enumerative geometry, intersection theory and …for any given enumerative question three problems...

Post on 05-Jan-2020

8 Views

Category:

Documents

0 Downloads

Preview:

Click to see full reader

TRANSCRIPT

Enumerative geometry, Intersection Theory andModuli Spaces

Enrico Arbarello

Pisa, May 28, 2008

Euclid (325-265 a.C.)

”Euclid-Bramante”

Postulate: There is one linethrough two distinct points.

Proposition: Two distinct linesmeet in at most one point.

Euclid (325-265 a.C.) ”Euclid-Bramante”

Postulate: There is one linethrough two distinct points.

Proposition: Two distinct linesmeet in at most one point.

Euclid (325-265 a.C.) ”Euclid-Bramante”

Postulate: There is oneline through two distinct points.

Proposition: Two distinct linesmeet in at most one point.

Euclid (325-265 a.C.) ”Euclid-Bramante”

Postulate: There is oneline through two distinct points.

Proposition: Two distinct linesmeet in at most one point.

Apollonius from Perga(262-190 a.C.)

”Conics”

387 Propositions on conics:

Apollonius from Perga(262-190 a.C.)

”Conics”

387 Propositions on conics:

Apollonius from Perga(262-190 a.C.)

”Conics”

387 Propositions on conics:

Apollonius from Perga(262-190 a.C.)

”Conics”

387 Propositions on conics:

Proposition: Through fivegeneric points passes exactlyone conic.

Proposition: Two genericconics meet in at most fourpoints.

3

Proposition: Through fivegeneric points passes exactlyone conic.

Proposition: Two genericconics meet in at most fourpoints.

3

Proposition: There are, at most, 4 lines that are tangent to twogiven conics.

Proposition: There are, at most, 4 lines that are tangent to twogiven conics.

Proposition: there are, at most, 8 circles that are tangent to threegiven circles.

Proposition: there are, at most, 8 circles that are tangent to threegiven circles.

Apollonius from Perga(262-190 a.C.)

I.Newton(1643-1727)

G. Leibniz(1646-1716)

Apollonius from Perga(262-190 a.C.)

I.Newton(1643-1727)

G. Leibniz(1646-1716)

M.Chasles (1793-1880)

There are (at most)3264 = 51× 24 conics that aretangent to 5 given conics.The difficulty comes fromdouble lines. These solutionsmust be discarded.

H. Schubert (1848-1911)

There are (at most)666.841.080 =23 × 3× 5× 653× 853 spacequadrics which are tanget to 9given quadrics.

M.Chasles (1793-1880)

There are (at most)3264 = 51× 24 conics that aretangent to 5 given conics.

The difficulty comes fromdouble lines. These solutionsmust be discarded.

H. Schubert (1848-1911)

There are (at most)666.841.080 =23 × 3× 5× 653× 853 spacequadrics which are tanget to 9given quadrics.

M.Chasles (1793-1880)

There are (at most)3264 = 51× 24 conics that aretangent to 5 given conics.The difficulty comes fromdouble lines. These solutionsmust be discarded.

H. Schubert (1848-1911)

There are (at most)666.841.080 =23 × 3× 5× 653× 853 spacequadrics which are tanget to 9given quadrics.

M.Chasles (1793-1880)

There are (at most)3264 = 51× 24 conics that aretangent to 5 given conics.The difficulty comes fromdouble lines. These solutionsmust be discarded.

H. Schubert (1848-1911)

There are (at most)666.841.080 =23 × 3× 5× 653× 853 spacequadrics which are tanget to 9given quadrics.

M.Chasles (1793-1880)

There are (at most)3264 = 51× 24 conics that aretangent to 5 given conics.The difficulty comes fromdouble lines. These solutionsmust be discarded.

H. Schubert (1848-1911)

There are (at most)666.841.080 =23 × 3× 5× 653× 853 spacequadrics which are tanget to 9given quadrics.

R. Descartes(1596-1650)

line: ax + by + c = 0

circle: x2 + y2 = 1 cubic: y2 = x3 − 1

R. Descartes(1596-1650)

y

x

line: ax + by + c = 0

circle: x2 + y2 = 1 cubic: y2 = x3 − 1

R. Descartes(1596-1650)

y

x

line: ax + by + c = 0

x

y

circle: x2 + y2 = 1

cubic: y2 = x3 − 1

R. Descartes(1596-1650)

y

x

line: ax + by + c = 0

x

y

circle: x2 + y2 = 1

x

y

cubic: y2 = x3 − 1

x

y

quartic: x4 + y4 = 1

nodal cubic: y2 = x3 + x2

x

y

quartic: x4 + y4 = 1

x

y

nodal cubic: y2 = x3 + x2

Proof of the fact that there are at most 4 lines that aretangent to two given conics:

The analytic represention of a conic shows that the tangent linesto a conic form a conic in the dual plane.

Thus the assertion about tangent lines reduces to the one aboutthe inersection of two conics.

Proof of the fact that there are at most 4 lines that aretangent to two given conics:

The analytic represention of a conic shows that the tangent linesto a conic form a conic in the dual plane.

Thus the assertion about tangent lines reduces to the one aboutthe inersection of two conics.

Proof of the fact that there are at most 4 lines that aretangent to two given conics:

The analytic represention of a conic shows that the tangent linesto a conic form a conic in the dual plane.

Thus the assertion about tangent lines reduces to the one aboutthe inersection of two conics.

Proof of the fact that there are at most 4 lines that aretangent to two given conics:

The analytic represention of a conic shows that the tangent linesto a conic form a conic in the dual plane.

Thus the assertion about tangent lines reduces to the one aboutthe inersection of two conics.

Proof of the fact that there are at most 4 lines that aretangent to two given conics:

The analytic represention of a conic shows that the tangent linesto a conic form a conic in the dual plane.

Thus the assertion about tangent lines reduces to the one aboutthe inersection of two conics.

Proof of Apollonius’ 8 Circles Theorem:

The equation of a circle:

x2 + y2 + ax + by + c = 0 , (con (a/2)2 + (b/2)2 − c > 0 ) .

depends on 3 real parameters: a, b e c. These are called themoduli of a circle

The tangency condition is quadratic in the variables a, b e c .

Thus, to find the circles that are tangent to 3 given circles onemust find the common solutions to 3 quadratic equations in thevariables a, b and c .

In general one obtains at most 8 solutions.Q.E.D.

9

Proof of Apollonius’ 8 Circles Theorem:

The equation of a circle:

x2 + y2 + ax + by + c = 0 ,

(con (a/2)2 + (b/2)2 − c > 0 ) .

depends on 3 real parameters: a, b e c. These are called themoduli of a circle

The tangency condition is quadratic in the variables a, b e c .

Thus, to find the circles that are tangent to 3 given circles onemust find the common solutions to 3 quadratic equations in thevariables a, b and c .

In general one obtains at most 8 solutions.Q.E.D.

9

Proof of Apollonius’ 8 Circles Theorem:

The equation of a circle:

x2 + y2 + ax + by + c = 0 , (con (a/2)2 + (b/2)2 − c > 0 ) .

depends on 3 real parameters: a, b e c. These are called themoduli of a circle

The tangency condition is quadratic in the variables a, b e c .

Thus, to find the circles that are tangent to 3 given circles onemust find the common solutions to 3 quadratic equations in thevariables a, b and c .

In general one obtains at most 8 solutions.Q.E.D.

9

Proof of Apollonius’ 8 Circles Theorem:

The equation of a circle:

x2 + y2 + ax + by + c = 0 , (con (a/2)2 + (b/2)2 − c > 0 ) .

depends on 3 real parameters: a, b e c. These are called themoduli of a circle

The tangency condition is quadratic in the variables a, b e c .

Thus, to find the circles that are tangent to 3 given circles onemust find the common solutions to 3 quadratic equations in thevariables a, b and c .

In general one obtains at most 8 solutions.Q.E.D.

9

Proof of Apollonius’ 8 Circles Theorem:

The equation of a circle:

x2 + y2 + ax + by + c = 0 , (con (a/2)2 + (b/2)2 − c > 0 ) .

depends on 3 real parameters: a, b e c. These are called themoduli of a circle

The tangency condition is quadratic in the variables a, b e c .

Thus, to find the circles that are tangent to 3 given circles onemust find the common solutions to 3 quadratic equations in thevariables a, b and c .

In general one obtains at most 8 solutions.Q.E.D.

9

Proof of Apollonius’ 8 Circles Theorem:

The equation of a circle:

x2 + y2 + ax + by + c = 0 , (con (a/2)2 + (b/2)2 − c > 0 ) .

depends on 3 real parameters: a, b e c. These are called themoduli of a circle

The tangency condition is quadratic in the variables a, b e c .

Thus, to find the circles that are tangent to 3 given circles onemust find the common solutions to 3 quadratic equations in thevariables a, b and c .

In general one obtains at most 8 solutions.

Q.E.D.9

Proof of Apollonius’ 8 Circles Theorem:

The equation of a circle:

x2 + y2 + ax + by + c = 0 , (con (a/2)2 + (b/2)2 − c > 0 ) .

depends on 3 real parameters: a, b e c. These are called themoduli of a circle

The tangency condition is quadratic in the variables a, b e c .

Thus, to find the circles that are tangent to 3 given circles onemust find the common solutions to 3 quadratic equations in thevariables a, b and c .

In general one obtains at most 8 solutions.Q.E.D.

9

For any given enumerative question three problems naturally arise.

1. Find the natural moduli space M.

2. Study the intersection theory of M.

3. Translate the enumerative problem into an intersectionproblem.

Only the last problem is usually easy to solve. The difficulties lie insolving the first two problems. As far as the second problem isconcerned, the fact that M is a moduli space is, in a sense,irrelevant. One would like to know the intersection theory of everyvariety.

For any given enumerative question three problems naturally arise.

1. Find the natural moduli space M.

2. Study the intersection theory of M.

3. Translate the enumerative problem into an intersectionproblem.

Only the last problem is usually easy to solve. The difficulties lie insolving the first two problems. As far as the second problem isconcerned, the fact that M is a moduli space is, in a sense,irrelevant. One would like to know the intersection theory of everyvariety.

For any given enumerative question three problems naturally arise.

1. Find the natural moduli space M.

2. Study the intersection theory of M.

3. Translate the enumerative problem into an intersectionproblem.

Only the last problem is usually easy to solve. The difficulties lie insolving the first two problems. As far as the second problem isconcerned, the fact that M is a moduli space is, in a sense,irrelevant. One would like to know the intersection theory of everyvariety.

For any given enumerative question three problems naturally arise.

1. Find the natural moduli space M.

2. Study the intersection theory of M.

3. Translate the enumerative problem into an intersectionproblem.

Only the last problem is usually easy to solve. The difficulties lie insolving the first two problems. As far as the second problem isconcerned, the fact that M is a moduli space is, in a sense,irrelevant. One would like to know the intersection theory of everyvariety.

For any given enumerative question three problems naturally arise.

1. Find the natural moduli space M.

2. Study the intersection theory of M.

3. Translate the enumerative problem into an intersectionproblem.

Only the last problem is usually easy to solve. The difficulties lie insolving the first two problems.

As far as the second problem isconcerned, the fact that M is a moduli space is, in a sense,irrelevant. One would like to know the intersection theory of everyvariety.

For any given enumerative question three problems naturally arise.

1. Find the natural moduli space M.

2. Study the intersection theory of M.

3. Translate the enumerative problem into an intersectionproblem.

Only the last problem is usually easy to solve. The difficulties lie insolving the first two problems. As far as the second problem isconcerned, the fact that M is a moduli space is, in a sense,irrelevant. One would like to know the intersection theory of everyvariety.

Looking for missing intersections (I):

Looking for missing intersections (I):

Looking for missing intersections (I):

Leon Battista Alberti(1404-1472)”De Pictura”

Piero della Francesca(1412- 1492)”De prospectiva pingendi”

Abrecht Durer(1471-1528)”Unterweisung der Messungmit dem Zirkel undRichtscheit”

Leon Battista Alberti(1404-1472)”De Pictura”

Piero della Francesca(1412- 1492)”De prospectiva pingendi”

Abrecht Durer(1471-1528)”Unterweisung der Messungmit dem Zirkel undRichtscheit”

Leon Battista Alberti(1404-1472)”De Pictura”

Piero della Francesca(1412- 1492)”De prospectiva pingendi”

Abrecht Durer(1471-1528)”Unterweisung der Messungmit dem Zirkel undRichtscheit”

Leon Battista Alberti(1404-1472)”De Pictura”

Piero della Francesca(1412- 1492)”De prospectiva pingendi”

Abrecht Durer(1471-1528)”Unterweisung der Messungmit dem Zirkel undRichtscheit”

15

15

15

With projective geometry a perfect duality is established betweenpoints and lines in the plane.

The sentence: there is onlyone line through two distinctpoints, is perfectly dual to: two

distinct lines intersect inexactly one point.

With projective geometry a perfect duality is established betweenpoints and lines in the plane.

The sentence: there is onlyone line through two distinctpoints,

is perfectly dual to: twodistinct lines intersect inexactly one point.

With projective geometry a perfect duality is established betweenpoints and lines in the plane.

The sentence: there is onlyone line through two distinctpoints,

is perfectly dual to: twodistinct lines intersect inexactly one point.

With projective geometry a perfect duality is established betweenpoints and lines in the plane.

The sentence: there is onlyone line through two distinctpoints,

is perfectly dual to: twodistinct lines intersect inexactly one point.

With projective geometry a perfect duality is established betweenpoints and lines in the plane.

The sentence: there is onlyone line through two distinctpoints,

is perfectly dual to: twodistinct lines intersect inexactly one point.

Looking for missing intersections (II):

x

y

( 3, 0 )

(0, 2) Circle: x2 + y2 = 3Line: y = 2Intersection points:x2 + 22 = 3, that isx2 + 4 = 3, that is x2 = −1.

√−1 = i

Intersection points: (i , 2) e (−i , 2).

Looking for missing intersections (II):

x

y

( 3, 0 )

(0, 2)

Circle: x2 + y2 = 3Line: y = 2Intersection points:x2 + 22 = 3, that isx2 + 4 = 3, that is x2 = −1.

√−1 = i

Intersection points: (i , 2) e (−i , 2).

Looking for missing intersections (II):

x

y

( 3, 0 )

(0, 2) Circle: x2 + y2 = 3Line: y = 2Intersection points:x2 + 22 = 3, that isx2 + 4 = 3, that is x2 = −1.

