rest of the stuff

62:38

that we had before just turns into the

62:41

product over all chords u j the u

62:44

variable to the power of xig.

62:52

That's what the string amplitude is. See

62:54

this is a much more elegant form.

62:58

This form makes it makes uh a number of

63:02

things uh obvious. In fact, it makes all

63:04

the qualitative and quantitative

63:07

features of the amplitude uh obvious.

63:10

For example, it makes it obvious that

63:12

the only singularities again this this

63:14

is this is a dlog form. Um the a sort of

63:17

cool thing is to show that this is a

63:18

dlog form that has logarithmic

63:20

singularities everywhere the 's and any

63:22

of the 's go to zero. Okay, that's a

63:24

small extra step that's not hard to

63:26

prove, but just just uh by that. Okay,

63:29

so anywhere. So this integral is only

63:31

going to develop singularities in the

63:33

neighborhood where some u's go to zero.

63:36

That might be at zero or infinity and y.

63:38

It doesn't matter sort of invariantly.

63:39

It's only developing singularities as

63:41

the u's go to zero. So what's rescuing

63:43

it is its power, right? So that's why

63:47

we're going to have poles that look like

63:48

one over xig

63:50

uh as some of the xigs go to zero. Okay,

63:53

so that's the sort of first thing which

63:54

is obvious. That was our locality,

63:56

right? Where are the poles where the x's

63:58

go to zero? Okay, where we're seeing

64:00

that. Okay, so we're going to have a

64:01

pole as xig goes to zero. As some xig go

64:05

to zero, this amplitude will go like one

64:07

over xig.

64:09

Okay, but now comes the real magic.

64:12

What happens to this factor at a given

64:14

uh xig goes to zero. Let's say given

64:16

again x i star jar goes to zero. Let's

64:19

imagine drawing a big n gone. This is

64:21

going to be true for any n right? So

64:23

let's imagine here's my chord iar jar

64:28

and this xig is going to zero.

64:32

That means that this integral is being

64:34

localized in the neighborhood of where

64:36

the corresponding u iiar jar goes to

64:39

zero.

64:41

So what happens to this factor, right?

64:43

Well, we're going to pull out of it some

64:45

u i star jar to the x i star jar. That's

64:49

a factor that's coming out of all of

64:51

this. That's in fact exactly the factor

64:54

that's getting slightly rescued by the

64:56

non-zero x to give me something that's

64:58

going to be 1 /x and is getting uh

65:00

regulated. Right? That's that's my my

65:02

poll. But what about everything else?

65:05

Well, notice all this chord divides the

65:08

the uh the uh the engon naturally into a

65:11

left part and the right part.

65:14

But all of the U's that correspond to

65:16

chords crossing here are going to one.

65:20

Right? That's the point. When a U goes

65:22

to zero, all the chords that cross it go

65:25

to one. So in this product, all of the

65:29

pieces that are a U to the^ of X

65:31

corresponding to something that crosses

65:33

are going to one.

65:35

So what we're left with is just this

65:37

factor that pulls out times the just a

65:39

product over the left of u to the x left

65:44

and a product over the right of u to the

65:46

x right.

65:49

This is factorization.

65:51

This is precisely the phenomenon of uh

65:56

uh

65:58

factorization. Okay. Because then it's

66:00

very easy to see that this form also

66:02

just splits. There's the part associated

66:04

with that going to zero and the rest of

66:06

it splits into a product on the left and

66:08

the right and therefore the whole

66:09

amplitude goes to this times the

66:12

amplitude on the left and the amplitude

66:14

on the right and in fact this has

66:17

nothing to do with taking the low energy

66:18

limit. This is a full exact property of

66:20

the full string amplitude which is one

66:23

of the things that makes string theory

66:24

consistent. Okay, even beyond field

66:26

theory. Right? So I hope you see very

66:29

vividly in this example the the uh the

66:33

kind of abstract discussion from

66:35

yesterday right we start with a picture

66:37

there's maybe Carolina started with a

66:39

mesh

66:41

some funny wave equation in this mesh

66:43

space uh you get a polytope you know you

66:46

you're following your nose I hope it's

66:48

clear at no step are we cheating on

66:50

looking at finding diagrams at the end

66:52

of the book right there's nothing like

66:53

that going on okay but then we're sort

66:55

of after a few steps we'll naturally let

66:57

to this object object. This object does

67:00

everything that fine diagrams do but

67:02

without having any reference to particle

67:04

trajectories or anything like that.

67:06

Okay, in fact the sort of stars of the

67:08

show here are variables associated with

67:10

like chords in this engon. Right? And

67:13

remember those chords in the engon are

67:15

related to the kinematic variables. The

67:16

kinematic variables are also associated

67:18

with chords on the uh on the engon.

67:21

Right? Okay.

67:24

All right. So, okay, let's uh pause now

67:27

and I'll ask if there's uh any

67:29

questions. Um, yes.

67:32

>> So, these U and Y variables, are they

67:35

somehow related to some cluster variet?

67:38

>> They're related to uh they're they're

67:40

related, but they're not precisely in

67:41

cluster variables for a variety of

67:43

reasons. Surface cluster algebbras are

67:45

not quite what is needed in this story.

67:47

They're close, but not exactly.

67:50

[Music]

67:51

Yes, they're they're more closely

67:53

related if you know they're more closely

67:55

related to uh uh fakoner coordinates,

67:57

but they're also not precisely that or

67:59

there's a very special set of fontro

68:01

coordinates that do this uh job. Okay,

68:03

but part of the point uh of these

68:06

lectures is to not assume that you know

68:08

fancy things and just you know build it

68:10

from the from the from the ground up. So

68:12

in the next uh 50 minutes we'll sort of

68:14

see where these things come from from

68:16

the ground up. Yes. Super. So you were

68:18

speaking about how it is uh uh

68:20

surprising that this tropical

68:22

representation exists for the uh for the

68:24

>> yes

68:25

>> uh full amplitude in one finger

68:27

parameterization.

68:28

>> Yes. So I wanted to ask so suppose I I

68:31

start doing this I uh instead of looking

68:34

for positive geometry

68:35

>> yes

68:35

>> I take some some new theory some

68:38

different theory and ask oh does it have

68:40

a global swinger parameterization for

68:42

example I think Bruno has some papers

68:44

where they have found

68:45

>> global swinger parameterization but in a

68:47

different structure than

68:48

>> yes I think everywhere we have global

68:50

swinger parameterization there is some

68:52

interesting uh positivity behind it okay

68:55

there are some there are some positive

68:57

parameization some set of polinomial

68:59

that you can in the end interpret as

69:01

giving you uh this picture of naturally

69:03

a bunch of Mowski sum ends that are

69:05

summing up to a complicated geometry.

69:06

That's the universal thing in all the

69:08

examples that that that we see so far.

69:10

And all the examples also have stringy

69:12

integrals that go along with them. Okay.

69:14

So there's extensions Nick Bruno uh

69:18

others have talked about uh uh uh CGM

69:21

theories and so on. um and uh uh the the

69:25

original motivation for those things

69:26

came from the chy formalism but in fact

69:29

there's fully stringy versions of them I

69:31

mean so it's uh it's not restricted to

69:33

the field theory limit and from my point

69:34

of view that's a more natural way of

69:36

thinking about what what they are so

69:37

that's

69:37

>> from the perspective of positive

69:38

geometries is some qualitative

69:40

difference in finding it through a

69:42

positive geometry or finding or are this

69:44

just equivalent completely

69:46

>> well I mean uh all I can say is that if

69:48

you is that um I don't know what to say

69:52

in I don't know what to say in in in

69:54

general. Um uh maybe maybe here is uh

69:57

the here is a place to uh to perhaps say

69:59

it. Um so uh so first of all uh

70:03

everything that I've been talking about

70:04

here is in the context of uh of the

70:08

trace cube theory. Okay. So the only

70:10

dependencies on simple scalar kinematics

70:13

um and we have expressions that look

70:16

like this like literally this this

70:18

expression. Sorry if we do this. This

70:20

was meant to be a general end. So this

70:22

would be some maybe dy13 up to dy1n. I

70:26

I'll say what this means in a moment.

