ScalingStacks

Proof. [04ZI]

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Proof.

The above expansions can be proved using the Jacobi fields. Fix a point q=(0k0,x1,…,xm−k0)∈U⊂Pq=(0^{k_{0}},x_{1},\ldots,x_{m-k_{0}})\in U\subset P, we we choose a unit vector v=∑α=1m−k0vα∂yα∈N(q)≅ℝk0v=\sum\limits_{\alpha=1}^{m-k_{0}}v_{\alpha}\partial_{y_{\alpha}}\in N(q)\cong\mathbb{R}^{k_{0}} with |v|=1|v|=1. Let ϑ\vartheta be the following radial geodesic in 𝒰\mathcal{U},

(3.21) ϑ⁡(t)=ExpP⁡(q,t​v)≡Expq⁡(t​v)\vartheta(t)=\Exp_{P}(q,tv)\equiv\Exp_{q}(tv)

such that ϑ′​(0)=v\vartheta^{\prime}(0)=v. In the normal coordinates, the geodesic ϑ\vartheta can represented as ϑ⁡(t)=(t​v1,…,t​vk0,x1,…,xm−k0)\vartheta(t)=(tv_{1},\ldots,tv_{k_{0}},x_{1},\ldots,x_{m-k_{0}}).

For each 1≤α≤k01\leq\alpha\leq k_{0} and 1≤i≤m−k01\leq i\leq m-k_{0}, we define the geodesic variations

(3.22) σα​(t,s)\displaystyle\sigma_{\alpha}(t,s) ≡((t​v1,…,t⁡(vα+s),…,t​vk0,x1,…,xm−k0)CLOSE,\displaystyle\equiv((tv_{1},\ldots,t(v_{\alpha}+s),\ldots,tv_{k_{0}},x_{1},\ldots,x_{m-k_{0}}),
(3.23) σi​(t,s)\displaystyle\sigma_{i}(t,s) ≡(t​v1,…,t​vk0,x1,…,xi+s,…​xm−k0).\displaystyle\equiv(tv_{1},\ldots,tv_{k_{0}},x_{1},\ldots,x_{i}+s,\ldots x_{m-k_{0}}).

Then variation fields of σα​(t,s)\sigma_{\alpha}(t,s) and σi​(t,s)\sigma_{i}(t,s) give the following Jacobi fields along the radial geodesic ϑ⁡(t)\vartheta(t) respectively:

(3.24) {Jα(t)=t⋅∂yα,1≤α≤k0Ji(t)=∂xi,1≤i≤m−k0.\displaystyle\begin{cases}J_{\alpha}(t)=t\cdot\partial_{y_{\alpha}},&1\leq\alpha\leq k_{0}\\ J_{i}(t)=\partial_{x_{i}},&1\leq i\leq m-k_{0}.\end{cases}

By definition,

(3.25) Jα(0)=0,Ji(0)=∂xi.J_{\alpha}(0)=0,\ J_{i}(0)=\partial_{x_{i}}.

Taking first derivatives at t=0t=0,

(3.26) Jα′(0)=∂yα,Ji′(0)=vα∇∂xi∂yα.J_{\alpha}^{\prime}(0)=\partial_{y_{\alpha}},\ J_{i}^{\prime}(0)=v_{\alpha}\nabla_{\partial_{x_{i}}}\partial_{y_{\alpha}}.

Then applying the Jacobi equation along the geodesic ϑ\vartheta,

(3.27) {Jα′′+Rm⁡(Jα,ϑ′)​ϑ′=0,Ji′′+Rm⁡(Ji,ϑ′)​ϑ′=0,\displaystyle\begin{cases}J_{\alpha}^{\prime\prime}+\Rm(J_{\alpha},\vartheta^{\prime})\vartheta^{\prime}=0,\\ J_{i}^{\prime\prime}+\Rm(J_{i},\vartheta^{\prime})\vartheta^{\prime}=0,\\ \end{cases}

where Rm⁡(X,Y)​Z≡∇X∇Y​Z−∇Y∇X​Z−∇[X,Y]Z\Rm(X,Y)Z\equiv\nabla_{X}\nabla_{Y}Z-\nabla_{Y}\nabla_{X}Z-\nabla_{[X,Y]}Z denotes the Riemann curvature tensor of gg, so it follows that

(3.28) Jα′′(0)=0,Jα′′′(0)=−vγvξRm(∂yα,∂yγ)∂yξ,\displaystyle J^{\prime\prime}_{\alpha}(0)=0,\ J^{\prime\prime\prime}_{\alpha}(0)=-v_{\gamma}v_{\xi}\Rm(\partial_{y_{\alpha}},\partial_{y_{\gamma}})\partial_{y_{\xi}},
(3.29) Ji′′(0)=−vγvξRm(∂xi,∂yγ)∂yξ.\displaystyle J^{\prime\prime}_{i}(0)=-v_{\gamma}v_{\xi}\Rm(\partial_{x_{i}},\partial_{y_{\gamma}})\partial_{y_{\xi}}.

Therefore,

(3.30) gα​β\displaystyle g_{\alpha\beta} =t−2​g​(Jα,Jβ)=δα​β−13​Rmα​γ​ξ​β​vγ​vξ​t2+O~​(t3),\displaystyle=t^{-2}g(J_{\alpha},J_{\beta})=\delta_{\alpha\beta}-\frac{1}{3}\Rm_{\alpha\gamma\xi\beta}v_{\gamma}v_{\xi}t^{2}+\widetilde{O}(t^{3}),
(3.31) gi​j\displaystyle g_{ij} =g(Ji,Jj)=gi​jP+2vαIIi​jαt−(Rmi​γ​ξ​j+⟨∇∂xi∂yγ,∇∂xj∂yξ⟩)vγvξt2+O~(t3),\displaystyle=g(J_{i},J_{j})=g^{P}_{ij}+2v_{\alpha}\IIs_{ij}^{\alpha}t-\Big(\Rm_{i\gamma\xi j}+\langle\nabla_{\partial_{x_{i}}}\partial_{y_{\gamma}},\nabla_{\partial_{x_{j}}}\partial_{y_{\xi}}\rangle\Big)v_{\gamma}v_{\xi}t^{2}+\widetilde{O}(t^{3}),
(3.32) gi​α\displaystyle g_{i\alpha} =t−1g(Ji,Jα)=⟨∇∂xi∂yγ,∂yα⟩vγt−23Rmi​γ​ξ​αvγvξt2+O~(t3).\displaystyle=t^{-1}g(J_{i},J_{\alpha})=\langle\nabla_{\partial_{x_{i}}}\partial_{y_{\gamma}},\partial_{y_{\alpha}}\rangle v_{\gamma}t-\frac{2}{3}\Rm_{i\gamma\xi\alpha}v_{\gamma}v_{\xi}t^{2}+\widetilde{O}(t^{3}).

Let yα=t​vαy_{\alpha}=tv_{\alpha}, then we obtain the desired expansions. ∎

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