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A Generalization of the Geroch Conjecture with Arbitrary Ends

Shuli Chen [email protected]
Abstract.

Using μ\mu-bubbles, we prove that for 3n73\leq n\leq 7, the connected sum of a Schoen–Yau–Schick nn-manifold with an arbitrary manifold does not admit a complete metric of positive scalar curvature.

When either 3n53\leq n\leq 5, 1mn11\leq m\leq n-1 or 6n76\leq n\leq 7, m{1,n2,n1}m\in\{1,n-2,n-1\}, we also show the connected sum (Mnm×𝕋m)#Xn(M^{n-m}\times\mathbb{T}^{m})\#X^{n} where XX is an arbitrary manifold does not admit a metric of positive mm-intermediate curvature. Here mm-intermediate curvature is a new notion of curvature introduced by Brendle, Hirsch and Johne interpolating between Ricci and scalar curvature.

1. Introduction

The well-known Geroch conjecture asks whether the torus 𝕋n\mathbb{T}^{n} admits a metric of positive scalar curvature. A negative answer to this conjecture was given by Schoen and Yau for 3n73\leq n\leq 7 using minimal hypersurfaces via the inductive descent method [SY79b], and by Gromov and Lawson for all dimensions using spinors [GL83]. This result has had several important consequences, including Schoen-Yau’s proof of the positive mass theorem in general relativity [SY79a, Sch89, SY17] and Schoen’s resolution of the Yamabe problem [Sch84].

The Geroch conjecture has been generalized in various ways. For instance, Chodosh and Li [CL20] proved the Geroch conjecture with arbitrary ends for 3n73\leq n\leq 7 via the μ\mu-bubble technique; namely, they proved for any nn-manifold XX, the connected sum 𝕋n#X\mathbb{T}^{n}\#X does not admit a complete metric of positive scalar curvature. The case n=3n=3 was also obtained independently by Lesourd, Unger, and Yau [LUY20]. Recently, in the spin setting, Wang and Zhang [WZ22] showed that for arbitrary nn and any spin nn-manifold XX, the connected sum 𝕋n#X\mathbb{T}^{n}\#X admits no complete metric of positive scalar curvature. Using a similar argument, Chodosh and Li [CL20] further extended their result to manifolds of the form (Mn1×S1)#X(M^{n-1}\times S^{1})\#X, where 3n73\leq n\leq 7, MM is a Schoen–Yau–Schick manifold and XX is arbitrary. Here we recall the definition of a Schoen–Yau–Schick manifold:

Definition 1.1 (Schoen–Yau–Schick manifold, [SY79b, Sch98, SY17, Gro18]).

An orientable closed manifold MnM^{n} is called a Schoen–Yau–Schick manifold (abbreviated as SYS manifold), if there are nonzero cohomology classes β1,β2,,βn2\beta_{1},\beta_{2},\dots,\beta_{n-2} in H1(M;)H^{1}(M;\mathbb{Z}) such that the homology class [M](β1β2βn2)H2(M;)[M]\frown(\beta_{1}\smile\beta_{2}\smile\dots\smile\beta_{n-2})\in H_{2}(M;\mathbb{Z}) is non-spherical, that is, it does not lie in the image of the Hurewicz homomorphism π2(M)H2(M;)\pi_{2}(M)\to H_{2}(M;\mathbb{Z}).

In particular, the torus is an SYS manifold. SYS manifolds were first considered by Schoen and Yau in [SY79b], where they proved that SYS manifolds of dimension at most 7 do not admit metrics of positive scalar curvature via the inductive descent argument. Later, Schick [Sch98] constructed an SYS manifold as a counterexample to the unstable Gromov–Lawson–Rosenberg conjecture.

Theorem 1.2.

[CL20] Let 3n73\leq n\leq 7, and let Mn1M^{n-1} be a Schoen–Yau–Schick manifold. For any nn-manifold XX, the connected sum (Mn1×S1)#X(M^{n-1}\times S^{1})\#X does not admit a complete metric of positive scalar curvature.

The presence of the S1S^{1} factor in the preceding theorem is to pass to an appropriate covering space in order to apply the μ\mu-bubble technique introduced by Gromov in [Gro96]. In this paper, we show that we can pass to the infinite cyclic cover obtained by cutting and pasting along a hypersurface (see Theorem 3.4), thereby obtain a generalization of Chodosh and Li’s result as follows:

Theorem 1.3.

Let 3n73\leq n\leq 7, and let MnM^{n} be a Schoen–Yau–Schick manifold. For any nn-manifold XX, the connected sum M#XM\#X does not admit a complete metric of positive scalar curvature.

We note that a version of this result was obtained by Lesourd, Unger, and Yau [LUY20] for n=3n=3 and 4n74\leq n\leq 7 with certain additional technical hypothesis on M#XM\#X.

In another direction to generalize the Geroch conjecture, Brendle, Hirsch, and Johne [BHJ22] defined a family of curvature conditions called mm-intermediate curvature, which reduces to Ricci curvature when m=1m=1 and to scalar curvature when m=n1m=n-1. The precise definition is as follows:

Definition 1.4 (mm-intermediate curvature, [BHJ22]).

Suppose (Nn,g)(N^{n},g) is a Riemannian manifold. Let RmN(X,Y,Z,W)=g(XYZYXZ[X,Y]Z,W)\operatorname{Rm}_{N}(X,Y,Z,W)=-g(\nabla_{X}\nabla_{Y}Z-\nabla_{Y}\nabla_{X}Z-\nabla_{[X,Y]}Z,W) denote the Riemann curvature tensor. Let 1mn11\leq m\leq n-1. For every orthonormal basis {e1,,en}\{e_{1},\dots,e_{n}\} of TpNT_{p}N, we define

𝒞m(e1,,em):=p=1mq=p+1nRmN(ep,eq,ep,eq).\mathcal{C}_{m}(e_{1},\dots,e_{m}):=\sum_{p=1}^{m}\sum_{q=p+1}^{n}\operatorname{Rm}_{N}(e_{p},e_{q},e_{p},e_{q}).