√−1 = i

Intersection points: (i , 2) e (−i , 2).

Looking for missing intersections (II):

x

y

( 3, 0 )

(0, 2) Circle: x2 + y2 = 3Line: y = 2Intersection points:x2 + 22 = 3, that isx2 + 4 = 3, that is x2 = −1.

√−1 = i

Intersection points: (i , 2) e (−i , 2).

Looking for missing intersections (II):

x

y

( 3, 0 )

(0, 2) Circle: x2 + y2 = 3Line: y = 2Intersection points:x2 + 22 = 3, that isx2 + 4 = 3, that is x2 = −1.

√−1 = i

Intersection points: (i , 2) e (−i , 2).

Numbers:1, 2, 3, . . .

0, 1, 2, 3, . . .

· · · − 3,−2,−1, 0, 1, 2, 3, . . .

−3

2,

7

2,

13

3

x2 = 2

The real line R:

Numbers:1, 2, 3, . . .

0, 1, 2, 3, . . .

· · · − 3,−2,−1, 0, 1, 2, 3, . . .

−3

2,

7

2,

13

3

x2 = 2

The real line R:

Numbers:1, 2, 3, . . .

0, 1, 2, 3, . . .

· · · − 3,−2,−1, 0, 1, 2, 3, . . .

−3

2,

7

2,

13

3

x2 = 2

The real line R:

Numbers:1, 2, 3, . . .

0, 1, 2, 3, . . .

· · · − 3,−2,−1, 0, 1, 2, 3, . . .

−3

2,

7

2,

13

3

x2 = 2

The real line R:

Numbers:1, 2, 3, . . .

0, 1, 2, 3, . . .

· · · − 3,−2,−1, 0, 1, 2, 3, . . .

−3

2,

7

2,

13

3

2

1

1

x2 = 2

The real line R:

Numbers:1, 2, 3, . . .

0, 1, 2, 3, . . .

· · · − 3,−2,−1, 0, 1, 2, 3, . . .

−3

2,

7

2,

13

3

2

1

1

x2 = 2

1. 2

π

The real line R:

Numbers:1, 2, 3, . . .

0, 1, 2, 3, . . .

· · · − 3,−2,−1, 0, 1, 2, 3, . . .

−3

2,

7

2,

13

3

2

1

1

x2 = 2

1. 2

π

The real line R:

.. . . ....π21 30 2-1

.5 2-8 3

Nicolo Tartaglia(Brescia 1500 - Venezia 1557)

Gerolamo Cardano(1515 Pavia - Roma 1576)

”Ars Magna”

Raffaele Bombelli(Bologna 1526 - Roma 1572)”Algebra”

Omar KhayyamGhiyath al-Din Abu’l-FathUmar ibn Ibrahim Al-Nisaburial-Khayyami(Nishapur 1048 - 1131)

Nicolo Tartaglia(Brescia 1500 - Venezia 1557)

Gerolamo Cardano(1515 Pavia - Roma 1576)

”Ars Magna”

Raffaele Bombelli(Bologna 1526 - Roma 1572)”Algebra”

Omar KhayyamGhiyath al-Din Abu’l-FathUmar ibn Ibrahim Al-Nisaburial-Khayyami(Nishapur 1048 - 1131)

Nicolo Tartaglia(Brescia 1500 - Venezia 1557)

Gerolamo Cardano(1515 Pavia - Roma 1576)

”Ars Magna”

Raffaele Bombelli(Bologna 1526 - Roma 1572)”Algebra”

Omar KhayyamGhiyath al-Din Abu’l-FathUmar ibn Ibrahim Al-Nisaburial-Khayyami(Nishapur 1048 - 1131)

Nicolo Tartaglia(Brescia 1500 - Venezia 1557)

Gerolamo Cardano(1515 Pavia - Roma 1576)

”Ars Magna”

Raffaele Bombelli(Bologna 1526 - Roma 1572)”Algebra”

Omar KhayyamGhiyath al-Din Abu’l-FathUmar ibn Ibrahim Al-Nisaburial-Khayyami(Nishapur 1048 - 1131)

Caspar Wessel(1745 - 1818)Geometrical interpretation ofcomplex numbers.

The complex plane C:Instead of a real variable x , one considers a complex variablez = u + iv and instead of the real variable y , one considers acomplex variable w = ξ + iη. What happens to plane curves?

Caspar Wessel(1745 - 1818)Geometrical interpretation ofcomplex numbers.

The complex plane C:

.

.

.. .

.3i+2

i

2i

-i

1 2

-1=

Instead of a real variable x , one considers a complex variablez = u + iv and instead of the real variable y , one considers acomplex variable w = ξ + iη. What happens to plane curves?

Caspar Wessel(1745 - 1818)Geometrical interpretation ofcomplex numbers.

The complex plane C:

.

.

.. .

.3i+2

i

2i

-i

1 2

-1=

Instead of a real variable x , one considers a complex variablez = u + iv and instead of the real variable y , one considers acomplex variable w = ξ + iη. What happens to plane curves?

Descartes:

A plane algebraic curve isgiven by a polynomial equationP(x , y) = 0 , in the real planewith coordinates x e y .

For example:

line: P(x , y) = x − y + 1circle: P(x , y) = x2 + y2 − 1cubic : P(x , y) = x3 − x2 − y2

What happens in the complexplane with complexcoordinates z e w ?

Descartes:

A plane algebraic curve isgiven by a polynomial equationP(x , y) = 0 , in the real planewith coordinates x e y .

For example:

line: P(x , y) = x − y + 1circle: P(x , y) = x2 + y2 − 1cubic : P(x , y) = x3 − x2 − y2

What happens in the complexplane with complexcoordinates z e w ?

Descartes:

A plane algebraic curve isgiven by a polynomial equationP(x , y) = 0 , in the real planewith coordinates x e y .

For example:

line: P(x , y) = x − y + 1circle: P(x , y) = x2 + y2 − 1cubic : P(x , y) = x3 − x2 − y2

x

y

P(x,y)=0

What happens in the complexplane with complexcoordinates z e w ?

Descartes:

A plane algebraic curve isgiven by a polynomial equationP(x , y) = 0 , in the real planewith coordinates x e y .

For example:

line: P(x , y) = x − y + 1circle: P(x , y) = x2 + y2 − 1cubic : P(x , y) = x3 − x2 − y2

x

y

P(x,y)=0

What happens in the complexplane with complexcoordinates z e w ?

Descartes:

A plane algebraic curve isgiven by a polynomial equationP(x , y) = 0 , in the real planewith coordinates x e y .

For example:

line: P(x , y) = x − y + 1circle: P(x , y) = x2 + y2 − 1cubic : P(x , y) = x3 − x2 − y2

x

y

P(x,y)=0

What happens in the complexplane with complexcoordinates z e w ?

P(z, w)=0 ?

z=u+iv

w=s+it

Bernhard Riemann(Breselenz [Hanover] 1826- Selasca [Como] 1866)

22

y

x

x − 23y − 1 = 0

z − 23w − 1 = 0

x2 + y2 = 1 z2 + w2 = 1

y

x

x − 23y − 1 = 0

z

w

z − 23w − 1 = 0

x2 + y2 = 1 z2 + w2 = 1

y

x

x − 23y − 1 = 0

z

w

z − 23w − 1 = 0

x

y

x2 + y2 = 1

z2 + w2 = 1

y

x

x − 23y − 1 = 0

z

w

z − 23w − 1 = 0

x

y

x2 + y2 = 1 z

w

z2 + w2 = 1

x

y

y2 = x3 − x

w2 = z3 − z

x4 + y4 = 1 z4 + w4 = 1

x

y

y2 = x3 − x

w

z

w2 = z3 − z

x4 + y4 = 1 z4 + w4 = 1

x

y

y2 = x3 − x

w

z

w2 = z3 − z

x

y

x4 + y4 = 1

z4 + w4 = 1

x

y

y2 = x3 − x

w

z

w2 = z3 − z

x

y

x4 + y4 = 1 z

w

z4 + w4 = 1

In conclusion, in the complex projective plane P2C, with complexcoordinates z and w , the solutions to the equation P(z ,w) = 0form a surface which is called a Rieman surface. The number of”holes” of this surface is called the genus of the surface and it isdenoted with the letter g.

In conclusion, in the complex projective plane P2C, with complexcoordinates z and w , the solutions to the equation P(z ,w) = 0form a surface which is called a Rieman surface. The number of”holes” of this surface is called the genus of the surface and it isdenoted with the letter g.

z

w........... P(z, w)=0

Riemann pulled algebraic curves out of their ambient space andmade them live in thin air.

So, when considering the cubic curve

Γ : y2 = x3 − 1 ,

one is really looking at an abstract, genus 1, compact Riemannsurface C and at pair of meromorphic functions x , y ∈M(C )realizing the embedding of C in PC2 (the poles of x and y go theline at infinity). The Riemann surface C is just a compact analyticmanifold of dimension 1.

(x,y)C Γ

Riemann pulled algebraic curves out of their ambient space andmade them live in thin air. So, when considering the cubic curve

Γ : y2 = x3 − 1 ,

one is really looking at an abstract, genus 1, compact Riemannsurface C and at pair of meromorphic functions x , y ∈M(C )realizing the embedding of C in PC2 (the poles of x and y go theline at infinity). The Riemann surface C is just a compact analyticmanifold of dimension 1.

(x,y)C Γ

Riemann pulled algebraic curves out of their ambient space andmade them live in thin air. So, when considering the cubic curve

Γ : y2 = x3 − 1 ,

one is really looking at an abstract, genus 1, compact Riemannsurface C and at pair of meromorphic functions x , y ∈M(C )realizing the embedding of C in PC2 (the poles of x and y go theline at infinity).

The Riemann surface C is just a compact analyticmanifold of dimension 1.

(x,y)C Γ

Riemann pulled algebraic curves out of their ambient space andmade them live in thin air. So, when considering the cubic curve

Γ : y2 = x3 − 1 ,

one is really looking at an abstract, genus 1, compact Riemannsurface C and at pair of meromorphic functions x , y ∈M(C )realizing the embedding of C in PC2 (the poles of x and y go theline at infinity). The Riemann surface C is just a compact analyticmanifold of dimension 1.

(x,y)C Γ

The Riemann surface C is the correct ambient space to dofunction theory in one variable, i.e. the theory of holomorphic andmeromorphic functions in one variable.

Choosing r meromorphicfunctions on C yields an analytic map from C to PCr andtherefore a projective realization of C . For instance, in the exampleabove, we could have looked only at the function x , then we wouldbe realizing C as a 2-sheeted cover of PC1. Looking at y , on theother hand, is like presenting C as a 3-sheeted cover of PC1.Bringing into the picture a third function z would map C to PC4

realizing it, perhaps, as a smooth quartic curve.From this non-cartesian point of view, algebraic equations are onlylinked to the accidental projective manifestations of a Riemannsurface and they position themselves in the background.

The Riemann surface C is the correct ambient space to dofunction theory in one variable, i.e. the theory of holomorphic andmeromorphic functions in one variable. Choosing r meromorphicfunctions on C yields an analytic map from C to PCr andtherefore a projective realization of C .

For instance, in the exampleabove, we could have looked only at the function x , then we wouldbe realizing C as a 2-sheeted cover of PC1. Looking at y , on theother hand, is like presenting C as a 3-sheeted cover of PC1.Bringing into the picture a third function z would map C to PC4

realizing it, perhaps, as a smooth quartic curve.From this non-cartesian point of view, algebraic equations are onlylinked to the accidental projective manifestations of a Riemannsurface and they position themselves in the background.

The Riemann surface C is the correct ambient space to dofunction theory in one variable, i.e. the theory of holomorphic andmeromorphic functions in one variable. Choosing r meromorphicfunctions on C yields an analytic map from C to PCr andtherefore a projective realization of C . For instance, in the exampleabove, we could have looked only at the function x , then we wouldbe realizing C as a 2-sheeted cover of PC1.

Looking at y , on theother hand, is like presenting C as a 3-sheeted cover of PC1.Bringing into the picture a third function z would map C to PC4

realizing it, perhaps, as a smooth quartic curve.From this non-cartesian point of view, algebraic equations are onlylinked to the accidental projective manifestations of a Riemannsurface and they position themselves in the background.

The Riemann surface C is the correct ambient space to dofunction theory in one variable, i.e. the theory of holomorphic andmeromorphic functions in one variable. Choosing r meromorphicfunctions on C yields an analytic map from C to PCr andtherefore a projective realization of C . For instance, in the exampleabove, we could have looked only at the function x , then we wouldbe realizing C as a 2-sheeted cover of PC1. Looking at y , on theother hand, is like presenting C as a 3-sheeted cover of PC1.

Bringing into the picture a third function z would map C to PC4

realizing it, perhaps, as a smooth quartic curve.From this non-cartesian point of view, algebraic equations are onlylinked to the accidental projective manifestations of a Riemannsurface and they position themselves in the background.

The Riemann surface C is the correct ambient space to dofunction theory in one variable, i.e. the theory of holomorphic andmeromorphic functions in one variable. Choosing r meromorphicfunctions on C yields an analytic map from C to PCr andtherefore a projective realization of C . For instance, in the exampleabove, we could have looked only at the function x , then we wouldbe realizing C as a 2-sheeted cover of PC1. Looking at y , on theother hand, is like presenting C as a 3-sheeted cover of PC1.Bringing into the picture a third function z would map C to PC4

realizing it, perhaps, as a smooth quartic curve.

From this non-cartesian point of view, algebraic equations are onlylinked to the accidental projective manifestations of a Riemannsurface and they position themselves in the background.

The Riemann surface C is the correct ambient space to dofunction theory in one variable, i.e. the theory of holomorphic andmeromorphic functions in one variable. Choosing r meromorphicfunctions on C yields an analytic map from C to PCr andtherefore a projective realization of C . For instance, in the exampleabove, we could have looked only at the function x , then we wouldbe realizing C as a 2-sheeted cover of PC1. Looking at y , on theother hand, is like presenting C as a 3-sheeted cover of PC1.Bringing into the picture a third function z would map C to PC4

realizing it, perhaps, as a smooth quartic curve.From this non-cartesian point of view, algebraic equations are onlylinked to the accidental projective manifestations of a Riemannsurface and they position themselves in the background.

Now that algebraic curves are pulled out from an ambient space, itis their intrinsic geometry that comes in the forefront.