70:27

But anyway, some some expression like

70:29

this is is uh is true. Um and so you

70:32

might think this is very special to the

70:34

trace 5 cube theory. Can you do this for

70:35

trace 5 to the fourth theory? No. Okay.

70:37

There's nothing sort of huh

70:39

>> n minus one.

70:40

>> Uh this is uh this is actually n minus n

70:43

minus one. Thank you. Okay.

70:46

uh you might think that uh anyway can we

70:48

do it for trace fun theory some other

70:50

theory no okay so uh at least not not in

70:53

uh any obvious way but one of the

70:55

surprises of the past few years is that

70:57

literally these functions just slightly

71:00

reinterpreting what you mean by the x's

71:02

if we take the x's and just shift the

71:04

x's in some simple linear way um take us

71:08

from describing the amplitudes for trace

71:10

cube which is a don toy model that maybe

71:12

none of us care about to describing real

71:15

world particle physics. Okay. So you

71:17

shift these amplitudes in one way. You

71:18

you shift these functions in one way. I

71:20

literally mean shift. I mean doing

71:22

nothing to them. Just reinterpreting

71:23

what you mean by X. Okay. Uh you just

71:25

just shift X goes to X plus some

71:27

constant depending on what I and J are.

71:30

And then all of a sudden you have the

71:31

amplitude for pi out which are some of

71:33

the particles associated with the strong

71:35

interactions. And if you do it literally

71:37

in this way at finite alpha prime uh and

71:40

shift x by a single unit x goes to x +

71:44

one x plus or minus one one over alpha

71:47

prime then this thing turns into the

71:49

scattering amplitude for gluons real

71:51

gluons. Um and unlike the story of

71:54

therin, this has nothing to do with

71:56

super symmetry. The words n equals 4,

71:58

superyang mills, etc. make no

71:59

appearance. This is for totally

72:00

non-supery symmetric gluons. And at loop

72:04

at loop order, they're loop order for

72:06

totally non-supy symmetric gluons. Okay,

72:08

these second two statements are a much

72:11

bigger surprise that somehow that this

72:13

uh seeming dumb uh toy model contains in

72:17

it

72:19

uh theories we care about a lot more.

72:22

And actually some of the surprising

72:23

properties that Carolina was mentioning

72:25

this morning that these amplitudes have

72:26

surprising zeros and they factoriize in

72:29

surprising ways in the neighborhoods of

72:30

these zeros they in fact port to all

72:32

these other theories too. Okay. So the

72:34

the theory of pions and of gluons have

72:36

exactly the same mysterious properties.

72:38

That's actually how with Carolina and

72:41

Jyn and friends we were left to discover

72:42

these things backwards. We ran into the

72:45

zeros. Then we observed just

72:47

experimentally the zeros were also there

72:49

for other theories that we cared about

72:50

more which is very surprising. Why the

72:52

hell? Those theories were not related to

72:54

the association. We didn't think. Well,

72:56

we were wrong. They are right. It's

72:58

exactly the same function shifted in

73:00

this interesting way takes us between

73:02

all these different theories. So, this

73:04

is maybe a kind of example of what

73:06

you're saying. Had you told me abonio

73:08

ahead of time, take the diagrams for the

73:10

nonlinear sigma model that describe

73:12

pounds and try to put them together in

73:13

shrinking parization. That's good luck,

73:16

right? That's a total disaster. I would

73:18

never try doing that in a million years.

73:20

And I would also not think in a million

73:21

years that all I had to do was go back

73:23

to this example and do some stupid shift

73:25

on the x's in order to get the right

73:26

answer. Never mind that I could do the

73:28

same thing for gluons which is utterly

73:30

shocking right that I would never

73:32

thought. So somehow that's the nature of

73:34

the beast in this business is it does

73:37

not commute with responsibility. I don't

73:39

know how to say it but uh but you want

73:41

to like do something say I'm going to

73:43

take every fineman diagram and you know

73:45

figure out how to put the numerators in

73:47

and shringer parameization then globally

73:49

swinger parameterize it. People have

73:51

tried to do that with some degree of

73:52

success but somehow does not have the

73:54

same you know remarkable striking

73:57

feature as what naturally comes out when

73:59

you pursue what the mathematical objects

74:02

want to do on their own terms. Okay. So

74:05

that's uh that's why I don't have a

74:06

general answer to give to your to your

74:08

question that

74:10

okay any other questions. Yes.

74:14

>> Uh I didn't quite understand why when

74:16

you set the xig to zero yes but also the

74:18

uj went to zero.

74:19

>> Oh yes because the the the the point is

74:22

uh remember if I didn't have this factor

74:24

at all this integral is very divergent.

74:26

Okay is logarithmically divergent both

74:28

on the y's go to zero and they go to

74:29

infinity. Okay. what this factor now it

74:33

turns out that the y is going to zero

74:34

and infinity in fact where this form has

74:37

a logarithmic divergence is in onetoone

74:39

correspondence with where the 's vanish

74:41

okay so so where this thing develops a

74:44

logarithmic uh singularity are where the

74:48

's vanish

74:49

now the x's are there to ensure that you

74:51

nonetheless get something finite right

74:53

it's like integral sorry maybe I should

74:55

have said this but this is just saying

74:57

you know integral zero to whatever d y

75:01

is log zero is infinite but dy y y y y y

75:04

y y y y y y y y y y y y y y y y y y y y

75:04

y y y y y y y y y y y y y y y y to the a

75:05

is 1 / a plus dot dot dot, right? So

75:09

just the point is that these little

75:10

exponents save the integral, right? They

75:13

make it convergent, but as that exponent

75:15

goes to zero, this integral develops a

75:18

pole.

75:19

Okay, so if we go back here, if a given

75:22

xigj goes to zero, there's a region in

75:26

this space that's going to have a

75:27

logarithmic divergence when the u goes

75:28

to zero, when the u for it goes to zero.

75:30

Okay, if the xig is not quite zero, the

75:33

amplitude will be dominated by this

75:35

neighborhood, it'll get a factor of 1

75:37

/xig and the rest of the integral will

75:40

be what you get from the other parts of

75:42

the integration uh in the neighborhood

75:44

of where that u goes to zero. And

75:46

because of this sort of magic fact that

75:47

as a given u goes to zero, all the u's

75:49

that cross it go to one. The rest of the

75:51

integral just dutifully factorizes.

75:54

Okay, so what you're left with is just

75:55

the product on the left and the product

75:56

on the right. Okay, I I want to stress

76:00

again this is qualitatively different

76:02

from where factorization comes from with

76:04

the picture of space-time processes and

76:06

fineman diagrams. Okay, and this

76:09

qualitative difference is related to

76:10

what may have seemed like a like a sort

76:12

of two vague uh remark yesterday that

76:16

it's the tuness of the pi.pj versus the

76:19

oneness of the pis that matter. See, the

76:21

fineman diagrams are all about oneness.

76:23

You know, you have a bunch of momenta

76:24

coming in. you're keeping track of the

76:26

momentum of the particles. Then there's

76:27

a propagator that's the sum of all those

76:29

momenta and it goes from from from here

76:32

to there. Right? So that's how finding

76:33

diagrams make manifest that

76:35

singularities are associated with

76:36

propagators.

76:38

This picture does not ever see single

76:41

indices. This picture is all about pairs

76:44

from the beginning. It's all about

76:46

pairs. It's about curves on the surface.

76:48

It's all about pairs. And therefore the

76:50

way it manifest factoriization looks

76:52

nothing like a particle propagating and

76:54

going on shell and cutting the picture.

76:56

It's just some something totally

76:57

different. It's this binary geometry.

77:00

Okay. And that's again a concrete

77:02

instantiation of this uh general fact

77:05

we've seen over and over in this

77:06

business of the existence of natural

77:08

geometric objects that factoriize on the

77:10

boundaries for their own private reasons

77:12

which don't uh don't on the face of it

77:15

have anything to do with particles going

77:17

on shell in space time. Yeah.

