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7.1. Algebro-geometric aspect [055J]

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7.1. Algebro-geometric aspect

7.1.1. Poincaré residue

We first recall some general facts about Poincaré residues. Given a smooth divisor ZZ in a complex manifold MM of dimension mm, the Poincaré residue map

(7.1) Res:H0​(M,KM⊗[Z])→H0​(Z,KZ)\Res:H^{0}(M,K_{M}\otimes[Z])\rightarrow H^{0}(Z,K_{Z})

can be defined as follows. Given a holomorphic mm form Ω\Omega on MM with a simple pole along ZZ, locally if we choose a defining function hh of ZZ, then h​Ωh\Omega is a holomorphic mm form, and we can write

(7.2) h​Ω=d​h∧Ω~h\Omega=dh\wedge\tilde{\Omega}

for some locally defined holomorphic m−1m-1 form Ω~\tilde{\Omega}. The Poincaré residue of Ω\Omega along ZZ is given by

(7.3) Res⁡(Ω)≡Ω~|Z\Res(\Omega)\equiv\tilde{\Omega}|_{Z}

It is straightforward to check that this does not depend on the choice of hh and Ω~\tilde{\Omega}, and gives rise to a well-defined holomorphic volume form ΩZ\Omega_{Z} globally on ZZ.

If we choose local holomorphic coordinates z1,⋯,zmz_{1},\cdots,z_{m} on MM, then we may write

(7.4) Ω=ghdz1∧⋯dzm.\Omega=\frac{g}{h}dz_{1}\wedge\cdots dz_{m}.

At a point on ZZ where ∂h∂z1≠0\frac{\partial h}{\partial z_{1}}\neq 0, we have then by definition

(7.5) Res⁡(Ω)=g∂h∂z1​d​z2∧⋯∧d​zm.\Res(\Omega)=\frac{g}{\frac{\partial h}{\partial z_{1}}}dz_{2}\wedge\cdots\wedge dz_{m}.

From the local expression one can see that if ZZ is an anti-canonical divisor in MM, and we pick a holomorphic volume form ΩM\Omega_{M} on M∖ZM\setminus Z with a simple pole along ZZ, and then Res⁡(ΩM)\Res(\Omega_{M}) gives a holomorphic volume form ΩZ\Omega_{Z} on ZZ.

A special case is when we have a globally defined holomorphic function h:M→ℂh:M\rightarrow\mathbb{C}, and we are given a holomorphic volume form Ω\Omega on MM, then for each w∈ℂw\in\mathbb{C}, we can apply the above construction to the meromorphic form (h−w)−1​Ω(h-w)^{-1}\Omega. In this way we obtain a nowhere vanishing section Ω′\Omega^{\prime} of the relative canonical bundle KM⊗(h∗​Kℂ)−1K_{M}\otimes(h^{*}K_{\mathbb{C}})^{-1}, on the set where hh is a submersion, and it satisfies the equation

(7.6) d​h∧Ω′=Ω.dh\wedge\Omega^{\prime}=\Omega.

We may also view Ω′\Omega^{\prime} as a holomorphic varying family of holomorphic volume forms on the fibers of hh.

7.1.2. A model partial resolution of singularities

Let 𝒮\mathcal{S} be a two dimensional Ak−1​(k≥2)A_{k-1}(k\geq 2) singularity, which is a hypersurface in ℂ3\mathbb{C}^{3} with defining equation

(7.7) z1​z2+z3k=0.z_{1}z_{2}+z_{3}^{k}=0.

Given two positive integers a1≥a2a_{1}\geq a_{2} with a1+a2=ka_{1}+a_{2}=k, we can define a partial resolution of 𝒮\mathcal{S} as follows. Let 𝒮¯\overline{\mathcal{S}} be the subvariety in the product space ℂ3×ℂ​ℙ2\mathbb{C}^{3}\times\mathbb{C}\mathbb{P}^{2} cut out by the following system of equations