From manypoints of view, two Riemann surfaces that are bianalyticallyequivalent (i.e. isomorphic) are indistinguishable. For instance theyhave exactly the same projective realizations.

Mg = {Riemann surfaces of genus g}/isomorphisms

This moduli space exists and it is an essentially smooth, complexvariety of dimension 3g − 3. (There is an exception when thegenus is 1. In fact, in order to prevent the occurrence of infinitelymany automorphisms one should always choose a point on a genus1 Riemann surface and insist that any automorphism should keepthat marked point fixed.)

Now that algebraic curves are pulled out from an ambient space, itis their intrinsic geometry that comes in the forefront. From manypoints of view, two Riemann surfaces that are bianalyticallyequivalent (i.e. isomorphic) are indistinguishable. For instance theyhave exactly the same projective realizations.

Mg = {Riemann surfaces of genus g}/isomorphisms

This moduli space exists and it is an essentially smooth, complexvariety of dimension 3g − 3. (There is an exception when thegenus is 1. In fact, in order to prevent the occurrence of infinitelymany automorphisms one should always choose a point on a genus1 Riemann surface and insist that any automorphism should keepthat marked point fixed.)

Now that algebraic curves are pulled out from an ambient space, itis their intrinsic geometry that comes in the forefront. From manypoints of view, two Riemann surfaces that are bianalyticallyequivalent (i.e. isomorphic) are indistinguishable. For instance theyhave exactly the same projective realizations.

Mg = {Riemann surfaces of genus g}/isomorphisms

This moduli space exists and it is an essentially smooth, complexvariety of dimension 3g − 3. (There is an exception when thegenus is 1. In fact, in order to prevent the occurrence of infinitelymany automorphisms one should always choose a point on a genus1 Riemann surface and insist that any automorphism should keepthat marked point fixed.)

Now that algebraic curves are pulled out from an ambient space, itis their intrinsic geometry that comes in the forefront. From manypoints of view, two Riemann surfaces that are bianalyticallyequivalent (i.e. isomorphic) are indistinguishable. For instance theyhave exactly the same projective realizations.

Mg = {Riemann surfaces of genus g}/isomorphisms

This moduli space exists and it is an essentially smooth, complexvariety of dimension 3g − 3.

(There is an exception when thegenus is 1. In fact, in order to prevent the occurrence of infinitelymany automorphisms one should always choose a point on a genus1 Riemann surface and insist that any automorphism should keepthat marked point fixed.)

Now that algebraic curves are pulled out from an ambient space, itis their intrinsic geometry that comes in the forefront. From manypoints of view, two Riemann surfaces that are bianalyticallyequivalent (i.e. isomorphic) are indistinguishable. For instance theyhave exactly the same projective realizations.

Mg = {Riemann surfaces of genus g}/isomorphisms

This moduli space exists and it is an essentially smooth, complexvariety of dimension 3g − 3. (There is an exception when thegenus is 1. In fact, in order to prevent the occurrence of infinitelymany automorphisms one should always choose a point on a genus1 Riemann surface and insist that any automorphism should keepthat marked point fixed.)

In some sense, the moduli space Mg plays the same role as themoduli space of circles that we saw before.

To solve anenumerative problem concerning circles, we translated this problemin an intersection problem in the moduli space. Thus one canimagine that to solve enumerative problems concerning algebraiccurves one should have a good understanding of the intersectiontheory of Mg .

In some sense, the moduli space Mg plays the same role as themoduli space of circles that we saw before. To solve anenumerative problem concerning circles, we translated this problemin an intersection problem in the moduli space.

Thus one canimagine that to solve enumerative problems concerning algebraiccurves one should have a good understanding of the intersectiontheory of Mg .

In some sense, the moduli space Mg plays the same role as themoduli space of circles that we saw before. To solve anenumerative problem concerning circles, we translated this problemin an intersection problem in the moduli space. Thus one canimagine that to solve enumerative problems concerning algebraiccurves one should have a good understanding of the intersectiontheory of Mg .

A quick way to see why the isomorphism class of a compactRiemann surface of genus g > 1 depends on 3g − 3 complexparameters, or 6g − 6 real ones, is to decompose the surface in2g − 2 pants by suitably cutting it along 3g − 3 curves:

We can endow, in a unique way, the Riemann surface C with acomplete hyperbolic metric with constant curvature equal to -1,and we can assume that the 3g − 3 dissecting curves are geodesics.Their lengths provide 3g − 3 real moduli. Once these are fixed, thevarious pants are analytically rigid and the only free parametersinvolved in reconstructing C from them are the 3g − 3 twists thatwe can perform when identifying their boundary curves. These arethe additional 3g − 3 real moduli.

A quick way to see why the isomorphism class of a compactRiemann surface of genus g > 1 depends on 3g − 3 complexparameters, or 6g − 6 real ones, is to decompose the surface in2g − 2 pants by suitably cutting it along 3g − 3 curves:

We can endow, in a unique way, the Riemann surface C with acomplete hyperbolic metric with constant curvature equal to -1,and we can assume that the 3g − 3 dissecting curves are geodesics.Their lengths provide 3g − 3 real moduli. Once these are fixed, thevarious pants are analytically rigid and the only free parametersinvolved in reconstructing C from them are the 3g − 3 twists thatwe can perform when identifying their boundary curves. These arethe additional 3g − 3 real moduli.

A quick way to see why the isomorphism class of a compactRiemann surface of genus g > 1 depends on 3g − 3 complexparameters, or 6g − 6 real ones, is to decompose the surface in2g − 2 pants by suitably cutting it along 3g − 3 curves:

We can endow, in a unique way, the Riemann surface C with acomplete hyperbolic metric with constant curvature equal to -1,and we can assume that the 3g − 3 dissecting curves are geodesics.

Their lengths provide 3g − 3 real moduli. Once these are fixed, thevarious pants are analytically rigid and the only free parametersinvolved in reconstructing C from them are the 3g − 3 twists thatwe can perform when identifying their boundary curves. These arethe additional 3g − 3 real moduli.

A quick way to see why the isomorphism class of a compactRiemann surface of genus g > 1 depends on 3g − 3 complexparameters, or 6g − 6 real ones, is to decompose the surface in2g − 2 pants by suitably cutting it along 3g − 3 curves:

We can endow, in a unique way, the Riemann surface C with acomplete hyperbolic metric with constant curvature equal to -1,and we can assume that the 3g − 3 dissecting curves are geodesics.Their lengths provide 3g − 3 real moduli.

Once these are fixed, thevarious pants are analytically rigid and the only free parametersinvolved in reconstructing C from them are the 3g − 3 twists thatwe can perform when identifying their boundary curves. These arethe additional 3g − 3 real moduli.

A quick way to see why the isomorphism class of a compactRiemann surface of genus g > 1 depends on 3g − 3 complexparameters, or 6g − 6 real ones, is to decompose the surface in2g − 2 pants by suitably cutting it along 3g − 3 curves:

We can endow, in a unique way, the Riemann surface C with acomplete hyperbolic metric with constant curvature equal to -1,and we can assume that the 3g − 3 dissecting curves are geodesics.Their lengths provide 3g − 3 real moduli. Once these are fixed, thevarious pants are analytically rigid and the only free parametersinvolved in reconstructing C from them are the 3g − 3 twists thatwe can perform when identifying their boundary curves.

These arethe additional 3g − 3 real moduli.

A quick way to see why the isomorphism class of a compactRiemann surface of genus g > 1 depends on 3g − 3 complexparameters, or 6g − 6 real ones, is to decompose the surface in2g − 2 pants by suitably cutting it along 3g − 3 curves:

We can endow, in a unique way, the Riemann surface C with acomplete hyperbolic metric with constant curvature equal to -1,and we can assume that the 3g − 3 dissecting curves are geodesics.Their lengths provide 3g − 3 real moduli. Once these are fixed, thevarious pants are analytically rigid and the only free parametersinvolved in reconstructing C from them are the 3g − 3 twists thatwe can perform when identifying their boundary curves. These arethe additional 3g − 3 real moduli.

Let us go back to a plane curve given by an equation P(z ,w) = 0.How does one compute the genus of a plane curve?

Examples:

line : z + w = 1 g = 0 ,

conic : z2 + w2 = 1 g = 0 ,

cubic : z3 + w3 = 1 g = 1 ,

quartic : z4 + w4 = 1 g = 3 ,

curve of degree d : zd + wd = 1 g =(d − 1)(d − 2)

2.

A curve of genus 0 is the natural generalization of a line.At first sight, it would seem that the only genus zero curves arethe lines and the conics.But it is not so. This depends on the fact that a plane curve mayhave ”nodes”. Let us look at a cubic:

30

Let us go back to a plane curve given by an equation P(z ,w) = 0.How does one compute the genus of a plane curve?Examples:

line : z + w = 1 g = 0 ,

conic : z2 + w2 = 1 g = 0 ,

cubic : z3 + w3 = 1 g = 1 ,

quartic : z4 + w4 = 1 g = 3 ,

curve of degree d : zd + wd = 1 g =(d − 1)(d − 2)

2.

A curve of genus 0 is the natural generalization of a line.At first sight, it would seem that the only genus zero curves arethe lines and the conics.But it is not so. This depends on the fact that a plane curve mayhave ”nodes”. Let us look at a cubic:

30

Let us go back to a plane curve given by an equation P(z ,w) = 0.How does one compute the genus of a plane curve?Examples:

line : z + w = 1 g = 0 ,

conic : z2 + w2 = 1 g = 0 ,

cubic : z3 + w3 = 1 g = 1 ,

quartic : z4 + w4 = 1 g = 3 ,

curve of degree d : zd + wd = 1 g =(d − 1)(d − 2)

2.

A curve of genus 0 is the natural generalization of a line.At first sight, it would seem that the only genus zero curves arethe lines and the conics.But it is not so. This depends on the fact that a plane curve mayhave ”nodes”. Let us look at a cubic:

30

Let us go back to a plane curve given by an equation P(z ,w) = 0.How does one compute the genus of a plane curve?Examples:

line : z + w = 1 g = 0 ,

conic : z2 + w2 = 1 g = 0 ,

cubic : z3 + w3 = 1 g = 1 ,

quartic : z4 + w4 = 1 g = 3 ,

curve of degree d : zd + wd = 1 g =(d − 1)(d − 2)

2.

A curve of genus 0 is the natural generalization of a line.At first sight, it would seem that the only genus zero curves arethe lines and the conics.But it is not so. This depends on the fact that a plane curve mayhave ”nodes”. Let us look at a cubic:

30

Let us go back to a plane curve given by an equation P(z ,w) = 0.How does one compute the genus of a plane curve?Examples:

line : z + w = 1 g = 0 ,

conic : z2 + w2 = 1 g = 0 ,

cubic : z3 + w3 = 1 g = 1 ,

quartic : z4 + w4 = 1 g = 3 ,

curve of degree d : zd + wd = 1 g =(d − 1)(d − 2)

2.

A curve of genus 0 is the natural generalization of a line.At first sight, it would seem that the only genus zero curves arethe lines and the conics.But it is not so. This depends on the fact that a plane curve mayhave ”nodes”. Let us look at a cubic:

30

Let us go back to a plane curve given by an equation P(z ,w) = 0.How does one compute the genus of a plane curve?Examples:

line : z + w = 1 g = 0 ,

conic : z2 + w2 = 1 g = 0 ,

cubic : z3 + w3 = 1 g = 1 ,

quartic : z4 + w4 = 1 g = 3 ,

curve of degree d : zd + wd = 1 g =(d − 1)(d − 2)

2.

A curve of genus 0 is the natural generalization of a line.At first sight, it would seem that the only genus zero curves arethe lines and the conics.But it is not so. This depends on the fact that a plane curve mayhave ”nodes”. Let us look at a cubic:

30

Let us go back to a plane curve given by an equation P(z ,w) = 0.How does one compute the genus of a plane curve?Examples:

line : z + w = 1 g = 0 ,

conic : z2 + w2 = 1 g = 0 ,

cubic : z3 + w3 = 1 g = 1 ,

quartic : z4 + w4 = 1 g = 3 ,

curve of degree d : zd + wd = 1 g =(d − 1)(d − 2)

2.

A curve of genus 0 is the natural generalization of a line.

At first sight, it would seem that the only genus zero curves arethe lines and the conics.But it is not so. This depends on the fact that a plane curve mayhave ”nodes”. Let us look at a cubic:

30

Let us go back to a plane curve given by an equation P(z ,w) = 0.How does one compute the genus of a plane curve?Examples:

line : z + w = 1 g = 0 ,

conic : z2 + w2 = 1 g = 0 ,

cubic : z3 + w3 = 1 g = 1 ,

quartic : z4 + w4 = 1 g = 3 ,

curve of degree d : zd + wd = 1 g =(d − 1)(d − 2)

2.

A curve of genus 0 is the natural generalization of a line.At first sight, it would seem that the only genus zero curves arethe lines and the conics.

But it is not so. This depends on the fact that a plane curve mayhave ”nodes”. Let us look at a cubic:

30

Let us go back to a plane curve given by an equation P(z ,w) = 0.How does one compute the genus of a plane curve?Examples:

line : z + w = 1 g = 0 ,

conic : z2 + w2 = 1 g = 0 ,

cubic : z3 + w3 = 1 g = 1 ,

quartic : z4 + w4 = 1 g = 3 ,

curve of degree d : zd + wd = 1 g =(d − 1)(d − 2)

2.

A curve of genus 0 is the natural generalization of a line.At first sight, it would seem that the only genus zero curves arethe lines and the conics.But it is not so.

This depends on the fact that a plane curve mayhave ”nodes”. Let us look at a cubic:

30

Let us go back to a plane curve given by an equation P(z ,w) = 0.How does one compute the genus of a plane curve?Examples:

line : z + w = 1 g = 0 ,

conic : z2 + w2 = 1 g = 0 ,

cubic : z3 + w3 = 1 g = 1 ,

quartic : z4 + w4 = 1 g = 3 ,

curve of degree d : zd + wd = 1 g =(d − 1)(d − 2)

2.