77:21

>> Okay. Any other questions? Yes.

77:23

>> In terms of complexity reduction. Yes.

77:26

>> So from going to four to the end

77:27

diagrams to do some note that this is

77:30

the you can do.

77:32

>> Uh I would be surprised if you could do

77:34

better, but uh I'm not sure. Yeah, I

77:36

mean it's it would be very interesting.

77:37

It would be and and just to maybe make a

77:41

point um uh uh whether we get there or

77:44

not. I hope now you can see why this way

77:46

of thinking offers some hope for uh

77:49

asking what happens when the number of

77:50

particles goes to infinity. Okay?

77:53

because we're going to have an integral

77:54

of something which is e to the minus

77:57

some peace-wise linear expression which

77:59

is not that complicated. It's a sum of

78:01

sort of n square pieces each one of

78:03

which is a max of things that involve

78:05

order n things. Of course, you're doing

78:06

an order n dimensional integral but it's

78:10

a single integral. It's a single

78:12

integral over one space that somehow

78:14

something nice should happen in the

78:16

large end limit. Okay, so that that's

78:18

not insane that something like that

78:19

should happen. And in a very precise uh

78:22

uh sense, what happens is that these

78:24

peace-wise linear things smooth out and

78:26

that uh the large end limit is a much

78:28

smoother object than you would naively

78:30

think from putting all these maxes uh on

78:32

on top of each other. That smoothing

78:34

phenomenon is a very interesting one

78:36

which if we get to it tomorrow uh uh

78:39

we'll uh talk about.

78:41

All right. So I have uh 40 minutes. 40

78:44

minutes. That's challenging. But let's

78:47

see what what what we can do. So now I

78:48

want to tell you where these things come

78:50

from.

78:52

Now first off, we're going to go back um

78:56

uh to this picture

78:58

where we sort of think that we have a

79:00

you know we have a scattering process.

79:02

But we already learned let's go back to

79:05

the case of the pentagon

79:08

that we can we can uh we can think about

79:10

this uh five particle tree amplitude in

79:14

terms of a triangulations of uh of a

79:17

fivegon or an engon uh in general. Okay.

79:21

And the kind of first way was the way

79:23

that uh uh Carolina mentioned in her

79:26

talk that we could sort of draw a duo of

79:28

this triangulation. And the duel of the

79:30

triangulation looks like uh you know

79:32

looks like the diagram that we had

79:34

talked about. There's a closely related

79:36

way of thinking about this which is uh

79:39

which is which is uh somehow deeper

79:43

and this has to do with going all the

79:45

way back to um uh to these being colored

79:48

particles. Okay. And in our three

79:50

discussions of color today only at the

79:52

very very end did the following picture

79:54

show up which I'm glad it eventually

79:55

showed up. Okay. So we're talking about

79:57

this trace 5 cub theory.

80:00

Uh the fi is a matrix. This is the

80:02

point. Fi is a fi is a matrix. So we

80:04

imagine the phi is an n byn matrix. It

80:06

has an upstairs and a downstairs index.

80:09

So when we write fi cubed, we really

80:11

mean 5 a b 5 bc 5 ca with einstein

80:16

summation convention. Sort of summing

80:17

over all these things.

80:19

And so it's convenient to keep track of

80:21

what these indices are with a double

80:24

arrow notation. Okay. Okay. So if I have

80:25

something like this, the upstairs arrow

80:28

will be uh a arrow going this way will

80:30

be a J. The downstairs arrow will be an

80:32

I. Right? And so when I write trace I

80:35

cubed, trace 5 cubed looks something

80:38

like this.

80:42

So this will be let's say an I. But the

80:44

fact that it's a trace means that this

80:46

index is identified with that one. Okay.

80:48

So this I survives out to here and this

80:50

J survives to here and this K survives

80:53

to there. Okay.

80:55

Okay.

80:59

So, how would I draw a four-point

81:02

diagram?

81:06

You would draw it like this. This is the

81:08

uh the fat graph uh ribbon graph that uh

81:12

Sergio was uh referring to. Okay,

81:15

that's one fact graph. This is another

81:18

fat graph for the other diagram that I

81:20

would draw. Okay.

81:29

Okay.

81:31

And if I had a loop diagram, you know,

81:33

it uh diagrams like you saw in Ruth's

81:36

talk, a diagram like that when the

81:38

particles have color would look like

81:40

this.

81:41

Everything just gets fattened out.

81:52

Okay. Now,

81:54

there's there's two very closely related

81:57

points, very simple, ancient, very well

82:00

appreciated, but but let's just say them

82:03

they're very slightly different. One of

82:05

them is that we can think of each one of

82:07

these diagrams as being drawn on some

82:10

surface. Okay? So for example, we can

82:12

think of the tree diagram as being drawn

82:14

on the plane uh you know within ordering

82:17

with the external lines without any

82:18

crossing lines. Okay,

82:21

that's one picture we can think of as

82:23

being drawn on on on a plane. The other

82:26

one is that we can think of every one of

82:28

these diagrams is actually defining a

82:30

surface.

82:33

These are two slightly different ideas.

82:34

Okay. So for example, this diagram is

82:38

going to define a surface which is a a

82:41

disc with four marked points

82:45

1 2 3 four.

82:48

Okay. So how does this correspondence

82:50

how does this correspondence work? Well,

82:52

how would you define a surface? You can

82:55

define a surface by getting a

82:56

triangulation of the surface. Okay. So

82:58

what is a triangulation? Is a collection

83:00

of triangles with an orientation, right?

83:03

Um, and there's they're supposed to at

83:05

most meet on common boundaries with

83:07

opposite orientation, right? So, we're

83:10

talking about orientable uh surfaces

83:12

here. So, I could give you the triangle

83:14

1 2 3 and the triangle 134. And those

83:17

triangles give one definition of this uh

83:20

of this surface. Okay?

83:26

A ribbon graph like this, a fat graph

83:28

like this is giving you exactly the same

83:30

data.

83:31

Okay?

83:33

You can think of the you can think of

83:34

each one of these vertices. You can

83:36

think about the roads coming in as being

83:39

the edges of the graph.

83:42

So the edges of the triangles and the

83:45

triangles that meet along common

83:46

boundaries are precisely the things that

83:48

are joined by these propagators.

83:51

Okay. So this picture where now I would

83:55

call this like color one. This is color

83:57

one. So since it's color one everywhere

83:59

here, I'll sort of just draw one

84:01

underneath here everywhere. It's like

84:02

there's a region one here that goes

84:04

along with that line. There's a region

84:06

two that goes with this line. Three that

84:07

goes with this line. Four that goes with

84:09

this line and so on. Right? This picture

84:12

is defining

84:15

this triangulation of the surface.

84:19

And we can see this now in in in various

84:22

uh in uh in various ways. Uh but instead

84:25

of drawing sort of dual diagrams, you

84:26

can just think about what happens to

84:27

this picture if you shrink the black

84:30

black regions to points. If you shrink

84:33

the black regions to point here, that

84:34

black region turns into this marked

84:36

point on the outside. This black region

84:38

turns to this mark point on the outside

84:39

and so on. Okay,

84:42

is that clear?

84:43

>> Sorry. Black means now the white shape.

84:45

>> Yeah, I'm sorry. This Yeah, this is the

84:47

usual blackboard problem. Yes, this is

84:49

black. Sorry, I apologize. Yeah, I'm

84:52

Yeah. Yes, this uh white black region

84:55

anyway this region you shrink it turns

84:57

into that one right

84:59

and I'll leave it for you to have fun to

85:01

see you know how how uh how you can

85:04

anyway just interpret every aspect of

85:06

this picture uh here but uh but again

85:09

the idea is that this vertex is a

85:11

triangle okay

85:13

uh this vertex is a triangle and they're

85:15

meeting along uh uh common common

85:18

boundaries okay so notice two different

85:20

things one of them is that all diagrams

85:23

can be drawn on the surface. The other

85:25

one is that any one diagram defines the

85:27

surface. Okay.

85:30

So when we say we're summing over all

85:32

triangulations, right, you first have to

85:34

tell me what surface I'm talking about.

