ScalingStacks

Proof. [0315]

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Proof.

We pull back (1.1) via T−σ∘p∘λtT_{-\sigma}\circ p\circ\lambda_{t} and get

(λt∗​p∗​T−σ∗​ω~t)n​(y,z)=ct​tn−m​(λt∗​p∗​T−σ∗​ωM)n​(y,z)=ct​(p∗​T−σ∗​ωM)n​(y,zt),\begin{split}(\lambda_{t}^{*}p^{*}T_{-\sigma}^{*}\tilde{\omega}_{t})^{n}(y,z)&=c_{t}t^{n-m}(\lambda_{t}^{*}p^{*}T_{-\sigma}^{*}\omega_{M})^{n}(y,z)\\ &=c_{t}(p^{*}T_{-\sigma}^{*}\omega_{M})^{n}\left(y,\frac{z}{\sqrt{t}}\right),\end{split}

since the pullback under λt\lambda_{t} of any volume form f⁡(y,z)​d​y1∧⋯∧d​z¯n−mf(y,z)dy^{1}\wedge\dots\wedge d\overline{z}^{n-m} on B×ℂn−mB\times\mathbb{C}^{n-m} equals tm−n​f​(y,zt)​d​y1∧⋯∧d​z¯n−m.t^{m-n}f(y,\frac{z}{\sqrt{t}})dy^{1}\wedge\dots\wedge d\overline{z}^{n-m}. We now claim that in fact we have

(p∗​T−σ∗​ωM)n​(y,zt)=(p∗​T−σ∗​ωM)n​(y,z).(p^{*}T_{-\sigma}^{*}\omega_{M})^{n}\left(y,\frac{z}{\sqrt{t}}\right)=(p^{*}T_{-\sigma}^{*}\omega_{M})^{n}(y,z).

To see this, consider the (n,0)(n,0)-form

d​y1∧⋯∧d​ym∧d​z1∧⋯∧d​zn−mdy^{1}\wedge\dots\wedge dy^{m}\wedge dz^{1}\wedge\dots\wedge dz^{n-m}

on B×ℂn−mB\times\mathbb{C}^{n-m}. This form is invariant under the ℤ2​n−2​m\mathbb{Z}^{2n-2m}-action described above

(n1,…,n2​n−2​m)⋅(y,z)=(y,z+∑ini​vi​(y)),(n_{1},\dots,n_{2n-2m})\cdot(y,z)=(y,z+\sum_{i}n_{i}v_{i}(y)),

where (y,z)=(y1,…,ym,z1,…,zn−m)(y,z)=(y_{1},\dots,y_{m},z_{1},\dots,z_{n-m}), and so it descends to a holomorphic (n,0)(n,0)-form to the quotient (B×ℂn−m)/Λ(B\times\mathbb{C}^{n-m})/\Lambda and using the biholomorphism with UU we get a holomorphic (n,0)(n,0)-form Ω\Omega on UU. We can then consider the volume form (−1)n2​Ω∧Ω¯(\sqrt{-1})^{n^{2}}\Omega\wedge\overline{\Omega}, and we have

T−σ∗​ωMn=h⋅(−1)n2​Ω∧Ω¯,T_{-\sigma}^{*}\omega_{M}^{n}=h\cdot(\sqrt{-1})^{n^{2}}\Omega\wedge\overline{\Omega},

where hh is a smooth positive function on UU. Taking −1​∂∂¯​log\sqrt{-1}\partial\overline{\partial}\log of both sides we get

−1​∂∂¯​log⁡h=−1​∂∂¯​log⁡T−σ∗​ωMn(−1)n2​Ω∧Ω¯=0,\sqrt{-1}\partial\overline{\partial}\log h=\sqrt{-1}\partial\overline{\partial}\log\frac{T_{-\sigma}^{*}\omega_{M}^{n}}{(\sqrt{-1})^{n^{2}}\Omega\wedge\overline{\Omega}}=0,

since T−σ∗​ωMT_{-\sigma}^{*}\omega_{M} is Ricci–flat and Ω\Omega is a holomorphic (n,0)(n,0)-form. So log⁡h\log h is pluriharmonic on UU, and this implies that its restriction to any fiber MyM_{y} with y∈By\in B is constant. Pulling back via pp we get

(p∗​T−σ∗​ωMn)​(y,z)=(h∘p)​(y,z)​(−1)n2​d​y1∧⋯∧d​z¯n−m,(p^{*}T_{-\sigma}^{*}\omega_{M}^{n})(y,z)=(h\circ p)(y,z)(\sqrt{-1})^{n^{2}}dy^{1}\wedge\dots\wedge d\overline{z}^{n-m},

but since hh is constant along the fibers of ff and pp is compatible with the projection to BB we get that the function (h∘p)​(y,z)(h\circ p)(y,z) on B×ℂn−mB\times\mathbb{C}^{n-m} is independent of zz. In particular we have

(p∗​T−σ∗​ωM)n​(y,zt)=(p∗​T−σ∗​ωM)n​(y,z),(p^{*}T_{-\sigma}^{*}\omega_{M})^{n}\left(y,\frac{z}{\sqrt{t}}\right)=(p^{*}T_{-\sigma}^{*}\omega_{M})^{n}(y,z),

and so the rescaled metrics λt∗​p∗​T−σ∗​ω~t\lambda_{t}^{*}p^{*}T_{-\sigma}^{*}\tilde{\omega}_{t} satisfy the nondegenerate complex Monge-Ampère equation

