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2. Hyperkähler mirror symmetry [030R]

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2. Hyperkähler mirror symmetry

In this section we discuss a version of mirror symmetry for hyperkähler manifolds analogous to the one used for K3 surfaces in [18].

The situation for general hyperkähler manifolds is considerably less developed, however, and we shall have to make many assumptions in this discussion. The goal is to show, modulo these assumptions, that one obtains the expected Gromov-Hausdorff collapse at a large complex structure limit of hyperkähler manifolds, and that the limit can be identified using the main results of this paper. This is completely analogous to [18], and this discussion represents a summary of known results.

First we review known facts about periods of hyperkähler manifolds. Fix MM a manifold of real dimension 4​n4n which supports a hyperkähler manifold structure with holonomy being the full group S​p​(n)Sp(n). (When a hyperkähler manifold has this full group as holonomy, it is said to be irreducible.) Set L=H2​(M,ℤ)L=H^{2}(M,\mathbb{Z}), Lℝ:=L⊗ℤℝL_{\mathbb{R}}:=L\otimes_{\mathbb{Z}}\mathbb{R}, Lℂ:=L⊗ℤℂL_{\mathbb{C}}:=L\otimes_{\mathbb{Z}}\mathbb{C}. Then there is a real-valued non-degenerate quadratic form qM:L→ℝq_{M}:L\rightarrow\mathbb{R}, called the Beauville-Bogomolov form, with the property that there is a constant cc such that

qM​(α)n=c​∫Mα2​nq_{M}(\alpha)^{n}=c\int_{M}\alpha^{2n}

for α∈L\alpha\in L, of signature (+,+,+,−,⋯,−)(+,+,+,-,\cdots,-). We write qM​(⋅,⋅)q_{M}(\cdot,\cdot) for the induced pairing, with qM​(α,α)=qM​(α)q_{M}(\alpha,\alpha)=q_{M}(\alpha).

We can define the period domain of MM to be

𝒫M:={[Ω]∈ℙ(Lℂ)|qM(Ω)=0,qM(Ω,Ω¯)>0}.\mathcal{P}_{M}:=\{[\Omega]\in\mathbb{P}(L_{\mathbb{C}})\,|\,q_{M}(\Omega)=0,\quad q_{M}(\Omega,\bar{\Omega})>0\}.

The Teichmüller space of MM, 𝐓𝐞𝐢𝐜𝐡M{\bf Teich}_{M}, is the set of hyperkähler complex structures on MM modulo elements of Diff0⁡(M)\operatorname{Diff}_{0}(M), the diffeomorphisms of MM isotopic to the identity. By the Bogomolov-Tian-Todorov theorem, this is a (non-Hausdorff) manifold. There is a period map

Per:𝐓𝐞𝐢𝐜𝐡M→𝒫M\operatorname{Per}:{\bf Teich}_{M}\rightarrow\mathcal{P}_{M}

taking a complex structure on MM to the class of the line H2,0​(M)H^{2,0}(M). Then Per\operatorname{Per} is étale, and was proved to be surjective by Huybrechts in [21]. Although we shall not make use of this here, we note that recently Verbitsky [41] proved a suitably formulated global Torelli theorem. However, one must keep in mind that Per\operatorname{Per} is not, in general, a diffeomorphism.

Next consider a complex structure on MM and Ricci–flat Kähler metric ωI\omega_{I} making MM hyperkähler. Then a choice of a holomorphic symplectic two-form ΩI\Omega_{I}, along with ωI\omega_{I}, completely determines this structure. In particular, if we write ΩI=ωJ+−1​ωK\Omega_{I}=\omega_{J}+\sqrt{-1}\omega_{K}, we can normalize ΩI\Omega_{I} so that qM​(ωI)=qM​(ωJ)=qM​(ωK)q_{M}(\omega_{I})=q_{M}(\omega_{J})=q_{M}(\omega_{K}). Furthermore, necessarily qM​(ωI,ωJ)=qM​(ωI,ωK)=qM​(ωJ,ωK)=0q_{M}(\omega_{I},\omega_{J})=q_{M}(\omega_{I},\omega_{K})=q_{M}(\omega_{J},\omega_{K})=0. The triple ωI,ωJ,ωK\omega_{I},\omega_{J},\omega_{K} is called a hyperkähler triple. It gives rise to an S2S^{2} worth of complex structures compatible with the same hyperkähler metric: in particular, one has the JJ complex structure with holomorphic symplectic form ΩJ:=ωK+−1​ωI\Omega_{J}:=\omega_{K}+\sqrt{-1}\omega_{I} and Kähler form ωJ\omega_{J}, and the KK complex structure with holomorphic symplectic form ΩK:=ωI+−1​ωJ\Omega_{K}:=\omega_{I}+\sqrt{-1}\omega_{J} and Kähler form ωK\omega_{K}.