Let

𝒞m(p):=min{𝒞m(e1,,em){e1,,en} is an orthonormal basis of TpN}.\mathcal{C}_{m}(p):=\min\{\mathcal{C}_{m}(e_{1},\dots,e_{m})\mid\{e_{1},\dots,e_{n}\}\text{ is an orthonormal basis of }T_{p}N\}.

Let CC\in\mathbb{R}. Then we say (Nn,g)(N^{n},g) has mm-intermediate curvature >C>C at pNp\in N, if 𝒞m(p)>C\mathcal{C}_{m}(p)>C. We say (Nn,g)(N^{n},g) has mm-intermediate curvature >C>C, if it has 𝒞m(p)>C\mathcal{C}_{m}(p)>C for all pNp\in N.

In particular, at any pNp\in N, sectional curvature sec>0\sec>0 implies 𝒞m(p)>0\mathcal{C}_{m}(p)>0, which in turn implies scalar curvature R>0R>0. On the other hand, Ric>0\operatorname{Ric}>0 at pp doesn’t necessarily imply 𝒞m(p)>0\mathcal{C}_{m}(p)>0 for 2mn22\leq m\leq n-2.

Brendle, Hirsch, and Johne investigated topological obstructions to positive mm-intermediate curvature and proved the following result.

Theorem 1.5.

[BHJ22, Theorem 1.5] Let 3n73\leq n\leq 7 and 1mn11\leq m\leq n-1. Let NnN^{n} be a closed manifold of dimension nn, and suppose that there exists a closed manifold MnmM^{n-m} and a map F:NnMnm×𝕋mF:N^{n}\to M^{n-m}\times\mathbb{T}^{m} with non-zero degree. Then the manifold NnN^{n} does not admit a metric of positive mm-intermediate curvature.

There are two reasons for the presence of the dimensional constraint n7n\leq 7 in Brendle–Hirsch–Johne’s result. The first reason comes from the regularity theory of stable minimal hypersurfaces in geometric measure theory. The second reason is that their proof requires some algebraic quantity, m2mn+2n2m^{2}-mn+2n-2, to be nonnegative. Kai Xu [Xu23] demonstrated the optimality of the dimensional constraint n7n\leq 7 by constructing concrete counterexamples. Namely, if m2mn+2n2<0m^{2}-mn+2n-2<0, then Snm×𝕋mS^{n-m}\times\mathbb{T}^{m} admits a metric of positive mm-intermediate curvature.

Chu–Kwong–Lee [CKL22] proved a corresponding rigidity statement for non-negative mm-intermediate curvature when n5n\leq 5, which was extended to n=6n=6 by Xu [Xu23]. Again, the dimensional constraint n6n\leq 6 was shown by Xu to be optimal.

In this paper, we also apply the μ\mu-bubble technique to obtain the following generalization of Brendle–Hirsch–Johne’s result to arbitrary ends:

Theorem 1.6.

Assume either 3n53\leq n\leq 5, 1mn11\leq m\leq n-1 or 6n76\leq n\leq 7, m{1,n2,n1}m\in\{1,n-2,n-1\}. Let NnN^{n} be a closed manifold of dimension nn, and suppose that there exists a closed manifold MnmM^{n-m} and a map F:NnMnm×𝕋mF:N^{n}\to M^{n-m}\times\mathbb{T}^{m} with non-zero degree. Then for any nn-manifold XX, the connected sum N#XN\#X does not admit a complete metric of positive mm-intermediate curvature.

For example, this implies that a punctured manifold of the form (Mnm×𝕋m){point}(M^{n-m}\times\mathbb{T}^{m})\setminus\{\text{point}\} does not admit a complete metric of positive mm-intermediate curvature when nn and mm are in the given range. Notice that we have a gap here; this is because in our proof, we need some extra algebraic quantity involving mm and nn to be positive (see Lemma 5.11 and Remark 5.12). It is an interesting question whether the same result still holds when 6n76\leq n\leq 7 and 2mn32\leq m\leq n-3.

This paper is organized as follows. In Section 2, we give some topological preliminaries. In Section 3, we discuss μ\mu-bubbles and prove a key result, Theorem 3.4, which allows us to reduce the non-compact setting to a compact setting. Using this, we give the proof of Theorem  1.3 in Section 4 and the proof of Theorem 1.6 in Section 5.

Acknowledgments.

The author is grateful for many useful discussions and suggestions of Otis Chodosh. The author is also grateful for helpful conversations with Sven Hirsch on the work [BHJ22]. The author also wants to thank the reviewers for their careful reading of the manuscript and their constructive remarks. The author is partially sponsored by the Ric Weiland Graduate Fellowship at Stanford University.

2. Topological Preliminaries

In this section we collect some basic topological facts for later use.

Lemma 2.1.

Let MnM^{n} be a closed connected orientable smooth manifold and let 0αHn1(M;)0\neq\alpha\in H_{n-1}(M;\mathbb{Z}) be a nonzero homology class. Then α\alpha is represented by a closed embedded orientable hypersurface Σ\Sigma.

Proof.

Notice the space S1S^{1} is a K(,1)K(\mathbb{Z},1), so H1(M;)=[M,S1]H^{1}(M;\mathbb{Z})=[M,S^{1}], where [M,S1][M,S^{1}] are homotopy classes of maps from MM to S1S^{1}. Thus we can choose a non-constant smooth map f:MS1f:M\to S^{1} representing the Poincaré dual of α\alpha in H1(M;)H^{1}(M;\mathbb{Z}). By Sard’s theorem we can take the preimage Σ\Sigma of a regular value as a representative of α\alpha. Then Σ\Sigma is a closed embedded orientable hypersurface by the regular value theorem.

\blacksquare

Lemma 2.2.