(7.8) {z3a1​u1=z1​u3;z3a2​u2=z2​u3;u1​u2+u32=0;z3a1−a2​u1​z2=u2​z1;z3a2​u3+u1​z2=0.\begin{cases}z_{3}^{a_{1}}u_{1}=z_{1}u_{3};\\ z_{3}^{a_{2}}u_{2}=z_{2}u_{3};\\ u_{1}u_{2}+u_{3}^{2}=0;\\ z_{3}^{a_{1}-a_{2}}u_{1}z_{2}=u_{2}z_{1};\\ z_{3}^{a_{2}}u_{3}+u_{1}z_{2}=0.\end{cases}

where [u1:u2:u3][u_{1}:u_{2}:u_{3}] denotes homogeneous coordinates on ℂ​ℙ2\mathbb{C}\mathbb{P}^{2}. Alternatively, 𝒮¯\overline{\mathcal{S}} can also be described as the closure in ℂ3×ℂ​ℙ2\mathbb{C}^{3}\times\mathbb{C}\mathbb{P}^{2} of the graph of the rational map 𝒮→ℂℙ2;(z1,z2,z3)↦[z1z3a1:z2z3a2:1]\mathcal{S}\rightarrow\mathbb{C}\mathbb{P}^{2};(z_{1},z_{2},z_{3})\mapsto[\frac{z_{1}}{z_{3}^{a_{1}}}:\frac{z_{2}}{z_{3}^{a_{2}}}:1]. On the affine chart {ui≠0}\{u_{i}\neq 0\} we shall denote by vj=uj/ui​(j≠i)v_{j}=u_{j}/u_{i}(j\neq i) the affine coordinates.

Lemma 7.1.

𝒮¯\overline{\mathcal{S}} has at most two possible singularities, which are of type Aa1−1A_{a_{1}-1} and Aa2−1A_{a_{2}-1} respectively, and the projection map 𝒮¯→𝒮\overline{\mathcal{S}}\rightarrow\mathcal{S} is a partial resolution, with exceptional divisor isomorphic to ℂ​ℙ1\mathbb{C}\mathbb{P}^{1}.

Proof.

We first show that the system of equations implies z1​z2+z3k=0z_{1}z_{2}+z_{3}^{k}=0, so that 𝒮¯\overline{\mathcal{S}} does project to 𝒮\mathcal{S}. To see this, we notice the first three equations imply

(7.9) u32​(z1​z2+z3k)=0.u_{3}^{2}(z_{1}z_{2}+z_{3}^{k})=0.

If u3≠0u_{3}\neq 0, then we get z1​z2+z3k=0z_{1}z_{2}+z_{3}^{k}=0. If u3=0u_{3}=0, then by the third equation we get that either u1≠0,u2=0u_{1}\neq 0,u_{2}=0 or u1=0,u2≠0u_{1}=0,u_{2}\neq 0. In the first case using the remaining equations we get z3=z2=0z_{3}=z_{2}=0. In the second case we get z3=z1=0z_{3}=z_{1}=0. In both cases the equation z1​z2+z3k=0z_{1}z_{2}+z_{3}^{k}=0 is indeed satisfied.

Now we study singularities of 𝒮¯\overline{\mathcal{S}}. In the affine chart {u1≠0}\{u_{1}\neq 0\}, we get

(7.10) {v2+v32=0;z2+z3a2​v3=0,\begin{cases}v_{2}+v_{3}^{2}=0;\\ z_{2}+z_{3}^{a_{2}}v_{3}=0,\end{cases}

so we reduce the defining equations to a single equation in the z1,z3,v3z_{1},z_{3},v_{3} variable given by

(7.11) z3a1=z1​v3.z_{3}^{a_{1}}=z_{1}v_{3}.

This has exactly one Aa1−1A_{a_{1}-1} singularity at {z1=z3=v3=0}\{z_{1}=z_{3}=v_{3}=0\}. Similarly, on the affine chart {u2≠0}\{u_{2}\neq 0\} we reduce the equations to

(7.12) z3a2=z2​v3.z_{3}^{a_{2}}=z_{2}v_{3}.

This has exactly one Aa2−1A_{a_{2}-1} singularity at {z2=z3=v3=0}\{z_{2}=z_{3}=v_{3}=0\}. On the affine chart {u3≠0}\{u_{3}\neq 0\}, we reduce the equations to

(7.13) v1​v2+1=0.v_{1}v_{2}+1=0.

which is smooth.

It is then easy to verify that the projection map 𝒮¯→𝒮\overline{\mathcal{S}}\rightarrow\mathcal{S} is an isomorphism outside the point {z1=z2=z3=0}\{z_{1}=z_{2}=z_{3}=0\}, and if z1=z2=z3=0z_{1}=z_{2}=z_{3}=0, we get the equation

