Moduli Space of Curves.
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Article:
Buryak, A (2017) Double Ramification Cycles and the n-Point Function for the Moduli
Space of Curves. Moscow Mathematical Journal, 17 (1). pp. 1-13. ISSN 1609-3321
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DOUBLE RAMIFICATION CYCLES AND THE
n
-POINT FUNCTION FOR
THE MODULI SPACE OF CURVES
ALEXANDR BURYAK
Abstract. In this paper, using the formula for the integrals of theψ-classes over the double ramification cycles found by S. Shadrin, L. Spitz, D. Zvonkine and the author, we derive a new explicit formula for then-point function of the intersection numbers on the moduli space of curves.
1.
Introduction
Consider the moduli space
M
g,nof stable complex algebraic curves of genus
g
with
n
marked
points. The class
ψ
i∈
H
2(
M
g,n,
Q
) is defined as the first Chern class of the line bundle
over
M
g,nformed by the cotangent lines at the
i
-th marked point. We define the intersection
numbers by
h
τ
d1τ
d2· · ·
τ
dni
g:=
Z
Mg,n
ψ
d11
ψ
d2 2
· · ·
ψ
dn
n
.
(1.1)
In the unstable case 2
g
−
2 +
n
≤
0 we define the bracket to be equal to zero. The bracket (1.1)
vanishes unless the dimension constraint
n
X
i=1
d
i= 3
g
−
3 +
n
is satisfied. Introduce variables
t
0, t
1, t
2, . . .
. The celebrated conjecture of E. Witten [Wit91],
proved by M. Kontsevich [Kon92], says that for the following generating function
F
(
t
0, t
1, . . .
) :=
X
g≥0
n≥1
X
d1,...,dn≥0
h
τ
d1· · ·
τ
dnigt
d1· · ·
t
dnn
!
,
the exponent
e
Fis a tau-function of the KdV hierarchy in the variables
T
2i+1
=
(2i+1)!!ti.
In this paper we discuss a different generating function for the intersection numbers (1.1).
Let
n
≥
1. Introduce variables
x
1, . . . , x
n. Define
F
(
x
1, . . . , x
n) :=
X
g≥0
F
g(
x
1, . . . , x
n)
,
where
F
g(
x
1, . . . , x
n) :=
X
d1,...,dn≥0
h
τ
d1· · ·
τ
dni
gx
d11
· · ·
x
dnn.
The function
F
(
x
1, . . . , x
n) is often called the
n
-point function. There are several known
closed formulas for it [BDY15, BH07, Oko02]. In this paper we derive a simple new formula
for
F
(
x
1, . . . , x
n) using the result of [BSSZ15]. We believe that our approach can be useful for
the understanding of the structure of more general Gromov-Witten invariants.
2010Mathematics Subject Classification. Primary 14H10, Secondary 14C17.
Key words and phrases. Moduli space of curves, intersection numbers.
The author was supported by grant Russian Science Foundation N16-11-10260, project ”Geometry and mathematical physics of integrable systems”. We are grateful to R. Pandharipande and S. Shadrin for useful discussions and to an anonymous referee for a number of suggestions that helped us to improve the exposition of the paper.
Let us formulate our main result. Introduce variables
a
1, a
2, . . . , a
n. We will use the following
notations.
•
Let
ζ
(
x
) :=
e
x2−
e
− x 2.
•
For a permuation
σ
∈
S
ndenote
a
′i:=
a
σ(i)and
x
′i:=
x
σ(i).
•
Finally,
a b
c d
=
ad
−
bc.
We define the functions
P
n(
a
1, . . . , a
n;
x
1, . . . , x
n) by
P
1(
a
1;
x
1) :=
1
x
1,
P
n(
a
1, . . . , a
n;
x
1, . . . , x
n) :=
(1.2)
=
X
σ∈Sn
σ(1)=1
x
′2· · ·
x
′n−1ζ
a
′1a
′2x
′1x
′2ζ
a
′1+
a
′2a
′3x
′1+
x
′2x
′3· · ·
ζ
a
′1+
· · ·
+
a
′n−1a
′nx
′1+
· · ·
+
x
′n−1x
′na
′1a
′2x
′1x
′2a
′2a
′3x
′2x
′3· · ·
a
′n−1a
′nx
′n−1x
′n,
n
≥
2
.
