• 沒有找到結果。

Special quantum invariance under the normalized frame

在文檔中 1. From Picard–Fuchs to small D (頁 27-33)

4.2.1. Compatibility on quantum products via WDVV. In order to deduce con-sequences on quantum products from Proposition 4.5, the following lemma is the starting point.

Lemma 4.6. The isomorphism in (4.14) is compatible with the small quantum D-module structures. Equivalently the quantum products of divisor classes Ta := ΨTa0 on X and of classes σTa0 on X0 are compatible along the small parameter ˆs ∈H2(X0).

Proof. We first notice that (4.15) σT00 =

µ

∂σµ/∂s0Tµ0 =

µ

δµ0Tµ0 =T00.

Take two divisor classes Ta0, Tb0. Then from the WDVV equations, (4.16) hhTa∗Tb, Ti, TjiiX=

λ

hhTa, Ti, TλiiXhhTb, Tλ, TjiiX.

Along the small parametersΨˆs, by Lemma 4.4, the sum is non-zero only in the non-kernel indices (Tλ 6∈K). By (4.12), the sum then becomes

λ

hhσTa0, T0i, Tλ0iiX0hhσTb0, T0λ, Tj0iiX0(σ(ˆs)). By the WDVV equations on the X0side we then conclude

(4.17) hhTa∗Tb, Ti, TjiiX(Ψˆs) = hhσTa00σTb0, T0i, Tj0iiX0(σ(ˆs)), where the tangent map σ is performed at ˆs and the quantum product on the right-hand-side is on X0at σ(ˆs).

By induction on r ∈ N, the equation (4.17) holds for Ta1 ∗. . .∗Tar and σTa01∗. . .∗σTa0r. The proof is complete.  4.2.2. Pseudo identity and the normalized frame. Recall that T0 ≡ T0 = id mod NE(X0). The next step is to transform T0to the identity element (sec-tion) e inT and normalized Ti’s accordingly.

For Tk ∈K, by Lemma 3.7 we may represent (4.18) TkΨˆs= Pk(h∗Ψˆs, ξΨˆs) where Pk is a polynomial with coefficient in x, y.

Definition 4.7. We define theC[[x, y]]-valued R0×R0matrix(Jµk)by (4.19)

R01

µ=0

JµkTµ0 := Pk(σ(ξ0−h0)∗0, σξ00) ∗0T00,

where the quantum product∗0is taken at σ(ˆs). Note thatJµa =∂σµ/∂safor a ∈ {0, 1, 2}andJµk ∼=δkµ mod NE(X0)for all k. Hence(Jµk)is invertible.

Then by Lemma 4.6, or rather equation (4.17), we have hhTk, Ti, TjiiX(Ψˆs) = hhPk(h∗, ξ∗) ∗T0, Ti, TjiiX(Ψˆs)

= hhPk(σ(ξ0−h0)∗0, σξ00) ∗0σT00, T0i, Tj0iiX0(σ(ˆs))

=

µ

JµkhhTµ0, T0i, Tj0iiX0(σ(ˆs)). (4.20)

Lemma 4.8. There is a unique element S0T such that S0T0 is the identity element (section) e inT (and so e acts as zero on K).

Proof. By our constructions, the structure constants cikj(u, y, z)defined by TkTj =

cikjTi

are series in u, y, z. In particular, by writing S0 = iwjTj, then S0can be solved explicitly using the relation T0Tj = ici0jTi. Indeed, from (4.8), the identity e inT is given by

e= T0

d1 j

=0

ej =

i

ϕiTi

for some series ϕi(u, y, z)in u, y, z. So we need to solve the R0×R0 linear system of equations

R01 j

=0

ci0jwj = ϕi, i=0, 1, . . . , R0−1.

Notice that, by Lemma 3.7 and the property that B1 ≡Id (mod x, y), ci0j = hhT0, Ti, TjiiX = hhT0, Ti, TjiiX+

k

f0k(u, y)hhTk, Ti, TjiiX is a series in u, y with f0k(0, 0) =0. AlsohhT0, Ti, TjiiX= ((Tj, Ti)) =δij. This shows that(ci0j)is invertible and the lemma is proved.  Definition 4.9. We call S0 the pseudo-inverse of T0, which is the inverse of T0inT, and we define the normalized frame

T˘µ := TµS0 onT.

AlongΨˆs, by setting j=0 in (4.20) we find (4.21) T0∗Tk =

µ

hhT0, Tk, TµiiXTµ =

µ

JµkTµ.

Applying S0∗to (4.21), Lemma 4.8 then leads to the important Proposition 4.10(Basic transformation rule). For k∈ [0, R0−1], we have

(4.22) Tk =

R01 µ

=0

JµkT˘µ (mod K).

In particular, the normalized frame ˘Tµis defined over x, y.

4.2.3. Special quantum invariance. With (4.22), then equation (4.20) becomes (4.23) hhT˜µ, Ti, TjiiX(Ψˆs) = hhTµ0, T0i, Tj0iiX0(σ(ˆs)).