(7.14) u1​u2+u32=0,u_{1}u_{2}+u_{3}^{2}=0,

which gives a conic in ℂ​ℙ2\mathbb{C}\mathbb{P}^{2}. ∎

From another point of view, we can view 𝒮\mathcal{S} and 𝒮¯\overline{\mathcal{S}} as families of algebraic curves by projecting to the z3z_{3} variable. For 𝒮\mathcal{S} this is simply the standard nodal degeneration of conics in ℂ2\mathbb{C}^{2}, modified by a base change. The family corresponding to 𝒮¯\overline{\mathcal{S}} is isomorphic to 𝒮\mathcal{S} over any general fiber {z3≠0}\{z_{3}\neq 0\}, and the special fiber of 𝒮¯\overline{\mathcal{S}} is now given by a chain consisting of three components, two of which are given by the proper transforms of the two lines {z1=0}\{z_{1}=0\} and {z2=0}\{z_{2}=0\} in ℂ2\mathbb{C}^{2}, and the middle component is the conic {u1u2+u32=0}\{u_{1}u_{2}+u_{3}^{2}=0\} in ℂ​ℙ2\mathbb{C}\mathbb{P}^{2}. In the special case when a1=a2=1a_{1}=a_{2}=1, 𝒮¯\overline{\mathcal{S}} is smooth and the projection map is precisely the minimal resolution of singularity.

It is well-known that 𝒮\mathcal{S} has a canonical singularity, meaning that the canonical line bundle K𝒮K_{\mathcal{S}} is trivial. An explicit holomorphic volume form Ω𝒮\Omega_{\mathcal{S}} can be written by applying the Poincaré residue to the standard meromorphic 1z1​z2+z3k​d​z1∧d​z2∧d​z3\frac{1}{z_{1}z_{2}+z_{3}^{k}}dz_{1}\wedge dz_{2}\wedge dz_{3} on ℂ3\mathbb{C}^{3}. In the chart {z1≠0}\{z_{1}\neq 0\}, it is given by

(7.15) Ω𝒮=d​z2∧d​z3z2.\Omega_{\mathcal{S}}=\frac{dz_{2}\wedge dz_{3}}{z_{2}}.

Notice 𝒮\mathcal{S} is isomorphic to the quotient ℂ2/ℤk\mathbb{C}^{2}/\mathbb{Z}_{k}, and Ω𝒮\Omega_{\mathcal{S}} pulls-back to a multiple of the standard holomorphic volume form on ℂ2\mathbb{C}^{2}.

Viewing 𝒮\mathcal{S} as fibered over z3∈ℂz_{3}\in\mathbb{C}, we further get a relative holomorphic volume form

(7.16) Ω′=−d​z2z2=d​z1z1.\Omega^{\prime}=-\frac{dz_{2}}{z_{2}}=\frac{dz_{1}}{z_{1}}.

One can see Ω′\Omega^{\prime} is smooth away from the singularity {z1=z2=z3=0}\{z_{1}=z_{2}=z_{3}=0\}, and on each component of the singular fiber it is a meromorphic 1-form with a simple pole along the singularity.

The partial resolution 𝒮¯\overline{\mathcal{S}} is a crepant resolution, i.e. the canonical line bundle K𝒮¯K_{\overline{\mathcal{S}}} is also trivial. Indeed the pull-back Ω𝒮¯\Omega_{\overline{\mathcal{S}}} of Ω𝒮\Omega_{\mathcal{S}} is nowhere vanishing on 𝒮¯\overline{\mathcal{S}}, and by applying the Poincaré residue to the function z3z_{3}, we then get a meromorphic 1-form on each component of the special fiber. On the conic {u1u2+u32=0}\{u_{1}u_{2}+u_{3}^{2}=0\} the meromorphic 1-form is given by v1−1​d​v1=−v2−1​d​v2v_{1}^{-1}dv_{1}=-v_{2}^{-1}dv_{2}. The upshot is that we still get a meromorphic section of the relative canonical bundle, which is smooth away from the two singularities {u1=u3=z1=z2=z3=0}\{u_{1}=u_{3}=z_{1}=z_{2}=z_{3}=0\} and {u2=u3=z1=z2=z3=0}\{u_{2}=u_{3}=z_{1}=z_{2}=z_{3}=0\} of S¯\overline{S}.