Let MnM^{n} be a closed connected orientable manifold and let Σn1M\Sigma^{n-1}\subset M be an orientable closed embedded connected hypersurface. Then Σ\Sigma is separating (i.e., MΣM\setminus\Sigma is the disjoint union of 2 connected open sets in MM) if and only if [Σ]=0[\Sigma]=0 in Hn1(M;)H_{n-1}(M;\mathbb{Z}).

Proof.

Suppose Σ\Sigma is non-separating, then MΣM\setminus\Sigma is connected, so there exists a simple loop SS in MM which crosses Σ\Sigma transversally in exactly one point. Orient SS so that this intersection is positive. Then the oriented intersection number I([Σ],[S])I([\Sigma],[S]) equals 11. Since the oriented intersection number is independent of the representative of the homology class, it follows that Σ\Sigma is homologically nontrivial.

Conversely, suppose that Σ\Sigma separates. Let UU be a tubular neighborhood of Σ\Sigma, and let V=MΣ=M+MV=M\setminus\Sigma=M_{+}\cup M_{-}. Then V=M+M=Σ+Σ\partial V=\partial M_{+}\cup\partial M_{-}=\Sigma_{+}\cup\Sigma_{-}, where Σ+\Sigma_{+} has the same orientation as Σ\Sigma while Σ\Sigma_{-} has the opposite orientation.

Let i:ΣMi:\Sigma\to M, i1:UVUi_{1}:U\cap V\to U, i2:UVVi_{2}:U\cap V\to V, j1:UMj_{1}:U\to M, j2:VMj_{2}:V\to M be inclusion maps. Consider the Mayer-Vietoris sequence in singular homology with \mathbb{Z} coefficients:

Hn1(UV)((i1),(i2))Hn1(U)Hn1(V)(j1)(j2)Hn1(M)\displaystyle\dots\to H_{n-1}(U\cap V)\xrightarrow{((i_{1})_{*},(i_{2})_{*})}H_{n-1}(U)\oplus H_{n-1}(V)\xrightarrow{(j_{1})_{*}-(j_{2})_{*}}H_{n-1}(M)\to\dots

Since UVU\cap V is homotopy equivalent to a disjoint union Σ+Σ\Sigma_{+}\cup\Sigma_{-}, we have Hn1(UV)Hn1(Σ+)Hn1(Σ)H_{n-1}(U\cap V)\cong H_{n-1}(\Sigma_{+})\oplus H_{n-1}(\Sigma_{-}), and the map (i1):Hn1(UV)Hn1(U)(i_{1})_{*}:H_{n-1}(U\cap V)\to H_{n-1}(U) is given by Hn1(Σ+)Hn1(Σ)Hn1(Σ),(a[Σ+],b[Σ])(ab)[Σ]H_{n-1}(\Sigma_{+})\oplus H_{n-1}(\Sigma_{-})\to H_{n-1}(\Sigma),(a[\Sigma_{+}],b[\Sigma_{-}])\mapsto(a-b)[\Sigma]. Since Σ\Sigma is the boundary of M+M_{+}, Σ\Sigma is null-homologous in M+M_{+} hence also in VV, showing the map Hn1(Σ)Hn1(UV)Hn1(V)H_{n-1}(\Sigma)\xrightarrow{\cong}H_{n-1}(U\cap V)\to H_{n-1}(V) is the zero map. Thus the Mayer-Vietoris sequence becomes

Hn1(Σ+)Hn1(Σ)((i1),0)Hn1(Σ)Hn1(V)i(j2)Hn1(M)\displaystyle\dots\to H_{n-1}(\Sigma_{+})\oplus H_{n-1}(\Sigma_{-})\xrightarrow{((i_{1})_{*},0)}H_{n-1}(\Sigma)\oplus H_{n-1}(V)\xrightarrow{i_{*}-(j_{2})_{*}}H_{n-1}(M)\to\dots

Exactness at Hn1(Σ)Hn1(V)H_{n-1}(\Sigma)\oplus H_{n-1}(V) shows that Hn1(Σ){0}=Im((i1),0)=Ker(i(j2))H_{n-1}(\Sigma)\oplus\{0\}=\operatorname{Im}\,((i_{1})_{*},0)=\operatorname{Ker}\,(i_{*}-(j_{2})_{*}), so Hn1(Σ)=KeriH_{n-1}(\Sigma)=\operatorname{Ker}i_{*}. That is, i:Hn1(Σ)Hn1(M)i_{*}:H_{n-1}(\Sigma)\to H_{n-1}(M) is the zero map, which means [Σ][\Sigma] is trivial in Hn1(M)H_{n-1}(M). \blacksquare

Construction 2.3 (dd-cyclic cover).

Let MM be a closed connected nn-manifold. Let Σ\Sigma be an embedded closed connected non-separating hypersurface in MM. Given any integer d1d\geq 1 or d=d=\infty, we can obtain a dd-cyclic cover M^\hat{M} by cutting and pasting along Σ\Sigma. The construction is as follows:

Cut MM along Σ\Sigma. Let M~=MΣ\tilde{M}=M\setminus\Sigma. Then M~\tilde{M} is a connected manifold with boundary, and M~\partial\tilde{M} has two components, both diffeomorphic to Σ\Sigma. Denote M~=ΣΣ+\partial\tilde{M}=\Sigma_{-}\cup\Sigma_{+}. Let G=/dG=\mathbb{Z}/d\mathbb{Z} when dd is finite and G=G=\mathbb{Z} when d=d=\infty. Let M~k\tilde{M}_{k}, kGk\in G be dd copies of M~\tilde{M}. Glue together M~k\tilde{M}_{k} along the boundary by gluing the Σ+\Sigma_{+} boundary component of M~k\tilde{M}_{k} with the Σ\Sigma_{-} boundary component of M~k+1\tilde{M}_{k+1}. Denote the resulting manifolds by

M^=kGM~k/,\hat{M}=\cup_{k\in G}\tilde{M}_{k}/\sim,

where the equivalence relation \sim is the gluing we just described. Then M^\hat{M} is a dd-cyclic cover of MM.