At first sight it appears that for
n
≥
2 the function
P
n(
a
;
x
) has simple poles along the
hy-perplanes
{
a
ix
j−
a
jx
i= 0
}
, but in [BSSZ15, Remark 1.6] it was shown that for
n
≥
2 the
function
P
n(
a
;
x
) is a power series in
x
1, . . . , x
nwith coefficients in
C
[
a
1, . . . , a
n]. Moreover,
by [BSSZ15, Remark 1.5], the function
P
n(
a
;
x
) is symmetric with respect to simultaneous
permutations of the variables
a
1, . . . , a
nand the variables
x
1, . . . , x
n. Our main result is the
following theorem.
Theorem 1.1.
We have
(1.3)
F
(
x
1, . . . , x
n) =
=
e
(Pxi)3 24
(
P
x
i)
Q
√
2
πx
iZ
Rn
e
−P a2i 2xi
P
n
(
√
−
1
a
1, . . . ,
√
−
1
a
n;
x
1, . . . , x
n)
da
−
δ
n,1x
21
−
δ
n,2x
1+
x
2,
where
da
:=
da
1· · ·
da
n.
Let us make a few comments about the right-hand side of equation (1.3) and, in particular,
show that it is a power series in
x
1, . . . , x
n. Note that for
x >
0 and
d
≥
0 we have
1
√
2
πx
Z
R
a
de
−a 2 2xda
=
(
(
d
−
1)!!
x
d2,
if
d
is even
,
0
,
if
d
is odd
.
(1.4)
Therefore, the transformation
1
Q
√
2
πx
iZ
Rn
e
−P a2i 2xi
P
n
(
√
−
1
a
;
x
)
da
(1.5)
just means that we replace each monomial
a
d11
· · ·
a
dnnin
P
n(
a
;
x
) by
(
−
1)
12 Pdi
Y
(
d
i
−
1)!!
x
di 2
i
,
if all exponents
d
iare even and by zero otherwise. The transformation (1.5) can also be
interpreted as the Laplace transformation. For
n
≥
3, in [BSSZ15, Remark 1.6] it was shown
that the function
xPn(a;x)1+···+xn
is a power series in
x
1, . . . , x
nwith coefficients from
C
[
a
1, . . . , a
n].
Therefore, the right-hand side of (1.3) is a power series in
x
1, . . . , x
n. In the case
n
= 2, again
from [BSSZ15, Remark 1.6] we know that
P2(a1,a2;x1,x2)x1+x2
−
1x1+x2
is a power series in
x
1, x
2with
DR CYCLES AND THE n-POINT FUNCTION 3
and
x
2. For
n
= 1 we immediately see that the right-hand side of (1.3) is equal to
e x31 24−1x21
that
is of course a power series in
x
1.
Let us describe briefly the plan of the proof of Theorem 1.1. The double ramification
cy-cle DR
g(
a
1, . . . , a
n) is a cohomology class in
H
2g(
M
g,n,
Q
). It depends on a list of integers
a
1, . . . , a
nsatisfying
P
a
i= 0. In [BSSZ15] the authors derived an explicit formula for the
generating series
X
g≥0 2g−2+n>0
X
d1,...,dn≥0
Z
Mg,n
DR
g(
a
1, . . . , a
n)
ψ
1d1· · ·
ψ
ndn!
x
d11
· · ·
x
dnn.
We recall it in Section 2. Denote by
π
m:
M
g,n→ M
g,n−mthe forgetful map that forgets the
last
m
marked points. Let
a
1, . . . , a
nand
b
1, . . . , b
gbe arbitrary integers and let
A
:=
P
a
iand
B
:=
P
b
j. The push-forward
π
g∗DRg(
a
1, . . . , a
n,
−
A
−
B, b
1, . . . , b
g) is a cohomology class of
degree 0 and it is equal to
g
!
b
21
b
22· · ·
b
2gtimes the unit. This observation together with the string
equation for the intersection numbers (1.1) implies that
g
!
b
21· · ·
b
2gX
x
iF
g(
x
1, . . . , x
n) =
=
X
d1,...,dn≥0
Z
Mg,n+g+1
π
g∗DR
g(
a
1, . . . , a
n,
−
A
−
B, b
1, . . . , b
g)
ψ
d11· · ·
ψ
ndn!
x
d11
· · ·
x
dnn.