We use these facts to speculate on mirror symmetry for hyperkähler manifolds, starting with the Strominger-Yau-Zaslow point of view. Suppose that we are given a complex structure on MM such that there is a fibration f:M→Nf:M\rightarrow N, with fibers being holomorphic Lagrangian subvarieties of MM. Suppose furthermore that NN is a Kähler manifold. Then by results of Matsushita (see [26] and [16], Proposition 24.8 for these results) the smooth fibers of ff are complex tori and NN is a Fano manifold with b2​(N)=1b_{2}(N)=1. Furthermore, if MM is projective of complex dimension 2​n2n then N=ℂ​ℙnN=\mathbb{CP}^{n} by a result of Hwang [22]. Let ωI\omega_{I} be a Ricci–flat Kähler form on MM. Write the holomorphic symplectic form ΩI\Omega_{I} on MM as ωJ+−1​ωK\omega_{J}+\sqrt{-1}\omega_{K}. Then after hyperkähler rotation, there is a a complex structure with holomorphic symplectic form ΩK=ωI+−1​ωJ\Omega_{K}=\omega_{I}+\sqrt{-1}\omega_{J} and Kähler form ωK\omega_{K}. If MyM_{y} is a fiber of ff, then ωJ|My=ωK|My=0\omega_{J}|_{M_{y}}=\omega_{K}|_{M_{y}}=0, from which it follows that Im⁡(ΩKn)|My=0\operatorname{Im}(\Omega_{K}^{n})|_{M_{y}}=0, so the fibers of ff are special Lagrangian.

The Strominger-Yau-Zaslow conjecture [36] predicts that mirror symmetry can be explained via dualizing such a special Lagrangian torus fibration. In a general situation, it can be hard to dualize torus fibrations, because of singular fibres. The case that MM is a K3 surface, treated in detail in [18], is rather special because Poincaré duality gives a canonical isomorphism between a two-torus and its dual.

With some additional assumptions, a similar situation holds in the hyperkähler case. Suppose that the Kähler form ωI\omega_{I} is integral, so that there is an ample line bundle ℒ\mathcal{L} on XX whose first Chern class is represented by ωI\omega_{I}. The restriction of this line bundle to a non-singular fiber MyM_{y} then induces a polarization of some type (d1,…,dn)(d_{1},\ldots,d_{n}). In particular there is a canonical map My→My∨M_{y}\rightarrow M_{y}^{\vee} given by

My∋x↦ℒ|My⊗tx∗​ℒ−1|My∈My∨.M_{y}\ni x\mapsto\mathcal{L}|_{M_{y}}\otimes t_{x}^{*}\mathcal{L}^{-1}|_{M_{y}}\in M_{y}^{\vee}.

Here My∨M_{y}^{\vee} is the dual abelian variety to MyM_{y}, classifying degree zero line bundles on MyM_{y}, and tx:My→Myt_{x}:M_{y}\rightarrow M_{y} is given by translation by xx, which makes sense once one chooses an origin in MyM_{y}. The kernel of this map is (ℤ/d1​ℤ⊕⋯⊕ℤ/dn​ℤ)⊕2(\mathbb{Z}/d_{1}\mathbb{Z}\oplus\cdots\oplus\mathbb{Z}/d_{n}\mathbb{Z})^{\oplus 2}. In particular, if ff possesses a section s:N→Ms:N\rightarrow M, and N0:=N∖f⁡(S)N_{0}:=N\setminus f(S) where SS is the critical locus of ff, then the dual of f−1​(N0)→N0f^{-1}(N_{0})\rightarrow N_{0} can be described as a quotient map, given by dividing out by the kernel of the polarization on each fiber. One can then hope that this dual fibration can be compactified to a hyperkähler manifold.