3. μ\mu-bubbles

In this section we first collect some general existence and stability results for μ\mu-bubbles. We refer the reader to [CL20] for more details, where they considered more generally the warped μ\mu-bubbles. For us, we do not need the warping and we simply take the warping function u=1u=1. We then use μ\mu-bubbles to prove a key result, Theorem 3.4, which is going to be applied in the proofs of both Theorem 1.3 and Theorem 1.6.

We begin by fixing some notations. For a Riemannian manifold (Mn,g¯)(M^{n},\overline{g}) we consider its Levi-Civita connection DD and its Riemann curvature tensor RmM\operatorname{Rm}_{M} given by the formula

RmM(X,Y,Z,W)=g¯(DXDYZDYDXZD[X,Y]Z,W)\operatorname{Rm}_{M}(X,Y,Z,W)=-\overline{g}(D_{X}D_{Y}Z-D_{Y}D_{X}Z-D_{[X,Y]}Z,W)

for vector fields X,Y,Z,WΓ(TM)X,Y,Z,W\in\Gamma(TM).

Consider a two-sided embedded submanifold (Σn1,g)(\Sigma^{n-1},g) with induced metric. We denote its induced Levi-Civita connection by DΣD_{\Sigma} and its unit normal vector field by νΓ(NΣ)\nu\in\Gamma(N\Sigma). We define its scalar-valued second fundamental form IIΣ{\rm II}_{\Sigma} by IIΣ(X,Y):=DXν,Y{\rm II}_{\Sigma}(X,Y):=\langle D_{X}\nu,Y\rangle. We define the scalar mean curvature of Σ\Sigma by HΣ=trgIIΣH_{\Sigma}=\operatorname{tr}_{g}{\rm II}_{\Sigma}. The gradient of a smooth function on MM or Σ\Sigma is denoted by DMfD_{M}f or DΣfD_{\Sigma}f.

For n7n\leq 7, consider (M,g¯)(M,\overline{g}), a Riemannian nn-manifold with boundary, and assume that M=M+M\partial M=\partial_{-}M\cup\partial_{+}M is a choice of labeling the components of M\partial M so that neither of the sets ±M\partial_{\pm}M are empty. Fix a smooth function hh on M̊\mathring{M} with h±h\to\pm\infty on ±M\partial_{\pm}M. Choose a Caccioppoli set Ω0\Omega_{0} with smooth boundary Ω0M̊\partial\Omega_{0}\subset\mathring{M} and +MΩ0\partial_{+}M\subset\Omega_{0}.

Consider the following functional

(1) 𝒜(Ω)=n1(Ω)M(χΩχΩ0)h𝑑n,\mathcal{A}(\Omega)=\mathcal{H}^{n-1}(\partial^{*}\Omega)-\int_{M}(\chi_{\Omega}-\chi_{\Omega_{0}})h\,d\mathcal{H}^{n},

for all Caccioppoli sets Ω\Omega in MM with ΩΔΩ0M̊\Omega\Delta\Omega_{0}\Subset\mathring{M}. We will call a Caccioppoli set Ω\Omega minimizing 𝒜\mathcal{A} in this class a μ\mu-bubble.

The functional 𝒜\mathcal{A} was first considered by Gromov in [Gro96]. The existence and regularity of a minimizer of 𝒜\mathcal{A} among all Caccioppoli sets was claimed by Gromov in [Gro19, Section 5.2], and was rigorously carried out in [Zhu21, Proposition 2.1] and also in [CL20, Proposition 12]. We thus record it here.

Proposition 3.1 ([Zhu21, Proposition 2.1][CL20, Proposition 12]).

There exists a smooth minimizer Ω\Omega for 𝒜\mathcal{A} such that ΩΔΩ0\Omega\Delta\Omega_{0} is compactly contained in the interior of M1M_{1}.

We next discuss the first and second variation for a μ\mu-bubble.

Lemma 3.2 ([CL20, Lemma 13]).

If Ωt\Omega_{t} is a smooth 11-parameter family of regions with Ω0=Ω\Omega_{0}=\Omega and normal speed ψ\psi at t=0t=0, then

ddt𝒜(Ωt)=Σt(Hh)ψ𝑑n1\frac{d}{dt}\mathcal{A}(\Omega_{t})=\int_{\Sigma_{t}}(H-h)\psi\,d\mathcal{H}^{n-1}

where HH is the scalar mean curvature of Ωt\partial\Omega_{t}. In particular, a μ\mu-bubble Ω\Omega satisfies

H=hH=h

along Ω\partial\Omega.

Lemma 3.3.

Consider a μ\mu-bubble Ω\Omega with Ω=Σ\partial\Omega=\Sigma. Assume that Ωt\Omega_{t} is a smooth 11-parameter family of regions with Ω0=Ω\Omega_{0}=\Omega and normal speed ψ\psi at t=0t=0, then 𝒬(ψ):=d2dt2|t=0(𝒜(Ωt))0\mathcal{Q}(\psi):=\frac{d^{2}}{dt^{2}}\big{|}_{t=0}(\mathcal{A}(\Omega_{t}))\geq 0 where 𝒬(ψ)\mathcal{Q}(\psi) satisfies

𝒬(ψ)=Σ(|DΣψ|2(|IIΣ|2+RicM(ν,ν)+DMh,ν)ψ2)𝑑n1,\displaystyle\mathcal{Q}(\psi)=\int_{\Sigma}\left(|D_{\Sigma}\psi|^{2}-\big{(}|{\rm II}_{\Sigma}|^{2}+\operatorname{Ric}_{M}(\nu,\nu)+\langle D_{M}h,\nu\rangle\big{)}\psi^{2}\right)d\mathcal{H}^{n-1},

where ν\nu is the outwards pointing unit normal.

Proof.