Moreover, this polynomial is the term of the lowest degree 3
g
−
2 +
n
with respect to the
x
-variables in the infinite series
X
m≥0
X
d1,...,dn≥0
Z
Mg,n+g+1
π
g∗DRm(
a
1, . . . , a
n,
−
A
−
B, b
1, . . . , b
g)
ψ
d11· · ·
ψ
ndn!
x
d1 1· · ·
x
dn
n
.
In Section 2 we derive an explicit formula for this series and then in Section 3 prove Theorem 1.1.
In Section 4 we do an explicit computation of the one-point and the two-point functions
using our general formula.
2.
Double ramification cycles
Let
n
≥
2 and let
a
1, . . . , a
nbe a list of integers satisfying
P
a
i= 0. The double ramification
cycle DR
g(
a
1, . . . , a
n) is a cohomology class in
H
2g(
M
g,n,
Q
). If not all of
a
i’s are equal to zero,
then the restriction
DR
g(
a
1, . . . , a
n)
|
Mg,nto the moduli space of smooth curves
M
g,n⊂ M
g,ncan be defined as the Poincar´e dual to
the locus of pointed smooth curves [
C, p
1, . . . , p
n] satisfying
O
C(
P
a
ip
i)
∼
=
O
C. We refer the
reader, for example, to [BSSZ15] for the general definition of the double ramification cycle on
the whole moduli space
M
g,n. We will often consider the Poincar´e dual to the double
ramifica-tion cycle DR
g(
a
1, . . . , a
n). It is an element of
H
2(2g−3+n)(
M
g,n,
Q
) and, abusing our notation
a little bit, it will also be denoted by DR
g(
a
1, . . . , a
n). An explicit formula for the double
ram-ification cycle DR
g(
a
1, . . . , a
n) in terms of tautological classes in the cohomology
H
∗(
M
g,n,
Q
)
was recently obtained in [JPPZ16]. In particular, it implies that the double ramification
cy-cle DR
g(
a
1, . . . , a
n) depends polynomially on the parameters
a
1, . . . , a
n.
Let us now formulate the main result of [BSSZ15]. Let
d
1, . . . , d
nbe non-negative integers
satisfying
P
d
i= 2
g
−
3 +
n
. Then the integral
Z
DRg(a1,...,an)
ψ
d11
· · ·
ψ
dn
n
is equal to the coefficient of
x
d11
· · ·
x
dnnin the generating function
P
n(
a
1, . . . , a
n;
x
1, . . . , x
n)
ζ
(
x
1+
· · ·
+
x
n)
−
δ
n,2x
1+
x
2.
(2.2)
As it was discussed in the introduction, this generating series is a power series in
x
1, . . . , x
nwith
coefficients from
C
[
a
1, . . . , a
n]. We see that the integral (2.1) is a polynomial in
a
1, . . . , a
n. Note
that
ζ
(
x
) =
P
i≥0 x2i+122i(2i+1)!
, then from the definition (1.2) it is easy to see that the series (2.2)
has the form
P
n(
a
1, . . . , a
n;
x
1, . . . , x
n)
ζ
(
x
1+
· · ·
+
x
n)
−
δ
n,2x
1+
x
2=
X
j≥0 2j−2+n>0
X
i
f
i,j(
a
)
g
i,j(
x
)
,
where
g
i,j(
x
)
∈
C
[
x
1, . . . , x
n] is a polynomial of degree 2
j
−
3 +
n
,
f
i,j(
a
)
∈
C
[
a
1, . . . , a
n] and
for any fixed
j
the second summation is finite. From this we conclude that all terms in the
series (2.2) have the geometrical meaning and, thus,
X
g≥0 2g−2+n>0
X
d1,...,dn≥0
Z
DRg(a1,...,an)
ψ
d11
· · ·
ψ
ndn!
x
d11
· · ·
x
dnn=
P
(
a
1, . . . , a
n;
x
1, . . . , x
n)
ζ
(
x
1+
· · ·
+
x
n)
−
δ
n,2x
1+
x
2.