(λt∗​p∗​T−σ∗​ω~t)n=(p∗​ω0+t​λt∗​p∗​T−σ∗​ωM+−1​∂∂¯​φ~t)n=ct​(p∗​T−σ∗​ωM)n(\lambda_{t}^{*}p^{*}T_{-\sigma}^{*}\tilde{\omega}_{t})^{n}=(p^{*}\omega_{0}+t\lambda_{t}^{*}p^{*}T_{-\sigma}^{*}\omega_{M}+\sqrt{-1}\partial\overline{\partial}\tilde{\varphi}_{t})^{n}=c_{t}(p^{*}T_{-\sigma}^{*}\omega_{M})^{n}

on B×ℂn−mB\times\mathbb{C}^{n-m}, where we have set

φ~t=φt∘T−σ∘p∘λt.\tilde{\varphi}_{t}=\varphi_{t}\circ T_{-\sigma}\circ p\circ\lambda_{t}.

We claim that the estimates (4.11) hold. To see this, we use (4.2) and get

(4.12) p∗​ωS​F=p∗​T−σ∗​ωM+p∗​T−σ∗​−1​∂∂¯​ξ,p^{*}\omega_{SF}=p^{*}T_{-\sigma}^{*}\omega_{M}+p^{*}T_{-\sigma}^{*}\sqrt{-1}\partial\overline{\partial}\xi,

for a function ξ\xi on UU. On B×ℂn−mB\times\mathbb{C}^{n-m} we can then use (4.10) and (4.12) and write

(4.13) λt∗​p∗​T−σ∗​ω~t=p∗​ω0+t​λt∗​p∗​T−σ∗​ωM+−1​∂∂¯​φ~t=p∗​ω0+t​λt∗​p∗​(ωS​F−T−σ∗​−1​∂∂¯​ξ)+−1​∂∂¯​φ~t=p∗​ω0+p∗​ωS​F−t​λt∗​p∗​T−σ∗​−1​∂∂¯​ξ+−1​∂∂¯​φ~t=p∗​(ω0+ωS​F)+−1​∂∂¯​ut,\begin{split}\lambda_{t}^{*}p^{*}T_{-\sigma}^{*}\tilde{\omega}_{t}&=p^{*}\omega_{0}+t\lambda_{t}^{*}p^{*}T_{-\sigma}^{*}\omega_{M}+\sqrt{-1}\partial\overline{\partial}\tilde{\varphi}_{t}\\ &=p^{*}\omega_{0}+t\lambda_{t}^{*}p^{*}(\omega_{SF}-T_{-\sigma}^{*}\sqrt{-1}\partial\overline{\partial}\xi)+\sqrt{-1}\partial\overline{\partial}\tilde{\varphi}_{t}\\ &=p^{*}\omega_{0}+p^{*}\omega_{SF}-t\lambda_{t}^{*}p^{*}T_{-\sigma}^{*}\sqrt{-1}\partial\overline{\partial}\xi+\sqrt{-1}\partial\overline{\partial}\tilde{\varphi}_{t}\\ &=p^{*}(\omega_{0}+\omega_{SF})+\sqrt{-1}\partial\overline{\partial}u_{t},\end{split}

where for simplicity we write ut=φ~t−t⁡(ξ∘T−σ∘p∘λt).u_{t}=\tilde{\varphi}_{t}-t(\xi\circ T_{-\sigma}\circ p\circ\lambda_{t}). The functions utu_{t} are uniformly bounded in C0​(B×ℂn−m)C^{0}(B\times\mathbb{C}^{n-m}) because of the L∞L^{\infty} bound for φt\varphi_{t} from [9, 10] and because ξ\xi is a fixed function on UU. The functions utu_{t} satisfy the complex Monge-Ampère equations

(4.14) (p∗​ω0+p∗​ωS​F+−1​∂∂¯​ut)n=ct​(p∗​T−σ∗​ωM)n(p^{*}\omega_{0}+p^{*}\omega_{SF}+\sqrt{-1}\partial\overline{\partial}u_{t})^{n}=c_{t}(p^{*}T_{-\sigma}^{*}\omega_{M})^{n}

on B×ℂn−mB\times\mathbb{C}^{n-m}, and on any compact subset KK of B×ℂn−mB\times\mathbb{C}^{n-m} the Kähler metric p∗​(ω0+ωS​F)p^{*}(\omega_{0}+\omega_{SF}) is C∞C^{\infty} equivalent to the Euclidean metric δ\delta (with constants that depend only on KK). The bounds (4.3) imply that

C−1​δ⩽p∗​(ω0+ωS​F)+−1​∂∂¯​ut⩽C​δ,C^{-1}\delta\leqslant p^{*}(\omega_{0}+\omega_{SF})+\sqrt{-1}\partial\overline{\partial}u_{t}\leqslant C\delta,

on KK for all small t>0t>0, where CC depends on KK. The constants ctc_{t} are bounded uniformly and away from zero. After shrinking KK slightly we can then apply the Evans-Krylov theory (as explained for example in [13, 32]) and Schauder estimates to get higher order estimates ‖ut‖Ck​(K,δ)⩽C⁡(k)\|u_{t}\|_{C^{k}(K,\delta)}\leqslant C(k) for all k⩾0k\geqslant 0, thus proving (4.11). ∎

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