Let Σt:=Ωt\Sigma_{t}:=\partial\Omega_{t}. By the variation formulas for hypersurfaces (see e.g. [HP99, Theorem 3.2]), we have

tHΣt|t=0=ΔΣψ(|IIΣ|2+RicM(ν,ν))ψ,\frac{\partial}{\partial t}H_{\Sigma_{t}}\Big{|}_{t=0}=-\Delta_{\Sigma}\psi-\left(|{\rm II}_{\Sigma}|^{2}+\operatorname{Ric}_{M}(\nu,\nu)\right)\psi,

Differentiating the first variation and using HΣ=hH_{\Sigma}=h, we thus have

𝒬(ψ)\displaystyle\mathcal{Q}(\psi) =t|t=0Σt(Hh)ψ𝑑n1\displaystyle=\frac{\partial}{\partial t}\Big{|}_{t=0}\int_{\Sigma_{t}}(H-h)\psi\,d\mathcal{H}^{n-1}
=Σ0((ΔΣψ(|IIΣ|2+RicM(ν,ν))ψDMh,ψν)ψdn1\displaystyle=\int_{\Sigma_{0}}\left((-\Delta_{\Sigma}\psi-\left(|{\rm II}_{\Sigma}|^{2}+\operatorname{Ric}_{M}(\nu,\nu)\right)\psi-\langle D_{M}h,\psi\nu\rangle\right)\psi\,d\mathcal{H}^{n-1}
=Σ(|DΣψ|2(|IIΣ|2+RicM(ν,ν)+DΣh,ν)ψ2)𝑑n1.\displaystyle=\int_{\Sigma}\left(|D_{\Sigma}\psi|^{2}-\big{(}|{\rm II}_{\Sigma}|^{2}+\operatorname{Ric}_{M}(\nu,\nu)+\langle D_{\Sigma}h,\nu\rangle\big{)}\psi^{2}\right)d\mathcal{H}^{n-1}.

\blacksquare

Below we prove the key result, where we reduce the non-compact case to the compact case via μ\mu-bubbles.

Theorem 3.4.

Let 3n73\leq n\leq 7, and let 1mn11\leq m\leq n-1. Let MnM^{n} be a closed connected orientable manifold such that there exists a closed connected orientable non-separating hypersurface Σ\Sigma. Let XX be any nn-manifold, and consider the connected sum Y=M#XY=M\#X. Suppose YY admits a complete metric of positive mm-intermediate curvature.

Then for any number a>0a>0, there exists a closed connected orientable Riemannian manifold (Y~,g~)(\tilde{Y},\tilde{g}), a smooth function hC(Y)h\in C^{\infty}(Y), and a closed embedded orientable hypersurface Λn1Y~\Lambda^{n-1}\subset\tilde{Y} such that

  • Y~=M#iX~i\tilde{Y}=M^{\prime}\#_{i}\tilde{X}_{i}, where MM^{\prime} is a finite cyclic covering of MM obtained by cutting and pasting along Σ\Sigma and the X~i\tilde{X}_{i}’s are a finite number of closed manifolds.

  • In a neighborhood of Λ\Lambda, Y~\tilde{Y} has positive mm-intermediate curvature.

  • p[Λ]=[Σ]Hn1(M)p_{*}[\Lambda]=[\Sigma]\in H_{n-1}(M^{\prime}), where p:Y~Mp:\tilde{Y}\to M^{\prime} is the projection map and [Σ][\Sigma] is the homology class represented by any copy of Σ\Sigma in MM^{\prime}.

  • On Λ\Lambda, we have

    H=h,H=h,
    (𝒞m)Y~+ah22|DY~h|>0(\mathcal{C}_{m})_{\tilde{Y}}+ah^{2}-2|D_{\tilde{Y}}h|>0

    and

    𝒬(ψ)=Λ(|DΛψ|2(|IIΛ|2+RicY~(ν,ν)+DY~h,ν)ψ2)𝑑n10\mathcal{Q}(\psi)=\int_{\Lambda}\left(|D_{\Lambda}\psi|^{2}-\big{(}|{\rm II}_{\Lambda}|^{2}+\operatorname{Ric}_{\tilde{Y}}(\nu,\nu)+\langle D_{\tilde{Y}}h,\nu\rangle\big{)}\psi^{2}\right)d\mathcal{H}^{n-1}\geq 0

    for all ψC(Λ)\psi\in C^{\infty}(\Lambda).

Proof.

We follow the approach of [CL20, Section 6 and 7]. Namely, we pass to an appropriate covering space of YY, construct a weight function hh, and apply the μ\mu-bubble technique. The main difference in our case is how to find the covering space and how to modify the construction of the weight function hh. An illustration of the construction is in Figure 1.

Let Y=M#XY=M\#X be as in the assumption. By taking the orientation double cover of XX we can assume XX is orientable. Let pMp\in M be a point such that B(p)Σ=B(p)\cap\Sigma=\emptyset, where B(p)B(p) is a small nn-ball around pp. Let M=MB(p)M^{\prime}=M\setminus B(p) and X=XBX^{\prime}=X\setminus B, where BB is a small nn-ball in XX. Then we can take Y=M#X=MXY=M\#X=M^{\prime}\cup X^{\prime}, where MM^{\prime} and XX^{\prime} are glued on the boundary sphere.

Suppose YY is endowed with a complete metric of positive mm-intermediate curvature. By scaling and compactness of MM^{\prime} we can assume 𝒞m>1\mathcal{C}_{m}>1 on MM^{\prime}. Let a>0a>0 be any number.

Refer to caption
Figure 1. Illustration of the construction in the proof of Theorem 3.4. The manifold is Y^=M^#X\hat{Y}=\hat{M}\#_{\mathbb{Z}}X, the infinite cyclic cover of M#XM\#X constructed in Step 1. The shaded region is the bounded set {|h|<}\{|h|<\infty\} obtained in Step 2. The red hypersurface is Λ\Lambda obtained in Step 3.