A curve of genus 0 is the natural generalization of a line.At first sight, it would seem that the only genus zero curves arethe lines and the conics.But it is not so. This depends on the fact that a plane curve mayhave ”nodes”. Let us look at a cubic:

30

x

y

y2 = x3 − x

w2 = z3 − z

y2 = x3 − x2 w2 = z3 − z2

x

y

y2 = x3 − x

w

z

w2 = z3 − z

y2 = x3 − x2 w2 = z3 − z2

x

y

y2 = x3 − x

w

z

w2 = z3 − z

x

y

y2 = x3 − x2

w2 = z3 − z2

x

y

y2 = x3 − x

w

z

w2 = z3 − z

x

y

y2 = x3 − x2 z

w

w2 = z3 − z2

A cubic with one node should be considered as a surface of genus0 and not of genus 1:

In an analogous way a surface like:

should be considered of genus3 and not of genus 5!

A cubic with one node should be considered as a surface of genus0 and not of genus 1:

In an analogous way a surface like:

should be considered of genus3 and not of genus 5!

A cubic with one node should be considered as a surface of genus0 and not of genus 1:

In an analogous way a surface like:

should be considered of genus3 and not of genus 5!

A cubic with one node should be considered as a surface of genus0 and not of genus 1:

In an analogous way a surface like:

should be considered of genus3 and not of genus 5!

A cubic with one node should be considered as a surface of genus0 and not of genus 1:

In an analogous way a surface like:

should be considered of genus3 and not of genus 5!

A cubic with one node should be considered as a surface of genus0 and not of genus 1:

In an analogous way a surface like:

should be considered of genus3 and not of genus 5!

A cubic with one node should be considered as a surface of genus0 and not of genus 1:

In an analogous way a surface like:

should be considered of genus3 and not of genus 5!

A cubic with one node should be considered as a surface of genus0 and not of genus 1:

In an analogous way a surface like:

should be considered of genus3 and not of genus 5!

In concusion: a degree d plane curve with δ nodes should beconsidered as a Riemann surface of genus

g =(d − 1)(d − 2)

2− δ .

Thus there are many genus 0 curves ! These are all degree d theplane curves with

δ =(d − 1)(d − 2)

2.

nodes. We now treat genus 0 curves in the way Euclid andApollonius were treating lines and conics. We can immediately seeone difference. Whereas, according to Euclid, there is a uniqueline through 2 distinct points and, according to Apollonius, there isa unique conic through 5 points in general position, things are notso simple for genus 0 curves of degree d , as soon as d > 2. Theonly thing that one can say without difficulty is that there is afinite number of degree d , genus 0, plane curves passing through3d − 1 points in general position. Let Nd be this number. How tocompute Nd?

In concusion: a degree d plane curve with δ nodes should beconsidered as a Riemann surface of genus

g =(d − 1)(d − 2)

2− δ .

Thus there are many genus 0 curves ! These are all degree d theplane curves with

δ =(d − 1)(d − 2)

2.

nodes. We now treat genus 0 curves in the way Euclid andApollonius were treating lines and conics. We can immediately seeone difference. Whereas, according to Euclid, there is a uniqueline through 2 distinct points and, according to Apollonius, there isa unique conic through 5 points in general position, things are notso simple for genus 0 curves of degree d , as soon as d > 2. Theonly thing that one can say without difficulty is that there is afinite number of degree d , genus 0, plane curves passing through3d − 1 points in general position. Let Nd be this number. How tocompute Nd?

In concusion: a degree d plane curve with δ nodes should beconsidered as a Riemann surface of genus

g =(d − 1)(d − 2)

2− δ .

Thus there are many genus 0 curves !

These are all degree d theplane curves with

δ =(d − 1)(d − 2)

2.

nodes. We now treat genus 0 curves in the way Euclid andApollonius were treating lines and conics. We can immediately seeone difference. Whereas, according to Euclid, there is a uniqueline through 2 distinct points and, according to Apollonius, there isa unique conic through 5 points in general position, things are notso simple for genus 0 curves of degree d , as soon as d > 2. Theonly thing that one can say without difficulty is that there is afinite number of degree d , genus 0, plane curves passing through3d − 1 points in general position. Let Nd be this number. How tocompute Nd?

In concusion: a degree d plane curve with δ nodes should beconsidered as a Riemann surface of genus

g =(d − 1)(d − 2)

2− δ .

Thus there are many genus 0 curves ! These are all degree d theplane curves with

δ =(d − 1)(d − 2)

2.

nodes.

We now treat genus 0 curves in the way Euclid andApollonius were treating lines and conics. We can immediately seeone difference. Whereas, according to Euclid, there is a uniqueline through 2 distinct points and, according to Apollonius, there isa unique conic through 5 points in general position, things are notso simple for genus 0 curves of degree d , as soon as d > 2. Theonly thing that one can say without difficulty is that there is afinite number of degree d , genus 0, plane curves passing through3d − 1 points in general position. Let Nd be this number. How tocompute Nd?

In concusion: a degree d plane curve with δ nodes should beconsidered as a Riemann surface of genus

g =(d − 1)(d − 2)

2− δ .

Thus there are many genus 0 curves ! These are all degree d theplane curves with

δ =(d − 1)(d − 2)

2.

nodes. We now treat genus 0 curves in the way Euclid andApollonius were treating lines and conics.

We can immediately seeone difference. Whereas, according to Euclid, there is a uniqueline through 2 distinct points and, according to Apollonius, there isa unique conic through 5 points in general position, things are notso simple for genus 0 curves of degree d , as soon as d > 2. Theonly thing that one can say without difficulty is that there is afinite number of degree d , genus 0, plane curves passing through3d − 1 points in general position. Let Nd be this number. How tocompute Nd?

In concusion: a degree d plane curve with δ nodes should beconsidered as a Riemann surface of genus

g =(d − 1)(d − 2)

2− δ .

Thus there are many genus 0 curves ! These are all degree d theplane curves with

δ =(d − 1)(d − 2)

2.

nodes. We now treat genus 0 curves in the way Euclid andApollonius were treating lines and conics. We can immediately seeone difference.

Whereas, according to Euclid, there is a uniqueline through 2 distinct points and, according to Apollonius, there isa unique conic through 5 points in general position, things are notso simple for genus 0 curves of degree d , as soon as d > 2. Theonly thing that one can say without difficulty is that there is afinite number of degree d , genus 0, plane curves passing through3d − 1 points in general position. Let Nd be this number. How tocompute Nd?

In concusion: a degree d plane curve with δ nodes should beconsidered as a Riemann surface of genus

g =(d − 1)(d − 2)

2− δ .

Thus there are many genus 0 curves ! These are all degree d theplane curves with

δ =(d − 1)(d − 2)

2.

nodes. We now treat genus 0 curves in the way Euclid andApollonius were treating lines and conics. We can immediately seeone difference. Whereas, according to Euclid, there is a uniqueline through 2 distinct points and, according to Apollonius, there isa unique conic through 5 points in general position,

things are notso simple for genus 0 curves of degree d , as soon as d > 2. Theonly thing that one can say without difficulty is that there is afinite number of degree d , genus 0, plane curves passing through3d − 1 points in general position. Let Nd be this number. How tocompute Nd?

In concusion: a degree d plane curve with δ nodes should beconsidered as a Riemann surface of genus

g =(d − 1)(d − 2)

2− δ .

Thus there are many genus 0 curves ! These are all degree d theplane curves with

δ =(d − 1)(d − 2)

2.

nodes. We now treat genus 0 curves in the way Euclid andApollonius were treating lines and conics. We can immediately seeone difference. Whereas, according to Euclid, there is a uniqueline through 2 distinct points and, according to Apollonius, there isa unique conic through 5 points in general position, things are notso simple for genus 0 curves of degree d , as soon as d > 2.

Theonly thing that one can say without difficulty is that there is afinite number of degree d , genus 0, plane curves passing through3d − 1 points in general position. Let Nd be this number. How tocompute Nd?

In concusion: a degree d plane curve with δ nodes should beconsidered as a Riemann surface of genus

g =(d − 1)(d − 2)

2− δ .

Thus there are many genus 0 curves ! These are all degree d theplane curves with

δ =(d − 1)(d − 2)

2.

nodes. We now treat genus 0 curves in the way Euclid andApollonius were treating lines and conics. We can immediately seeone difference. Whereas, according to Euclid, there is a uniqueline through 2 distinct points and, according to Apollonius, there isa unique conic through 5 points in general position, things are notso simple for genus 0 curves of degree d , as soon as d > 2. Theonly thing that one can say without difficulty is that there is afinite number of degree d , genus 0, plane curves passing through3d − 1 points in general position.

Let Nd be this number. How tocompute Nd?

In concusion: a degree d plane curve with δ nodes should beconsidered as a Riemann surface of genus

g =(d − 1)(d − 2)

2− δ .

Thus there are many genus 0 curves ! These are all degree d theplane curves with

δ =(d − 1)(d − 2)

2.

nodes. We now treat genus 0 curves in the way Euclid andApollonius were treating lines and conics. We can immediately seeone difference. Whereas, according to Euclid, there is a uniqueline through 2 distinct points and, according to Apollonius, there isa unique conic through 5 points in general position, things are notso simple for genus 0 curves of degree d , as soon as d > 2. Theonly thing that one can say without difficulty is that there is afinite number of degree d , genus 0, plane curves passing through3d − 1 points in general position. Let Nd be this number.

How tocompute Nd?

In concusion: a degree d plane curve with δ nodes should beconsidered as a Riemann surface of genus

g =(d − 1)(d − 2)

2− δ .

Thus there are many genus 0 curves ! These are all degree d theplane curves with

δ =(d − 1)(d − 2)

2.

nodes. We now treat genus 0 curves in the way Euclid andApollonius were treating lines and conics. We can immediately seeone difference. Whereas, according to Euclid, there is a uniqueline through 2 distinct points and, according to Apollonius, there isa unique conic through 5 points in general position, things are notso simple for genus 0 curves of degree d , as soon as d > 2. Theonly thing that one can say without difficulty is that there is afinite number of degree d , genus 0, plane curves passing through3d − 1 points in general position. Let Nd be this number. How tocompute Nd?

Thus the misterious number Nd is number of plane curves ofdegree d and genus 0 passing through 3d − 1 given points ingeneral position.

What to we know about Nd?

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

Schubert 5 14 N5 = 87304

Why do we care?

35

Thus the misterious number Nd is number of plane curves ofdegree d and genus 0 passing through 3d − 1 given points ingeneral position. What to we know about Nd?

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

Schubert 5 14 N5 = 87304

Why do we care?

35

Thus the misterious number Nd is number of plane curves ofdegree d and genus 0 passing through 3d − 1 given points ingeneral position. What to we know about Nd?

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

Schubert 5 14 N5 = 87304

Why do we care?

35

Thus the misterious number Nd is number of plane curves ofdegree d and genus 0 passing through 3d − 1 given points ingeneral position. What to we know about Nd?

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

Schubert 5 14 N5 = 87304

Why do we care?

35

Thus the misterious number Nd is number of plane curves ofdegree d and genus 0 passing through 3d − 1 given points ingeneral position. What to we know about Nd?

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

Schubert 5 14 N5 = 87304

Why do we care?

35

Thus the misterious number Nd is number of plane curves ofdegree d and genus 0 passing through 3d − 1 given points ingeneral position. What to we know about Nd?

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

Schubert 5 14 N5 = 87304

Why do we care?

35

Thus the misterious number Nd is number of plane curves ofdegree d and genus 0 passing through 3d − 1 given points ingeneral position. What to we know about Nd?

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

Schubert 5 14 N5 = 87304

Why do we care?

35

Thus the misterious number Nd is number of plane curves ofdegree d and genus 0 passing through 3d − 1 given points ingeneral position. What to we know about Nd?

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

Schubert 5 14 N5 = 87304

Why do we care?

35

Thus the misterious number Nd is number of plane curves ofdegree d and genus 0 passing through 3d − 1 given points ingeneral position. What to we know about Nd?

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

Schubert 5 14 N5 = 87304

Why do we care?

35

Soliton waves,

J.Scott-Russell (1808-1882)

The ”Scott Russell” Aqueduct, Union Canal, not far fromHeriot-Watt University (July 12, 1995).

Soliton waves,

J.Scott-Russell (1808-1882)

The ”Scott Russell” Aqueduct, Union Canal, not far fromHeriot-Watt University (July 12, 1995).

Soliton waves,

J.Scott-Russell (1808-1882)

The ”Scott Russell” Aqueduct, Union Canal, not far fromHeriot-Watt University (July 12, 1995).

Soliton waves,

J.Scott-Russell (1808-1882)

The ”Scott Russell” Aqueduct, Union Canal, not far fromHeriot-Watt University (July 12, 1995).

Soliton waves,

J.Scott-Russell (1808-1882)

u

x

.u(x,t)

The ”Scott Russell” Aqueduct, Union Canal, not far fromHeriot-Watt University (July 12, 1995).

Soliton waves,

J.Scott-Russell (1808-1882)

u

x

.u(x,t)

The ”Scott Russell” Aqueduct, Union Canal, not far fromHeriot-Watt University (July 12, 1995).

“ I believe I shall best introduce this phenomenon by describing thecircumstances of my own first acquaintances with it. I was observing themotion of a boat which was rapidly drawn along a narrow channel by apair of horses, when the boat suddenly stopped — not so the mass ofwater in the channel which it had put in motion; it accumulated roundthe prow of the vessel in a state of violent agitation, then suddenlyleaving it behind, rolled forward with great velocity, assuming the form ofa large solitary elevation, a rounded, smooth and well defined heap ofwater, which continued its course along the channel apparently withoutchange of form or diminution of speed. I followed it on horseback andovertook it still rolling on at a rate of some eight or nine miles an hour,preserving its original figure some thirty feet long and a foot to a foot anda half in height. Its height gradually diminished and after a chase of oneor two miles I lost it in the windings of the channel. Such in the monthof August 1834 was my first chance interview with that singular andbeautiful phenomenon which I have called the Wave of Translation...”

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

Two soliton waves of differentamplitude and speed,interacting and thencontinuing their course withintact profile and unchangedspeed.

The differential equation governing solitary waves was discoveredby two dutch mathematical-physicists Korteweg and de Vriesaround 1890. This equation is known as KdV equation

ut = 6uux − uxxx , u = u(x , t) .

(ut = c · uxx)

31

The many unexpected incarnations of the KdV

In 1952, in Los Alamos, Fermi, Pasta and Ulam came across theKdV equation studying a system of N particles moving on a line,coupled with a quadratic potential

In 1961, Kadomtzev and Petviashvilii met the KdV in their studyof cosmic plasma.