Lemma 4.11. With respect to the pairing ˘gij = (T˘i, ˘Tj), the dual frame ˘Ti :=

j ˘gijT˘j is given by ˘Ti = TiT0. Proof. Indeed,

(TjS0, TiT0) = (TjS0T0, Ti) = (Tj, Ti) =δij.

Here, the Frobenius property on the pairing is used.  Hence for any class a we have

hha, ˘Tj, ˘Tiii = (a∗T˘j, ˘Ti) = (aTjS0, TiT0)

= (a∗TjS0T0, Ti) = (a∗Tj, Ti)

= hha, Tj, Tiii. (4.24)

Together with (4.23), we arrive at a simple statement:

Theorem 4.12. Under theC[[NE(X0)]]-linear map

aiT˘i 7→

aiTi0,

the quantum product onT at Ψˆs∈ H2(X)is isomorphic to the quantum product on H(X0)at σ(ˆs) ∈H(X0) ⊗C[[NE(X0)]]. Namely

(4.25) hhT˘µ, ˘Ti, ˘TjiiX(Ψˆs) = hhTµ0, T0i, Tj0iiX0(σ(ˆs)) for all 0≤i, j, µ≤ R0−1.

The “subring”, or rather “ideal”, (T,∗)of Q0H(X)is not isomorphic to Q0H(X0)since σ(0) 6= 0 (cf. Corollary 6.9 for contributions from the ex-tremal ray). Nevertheless a standard induction on Mori cone implies that Corollary 4.13. The big quantum cohomology QH(X0) can be effectively com-puted from QH(X)through equation (4.25).

4.3. Non-linear reconstructions. In this subsection we will complete the proof of Theorem 0.1 by constructing the embedding bΨ with the imposed properties.

4.3.1. Remarks on reconstructions over the big parameter spaces. The complica-tion in dealing with the GMT ˆs 7→ σ(ˆs) lies on the fact that it is a graph over the small parameters instead of an invertible transformation. The ba-sic idea to resolve the problem is to apply suitable reconstruction theorems on X and X0 respectively and to study the compatibility between them.

When the total cohomology H is generated by H2under cup product, the reconstruction from 3-point genus zero GW invariants to all n-point genus zero invariants follows from the WDVV equations as done by Kontsevich–

Manin. Under the same condition, a version in the setup of abstract quan-tumD-modules was formulated and carried out by Iritani in [6, Theorem 4.9], which says that the “abstract big QDM” is naturally determined by the “abstract small QDM”. The abstract version is suitable in our current context since it does not require inductions on the Mori cone.

To trace the reconstruction procedure in all directions of H0consistently, we set ˆs = 0 and keep only the Novikov variables{q01, q02} = {q`0, qγ0}in equation (4.25) as the starting point. Namely we decouple the roles played by ˆs and q0a’s back to the status they are in the definition in (0.1).

Denote the resulting frames byTi(q0)and let σ0 =σ0(q0)be the general-ized mirror point at ˆs=0. Equation (4.12), via (4.24), takes the form (4.26) hTa,Tj,TiiX =

µ



δaµ+q0a∂σ0µ

∂q0a

hhTµ0, Tj0, T0iiiX0(σ0).

Here δaµis inserted since ∂σµ/∂saδµa mod NE(X0). Also (4.25) becomes (4.27) hTµ,Tj,TiiX = hhTµ0, Tj0, T0iiiX0(σ0).

We regard (4.26) as the connection matrix Aa(q0, s)at s=0 for z∇a = z∂a−Aa ≡ zq0a

∂q0a −Aa, and (4.27) as the connection matrixΩµ(q0, s)at s=0 for

z∇µ =z∂µµ ≡z

∂sµµ.

Notice that the coordinates s0, . . . , sR01are centered at σ0when viewing on the H(X0)side and centered at 0 on the H(X)side. Also while the matrices Aa andΩµare identically the same for X and X0, their meaning in quantum product are taken in completely different manners.

The flatness of∇is equivalent to the WDVV equations [Aa, Ab] = [Aa,Ωµ] = [µ,Ων] =0,

aAb =bAa, aµ =µAa, µν=νµ. (4.28)

Consider the ideal m= (s0, s1, . . . , sR01). By induction on k∈N, we may (i) solve Aa(q0, s) (mod mk)from ∂µAa =aµ (mod mk1), and then (ii) solveΩµ(q0, s) (mod mk)as a polynomial inΩj(q0, s)’s (mod mk1)

and Aa’s (mod mk).

The starting case k = 1 for (ii) is essentially Theorem 4.12. The relevant formulas are (4.19) and (4.20) used in the proof of Lemma 4.8. Indeed, let

I(q0) = (Ikµ):=J1

be the inverse matrix of(Jµk)which depends only on q0’s. Then at σ0, Tµ00 =

k

IkµPk(σ(ξ0−h0)∗0, σξ00)

=

k

IkµPk(A2−A1, A2), (4.29)

andΩµ(q0, 0)is given by (4.25) via (4.22).