Step 1: pass to an infinite cyclic cover by cutting and pasting MM along Σ\Sigma. Cut MM along Σ\Sigma. Let M~=MΣ\tilde{M}=M\setminus\Sigma and M~=MΣ=(MB(p))Σ\tilde{M}^{\prime}=M^{\prime}\setminus\Sigma=(M\setminus B(p))\setminus\Sigma. Then M~\tilde{M} is a connected manifold with boundary, and M~\partial\tilde{M} has two components, both diffeomorphic to Σ\Sigma. Denote M~=ΣΣ+\partial\tilde{M}=\Sigma_{-}\cup\Sigma_{+}. Let M~k\tilde{M}_{k}, kk\in\mathbb{Z} be \mathbb{Z} copies of M~\tilde{M}, and let M~k\tilde{M}^{\prime}_{k} be the corresponding M~M~\tilde{M}^{\prime}\subset\tilde{M}. Glue together M~k\tilde{M}_{k} along the boundary by gluing the Σ+\Sigma_{+} boundary component of M~k\tilde{M}_{k} with the Σ\Sigma_{-} boundary component of M~k+1\tilde{M}_{k+1}. Denote the resulting manifolds by

M^=kM~k/,\hat{M}=\cup_{k\in\mathbb{Z}}\tilde{M}_{k}/\sim,
M^=kM~k/,\hat{M}^{\prime}=\cup_{k\in\mathbb{Z}}\tilde{M}^{\prime}_{k}/\sim,

where the equivalence relation \sim is the gluing we just described. Then M^\hat{M} is an infinite cyclic covering of MM. Denote the closed hypersurface in M^\hat{M} coming from the Σ\Sigma_{-} boundary component of M~k\tilde{M}_{k} (equivalently, the Σ+\Sigma_{+} boundary component of M~k1\tilde{M}_{k-1}) by Σk\Sigma_{k}. Orient Σk\Sigma_{k} so that its normal is pointing towards M~k\tilde{M}_{k}.

Let XkX_{k}^{\prime}, kk\in\mathbb{Z} be \mathbb{Z} copies of XX^{\prime}. Then we have

Y^=M^#X=M^(kXk),\hat{Y}=\hat{M}\#_{\mathbb{Z}}X=\hat{M}^{\prime}\cup(\cup_{k\in\mathbb{Z}}X_{k}^{\prime}),

where M^\hat{M}^{\prime} and each XkX_{k}^{\prime} are glued on the boundary spheres. The manifold YY is an infinite cyclic cover of M#XM\#X.

We endow Y^\hat{Y} with the pullback Riemannian metric such that Y^Y\hat{Y}\to Y is a Riemannian covering map. Then by our assumption that 𝒞m>1\mathcal{C}_{m}>1 on MM^{\prime}, we also have 𝒞m>1\mathcal{C}_{m}>1 on M^\hat{M}^{\prime}.

Step 2: construct the weight function hh.

We now define ρ0:Y^\rho_{0}:\hat{Y}\to\mathbb{R} as the signed distance function to the hypersurface Σ0\Sigma_{0}. Then ρ0\rho_{0} is Lipschitz. We then take ρ1\rho_{1} to be a smoothing of ρ0\rho_{0} such that for each kk, ρ1Ak\rho_{1}\equiv A_{k} for some constant AkA_{k} in a small neighborhood of Xk\partial X_{k}^{\prime} (i.e., where M^\hat{M}^{\prime} and XkX_{k}^{\prime} are glued together), and Ak>0A_{k}>0 if k0k\geq 0 and Ak<0A_{k}<0 if k<0k<0. We can further assume that ρ1Ak\rho_{1}\geq A_{k} on XkX_{k}^{\prime} if k0k\geq 0 and ρ1Ak\rho_{1}\leq A_{k} on XkX_{k}^{\prime} if k<0k<0.

Then there is L>0L>0 so that

|Lip(ρ1)|g<a2L.|\operatorname{Lip}(\rho_{1})|_{g}<\frac{\sqrt{a}}{2}L.

We now define a function hC(Y^,[,])h\in C(\hat{Y},[-\infty,\infty]) as follows. On M^{πL2ρ1πL2}\hat{M}^{\prime}\cap\{-\tfrac{\pi L}{2}\leq\rho_{1}\leq\tfrac{\pi L}{2}\}, we define

h(p)=1atan(1Lρ1(p)).h(p)=-\frac{1}{\sqrt{a}}\tan(\tfrac{1}{L}\rho_{1}(p)).

On the rest of M^\hat{M}^{\prime} we set h=±h=\pm\infty such that it is continuous to [,][-\infty,\infty]. We then define hh on XkX_{k}^{\prime}. When AkπL2A_{k}\geq\tfrac{\pi L}{2}, set h=h=-\infty on XkX_{k}^{\prime}. When AkπL2A_{k}\leq-\tfrac{\pi L}{2}, set h=h=\infty on XkX_{k}^{\prime}. Now assume |Ak|πL2|A_{k}|\leq\tfrac{\pi L}{2}.

For k0k\geq 0 and

xXk{ρ1<Ak+2Ltan(L1Ak)},x\in X_{k}^{\prime}\cap\left\{\rho_{1}<A_{k}+\frac{2L}{\tan(L^{-1}A_{k})}\right\},

or for k<0k<0 and

xXk{ρ1>Ak+2Ltan(L1Ak)},x\in X_{k}^{\prime}\cap\left\{\rho_{1}>A_{k}+\frac{2L}{\tan(L^{-1}A_{k})}\right\},

we set

h(x)=2La(ρ1(x)Ak2Ltan(L1Ak)).h(x)=\frac{2L}{\sqrt{a}(\rho_{1}(x)-A_{k}-\frac{2L}{\tan(L^{-1}A_{k})})}.

Otherwise we set h(p)=±h(p)=\pm\infty such that hh is continuous. Observe that by definition, hh is finite on only finitely many XkX_{k}^{\prime}.