In general, if MyM_{y} carries a polarization of type (d1,…,dn)(d_{1},\ldots,d_{n}), it is not difficult to check that the dual abelian variety My∨M_{y}^{\vee} carries a polarization of type (dn/dn,dn/dn−1,…,dn/d1)(d_{n}/d_{n},d_{n}/d_{n-1},\ldots,d_{n}/d_{1}). Thus it is possible that the SYZ dual hyperkähler manifold need not be the same as MM. There do indeed exist examples of abelian variety fibrations on hyperkähler manifolds which are not principally polarized; these were discovered by Justin Sawon, see Example 3.8 and Remark 3.9 of [31]. It is quite possible these fibrations do not have duals which are hyperkähler manifolds, as a natural compactification might be a holomorphic symplectic variety without a holomorphic symplectic resolution of singularities.

On the other hand, if ωI\omega_{I} induces a principal polarization on each fiber MyM_{y}, i.e., the map My→My∨M_{y}\rightarrow M_{y}^{\vee} is an isomorphism, then the SYZ dual of the fibration f−1​(N0)→N0f^{-1}(N_{0})\rightarrow N_{0}, assuming again the existence of a section, can be canonically identified with f−1​(N0)→N0f^{-1}(N_{0})\rightarrow N_{0}, and thus it is natural to consider f:M→Nf:M\rightarrow N to be a self-dual fibration, at least at the purely topological level. In this case, and only in this case, SYZ mirror symmetry predicts that hyperkähler manifolds are self-mirror. The idea that hyperkähler manifolds should be self-mirror was first suggested and explored by Verbitsky in [40].

In this case only, we can be more explicit about mirror symmetry. We summarize our assumptions so far:

Assumptions 2.1.

Let MIM_{I} be a hyperkähler manifold with f:MI→Nf:M_{I}\rightarrow N a complex torus fibration, along with a section s:N→MIs:N\rightarrow M_{I} and an ample line bundle ℒ\mathcal{L} with first Chern class represented by a hyperkähler metric ωI\omega_{I}. We assume further the induced polarization on the smooth fibers of ff is principal and that NN is projective.

Thus, with these assumptions, it is natural to assume that mirror symmetry exchanges complex and Kähler moduli for the fixed underlying space MM. This can be described at the level of period domains as follows.

Let σ∈Lℝ\sigma\in L_{\mathbb{R}} be the class represented by ωI\omega_{I}. Fix an integral Kähler class ωN\omega_{N} on NN, and let E∈LE\in L be represented by f∗​ωNf^{*}\omega_{N}, so that qM​(E)=0q_{M}(E)=0.

Lemma 2.2.

In the above situation, we have qM​(E,σ)≠0q_{M}(E,\sigma)\not=0.

Proof.

By [16], Exercise 23.2, we have

qM​(E,σ)​∫Mσ2​n=2​qM​(σ)​∫Mσ2​n−1∧f∗​ωN≠0,q_{M}(E,\sigma)\int_{M}\sigma^{2n}=2q_{M}(\sigma)\int_{M}\sigma^{2n-1}\wedge f^{*}\omega_{N}\not=0,

so qM​(E,σ)≠0q_{M}(E,\sigma)\not=0. ∎

Denote by E⟂⊆LℝE^{\perp}\subseteq L_{\mathbb{R}} the orthogonal complement of EE under qMq_{M}, and denote by E⟂/EE^{\perp}/E the quotient space E⟂/ℝ​EE^{\perp}/\mathbb{R}E. Then qMq_{M} induces a quadratic form on E⟂/EE^{\perp}/E. Let

𝒞⁡(M):={x∈E⟂/E|qM​(x)>0},\mathcal{C}(M):=\{x\in E^{\perp}/E\,|\,q_{M}(x)>0\},

and define the complexified Kähler moduli space of MM to be

𝒦⁡(M):=E⟂/E⊕i​𝒞​(M)⊆(E⟂/E)⊗ℂ.\mathcal{K}(M):=E^{\perp}/E\oplus i\mathcal{C}(M)\subseteq(E^{\perp}/E)\otimes\mathbb{C}.

We then have an isomorphism

mE,σ:𝒦⁡(M)→𝒫M∖E⟂m_{E,\sigma}:\mathcal{K}(M)\rightarrow\mathcal{P}_{M}\setminus E^{\perp}

via, representing an element of (E⟂/E)⊗ℂ(E^{\perp}/E)\otimes\mathbb{C} by α∈E⟂⊗ℂ\alpha\in E^{\perp}\otimes\mathbb{C},

α↦[1qM​(E,σ)​σ+α−12​(qM​(σ)qM​(E,σ)2+qM​(α)+2​qM​(α,σ)qM​(E,σ))​E].\alpha\mapsto\left[\frac{1}{q_{M}(E,\sigma)}\sigma+\alpha-\frac{1}{2}\left(\frac{q_{M}(\sigma)}{q_{M}(E,\sigma)^{2}}+q_{M}(\alpha)+2\frac{q_{M}(\alpha,\sigma)}{q_{M}(E,\sigma)}\right)E\right].