In 1972, Novikov ran into the KdV in his study of Riemann’s θfunction for hyperelliptic curves.

In 1975, Peter Lax interprets the KdV as a completely inetgrable,infinite dimensional, hamiltonian system. The constants of motionare the eigenvalues of the Schroedinger operator.

L(t) =d2

dx2+ u(x , t) , L(t)v(x , t) = λ · v(x , t) .

The many unexpected incarnations of the KdV

In 1952, in Los Alamos, Fermi, Pasta and Ulam came across theKdV equation studying a system of N particles moving on a line,coupled with a quadratic potential

In 1961, Kadomtzev and Petviashvilii met the KdV in their studyof cosmic plasma.

In 1972, Novikov ran into the KdV in his study of Riemann’s θfunction for hyperelliptic curves.

In 1975, Peter Lax interprets the KdV as a completely inetgrable,infinite dimensional, hamiltonian system. The constants of motionare the eigenvalues of the Schroedinger operator.

L(t) =d2

dx2+ u(x , t) , L(t)v(x , t) = λ · v(x , t) .

The many unexpected incarnations of the KdV

In 1952, in Los Alamos, Fermi, Pasta and Ulam came across theKdV equation studying a system of N particles moving on a line,coupled with a quadratic potential

In 1961, Kadomtzev and Petviashvilii met the KdV in their studyof cosmic plasma.

In 1972, Novikov ran into the KdV in his study of Riemann’s θfunction for hyperelliptic curves.

In 1975, Peter Lax interprets the KdV as a completely inetgrable,infinite dimensional, hamiltonian system. The constants of motionare the eigenvalues of the Schroedinger operator.

L(t) =d2

dx2+ u(x , t) , L(t)v(x , t) = λ · v(x , t) .

The many unexpected incarnations of the KdV

In 1952, in Los Alamos, Fermi, Pasta and Ulam came across theKdV equation studying a system of N particles moving on a line,coupled with a quadratic potential

In 1961, Kadomtzev and Petviashvilii met the KdV in their studyof cosmic plasma.

In 1972, Novikov ran into the KdV in his study of Riemann’s θfunction for hyperelliptic curves.

In 1975, Peter Lax interprets the KdV as a completely inetgrable,infinite dimensional, hamiltonian system. The constants of motionare the eigenvalues of the Schroedinger operator.

L(t) =d2

dx2+ u(x , t) , L(t)v(x , t) = λ · v(x , t) .

The many unexpected incarnations of the KdV

In 1952, in Los Alamos, Fermi, Pasta and Ulam came across theKdV equation studying a system of N particles moving on a line,coupled with a quadratic potential

In 1961, Kadomtzev and Petviashvilii met the KdV in their studyof cosmic plasma.

In 1972, Novikov ran into the KdV in his study of Riemann’s θfunction for hyperelliptic curves.

In 1975, Peter Lax interprets the KdV as a completely inetgrable,infinite dimensional, hamiltonian system.

The constants of motionare the eigenvalues of the Schroedinger operator.

L(t) =d2

dx2+ u(x , t) , L(t)v(x , t) = λ · v(x , t) .

The many unexpected incarnations of the KdV

In 1952, in Los Alamos, Fermi, Pasta and Ulam came across theKdV equation studying a system of N particles moving on a line,coupled with a quadratic potential

In 1961, Kadomtzev and Petviashvilii met the KdV in their studyof cosmic plasma.

In 1972, Novikov ran into the KdV in his study of Riemann’s θfunction for hyperelliptic curves.

In 1975, Peter Lax interprets the KdV as a completely inetgrable,infinite dimensional, hamiltonian system. The constants of motionare the eigenvalues of the Schroedinger operator.

L(t) =d2

dx2+ u(x , t) , L(t)v(x , t) = λ · v(x , t) .

The many unexpected incarnations of the KdV

In 1952, in Los Alamos, Fermi, Pasta and Ulam came across theKdV equation studying a system of N particles moving on a line,coupled with a quadratic potential

In 1961, Kadomtzev and Petviashvilii met the KdV in their studyof cosmic plasma.

In 1972, Novikov ran into the KdV in his study of Riemann’s θfunction for hyperelliptic curves.

In 1975, Peter Lax interprets the KdV as a completely inetgrable,infinite dimensional, hamiltonian system. The constants of motionare the eigenvalues of the Schroedinger operator.

L(t) =d2

dx2+ u(x , t) , L(t)v(x , t) = λ · v(x , t) .

The many unexpected incarnations of the KdV

In 1952, in Los Alamos, Fermi, Pasta and Ulam came across theKdV equation studying a system of N particles moving on a line,coupled with a quadratic potential

In 1961, Kadomtzev and Petviashvilii met the KdV in their studyof cosmic plasma.

In 1972, Novikov ran into the KdV in his study of Riemann’s θfunction for hyperelliptic curves.

In 1975, Peter Lax interprets the KdV as a completely inetgrable,infinite dimensional, hamiltonian system.

In 1990, Douglas, Kazakov introduce the KdV in string theory.

In 1990-1992, Witten e Kontsevich make use of the KdV to solvefundamental problems in enumerative geometry.

The many unexpected incarnations of the KdV

In 1952, in Los Alamos, Fermi, Pasta and Ulam came across theKdV equation studying a system of N particles moving on a line,coupled with a quadratic potential

In 1961, Kadomtzev and Petviashvilii met the KdV in their studyof cosmic plasma.

In 1972, Novikov ran into the KdV in his study of Riemann’s θfunction for hyperelliptic curves.

In 1975, Peter Lax interprets the KdV as a completely inetgrable,infinite dimensional, hamiltonian system.

In 1990, Douglas, Kazakov introduce the KdV in string theory.

In 1990-1992, Witten e Kontsevich make use of the KdV to solvefundamental problems in enumerative geometry.

The many unexpected incarnations of the KdV

In 1952, in Los Alamos, Fermi, Pasta and Ulam came across theKdV equation studying a system of N particles moving on a line,coupled with a quadratic potential

In 1961, Kadomtzev and Petviashvilii met the KdV in their studyof cosmic plasma.

In 1972, Novikov ran into the KdV in his study of Riemann’s θfunction for hyperelliptic curves.

In 1975, Peter Lax interprets the KdV as a completely inetgrable,infinite dimensional, hamiltonian system.

In 1990, Douglas, Kazakov introduce the KdV in string theory.

In 1990-1992, Witten e Kontsevich make use of the KdV to solvefundamental problems in enumerative geometry.

Forces in Nature

Gravity(Newton, Einstein)Elettromagnetic forces

(Maxwell)World of particles:Strong forces.Weak forces.(Planck, Bohr,Shroedinger,Heisenberg)

Forces in Nature

Gravity(Newton, Einstein)

Elettromagnetic forces(Maxwell)World of particles:Strong forces.Weak forces.(Planck, Bohr,Shroedinger,Heisenberg)

Forces in Nature

Gravity(Newton, Einstein)

Elettromagnetic forces(Maxwell)World of particles:Strong forces.Weak forces.(Planck, Bohr,Shroedinger,Heisenberg)

Forces in Nature

Gravity(Newton, Einstein)

Elettromagnetic forces(Maxwell)World of particles:Strong forces.Weak forces.(Planck, Bohr,Shroedinger,Heisenberg)

Forces in Nature

Gravity(Newton, Einstein)

Elettromagnetic forces(Maxwell)

World of particles:Strong forces.Weak forces.(Planck, Bohr,Shroedinger,Heisenberg)

Forces in Nature

Gravity(Newton, Einstein)

Elettromagnetic forces(Maxwell)

World of particles:Strong forces.Weak forces.(Planck, Bohr,Shroedinger,Heisenberg)

Forces in Nature

Gravity(Newton, Einstein)

Elettromagnetic forces(Maxwell)

World of particles:Strong forces.Weak forces.(Planck, Bohr,Shroedinger,Heisenberg)

Forces in Nature

Gravity(Newton, Einstein)

Elettromagnetic forces(Maxwell)

World of particles:Strong forces.Weak forces.(Planck, Bohr,Shroedinger,Heisenberg)

Forces in Nature

Gravity(Newton, Einstein)

Elettromagnetic forces(Maxwell)

World of particles:Strong forces.Weak forces.(Planck, Bohr,Shroedinger,Heisenberg)

Forces in Nature

Gravity(Newton, Einstein)

Elettromagnetic forces(Maxwell)

World of particles:Strong forces.Weak forces.(Planck, Bohr,Shroedinger,Heisenberg)

Forces in Nature

Gravity(Newton, Einstein)

Elettromagnetic forces(Maxwell)

World of particles:Strong forces.Weak forces.(Planck, Bohr,Shroedinger,Heisenberg)

String theory as an attempt to unification.

The problem is to find a geometrical model to reconcile quantummechanics, electromagnetism and gravity

The geometry of general relativity.

Stephen Hawking

The mass tells the space how to curve.The space tells the mass how to move.

String theory as an attempt to unification.

The problem is to find a geometrical model to reconcile quantummechanics, electromagnetism and gravity

The geometry of general relativity.

Stephen Hawking

The mass tells the space how to curve.The space tells the mass how to move.

String theory as an attempt to unification.

The problem is to find a geometrical model to reconcile quantummechanics, electromagnetism and gravity

The geometry of general relativity.

Stephen Hawking

The mass tells the space how to curve.The space tells the mass how to move.

String theory as an attempt to unification.

The problem is to find a geometrical model to reconcile quantummechanics, electromagnetism and gravity

The geometry of general relativity.

Stephen Hawking

The mass tells the space how to curve.The space tells the mass how to move.

String theory as an attempt to unification.

The problem is to find a geometrical model to reconcile quantummechanics, electromagnetism and gravity

The geometry of general relativity.

Stephen Hawking

The mass tells the space how to curve.

The space tells the mass how to move.

String theory as an attempt to unification.

The problem is to find a geometrical model to reconcile quantummechanics, electromagnetism and gravity

The geometry of general relativity.

Stephen Hawking

The mass tells the space how to curve.The space tells the mass how to move.

String theory as an attempt to unification.

The problem is to find a geometrical model to reconcile quantummechanics, electromagnetism and gravity

The geometry of general relativity.

Stephen Hawking

The mass tells the space how to curve.The space tells the mass how to move.

The world of quantum mechanics

The energy and the momenta of elementary particles franticallychange from statum to statum. Particles go through a process ofcontinuous creation and destruction. The notion of a smoothspace, which is central in general relativity seems to be destroid bythe violent fluctuations of quantum mechanics.The world ofgeneral relativity is deterministic the world of quantum mechanicsis governed by Heisenberg’s uncertainty principle.

The world of quantum mechanics

The energy and the momenta of elementary particles franticallychange from statum to statum. Particles go through a process ofcontinuous creation and destruction.

The notion of a smoothspace, which is central in general relativity seems to be destroid bythe violent fluctuations of quantum mechanics.The world ofgeneral relativity is deterministic the world of quantum mechanicsis governed by Heisenberg’s uncertainty principle.

The world of quantum mechanics

The energy and the momenta of elementary particles franticallychange from statum to statum. Particles go through a process ofcontinuous creation and destruction. The notion of a smoothspace, which is central in general relativity seems to be destroid bythe violent fluctuations of quantum mechanics.

The world ofgeneral relativity is deterministic the world of quantum mechanicsis governed by Heisenberg’s uncertainty principle.

The world of quantum mechanics

The energy and the momenta of elementary particles franticallychange from statum to statum. Particles go through a process ofcontinuous creation and destruction. The notion of a smoothspace, which is central in general relativity seems to be destroid bythe violent fluctuations of quantum mechanics.The world ofgeneral relativity is deterministic

the world of quantum mechanicsis governed by Heisenberg’s uncertainty principle.

The world of quantum mechanics

The energy and the momenta of elementary particles franticallychange from statum to statum. Particles go through a process ofcontinuous creation and destruction. The notion of a smoothspace, which is central in general relativity seems to be destroid bythe violent fluctuations of quantum mechanics.The world ofgeneral relativity is deterministic the world of quantum mechanicsis governed by Heisenberg’s uncertainty principle.

Interactions of elementary particles

Collision between an electron and a positron with the emission of aphoton:

Feynman diagrams.R.Feynmann (1918-1988)

Interactions of elementary particles

Collision between an electron and a positron with the emission of aphoton:

Feynman diagrams.R.Feynmann (1918-1988)

Interactions of elementary particles

Collision between an electron and a positron with the emission of aphoton:

e

e

e

+ +

- -

Feynman diagrams.R.Feynmann (1918-1988)

Interactions of elementary particles

Collision between an electron and a positron with the emission of aphoton:

e

e

e

+ +

- -

Feynman diagrams.

R.Feynmann (1918-1988)

Interactions of elementary particles

Collision between an electron and a positron with the emission of aphoton:

e

e

e

+ +

- -

Feynman diagrams.

R.Feynmann (1918-1988)

Interactions of elementary particles

Collision between an electron and a positron with the emission of aphoton:

e

e

e

+ +

- -

Feynman diagrams.

R.Feynmann (1918-1988)

Interactions of elementary particles

Collision between an electron and a positron with the emission of aphoton:

e

e

e

+ +

- -

Feynman diagrams.

R.Feynmann (1918-1988)

Classical mechanics is governed by the principle of action.

Minimizing the action one gets the equation of motion. Fromthese one can describe trajectories.

In quantum mechanics one looks for a partition function. Thisfunction, which is usually denoted with the symbol Z , contains allthe probabilistic information of the event under exam.

One often expresses this function as a series in one or severalparameters (temperature, etc.); sometimes even in infinitely manyparameters

Z = Z (t) = a0 + a1t + a2t2 + a3t3 + · · ·+ ad td + . . .

Z = Z (t0, t1, t2, . . . , tn)

Z = Z (t0, t1, t2, . . . )

Sometimes the partition function can be expressed as an infinitesum where the ”indices” of the sum are Feynman diagrams

Classical mechanics is governed by the principle of action.

Minimizing the action one gets the equation of motion. Fromthese one can describe trajectories.

In quantum mechanics one looks for a partition function. Thisfunction, which is usually denoted with the symbol Z , contains allthe probabilistic information of the event under exam.

One often expresses this function as a series in one or severalparameters (temperature, etc.); sometimes even in infinitely manyparameters

Z = Z (t) = a0 + a1t + a2t2 + a3t3 + · · ·+ ad td + . . .