Notice that for xXkx\in\partial X_{k}^{\prime}, we have that

h(x)=1atan(L1Ak)=1atan(L1ρ1(x)),h(x)=-\frac{1}{\sqrt{a}}\tan(L^{-1}A_{k})=-\frac{1}{\sqrt{a}}\tan(L^{-1}\rho_{1}(x)),

and thus hh is Lipschitz across Xk\partial X_{k}^{\prime}. If 0Ak<πL20\leq A_{k}<\tfrac{\pi L}{2}, xXkx\in X_{k}^{\prime} and

ρ1(x)Ak+2Ltan(L1Ak),\rho_{1}(x)\nearrow A_{k}+\frac{2L}{\tan(L^{-1}A_{k})},

we have that h(x)h(x)\to-\infty. Similarly, if πL2<Ak<0-\tfrac{\pi L}{2}<A_{k}<0, xXkx\in X_{k}^{\prime} and

ρ1(x)Ak+2Ltan(L1Ak),\rho_{1}(x)\searrow A_{k}+\frac{2L}{\tan(L^{-1}A_{k})},

we have that h(x)h(x)\to\infty. Thus hh is continuous on XkX_{k}^{\prime}.

Note that the set {|h|<}\{|h|<\infty\} is bounded. This is because this region is bounded in M^\hat{M}^{\prime}, only finitely many ends XkX_{k}^{\prime} are included in this set, and in each XkX_{k}^{\prime}, the region where {|h|<}\{|h|<\infty\} is bounded.

Similar to [CL20], we have

Lemma 3.5.

We can smooth hh slightly to find a function hC(Y^)h\in C^{\infty}(\hat{Y}) satisfying

(2) (𝒞m)Y^+ah22|DY^h|>0(\mathcal{C}_{m})_{\hat{Y}}+ah^{2}-2|D_{\hat{Y}}h|>0

on {|h|<}\{|h|<\infty\}.

Proof.

The function hh constructed above is smooth away from Xk\partial X_{k}^{\prime} (and Lipschitz there). Since each Xk\partial X_{k}^{\prime} is compact and only a finite number of them are contained in {|h|<}\{|h|<\infty\}, if we prove (2) for function hh considered above, then we can easily find a smooth function satisfying (2).

Recall |(ρ1)|<a2L|\nabla(\rho_{1})|<\frac{\sqrt{a}}{2}L. We first check (2) on M^\hat{M}^{\prime}. There, 𝒞m>1\mathcal{C}_{m}>1. As such, we have that

𝒞m+ah22|DY^h|>1+tan2(L1ρ1(p))cos2(L1ρ1(p))=0.\mathcal{C}_{m}+ah^{2}-2|D_{\hat{Y}}h|>1+\tan^{2}(L^{-1}\rho_{1}(p))-\cos^{-2}(L^{-1}\rho_{1}(p))=0.

On the other hand, on XkX_{k}^{\prime} (we assume that k0k\geq 0 as the k<0k<0 case is similar), we only know that 𝒞m>0\mathcal{C}_{m}>0. Nevertheless, we compute

𝒞m+ah22|DY^h|\displaystyle\mathcal{C}_{m}+ah^{2}-2|D_{\hat{Y}}h|
>\displaystyle>  0+4L2(ρ1(p)Ak2Ltan(L1Ak))2L2(ρ1(p)Ak2Ltan(L1Ak))2\displaystyle\,0+\frac{4L^{2}}{\left(\rho_{1}(p)-A_{k}-\frac{2L}{\tan(L^{-1}A_{k})}\right)^{2}}-\frac{L^{2}}{\left(\rho_{1}(p)-A_{k}-\frac{2L}{\tan(L^{-1}A_{k})}\right)^{2}}
>\displaystyle>  0.\displaystyle\,0.

This completes the proof. \blacksquare

Step 3: apply the μ\mu-bubble technique.

We consider μ\mu-bubbles with respect to the smooth function hh we have just defined. We fix

Ω0:=(k<0M~k)(k<0Xk).\Omega_{0}:=(\cup_{k<0}\tilde{M}^{\prime}_{k})\cup(\cup_{k<0}X_{k}^{\prime}).

We can minimize

𝒜(Ω)=n1(Ω)M(χΩχΩ0)h𝑑n\mathcal{A}(\Omega)=\mathcal{H}^{n-1}(\partial^{*}\Omega)-\int_{M}(\chi_{\Omega}-\chi_{\Omega_{0}})h\,d\mathcal{H}^{n}

among all Cacioppoli sets Ω\Omega such that ΩΔΩ0\Omega\Delta\Omega_{0} is compactly contained in {|h|<}\{|h|<\infty\} by Proposition 3.1. Denote by Ω\Omega the connected component of the minimizer containing {ρ1=πL2}\{\rho_{1}=-\frac{\pi L}{2}\}. Since n7n\leq 7, each component of Ω\partial\Omega is compact and regular. By the first variation formula from Lemma 3.2 and the stability inequality for 𝒜\mathcal{A} from Lemma 3.3, we see that Λ=Ω\Lambda=\partial\Omega satisfies H=hH=h and

(3) 𝒬(ψ)=Λ(|DΛψ|2(|IIΛ|2+RicY^(ν,ν)+DY^h,ν)ψ2)𝑑n10\mathcal{Q}(\psi)=\int_{\Lambda}\left(|D_{\Lambda}\psi|^{2}-\big{(}|{\rm II}_{\Lambda}|^{2}+\operatorname{Ric}_{\hat{Y}}(\nu,\nu)+\langle D_{\hat{Y}}h,\nu\rangle\big{)}\psi^{2}\right)d\mathcal{H}^{n-1}\geq 0

for all ψC(Λ)\psi\in C^{\infty}(\Lambda).

We can find a compact region YYY^{\prime}\subset Y with smooth boundary so that ΩY\partial\Omega\subset Y^{\prime}. Furthermore, we can arrange that YM^=ΣIΣI\partial Y^{\prime}\cap\hat{M}=\Sigma_{I}\cup\Sigma_{-I}, for some large II\in\mathbb{N}. Note that the other boundary components of YY^{\prime} thus lie completely in some XkX_{k}^{\prime}.