Indeed, one first checks that this is independent of which representative α\alpha is chosen. Then one notes that the coefficient of EE is chosen so that qM​(mE,σ​(α))=0q_{M}(m_{E,\sigma}(\alpha))=0, and qM​(mE,σ​(α),mE,σ​(α¯))=2​qM​(Im⁡α)>0q_{M}(m_{E,\sigma}(\alpha),m_{E,\sigma}(\bar{\alpha}))=2q_{M}(\operatorname{Im}\alpha)>0 by assumption that α∈𝒦⁡(M)\alpha\in\mathcal{K}(M). Further, mE,σm_{E,\sigma} is clearly injective, since α=mE,σ​(α)−σ/qM​(E,σ)modE\alpha=m_{E,\sigma}(\alpha)-\sigma/q_{M}(E,\sigma)\mod E. It is surjective, since given [Ω]∈𝒫M∖E⟂[\Omega]\in\mathcal{P}_{M}\setminus E^{\perp}, we can rescale Ω\Omega so that qM​(Ω,E)=1q_{M}(\Omega,E)=1, and then [Ω]=mE,σ​(Ω−σ/qM​(E,σ)modE)[\Omega]=m_{E,\sigma}(\Omega-\sigma/q_{M}(E,\sigma)\mod E).

We can then view the mirror map mE,σm_{E,\sigma} described above as realising mirror symmetry on the level of period domains as follows, defining an exchange of data

(M,Ω,𝐁+−1​ω)↔(M,Ωˇ,𝐁ˇ+−1​ωˇ).(M,\Omega,{\bf B}+\sqrt{-1}\omega)\leftrightarrow(M,\check{\Omega},\check{\bf B}+\sqrt{-1}\check{\omega}).

Here [Ω],[Ωˇ]∈𝒫M[\Omega],[\check{\Omega}]\in\mathcal{P}_{M}, with qM​(E,Ω),qM​(E,Ωˇ)≠0q_{M}(E,\Omega),q_{M}(E,\check{\Omega})\not=0, so that we can assume Ω\Omega and Ωˇ\check{\Omega} are normalized with qM​(E,Ω)=qM​(E,Ωˇ)=1q_{M}(E,\Omega)=q_{M}(E,\check{\Omega})=1. Furthermore, 𝐁,𝐁ˇ∈E⟂/E{\bf B},\check{\bf B}\in E^{\perp}/E and ω,ωˇ∈E⟂\omega,\check{\omega}\in E^{\perp} satisfy qM​(ω,Ω)=qM​(ωˇ,Ωˇ)=0q_{M}(\omega,\Omega)=q_{M}(\check{\omega},\check{\Omega})=0 and qM​(ω),qM​(ωˇ)>0q_{M}(\omega),q_{M}(\check{\omega})>0. The relationship between the two triples is that Ωˇ=mE,σ​(𝐁+−1​ω)\check{\Omega}=m_{E,\sigma}({\bf B}+\sqrt{-1}\omega) and 𝐁ˇ,ωˇ\check{\bf B},\check{\omega} are the unique cohomology classes satisfying the above conditions and Ω=mE,σ​(𝐁ˇ+−1​ωˇ)\Omega=m_{E,\sigma}(\check{\bf B}+\sqrt{-1}\check{\omega}). Indeed, 𝐁ˇ\check{\bf B} and ωˇ\check{\omega} exist, since as qM​(E,Ω)=1q_{M}(E,\Omega)=1, we can write Ω=1qM​(E,σ)​σ+𝐁ˇ+−1​ωˇmodE\Omega=\frac{1}{q_{M}(E,\sigma)}\sigma+\check{\bf B}+\sqrt{-1}\check{\omega}\mod E, and replacing a chosen representative ωˇ\check{\omega} with ωˇ−(qM​(ωˇ,σ)/qM​(E,σ)−qM​(ωˇ,𝐁))​E\check{\omega}-(q_{M}(\check{\omega},\sigma)/q_{M}(E,\sigma)-q_{M}(\check{\omega},{\bf B}))E, one guarantees that qM​(Ωˇ,ωˇ)=0q_{M}(\check{\Omega},\check{\omega})=0.