85:36

Then I'm solving summing over all

85:37

triangulations of the of the surface.

85:40

Okay? And so I'm going to pick one

85:43

diagram to define the surface. Not going

85:46

to draw all the diagrams. I know one

85:48

diagram to draw the surface. I want to

85:50

emphasize this is not even a fineman

85:51

diagram. We're not computing anything

85:52

with it. It's just representing if you

85:54

like nothing other than the flow of

85:56

color. Right? These pictures are just

85:58

about the sort of flow of color which

86:00

tells you what defines the the surface.

86:02

Okay? So I'm going to choose one diagram

86:04

to uh define my surface.

86:09

Okay. So

86:11

let's uh let's do that. And now we're

86:13

going to work with the fivepoint example

86:15

again. Right.

86:17

>> Sorry, I have a quick question.

86:20

Does the the genus in the second row not

86:22

play any role in it that they have a

86:23

genus one?

86:24

>> Very much so. Yes. Yes. So so uh the in

86:27

fact uh the the thing that uh Chingling

86:30

mentioned maybe maybe I'll I'll give you

86:31

uh an example here. Okay. Uh so so let's

86:35

look at this example.

86:37

So this has four lines sticking out of

86:39

it. And let's look at another example.

86:42

[Music]

86:44

Oops. Very bad at drawing. Um

86:53

this also have four lines sticking out

86:54

of it. Okay, these are two diagrams that

86:57

have four lines sticking out of it. This

86:59

is the triangulation of

87:03

a surface that has four marked points on

87:05

the outside and a little hole in the

87:07

middle. Sometimes the hole is called a

87:09

puncture. Okay,

87:13

is that clear? So if this is region you

87:14

know 1 2 3 4 um uh this would be you

87:19

know again 1 2 3 4 and this would

87:22

correspond to sort of this kind of

87:23

triangulation of the surface. Okay. What

87:27

about this guy? This guy is a

87:29

triangulation of an annulus.

87:31

This is this is an annulus

87:34

with three things on the outside. Three

87:36

mark points on the outside and one

87:38

marked point on the inside. I'll you

87:39

know if you don't see that immediately

87:41

I'll leave that as a little exercise. uh

87:44

for you to uh uh to play with. Okay. So

87:46

this color line four going around this

87:48

region four. You see this is color line

87:50

four. So this whole region shrunk to a

87:52

point is giving me uh that guy. So this

87:54

would be four with 1 2 3 let's say.

87:57

Okay.

87:59

Okay. And this is also you know it's not

88:02

literally this one but it'll look

88:03

something like this. I don't know some

88:04

triangulation that looks looks looks

88:06

like that. Right. So this is a

88:07

triangulation of the surface. But now

88:10

remember we're supposed to uh all of

88:13

these lines have uh have a color. So the

88:17

color here is specified by the external

88:19

color red. Red stays red stays red goes

88:22

red. Blue stays blue stays blue goes out

88:24

here. Right? But in this loop I don't

88:26

know what the color is. It can be any

88:28

color. So I should sum over all of the

88:30

colors. And that's why the final answer

88:33

here is proportional to the number of

88:35

colors n. Okay. So this is a planer

88:39

diagram and it's proportional to the

88:40

number of colors n.

88:42

This diagram has all the colors are also

88:45

determined right red on the outside blue

88:48

green cyan on the inside all the colors

88:51

are determined. There is no n. So this

88:54

is the simplest example to see that the

88:56

planer diagram is more enhanced by

88:59

powers of n than the uh than the

89:01

non-planer one. Okay. And that's a

89:05

special case. You can have fun drawing

89:07

two three points.

89:11

You know, draw something like this. A

89:13

three point on one side, three point on

89:15

the other. And you can either join them

89:16

up straight across. That's one diagram.

89:19

Or you can join them up like a pretzel.

89:24

That's another diagram.

89:27

This one's a Taurus. The first one is

89:30

just is just a a sphere with three

89:33

punctures.

89:35

uh and uh the first one uh the the

89:38

serial three punctures is proportional

89:40

to n squ this has no ends the color line

89:43

just goes around once

89:46

uh and so again that sorry there's just

89:48

one power of n the other one has three

89:50

three powers of n so it's enhanced by

89:52

another factor of n squ in general the

89:55

the powers of n are given by the oiler

89:57

characteristic so that's where the a

89:59

genus comes from and that's why we uh if

90:03

you send the number of colors to

90:04

infinity the physics gets dominated by

90:06

planer graphs. Okay, so that's one

90:09

reason physicists care about the planer

90:11

limit. Um but um uh but nothing in this

90:16

story depends on on on that fact. Okay,

90:18

so we can do things uh planer non

90:20

non-planer. It doesn't make any any

90:22

difference.

90:23

Okay, now let's uh continue.

90:29

So, we're going to draw a um we're going

90:32

to draw

90:36

we're going to do that fivepoint tree.

90:39

And I'm going to choose my

90:41

representative graph. Um just to be the

90:44

sort of obvious uh keep running out of

90:47

chalk here. Oh, here's some white chalk.

90:51

Oh, it's not white.

90:53

>> Oh, there's some white. No, there's some

90:55

white. White chalk here. It's fine. It's

90:56

good.

90:59

Okay. So let's uh let's take this is our

91:03

our our our surface

91:08

[Music]

91:12

and this is going to be uh we have this

91:14

triangulation

91:17

that was the one that Carolina was also

91:19

talking about and that corresponds to

91:21

this fact graph.

91:27

Okay, again let's see why this triangle

91:30

1 2 2 3 1 3 is this vertex here and this

91:35

is the road one two see 1 2 is 1 2 2 3

91:39

is 2 3 and 1 3 is 1 13 right

91:45

so this vertex corresponds to this

91:48

triangle this vertex corresponds to this

91:50

triangle this vertex corresponds to that

91:54

triangle Okay.

91:57

So, having picked your parent, you know,

92:00

base fat graph to define the surface,

92:04

we're done. Okay. Uh, in the sense that

92:07

our world is now fixed. From now on,

92:09

we're going to live in the world of this

92:11

fat graph. Not going to talk about

92:13

surface. We're not going to talk about

92:14

everything else. Our entire universe is

92:16

living inside uh these uh these graphs.

92:20

All right.

92:23

So in particular,

92:25

you know, when I go back to this

92:27

picture, I say, but what about all the

92:28

other triangulations, finding diagrams,

92:30

all all the rest of them? We're supposed

92:31

to sum over all the triangulations of

92:33

this uh of this graph, right? How do I

92:36

think about the other triangulations if

92:37

I'm not allowed to look at this picture?

92:39

I only can look at this picture. Okay?

92:41

So that's what we're going to just learn

92:42

to do now. Just take take a second and

92:45

learn, you know, how do I think about

92:47

all the curves on the surface in this

92:49

picture,

92:50

right?

92:52

Well, okay. Uh, how would I do it? So,

92:55

um, let's say I want to draw this curve.

92:59

Let's say I want to draw the curve, I

93:00

don't know, uh, 24.

93:03

That's one of the things that we were

93:04

talking about before.

93:06

Okay.

93:08

So, how would I draw 24

93:12

uh in in this world?

93:16

Well, it's a little bit annoying, right?

93:18

Because here, like what is two? two is

93:21

this kind of like black region here.

93:22

Four is this sort of uh black region

93:25

here somehow. Right? So if I want to

93:27

draw curve from two to four, I have to

93:30

sort of find something that maybe starts

93:31

here and then ends there somewhere.

93:34

Okay, that's perfectly okay. We could we

93:37

could uh we could talk about that. But

93:40

it's a little funny to anchor these

93:41

curves. You know, it's not obvious where

93:43

to put it. Okay, I could put it anywhere

93:46

uh uh uh along here. Um there's a more

93:50

natural thing that you can do. There's a

93:51

more na there's something more natural

93:53

in this uh in this picture

93:57

which is uh also here when I talked

93:59

about the sort of curve 24 I mean these

94:02

black dots are somehow telling you that

94:03

two and four don't belong to the surface

94:05

but to denote what I mean by by 24 let

94:08

me draw instead something which is the

94:11

same curve but I just tilt it slightly

94:13

the whole picture uh let's say

94:16

clockwise. Okay. So, I'm going to draw

94:17

it from like uh from a little bit to the

94:19

right of two to a little bit to the

94:21

right of four instead.

