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3.2. Proof of the Transformation theorem [01Y6]

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3.2. Proof of the Transformation theorem

In this subsection, we prove the Transformation theorem (Theorem 1.11) which constitutes the technical heart of the Slicing theorem (Theorem 1.8). We will assume for notational simplicity that MnM^{n} is complete, but it is an easy exercise to show that this may be weakened to the local assumption that B4​(p)B_{4}(p) has compact closure in MnM^{n}. First we recall the definition of the singular scale:

Let u:B2​(p)→ℝku:B_{2}(p)\to\mathds{R}^{k} be a harmonic function. For δ>0\delta>0 let us define for x∈B1​(p)x\in B_{1}(p) the singular scale sxδ≥0s^{\delta}_{x}\geq 0 as the infimum of all radii ss, such that for all s<r<12s<r<\frac{1}{2} and all 1≤ℓ≤k1\leq\ell\leq k we have the estimate

r2​⨏Br​(x)|Δ​|ωℓ||≤δ​⨏Br​(x)|ωℓ|,r^{2}\fint_{B_{r}(x)}|\Delta|\omega^{\ell}||\leq\delta\fint_{B_{r}(x)}|\omega^{\ell}|\,,

where ωℓ=d​u1∧⋯∧d​uℓ\omega^{\ell}=du^{1}\wedge\cdots\wedge du^{\ell}.

Next recall that Theorem 1.11 states the following.

For every ϵ>0\epsilon>0 there exists δ=δ⁡(n,ϵ)>0\delta=\delta(n,\epsilon)>0 such that if RicMn≥−δ2{\rm Ric}_{M^{n}}\geq-\delta^{2} and u:B2​(p)→ℝku:B_{2}(p)\to\mathds{R}^{k} is a harmonic δ2\delta^{2}-splitting map, then for each x∈B1​(p)x\in B_{1}(p) and r≥sxδr\geq s^{\delta}_{x} there exists a lower triangular matrix A=A⁡(x,r)A=A(x,r) such that A∘u:Br​(x)→ℝkA\circ u:B_{r}(x)\to\mathds{R}^{k} is a harmonic ϵ\epsilon-splitting map.

Proof of Theorem 1.11:

The strategy will be a proof by induction. Thus, we will begin with the simplest case of k=1k=1. The following is a slightly more general form of the statement we wish to prove.

Lemma 3.1.

Let u:B2​r​(x)→ℝu:B_{2r}(x)\to\mathds{R} be a harmonic function with r≤1r\leq 1. Then for every ϵ>0\epsilon>0 there exists δ⁡(n,ϵ)>0\delta(n,\epsilon)>0 such that if RicMn≥−(n−1)​δ2{\rm Ric}_{M^{n}}\geq-(n-1)\delta^{2} and

r2​⨏B2​r​(x)|Δ​|∇u||≤δ​⨏B2​r​(x)|∇u|,\displaystyle r^{2}\fint_{B_{2r}(x)}|\Delta|\nabla u||\leq\delta\fint_{B_{2r}(x)}|\nabla u|\,, (3.23)

then for A=(⨏Br​(x)|∇u|)−1>0A=\Big(\fint_{B_{r}(x)}|\nabla u|\Big)^{-1}>0 we have that A∘u:Br​(x)→ℝA\circ u:B_{r}(x)\to\mathds{R} is an ϵ\epsilon-splitting map.

As in (3.6)–(3.8), the Bochner formula (3.11) and the fact that uu is harmonic leads to the improved Kato inequality, |∇|∇ua||2≤n−1n​|∇2ua|2|\nabla|\nabla u^{a}|\,|^{2}\leq\frac{n-1}{n}|\nabla^{2}u^{a}|^{2}, from which we can compute

Δ​|∇u|≥1n​|∇2u|2|∇u|−(n−1)​δ2​|∇u|.\displaystyle\Delta|\nabla u|\geq\frac{1}{n}\frac{|\nabla^{2}u|^{2}}{|\nabla u|}-(n-1)\delta^{2}|\nabla u|\,. (3.24)

In particular, the estimate (3.23) gives rise to the estimate

r2​⨏B2​r​(x)|∇2u|2|∇u|≤C⁡(n)​δ​⨏B2​r​(x)|∇u|,\displaystyle r^{2}\fint_{B_{2r}(x)}\frac{|\nabla^{2}u|^{2}}{|\nabla u|}\leq C(n)\delta\fint_{B_{2r}(x)}|\nabla u|\,, (3.25)

from which, as previously noted (see (3.3), (3.4) ) we get

r​⨏B2​r​(x)|∇2u|≤(r2​⨏B2​r​(x)|∇2u|2|∇u|)1/2⋅(⨏B2​r​(x)|∇u|)1/2≤C​δ1/2​⨏B2​r​(x)|∇u|.\displaystyle r\fint_{B_{2r}(x)}|\nabla^{2}u|\leq\Big(r^{2}\fint_{B_{2r}(x)}\frac{|\nabla^{2}u|^{2}}{|\nabla u|}\Big)^{1/2}\cdot\Big(\fint_{B_{2r}(x)}|\nabla u|\Big)^{1/2}\leq C\delta^{1/2}\fint_{B_{2r}(x)}|\nabla u|\,. (3.26)

Let us put v=(⨏B2​r​(x)|∇u|)−1​uv=\Big(\fint_{B_{2r}(x)}|\nabla u|\Big)^{-1}u, so that ⨏B2​r​(x)|∇v|=1\fint_{B_{2r}(x)}|\nabla v|=1. The lower Ricci bound implies that a Poincaré inequality holds. When combined with the last inequality this implies

⨏B2​r​(x)||∇v|−1|≤C⁡(n)​δ1/2.\displaystyle\fint_{B_{2r}(x)}\big||\nabla v|-1\big|\leq C(n)\delta^{1/2}\,. (3.27)

By using the doubling property, we have after possible increasing C⁡(n)C(n), that for every y∈B3​r/2​(x)y\in B_{3r/2}(x)

⨏Br/2​(y)||∇v|−1|≤C​δ1/2.\displaystyle\fint_{B_{r/2}(y)}\big||\nabla v|-1\big|\leq C\delta^{1/2}\,. (3.28)

In particular,

1−C​δ1/2≤⨏B2​r​(x)|∇u|⨏Br​(x)|∇u|≤1+C​δ1/2.\displaystyle 1-C\delta^{1/2}\leq\frac{\fint_{B_{2r}(x)}|\nabla u|}{\fint_{B_{r}(x)}|\nabla u|}\leq 1+C\delta^{1/2}\,. (3.29)

Hence, if we can show that, δ\delta sufficiently small, the map v:Br​(x)→ℝv:B_{r}(x)\to\mathds{R} is an ϵ/2\epsilon/2-splitting, for k=1k=1, the proof will be complete

Now as in [ChCo1], let φ≥0\varphi\geq 0 be a cutoff function satisfying φ⁡(y)=1\varphi(y)=1 if y∈B5​r/3​(x)y\in B_{5r/3}(x) with φ⁡(y)≡0\varphi(y)\equiv 0 if y∉B2​r​(x)y\not\in B_{2r}(x), and such that r​|∇φ|,r2​|Δ​φ|≤C⁡(n)r|\nabla\varphi|,r^{2}|\Delta\varphi|\leq C(n). Let ρt​(y,d​z)\rho_{t}(y,dz) be the heat kernel on MnM^{n}. Consider for y∈B3​r/2​(x)y\in B_{3r/2}(x) the one parameter family

∫(|∇v|−1)​ϕ​ρt​(y,𝑑z).\displaystyle\int\big(|\nabla v|-1\big)\phi\,\rho_{t}(y,dz)\,. (3.30)

Note that

dd​t​∫(|∇v|−1)​φ​ρt​(y,𝑑z)\displaystyle\frac{d}{dt}\int\Big(|\nabla v|-1\Big)\varphi\,\rho_{t}(y,dz) =∫(|∇2v||∇v|​φ+⟨∇|∇v|,∇φ⟩+(|∇v|−1)​Δ​φ)​ρt​(y,𝑑z),\displaystyle=\int\Big(\frac{|\nabla^{2}v|}{|\nabla v|}\varphi+\langle\nabla|\nabla v|,\nabla\varphi\rangle+(|\nabla v|-1)\Delta\varphi\Big)\rho_{t}(y,dz)\,,
≥−C(n)∫A⁡(3​r/2,2​r)r−1|∇2v|+r−2||∇v|−1|ρt(y,dz),\displaystyle\geq-C(n)\int_{A(3r/2,2r)}r^{-1}|\nabla^{2}v|+r^{-2}\big||\nabla v|-1\big|\rho_{t}(y,dz)\,,
≥−C​δ1/2​r−2,\displaystyle\geq-C\delta^{1/2}r^{-2}\,, (3.31)

where the last inequality is for t∈[0,r2]t\in[0,r^{2}]. Integrating this yields

(|∇v|​(y)−1)≤C​δ1/2+∫(|∇v|−1)​φ​ρr2​(y,𝑑z)≤C​δ1/2+⨏B2​r​(x)||∇v|−1|≤C​δ1/2.\displaystyle(|\nabla v|(y)-1)\leq C\delta^{1/2}+\int\Big(|\nabla v|-1\big)\varphi\,\rho_{r^{2}}(y,dz)\leq C\delta^{1/2}+\fint_{B_{2r}(x)}\big||\nabla v|-1\big|\leq C\delta^{1/2}\,. (3.32)

In particular we have

supB3​r/2​(x)|∇v|≤1+C​δ1/2.\displaystyle\sup_{B_{3r/2}(x)}|\nabla v|\leq 1+C\delta^{1/2}\,. (3.33)

Combining this with the integral estimate (3.28) we get

⨏B3​r/2​(x)||∇v|2−1|≤C​δ1/2.\displaystyle\fint_{B_{3r/2}(x)}\big||\nabla v|^{2}-1\big|\leq C\delta^{1/2}\,. (3.34)