7.1.3. A modification of the degenerating family

We now recall the set-up in the introduction. Let n≥2n\geq 2 be an integer. Let f1,f2,ff_{1},f_{2},f be homogeneous polynomials of degree d1≥d2,d1+d2=n+2d_{1}\geq d_{2},d_{1}+d_{2}=n+2 respectively, and let 𝒳⊂ℂ​ℙn+1×Δ\mathcal{X}\subset\mathbb{C}\mathbb{P}^{n+1}\times\Delta be a family of Calabi-Yau hypersurfaces in ℂ​ℙn+1\mathbb{C}\mathbb{P}^{n+1} defined by the equation Ft​(x)=0F_{t}(x)=0, where

(7.17) Ft​(x)≡f1​(x)​f2​(x)+t​f​(x)F_{t}(x)\equiv f_{1}(x)f_{2}(x)+tf(x)

and tt is the complex parameter on the unit disc Δ⊂ℂ\Delta\subset\mathbb{C}. Let p:𝒳→Δp:\mathcal{X}\rightarrow\Delta be the projection map and we denote X^t=p−1​(t)\widehat{X}_{t}=p^{-1}(t).

We further assume f1,f2,ff_{1},f_{2},f are sufficiently general so that the following hold:

  1. (i)

    X0=Y1∪Y2X_{0}=Y_{1}\cup Y_{2}, where Y1={f1=0}Y_{1}=\{f_{1}=0\} and Y2={f2=0}Y_{2}=\{f_{2}=0\} are smooth;

  2. (ii)

    X^t\widehat{X}_{t} is smooth for t≠0t\neq 0.;

  3. (iii)

    D={f1=f2=0}D=\{f_{1}=f_{2}=0\} is a smooth complete intersection;

  4. (iv)

    H={f1=f2=f=0}H=\{f_{1}=f_{2}=f=0\} is a smooth complete intersection in ℂ​ℙn+1\mathbb{C}\mathbb{P}^{n+1}.

The total space 𝒳\mathcal{X} is singular along HH and transverse to H×{0}H\times\{0\} the singularities are locally modeled on a two dimensional ordinary double point. For our purpose we need to perform certain birational transformations to 𝒳\mathcal{X} keeping the general fibers unchanged.

We first do a base change t↦tn+2t\mapsto t^{n+2}, and work on the new family, which we still denote by 𝒳\mathcal{X}. Then 𝒳\mathcal{X} now has singularities along D×{0}D\times\{0\}, transversal to which generically it is a two dimensional Ad−1A_{d-1} singularity, which becomes worse along H×{0}H\times\{0\}. This is usually referred to as a compounded Du Val (cDV) singularity .

Now we apply the family version of the above model partial resolution to 𝒳\mathcal{X}. Let 𝒳^\widehat{\mathcal{X}} be the subvariety in the projective bundle ℙ⁡(𝒪⁡(d2)⊕𝒪⁡(d1)⊕ℂ)\mathbb{P}(\mathcal{O}(d_{2})\oplus\mathcal{O}(d_{1})\oplus\mathbb{C}) over ℂ​ℙn+1×Δ\mathbb{C}\mathbb{P}^{n+1}\times\Delta cut out by the equations

(7.18) {td1​s1=s3​f2​(x);td2​s2=s3​f1​(x);s1⊗s2+s32​f​(x)=0;td1−d2​s1⊗f1​(x)=f2​(x)⊗s2;td2​s3​f​(x)+s1⊗f1​(x)=0.\begin{cases}t^{d_{1}}s_{1}=s_{3}f_{2}(x);\\ t^{d_{2}}s_{2}=s_{3}f_{1}(x);\\ s_{1}\otimes s_{2}+s_{3}^{2}f(x)=0;\\ t^{d_{1}-d_{2}}s_{1}\otimes f_{1}(x)=f_{2}(x)\otimes s_{2};\\ t^{d_{2}}s_{3}f(x)+s_{1}\otimes f_{1}(x)=0.\end{cases}

where naturally we view fi∈H0​(ℂ​ℙn+1,𝒪⁡(di))f_{i}\in H^{0}(\mathbb{C}\mathbb{P}^{n+1},\mathcal{O}(d_{i})), f∈H0​(ℂ​ℙn+1,𝒪⁡(n+2))f\in H^{0}(\mathbb{C}\mathbb{P}^{n+1},\mathcal{O}(n+2)), and [s1:s2:s3][s_{1}:s_{2}:s_{3}] denotes a point in the fiber of the projective bundle over the point (x,t)∈ℂ​ℙn+1×Δ(x,t)\in\mathbb{C}\mathbb{P}^{n+1}\times\Delta.