(2.3)
Now we want to generalize formula (2.3) for the integrals over the double ramification cycles
with forgotten points. We begin with the following lemma.
Lemma 2.1.
For
n
≥
2
we have
P
n(
a
1, . . . , a
n;
x
1, . . . , x
n)
|
xn=0=
ζ
(
a
n(
x
1+
· · ·
+
x
n−1))
a
nP
n−1(
a
1, . . . , a
n−1;
x
1, . . . , x
n−1)
.
Proof.
For
n
= 2 we have
P
2(
a
1, a
2;
x
1, x
2) =
ζ
(
a
1x
2−
a
2x
1)
a
1x
2−
a
2x
1.
Therefore,
P
2(
a
1, a
2;
x
1, x
2)
|
x2=0=
ζ
(
a
2x
1)
a
2x
1=
ζ
(
a
2x
1)
a
2P
1(
a
1;
x
1)
.
Suppose
n
≥
3. Note that if we set
x
n= 0, then the product
x
′2· · ·
x
′n−1on the right-hand
side of (1.2) vanishes unless
σ
(
n
) =
n
. Therefore, we obtain
P
n(
a
1, . . . , a
n;
x
1, . . . , x
n)
|
xn=0=
X
σ∈Sn
σ(1)=1, σ(n)=n
x
′2· · ·
x
′n−1×
×
ζ
a
′1a
′2x
′1x
′2· · ·
ζ
a
′1+
a
′2+
· · ·
+
a
′n−2a
′n−1x
′1+
x
′2+
· · ·
+
x
′n−2x
′n−1ζ
a
′1+
· · ·
+
a
′n−1a
nx
′1+
· · ·
+
x
′n−10
a
′1
a
′2x
′1
x
′2· · ·
a
′n−2
a
′n−1x
′n−2
x
′n−1a
′n−1
a
nx
′n−1
0
=
=
ζ
(
a
n(
x
1+
· · ·
+
x
n−1))
a
nX
σ∈Sn−1
σ(1)=1
x
′2. . . x
′n−2ζ
a
′1a
′2x
′1
x
′2· · ·
ζ
a
′1+
a
′2+
· · ·
+
a
′n−2a
′n−1x
′1
+
x
′2+
· · ·
+
x
′n−2x
′n−1a
′1a
′2x
′1x
′2· · ·
a
′n−2a
′n−1x
′n−2x
′n−1=
=
ζ
(
a
n(
x
1+
· · ·
+
x
n−1))
a
nP
n−1(
a
1, . . . , a
n−1;
x
1, . . . , x
n−1)
.
The lemma is proved.
DR CYCLES AND THE n-POINT FUNCTION 5
Lemma 2.2.
Let
n
≥
3
,
m
≥
0
and
a
1, . . . , a
n, b
1, . . . , b
mbe integers satisfying
P
a
i+
P
b
j= 0
.
Then we have
X
g≥0
X
d1,...,dn≥0
Z
DRg(a1,...,an,b1,...,bm)
ψ
d11
· · ·
ψ
dn
n
!
x
d1 1· · ·
x
dn
n
=
=
Q
mi=1
S
(
b
iX
)
S
(
X
)
X
m−1
P
n
(
a
1, . . . , a
n;
x
1, . . . , x
n)
,
where
X
:=
P
x
i.
Proof.
Using equation (2.3) and Lemma 2.1, we compute
X
g≥0
X
d1,...,dn≥0
Z
DRg(a1,...,an,b1,...,bm)
ψ
d11
· · ·
ψ
ndn!
x
d11
· · ·
x
dnn=
=
P
n+m(
a
1, . . . , a
n, b
1, . . . , b
m;
x
1, . . . , x
n+m)
ζ
(
x
1+
· · ·
+
x
n+m)
xn+1=···=xn+m=0
=
=
1
ζ
(
X
)
m
Y
i=1
ζ
(
b
iX
)
b
i!
P
n(
a
1, . . . , a
n;
x
1, . . . , x
n) =
=
Q
mi=1
S
(
b
iX
)
S
(
X
)
X
m−1
P
n
(
a
1, . . . , a
n;
x
1, . . . , x
n)
.
The lemma is proved.