Z = Z (t0, t1, t2, . . . , tn)

Z = Z (t0, t1, t2, . . . )

Sometimes the partition function can be expressed as an infinitesum where the ”indices” of the sum are Feynman diagrams

Classical mechanics is governed by the principle of action.

Minimizing the action one gets the equation of motion. Fromthese one can describe trajectories.

In quantum mechanics one looks for a partition function. Thisfunction, which is usually denoted with the symbol Z , contains allthe probabilistic information of the event under exam.

One often expresses this function as a series in one or severalparameters (temperature, etc.); sometimes even in infinitely manyparameters

Z = Z (t) = a0 + a1t + a2t2 + a3t3 + · · ·+ ad td + . . .

Z = Z (t0, t1, t2, . . . , tn)

Z = Z (t0, t1, t2, . . . )

Sometimes the partition function can be expressed as an infinitesum where the ”indices” of the sum are Feynman diagrams

Classical mechanics is governed by the principle of action.

Minimizing the action one gets the equation of motion. Fromthese one can describe trajectories.

In quantum mechanics one looks for a partition function. Thisfunction, which is usually denoted with the symbol Z , contains allthe probabilistic information of the event under exam.

One often expresses this function as a series in one or severalparameters (temperature, etc.); sometimes even in infinitely manyparameters

Z = Z (t) = a0 + a1t + a2t2 + a3t3 + · · ·+ ad td + . . .

Z = Z (t0, t1, t2, . . . , tn)

Z = Z (t0, t1, t2, . . . )

Sometimes the partition function can be expressed as an infinitesum where the ”indices” of the sum are Feynman diagrams

Classical mechanics is governed by the principle of action.

Minimizing the action one gets the equation of motion. Fromthese one can describe trajectories.

In quantum mechanics one looks for a partition function. Thisfunction, which is usually denoted with the symbol Z , contains allthe probabilistic information of the event under exam.

One often expresses this function as a series in one or severalparameters (temperature, etc.); sometimes even in infinitely manyparameters

Z = Z (t) = a0 + a1t + a2t2 + a3t3 + · · ·+ ad td + . . .

Z = Z (t0, t1, t2, . . . , tn)

Z = Z (t0, t1, t2, . . . )

Sometimes the partition function can be expressed as an infinitesum where the ”indices” of the sum are Feynman diagrams

Classical mechanics is governed by the principle of action.

Minimizing the action one gets the equation of motion. Fromthese one can describe trajectories.

In quantum mechanics one looks for a partition function. Thisfunction, which is usually denoted with the symbol Z , contains allthe probabilistic information of the event under exam.

One often expresses this function as a series in one or severalparameters (temperature, etc.); sometimes even in infinitely manyparameters

Z = Z (t) = a0 + a1t + a2t2 + a3t3 + · · ·+ ad td + . . .

Z = Z (t0, t1, t2, . . . , tn)

Z = Z (t0, t1, t2, . . . )

Sometimes the partition function can be expressed as an infinitesum where the ”indices” of the sum are Feynman diagrams

Classical mechanics is governed by the principle of action.

Minimizing the action one gets the equation of motion. Fromthese one can describe trajectories.

In quantum mechanics one looks for a partition function. Thisfunction, which is usually denoted with the symbol Z , contains allthe probabilistic information of the event under exam.

One often expresses this function as a series in one or severalparameters (temperature, etc.); sometimes even in infinitely manyparameters

Z = Z (t) = a0 + a1t + a2t2 + a3t3 + · · ·+ ad td + . . .

Z = Z (t0, t1, t2, . . . , tn)

Z = Z (t0, t1, t2, . . . )

Sometimes the partition function can be expressed as an infinitesum where the ”indices” of the sum are Feynman diagrams

Classical mechanics is governed by the principle of action.

Minimizing the action one gets the equation of motion. Fromthese one can describe trajectories.

In quantum mechanics one looks for a partition function. Thisfunction, which is usually denoted with the symbol Z , contains allthe probabilistic information of the event under exam.

One often expresses this function as a series in one or severalparameters (temperature, etc.); sometimes even in infinitely manyparameters

Z = Z (t) = a0 + a1t + a2t2 + a3t3 + · · ·+ ad td + . . .

Z = Z (t0, t1, t2, . . . , tn)

Z = Z (t0, t1, t2, . . . )

Sometimes the partition function can be expressed as an infinitesum where the ”indices” of the sum are Feynman diagrams

String theory started,accidentally, with the workof Gabriele Veneziano onthe so called dual models.

Later Green and Schwarzand especially EdwardWitten proposed stringtheory as a model forunification.

Gabriele Veneziano(Firenze 1942-)CERN Geneva

Edward Witten(Baltimore 1951-)IAS Princeton

The hypothesis is that the various particles (including thegraviton!) correspond to the various ways in which a single stringvibrates. A particle is no longer thought of as a point-like objectbut as a string, which may be open or closed. The various particlesare incarnations of this string. The string is like a violin string andthe patrticles are the musical notes.

String theory started,accidentally, with the workof Gabriele Veneziano onthe so called dual models.

Later Green and Schwarzand especially EdwardWitten proposed stringtheory as a model forunification.

Gabriele Veneziano(Firenze 1942-)CERN Geneva

Edward Witten(Baltimore 1951-)IAS Princeton

The hypothesis is that the various particles (including thegraviton!) correspond to the various ways in which a single stringvibrates. A particle is no longer thought of as a point-like objectbut as a string, which may be open or closed. The various particlesare incarnations of this string. The string is like a violin string andthe patrticles are the musical notes.

String theory started,accidentally, with the workof Gabriele Veneziano onthe so called dual models.Later Green and Schwarzand especially EdwardWitten proposed stringtheory as a model forunification.

Gabriele Veneziano(Firenze 1942-)CERN Geneva

Edward Witten(Baltimore 1951-)IAS Princeton

The hypothesis is that the various particles (including thegraviton!) correspond to the various ways in which a single stringvibrates. A particle is no longer thought of as a point-like objectbut as a string, which may be open or closed. The various particlesare incarnations of this string. The string is like a violin string andthe patrticles are the musical notes.

String theory started,accidentally, with the workof Gabriele Veneziano onthe so called dual models.Later Green and Schwarzand especially EdwardWitten proposed stringtheory as a model forunification.

Gabriele Veneziano(Firenze 1942-)CERN Geneva

Edward Witten(Baltimore 1951-)IAS Princeton

The hypothesis is that the various particles (including thegraviton!) correspond to the various ways in which a single stringvibrates. A particle is no longer thought of as a point-like objectbut as a string, which may be open or closed. The various particlesare incarnations of this string. The string is like a violin string andthe patrticles are the musical notes.

String theory started,accidentally, with the workof Gabriele Veneziano onthe so called dual models.Later Green and Schwarzand especially EdwardWitten proposed stringtheory as a model forunification.

Gabriele Veneziano(Firenze 1942-)CERN Geneva

Edward Witten(Baltimore 1951-)IAS Princeton

The hypothesis is that the various particles (including thegraviton!) correspond to the various ways in which a single stringvibrates.

A particle is no longer thought of as a point-like objectbut as a string, which may be open or closed. The various particlesare incarnations of this string. The string is like a violin string andthe patrticles are the musical notes.

String theory started,accidentally, with the workof Gabriele Veneziano onthe so called dual models.Later Green and Schwarzand especially EdwardWitten proposed stringtheory as a model forunification.

Gabriele Veneziano(Firenze 1942-)CERN Geneva

Edward Witten(Baltimore 1951-)IAS Princeton

The hypothesis is that the various particles (including thegraviton!) correspond to the various ways in which a single stringvibrates. A particle is no longer thought of as a point-like objectbut as a string, which may be open or closed.

The various particlesare incarnations of this string. The string is like a violin string andthe patrticles are the musical notes.

String theory started,accidentally, with the workof Gabriele Veneziano onthe so called dual models.Later Green and Schwarzand especially EdwardWitten proposed stringtheory as a model forunification.

Gabriele Veneziano(Firenze 1942-)CERN Geneva

Edward Witten(Baltimore 1951-)IAS Princeton

The hypothesis is that the various particles (including thegraviton!) correspond to the various ways in which a single stringvibrates. A particle is no longer thought of as a point-like objectbut as a string, which may be open or closed. The various particlesare incarnations of this string. The string is like a violin string andthe patrticles are the musical notes.

40

40

40

40

40

40

Where do strings live, according to this model?

Where do strings live, according to this model?

Where do strings live, according to this model?

Where do strings live, according to this model?

Where do strings live, according to this model?

They live in a tiny6-dimensional compact varietyX .

This is a Calabi-Yauvariety.

X

In this model one sees aCalabi-Yau variety atevery point of thespace-time. Thus, inthis model, the universeis 10-dimensional.

They live in a tiny6-dimensional compact varietyX . This is a Calabi-Yauvariety.

X

In this model one sees aCalabi-Yau variety atevery point of thespace-time. Thus, inthis model, the universeis 10-dimensional.

X X X X X X

X X X X X X

X X X XX X

They live in a tiny6-dimensional compact varietyX . This is a Calabi-Yauvariety.

X

In this model one sees aCalabi-Yau variety atevery point of thespace-time. Thus, inthis model, the universeis 10-dimensional.

X X X X X X

X X X X X X

X X X XX X

They live in a tiny6-dimensional compact varietyX . This is a Calabi-Yauvariety.

X

In this model one sees aCalabi-Yau variety atevery point of thespace-time.

Thus, inthis model, the universeis 10-dimensional.

X X X X X X

X X X X X X

X X X XX X

They live in a tiny6-dimensional compact varietyX . This is a Calabi-Yauvariety.

X

In this model one sees aCalabi-Yau variety atevery point of thespace-time.

Thus, inthis model, the universeis 10-dimensional.

X X X X X X

X X X X X X

X X X XX X

They live in a tiny6-dimensional compact varietyX . This is a Calabi-Yauvariety.

X

In this model one sees aCalabi-Yau variety atevery point of thespace-time. Thus, inthis model, the universeis 10-dimensional.

X X X X X X

X X X X X X

X X X XX X

An example of a Calabi-Yau variety:

x5 + y5 + z5 + t5 = 1

Any smooth quintic in P4 is a Calabi-Yau variety.

Eugenio Calabi(Torino 1924 -)

Shing-Tung Yau(Shantou 1949 -)

An example of a Calabi-Yau variety:

x5 + y5 + z5 + t5 = 1

Any smooth quintic in P4 is a Calabi-Yau variety.

Eugenio Calabi(Torino 1924 -)

Shing-Tung Yau(Shantou 1949 -)

An example of a Calabi-Yau variety:

x5 + y5 + z5 + t5 = 1

Any smooth quintic in P4 is a Calabi-Yau variety.

Eugenio Calabi(Torino 1924 -)

Shing-Tung Yau(Shantou 1949 -)

An example of a Calabi-Yau variety:

x5 + y5 + z5 + t5 = 1

Any smooth quintic in P4 is a Calabi-Yau variety.

Eugenio Calabi(Torino 1924 -)

Shing-Tung Yau(Shantou 1949 -)

An example of a Calabi-Yau variety:

x5 + y5 + z5 + t5 = 1

Any smooth quintic in P4 is a Calabi-Yau variety.

Eugenio Calabi(Torino 1924 -)

Shing-Tung Yau(Shantou 1949 -)

Also in string theory one considers partition functions.

Thepartition function for the string theory on a Calabi-Yau variety X isdenoted with the symbol

ZX = ZX (t0, t1, t2, . . . ) =∑

i0,i1,i2,...,in

ai0i1i2...int i00 t i1

1 t i22 · · · t

inn

Calabi-Yau varieties come into the picture because of physicalconstrains. These are irrelevant from a mathematical point of view.The interesting thing is the process that leads from X to ZX .Questions:

Can one associate a ”partition function” ZX to any variety X ?

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ?

How to compute ZX ?

Also in string theory one considers partition functions. Thepartition function for the string theory on a Calabi-Yau variety X isdenoted with the symbol

ZX = ZX (t0, t1, t2, . . . ) =∑

i0,i1,i2,...,in

ai0i1i2...int i00 t i1

1 t i22 · · · t

inn

Calabi-Yau varieties come into the picture because of physicalconstrains. These are irrelevant from a mathematical point of view.The interesting thing is the process that leads from X to ZX .Questions:

Can one associate a ”partition function” ZX to any variety X ?

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ?

How to compute ZX ?

Also in string theory one considers partition functions. Thepartition function for the string theory on a Calabi-Yau variety X isdenoted with the symbol

ZX = ZX (t0, t1, t2, . . . ) =∑

i0,i1,i2,...,in

ai0i1i2...int i00 t i1

1 t i22 · · · t

inn

Calabi-Yau varieties come into the picture because of physicalconstrains.

These are irrelevant from a mathematical point of view.The interesting thing is the process that leads from X to ZX .Questions:

Can one associate a ”partition function” ZX to any variety X ?

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ?

How to compute ZX ?

Also in string theory one considers partition functions. Thepartition function for the string theory on a Calabi-Yau variety X isdenoted with the symbol

ZX = ZX (t0, t1, t2, . . . ) =∑

i0,i1,i2,...,in

ai0i1i2...int i00 t i1

1 t i22 · · · t

inn

Calabi-Yau varieties come into the picture because of physicalconstrains. These are irrelevant from a mathematical point of view.

The interesting thing is the process that leads from X to ZX .Questions:

Can one associate a ”partition function” ZX to any variety X ?

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ?

How to compute ZX ?

Also in string theory one considers partition functions. Thepartition function for the string theory on a Calabi-Yau variety X isdenoted with the symbol

ZX = ZX (t0, t1, t2, . . . ) =∑

i0,i1,i2,...,in

ai0i1i2...int i00 t i1

1 t i22 · · · t

inn

Calabi-Yau varieties come into the picture because of physicalconstrains. These are irrelevant from a mathematical point of view.The interesting thing is the process that leads from X to ZX .

Questions:

Can one associate a ”partition function” ZX to any variety X ?

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ?

How to compute ZX ?

Also in string theory one considers partition functions. Thepartition function for the string theory on a Calabi-Yau variety X isdenoted with the symbol

ZX = ZX (t0, t1, t2, . . . ) =∑

i0,i1,i2,...,in

ai0i1i2...int i00 t i1

1 t i22 · · · t

inn

Calabi-Yau varieties come into the picture because of physicalconstrains. These are irrelevant from a mathematical point of view.The interesting thing is the process that leads from X to ZX .Questions:

Can one associate a ”partition function” ZX to any variety X ?