Now using the Bochner formula

Δ​|∇v|2=2​|∇2v|2+2​R​i​c​(∇v,∇v)≥2​|∇2v|2−C​δ2​|∇v|2,\displaystyle\Delta|\nabla v|^{2}=2|\nabla^{2}v|^{2}+2{\rm Ric}(\nabla v,\nabla v)\geq 2|\nabla^{2}v|^{2}-C\delta^{2}|\nabla v|^{2}\,, (3.35)

we can estimate

⨏Br​(x)|∇2v|2\displaystyle\fint_{B_{r}(x)}|\nabla^{2}v|^{2} ≤C⁡(n)​⨏B3​r/2​(x)φ​|∇2v|2\displaystyle\leq C(n)\fint_{B_{3r/2}(x)}\varphi|\nabla^{2}v|^{2} (3.36)
≤C​⨏B3​r/2​(x)φ⁡(Δ⁡(|∇v|2−1)+δ2​|∇v|2)\displaystyle\leq C\fint_{B_{3r/2}(x)}\varphi\Big(\Delta(|\nabla v|^{2}-1)+\delta^{2}|\nabla v|^{2}\Big)
≤C​⨏B3​r/2​(x)|Δ​φ|​||∇v|2−1|+C​δ2​⨏B3​r/2​(x)|∇v|2,\displaystyle\leq C\fint_{B_{3r/2}(x)}|\Delta\varphi|\big||\nabla v|^{2}-1\big|+C\delta^{2}\fint_{B_{3r/2}(x)}|\nabla v|^{2}\,,
≤C​r−2​δ1/2.\displaystyle\leq Cr^{-2}\delta^{1/2}\,. (3.37)

Hence, for δ⁡(n,ϵ)\delta(n,\epsilon) sufficiently we have that vv is an ϵ/2\epsilon/2-splitting, which as previously remarked, proves the theorem for the case k=1k=1.

We now turn to the proof of Theorem 1.11, which will proceed by induction.

Assume the Theorem has been proved for some k−1≥1k-1\geq 1. We will prove the result for kk by arguing by contradiction.

Thus, we can suppose that for some ϵ>0\epsilon>0 the result is false. There is no harm is assuming 0<ϵ≤ϵ⁡(n)0<\epsilon\leq\epsilon(n) is sufficiently small. Then, for some δj→0\delta_{j}\to 0 we can find a sequence of spaces (Mjn,gj,pj)(M^{n}_{j},g_{j},p_{j}) with RicMjn≥−δj2{\rm Ric}_{M^{n}_{j}}\geq-\delta_{j}^{2} and mappings uj:B2​(pj)→ℝku_{j}:B_{2}(p_{j})\to\mathds{R}^{k} which are δj2\delta_{j}^{2}-splitting mappings, for which there exists xj∈B1​(pj)x_{j}\in B_{1}(p_{j}) and radii rj≥sδj​(xj)r_{j}\geq s^{\delta_{j}}(x_{j}), such that there is no matrix AA such that A∘u:Brj​(xj)→ℝkA\circ u:B_{r_{j}}(x_{j})\to\mathds{R}^{k} is an ϵ\epsilon-splitting map. Without loss of generality, we can assume rjr_{j} is the supremum of those radii for which there is no such matrix. In particular, there exists such a matrix AjA_{j} corresponding to the radius 2​rj2r_{j}. Observe that rj→0r_{j}\to 0. Indeed, we can see this just by using the identity map A=IA=I, since δj→0\delta_{j}\to 0 and u:B2​(p)→ℝ2u:B_{2}(p)\to\mathds{R}^{2} is a δj2\delta_{j}^{2}-splitting map.

Now, consider the rescaled spaces (Mjn,gj′,xj)(M^{n}_{j},g^{\prime}_{j},x_{j}) with gj′≡rj−2​gg^{\prime}_{j}\equiv r_{j}^{-2}g, and let vj≡Aj∘(uj−uj​(xj)):B2​rj−1​(xj)→ℝkv_{j}\equiv A_{j}\circ\big(u_{j}-u_{j}(x_{j})\big):B_{2r^{-1}_{j}}(x_{j})\to\mathds{R}^{k} be a harmonic function on this space. We have normalized so that v⁡(xj)=0v(x_{j})=0.

We have that vj:B2​(xj)→ℝkv_{j}:B_{2}(x_{j})\to\mathds{R}^{k} is an ϵ\epsilon-splitting, and indeed for any 2≤r≤2​rj−12\leq r\leq 2r_{j}^{-1} there exists some matrix ArA_{r} such that Ar∘v:Br​(xj)→ℝkA_{r}\circ v:B_{r}(x_{j})\to\mathds{R}^{k} is an ϵ\epsilon-splitting.

Note: Throughout the remainder of the argument, when there is no danger of confusion, for ease of notation, we will sometimes omit the subscript jj from various quantities including vv and AA, which in actuality depend on jj. For example, we omit the subcript jj from the matrices Ar,A2​rA_{r},\,A_{2r} in Claim 1 below.

We will now break the proof into a series of claims.

Claim 1: For each 2≤r≤rj−22\leq r\leq r_{j}^{-2} we have

(1−C⁡(n)​ϵ)​A2​r≤Ar≤(1+C⁡(n)​ϵ)​A2​r.(1-C(n)\epsilon)A_{2r}\leq A_{r}\leq(1+C(n)\epsilon)A_{2r}\,. (3.38)

The defining properties of the matrices A2​rA_{2r} is that they are lower triangular and that A2​r∘v:B2​r​(xj)→ℝkA_{2r}\circ v:B_{2r}(x_{j})\to\mathds{R}^{k} is an ϵ\epsilon-splitting map. In particular, we have the estimate

(2​r)2​⨏B2​r​(xj)|⟨∇(A2​r∘v)a,∇(A2​r∘v)b⟩−δa​b|<ϵ,\displaystyle(2r)^{2}\fint_{B_{2r}(x_{j})}\big|\langle\nabla(A_{2r}\circ v)_{a},\nabla(A_{2r}\circ v)_{b}\rangle-\delta_{ab}\big|<\epsilon\,, (3.39)

and thus, by doubling of the volume measure, we have

r2​⨏Br​(xj)|⟨∇(A2​r∘v)a,∇(A2​r∘v)b⟩−δa​b|<C⁡(n)​ϵ.\displaystyle r^{2}\fint_{B_{r}(x_{j})}\big|\langle\nabla(A_{2r}\circ v)_{a},\nabla(A_{2r}\circ v)_{b}\rangle-\delta_{ab}\big|<C(n)\epsilon\,. (3.40)

However in addition we also have

r2​⨏Br​(xj)|⟨∇(Ar∘v)a,∇(Ar∘v)b⟩−δa​b|<ϵ.\displaystyle r^{2}\fint_{B_{r}(x_{j})}\big|\langle\nabla(A_{r}\circ v)_{a},\nabla(A_{r}\circ v)_{b}\rangle-\delta_{ab}\big|<\epsilon\,. (3.41)

Combining this with the assumption that both Ar,A2​rA_{r},\,A_{2r} are lower triangular proves the claim. □\square

Now let us record some very important consequences of Claim 1. First, since by our normalization, A2≡IA_{2}\equiv I, we have for r≥2r\geq 2 the sublinear growth estimate

|Ar|,|Ar−1|≤rC⁡(n)​ϵ.\displaystyle|A_{r}|,\,|A^{-1}_{r}|\leq r^{C(n)\epsilon}\,. (3.42)

In particular, since Ar∘v:Br​(xj)→ℝkA_{r}\circ v:B_{r}(x_{j})\to\mathds{R}^{k} is an ϵ\epsilon-splitting, and hence supBr​(xj)|∇(Ar∘v)|≤1+ϵ\sup_{B_{r}(x_{j})}|\nabla(A_{r}\circ v)|\leq 1+\epsilon, we have for any 2≤r≤rj−12\leq r\leq r_{j}^{-1} the sublinear growth conditions

supBr​(xj)|∇vja|≤(1+C​ϵ)​rC​ϵ,\displaystyle\sup_{B_{r}(x_{j})}|\nabla v^{a}_{j}|\leq(1+C\epsilon)r^{C\epsilon}\,,
supBr​(xj)|ωj|≤(1+C​ϵ)​rC​ϵ,\displaystyle\sup_{B_{r}(x_{j})}|\omega_{j}|\leq(1+C\epsilon)r^{C\epsilon}\,,
r2​⨏Br​(xj)|∇2vja|2≤C​ϵ​rC​ϵ,\displaystyle r^{2}\fint_{B_{r}(x_{j})}|\nabla^{2}v^{a}_{j}|^{2}\leq C\epsilon r^{C\epsilon}\,, (3.43)

where ωj≡d​vj1∧⋯∧d​vjk\omega_{j}\equiv dv_{j}^{1}\wedge\cdots\wedge dv_{j}^{k} is the pullback kk-form.

Remark 3.1.

The sublinearity of the growth estimates in (3.43) will play a fundamental role in the proof; see in particular, Claims 3–5.

Our first application of these estimates is the following, which uses the induction statement to conclude that vj1,…,vjk−1v_{j}^{1},\ldots,v_{j}^{k-1} are improving in their splitting behavior as j→∞j\to\infty.

Claim 2: There exists a lower triangular matrix AA such that A∘v:B2​(xj)→ℝkA\circ v:B_{2}(x_{j})\to\mathds{R}^{k} is a C⁡(n)​ϵC(n)\epsilon-splitting while for each R>0R>0 the restricted map A∘v:BR​(xj)→ℝk−1A\circ v:B_{R}(x_{j})\to\mathds{R}^{k-1}, obtained by dropping the last function, is an ϵj​(R)\epsilon_{j}(R)-splitting map, where ϵj​(R)→0\epsilon_{j}(R)\to 0.