For our discussion in the rest of this section we shall always take [x0:x1:⋯:xn+1][x_{0}:x_{1}:\cdots:x_{n+1}] to be the homogeneous coordinates of a point xx on ℂ​ℙn+1\mathbb{C}\mathbb{P}^{n+1}. On the affine chart {xi≠0}\{x_{i}\neq 0\} of ℂ​ℙn+1\mathbb{C}\mathbb{P}^{n+1} we denote by u={uj=xj/xi,j≠i}u=\{u_{j}=x_{j}/x_{i},j\neq i\} the affine coordinates, and we view xix_{i} as a local trivialization of 𝒪⁡(1)\mathcal{O}(1). Then on this chart we can view any holomorphic sections of powers of 𝒪⁡(1)\mathcal{O}(1) as local holomorphic functions. In particular, for a homogeneous function R⁡(x)R(x), we denote by R⁡(u)R(u) the corresponding inhomogeneous function. On the affine trivialization of the projective bundle {si≠0}\{s_{i}\neq 0\}, we denote by {ζj=sj/si,j≠i}\{\zeta_{j}=s_{j}/s_{i},j\neq i\} the affine coordinates on the fibers.

We define

(7.19) D1\displaystyle D_{1} ≡{f1(x)=f2(x)=t=0,s2=s3=0},\displaystyle\equiv\{f_{1}(x)=f_{2}(x)=t=0,s_{2}=s_{3}=0\},
(7.20) D2\displaystyle D_{2} ≡{f1(x)=f2(x)=t=0,s1=s3=0}.\displaystyle\equiv\{f_{1}(x)=f_{2}(x)=t=0,s_{1}=s_{3}=0\}.
Lemma 7.2.

𝒳^\widehat{\mathcal{X}} is smooth away from the union D1∪D2D_{1}\cup D_{2}, and transverse to each DiD_{i} the singularity is a two dimensional Adi−1A_{d_{i}-1} singularity.

Proof.

We know 𝒳^\widehat{\mathcal{X}} is isomorphic to 𝒳\mathcal{X} away from D×{0}D\times\{0\}, so it suffices to consider around a point (x,0)(x,0) where f1​(x)=f2​(x)=0f_{1}(x)=f_{2}(x)=0. Locally in an affine chart {s1≠0}\{s_{1}\neq 0\}, 𝒳^\widehat{\mathcal{X}} is then cut out by the equations

(7.21) {f2​(u)​ζ3=td1;f1​(u)​ζ3=td2​ζ2;ζ2+ζ32​f​(u)=0;f2​(u)​ζ2=td1−d2​f1​(u);td2​ζ3​f​(u)+f1​(u)=0.\begin{cases}f_{2}(u)\zeta_{3}=t^{d_{1}};\\ f_{1}(u)\zeta_{3}=t^{d_{2}}\zeta_{2};\\ \zeta_{2}+\zeta_{3}^{2}f(u)=0;\\ f_{2}(u)\zeta_{2}=t^{d_{1}-d_{2}}f_{1}(u);\\ t^{d_{2}}\zeta_{3}f(u)+f_{1}(u)=0.\end{cases}

These can be reduced to two equations on the coordinates uu, tt and ζ3\zeta_{3}, given by

(7.22) {f2​(u)​ζ3−td1=0td2​ζ3​f​(u)+f1​(u)=0.\begin{cases}f_{2}(u)\zeta_{3}-t^{d_{1}}=0\\ t^{d_{2}}\zeta_{3}f(u)+f_{1}(u)=0.\end{cases}

By our assumption (iii) locally we may use v1=f1​(u)v_{1}=f_{1}(u) and v2=f2​(u)v_{2}=f_{2}(u) to replace u1,u2u_{1},u_{2} (say) as local holomorphic coordinates on a neighborhood of xx in ℂ​ℙn+1\mathbb{C}\mathbb{P}^{n+1}. Then it is easy to see the corresponding subvariety is smooth if ζ3≠0\zeta_{3}\neq 0, and has transversal Ad1−1A_{d_{1}-1} singularities along D1D_{1}. So this gives the local description of 𝒳^\widehat{\mathcal{X}} in a neighborhood of D1D_{1}. Similarly on {s2≠0}\{s_{2}\neq 0\} we also know the space is smooth except with transversal Ad2−1A_{d_{2}-1} singularities along D2D_{2}.