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ?

How to compute ZX ?

Also in string theory one considers partition functions. Thepartition function for the string theory on a Calabi-Yau variety X isdenoted with the symbol

ZX = ZX (t0, t1, t2, . . . ) =∑

i0,i1,i2,...,in

ai0i1i2...int i00 t i1

1 t i22 · · · t

inn

Calabi-Yau varieties come into the picture because of physicalconstrains. These are irrelevant from a mathematical point of view.The interesting thing is the process that leads from X to ZX .Questions:

Can one associate a ”partition function” ZX to any variety X ?

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ?

How to compute ZX ?

Also in string theory one considers partition functions. Thepartition function for the string theory on a Calabi-Yau variety X isdenoted with the symbol

ZX = ZX (t0, t1, t2, . . . ) =∑

i0,i1,i2,...,in

ai0i1i2...int i00 t i1

1 t i22 · · · t

inn

Calabi-Yau varieties come into the picture because of physicalconstrains. These are irrelevant from a mathematical point of view.The interesting thing is the process that leads from X to ZX .Questions:

Can one associate a ”partition function” ZX to any variety X ?

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ?

How to compute ZX ?

Also in string theory one considers partition functions. Thepartition function for the string theory on a Calabi-Yau variety X isdenoted with the symbol

ZX = ZX (t0, t1, t2, . . . ) =∑

i0,i1,i2,...,in

ai0i1i2...int i00 t i1

1 t i22 · · · t

inn

Calabi-Yau varieties come into the picture because of physicalconstrains. These are irrelevant from a mathematical point of view.The interesting thing is the process that leads from X to ZX .Questions:

Can one associate a ”partition function” ZX to any variety X ?

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ?

How to compute ZX ?

Can one associate a ”partition function” ZX to any variety X ?

Yes.

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ? Thesenumbers are linked to the intersection theory of algebraic curves inX . In any event one knows that these are rational numbers!

How to compute ZX ? In general one does not really know.

The first case is when X = {point}. In this case ZX should tell ussomething about abstract Riemann surfaces, or, more precisely,about the moduli spaces Mg . In fact Witten found out exactlywhat these numbers tell us about Mg and has a bold conjecture onhow to compute them. Maxim Kontsevich proves this conjecture.

Theorem. the partition function Z{point}(t0, t1, t2, . . . ) satisfies theKdV equation.

52

Can one associate a ”partition function” ZX to any variety X ? Yes.

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ? Thesenumbers are linked to the intersection theory of algebraic curves inX . In any event one knows that these are rational numbers!

How to compute ZX ? In general one does not really know.

The first case is when X = {point}. In this case ZX should tell ussomething about abstract Riemann surfaces, or, more precisely,about the moduli spaces Mg . In fact Witten found out exactlywhat these numbers tell us about Mg and has a bold conjecture onhow to compute them. Maxim Kontsevich proves this conjecture.

Theorem. the partition function Z{point}(t0, t1, t2, . . . ) satisfies theKdV equation.

52

Can one associate a ”partition function” ZX to any variety X ? Yes.

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ?

Thesenumbers are linked to the intersection theory of algebraic curves inX . In any event one knows that these are rational numbers!

How to compute ZX ? In general one does not really know.

The first case is when X = {point}. In this case ZX should tell ussomething about abstract Riemann surfaces, or, more precisely,about the moduli spaces Mg . In fact Witten found out exactlywhat these numbers tell us about Mg and has a bold conjecture onhow to compute them. Maxim Kontsevich proves this conjecture.

Theorem. the partition function Z{point}(t0, t1, t2, . . . ) satisfies theKdV equation.

52

Can one associate a ”partition function” ZX to any variety X ? Yes.

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ? Thesenumbers are linked to the intersection theory of algebraic curves inX .

In any event one knows that these are rational numbers!

How to compute ZX ? In general one does not really know.

The first case is when X = {point}. In this case ZX should tell ussomething about abstract Riemann surfaces, or, more precisely,about the moduli spaces Mg . In fact Witten found out exactlywhat these numbers tell us about Mg and has a bold conjecture onhow to compute them. Maxim Kontsevich proves this conjecture.

Theorem. the partition function Z{point}(t0, t1, t2, . . . ) satisfies theKdV equation.

52

Can one associate a ”partition function” ZX to any variety X ? Yes.

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ? Thesenumbers are linked to the intersection theory of algebraic curves inX . In any event one knows that these are rational numbers!

How to compute ZX ? In general one does not really know.

The first case is when X = {point}. In this case ZX should tell ussomething about abstract Riemann surfaces, or, more precisely,about the moduli spaces Mg . In fact Witten found out exactlywhat these numbers tell us about Mg and has a bold conjecture onhow to compute them. Maxim Kontsevich proves this conjecture.

Theorem. the partition function Z{point}(t0, t1, t2, . . . ) satisfies theKdV equation.

52

Can one associate a ”partition function” ZX to any variety X ? Yes.

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ? Thesenumbers are linked to the intersection theory of algebraic curves inX . In any event one knows that these are rational numbers!

How to compute ZX ?

In general one does not really know.

The first case is when X = {point}. In this case ZX should tell ussomething about abstract Riemann surfaces, or, more precisely,about the moduli spaces Mg . In fact Witten found out exactlywhat these numbers tell us about Mg and has a bold conjecture onhow to compute them. Maxim Kontsevich proves this conjecture.

Theorem. the partition function Z{point}(t0, t1, t2, . . . ) satisfies theKdV equation.

52

Can one associate a ”partition function” ZX to any variety X ? Yes.

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ? Thesenumbers are linked to the intersection theory of algebraic curves inX . In any event one knows that these are rational numbers!

How to compute ZX ? In general one does not really know.

The first case is when X = {point}. In this case ZX should tell ussomething about abstract Riemann surfaces, or, more precisely,about the moduli spaces Mg . In fact Witten found out exactlywhat these numbers tell us about Mg and has a bold conjecture onhow to compute them. Maxim Kontsevich proves this conjecture.

Theorem. the partition function Z{point}(t0, t1, t2, . . . ) satisfies theKdV equation.

52

Can one associate a ”partition function” ZX to any variety X ? Yes.

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ? Thesenumbers are linked to the intersection theory of algebraic curves inX . In any event one knows that these are rational numbers!

How to compute ZX ? In general one does not really know.

The first case is when X = {point}. In this case ZX should tell ussomething about abstract Riemann surfaces, or, more precisely,about the moduli spaces Mg .

In fact Witten found out exactlywhat these numbers tell us about Mg and has a bold conjecture onhow to compute them. Maxim Kontsevich proves this conjecture.

Theorem. the partition function Z{point}(t0, t1, t2, . . . ) satisfies theKdV equation.

52

Can one associate a ”partition function” ZX to any variety X ? Yes.

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ? Thesenumbers are linked to the intersection theory of algebraic curves inX . In any event one knows that these are rational numbers!

How to compute ZX ? In general one does not really know.

The first case is when X = {point}. In this case ZX should tell ussomething about abstract Riemann surfaces, or, more precisely,about the moduli spaces Mg . In fact Witten found out exactlywhat these numbers tell us about Mg and has a bold conjecture onhow to compute them.

Maxim Kontsevich proves this conjecture.

Theorem. the partition function Z{point}(t0, t1, t2, . . . ) satisfies theKdV equation.

52

Can one associate a ”partition function” ZX to any variety X ? Yes.

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ? Thesenumbers are linked to the intersection theory of algebraic curves inX . In any event one knows that these are rational numbers!

How to compute ZX ? In general one does not really know.

The first case is when X = {point}. In this case ZX should tell ussomething about abstract Riemann surfaces, or, more precisely,about the moduli spaces Mg . In fact Witten found out exactlywhat these numbers tell us about Mg and has a bold conjecture onhow to compute them. Maxim Kontsevich proves this conjecture.

Theorem. the partition function Z{point}(t0, t1, t2, . . . ) satisfies theKdV equation.

52

Can one associate a ”partition function” ZX to any variety X ? Yes.

What do the coefficients ai0i1i2...in ’s of ZX tell us about X ? Thesenumbers are linked to the intersection theory of algebraic curves inX . In any event one knows that these are rational numbers!

How to compute ZX ? In general one does not really know.

The first case is when X = {point}. In this case ZX should tell ussomething about abstract Riemann surfaces, or, more precisely,about the moduli spaces Mg . In fact Witten found out exactlywhat these numbers tell us about Mg and has a bold conjecture onhow to compute them. Maxim Kontsevich proves this conjecture.

Theorem. the partition function Z{point}(t0, t1, t2, . . . ) satisfies theKdV equation.

52

Finally, consider the case in which Xis the complex projective plane.X = P2C. Kontsevich proves thatZP2C can be expressed in this way:

ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

where Nd is the number of degree dplane curves of genus 0 passingthrough 3d − 1 general points in P2 !

Maxim Kontsevich (1964- )(Paris IHES)

Kontsevich proves that the ”partition function” ZP2C satisfies theWDVV equation. This suffices to find a recursive way to computethe numbers Nd ’s.

Finally, consider the case in which Xis the complex projective plane.X = P2C.

Kontsevich proves thatZP2C can be expressed in this way:

ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

where Nd is the number of degree dplane curves of genus 0 passingthrough 3d − 1 general points in P2 !

Maxim Kontsevich (1964- )(Paris IHES)

Kontsevich proves that the ”partition function” ZP2C satisfies theWDVV equation. This suffices to find a recursive way to computethe numbers Nd ’s.

Finally, consider the case in which Xis the complex projective plane.X = P2C. Kontsevich proves thatZP2C can be expressed in this way:

ZP2C(t0, t1)

=∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

where Nd is the number of degree dplane curves of genus 0 passingthrough 3d − 1 general points in P2 !

Maxim Kontsevich (1964- )(Paris IHES)

Kontsevich proves that the ”partition function” ZP2C satisfies theWDVV equation. This suffices to find a recursive way to computethe numbers Nd ’s.

Finally, consider the case in which Xis the complex projective plane.X = P2C. Kontsevich proves thatZP2C can be expressed in this way:

ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

where Nd is the number of degree dplane curves of genus 0 passingthrough 3d − 1 general points in P2 !

Maxim Kontsevich (1964- )(Paris IHES)

Kontsevich proves that the ”partition function” ZP2C satisfies theWDVV equation. This suffices to find a recursive way to computethe numbers Nd ’s.

Finally, consider the case in which Xis the complex projective plane.X = P2C. Kontsevich proves thatZP2C can be expressed in this way:

ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

where Nd is the number of degree dplane curves of genus 0 passingthrough 3d − 1 general points in P2 !

Maxim Kontsevich (1964- )(Paris IHES)

Kontsevich proves that the ”partition function” ZP2C satisfies theWDVV equation. This suffices to find a recursive way to computethe numbers Nd ’s.

Finally, consider the case in which Xis the complex projective plane.X = P2C. Kontsevich proves thatZP2C can be expressed in this way:

ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

where Nd is the number of degree dplane curves of genus 0 passingthrough 3d − 1 general points in P2 !

Maxim Kontsevich (1964- )(Paris IHES)

Kontsevich proves that the ”partition function” ZP2C satisfies theWDVV equation. This suffices to find a recursive way to computethe numbers Nd ’s.

The partition function for P2:

Z = ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

The WDVV equation:

∂3Z

∂t13=

(∂3Z

∂t02∂t1

)2

−(

∂3Z

∂t0∂t12

)(∂3Z

∂t13

).

The recurrence formula for the numbers Nd ’s:

Nd =∑

d1+d2=d , d1,d2>0

Nd1Nd2

(d21 d2

2

(3d − 4

3d1 − 2

)− d3

1 d2

(3d − 4

3d1 − 1

)).

The partition function for P2:

Z = ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

The WDVV equation:

∂3Z

∂t13=

(∂3Z

∂t02∂t1

)2

−(

∂3Z

∂t0∂t12

)(∂3Z

∂t13

).

The recurrence formula for the numbers Nd ’s:

Nd =∑

d1+d2=d , d1,d2>0

Nd1Nd2

(d21 d2

2

(3d − 4

3d1 − 2

)− d3

1 d2

(3d − 4

3d1 − 1

)).

The partition function for P2:

Z = ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

The WDVV equation:

∂3Z

∂t13=

(∂3Z

∂t02∂t1

)2

−(

∂3Z

∂t0∂t12

)(∂3Z

∂t13

).

The recurrence formula for the numbers Nd ’s:

Nd =∑

d1+d2=d , d1,d2>0

Nd1Nd2

(d21 d2

2

(3d − 4

3d1 − 2

)− d3

1 d2

(3d − 4

3d1 − 1

)).

The partition function for P2:

Z = ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

The WDVV equation:

∂3Z

∂t13=

(∂3Z

∂t02∂t1

)2

−(

∂3Z

∂t0∂t12

)(∂3Z

∂t13

).

The recurrence formula for the numbers Nd ’s:

Nd =∑

d1+d2=d , d1,d2>0

Nd1Nd2

(d21 d2

2

(3d − 4

3d1 − 2

)− d3

1 d2

(3d − 4

3d1 − 1

)).

The partition function for P2:

Z = ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

The WDVV equation:

∂3Z

∂t13=

(∂3Z

∂t02∂t1

)2

−(

∂3Z

∂t0∂t12

)(∂3Z

∂t13

).

The recurrence formula for the numbers Nd ’s:

Nd =∑

d1+d2=d , d1,d2>0

Nd1Nd2

(d21 d2

2

(3d − 4

3d1 − 2

)− d3

1 d2

(3d − 4

3d1 − 1

)).

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

5 14 N5 = 87304

Konstevich(1993) 6 17 N6 = 2631297

7 20 N7 = 14616808192

8 23 N8 = 13525751027392

. . .

. . .

12 35 N12 =48211368061802

929292368686080

. . .

. . .

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

5 14 N5 = 87304

Konstevich(1993) 6 17 N6 = 2631297

7 20 N7 = 14616808192

8 23 N8 = 13525751027392

. . .

. . .

12 35 N12 =48211368061802

929292368686080

. . .

. . .

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

5 14 N5 = 87304

Konstevich(1993) 6 17 N6 = 2631297

7 20 N7 = 14616808192

8 23 N8 = 13525751027392

. . .

. . .

12 35 N12 =48211368061802

929292368686080

. . .

. . .

