Abstract
We show that for certain locally collapsing initial data with Ricci curvature bounded below, one could start the Ricci flow for a definite period of time. This provides a Ricci flow smoothing tool, with which we find topological conditions that detect the collapsing infranil fiber bundles over controlled Riemannian orbifolds among those locally collapsing regions with Ricci curvature bounded below. In the appendix, we also provide a local distance distortion estimate for certain Ricci flows with collapsing initial data.
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Acknowledgements
Both authors would like to thank Xiaochun Rong for enlightening discussions and his warm encouragement, as well as the anonymous referee for helpful comments on the manuscript of the paper. The second-named author is partially supported by NSFC 11971452, NSFC 12026251 and YSBR-001.
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Appendix A: Local distance distortion estimates for Ricci flows with collapsing initial data
Appendix A: Local distance distortion estimates for Ricci flows with collapsing initial data
The distance distortion estimates along Ricci flows is a crucial issue in view of its many natural applications (besides Lemma 4.1 in the proof of Theorem 1.4, see also e.g. [11] for a survey). In [29] a uniform distance distortion estimate for Ricci flows with collapsing initial data has been obtained. That estimate is for compact Ricci flow solutions and only compares the distance functions on nearby positive time slices. Here we present a new distance distortion estimate which can be seen both as an extension (to \(t=0\)) and a localization of the estimate in [29, Theorem 1.1] under some extra assumption on the Ricci curvature:
Theorem A.1
Given a positive integer m, positive constants \({\bar{C}}_0\), \(C_R\), \(T\le 1\) and \(\alpha \in (0,\frac{1}{2(m-1)})\), there are constants \(C_D({\bar{C}}_0,C_R,m)\ge 1\) and \(T_D({\bar{C}}_0,C_R,m)\in (0,T]\) such that for an m-dimensional complete Ricci flow (M, g(t)) with bounded curvature for \(t\in [0,T]\), if for some \(x_0\in M\) and any \(t\in [0,T]\) we have
and the initial metric has a uniform bound \({\bar{C}}_0\) on the doubling and Poincaré constant for the geodesic ball \(B_{g(0)}(x_0,10)\), then for any \(x,y\in B_{g(0)}(x_0,\sqrt{T_D})\) and \(t\in [0,T_D]\), we have
The proof of the lemma is based on the theory of local entropy developed in [48, 49], as well as the local entropy lower bound by volume ratio obtained in [29]. It is inspired by the corresponding results for non-collapsing initial data in [28], and relies on a ball containment argument as surveyed in [11, §3].
Remark 9
Here we will rely on [41, Theorem 2.1], and we point out that the assumptions [41, (1) and (2)] are only needed locally, i.e. the same conclusion of [41, Theorem 2.1] holds even if these conditions on the doubling and Poincaré constants are assumed only within the geodesic ball \(B_{g(0)}\left( x_0,10\right) \): notice that the only global result needed in the proof of this theorem is [41, Theorem 2.2], in which the constants involved only depend on the dimension of the manifold; whereas all other arguments leading to the application of [41, Theorem 2.2] only depend on the doubling and Poincaré constants within the geodesic ball in question.
Proof
By taking \(r_0=\sqrt{t}\) in [39, Lemma 8.3] (see also [23, §17]), the Ricci curvature upper bound in (A.2) tells that if \(x,y\in B_{g(t)}\left( x_0,10\right) \) whenever \(t\le T\), then
To control the distance expansion, we first establish the following a priori estimate
Claim A.2
There exists a uniform constant \({\bar{C}}_1({\bar{C}}_0,C_R, m)>0\) such that if \(x,y \in B_{g(t)}(x_0,10)\) for any \(t\le t_0:=d_0^2\) with \(d_0:=d_{g(0)}(x,y)\le \sqrt{T}\), then \(d_{g(t_0)}(x,y)\le {\bar{C}}_1d_0\).