We keep the assumptions of the last lemma. Recall that by
π
m:
M
g,n+m→ M
g,nwe denote
the forgetful map that forgets the last
m
marked points. For a subset
I
⊂ {
1
, . . . , m
}
let
B
I:=
X
i∈I
b
i.
The following proposition generalizes formula (2.3).
Proposition 2.3.
We have
(2.4)
X
g≥0
X
d1,...,dn≥0
Z
πm∗DRg(a1,...,an,b1,...,bm)
ψ
d11
· · ·
ψ
dn
n
!
x
d1 1· · ·
x
dn
n
=
=
1
S
(
X
)
X
I0⊔I1⊔...⊔In={1,...,m}
X
|I0|−1n
Y
i=1
(
−
x
i)
|Ii|Y
i∈I0
S
(
b
iX
)
P
n(
a
1+
B
I1, . . . , a
n+
B
In;
x
)
.
Proof.
For a subset
I
=
{
i
1, i
2, . . . , i
|I|} ⊂ {
1
, . . . , m
}
, where
i
1< i
2<
· · ·
< i
|I|, we denote
by
b
Ithe string
b
i1, b
i2, . . . , b
i|I|. Clearly, formula (2.4) follows from Lemma 2.2 and the equation
Z
πm∗DRg(a1,...,an,b1,...,bm)
ψ
d11
· · ·
ψ
ndn=
X
`n
i=0Ii={1,...,m}
|Ii|≤di
(
−
1)
m−|I0|Z
DRg
(
a1+BI1,...,an+BIn,bI0)
n
Y
i=1
ψ
di−|Ii|i
.
(2.5)
Z
πm∗DRg(a1,...,an,b1,...,bm)
ψ
d11
· · ·
ψ
dn
n
=
Z
(πm−1)∗DRg(a1,...,an,bm,b1,...,bm−1)
ψ
d11
· · ·
ψ
dn
n
(2.6)
−
X
1≤i≤ndi>0
Z
(πm−1)∗DRg(a1,...,ai+bm,...,an,b1,...,bm−1)
ψ
di−1i
Y
j6=i
ψ
djj
.
For this we write
π
m=
π
1◦
π
m−1, where
π
m−1:
M
g,n+m→ M
g,n+1and
π
1:
M
g,n+1→ M
g,n.
Then we have
Z
πm∗DRg(a1,...,an,b1,...,bm)
ψ
d11
· · ·
ψ
ndn=
Z
(πm−1)∗DRg(a1,...,an,bm,b1,...,bm−1)
π
1∗ψ
d11
· · ·
ψ
ndn.
For an integer
N
≥
2 and a subset
J
∈ {
1
, . . . , N
}
,
|
J
| ≥
2, denote by
δ
J0
the cohomology class
in
H
2(
M
g,N,
Q
) that is Poincar´e dual to the divisor whose generic point is a nodal curve made
of one smooth component of genus 0 with the marked points labeled by the set
J
and of another
smooth component of genus
g
with the remaining marked points, joined at a separating node.
If 1
≤
i
≤
n
and
d
≥
1, then we have
π
1∗ψ
di
=
ψ
di−
δ
{i,n+1}
0
π
1∗ψ
id−1. Therefore,
π
∗1ψ
d11
· · ·
ψ
ndn=
ψ
d11
· · ·
ψ
dnn−
X
1≤i≤n di>0
δ
0{i,n+1}π
1∗ψ
di−1i
Y
j6=i
ψ
djj
!
.
We have (see [BSSZ15] and, in particular, Section 2.1 there for the explanation of the
nota-tion
⊠
)
δ
{0i,n+1}·
(
π
m−1)∗
DR
g(
a
1, . . . , a
n, b
m, b
1, . . . , b
m−1) =
= (
π
m−1)
∗(DR
0(
a
i, b
m,
−
a
i−
b
m)
⊠
DR
g(
a
1, . . . ,
a
b
i, . . . , a
n, b
1, . . . , b
m−1, a
i+
b
m))
.
Therefore,
Z
(πm−1)∗DRg(a1,...,an,bm,b1,...,bm−1)
δ
{0i,n+1}π
∗1ψ
di−1i
Y
j6=i
ψ
djj
!