94:23

Okay. Now, it's obvious that I can go

94:25

forwards and backwards between these two

94:26

pictures because we're talking about

94:27

orientable surfaces. It's obvious here

94:30

for the uh for for for this case, but

94:32

also for any surface what it means by

94:34

rotating to the right is well defined

94:36

because there's a well- definfined

94:38

notion of orientation on on the surface.

94:40

to surface a efficionados.

94:43

uh these I don't remember what they're

94:44

called but these things are maybe called

94:46

I call them chords and these things are

94:50

called uh well it's a surface efficient

94:52

we'll call them laminations and you know

94:55

we call them just curves because this is

94:57

a chord this is a curve all right and so

95:01

the curve is easier to draw in this

95:03

picture the curve 24 well it just you

95:06

know starts up here somewhere

95:13

a little to the right of two. So it

95:14

starts in two and then it meanders

95:18

around and it exits at four. Right?

95:23

All right.

95:25

So every variable remember this is uh so

95:28

much of this entire story of positive

95:30

geometries and amplitudes are about

95:32

thinking about kinematic space. The big

95:34

surprise is you think hard about

95:36

kinematic space and kinematic space has

95:38

way more structure than you would have

95:39

naively thought. So in Karolina's story,

95:42

the kinematic space is just the XIS.

95:44

What could be exciting about XIS?

95:45

There's just a bunch of points on a

95:47

grid, but you draw the points on a grid

95:48

and then all of a sudden, oh gez,

95:50

they're repeated twice. So I have to

95:51

find a chunk of the grid in which they

95:53

all occur once and only once. And oh

95:55

gez, that brings to life these funny

95:56

triangles. And then the whole story

95:58

starts uh developing from there. Okay,

96:00

so we're doing the same thing now except

96:02

we're really starting from scratch. Um,

96:04

we're just taking we this is our

96:06

picture. We know that kinematics are

96:08

associated with these chords. We're

96:10

defining our surface by drawing one of

96:12

these pictures. And I just want to learn

96:13

how what how would I draw 24. The way I

96:16

draw 24 is in this like slightly more

96:18

natural way by going slightly to the

96:20

right of two, taking that road, going

96:22

out and moving slightly to the right of

96:23

four. Okay, so is that clear? Every xig

96:28

which is a kinematic variable, every xig

96:30

is naturally associated with some chord

96:33

j which is further more naturally

96:36

associated with the curve. Okay. This it

96:38

cousin curve uh J.

96:42

Okay.

96:45

Okay.

96:46

Now something very interesting uh

96:50

happens.

96:51

So um

96:54

uh so I I hope it's clear we're not we

96:55

haven't done anything yet right we've

96:57

just drawn a picture and now we know how

96:59

to describe every variable right every

97:01

variable is some curve in this surface

97:04

okay so for example even the ones in the

97:06

triangulation 13 is not just that

97:09

segment 13 would look like this curve

97:11

okay every single variable is some curve

97:14

on the surface the kinematics are

97:16

associated with curves on surfaces

97:20

Okay.

97:24

Okay. And now uh remember uh uh we saw

97:27

in the in the previous in our discussion

97:29

from the first hour kind of two magical

97:32

things happened. One uh the first one

97:35

was that um starting from the assoc

97:39

uh we got this fan which was cones the

97:41

cones correspond to diagrams and they

97:43

tiled the entire space. Okay, so that

97:46

was already one remarkable thing and the

97:47

second one was that we could somehow

97:48

efficiently generate those cones from

97:50

these polomials and the tropicalization,

97:52

right? Those were the the two ideas I'm

97:55

now in the time I have I'll be able to

97:57

explain or at least show you the first

97:59

magical thing and then tomorrow we'll

98:00

pick up and talk about the uh the second

98:02

one. Okay, but the first magical thing

98:05

is that uh is that uh uh we're going to

98:08

see where cones come from. They're going

98:10

to cover the entire space. Okay. And

98:13

we're going to do that without uh uh um

98:16

by just uh uh just listing all of these

98:20

curves. Right. So, right. So, uh we're

98:23

now going to talk about how would you

98:25

record the how would you present a

98:26

curve? Okay.

98:29

So, let's say you're you're you're

98:31

blind. You you you couldn't see the

98:32

picture and you just wanted to tell

98:34

someone what all all the curves were.

98:36

Okay.

98:38

All right. Well, what we're going to do,

98:40

and it's the only uh the only reasonable

98:42

thing to do is we're going to uh give

98:45

the uh Google navigate instructions for

98:48

how you would drive along the road

98:50

corresponding to this curve. Okay? So,

98:53

you want to say I want to follow, you

98:55

know, 24.

98:57

Uh again, I'm living in this universe.

98:59

Okay. But, um uh let me draw this uh let

99:03

me draw this picture less slightly

99:04

bigger and less messy.

99:07

Okay.

99:09

And this is my world.

99:13

This is also my map. And if I want to

99:16

take this road uh 24

99:20

then um well I could label all these

99:22

roads. I mean I could label this road.

99:24

This is road A B C D E F G.

99:29

Okay. Let me slightly more reasonably

99:31

label the roads in this case just by I

99:34

mean you will forgive me if I label this

99:36

road one two. I think it's clear what I

99:38

mean by that, right? It's bounded by one

99:39

and two, two and three, three and four,

99:43

four and five, five and one, one and

99:46

three, one and four. This is not always

99:48

possible, but in this very simple

99:49

example, we might as well uh label the

99:51

roads like that. You can also label them

99:52

ABCDE EFG. That's fine. Okay.

99:56

And now what is that road? I just have

99:58

to I just have to do what what I'm uh

100:01

what what Google navigate would tell me

100:02

to do. So, uh,

100:22

>> sorry, what do you mean by this? Is that

100:23

always possible? Like

100:25

>> I mean it's not always possible to

100:26

uniquely label a road by the by the by

100:29

the things that uh touch it that by the

100:31

yeah sometimes I mean in very

100:33

complicated surfaces is not always

100:34

possible but uh but it's not necessary.

100:37

This is just in this in this example for

100:39

convenience

100:40

>> but probably like one thing

100:41

>> yes that's yes exactly yes in the planer

100:44

cases is always possible. Yes that's

100:45

true. So, for example, here I start on

100:48

the road 23

100:50

and Google Navigate says make a left

100:53

turn onto the road 13. Okay? So, all

100:56

you're going to do is give instructions.

100:58

All you can do, by the way, the only

101:00

there's one caveat on these roads that I

101:02

draw. All you can do is travel along a

101:04

road till you get to the next

101:05

intersection and then you can turn left

101:07

or right at that intersection and that's

101:09

it. You can't double back. You can't go

101:12

halfway down a road and decide, "Oh, I

101:14

changed my mind. they don't want to go

101:15

go down this road. That's the only thing

101:16

you're not uh allowed to do. Um

101:20

otherwise, you just proceed until you

101:22

got the intersection and you go left to

101:23

right. So, it says I start on the road

101:24

23. I make a left turn

101:28

on the road 13

101:31

and then I make a right turn on the road

101:34

14

101:37

and they make a left turn onto the road

101:39

45.

101:42

Okay, so this is what you could call the

101:44

word for the curve 24.

101:47

Okay,

101:49

every curve has a word,

101:52

right? Which is just the Google navigate

101:54

instructions. Let's do another one.

101:57

Let's do one of these simple ones like

101:58

what's what's this curve that

102:00

corresponds uh uh to 13. This would be

102:04

we start at one two. I make a right turn

102:08

on the road three and then make a left

102:11

turn onto the uh word uh three onto the

102:14

road 3 four. This would be the word for

102:18

13.

102:19

Okay. So every curve has a word.

102:25

All right.