To prove the claim let us first denote by v~:B2​rj−1​(xj)→ℝk−1\tilde{v}:B_{2r_{j}^{-1}}(x_{j})\to\mathds{R}^{k-1} the map obtained by dropping the last function vkv^{k}. By our induction hypothesis there exists for every r≥2r\geq 2 an lower triangular matrix A~r∈G​L​(k−1)\tilde{A}_{r}\in GL(k-1) such that A~r∘v~:Br​(xj)→ℝk−1\tilde{A}_{r}\circ\tilde{v}:B_{r}(x_{j})\to\mathds{R}^{k-1} is an ϵj\epsilon_{j}-splitting map with ϵj→0\epsilon_{j}\to 0. Since both v~\tilde{v} and A~2∘v~\tilde{A}_{2}\circ\tilde{v} are in particular ϵ\epsilon-splittings on B2​(xj)B_{2}(x_{j}) with A~2\tilde{A}_{2} lower triangular, then arguments similar to those in Claim 1 give |A~2−I|<C⁡(n)​ϵ|\tilde{A}_{2}-I|<C(n)\epsilon, and the growth estimates

supBr​(xj)|∇(A~2∘v~)|\displaystyle\sup_{B_{r}(x_{j})}|\nabla(\tilde{A}_{2}\circ\tilde{v})| ≤(1+C​ϵj)​rC​ϵj,\displaystyle\leq(1+C\epsilon_{j})r^{C\epsilon_{j}}\,,
r2​⨏Br​(xj)|∇2(A~2∘v~)|2\displaystyle r^{2}\fint_{B_{r}(x_{j})}|\nabla^{2}(\tilde{A}_{2}\circ\tilde{v})|^{2} ≤C​ϵj​rC​ϵj.\displaystyle\leq C\epsilon_{j}r^{C\epsilon_{j}}\,. (3.44)

In particular, we can use the Hessian estimate and a Poincaré inequality to conclude

|⨏B2|⟨∇(A~2∘v~)a,\displaystyle\Big|\fint_{B_{2}}\big|\langle\nabla(\tilde{A}_{2}\circ\tilde{v})^{a}, ∇(A~2∘v~)b⟩−δa​b|−⨏BR|⟨∇(A~2∘v~)a,∇(A~2∘v~)b⟩−δa​b||\displaystyle\nabla(\tilde{A}_{2}\circ\tilde{v})^{b}\rangle-\delta^{ab}\big|-\fint_{B_{R}}\big|\langle\nabla(\tilde{A}_{2}\circ\tilde{v})^{a},\nabla(\tilde{A}_{2}\circ\tilde{v})^{b}\rangle-\delta^{ab}\big|\Big|
≤⨏B2||⟨∇(A~2∘v~)a,∇(A~∘​2​v~)b⟩−δa​b|−⨏BR|⟨∇(A~2∘v~)a,∇(A~2∘v~)b⟩−δa​b||\displaystyle\leq\fint_{B_{2}}\Big||\langle\nabla(\tilde{A}_{2}\circ\tilde{v})^{a},\nabla(\tilde{A}_{\circ}2\tilde{v})^{b}\rangle-\delta^{ab}\big|-\fint_{B_{R}}\big|\langle\nabla(\tilde{A}_{2}\circ\tilde{v})^{a},\nabla(\tilde{A}_{2}\circ\tilde{v})^{b}\rangle-\delta^{ab}\big|\Big|
≤C⁡(n,R)​⨏BR||⟨∇(A~2∘v~)a,∇(A~2∘v~)b⟩−δa​b|−⨏BR|⟨∇(A~2∘v~)a,∇(A~2∘v~)b⟩−δa​b||\displaystyle\leq C(n,R)\fint_{B_{R}}\Big||\langle\nabla(\tilde{A}_{2}\circ\tilde{v})^{a},\nabla(\tilde{A}_{2}\circ\tilde{v})^{b}\rangle-\delta^{ab}\big|-\fint_{B_{R}}\big|\langle\nabla(\tilde{A}_{2}\circ\tilde{v})^{a},\nabla(\tilde{A}_{2}\circ\tilde{v})^{b}\rangle-\delta^{ab}\big|\Big|
≤C⁡(n,R)​⨏BR|∇⟨∇(A~2∘v~)a,∇(A~2∘v~)b⟩|≤ϵj​(R)→0.\displaystyle\leq C(n,R)\fint_{B_{R}}\big|\nabla\langle\nabla(\tilde{A}_{2}\circ\tilde{v})^{a},\nabla(\tilde{A}_{2}\circ\tilde{v})^{b}\rangle\big|\leq\epsilon_{j}(R)\to 0\,. (3.45)

Thus for each R>0R>0 we have A~2∘v~:BR​(xj)→ℝk−1\tilde{A}_{2}\circ\tilde{v}:B_{R}(x_{j})\to\mathds{R}^{k-1} is an ϵj​(R)\epsilon_{j}(R)-splitting. Finally, if we let A=A~2⊕1A=\tilde{A}_{2}\oplus 1 act on ℝk\mathds{R}^{k} by fixing the last component then we have proved the claim. □\square

Note: We will from time to time in the proof replace vv by A∘vA\circ v, where AA is a lower triangular matrix with |A−I|<C⁡(n)​ϵ|A-I|<C(n)\epsilon. In particular, from this point on in the proof, we will assume vav^{a} has been normalized as in Claim 2. Thus va:B2​(xj)→ℝkv^{a}:B_{2}(x_{j})\to\mathds{R}^{k} will be taken to be an C​ϵC\epsilon-splitting, while va:BR​(xj)→ℝk−1v^{a}:B_{R}(x_{j})\to\mathds{R}^{k-1} is an ϵj​(R)\epsilon_{j}(R)-splitting map.

A useful consequence is that we have for each R>0R>0 and 1≤ℓ≤k−11\leq\ell\leq k-1 that

⨏BR​(xj)|∇2va|2≤ϵj​(R)→0.\displaystyle\fint_{B_{R}(x_{j})}|\nabla^{2}v^{a}|^{2}\leq\epsilon_{j}(R)\to 0\,. (3.46)
Remark 3.2.

By way of orientation, we mention at this point that our long term goal is to show

⨏BR​(xj)|∇2vjk|2≤ϵj​(R)→0\fint_{B_{R}(x_{j})}|\nabla^{2}v^{k}_{j}|^{2}\leq\epsilon_{j}(R)\to 0\,

which is the content of Claim 6. Once this has been achieved, the proof will be virtually complete.

Our next goal is to study in more detail the properties of ωj=ωjk=d​vj1∧⋯∧d​vjk\omega_{j}=\omega^{k}_{j}=dv^{1}_{j}\wedge\cdots\wedge dv^{k}_{j}. First, since

∇ωj=∇(d​vj1)∧⋯∧d​vjk+⋯+d​vj1∧⋯∧∇(d​vjk),\displaystyle\nabla\omega_{j}=\nabla(dv^{1}_{j})\wedge\cdots\wedge dv^{k}_{j}+\cdots+dv^{1}_{j}\wedge\cdots\wedge\nabla(dv^{k}_{j})\,, (3.47)

we can use (3.43) to obtain for 2≤r≤rj−12\leq r\leq r_{j}^{-1} that

r2​⨏Br​(xj)|∇ωj|2≤C​ϵ​rC​ϵ.\displaystyle r^{2}\fint_{B_{r}(x_{j})}|\nabla\omega_{j}|^{2}\leq C\epsilon\,r^{C\epsilon}\,. (3.48)

Recall that our underlying assumptions are that we have for every r≥1r\geq 1 the estimate

r2​⨏Br​(xj)|Δ​|ωj||≤δj​⨏Br​(xj)|ωj|.\displaystyle r^{2}\fint_{B_{r}(x_{j})}|\Delta|\omega_{j}|\,|\leq\delta_{j}\fint_{B_{r}(x_{j})}|\omega_{j}|\,. (3.49)

By combining this with (3.43), we get that for every 2≤r≤rj−12\leq r\leq r_{j}^{-1},

r2​⨏Br​(xj)|Δ​|ωj||≤C​δj​rC​ϵ.\displaystyle r^{2}\fint_{B_{r}(x_{j})}|\Delta|\omega_{j}|\,|\leq C\delta_{j}r^{C\epsilon}\,. (3.50)

Now we are ready to make our third claim:

Claim 3: For each fixed R≥1R\geq 1, we have ⨏BR​(xj)||ωj|2−⨏BR​(xj)|ωj|2|→0\fint_{B_{R}(x_{j})}\big||\omega_{j}|^{2}-\fint_{B_{R}(x_{j})}|\omega_{j}|^{2}\big|\to 0.

The proof of Claim 3 will rely on the sublinear growth estimates (3.43), (3.48), (3.50), standard heat kernel estimates for almost nonnegative Ricci curvature, (3.55)–(3.57) and the Bakry-Emery gradient estimate for the heat kernel (3.64). In particular, the sublinear growth condition in (3.48) enters crucially in (3.63) and its consequence (3.66).

Fix R≥1R\geq 1 and consider the maximal function

MR​(x)≡supr≤R⨏Br​(x)|Δ​|ωj||,\displaystyle M^{R}(x)\equiv\sup_{r\leq R}\fint_{B_{r}(x)}|\Delta|\omega_{j}||\,, (3.51)

for x∈BR​(xj)x\in B_{R}(x_{j}). Since by the Bishop-Gromov inequality, the Riemannian measure is doubling, we can combine the usual maximal function arguments with (3.50) and conclude that there exists a subset Uj⊆BR​(xj)U_{j}\subseteq B_{R}(x_{j}) such that

Vol⁡(BR​(xj)∖Uj)Vol⁡(BR​(xj))≤ϵj​(R)→0,\displaystyle\frac{{\rm Vol}(B_{R}(x_{j})\setminus U_{j})}{{\rm Vol}(B_{R}(x_{j}))}\leq\epsilon_{j}(R)\to 0\,,
MR​(x)≤ϵj​(R)→0,\displaystyle M^{R}(x)\leq\epsilon_{j}(R)\to 0\,, (3.52)

for all x∈Ujx\in U_{j}. Relation (3.52) will be used in (3.59).