Thus it remains to understand the geometric meanings on both sides under the WDVV reconstruction. On X0this is standard and it leads to

(µ)ij(q0, s) = hhTµ0, Tj0, T0iiiX0(σ0+s). In particular(µ)i0(q0, s) =δµi since T00 is the identity.

On X the reconstruction is not linear—in each step of (ii) the identity sec-tionT0(q0, s) (mod mk)receives new correction terms. With this modifi-cation been done for each k, which is hard, the resulting structure should then lead to deformations of the embeddingΨ : H(X0) ,→ H(X)to certain Ψb(q0, s)which relates quantum products of X and X0.

When the GW theory under consideration is analytic, alternatively we may view WDVV as a Frobenius integrability condition in the context of integrable distributions and to construct bΨ through certain “canonical co-ordinates”. We will take this approach in the next section, and it is best described in terms of the notion of F-manifolds.

4.3.2. Integrable distribution and the canonical coordinates. Recall that an F-manifold M is a complex F-manifold equipped with a commutative and as-sociative product structure on each tangent space TpM, such that a WDVV-type integrability condition is forced when p varies. In the context of tum cohomology, this is simply the structure which remembers the quan-tum product but forgets the metric gij, and with a coordinate-free form of the WDVV (integrability) equations.

Indeed, viewing the quantum product∗as a(2, 1)tensor, Hertling and Manin (cf. [5, Definition 2.8, Theorem 2.14, 2.15] had shown that the WDVV equations can be rewritten as

(4.30) LXY∗ =X∗LY∗ +Y∗LX

for any local vector fields X and Y, where L denotes the Lie derivatives. In explicit terms this means that for any local vector fields X, Y, Z, W we have

[X∗Y, Z∗W] − [X∗Y, Z] ∗W− [X∗Y, W] ∗Z

=X∗ [Y, Z∗W] −X∗ [Y, Z] ∗W−X∗ [Y, W] ∗Z +Y∗ [X, Z∗W] −Y∗ [X, Z] ∗W−Y∗ [X, W] ∗Z.

(4.31)

To apply it to our flip situation, we denote byKthe irregular eigenbun-dle and its orthogonal complementT = Kthe regular eigenbundle which extend the correspondingK and T from s=0 to the big parameter space.

Lemma 4.14. Both KandT and the irregular/regular decomposition of the big quantum product on THR0 are defined over the big parameter space HR0 over a punctured neighborhood of q`0 =0.

Proposition 4.15. The regular eigenbundleT is an integrable distribution of the relative tangent bundle THR0.

In particular, the image of bΨ is the integrable submanifoldM(overR0) contain-ing the slice(q`0 6= 0, t = 0)which contains the classical correspondence when moduloR0.

Proof. Let X, Z be any two local vector fields valued inT = K. Let Y=ei and W =ej be two idempotents valued inK. Since a∗b=0 for any a∈ K and b∈ K, (4.31) becomes

(4.32) 0= −X∗Z∗ [ei, ej] −δijej∗ [X, Z].

Let i= j we conclude that ej∗ [X, Z] =0 for all j. Hence[X, Z] ∈ K.  Remark 4.16. The above proof requires only thatK contains no nilpotent sections, i.e. generically semi-simple. Hence Proposition 4.15 works in the global case as well, though in the formal setting. In the local case all the local models are toric and the analyticity is known (by Iritani), thus the Frobenius theorem needed is the classical one. In the global case we need to invoke the Frobenius theorem in the formal setting.

Now we use the full strength of the local model structure. The quantum product on the Frobenius manifold H(X0) ⊗R0 is semi-simple. Deonte by the idempotent vector fields on H(X0) ⊗R0by v00, . . . , v0R01. A well-known result of Dubrovin [2, Main Lemma (3.47)] says that canonical coordinates exist. In our setting, we apply it in a family in q0 with center at σ0(q0): Lemma 4.17. We have[v0i, v0j] = 0 for all 0 ≤ i, j ≤ R0−1. Hence the corre-sponding canonical coordinates u00, . . . , u0R01satisfying

(u0i(q0, s=0)) =σ0(q0) and v0i = ∂/∂u0iexist.

Dubrovin’s result was extended to F-manifolds by Hertling [5, Theorem 2.11]. In our setting, the F-manifoldM is semi-simple (or massive) in the sense that the quantum product on TpMfor p∈ Mis semi-simple. Denote the idempotent vector field be v1. . . . , vR0.

Lemma 4.18. We have[vi, vj] =0 for all 0≤i, j≤ R0−1. Hence the canonical coordinates u0, . . . , uR01onMexist in the sense that vi =∂/∂ui.

We emphasize that we have constructed an analytic family of coordinate systems(u0(q0, p), . . . , uR01(q0, p))parametrized by q0R0. Write

(4.33) Ti(q0) =

R01

j=0

aji(q0)vj(q0, s=0)

for an invertible R0×R0 matrix(aji(q0)). From Theorem 4.12 (or (4.27)), we see easily that the same linear combination passes to the X0 side:

在文檔中 1. From Picard–Fuchs to small D (頁 27-33)

相關文件