=
=
Z
(πm−1)∗DRg(a1,...,ai+bm,...,an,b1,...,bm−1)
ψ
di−1i
Y
j6=i
ψ
djj
.
This completes the proof of equation (2.6).
It is easy to see that, applying formula (2.6)
m
times, we get equation (2.5). The proposition
is proved.
Finally, let us formulate an important geometric property of the double ramification cycle
that we will use in the next section. Let
g
≥
0,
n
≥
3 and
a
1, . . . , a
n, b
1, . . . , b
gbe integers
satisfying
P
a
i+
P
b
j= 0. Then we have (see [BSSZ15, Example 3.7])
π
g∗DR
g(
a
1, . . . , a
n, b
1, . . . , b
g) =
g
!
b
21· · ·
b
2g[
M
g,n]
,
(2.7)
π
g∗DRm(
a
1, . . . , a
n, b
1, . . . , b
g) = 0
,
m < g.
(2.8)
The last property implies that the coefficient of a monomial
x
d11
· · ·
x
dnnin the generating
se-ries (2.4) is zero, if
P
d
i<
3
m
−
3 +
n
. We will use this observation in the next section.
3.
Proof of Theorem 1.1
DR CYCLES AND THE n-POINT FUNCTION 7
3.1.
Reduction to the case
n
≥
3
.
The intersection numbers
h
τ
d1· · ·
τ
dni
gsatisfy the string
equation
h
τ
0τ
d1· · ·
τ
dni
g=
X
1≤i≤n di>0
*
τ
di−1Y
j6=i
τ
dj+
g
,
with one exceptional case
h
τ
03i0
= 1. The string equation implies that for
n
≥
2 we have
F
(
x
1, . . . , x
n)
|
xn=0= (
x
1+
· · ·
+
x
n−1)
F
(
x
1, . . . , x
n−1) +
δ
n,3.
(3.1)
Denote the right-hand side of (1.3) by
G
(
x
1, . . . , x
n). Let us show that the function
G
also
satisfies equation (3.1). We compute
1
Q
n i=1√
2
πx
iZ
Rn
e
−Pn i=1
a2i 2xi
P
n
√
−
1
a
1, . . . ,
√
−
1
a
n;
x
1, . . . , x
nda
1· · ·
da
n xn=0=
=
1
(2
π
)
n2Z
Rn
e
−Pni=1 a2i2
P
n√
−
x
1a
1, . . . ,
√
−
x
na
n;
x
1, . . . , x
nda
1· · ·
da
nxn=0
by Lemma 2.1
=
=
x
1+
· · ·
+
x
n−1(2
π
)
n2Z
Rn
e
−Pni=1 a2i2
P
n−1
√
−
x
1a
1, . . . ,
√
−
x
n−1a
n−1;
x
1, . . . , x
n−1da
1· · ·
da
n=
=
x
1Q
+
n−· · ·
1+
x
n−1i=1
√
2
πx
iZ
Rn−1
e
−Pn−1 i=1
a2i 2xi
P
n−1
√
−
1
a
1, . . . ,
√
−
1
a
n−1;
x
1, . . . , x
n−1da
1· · ·
da
n−1.
Thus, we obtain
G
(
x
1, . . . , x
n)
|
xn=0= (
x
1+
· · ·
+
x
n−1)
G
(
x
1, . . . , x
n−1) +
δ
n,3.
(3.2)
We see that if equation (1.3) holds for
n
=
n
0, then it holds for all
n
≤
n
0. Hence, it is sufficient
to prove equation (1.3) for
n
≥
3.
3.2.
Case
n
≥
3
.
We assume that
n
≥
3. Let
g
≥
0 and consider arbitrary integers
a
1, . . . , a
nand
b
1, . . . , b
g. Let
A
:=
n
X
i=1
a
i,
B
:=
gX
i=1
b
i,
X
:=
nX
i=1
x
i.