This mirror symmetry on the level of period domains doesn’t quite give an exact mirror symmetry on the level of moduli spaces, since global Torelli does not in general hold for hyperkähler manifolds, so there might be a number of choices of complex structure on MM with period [Ω][\Omega]. In addition, ω\omega or ωˇ\check{\omega} need not represent a Kähler form except for very general choices of complex structure.

Nevertheless, this allows us to identify a large complex structure limit as being mirror to a large Kähler limit. The family

(M,Ω=1qM​(E,σ)​σ+𝐁ˇ+−1​ωˇmodE,s​ω),\left(M,\Omega=\frac{1}{q_{M}(E,\sigma)}\sigma+\check{\bf B}+\sqrt{-1}\check{\omega}\bmod E,s\omega\right),

represents a large Kähler limit, with the Kähler class moving off to infinity while the complex structure is fixed, and this is mirror to the triple

(M,Ωˇs=1qM​(E,σ)​σ+−1​s​ωmodE,𝐁ˇ+−1​ωˇ).\left(M,\check{\Omega}_{s}=\frac{1}{q_{M}(E,\sigma)}\sigma+\sqrt{-1}s\omega\bmod E,\check{\bf B}+\sqrt{-1}\check{\omega}\right).

If for each ss, we have an actual hyperkähler manifold with period Ωˇs\check{\Omega}_{s} and Kähler form ωˇ\check{\omega}, we would like to understand the limiting metric behaviour.

To do so, we use hyperkähler rotation, and to do this we need to normalize the holomorphic symplectic form, defining

Ωˇsnor=s−1​qM​(ωˇ)qM​(ω)​Ωˇs.\check{\Omega}_{s}^{{\operatorname{nor}}}=s^{-1}\sqrt{\frac{q_{M}(\check{\omega})}{q_{M}(\omega)}}\check{\Omega}_{s}.

Then we have qM​(Re⁡Ωˇsnor)=qM​(Im⁡Ωˇsnor)=qM​(ωˇ)q_{M}(\operatorname{Re}\check{\Omega}^{{\operatorname{nor}}}_{s})=q_{M}(\operatorname{Im}\check{\Omega}^{{\operatorname{nor}}}_{s})=q_{M}(\check{\omega}). So Re⁡Ωˇsnor\operatorname{Re}\check{\Omega}^{{\operatorname{nor}}}_{s}, Im⁡Ωˇsnor\operatorname{Im}\check{\Omega}^{{\operatorname{nor}}}_{s} and ωˇ\check{\omega} form a hyperkähler triple, and hence we can hyperkähler rotate to obtain a hyperkähler manifold with holomorphic two-form

Ωˇs,J:=Im⁡Ωˇsnor+−1​ωˇ=qM​(ωˇ)qM​(ω)​(ω−qM​(ω,σ)qM​(E,σ)​E)+−1​ωˇ\check{\Omega}_{s,J}:=\operatorname{Im}\check{\Omega}^{{\operatorname{nor}}}_{s}+\sqrt{-1}\check{\omega}=\sqrt{\frac{q_{M}(\check{\omega})}{q_{M}(\omega)}}\left(\omega-\frac{q_{M}(\omega,\sigma)}{q_{M}(E,\sigma)}E\right)+\sqrt{-1}\check{\omega}

and Kähler form

ωˇs,J=Re⁡Ωˇsnor=qM​(ωˇ)qM​(ω)​[1s​(1qM​(E,σ)​σ−12​qM​(σ)qM​(E,σ)2​E)+s2​qM​(ω)​E].\check{\omega}_{s,J}=\operatorname{Re}\check{\Omega}^{{\operatorname{nor}}}_{s}=\sqrt{\frac{q_{M}(\check{\omega})}{q_{M}(\omega)}}\left[\frac{1}{s}\left(\frac{1}{q_{M}(E,\sigma)}\sigma-\frac{1}{2}\frac{q_{M}(\sigma)}{q_{M}(E,\sigma)^{2}}E\right)+\frac{s}{2}q_{M}(\omega)E\right].