102:27

Now there's a very uh there's a very

102:29

obvious and natural way to keep track of

102:32

all of these uh uh words. um you can

102:35

make associate with any one of these

102:37

curves any of these words what's you can

102:39

call the geometric vector of the curve

102:42

so I'm going to call that for a curve C

102:48

for a curve C I'm going to define

102:51

for a curve C I'm going to define the

102:53

geometric vector

102:55

you can call it gam of C

102:59

and this lives in a space whose

103:00

dimensionality is equal to the total

103:02

number of roads in the picture. Okay, so

103:05

in this case it would be a

103:06

seven-dimensional vector because I have

103:07

seven roads. I I erased the picture.

103:10

Sorry, draw this for the teenth time.

103:13

Okay,

103:16

there's seven roads in this picture. 1 2

103:18

3 4 5 and the two internal ones. Seven.

103:20

Seven roads. So this would be a

103:22

seven-dimensional vector. And what is

103:24

this seven dimensional vector in this

103:25

example? you know it would be labeled by

103:29

uh 1 2 2 3 3 4 5 5 1 and the internal

103:34

ones 1 3 and 1 4 and just the entry is

103:37

just the number of times a curve visits

103:40

that road that's it so in this case it

103:42

would be a 1 one zero vector okay so for

103:45

example the geometric vector for the

103:47

curve 24 the geometric vector for this

103:50

curve 24 has a one in entries 2 3 1 3 1

103:53

4 and 45 and zero everywhere else okay

103:57

So the uh the the geome

104:00

of the curve 24 would be just as I said

104:03

one one

104:06

uh one and zero everywhere else. Okay,

104:09

so this this seven vector. Okay,

104:13

I hope you agree so far so boring.

104:15

Nothing interesting is happening yet.

104:17

Okay, um I have my surface that I've

104:20

defined by the parent fat graph. I draw

104:22

all the curves. Each one has a geometric

104:24

vector. I have a big stack of geometric

104:26

vectors. Okay, in this problem, how many

104:29

geometric vectors do I have? I have 10

104:32

geometric vectors. Um let's look at uh

104:35

because I also have geometric vectors

104:37

for these boundary curves. Let's take

104:39

this curve one two. This is just one of

104:41

the boundary curves of the problem. It

104:42

has a geometric vector, right? This guy

104:44

is uh the the geome vector for this sort

104:48

of boundary curve one two would just be

104:50

you know 1 one 0 0 for everyone else.

104:53

Okay.

104:55

Okay. So both the internal the five

104:57

internal curves and the five external

105:00

boundary curves each have geometric

105:02

vectors that are seven-dimensional.

105:04

Okay. So far there's nothing good about

105:07

these curves, good or bad about these

105:09

vectors. They're just about the positive

105:11

vectors and the positive or things

105:12

because they're all have plus signs,

105:14

right? Uh okay,

105:17

now comes the cool thing.

105:20

This is the the sort of surface avatar

105:22

of going on shell. Okay, because there

105:26

is after all a distinction between the

105:27

boundary curves and the internal ones.

105:30

We don't associate variables with the

105:32

boundary curves, right? They're on

105:34

shell. We only care about the the

105:36

variables for the internal curves. Okay.

105:38

So what is a natural way in this picture

105:41

of ignoring the boundary curves? How

105:44

would you go about ignoring the boundary

105:45

curves?

105:47

The most natural way to do it is to just

105:49

project through them. Okay, so in other

105:51

words, you have all these geometric

105:52

vectors are sticking out in various

105:54

directions, but you don't really care

105:56

about the curve one two. So I'm just

105:57

going to look at the whole picture in

105:59

the direction of the curve one two. So

106:00

one two is gone. I've projected through

106:02

one two and I've go gone down to a one

106:04

lower dimensional space. Okay. And I'm

106:06

going to do that with all of the

106:08

boundary curves. I'm just going to get

106:09

rid of all of the boundary curves. Okay.

106:12

Just by projecting through them. When I

106:15

do that, I'm going to go from a

106:18

seven-dimensional space to a

106:20

fivedimensional space. Right now, the

106:22

space is more natural. The

106:23

dimensionality is just the number of

106:25

internal propagators. I'm just I'm just

106:27

projecting through five vectors.

106:30

And okay, I'm going to be now now all of

106:32

the boundary vectors are mapped to the

106:34

origin of course because I've projected

106:36

through them. That's the whole point of

106:37

mapping them all to the origin. Uh and

106:40

uh I'm left with the five remaining ones

106:41

in a two dimensional space. Okay.

106:44

>> Sorry, but they're like two internal

106:45

propagators.

106:46

>> There's two internal propagators.

106:47

There's that's why the space is two

106:49

dimensional. There's two internal prop

106:50

space is two dimensional. I still have

106:52

five curves though that are not that are

106:54

not uh boundary curves. I have the

106:56

internal curves that are left. So I'm

106:58

going to have five two dimensional

106:59

vectors. I started with 10

107:01

seven-dimensional vectors. Five of them

107:03

were boundaries. Five of them were

107:04

internal. I project through the boundary

107:07

guys. Notice projecting through the

107:08

boundary guys is not the same as just

107:10

truncating the top five components,

107:13

right? Because the the boundary vectors

107:15

are interesting vectors in this

107:16

geometric space. I project through them.

107:18

Okay? I project through them, but I end

107:20

up with a two-dimensional space. Okay?

107:25

All right. Now, that's just a LINEAR

107:26

ALGEBRA EXERCISE. IT'S trivial to do the

107:28

uh uh uh linear algebra exercise. Uh

107:31

I'll leave it for you as an exercise to

107:33

do it while right now by doing it in

107:35

this super direct dumb uh dumb way. But

107:38

I'll write down what it uh uh what it

107:41

looks like when you do it. So you're

107:43

left with a two dimensional vector

107:45

space.

107:46

And so you know I can choose any basis I

107:48

like for the two dimensional vector

107:49

space. Of course it's natural to choose

107:51

the basis. It's natural to choose the

107:54

basis to be the one that you get uh uh

107:58

by by projecting uh 13 and 14. You know

108:02

13 and 1/4 were the where the were

108:05

defining in the triangulation. So

108:06

they're clearly somehow special.

108:09

So let me just tell you what happens

108:11

after you project through the

108:12

boundaries. After you project through

108:14

the boundaries,

108:20

you get a two-dimensional picture. So

108:21

I'm going to choose as a basis. This is

108:23

what 13 turns into

108:27

just a basis of 1 13 and 1/4. And guess

108:29

what? Of course 24 is that vector. 25 is

108:34

that vector and 35 is that vector.

108:40

Exactly the picture that we had before

108:44

except I didn't do anything. I didn't

108:45

start with ABHYN

108:48

blah blah all of Carolina's talk. Forget

108:50

about it. Right. Um

108:54

we're just defining the surface,

108:57

recording all the curves and then this

108:59

one interesting operation of projecting

109:01

through the boundaries to be the kind of

109:03

analog of forgetting about them. We

109:05

don't care about them. we project

109:07

through the uh the boundaries and then

109:09

instead of having the stack of vectors

109:11

all with positive coordin you know in

109:13

the positive or after I project I get

109:16

this picture and miraculously amazingly

109:20

I get something that tiles the entire

109:22

space and the cones are fineman diagrams

109:25

the cones are triangulations of the

109:26

surface which are fineman diagrams okay

109:29

I find this absolutely remarkable right

109:32

because this in a very concrete sense is

109:34

like all the pictures of All the

109:36

space-time processes just come out just

109:39

come out with no no thought. Okay, they

109:42

just come out from this automatic uh

109:44

operation.

109:47

Now I'm going to tell you the rule for

109:48

reading off these uh uh this picture

109:51

without this work and and you'll also

109:53

see from the nature of the rule what the

109:55

proof is uh that that it corresponds to

109:57

the process that I was telling you

109:58

about. In order to do this, let me go

110:00

back to the picture

110:03

and uh let's look at some of our words

110:05

again. Except uh I'm going to I'm going

110:08

to denote the words slightly

110:10

differently. Actually uh here we are.