As a point of notation, we mention that below, the symbol, ϵj​(R)\epsilon_{j}(R), will always denote a quantity, regardless of origin, satisfying ϵj​(R)→0\epsilon_{j}(R)\to 0 when j→∞j\to\infty with RR fixed. Likewise for the symbol ϵj​(S)\epsilon_{j}(S).

Now let φ≥0\varphi\geq 0 be a smooth cutoff function as in [ChCo1], such that φ≡1\varphi\equiv 1 on Brj−1/2​(p)B_{r_{j}^{-1}/2}(p), supp​(φ)⊂Brj−1​(p){\rm supp}(\varphi)\subset B_{r_{j}^{-1}}(p), and such that r−1j|∇φ|,rj−2|r^{-1}_{j}|\nabla\varphi|,r_{j}^{-2}|Δ​φ|≤C⁡(n)\Delta\varphi|\leq C(n). For x∈BR​(xj)x\in B_{R}(x_{j}) let us consider the function

∫|ωj|​φ​ρt​(x,𝑑y),\displaystyle\int|\omega_{j}|\varphi\rho_{t}(x,dy)\,, (3.53)

where ρt\rho_{t} is the heat kernel centered at xx. Then we have the equality

dd​t​∫|ωj|​φ​ρt​(x,𝑑y)=∫(Δ​|ωj|​φ+⟨∇|ωj|,∇φ⟩+|ωj|​Δ​φ)​ρt​(x,𝑑y).\displaystyle\frac{d}{dt}\int|\omega_{j}|\varphi\rho_{t}(x,dy)=\int\Big(\Delta|\omega_{j}|\varphi+\langle\nabla|\omega_{j}|,\nabla\varphi\rangle+|\omega_{j}|\Delta\varphi\Big)\rho_{t}(x,dy)\,. (3.54)

As a consequence of our assumption that RicMjn≥−δj2​rj2{\rm Ric}_{M^{n}_{j}}\geq-\delta^{2}_{j}r_{j}^{2}, we have the usual heat kernel estimates [SY]

ρt(x,y)≤C(n)Vol(Bt(x))−1/2Vol(Bt(y))−1/2e−d2​(x,y)2​t+C⁡(n)​δj2​rj2​t,\rho_{t}(x,y)\leq C(n){\rm Vol}(B_{\sqrt{t}}(x))^{-1/2}{\rm Vol}(B_{\sqrt{t}}(y))^{-1/2}e^{-\frac{d^{2}(x,y)}{2t}+C(n)\delta^{2}_{j}r_{j}^{2}t}\,, (3.55)

which implies that for y∈Brj−1​(x)y\in B_{r_{j}^{-1}}(x) and t≤rj−2t\leq r_{j}^{-2}, we have

ρt(x,y)≤C(n)Vol(Bt(x))−1/2Vol(Bt(y))−1/2e−d2​(x,y)2​t.\rho_{t}(x,y)\leq C(n){\rm Vol}(B_{\sqrt{t}}(x))^{-1/2}{\rm Vol}(B_{\sqrt{t}}(y))^{-1/2}e^{-\frac{d^{2}(x,y)}{2t}}\,. (3.56)

We can use the volume doubling and monotonicity property to observe the following useful inequality. If y∈Br​(x)y\in B_{r}(x), then

ρt​(x,y)\displaystyle\rho_{t}(x,y) ≤C⁡(n)​(Vol​(Br​(x))Vol​(Bt​(x))1/2​Vol​(Bt​(y))1/2)​Vol​(Br​(x))−1​e−d2​(x,y)2​t\displaystyle\leq C(n)\Big(\frac{{\rm Vol}(B_{r}(x))}{{\rm Vol}(B_{\sqrt{t}}(x))^{1/2}{\rm Vol}(B_{\sqrt{t}}(y))^{1/2}}\Big){\rm Vol}(B_{r}(x))^{-1}e^{-\frac{d^{2}(x,y)}{2t}}
≤C⁡(n)​(rt1/2)n​Vol​(Br​(x))−1​e−d2​(x,y)2​t.\displaystyle\leq C(n)\Big(\frac{r}{t^{1/2}}\Big)^{n}{\rm Vol}(B_{r}(x))^{-1}e^{-\frac{d^{2}(x,y)}{2t}}\,. (3.57)

Let us fix S>>R≥2S>>R\geq 2 and consider times 0<t≤S20<t\leq S^{2}. By combining the heat kernel estimate, (3.57), with the growth estimates (3.43), (3.48), for all x∈BR​(xj)x\in B_{R}(x_{j}) and 0<t≤S20<t\leq S^{2}, we can bound the second two terms of the last equation by

∫|⟨∇|ωj|,∇φ⟩+|ωj|​Δ​φ|​ρt​(x,𝑑y)\displaystyle\int\big|\langle\nabla|\omega_{j}|,\nabla\varphi\rangle+|\omega_{j}|\Delta\varphi|\rho_{t}(x,dy) =∫Arj−1/2,rj−1​(xj)|⟨∇|ωj|,∇φ⟩+|​ωj​‖Δ​φ‖​ρt​(x,𝑑y)\displaystyle=\int_{A_{r_{j}^{-1}/2,r_{j}^{-1}}(x_{j})}\big|\langle\nabla|\omega_{j}|,\nabla\varphi\rangle+|\omega_{j}|\,|\Delta\varphi|\big|\rho_{t}(x,dy)\,
≤CrjrjC​ϵVol(Brj(xj))Vol(Bt(x))−1/2Vol(Bt(y))−1/2e−12​t​rj−2\displaystyle\leq Cr_{j}r_{j}^{C\epsilon}{\rm Vol}(B_{r_{j}}(x_{j})){\rm Vol}(B_{\sqrt{t}}(x))^{-1/2}{\rm Vol}(B_{\sqrt{t}}(y))^{-1/2}\,e^{-\frac{1}{2t}r^{-2}_{j}}
≤C​rj2+C​ϵ​(rjt1/2)n​e−12​t​rj−2≤ϵj​(S)→0.\displaystyle\leq Cr_{j}^{2+C\epsilon}\Big(\frac{r_{j}}{t^{1/2}}\Big)^{n}e^{-\frac{1}{2t}r^{-2}_{j}}\leq\epsilon_{j}(S)\to 0\,. (3.58)

Note that the sublinear growth in (3.43), (3.48), is not crucial here. Polynomial growth would suffice.

To estimate the first term of (3.54) is more involved. To this end, we begin with an estimate in which we must restrict attention to points x∈Uj⊆BR​(xj)x\in U_{j}\subseteq B_{R}(x_{j}); see (3.52). Below, we write t=r2t=r^{2} and so, we consider 0<r<S0<r<S. We also put rα=2α​rr^{\alpha}=2^{\alpha}r. Suppose first that t=r≤R\sqrt{t}=r\leq R. Then we have

∫|Δ​|ωj||φ​ρr2​(x,𝑑y)\displaystyle\int\big|\Delta|\omega_{j}|\big|\varphi\rho_{r^{2}}(x,dy) =∫Br​(x)|Δ|​ωj​‖φ​ρr2​(x,𝑑y)+∑α∫Arα,rα+1​(x)|Δ|​ωj‖​φ​ρr2​(x,𝑑y)\displaystyle=\int_{B_{r}(x)}\big|\Delta|\omega_{j}|\big|\varphi\rho_{r^{2}}(x,dy)+\sum_{\alpha}\int_{A_{r^{\alpha},r^{\alpha+1}}(x)}\big|\Delta|\omega_{j}|\big|\varphi\rho_{r^{2}}(x,dy)\, (3.59)
≤C⁡(n)​⨏Br​(x)|Δ​|ωj||+C⁡(n)​∑α(rαr)n​e−(r−1​rα)2​⨏B2α​r​(x)|Δ​|ωj||\displaystyle\leq C(n)\fint_{B_{r}(x)}\big|\Delta|\omega_{j}|\,\big|+C(n)\sum_{\alpha}\Big(\frac{r_{\alpha}}{r}\Big)^{n}e^{-\big(r^{-1}r^{\alpha}\big)^{2}}\fint_{B_{2^{\alpha}r}(x)}\big|\Delta|\omega_{j}|\,\big|
≤C⁡(n)​⨏Br​(x)|Δ​|ωj||+C⁡(n)​∑α2n​α​e−22​α​⨏B2α​r​(x)|Δ​|ωj||\displaystyle\leq C(n)\fint_{B_{r}(x)}\big|\Delta|\omega_{j}|\,\big|+C(n)\sum_{\alpha}2^{n\alpha}e^{-2^{2\alpha}}\fint_{B_{2^{\alpha}r}(x)}\big|\Delta|\omega_{j}|\,\big|
=C⁡(n)​⨏Br​(x)|Δ​|ωj||+C⁡(n)​∑rα≤R2n​α​e−22​α​⨏B2α​r​(x)|Δ​|ωj||+C⁡(n)​∑rα>R2n​α​e−22​α​⨏B2α​r​(x)|Δ​|ωj||\displaystyle=C(n)\fint_{B_{r}(x)}\big|\Delta|\omega_{j}|\big|+C(n)\sum_{r^{\alpha}\leq R}2^{n\alpha}e^{-2^{2\alpha}}\fint_{B_{2^{\alpha}r}(x)}\big|\Delta|\omega_{j}|\,\big|+C(n)\sum_{r^{\alpha}>R}2^{n\alpha}e^{-2^{2\alpha}}\fint_{B_{2^{\alpha}r}(x)}\big|\Delta|\omega_{j}|\,\big|\,
≤C​ϵj​(R)+C​∑rα≤R2n​α​e−22​α​ϵj​(R)+C​R−2​∑rα>R2n​α​e−22​α​δj→0.\displaystyle\leq C\epsilon_{j}(R)+C\sum_{r^{\alpha}\leq R}2^{n\alpha}e^{-2^{2\alpha}}\epsilon_{j}(R)+CR^{-2}\sum_{r^{\alpha}>R}2^{n\alpha}e^{-2^{2\alpha}}\delta_{j}\to 0\,.