We note that the period Ωˇs,J\check{\Omega}_{s,J} is in fact independent of ss, so we can fix the complex structure on MM independent of ss. Assume that EE is the first Chern class of a nef line bundle on MM with respect to a complex structure with period Ωˇs,J\check{\Omega}_{s,J}, and ωˇs,J\check{\omega}_{s,J} is a Kähler class with respect to this complex structure if s⩾s0s\geqslant s_{0}, for some s0≫0s_{0}\gg 0. We now take s=s0​t+1ts=s_{0}\sqrt{\frac{t+1}{t}}, so that as tt goes to zero, ss goes to infinity and we define the rescaled metrics

ωˇt,Jnor=t⁡(t+1)​ωˇs⁡(t),J=t​ωˇs0,J+s02​qM​(ωˇ)​qM​(ω)​E.\check{\omega}_{t,J}^{\mathrm{nor}}=\sqrt{t(t+1)}\check{\omega}_{s(t),J}=t\check{\omega}_{s_{0},J}+\frac{s_{0}}{2}\sqrt{q_{M}(\check{\omega})q_{M}(\omega)}E.

So as t→0t\rightarrow 0, ωˇt,Jnor\check{\omega}_{t,J}^{\mathrm{nor}} moves on a straight line towards s02​qM​(ωˇ)​qM​(ω)​E\frac{s_{0}}{2}\sqrt{q_{M}(\check{\omega})q_{M}(\omega)}E, and ωˇs0,J\check{\omega}_{s_{0},J} is Kähler.

To relate this to the results of this paper, we have the following conjecture, stated in [19, 42]:

Conjecture 2.3.

Let MM be an irreducible hyperkähler manifold and ℒ\mathcal{L} a non-trivial nef bundle on MM, with qM​(c1​(ℒ))=0q_{M}(c_{1}(\mathcal{L}))=0. Then ℒ\mathcal{L} induces a holomorphic map f′:M→N′f^{\prime}:M\rightarrow N^{\prime} to a projective variety N′N^{\prime} with ℒm≅f′⁣∗​(𝒪⁡(1))\mathcal{L}^{m}\cong f^{\prime*}(\mathcal{O}(1)) for some m>0m>0.

If such a map exists, it is necessarily a holomorphic Lagrangian fibration. If furthermore MM is projective then N′=ℂ​ℙnN^{\prime}=\mathbb{CP}^{n} by [22]. This conjecture follows from the log abundance conjecture if some multiple of ℒ\mathcal{L} is effective, and has been studied for example in [1, 4, 19, 42].

Let us suppose this conjecture holds. By choosing s0s_{0} properly, we assume that s02​qM​(ωˇ)​qM​(ω)\frac{s_{0}}{2}\sqrt{q_{M}(\check{\omega})q_{M}(\omega)} is a integer, and thus s02​qM​(ωˇ)​qM​(ω)​E=f′⁣∗​α\frac{s_{0}}{2}\sqrt{q_{M}(\check{\omega})q_{M}(\omega)}E=f^{\prime*}\alpha for an ample class α\alpha on N′N^{\prime}, where f′f^{\prime} and N′N^{\prime} are obtained by Conjecture 2.3. Because of the hyperkähler rotation, the Riemannian metrics defined by (Ωˇsnor,ωˇ)(\check{\Omega}^{{\operatorname{nor}}}_{s},\check{\omega}) and by (Ωˇs,J,ωˇs,J)(\check{\Omega}_{s,J},\check{\omega}_{s,J}) are the same. Therefore, to understand the Gromov-Hausdorff limit of the large complex structure limit (M,Ωˇsnor,ωˇ)(M,\check{\Omega}^{{\operatorname{nor}}}_{s},\check{\omega}) (this is the same that appears in the statement of Theorem 1.3) we can instead consider (M,Ωˇs,J,ωˇs,J)(M,\check{\Omega}_{s,J},\check{\omega}_{s,J}). Now Ωˇs,J\check{\Omega}_{s,J} is independent of ss, so we are simply changing the Kähler class, and the rescaled metrics ωˇt,J=t⁡(t+1)​ωˇs⁡(t),J=t​ωˇs0,J+f′⁣∗​α\check{\omega}_{t,J}=\sqrt{t(t+1)}\check{\omega}_{s(t),J}=t\check{\omega}_{s_{0},J}+f^{\prime*}\alpha move towards f′⁣∗​αf^{\prime*}\alpha along a straight line. Therefore we are exactly in the setting of Theorem 1.1 and Theorem 1.2, which describe the Gromov-Hausdorff limit of (M,ωˇt,J)(M,\check{\omega}_{t,J}) as tt goes to zero. But as remarked in the Introduction, we also have that the diameter of ωˇt,J\check{\omega}_{t,J} is bounded uniformly away from zero and infinity, so if we further rescale the metrics ωˇt,J\check{\omega}_{t,J} to have diameter 11, then up to a subsequence the Gromov-Hausdorff limit only changes by a rescaling, and Theorem 1.3 follows.

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