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

5 14 N5 = 87304

Konstevich(1993) 6 17 N6 = 2631297

7 20 N7 = 14616808192

8 23 N8 = 13525751027392

. . .

. . .

12 35 N12 =48211368061802

929292368686080

. . .

. . .

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

5 14 N5 = 87304

Konstevich(1993) 6 17 N6 = 2631297

7 20 N7 = 14616808192

8 23 N8 = 13525751027392

. . .

. . .

12 35 N12 =48211368061802

929292368686080

. . .

. . .

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

5 14 N5 = 87304

Konstevich(1993) 6 17 N6 = 2631297

7 20 N7 = 14616808192

8 23 N8 = 13525751027392

. . .

. . .

12 35 N12 =48211368061802

929292368686080

. . .

. . .

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

5 14 N5 = 87304

Konstevich(1993) 6 17 N6 = 2631297

7 20 N7 = 14616808192

8 23 N8 = 13525751027392

. . .

. . .

12 35 N12 =48211368061802

929292368686080

. . .

. . .

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

5 14 N5 = 87304

Konstevich(1993) 6 17 N6 = 2631297

7 20 N7 = 14616808192

8 23 N8 = 13525751027392

. . .

. . .

12 35 N12 =48211368061802

929292368686080

. . .

. . .

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

5 14 N5 = 87304

Konstevich(1993) 6 17 N6 = 2631297

7 20 N7 = 14616808192

8 23 N8 = 13525751027392

. . .

. . .

12 35 N12 =48211368061802

929292368686080

. . .

. . .

d 3d − 1 Nd

Euclid (≈300 a.C.) 1 2 N1 = 1

Apollonius (≈240 a.C.) 2 5 N2 = 1

Chasles (≈1820) 3 8 N3 = 12

Schubert (≈1870) 4 11 N4 = 620

5 14 N5 = 87304

Konstevich(1993) 6 17 N6 = 2631297

7 20 N7 = 14616808192

8 23 N8 = 13525751027392

. . .

. . .

12 35 N12 =48211368061802

929292368686080

. . .

. . .

Intersection Theory

Poincare de Rham duality: intersectionnumbers can be computed viaintegration of differential forms. Let Mbe a compact differentiable manifold. Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV ( ωV =

loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M . Let Nbe the number of these points. ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M, and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .Georges de Rham (1903-1990 )

Intersection TheoryPoincare de Rham duality:

intersectionnumbers can be computed viaintegration of differential forms. Let Mbe a compact differentiable manifold. Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV ( ωV =

loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .

Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M . Let Nbe the number of these points. ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M, and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .

Georges de Rham (1903-1990 )

Intersection TheoryPoincare de Rham duality: intersectionnumbers can be computed viaintegration of differential forms.

Let Mbe a compact differentiable manifold. Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV ( ωV =

loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .

Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M . Let Nbe the number of these points. ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M, and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .

Georges de Rham (1903-1990 )

Intersection TheoryPoincare de Rham duality: intersectionnumbers can be computed viaintegration of differential forms. Let Mbe a compact differentiable manifold.

Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV ( ωV =

loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .

Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M . Let Nbe the number of these points. ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M, and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .

Georges de Rham (1903-1990 )

Intersection TheoryPoincare de Rham duality: intersectionnumbers can be computed viaintegration of differential forms. Let Mbe a compact differentiable manifold. Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV

( ωV =loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .

Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M . Let Nbe the number of these points. ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M, and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .

Georges de Rham (1903-1990 )

Intersection TheoryPoincare de Rham duality: intersectionnumbers can be computed viaintegration of differential forms. Let Mbe a compact differentiable manifold. Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV ( ωV =

loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .

Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M . Let Nbe the number of these points. ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M, and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .

Georges de Rham (1903-1990 )

Intersection TheoryPoincare de Rham duality: intersectionnumbers can be computed viaintegration of differential forms. Let Mbe a compact differentiable manifold. Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV ( ωV =

loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M . Let Nbe the number of these points. ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M, and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .

Georges de Rham (1903-1990 )

Intersection TheoryPoincare de Rham duality: intersectionnumbers can be computed viaintegration of differential forms. Let Mbe a compact differentiable manifold. Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV ( ωV =

loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M . Let Nbe the number of these points. ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M, and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .

Georges de Rham (1903-1990 )

Intersection TheoryPoincare de Rham duality: intersectionnumbers can be computed viaintegration of differential forms. Let Mbe a compact differentiable manifold. Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV ( ωV =

loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M .

Let Nbe the number of these points. ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M, and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .

Georges de Rham (1903-1990 )

Intersection TheoryPoincare de Rham duality: intersectionnumbers can be computed viaintegration of differential forms. Let Mbe a compact differentiable manifold. Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV ( ωV =

loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M . Let Nbe the number of these points.

ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M, and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .

Georges de Rham (1903-1990 )

Intersection TheoryPoincare de Rham duality: intersectionnumbers can be computed viaintegration of differential forms. Let Mbe a compact differentiable manifold. Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV ( ωV =

loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M . Let Nbe the number of these points. ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M,

and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .

Georges de Rham (1903-1990 )

Intersection TheoryPoincare de Rham duality: intersectionnumbers can be computed viaintegration of differential forms. Let Mbe a compact differentiable manifold. Toevery codimension k subvariety V ⊂ M,one associates a degree k differentialform ωV ( ωV =

loc

∑fi1...ik dxi1 ∧ · · ·∧dxik )

with following property. Let V1, . . . ,Vs

be subvarieties of M with dim Vi = ni .Henri Poincare (1854-1912 )

Assume V1, . . . ,Vs intersect transverselyin a finite number of points. Inparticular n1 + · · ·+ ns = dim M . Let Nbe the number of these points. ThenωV1 ∧ · · · ∧ ωVs is a top-dimensionaldifferential form on M, and the numberN can be expressed as an integral:

N =

∫M

ωV1 ∧ · · · ∧ ωVs .Georges de Rham (1903-1990 )

N = [V1] · · · [Vs ]

=

∫MωV1 ∧ · · · ∧ ωVs .

Via intersection theory, the homologyvector space H∗(M) = ⊕k≥0Hk(M)becomes a ring. If [U0], . . . , [UN ] is abasis of H∗(M) then themultiplicative structure is capturedby the matrix (gij):

gij =

{[Ui ] · [Uj ] =

∫V ωUi

∧ ωUi, if i + j = dim(V ) ,

0 , otherwise.

.1V

M

.

V2

One tries to deform the intersection pairing by insisting that thedeformed multiplicative structure is still associative:

N = [V1] · · · [Vs ]

=

∫MωV1 ∧ · · · ∧ ωVs .

Via intersection theory, the homologyvector space H∗(M) = ⊕k≥0Hk(M)becomes a ring. If [U0], . . . , [UN ] is abasis of H∗(M) then themultiplicative structure is capturedby the matrix (gij):

gij =

{[Ui ] · [Uj ] =

∫V ωUi

∧ ωUi, if i + j = dim(V ) ,

0 , otherwise.

.1V

M

.

V2

One tries to deform the intersection pairing by insisting that thedeformed multiplicative structure is still associative:

N = [V1] · · · [Vs ]

=

∫MωV1 ∧ · · · ∧ ωVs .

Via intersection theory, the homologyvector space H∗(M) = ⊕k≥0Hk(M)becomes a ring.

If [U0], . . . , [UN ] is abasis of H∗(M) then themultiplicative structure is capturedby the matrix (gij):

gij =

{[Ui ] · [Uj ] =

∫V ωUi

∧ ωUi, if i + j = dim(V ) ,

0 , otherwise.

.1V

M

.

V2

One tries to deform the intersection pairing by insisting that thedeformed multiplicative structure is still associative:

N = [V1] · · · [Vs ]

=

∫MωV1 ∧ · · · ∧ ωVs .

Via intersection theory, the homologyvector space H∗(M) = ⊕k≥0Hk(M)becomes a ring. If [U0], . . . , [UN ] is abasis of H∗(M)

then themultiplicative structure is capturedby the matrix (gij):

gij =

{[Ui ] · [Uj ] =

∫V ωUi

∧ ωUi, if i + j = dim(V ) ,

0 , otherwise.

.1V

M

.

V2

One tries to deform the intersection pairing by insisting that thedeformed multiplicative structure is still associative:

N = [V1] · · · [Vs ]

=

∫MωV1 ∧ · · · ∧ ωVs .

Via intersection theory, the homologyvector space H∗(M) = ⊕k≥0Hk(M)becomes a ring. If [U0], . . . , [UN ] is abasis of H∗(M) then themultiplicative structure is capturedby the matrix (gij):

gij =

{[Ui ] · [Uj ] =

∫V ωUi

∧ ωUi, if i + j = dim(V ) ,

0 , otherwise.

.1V

M

.

V2

One tries to deform the intersection pairing by insisting that thedeformed multiplicative structure is still associative:

N = [V1] · · · [Vs ]

=

∫MωV1 ∧ · · · ∧ ωVs .

Via intersection theory, the homologyvector space H∗(M) = ⊕k≥0Hk(M)becomes a ring. If [U0], . . . , [UN ] is abasis of H∗(M) then themultiplicative structure is capturedby the matrix (gij):

gij =

{[Ui ] · [Uj ] =

∫V ωUi

∧ ωUi, if i + j = dim(V ) ,

0 , otherwise.

.1V

M

.

V2

One tries to deform the intersection pairing by insisting that thedeformed multiplicative structure is still associative:

Quantum intersection ring

- Basis [U0], . . . , [UN ] of H∗(M).- Potential:

Φ(t0, . . . , tN) =∑

n0+···+nN≥3

cn0,...,nN

tn00

n0!· · ·

tnNN

nN !

Quantum intersection product on H∗(M)⊗Q[[t0, t1, . . . , tN ]]:

[Ui ] ∗ [Uj ] =∑kl

∂3Φ

∂ti∂tj∂tkgkl [Ul ]

The associativity equation for the quantum product ∗ givesdifferential equations for the Gromov-Witten potential Φ.These are the WDVV equations !

Quantum intersection ring

- Basis [U0], . . . , [UN ] of H∗(M).

- Potential:

Φ(t0, . . . , tN) =∑

n0+···+nN≥3

cn0,...,nN

tn00

n0!· · ·

tnNN

nN !

Quantum intersection product on H∗(M)⊗Q[[t0, t1, . . . , tN ]]:

[Ui ] ∗ [Uj ] =∑kl

∂3Φ

∂ti∂tj∂tkgkl [Ul ]

The associativity equation for the quantum product ∗ givesdifferential equations for the Gromov-Witten potential Φ.These are the WDVV equations !

Quantum intersection ring

- Basis [U0], . . . , [UN ] of H∗(M).- Potential:

Φ(t0, . . . , tN) =∑

n0+···+nN≥3

cn0,...,nN

tn00

n0!· · ·

tnNN

nN !

Quantum intersection product on H∗(M)⊗Q[[t0, t1, . . . , tN ]]:

[Ui ] ∗ [Uj ] =∑kl

∂3Φ

∂ti∂tj∂tkgkl [Ul ]

The associativity equation for the quantum product ∗ givesdifferential equations for the Gromov-Witten potential Φ.These are the WDVV equations !

Quantum intersection ring

- Basis [U0], . . . , [UN ] of H∗(M).- Potential:

Φ(t0, . . . , tN) =∑

n0+···+nN≥3

cn0,...,nN

tn00

n0!· · ·

tnNN

nN !

Quantum intersection product on H∗(M)⊗Q[[t0, t1, . . . , tN ]]:

[Ui ] ∗ [Uj ] =∑kl

∂3Φ

∂ti∂tj∂tkgkl [Ul ]

The associativity equation for the quantum product ∗ givesdifferential equations for the Gromov-Witten potential Φ.These are the WDVV equations !

Quantum intersection ring

- Basis [U0], . . . , [UN ] of H∗(M).- Potential:

Φ(t0, . . . , tN) =∑

n0+···+nN≥3

cn0,...,nN

tn00

n0!· · ·

tnNN

nN !

Quantum intersection product on H∗(M)⊗Q[[t0, t1, . . . , tN ]]:

[Ui ] ∗ [Uj ] =∑kl

∂3Φ

∂ti∂tj∂tkgkl [Ul ]

The associativity equation for the quantum product ∗ givesdifferential equations for the Gromov-Witten potential Φ.

These are the WDVV equations !

Quantum intersection ring

- Basis [U0], . . . , [UN ] of H∗(M).- Potential:

Φ(t0, . . . , tN) =∑

n0+···+nN≥3

cn0,...,nN

tn00

n0!· · ·

tnNN

nN !

Quantum intersection product on H∗(M)⊗Q[[t0, t1, . . . , tN ]]:

[Ui ] ∗ [Uj ] =∑kl

∂3Φ

∂ti∂tj∂tkgkl [Ul ]

The associativity equation for the quantum product ∗ givesdifferential equations for the Gromov-Witten potential Φ.These are the WDVV equations !

In particular when M = P2, the basis of H∗(M) has two elements:U0 = 1 and U1 = [class of a line].

We take as potential thepartition function for P2:

Φ = Z = ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

The associativity equation is the WDVV equation:

∂3Z

∂t13=

(∂3Z

∂t02∂t1

)2

−(

∂3Z

∂t0∂t12

)(∂3Z

∂t13

).

In particular when M = P2, the basis of H∗(M) has two elements:U0 = 1 and U1 = [class of a line]. We take as potential thepartition function for P2:

Φ = Z = ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

The associativity equation is the WDVV equation:

∂3Z

∂t13=

(∂3Z

∂t02∂t1

)2

−(

∂3Z

∂t0∂t12

)(∂3Z

∂t13

).

In particular when M = P2, the basis of H∗(M) has two elements:U0 = 1 and U1 = [class of a line]. We take as potential thepartition function for P2:

Φ = Z = ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

The associativity equation is the WDVV equation:

∂3Z

∂t13=

(∂3Z

∂t02∂t1

)2

−(

∂3Z

∂t0∂t12

)(∂3Z

∂t13

).

In particular when M = P2, the basis of H∗(M) has two elements:U0 = 1 and U1 = [class of a line]. We take as potential thepartition function for P2:

Φ = Z = ZP2C(t0, t1) =∞∑

d=1

Ndt3d−11

(3d − 1)!edt0

The associativity equation is the WDVV equation:

∂3Z

∂t13=

(∂3Z

∂t02∂t1

)2

−(

∂3Z

∂t0∂t12

)(∂3Z

∂t13

).

top related