110:12

Okay. So let's say I have this word

110:16

I'm going to draw instead of writing LR

110:20

I'm going to make a little mountainscape

110:22

out of it. Whenever there's an L I'm

110:24

going to draw something going up.

110:25

Whenever there's an R, I'm going to draw

110:27

something going down. Okay? So from here

110:29

instead I would write this as 2 three up

110:32

to 13 down to 14 up to four five.

110:37

Okay.

110:40

Now what instead uh what the word for

110:43

like this boundary curve let's let's do

110:45

let's do this this let's do this

110:47

boundary curve let's say we do this one

110:49

51 right? What does this look like? It

110:51

looks like one two right onto one three

110:53

right onto 14 right onto 15. They all go

110:56

right or they all go left. Okay, I went

110:59

backwards that all go left. So for

111:01

example, yeah, so that one would look

111:02

like one five up onto 14 up onto one

111:05

three up onto one two. This is what a

111:07

boundary curves look like. It's all up.

111:09

All up or all down.

111:11

But these guys uh uh internal curves

111:14

have interesting ups and downs in them.

111:16

Okay.

111:18

And so this should make it obvious what

111:21

the formula is for the vector associated

111:24

with these curves after projection. The

111:27

vector associated these curves after

111:28

projection are called G vectors. Not

111:31

geometric vectors but G vectors.

111:34

And the G vector for a curve C can be

111:37

read off in a very simple way from its

111:39

word. Okay. So the G vector not the G

111:43

vector but the G vector for the curve C

111:44

is simply equal to

111:49

the sum over all the valleys

111:54

minus the sum over all peaks of the

111:56

word.

112:00

What I mean by this is that you you

112:02

imagine uh you imagine associating a

112:04

basis element with each one of the

112:06

internal words. Okay. So I'll just call

112:09

that I mean I could call it E13 and E14

112:13

although sometimes just call it 13 and

112:15

14. But then what is the G vector

112:17

associated with this word? The 14 is a

112:21

valley so it's positive E14. The 13 is a

112:24

peak so it's uh minus E13. So the G

112:27

vector for 24 would be E14 minus E13.

112:32

And indeed if you look at the picture

112:37

that's what we got for 24 right plus E14

112:40

minus E13. Okay

112:43

so you can easily see why this peak

112:45

minus value formula must be correct

112:47

because this is just a linear map on the

112:50

original vectors and this linear map has

112:53

a job to do. It has to send to zero

112:55

everything which is all upward going. So

112:58

that's why it cares about peaks and

112:59

valleys. Okay, you have to have a peak

113:01

or valley in order to get something non

113:03

zero. And a moment slot shows this is

113:06

essentially the unique uh linear map

113:09

that has a property that it sends all

113:10

the upward or downward going things uh

113:13

to zero and uh well preserves the rest

113:15

of them in some way. All right. So let's

113:18

now pause. Yes.

113:20

>> So but this is now the G vector that

113:22

comes from the cluster algebra

113:24

>> in this case. This is a G vector that

113:25

comes from the from the uh from the

113:27

cluster algebra. As I said a few times

113:30

for general surfaces, there's a the

113:32

cluster algebra is not quite the right

113:33

thing. Okay. Uh and so that's why I I

113:36

keep insisting on this uh on this

113:38

difference also because it ruined a year

113:39

and a half of my life uh sort of

113:41

thinking that the cluster algebra was

113:43

was the right thing. So it was not the

113:44

right thing and uh so I still have a lot

113:46

of energy. Uh but yes, here in these

113:49

examples um uh uh uh it's the same as

113:53

the as the uh uh the G vectors associate

113:56

with the cluster algebra. All right.

113:58

So uh we have five minutes left. So let

114:01

me just uh sum up. Okay.

114:05

So um what you can do and and uh I

114:08

invite you to try this in the uh just in

114:10

the next example in a uh in for a uh for

114:14

a sixpoint disc or a six particle tree

114:18

amplitude. Draw your favorite uh draw

114:21

your favorite fact graph for it. you

114:23

know, uh, our favorite fat graph for,

114:27

uh, for many purposes has been this one

114:29

that Karolina was talking about where

114:31

you just add more and more things to it.

114:34

Okay? So, you could draw something like

114:35

that or, you know, at six points, you

114:38

could draw something like this. This

114:39

Mercedes-Benz type picture. Okay? So,

114:42

draw any of these pictures you like. Any

114:45

one of these things gives you an equally

114:46

good triangulation of the surface,

114:49

equally good parrot fact graph. Okay?

114:51

And then just write in this case there's

114:53

nine internal curves. So draw nine

114:55

curves make nine words make nine sets of

114:58

peaks and valleys nine sets of G vectors

115:01

plot them just in mathematical or if if

115:04

you or by hand plot them and see to your

115:07

wonder that that they form cones and

115:11

each cone corresponds to a particular

115:13

way that these three curves can come

115:14

together to give you a triangulation of

115:15

the surface. Right? You didn't ask for

115:17

it. It's just ploning down the names of

115:20

the curves, drawing the projections, and

115:22

it just automatically uh divides the

115:24

space up into these cones. All right.

115:27

Now, the proof of this statement is

115:29

relatively easy.

115:32

It has to do with the fact that uh uh

115:34

that um if you take a uh random

115:37

geometric vector, so we can step back. I

115:40

gave you a definition of the geometric

115:42

vector. Um but you can step back and say

115:45

if I hand you a random vector, how do

115:47

you know it's a John vector for

115:49

something? Okay, can you check whether

115:51

it's some vector of all positive integer

115:53

entries? How can I check if it's a

115:54

geometric vector of something? And in

115:57

fact, there's a set of inequalities that

115:59

there's a sort of cone, what you call

116:00

the geometric vector cone that specifies

116:03

all possible consistent geometric

116:05

vectors. Okay, given a surface, very

116:07

simple picture. I'll say it in the

116:09

language of triangulations. Um uh maybe

116:13

I'll just draw here. Uh

116:22

so let's say you draw any set of uh any

116:25

either a single curve on the surface or

116:27

indeed any collection of and here's the

116:30

important word non-intersecting curves

116:32

on a surface. One maybe the surface is

116:34

very complicated. The curve comes around

116:36

circles in lots of ways or I draw 10

116:38

curves on top of each other that are

116:40

non-intersecting. Okay. But that the

116:41

sort of key thing is that you're drawing

116:43

a bunch of non-intersection curves. Then

116:46

what can these curves look like in any

116:48

triangle in the triangulation? Okay. So

116:50

here's some triangle in the

116:51

triangulation. This giant collection of

116:54

curves. What can it look like inside

116:55

this triangle? It has to look like this.

117:02

Right? There can't be anything that

117:04

crosses through this triangle. Otherwise

117:05

there'd be crossing. Okay?

117:09

So if so if this is the edge a uh an

117:12

edge b and edge c in the triangulation

117:16

and so if the geometric vector if the

117:18

component is some integer a some integer

117:20

b and some integer c then in order for

117:24

this to be compatible with this picture

117:26

if there's x things going through here y

117:28

things going through here and z things

117:29

going through here then we have to have

117:31

that x is equal to a plus b uh sorry

117:34

that the other way a is equal to x plus

117:37

z B is equal to uh X + Y

117:44

and C is equal to X + Z which we can

117:47

invert to solve for X is equal to uh A +

117:51

B

117:52

minus C / 2 and so on. Okay.

117:58

Um did I do that right? Uh uh no let's

118:02

see X should be did I do this right?

118:06

Sorry. C sorry C is uh C is Z + one.

118:10

Sorry about that.

118:12

Okay. So now now this is correct right.

118:14

So A plus B minus C uh is 2X. So X is A

118:18

plus B minus C over 2 and so on. Okay.

118:21

So that means that these numbers A, B

118:22

and C have to satisfy that A plus B

118:25

minus C over two is greater than or

118:27

equal to zero integer.