On {s3≠0}\{s_{3}\neq 0\}, we use u,t,ζ1,ζ2u,t,\zeta_{1},\zeta_{2} as coordinates, and we get the constraint equations

(7.23) {ζ1​ζ2+f⁡(u)=0,f2​(u)−td1​ζ1=0,f1​(u)−td2​ζ2=0.\begin{cases}\zeta_{1}\zeta_{2}+f(u)=0,\\ f_{2}(u)-t^{d_{1}}\zeta_{1}=0,\\ f_{1}(u)-t^{d_{2}}\zeta_{2}=0.\end{cases}

We only need to consider the points where ζ1=ζ2=t=0\zeta_{1}=\zeta_{2}=t=0, so in particular we also have f⁡(u)=0f(u)=0. At such a point, the differentials of these three equations are (∇f​(u),∇f2​(u),∇f1​(u))(\nabla f(u),\nabla f_{2}(u),\nabla f_{1}(u)). This is non-zero by our assumption (iv). ∎

One can see that the new central fiber X^0\hat{X}_{0} consists of a chain of three smooth components intersecting transversally, given by the proper transforms Y^1,Y^2\hat{Y}_{1},\hat{Y}_{2} of Y1,Y2Y_{1},Y_{2} respectively and the submanifold 𝒩\mathcal{N} in the projective bundle ℙ⁡(L1⊕L2⊕ℂ)\mathbb{P}(L_{1}\oplus L_{2}\oplus\mathbb{C}) over DD cut out by the equation s1​s2=s32​f​(x)s_{1}s_{2}=s_{3}^{2}f(x) (so that 𝒩\mathcal{N} is a quadric bundle over DD, and singular fibers are over HH). Notice 𝒩\mathcal{N} itself is a smooth manifold.

∙\bullet∙\bullet∙\bullet∙\bullet∙\bulletX^t\widehat{X}_{t}Y^1\hat{Y}_{1}Y^2\hat{Y}_{2}D1D_{1}D2D_{2}𝒩\mathcal{N}H×{t}H\times\{t\}X^0=Y^1∪D1𝒩∪D2Y^2\widehat{X}_{0}=\hat{Y}_{1}\cup_{D_{1}}\mathcal{N}\cup_{D_{2}}\hat{Y}_{2}
Figure 7.1. The modified family 𝒳^\widehat{\mathcal{X}}

We then have

(7.24) D1=Y^1∩𝒩,D2=Y^2∩𝒩.D_{1}=\hat{Y}_{1}\cap\mathcal{N},\ \ D_{2}=\hat{Y}_{2}\cap\mathcal{N}.

It is straightforward to see that the normal bundle of DiD_{i} in 𝒩\mathcal{N} is Li−1L_{i}^{-1}.

Next we consider holomorphic volume forms. Viewing 𝒳\mathcal{X} as an anti-canonical divisor in ℂ​ℙn+1×Δ\mathbb{C}\mathbb{P}^{n+1}\times\Delta, then away from D×{0}D\times\{0\}, 𝒳\mathcal{X} is smooth and we then obtain a holomorphic volume form Γ\Gamma. In the affine chart {x0≠0}×Δ⊂ℂℙn+1×Δ\{x_{0}\neq 0\}\times\Delta\subset\mathbb{C}\mathbb{P}^{n+1}\times\Delta, the meromorphic volume form is given by

(7.25) 1Ft​(u)​d​t∧d​u1∧⋯∧d​un+1.\frac{1}{F_{t}(u)}dt\wedge du_{1}\wedge\cdots\wedge du_{n+1}.

So the Poincaré residue on 𝒳\mathcal{X} is

(7.26) Γ=−1(n+2)​tn+1​f​(u)du1∧⋯dun+1.\Gamma=-\frac{1}{(n+2)t^{n+1}f(u)}du_{1}\wedge\cdots du_{n+1}.

It is easy to check using the equation and the genericity assumptions that Γ\Gamma is indeed holomorphic on 𝒳∖D×{0}\mathcal{X}\setminus D\times\{0\}.

Now applying the above discussion to the global function tt on 𝒳\mathcal{X}, then we get a holomorphic family of holomorphic volume forms Γt\Gamma_{t} on each X^t\widehat{X}_{t}. Differentiating the equation Ft​(u)=f1​(u)​f2​(u)+tn+2​f​(u)=0F_{t}(u)=f_{1}(u)f_{2}(u)+t^{n+2}f(u)=0, we get

(7.27) (n+2)​tn+1​f​(u)​d​t+du​Ft=0.(n+2)t^{n+1}f(u)dt+d_{u}F_{t}=0.

In the above affine chart, on the set where ∂Ft∂u1≠0\frac{\partial F_{t}}{\partial u_{1}}\neq 0, we have

(7.28) Γt=1∂Ft​(u)∂u1du2∧⋯dun+1.\Gamma_{t}=\frac{1}{\frac{\partial F_{t}(u)}{\partial u_{1}}}du_{2}\wedge\cdots du_{n+1}.