Equations (2.7) and (3.1) imply that
g
!
b
21· · ·
b
2gX
F
g(
x
1, . . . , x
n) =
g
!
b
12· · ·
b
2gF
g(
x
1, . . . , x
n, x
n+1)
|
xn+1=0=
=
X
d1,...,dn≥0
Z
πg∗DRg(a1,...,an,−A−B,b1,...,bg)
ψ
d11
· · ·
ψ
ndn!
x
d11
· · ·
x
dnn(3.3)
independently of
a
1, . . . , a
n. Moreover, by the remark at the end of Section 2, expression (3.3)
is equal to the term of the lowest degree 3
g
−
2 +
n
with respect to the
x
-variables in the series
X
m≥0
X
d1,...,dn≥0
Z
πg∗DRm(a1,...,an,−A−B,b1,...,bg)
ψ
d11
· · ·
ψ
dn
n
!
x
d1 1· · ·
x
dn
n
.
(3.4)
Proposition 2.3 and Lemma 2.1 imply that
X
m≥0
X
d1,...,dn≥0
Z
πg∗DRm(a1,...,an,−A−B,b1,...,bg)
ψ
d11
· · ·
ψ
ndn!
x
d11
· · ·
x
dnn=
(3.5)
=
S
((
−
A
−
B
)
X
)
S
(
X
)
X
`n
i=0Ii={1,...,g}
X
|I0|n
Y
i=1
(
−
x
i)
|Ii|Y
i∈I0
In the last expression the multiplication by
S((−SA(−XB))X)doesn’t change the lowest degree term
with respect to the
x
-variables. Therefore, we obtain
g
!
b
21· · ·
b
2gX
F
g(
x
1, . . . , x
n) =
=
X
`n
i=0Ii={1,...,g}
X
|I0|n
Y
i=1
(
−
x
i)
|Ii|Y
i∈I0
S
(
b
iX
)
P
n(
a
1+
B
I1, . . . , a
n+
B
In;
x
)
3g−2+n
=
=
X
`n
i=0Ii={1,...,g}
X
|I0|n
Y
i=1
(
−
x
i)
|Ii|Y
i∈I0
S
(
b
iX
)
P
n(
B
I1, . . . , B
In;
x
)
3g−2+n
,
where by [
·
]
dwe denote the degree
d
part with respect to the
x
-variables. Equivalently, we can
write
(3.6)
g
!
X
F
g(
x
1, . . . , x
n) =
=
Coef
b21···b2 gX
`n
i=0Ii={1,...,g}
X
|I0|n
Y
i=1
(
−
x
i)
|Ii|Y
i∈I0
S
(
b
iX
)
P
n(
B
I1, . . . , B
In;
x
)
3g−2+n
.
From the definition (1.2) we see that the series
P
n(
a
1, . . . , a
n;
x
1, . . . , x
n) satisfies the following
homogeneity property:
P
n(
λ
−1a
1, . . . , λ
−1a
n;
λx
1, . . . , λx
n) =
λ
n−2P
n(
a
1, . . . , a
n;
x
1, . . . , x
n)
.
Therefore, the expression in the square brackets on the right-hand side of (3.6) has automatically
degree 3
g
−
2 +
n
in the
x
-variables. Since
S
(
z
) = 1 +
z224
+
. . .
, we have
Coef
b2 1···b2gY
i∈I0
S
(
b
iX
)
P
n(
B
I1, . . . , B
In;
x
)
!
=
X
2|I0|
24
|I0|Coef
Qi /∈I0b2i
P
n(
B
I1, . . . , B
In;
x
)
.
Note that
Coef
Qi /∈I0b 2 i
n
Y
i=1
B
diIi
=
(Q
ni=1
di!
2di/2
,
if
d
i= 2
|
I
i|
,
0
,
otherwise
.
Therefore, we get
Coef
b2 1···b2gX
`n
i=0Ii={1,...,g}
X
|I0|n
Y
i=1
(
−
x
i)
|Ii|Y
i∈I0
S
(
b
iX
)
P
n(
B
I1, . . . , B
In;
x
) =
=
X
`n
i=0Ii={1,...,g}
X
3|I0|24
|I0|n
Y
i=1
(
−
x
i)
|Ii|(2
|
I
i|
)!
2
|Ii|Coef
Qn i=1a2|Ii|
i
P
n(
a
;
x
) =
=
X
m0,m1,...,mn≥0
m0+···+mn=g
g
!
m
0!
· · ·
m
n!
X
324
m0Y
ni=1
(
−
x
i)
mi(2
m
i)!