118:30

Okay. So that's how you can check. If

118:32

someone hands you a random geometric

118:34

vector, you have to just check the stack

118:36

of inequalities, right? They said they

118:37

hand you the triangulation. So you know

118:39

what all the ABCs are for all the

118:41

triangles. You just have to check the

118:42

stack of inequalities and that will tell

118:44

you if it's a legal uh geometric vector.

118:47

Okay. And now there's a cool point which

118:50

is obvious when you think about it, but

118:52

one of those things you have to just

118:53

think about it a little bit. I don't

118:54

know. I can give a I can give a a formal

118:56

proof but the formal proof is like is

118:58

harder than just uh uh thinking about

119:01

it. Um uh which is the following. So

119:05

first of all given any picture like this

119:07

you can also decide whether this

119:09

corresponds to a single curve or

119:11

multiple curves okay and uh on top of

119:14

each other and basically there's

119:16

essentially an algorithm like pick a

119:17

strand here and just follow it see where

119:20

it goes right if it goes and you sort of

119:22

exit the surface in one one place or

119:25

another then take it out if there's

119:26

anything left it's not a single

119:27

component curve right there are there

119:29

are other curves around right so you can

119:32

decide whether you have a single

119:33

component curve or

119:35

And the final comment then is that given

119:37

any legal geometric vector, any legal

119:40

geometric vector is uniquely represented

119:42

as a positive integer sum of single

119:45

component geometric vectors. Okay,

119:47

that's a sort of key point is that you

119:49

can uniquely say given any legal

119:51

geometric vector which set of curves

119:53

have been put on top of each other in a

119:55

non-intersecting way to uh preserve.

119:59

Once you know that fact, it's a really a

120:01

few line argument to say that after you

120:03

project to get down to the uh uh to the

120:07

G vectors that you get uh that that a uh

120:12

there are uh a uh the cones that that a

120:17

if you make a cone out of single

120:19

component curves that don't cross each

120:21

other then such cones cannot intersect.

120:25

Okay, so that's a very very simple uh

120:27

consequence of this fact. So that tells

120:30

you that that the cones that correspond

120:32

to triangulations do not overlap each

120:33

other. And B, you can see that they

120:36

cover the entire space. And there

120:38

there's a very simple argument um that

120:41

uh that that the linear span of all

120:43

these cones must cover the entire space

120:45

because we get the positive or for free

120:48

out of the parent underlying curves,

120:51

right, that go into the triangulation.

120:53

But there's also a set of curves that

120:55

are the negative orthodont. And who are

120:57

they? Remember right at the beginning of

120:59

this story, we made a choice of whether

121:01

we're we're going to rotate the curves

121:02

to the right or to the left to define

121:05

them. I just chose to rotate them

121:06

clockwise. Well, if you rotate all the

121:09

curves counterclockwise, you get another

121:10

set of curves on the surface. And their

121:12

G vectors are precisely the negative of

121:14

the ones where you uh do it the other

121:16

way. Okay? So there's in fact two sets

121:19

of there's a positive orant and kind of

121:21

a negative orant. So together that

121:23

guarantees the entire space is covered.

121:25

Okay. Uh so these two arguments together

121:27

tells you that uh that the entire space

121:30

is tiled by cones uh that correspond to

121:33

triangulations and that cover the entire

121:34

space. Okay. So in the end is a very

121:36

simple argument. Um but it's still quite

121:39

quite the remarkable again that uh this

121:42

is a this is an an algorithm that you

121:44

can quickly you know put on a computer

121:46

generate these uh G vectors. there's a

121:48

bunch of cones. And so I've made all the

121:50

diagrams, all the triangulations have

121:52

sort of come out for free um uh from

121:55

this extremely simple point of view.

121:57

Okay. So what we'll pick up on tomorrow

122:00

is the much more the the more

122:02

interesting maybe much more interesting

122:04

uh aspect of this story that uh as we

122:07

emphasize already, but I'll just say it

122:08

again uh before we go. It's one thing to

122:11

know that all the diagrams come to life

122:12

just by recording all the curves and

122:14

projecting down to G vector space. But

122:17

this is is still not useful for

122:19

computing an amplitude. If what you have

122:20

to do is in every cone go and compute

122:23

something for the cone and add them all

122:24

up, then we we're just doing fineman

122:25

diagrams all over again. The more

122:28

interesting second fact is that we can

122:30

this this whole fan sometimes called the

122:33

G vector fan or we call it the fineman

122:35

fan. Okay, this fan uh is the result of

122:40

the common refinement of a bunch of

122:42

simple tropical functions or that there

122:44

is a bunch of polomials that are

122:46

associated with these pictures and most

122:49

fundamentally there are U variables

122:51

associated with all these pictures

122:53

and um and the magic is going to be that

122:57

we're going to find a way to solve the U

122:59

equations. Okay, we're going to present

123:00

the solution to the U equations. I'm

123:02

going to tell you how to give a formula

123:04

for every U, right?

123:06

Now you might think these U equations

123:07

look very global. I mean that's the

123:10

whole point. They're somehow telling you

123:11

how curves interact with all other

123:12

curves, right? So this curve, what are

123:14

the other curves that intersects? The U

123:16

equations feel very very global. The

123:19

amazing thing is that there's going to

123:20

be a totally local formula for the U's.

123:23

In other words, if you give me a curve

123:25

and the word for the curve, from the

123:27

word for the curve, there's going to be

123:29

a simple computation that gives you the

123:31

u variable associated with that curve

123:33

without looking at any of the other

123:35

curves. You don't even think about the

123:36

other curves. Someone just hands you the

123:38

word for a curve and we're going to give

123:40

a very simple formula that's associated

123:42

with a nice combinatorial counting

123:43

problem associated with that word. Uh

123:46

whose solution is going to be the u

123:47

variables. Okay. So that's the somehow

123:50

magic of this story that while we can

123:51

prove it and understand it in various

123:53

ways, I still feel is not completely

123:55

understood. This local global

123:58

uh fact that the U variables can be

124:00

computed entirely locally from the

124:02

knowledge of uh the the word specifying

124:05

a curve and yet they knew know to do

124:07

this thing to solve the U equations and

124:10

keep all of the uh and control the the

124:13

accommodators of how all of these uh

124:15

curves come come together. But once we

124:18

get those U variables, we'll see the

124:20

polomials that go along with those U

124:22

variables. The the the the U variables

124:25

we associate with certain polinomials.

124:26

These polinomials are called F

124:28

polinomials that are associated with the

124:29

curves and um and they give you the

124:33

stringy integral in both the forms and

124:36

the integral u to the x form as well as

124:38

the form where you just write down

124:39

powers of y and polomials to the minus

124:42

c. Okay, so those are the two forms and

124:44

the tropicalize to give you the global

124:47

shringer parametric form for the

124:48

amplitude. So that's the first part of

124:50

what we'll talk about tomorrow is uh

124:52

where these uh u variables come from.

124:53

All right, thanks a lot.

Interactive Summary

The speaker begins by adjusting the lecture order, deciding to present the simpler story of trace-cubed theory first, followed by the more complex amplituhedron story. They explain that trace-cubed theory, when understood to all orders in perturbation theory, connects to simple pictures of curves on surfaces and combinatorics, offering a bottom-up discovery of string theory. The presentation then delves into an example involving the five-point amplitude and an icosahedron realization, emphasizing the need for a rational explanation for seemingly 'pulled out of thin air' steps. An alternate viewpoint using a dual picture, inward-pointing normals, and the normal fan of a polytope is introduced. The concept of Minkowski sums is highlighted as a remarkable fact with implications for predicting amplitude vanishing and factorization. The lecture then explores associating polynomials with these pictures and their 'tropicalization' in T13-T14 space, leading to a discussion of string amplitudes and their low-energy field theory limits. The connection between Minkowski sums and string theory is made explicit, showing how sum ends translate to powers in string amplitudes. Finally, the speaker introduces 'binary geometry' and nonlinear equations associated with chords on surfaces, demonstrating their role in keeping crossing chords apart and their connection to positively-oriented solutions. The lecture concludes by reiterating the surprising fact that these concepts, originating from a toy model, can describe real-world particle physics like pions and gluons, and that their mysterious properties are shared across these theories.

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