This is indeed well-defined on X^t\widehat{X}_{t} for t≠0t\neq 0 and also on X0∖DX_{0}\setminus D. On each component YiY_{i} of X0X_{0}, it has a simple pole along DD. Notice Γt\Gamma_{t} is also the natural holomorphic volume form on X^t\widehat{X}_{t} when we apply the Poincaré residue to the divisor X^t\widehat{X}_{t} in ℂ​ℙn+1\mathbb{C}\mathbb{P}^{n+1}.

Now we pass to the resolution 𝒳^\widehat{\mathcal{X}}. Abusing notation we still denote by Γ\Gamma its pull-back.

Lemma 7.3.

Γ\Gamma extends to a global holomorphic volume form on 𝒳^∖(D1∪D2)\widehat{\mathcal{X}}\setminus(D_{1}\cup D_{2}).

Proof.

We only need to consider around a point (x,t,s)(x,t,s) on the exceptional set 𝒩\mathcal{N}, so (x,t)∈D×{0}(x,t)\in D\times\{0\}. Without loss of generality may assume x0≠0x_{0}\neq 0. Since DD is a complete intersection by assumption (iii), we may use v1=f1​(u)v_{1}=f_{1}(u) and v2=f2​(u)v_{2}=f_{2}(u) to replace u1,u2u_{1},u_{2} (say) as local holomorphic coordinates on a neighborhood of xx in ℂ​ℙn+1\mathbb{C}\mathbb{P}^{n+1}. So we can write

(7.29) Γ=−J−1(n+2)​tn+1​f​(u)​d​v1∧d​v2∧d​u3∧⋯∧d​un+1,\Gamma=-\frac{J^{-1}}{(n+2)t^{n+1}f(u)}dv_{1}\wedge dv_{2}\wedge du_{3}\cdots\wedge du_{n+1},

where JJ is the Jacobian given by

(7.30) J=∂f1∂u1​∂f2∂u2−∂f1∂u2​∂f2∂u1.J=\frac{\partial f_{1}}{\partial u_{1}}\frac{\partial f_{2}}{\partial u_{2}}-\frac{\partial f_{1}}{\partial u_{2}}\frac{\partial f_{2}}{\partial u_{1}}.

Suppose first we work on the affine chart {s1≠0}\{s_{1}\neq 0\}. Then we get the local equations for 𝒳^\widehat{\mathcal{X}} given by (7.22). Since we are away from D1D_{1}, we must have ζ3≠0\zeta_{3}\neq 0. Then we can use ζ3,t,u3,⋯,un+1\zeta_{3},t,u_{3},\cdots,u_{n+1} as local holomorphic coordinates on 𝒳^\widehat{\mathcal{X}}. We have

(7.31) d​v1=−td2​f​d​ζ3−d2​td2−1​ζ3​f​d​t−tn+2​ζ3​d​f,dv_{1}=-t^{d_{2}}fd\zeta_{3}-d_{2}t^{d_{2}-1}\zeta_{3}fdt-t^{n+2}\zeta_{3}df,
(7.32) d​v2=d1​td1−1​ζ3−1​d​t−ζ3−2​td1​d​ζ3dv_{2}=d_{1}t^{d_{1}-1}\zeta_{3}^{-1}dt-\zeta_{3}^{-2}t^{d_{1}}d\zeta_{3}

and

(7.33) d​f=∂f∂v1​d​v1+∂f∂v2​d​v2+∑j≥3∂f∂uj​d​uj.df=\frac{\partial f}{\partial v_{1}}dv_{1}+\frac{\partial f}{\partial v_{2}}dv_{2}+\sum_{j\geq 3}\frac{\partial f}{\partial u_{j}}du_{j}.

So we get

(1+td2​ζ3​∂f∂v1)​d​v1\displaystyle(1+t^{d_{2}}\zeta_{3}\frac{\partial f}{\partial v_{1}})dv_{1}
(7.34) =\displaystyle= (−td2​f+tn+2​ζ3−1​∂f∂v2)​d​ζ3−(d2​td2−1​ζ3​f+d1​tn+1​∂f∂v2)​d​t\displaystyle(-t^{d_{2}}f+t^{n+2}\zeta_{3}^{-1}\frac{\partial f}{\partial v_{2}})d\zeta_{3}-(d_{2}t^{d_{2}-1}\zeta_{3}f+d_{1}t^{n+1}\frac{\partial f}{\partial v_{2}})dt mod(d​u3,⋯,d​un+1).\displaystyle\mod(du_{3},\cdots,du_{n+1}).