Note that in estimating the first two terms in the last line of (3.59) we use the maximal function estimate (3.52), which is the reason for restricting attention to x∈Ujx\in U_{j}. For the third term in the last line we use (3.50).

Similarly, t=r>R\sqrt{t}=r>R, the first two terms on the last line of (3.59) are absent and we just get

∫|Δ​|ωj||φ​ρr2​(x,𝑑y)≤C​R−2​∑α2n​α​e−22​α​δj→0.\displaystyle\int\big|\Delta|\omega_{j}|\big|\varphi\rho_{r^{2}}(x,dy)\leq CR^{-2}\sum_{\alpha}2^{n\alpha}e^{-2^{2\alpha}}\delta_{j}\to 0\,.\ (3.60)

By combining (3.54), (3.58), (3.59), (3.60), we get for x∈Ujx\in U_{j} and 0<t≤S20<t\leq S^{2},

|dd​t​∫|ωj|​φ​ρt​(x,𝑑y)|≤ϵj​(S)→0,\displaystyle\Big|\frac{d}{dt}\int|\omega_{j}|\varphi\rho_{t}(x,dy)\Big|\leq\epsilon_{j}(S)\to 0\,, (3.61)

uniformly in UjU_{j}.

At this point, by using (3.61) and integrating with respect to tt from 00 to S2S^{2}, we have for any x∈Uj⊆BR​(xj)x\in U_{j}\subseteq B_{R}(x_{j}),

||ωj|​(x)−∫|ωj|​φ​ρS2​(x,𝑑y)|≤ϵj​(S)⋅S2→0,\displaystyle\Big||\omega_{j}|(x)-\int|\omega_{j}|\varphi\rho_{S^{2}}(x,dy)\Big|\leq\epsilon_{j}(S)\cdot S^{2}\to 0\,, (3.62)

uniformly in UjU_{j}.

By arguing in a manner similar to the above (but without the need for a maximal function estimate) we can use (3.48), to see that for all x∈B2​R​(xj)x\in B_{2R}(x_{j})

∫|∇(|ωj|​φ)|2​ρS2​(x,𝑑y)\displaystyle\int\big|\nabla(|\omega_{j}|\varphi)\big|^{2}\rho_{S^{2}}(x,dy) ≤2​∫|∇ωj|2+|ωj|2​|∇φ|2​ρS2​(x,𝑑y)\displaystyle\leq 2\int|\nabla\omega_{j}|^{2}+|\omega_{j}|^{2}|\nabla\varphi|^{2}\rho_{S^{2}}(x,dy)
≤C​∑2n​α​e−22​α​⨏B2α​S​(x)|∇ωj|2+C​rj2−C​ϵ​(rjS)n​e−1S2​rj−2\displaystyle\leq C\sum 2^{n\alpha}e^{-2^{2\alpha}}\fint_{B_{2^{\alpha}S}(x)}|\nabla\omega_{j}|^{2}+Cr_{j}^{2-C\epsilon}\Big(\frac{r_{j}}{S}\Big)^{n}e^{-\frac{1}{S^{2}}r_{j}^{-2}}\,
≤C​S−2+C​ϵ+ϵj​(S),\displaystyle\leq C\,S^{-2+C\epsilon}+\epsilon_{j}(S)\,, (3.63)

where without loss of generality, we can assume that our original ϵ\epsilon has been chosen so that −2+C​ϵ<0-2+C\epsilon<0. As previously mentioned, it is at just this point that the sublinearity in (3.48) has entered crucially, giving rise to the negative power of SS in (3.63), which comes to fruition in (3.66).

We have that Ht​(|ωj|​φ)=∫|ωj|​φ​ρt​(x,𝑑y)H_{t}\big(|\omega_{j}|\varphi\big)=\int|\omega_{j}|\varphi\rho_{t}(x,dy) solves the heat equation. So using the Bakry-Emery gradient estimate, [BE85], we have for any x∈B2​R​(xj)x\in B_{2R}(x_{j})

|∇Ht​(|ωj|​φ)|2​(x)≤eδj2​rj2​t​Ht​|∇(|ωj|​φ)|2​(x).\displaystyle|\nabla H_{t}\big(|\omega_{j}|\varphi\big)|^{2}(x)\leq e^{\delta_{j}^{2}r_{j}^{2}t}H_{t}|\nabla(|\omega_{j}|\varphi)|^{2}(x)\,. (3.64)

In particular, using (3.63) we have

supB2​R​(xj)|∇x∫|ωj|φρS2(x,dy)|≤CS1−C​ϵ/2+ϵj(S).\displaystyle{}\sup_{B_{2R}(x_{j})}\Big|\nabla_{x}\int|\omega_{j}|\varphi\rho_{S^{2}}(x,dy)\Big|\leq\frac{C}{S^{1-C\epsilon/2}}+\epsilon_{j}(S)\,. (3.65)

Combining this with (3.62) we get for any pair of points, x,y∈Ujx,y\in U_{j},

||ωj|​(x)−|​ωj​|(y)|\displaystyle\big|\,|\omega_{j}|(x)-|\omega_{j}|(y)\big| ≤|ωj​(x)−∫|ωj|​φ​ρS2​(x,𝑑z)|+|ωj​(y)−∫|ωj|​φ​ρS2​(y,𝑑z)|\displaystyle\leq\big|\omega_{j}(x)-\int|\omega_{j}|\varphi\rho_{S^{2}}(x,dz)\big|+\big|\omega_{j}(y)-\int|\omega_{j}|\varphi\rho_{S^{2}}(y,dz)\big|
+|∫|ωj​|φ​ρS2​(x,𝑑y)−∫|ωj|​φ​ρS2​(y,𝑑z)|\displaystyle+\big|\int|\omega_{j}|\varphi\rho_{S^{2}}(x,dy)-\int|\omega_{j}|\varphi\rho_{S^{2}}(y,dz)\big|
≤ϵj​(S)+C​RS1−C​ϵ/2.\displaystyle\leq\epsilon_{j}(S)+\frac{CR}{S^{1-C\epsilon/2}}\,. (3.66)

By letting SS tend to infinity sufficiently slowly, we get for x,y∈Ujx,y\in U_{j}, that

||ωj|​(x)−|​ωj​|(y)|\displaystyle\big|\,|\omega_{j}|(x)-|\omega_{j}|(y)\big| ≤ϵj​(R)→0.\displaystyle\leq\epsilon_{j}(R)\to 0\,. (3.67)

Finally, to finish the proof, we use the supremum bound (3.48) on |ω||\omega| to note that for x∈Ujx\in U_{j}, we have

|⨏BR​(xj)|ωj|2−|ωj|2​(x)|\displaystyle\Big|\fint_{B_{R}(x_{j})}|\omega_{j}|^{2}-|\omega_{j}|^{2}(x)\Big| ≤⨏BR​(xj)||ωj|2−|ωj|2​(x)|\displaystyle\leq\fint_{B_{R}(x_{j})}\Big||\omega_{j}|^{2}-|\omega_{j}|^{2}(x)\Big|
≤⨏BR​(xj)||ωj|−|​ωj​|(x)|⋅||ωj|+|​ωj​|(x)|\displaystyle\leq\fint_{B_{R}(x_{j})}\big||\omega_{j}|-|\omega_{j}|(x)\big|\cdot\big||\omega_{j}|+|\omega_{j}|(x)\big| (3.68)
≤C⁡(n,R)​⨏BR​(xj)||ωj|−|​ωj​|(x)|\displaystyle\leq C(n,R)\fint_{B_{R}(x_{j})}\big||\omega_{j}|-|\omega_{j}|(x)\big|
≤C⁡(n,R)​⨏Uj||ωj|−|ωj|​(x)|+C⁡(n,R)​⨏BR​(xj)∖Uj||ωj|−|ωj|​(x)|\displaystyle\leq C(n,R)\fint_{U_{j}}\big||\omega_{j}|-|\omega_{j}|(x)\big|+C(n,R)\fint_{B_{R}(x_{j})\setminus U_{j}}\big||\omega_{j}|-|\omega_{j}|(x)\big|
≤C⁡(n,R)​ϵj​(R)+C⁡(n,R)⋅Vol⁡(BR​(xj)∖Uj)Vol⁡(BR​(xj))→0.\displaystyle\leq C(n,R)\epsilon_{j}(R)+C(n,R)\cdot\frac{{\rm Vol}(B_{R}(x_{j})\setminus U_{j})}{{\rm Vol}(B_{R}(x_{j}))}\to 0\,. (3.69)

Hence, we have

⨏BR​(xj)||ωj|2−⨏BR​(xj)|ωj|2|≤|⨏BR​(xj)|ωj|2−|ωj|2​(x)|+⨏BR​(xj)||ωj|2−|ωj|2​(x)|→0,\displaystyle\fint_{B_{R}(x_{j})}\Big|\,|\omega_{j}|^{2}-\fint_{B_{R}(x_{j})}|\omega_{j}|^{2}\Big|\leq\Big|\fint_{B_{R}(x_{j})}|\omega_{j}|^{2}-|\omega_{j}|^{2}(x)\Big|+\fint_{B_{R}(x_{j})}\Big||\omega_{j}|^{2}-|\omega_{j}|^{2}(x)\Big|\to 0\,, (3.70)

which proves the claim. □\square

We know from (3.43), (3.48) that |∇ωj||\nabla\omega_{j}| has L2L^{2} bounds. It is crucial to improve these to bounds that are small compared to ϵ\epsilon. This is the content of the next claim:

Claim 4: For fixed RR we have

⨏BR​(xj)|∇ωj|2≤ϵj​(R)→0.\fint_{B_{R}(x_{j})}|\nabla\omega_{j}|^{2}\leq\epsilon_{j}(R)\to 0\,. (3.71)

To see this fix RR and as in [ChCo1], let φ:B2​R​(xj)→ℝ+\varphi:B_{2R}(x_{j})\to\mathds{R}^{+} be a cutoff function with φ≡1\varphi\equiv 1 on BR​(xj)B_{R}(x_{j}) and R​|∇φ|,R2​|Δ​φ|≤C⁡(n)R|\nabla\varphi|,\,R^{2}|\Delta\varphi|\leq C(n). We use the Bochner formula

Δ​|ωj|2\displaystyle\Delta|\omega_{j}|^{2} =2|∇ωj|2+2⟨∑bdvj1∧⋯Ric(dvjb)∧⋯∧dvjk,ω⟩\displaystyle=2|\nabla\omega_{j}|^{2}+2\langle\sum_{b}dv^{1}_{j}\wedge\cdots{\rm Ric}(dv^{b}_{j})\wedge\cdots\wedge dv^{k}_{j},\omega\rangle
+⟨∑a≠bd​vj1∧∇c(d​vja)∧⋯∧∇c(d​vjb)∧⋯∧d​vjk,ωj⟩\displaystyle\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,+\langle\sum_{a\neq b}dv^{1}_{j}\wedge\nabla^{c}(dv^{a}_{j})\wedge\cdots\wedge\nabla_{c}(dv^{b}_{j})\wedge\cdots\wedge dv^{k}_{j},\omega_{j}\rangle
≥2​|∇ωj|2−C⁡(n)​δj2​rj2​|ωj|2−C⁡(n)​|∇(d​v)|2​|ωj|2\displaystyle\geq 2|\nabla\omega_{j}|^{2}-C(n)\delta_{j}^{2}r_{j}^{2}|\omega_{j}|^{2}-C(n)|\nabla(dv)|^{2}|\omega_{j}|^{2}
+⟨∑a≠bd​vj1∧∇c(d​vja)∧⋯∧∇c(d​vjb)∧⋯∧d​vjk,ωj⟩,\displaystyle\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,+\langle\sum_{a\neq b}dv^{1}_{j}\wedge\nabla^{c}(dv^{a}_{j})\wedge\cdots\wedge\nabla_{c}(dv^{b}_{j})\wedge\cdots\wedge dv^{k}_{j},\omega_{j}\rangle\,, (3.72)

which together with the growth estimates (3.43) allows us to compute

⨏BR​(xj)|∇ωj|2\displaystyle\fint_{B_{R}(x_{j})}|\nabla\omega_{j}|^{2} ≤C⁡(n)​⨏B2​R​(xj)φ​Δ​|ωj|2+C⁡(n,R)​∑a≠b⨏B2​R​(xj)|∇2vja|​|∇2vb|+C⁡(n,R)​δj2​rj2\displaystyle\leq C(n)\fint_{B_{2R}(x_{j})}\varphi\Delta|\omega_{j}|^{2}+C(n,R)\sum_{a\neq b}\fint_{B_{2R}(x_{j})}|\nabla^{2}v^{a}_{j}|\,|\nabla^{2}v^{b}|+C(n,R)\delta_{j}^{2}r_{j}^{2}
≤C​⨏B2​R​(xj)Δ​φ​(|ωj|2−⨏B2​R​(xj)|ωj|2)\displaystyle\leq C\fint_{B_{2R}(x_{j})}\Delta\varphi\,\big(|\omega_{j}|^{2}-\fint_{B_{2R}(x_{j})}|\omega_{j}|^{2}\big)
+C(n,R)∑a≠b(⨏B2​R​(xj)|∇2va|2)1/2(⨏B2​R​(xj)|∇2vb|2)1/2+ϵj(R)\displaystyle\,\,\,\,\,\,+C(n,R)\sum_{a\neq b}\Big(\fint_{B_{2R}(x_{j})}|\nabla^{2}v^{a}|^{2}\Big)^{1/2}\Big(\fint_{B_{2R}(x_{j})}|\nabla^{2}v^{b}|^{2}\Big)^{1/2}+\epsilon_{j}(R)
≤C​⨏B2​R​(xj)||ωj|2−⨏B2​R​(x)|ωj|2|+ϵj​(R)≤ϵj​(R)→0,\displaystyle\leq C\fint_{B_{2R}(x_{j})}\big||\omega_{j}|^{2}-\fint_{B_{2R}(x)}|\omega_{j}|^{2}\big|+\epsilon_{j}(R)\leq\epsilon_{j}(R)\to 0\,, (3.73)

where we have used Claim 3 and (3.46). Note that it is important that we have a≠ba\neq b in the summation, so that at least one of the Hessian terms in each factor is going to zero as j→∞j\to\infty. This proves the claim.∎

As mentioned in Remark 3.2, to complete the proof we must show that ⨏BR​(xj)|∇2vjk|2→0\fint_{B_{R}(x_{j})}|\nabla^{2}v^{k}_{j}|^{2}\to 0 as j→∞j\to\infty. To prove this we will first pass to limits and obtain information on the limiting space. That is, we have been considering a sequence (Mjn,dj,xj)(M^{n}_{j},d_{j},x_{j}) with RicMjn≥−δj2​rj2→0{\rm Ric}_{M^{n}_{j}}\geq-\delta_{j}^{2}r_{j}^{2}\to 0. After passing to a subsequence if necessary, we can take a measured pointed Gromov-Hausdorff limit

(Mjn,dj′,xj)⟶dG​H(X,d,x),\displaystyle(M^{n}_{j},d^{\prime}_{j},x_{j})\stackrel{{\scriptstyle d_{GH}}}{{\longrightarrow}}(X,d,x)\,, (3.74)

to obtain an R​C​D​(n,0)RCD(n,0) space XX, see [AGS12], [AGS12-2]. The fact that XX is an R​C​D​(n,0)RCD(n,0) space is used below in applying the mean value estimate (3.84), which is known to hold for such spaces.

In addition, we can assume that the functions vjℓv_{j}^{\ell} converge to harmonic functions.

vjℓ→vℓ:X→ℝ.\displaystyle v_{j}^{\ell}\to v^{\ell}:X\to\mathds{R}\,. (3.75)

Indeed, for any ball BR​(xj)B_{R}(x_{j}) we can characterize vjℓv^{\ell}_{j} as minimizers of the Dirichlet energy with fixed Dirichlet boundary values. Our assertion then follows from the lower semicontinuity of the Dirichlet energy [AGS12-2] combined with the Mosco convergence of the Dirichlet form [GMS14], to see that the limit also minimizes the Dirichlet energy on any ball.

Observe first, that by using Claim 2 and Lemma 1.7, we have

X=ℝk−1×Y,\displaystyle X=\mathds{R}^{k-1}\times Y\,, (3.76)

where v1,…,vk−1:X→ℝv^{1},\ldots,v^{k-1}:X\to\mathds{R} are linear functions which induce the ℝk−1\mathds{R}^{k-1} factor and we can identify Y=(v1,…,vk−1)−1​(0k−1)Y=(v^{1},\ldots,v^{k-1})^{-1}(0^{k-1}). We are left with understanding the behavior of vkv^{k}. We will seein Claim 6 that it too is linear, and in the process prove our Hessian estimate. We first show the following:

Claim 5: There exists a1,…,ak−1∈ℝa_{1},\ldots,a_{k-1}\in\mathds{R} with |aℓ|<C⁡(n)​ϵ|a_{\ell}|<C(n)\epsilon such that vk−a1​v1−⋯−ak−1​vk−1:X→ℝv^{k}-a_{1}v^{1}-\cdots-a_{k-1}v^{k-1}:X\to\mathds{R} is a function of only the YY variable.

To prove the claim let us fix any vector V∈ℝk−1V\in\mathds{R}^{k-1} and consider the map D​vk:X→ℝDv^{k}:X\to\mathds{R} defined by

D​vk​(y)=vk​(y+V)−vk​(y),\displaystyle Dv^{k}(y)=v^{k}(y+V)-v^{k}(y)\,, (3.77)

where of course, the translation x→x+Vx\to x+V is well defined, since X≡ℝk−1×YX\equiv\mathds{R}^{k-1}\times Y. The function vk​(y)v^{k}(y) is harmonic, and the translation map x→x+Vx\to x+V is a measure preserving isometry. Thus, vk​(x+V)v^{k}(x+V) is a harmonic function as well. Since XX is an R​C​DRCD space, and hence the Laplacian Δ\Delta on XX is linear, it follows that D​vkDv^{k} is harmonic. Using the estimates (3.43) we have the growth condition

supBr​(x)|D​vk|≤C​|V|1+C​ϵ⋅rC​ϵ.\displaystyle\sup_{B_{r}(x)}|Dv^{k}|\leq C|V|^{1+C\epsilon}\cdot r^{C\epsilon}\,. (3.78)

This is to say that D​vkDv^{k} is a harmonic function with sublinear growth. It follows that D​vkDv^{k} must be a constant. Indeed, let φ\varphi be a cutoff on B2​RB_{2R} with φ≡1\varphi\equiv 1 on BR​(x)B_{R}(x) and |∇φ|≤10​R−1|\nabla\varphi|\leq 10R^{-1}. Then on the one hand, we have since D​vkDv^{k} is harmonic and the Dirichlet form is bilinear that

0\displaystyle 0 =⨏B2​R​(x)⟨∇Dvk,∇(φ2Dvk)⟩\displaystyle=\fint_{B_{2R}(x)}\langle\nabla Dv^{k},\nabla(\varphi^{2}Dv^{k})\rangle (3.79)
=⨏B2​R​(x)φ2|∇Dvk|2+2⨏B2​R​(x)φDvk⟨∇Dvk,∇φ⟩.\displaystyle=\fint_{B_{2R}(x)}\varphi^{2}|\nabla Dv^{k}|^{2}+2\fint_{B_{2R}(x)}\varphi\,Dv^{k}\,\langle\nabla Dv^{k},\nabla\varphi\rangle\,. (3.80)