Proof of the claim
To see this, we let \(\sigma :[0,1]\rightarrow B_{g(0)}\left( x,d_0\right) \) be a minimal g(0)-geodesic realizing \(d_0\), and without loss of generality we may assume that \(d_{g(t_0)}(x,y)\ge 10d_0\). Now let \(\{\sigma (s_i)\}_{i=1}^N\) be a maximal collection of points on the image of \(\sigma \) so that \(d_{g(t_0)}(\sigma (s_i),\sigma (s_{j}))\ge 2d_0\) when \(i\not =j\). By the maximality of \(\left\{ \sigma (s_i)\right\} \), we see that \(B_{g(t_0)}(\sigma (s_i), d_0)\cap B_{g(t_0)}(\sigma (s_j),d_0)=\emptyset \), and it is also clear that \(\left\{ B_{g(t_0)}(\sigma (s_i),2d_0)\right\} \) cover \(Image(\sigma )\). Especially, we have
We therefore only need to bound N uniformly from above. Moreover, by (A.4) we see that for each \(i=1,\ldots ,N\),
Therefore, it is easily seen that each \(B_{g(t_0)}(\sigma (s_i),d_0)\subset B_{g(0)}(\sigma (s_i),(1+8(m-1)\sqrt{\alpha })d_0)\), and consequently, as each \(\sigma (s_i)\in B_{g(0)}(x,d_0)\), we have
We now study the local entropy associated to the various metric balls. We first recall that the uniform bound \({\bar{C}}_0\) on the doubling and Poincaré constants gives a uniform bound on the Sobolev constant \(C_S=C_S(m,{\bar{C}}_0)\), according to [41, Theorem 2.1] (see also Remark 9 and [29, Proposition 2.1]). Therefore, following the argument in [29, §3.1], we get to [29, (3.1)], and by (A.1) we have
for any \(\tau >0\) and any \(v\in W^{1,2}_0(B_{g(0)}(x,8md_0))\) with \(\int _{M}v^2\text {d}V_g=1\). Here due to the selection of v, we have the Perelman’s \({\mathcal {W}}\)-entropy equal to the local entropy \({\mathcal {W}}\left( B_{g(0)}(x,8md_0),g(0),v^2,\tau \right) \), as defined in [48, §2]. Taking the infimum of \({\mathcal {W}} \left( B_{g(0)}(x,8md_0),g(0),v^2,\tau \right) \) among all admissible v described above, we see that for any \(\tau >0\),
Consequently, for \(\varvec{\nu }\left( B_{g(0)}(x,8md_0),g(0),\tau \right) =\inf _{s\in (0,\tau ]}\varvec{\mu }\left( B_{g(0)}(x,8md_0),g(0),s\right) \) we have
On the other hand, by (A.2) we have \(\left| {\mathbf {R}}_{g(t)}\right| \le 2m(m-1)\alpha t^{-1}\) for \(t>0\), and applying [48, Theorem 3.6], we can bound the local entropy from above by volume ratio:
while by (A.2) and the effective monotonicity of the local entropy ([48, Theorem 5.4]), we see that
Moreover, since \(B_{g(0)}(\sigma (s_i),3d_0)\subset B_{g(0)}(x,8md_0)\) for each \(i=1,\ldots ,N\), applying [48, Proposition 2.1] and (A.6) we see that
We now obtain a uniform bound on N. Denoting \(\varvec{\nu }_{i,s}(r,\tau ) :=\varvec{\nu } (B_{g(s)}(\sigma (s_i),r),g(s),\tau )\) for each \(i=1,\ldots ,N\), \(r\le 8md_0\), \(s\le t_0\) and \(\tau \le d_0^2+t_0\), we consecutively apply (A.7), (A.8) and (A.9) with \(t_0=d_0^2\) to see that
Therefore, by the mutual disjointness of \(\left\{ B_{g(t_0)}(\sigma (s_i),d_0)\right\} \) and (A.5) we have
where \(C=\omega _m e^{-2^{m+7}-2C_Rd_0^2-2m(m-1)\alpha -2}(512C_S em^3\pi )^{-\frac{m}{2}}\). Consequently, we easily see that
since \(\alpha <1\), and we emphasize that \(C_S\) is solely determined by \({\bar{C}}_0\) and m. \(\square \)
Now let \(T_0\le T\) be the first time when some point \(y\in B_{g(0)}(x_0,\sqrt{T_0})\) sees \(d_{g(T_0)}(x_0,y)\ge 10\), then applying the estimate established by the claim with \(x_0,y\), we have \(T_0\ \ge \ 100{\bar{C}}_1^{-2}=:T_D({\bar{C}}_0,C_R,m)\). Especially, for any \(x,y\in B_{g(0)}(x_0,\sqrt{T_D})\), we have (A.4) holds without any extra assumption, and for any such points,
Therefore, reasoning in the same way as in [28, Appendix], we have
We now show the other side of the estimate following the same argument as in [28, Appendix]. Given \(x,y\in B_{g(0)}(x_0,\sqrt{T_D})\) satisfying \(d_0=d_{g(0)}(x,y)\le \sqrt{T_D}\) and given \(t\le T_D\), we begin with setting \(N:= \left\lceil d_0t^{-\frac{1}{2}}\right\rceil +1\) so that \(d_0<N\sqrt{t} \le 2\sqrt{T}\le 2\). Dividing a minimal g(0)-geodesic \(\sigma \) that realizes \(d_0\) into N pieces of equal length, i.e. \(\left| \sigma |_{[s_i,s_{i+1}]}\right| =N^{-1}d_0\) for \(0=s_0<\cdots <s_N=1\), by the claim above we see that
moreover, since \(t>N^{-2}d_0^2\), by (A.13) we have
Now adding through \(i=0,1,\ldots ,N-1\), by these inequalities we have
and consequently, we have \(d_{g(t)}(x,y)\le 16^m{\bar{C}}_1d_0^{1-4(m-1)\alpha }\).
Combining this with (A.14) we have the desired estimate
where \(C_D:=\max \left\{ (8m)^{4m},16^m{\bar{C}}_1\right\} \), only depending on \({\bar{C}}_0\) and \(C_R\). \(\square \)
Arguing in the same way, if (A.2) can be assumed globally on M, then we have the following
Corollary A.3
With the same assumptions as in Theorem A.1, but with (A.2) replaced by
then we have for any \(t\le T\) and \(x,y\in B_{g(0)}(x_0,5)\) satisfying \(d_{g(0)}(x,y)\le 1\),
Proof
By (A.15), we see that (A.4) holds for any \(x,y\in B_{g(0)}(x_0,5)\), without any extra assumption, and thus Claim A.2 holds for all such points. Therefore, the rest of the arguments follow without needing to confine ourselves in a smaller geodesic ball. \(\square \)
Remark 10
The referee kindly pointed out to us that a similar distance distortion should hold under curvature bound and scaling invariant injectivity radius lower bond \(r_{inj}\ge ct^{\frac{1}{2}}\) using a similar argument in the proof.