Hence we get

(7.35) Γ=ζ3−1(1+td2​ζ3​∂f∂v1)​J−1​d​ζ3∧d​t∧d​u3∧⋯∧d​un+1.\Gamma=\frac{\zeta_{3}^{-1}}{(1+t^{d_{2}}\zeta_{3}\frac{\partial f}{\partial v_{1}})}J^{-1}d\zeta_{3}\wedge dt\wedge du_{3}\wedge\cdots\wedge du_{n+1}.

Near t=0t=0 we see Γ\Gamma is smooth around such a point. Similarly we can deal with the chart {s2≠0}\{s_{2}\neq 0\}.

Now on {s3≠0}\{s_{3}\neq 0\}, we only need to consider a point on DD where f=0f=0, then by our assumption (iv) we may use v3=fv_{3}=f as a local holomorphic coordinate to replace u3u_{3} for instance. Then we can write

(7.36) Γ=−1(n+2)​tn+1​f​K−1​d​v1∧d​v2∧d​v3∧d​u4∧⋯∧d​un+1,\Gamma=-\frac{1}{(n+2)t^{n+1}f}K^{-1}dv_{1}\wedge dv_{2}\wedge dv_{3}\wedge du_{4}\cdots\wedge du_{n+1},

where KK is the Jacobian for the change of coordinates. We have

(7.37) d​v3=−(ζ1​d​ζ2+ζ2​d​ζ1),dv_{3}=-(\zeta_{1}d\zeta_{2}+\zeta_{2}d\zeta_{1}),
(7.38) d​v1=td2​d​ζ2+d2​ζ2​td2−1​d​t,dv_{1}=t^{d_{2}}d\zeta_{2}+d_{2}\zeta_{2}t^{d_{2}-1}dt,
(7.39) d​v2=td1​d​ζ1+d1​ζ1​td1−1​d​t.dv_{2}=t^{d_{1}}d\zeta_{1}+d_{1}\zeta_{1}t^{d_{1}-1}dt.

Then we get

(7.40) Γ=K−1​d​t∧d​ζ1∧d​ζ2∧d​u4∧⋯∧d​un+1,\Gamma=K^{-1}dt\wedge d\zeta_{1}\wedge d\zeta_{2}\wedge du_{4}\cdots\wedge du_{n+1},

which is smooth. ∎

Now we can apply the previous Poincaré residue to the function tt on 𝒳^\widehat{\mathcal{X}}. Since the exceptional set of the resolution lies over D×{0}D\times\{0\}, we still get Γt\Gamma_{t} for t≠0t\neq 0. On the central fiber X^0\hat{X}_{0}, we still get Γ0\Gamma_{0} on Y^1∖D1\hat{Y}_{1}\setminus D_{1} and Y^2∖D2\hat{Y}_{2}\setminus D_{2}. Over 𝒩∖(D1∪D2)\mathcal{N}\setminus(D_{1}\cup D_{2}), using (7.35) and (7.40) we get the corresponding Poincaré residue

(7.41) Γ𝒩=J−1​d​ζ1ζ1∧d​u3∧⋯∧d​un+1=−J−1​d​ζ2ζ2∧d​u3∧⋯∧d​un+1.\Gamma_{\mathcal{N}}=J^{-1}\frac{d\zeta_{1}}{\zeta_{1}}\wedge du_{3}\wedge\cdots\wedge du_{n+1}=-J^{-1}\frac{d\zeta_{2}}{\zeta_{2}}\wedge du_{3}\wedge\cdots\wedge du_{n+1}.

Notice by applying Poincaré residue twice to the complete intersection D={f1=f2=0}D=\{f_{1}=f_{2}=0\}, we obtain a holomorphic volume form ΩD\Omega_{D} on DD, which in the above local coordinates can be written as

(7.42) ΩD=J−1​d​u3∧⋯∧d​un+1.\Omega_{D}=J^{-1}du_{3}\wedge\cdots\wedge du_{n+1}.

So we get

(7.43) Γ𝒩=d​ζ1ζ1∧ΩD.\Gamma_{\mathcal{N}}=\frac{d\zeta_{1}}{\zeta_{1}}\wedge\Omega_{D}.

This means that up to multiplying by −−1-\sqrt{-1}, Γ𝒩\Gamma_{\mathcal{N}} agrees with the natural holomorphic volume form Ω0\Omega_{0} on 𝒩0\mathcal{N}_{0} defined in Section 4.2, under the identification k−=d2,k+=−d1k_{-}=d_{2},k_{+}=-d_{1}.

Original mathematics by the credited authors. Source-backed reader collection; mathematical self-containment is not assessed.