By rearranging terms, we obtain

⨏BR​(x)|∇Dvk|2\displaystyle\fint_{B_{R}(x)}|\nabla Dv^{k}|^{2} ≤⨏B2​R​(x)φ2|∇Dvk|2\displaystyle\leq\fint_{B_{2R}(x)}\varphi^{2}|\nabla Dv^{k}|^{2} (3.81)
≤12⨏B2​R​(x)φ2|∇Dvk|2+8⨏B2​R​(x)|Dvk|2|∇φ|2\displaystyle\leq\frac{1}{2}\fint_{B_{2R}(x)}\varphi^{2}|\nabla Dv^{k}|^{2}+8\fint_{B_{2R}(x)}|Dv^{k}|^{2}|\nabla\varphi|^{2} (3.82)
≤C​R−2+C​ϵ.\displaystyle\leq CR^{-2+C\epsilon}\,. (3.83)

On the other hand, RicMjn≥−(n−1)​δj2​rj2→0{\rm Ric}_{M^{n}_{j}}\geq-(n-1)\delta^{2}_{j}r_{j}^{2}\to 0 and so XX is an R​C​D​(n,0)RCD(n,0) space. On such spaces, there is a mean value inequalilty for the norm squared of the gradient of a harmonic function; see for instance [MN14]. When applied to the harmonic function D​vkDv^{k} it gives for r>0r>0 fixed and R→∞R\to\infty

supBr​(x)|∇Dvk|2≤C⨏BR​(x)|∇Dvk|2≤CR−2+C​ϵ→0.\displaystyle\sup_{B_{r}(x)}|\nabla Dv^{k}|^{2}\leq C\fint_{B_{R}(x)}|\nabla Dv^{k}|^{2}\leq CR^{-2+C\epsilon}\to 0\,. (3.84)

Note that once again we have exploited the sublinearity of the growth estimates. In particular, it now follows that D​vkDv^{k} is a constant. Since this holds for any V∈ℝk−1V\in\mathds{R}^{k-1}, we have that vkv^{k} is linear in the ℝk−1\mathds{R}^{k-1} variable. More precisely, since the ℝk−1\mathds{R}^{k-1} factor is spanned by v1,…,vk−1v^{1},\ldots,v^{k-1} we have

vk=vYk+a1​v1+⋯+ak−1​vk−1,\displaystyle v^{k}=v^{k}_{Y}+a_{1}v^{1}+\cdots+a_{k-1}v^{k-1}\,, (3.85)

where vYk:Y→ℝv^{k}_{Y}:Y\to\mathds{R}. Since vj→v:X→ℝkv_{j}\to v:X\to\mathds{R}^{k} are C​ϵC\epsilon-splittings on B2​(xj)B_{2}(x_{j}), we automatically have the bounds |aℓ|≤C⁡(n)​ϵ|a_{\ell}|\leq C(n)\epsilon. This finishes the claim. □\square

To complete the proof, we want to see that the Hessians of vjkv^{k}_{j} are tending to zero as j→∞j\to\infty. This is the content of Claim 6 below. However, prior to stating this claim, we will make some additional normalizations.

To begin with, we can use Claim 5 to further normalize the mappings vjv_{j} by composing with another lower triangular matrix. Indeed, as a corollary of Claim 5 we may choose a lower triangular matrix AA with |A−I|<C⁡(n)​ϵ|A-I|<C(n)\epsilon, and whose restriction to the first (k−1)×(k−1)(k-1)\times(k-1) terms is the identity, such that A​vj:B2​(xj)→ℝkAv_{j}:B_{2}(x_{j})\to\mathds{R}^{k} is still an C⁡(n)​ϵC(n)\epsilon-splitting, while A∘vjk→A∘vk:ℝk−1×Y→ℝA\circ v^{k}_{j}\to A\circ v^{k}:\mathds{R}^{k-1}\times Y\to\mathds{R} is independent of the ℝk−1\mathds{R}^{k-1} factor. Further, let us consider the induced form A∘ωj=d⁡(A∘vj1)∧⋯∧d⁡(A∘vjk)=d​vj1∧⋯∧d⁡(A∘vjk)A\circ\omega_{j}=d(A\circ v_{j}^{1})\wedge\cdots\wedge d(A\circ v^{k}_{j})=dv_{j}^{1}\wedge\cdots\wedge d(A\circ v^{k}_{j}). Then after multiplying the kt​hk^{th} row of AA by a constant cc with |c−1|≤C⁡(n)​ϵ|c-1|\leq C(n)\epsilon we may further assume that

⨏B2​(xj)|A∘ωj|2=1.\displaystyle\fint_{B_{2}(x_{j})}|A\circ\omega_{j}|^{2}=1\,. (3.86)

From this point forward in the proof, for ease of notation, we will write vjv_{j} for what was denoted above by A∘vjA\circ v_{j} In particular, this vjv_{j} differs from the original mapping uju_{j} only by composition with a lower triangular matrix. We will eventually see that vj:B1​(xj)→ℝkv_{j}:B_{1}(x_{j})\to\mathds{R}^{k} is an ϵj\epsilon_{j}-splitting, which will give the desired contradiction and finish the proof.

Claim 6. For each R>0R>0, we have ⨏BR​(xj)|∇2vjk|2≤ϵj​(R)→0\fint_{B_{R}(x_{j})}|\nabla^{2}v^{k}_{j}|^{2}\leq\epsilon_{j}(R)\to 0.

The fact that vj:BR​(xj)→ℝk−1v_{j}:B_{R}(x_{j})\to\mathds{R}^{k-1} is an ϵj​(R)\epsilon_{j}(R)-splitting,

⨏B2​(xj)|ωj|2=1,\fint_{B_{2}(x_{j})}|\omega_{j}|^{2}=1\,,

together with

⨏BR​(xj)|∇ωj|2≤ϵj​(R)→0,\fint_{B_{R}(x_{j})}|\nabla\omega_{j}|^{2}\leq\epsilon_{j}(R)\to 0\,,

implies

⨏BR​(xj)||ωjℓ|−1|≤ϵj​(R)(for​all​  1≤ℓ≤k).\displaystyle\fint_{B_{R}(x_{j})}\big||\omega^{\ell}_{j}|-1\big|\leq\epsilon_{j}(R)\qquad({\rm for\,\,all}\,\,1\leq\ell\leq k)\,. (3.88)

Now we will show that

⨏BR​(xj)||∇vjk|2−1|≤ϵj​(R)→0.\displaystyle\fint_{B_{R}(x_{j})}\big||\nabla v^{k}_{j}|^{2}-1\big|\leq\epsilon_{j}(R)\to 0\,. (3.89)

Once this is accomplished, as we have done repeatedly, we can argue with Bochner’s formula to obtain the Hessian estimate in the claim.

Define the 11-form

Vj≡⟨ωjk−1,ωj⟩.\displaystyle V_{j}\equiv\langle\omega^{k-1}_{j},\omega_{j}\rangle\,. (3.90)

Note ωjk−1∧Vj\omega^{k-1}_{j}\wedge V_{j} is proportional to ωj=ωjk−1∧d​vjk=ωjk−1∧(d​vjk−πk−1​d​vjk)\omega_{j}=\omega^{k-1}_{j}\wedge dv^{k}_{j}=\omega^{k-1}_{j}\wedge\big(dv^{k}_{j}-\pi_{k-1}dv^{k}_{j}\big). More generally, we have that Vj∈span​{∇vj1,…,∇vjk}V_{j}\in\text{span}\{\nabla v^{1}_{j},\ldots,\nabla v^{k}_{j}\} is perpendicular to span​{∇vj1,…,∇vjk−1}\text{span}\{\nabla v^{1}_{j},\ldots,\nabla v^{k-1}_{j}\}. From the above, we get

⨏BR​(xj)|Vj−(d​vjk−πk−1​d​vjk)|≤ϵj​(R).\displaystyle\fint_{B_{R}(x_{j})}|V_{j}-\big(dv^{k}_{j}-\pi_{k-1}dv^{k}_{j}\big)|\leq\epsilon_{j}(R)\,. (3.91)

On the other hand, by (3.73) we have

⨏BR​(xj)|∇Vj|2≤ϵj​(R)→0,\displaystyle\fint_{B_{R}(x_{j})}|\nabla V_{j}|^{2}\leq\epsilon_{j}(R)\to 0\,, (3.92)

and thus using (3.88) we have

⨏BR​(xj)||Vj|−1|≤ϵj​(R).\displaystyle\fint_{B_{R}(x_{j})}\big||V_{j}|-1\big|\leq\epsilon_{j}(R)\,. (3.93)

Therefore, from (3.91) we get

⨏BR​(xj)||d​vjk−πk−1​d​vjk|−1|≤ϵj​(R)→0.\displaystyle\fint_{B_{R}(x_{j})}\Big||dv^{k}_{j}-\pi_{k-1}dv^{k}_{j}|-1\Big|\leq\epsilon_{j}(R)\to 0\,. (3.94)

It follows that our main concern is to show |πk−1​(d​vjk)|→0|\pi_{k-1}(dv^{k}_{j})|\to 0 as j→∞j\to\infty.