2
miCoef
Qn i=1a2mi
i
P
n(
a
;
x
) =
=
X
m0,m1,...,mn≥0
m0+···+mn=g
g
!
m
0!
X
324
m0Y
ni=1
((
−
x
i)
mi(2
m
i−
1)!!) Coef
Qn i=1a2mi
DR CYCLES AND THE n-POINT FUNCTION 9
Finally, we obtain
X
F
(
x
1, . . . , x
n) =
X
g≥0
X
F
g(
x
1, . . . , x
n) =
=
X
m0,m1,...,mn≥0
1
m
0!
X
324
m0Y
ni=1
((
−
x
i)
mi(2
m
i−
1)!!) Coef
Qn i=1a2mi i
P
n(
a
;
x
)
by (1.4)
=
=
e
X3 24Q
√
2
πx
iZ
Rn
e
−P a2i 2xi
P
n
√
−
1
a
;
x
da.
This completes the proof of the theorem.
4.
Examples
For
n
= 1 Theorem 1.1 immediately gives the well-known formula (see e.g. [FP00])
F
(
x
1) =
e
x3 1 24
−
1
x
2 1.
Suppose
n
= 2. We have
P
2(
a
1, a
2;
x
1, x
2) =
ζ
(
a
1x
2−
a
2x
1)
a
1x
2−
a
2x
1=
S
(
a
1x
2−
a
2x
1) =
X
n≥0
(
a
1x
2−
a
2x
1)
2n(2
n
+ 1)!2
2n=
=
X
n≥0
X
m1+m2=2n
(
a
1x
2)
m1(
−
a
2x
1)
m2(2
n
+ 1)2
2nm
1
!
m
2!
.
Therefore, we obtain
e
(x1+x2) 3 242
π
√
x
1x
2Z
R2
e
−a21 2x1−
a22 2x2
P
2
(
√
−
1
a
1,
√
−
1
a
2;
x
1, x
2)
da
=
=
e
(x1+x2)3 24
2
π
√
x
1x
2X
n≥0
X
m1+m2=n
Z
R2
e
−a21 2x1−
a22 2x2
(
−
1)
na
2m12
a
21m2x
21m1x
22m22
2n(2
n
+ 1)(2
m
1
)!(2
m
2)!
da
=
=
e
(x1+x2) 324
X
n≥0
X
m1+m2=n
(
−
1)
nx
m12
x
m12x
21m1x
22m22
3n(2
n
+ 1)
m
1
!
m
2!
=
=
e
x 3 1+x3224
e
x1x2(x1+x2)
8
X
n≥0
(
−
1)
n(
x
1
x
2(
x
1+
x
2))
n8
n(2
n
+ 1)
n
!
=
=
e
x 3 1+x3224
X
n≥0
x
1x
2(
x
1+
x
2)
8
nX
m1+m2=n
(
−
1)
m2m
1!
m
2!(2
m
2+ 1)
.
Let
C
n:=
P
m1+m2=n(−1)m2
m1!m2!(2m2+1)
. For
n
≥
1 we compute
C
n=
1
n
!
Z
10
(1
−
y
2)
ndy
=
2
(
n
−
1)!
Z
10
y
2(1
−
y
2)
n−1dy
=
−
2
nC
n+ 2
C
n−1.
Therefore,
C
n=
2n2+1C
n−1, and, since
C
0= 1, we get
C
n=
2n
(2n+1)!!
. Hence, we obtain
e
(x1+x2) 3 242
π
√
x
1x
2Z
R2
e
−a21 2x1−
a22
2x2
P
2(
√
−
1
a
1,
√
−
1
a
2;
x
1, x
2)
da
=
e
x31+x3224
X
n≥0
n
!
(2
n
+ 1)!
x
1
x
2(
x
1+
x
2)
2
nAs a result, we get the following formula for the two-point function:
F
(
x
1, x
2) =
e
x31+x32 24
(
x
1+
x
2)
X
n≥0
n
!
(2
n
+ 1)!
x
1
x
2(
x
1+
x
2)
2
n−
x
1
1+
x
2.
This formula was found by R. Dijkgraaf (see e.g. [FP00]).
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Department of Mathematics, ETH Z¨urich, Switzerland, and
Faculty of Mechanics and Mathematics, Lomonosov Moscow State University, Russian Fed-eration