For R>0R>0, we can use the segment inequality of [ChCo1] along with (3.54) to find a subset UR⊆BR​(xj)U_{R}\subseteq B_{R}(x_{j}) with

Vol⁡(BR​(xj)∖UR)≤ϵj​(R)→0,\displaystyle{\rm Vol}(B_{R}(x_{j})\setminus U_{R})\leq\epsilon_{j}(R)\to 0\,, (3.95)

such that for each x∈URx\in U_{R} there exists a subset UR​(x)⊆B2​R​(xj)U_{R}(x)\subseteq B_{2R}(x_{j}) with

Vol⁡(BR​(xj)∖UR​(x))≤ϵj​(R)→0,\displaystyle{\rm Vol}(B_{R}(x_{j})\setminus U_{R}(x))\leq\epsilon_{j}(R)\to 0\,, (3.96)

and such that if y∈UR​(x)y\in U_{R}(x) then there is a unique geodesic γ\gamma connecting xx and yy, and for 1≤ℓ≤k−11\leq\ell\leq k-1, we have the estimates

∫γ|∇2vjℓ|2≤ϵj​(R),\displaystyle\int_{\gamma}|\nabla^{2}v^{\ell}_{j}|^{2}\leq\epsilon_{j}(R)\,,
∫γ|∇2vjk|2≤C​ϵ.\displaystyle\int_{\gamma}|\nabla^{2}v^{k}_{j}|^{2}\leq C\epsilon\,. (3.97)

Now, for x∈URx\in U_{R} let us choose x1,…,xk−1∈UR​(x)x_{1},\ldots,x_{k-1}\in U_{R}(x) such that

|vjℓ(x)−vjℓ((xℓ)−1|<ϵj(R),\displaystyle|v^{\ell}_{j}(x)-v^{\ell}_{j}((x_{\ell})-1|<\epsilon_{j}(R)\,,
|vjk((x)−vjk((xℓ)|<ϵj(R),\displaystyle|v^{k}_{j}((x)-v^{k}_{j}((x_{\ell})|<\epsilon_{j}(R)\,,
||∇vjℓ|−1|​(xℓ)≤ϵj​(R).\displaystyle\big||\nabla v^{\ell}_{j}|-1\big|(x_{\ell})\leq\epsilon_{j}(R)\,. (3.98)

Note that the geodesic γℓ\gamma_{\ell} connecting xx and xℓx_{\ell} is contained in the approximate ℝk−1\mathds{R}^{k-1} factor from the splitting induced by vj1,…,vjk−1v^{1}_{j},\ldots,v^{k-1}_{j}. Thus, we get the pointwise estimate

|vjk((x)−vjk(γℓ(t))|<ϵj(R),\displaystyle|v^{k}_{j}((x)-v^{k}_{j}(\gamma_{\ell}(t))|<\epsilon_{j}(R)\,, (3.99)

along all of γℓ\gamma_{\ell}. In particular, for every interval I⊆γℓI\subseteq\gamma_{\ell}, we have

|∫I⟨∇vjk,γ˙ℓ⟩|<ϵj​(R).\displaystyle\big|\int_{I}\langle\nabla v^{k}_{j},\dot{\gamma}_{\ell}\rangle\big|<\epsilon_{j}(R)\,. (3.100)

Thus, it follows from the mean value theorem that for each interval II, there is a point tI∈It_{I}\in I such that

|⟨∇vjk​(γ⁡(tI)),γ˙​(tI)⟩|<ϵj​(R)|I|.\displaystyle|\langle\nabla v^{k}_{j}(\gamma(t_{I})),\dot{\gamma}(t_{I})\rangle|<\frac{\epsilon_{j}(R)}{|I|}\,. (3.101)

Now let us use (3.97) and the Schwarz inequality to get

∫γℓ|∇γ˙ℓ⟨∇vjk,γ˙ℓ⟩|<C​ϵ12​|I|12.\displaystyle\int_{\gamma_{\ell}}\big|\nabla_{\dot{\gamma}_{\ell}}\langle\nabla v^{k}_{j},\dot{\gamma}_{\ell}\rangle\big|<C\epsilon^{\frac{1}{2}}|I|^{\frac{1}{2}}\,. (3.102)

By combining this with (3.101), we get that for each interval II,

supI|⟨∇vjk,γ˙⟩|≤C⋅ϵj​(R)|I|12.\displaystyle\sup_{I}\,|\langle\nabla v^{k}_{j},\dot{\gamma}\rangle|\leq C\cdot\frac{\epsilon_{j}(R)}{|I|^{\frac{1}{2}}}\,. (3.103)

By covering γ\gamma with intervals whose size decreases to zero sufficiently slowly as j→∞j\to\infty, we get the pointwise estimate

supI|⟨∇vjk,γ˙⟩|≤ϵj​(R)→0,\displaystyle{\sup_{I}}\,|\langle\nabla v^{k}_{j},\dot{\gamma}\rangle|\leq\epsilon_{j}(R)\to 0\,, (3.104)

and in particular, at x=γ⁡(0)x=\gamma(0), we have

|⟨∇vjk,γ˙ℓ⟩|​(x)<ϵj​(R)→0.|\langle\nabla v^{k}_{j},\dot{\gamma}_{\ell}\rangle|(x)<\epsilon_{j}(R)\to 0\,.

For 1≤ℓ≤k−11\leq\ell\leq k-1, we can argue similarly with vjℓv^{\ell}_{j} in place of vjkv^{k}_{j}. Namely, by (3.97) and (3.98), we have

|∫γℓ(1−⟨∇vjℓ,γ˙ℓ⟩)|<ϵj​(R),\displaystyle\big|\int_{\gamma_{\ell}}\big(1-\langle\nabla v^{\ell}_{j},\dot{\gamma}_{\ell}\rangle\big)\,\big|<\epsilon_{j}(R)\,,
∫γℓ|∇γ˙ℓ⟨∇vjℓ,γ˙ℓ⟩|<ϵj​(R).\displaystyle\int_{\gamma_{\ell}}|\nabla_{\dot{\gamma}_{\ell}}\langle\nabla v^{\ell}_{j},\dot{\gamma}_{\ell}\rangle|<\epsilon_{j}(R)\,. (3.105)

Thus, we get

supγℓ|1−⟨∇vjℓ,γ˙ℓ⟩|​(γℓ)<ϵj​(R).\displaystyle\sup_{\gamma_{\ell}}|1-\langle\nabla v^{\ell}_{j},\dot{\gamma}_{\ell}\rangle|(\gamma_{\ell})<\epsilon_{j}(R)\,. (3.106)

At x=γℓ​(0)x=\gamma_{\ell}(0), this leads to

|γ˙ℓ−πk−1​γ˙ℓ|​(x)<ϵj​(R).\displaystyle|\dot{\gamma}_{\ell}-\pi_{k-1}\dot{\gamma}_{\ell}|(x)<\epsilon_{j}(R)\,. (3.107)

From this together with (3.104) we get

|πk−1​(∇vjk)|​(x)<ϵj​(R).\displaystyle|\pi_{k-1}(\nabla v^{k}_{j})|(x)<\epsilon_{j}(R)\,. (3.108)

Since |∇vjk|≤C⁡(R)|\nabla v^{k}_{j}|\leq C(R), we obtain from (3.95) that

⨏BR​(xj)|πk−1​(∇vjk)|\displaystyle\fint_{B_{R}(x_{j})}|\pi_{k-1}(\nabla v^{k}_{j})| =Vol​(BR​(xj))−1​∫UR|πk−1​(∇vjk)|+Vol​(BR​(xj))−1​∫BR∖UR|πk−1​(∇vjk)|\displaystyle={\rm Vol}(B_{R}(x_{j}))^{-1}\int_{U_{R}}|\pi_{k-1}(\nabla v^{k}_{j})|+{\rm Vol}(B_{R}(x_{j}))^{-1}\int_{B_{R}\setminus U_{R}}|\pi_{k-1}(\nabla v^{k}_{j})|
≤ϵj​(R)→0.\displaystyle\leq\epsilon_{j}(R)\to 0\,. (3.109)

By combining this with (3.94), we get the desired estimate

⨏BR​(xj)||∇vjk|2−1|≤ϵj​(R)→0.\displaystyle\fint_{B_{R}(x_{j})}\big||\nabla v^{k}_{j}|^{2}-1\big|\leq\epsilon_{j}(R)\to 0\,. (3.110)

Since vjkv^{k}_{j} is harmonic we can now argue with Bochner’s formula as in the proof of (3.5), to obtain the Hessian estimate, ⨏BR​(xj)|∇2vjk|2≤ϵj​(R)→0\fint_{B_{R}(x_{j})}|\nabla^{2}v^{k}_{j}|^{2}\leq\epsilon_{j}(R)\to 0. This completes the proof of the claim.□\square

Now we can finish the proof of the Transformation theorem. Indeed, we will see that vj=A∘u:B1​(xj)→ℝkv_{j}=A\circ u:B_{1}(x_{j})\to\mathds{R}^{k} is the desired ϵj​(R)\epsilon_{j}(R)-splitting. Claim 6 gives

⨏BR​(xj)|∇2vjℓ|2→0,\displaystyle\fint_{B_{R}(x_{j})}|\nabla^{2}v^{\ell}_{j}|^{2}\to 0\,, (3.111)

for all 1≤ℓ≤k1\leq\ell\leq k, while (3.109) and (3.110) imply

⨏BR​(xj)|⟨∇vja,∇vjb⟩−δa​b|→0.\displaystyle\fint_{B_{R}(x_{j})}|\langle\nabla v^{a}_{j},\nabla v^{b}_{j}\rangle-\delta^{ab}|\to 0\,. (3.112)

To see that vj:B1​(xj)→ℝkv_{j}:B_{1}(x_{j})\to\mathds{R}^{k} is an ϵj​(R)\epsilon_{j}(R)-splitting on B1​(xj)B_{1}(x_{j}), the last step is to show that |∇vjk|≤1+ϵj→1|\nabla v^{k}_{j}|\leq 1+\epsilon_{j}\to 1. However this follows immediately from (3.111) and (3.112) by using precisely the same argument as in (3.30)–(3.34).

Thus, for jj sufficiently large we see that vj:B1​(xj)→ℝkv_{j}:B_{1}(x_{j})\to\mathds{R}^{k} is an ϵ\epsilon-splitting. This is a contradiction, so the proof is complete.

∎

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