In particular, YM^\partial Y^{\prime}\setminus\hat{M} bounds some compact manifold with boundary. Cap these components off and then glue the hypersurfaces ΣI\Sigma_{I} and ΣI\Sigma_{-I} to each other. We thus obtain a manifold Y~\tilde{Y} diffeomorphic to M#iX~iM^{\prime}\#_{i}\tilde{X}_{i}, where MM^{\prime} is a 2I2I-cyclic covering of MM obtained by cutting and pasting along Σ\Sigma, and each X~i\tilde{X}_{i} is closed and we have finitely many of them. We also have a hypersurface Λn1Y~\Lambda^{n-1}\subset\tilde{Y} homologous to [Σn1×{}]Hn1(Y~)[\Sigma^{n-1}\times\{*\}]\in H_{n-1}(\tilde{Y}) that satisfies H=hH=h and (3). We can make hh to be a smooth function on Y~\tilde{Y} that agrees with our old hh in a neighborhood of Λ\Lambda, so that (2) is satisfied. We can also construct a metric on Y~\tilde{Y} such that it is isometric to the original metric on YY in a neighborhood of Λ\Lambda. Since YY has positive mm-intermediate curvature, this means Y~\tilde{Y} has positive mm-intermediate curvature in a neighborhood of Λ\Lambda. This also means that on Λ\Lambda, we have

HΛ=h,H_{\Lambda}=h,
(𝒞m)Y~+ah22|DY~h|>0,(\mathcal{C}_{m})_{\tilde{Y}}+ah^{2}-2|D_{\tilde{Y}}h|>0,

and

𝒬(ψ)=Λ(|DΛψ|2(|IIΛ|2+RicY~(ν,ν)+DY~h,ν)ψ2)𝑑n10\mathcal{Q}(\psi)=\int_{\Lambda}\left(|D_{\Lambda}\psi|^{2}-\big{(}|{\rm II}_{\Lambda}|^{2}+\operatorname{Ric}_{\tilde{Y}}(\nu,\nu)+\langle D_{\tilde{Y}}h,\nu\rangle\big{)}\psi^{2}\right)d\mathcal{H}^{n-1}\geq 0

for all ψC(Λ)\psi\in C^{\infty}(\Lambda). \blacksquare

4. Proof of Theorem 1.3

We begin this section by proving some simple facts about SYS manifolds. We first give an equivalent definition of an SYS manifold. This is the definition given in e.g. [Gro19] and [LUY20].

Lemma 4.1.

Let MnM^{n} be an orientable closed manifold. Then MM being an SYS manifold is equivalent to the following condition: There exists a smooth map F:M𝕋n2F:M\to\mathbb{T}^{n-2}, such that the homology class of the pullback of a regular value, [F1(t)]H2(M)[F^{-1}(t)]\in H_{2}(M), is non-spherical.

Proof.

Since the space S1S^{1} is a K(,1)K(\mathbb{Z},1), we have [M,S1]=H1(M;)[M,S^{1}]=H^{1}(M;\mathbb{Z}), and the bijection is given by f(f:H1(M)H1(S1))f\mapsto(f_{*}:H_{1}(M)\to H_{1}(S^{1})\cong\mathbb{Z}). Thus for any βH1(M;)\beta\in H^{1}(M;\mathbb{Z}) we can get a smooth map f:MS1f:M\to S^{1} and vice versa. Further, the preimage of any regular value of ff represents the Poincaré dual of β\beta. Thus given β1,βn2H1(M;)\beta_{1},\dots\beta_{n-2}\in H^{1}(M;\mathbb{Z}) we can get a smooth map F=(F1,,Fn2):M𝕋n2F=(F_{1},\dots,F_{n-2}):M\to\mathbb{T}^{n-2} and vice versa. Since the cup product is the Poincaré dual to intersection, we have

[M](β1β2βn2)=[F11(t1)Fn21(tn2)]=[F1(t)],[M]\frown(\beta_{1}\smile\beta_{2}\smile\dots\smile\beta_{n-2})=[F_{1}^{-1}(t_{1})\cap\dots\cap F_{n-2}^{-1}(t_{n-2})]=[F^{-1}(t)],

where t=(t1,,tn2)t=(t_{1},\dots,t_{n-2}) is any regular value of FF. Then the assertion follows.

\blacksquare

In [Gro18, Section 5], Gromov gave some examples of SYS manifolds. For example, we can directly verify that if a closed orientable nn-manifold admits a map to 𝕋n\mathbb{T}^{n} of non-zero degree, then it is SYS. Here we establish some simple ways to obtain new SYS manifolds from an old one.

Lemma 4.2 ([Gro18, Section 5, Example 3]).

Let MnM^{n} be an SYS manifold and let M^\hat{M} be a closed orientable nn-manifold such that there exists a map f:M^Mf:\hat{M}\to M of degree 1. Then M^\hat{M} is also an SYS manifold.

Proof.

Since MM is an SYS manifold, there are nonzero cohomology classes β1,,βn2\beta_{1},\dots,\beta_{n-2} in H1(M;)H^{1}(M;\mathbb{Z}) such that the homology class [M](β1βn2)H2(M;)[M]\frown(\beta_{1}\smile\dots\smile\beta_{n-2})\in H_{2}(M;\mathbb{Z}) is non-spherical.

Then we get pullbacks fβ1,,fβn2f^{*}\beta_{1},\dots,f^{*}\beta_{n-2} in H1(M^;)H^{1}(\hat{M};\mathbb{Z}). Claim the class fβ1fβn2H2(M^;)f^{*}\beta_{1}\smile\dots\smile f^{*}\beta_{n-2}\in H_{2}(\hat{M};\mathbb{Z}) is non-spherical. Suppose not. Then there exists a map ϕ:S2M^\phi:S^{2}\to\hat{M} such that

[M^](fβ1fβn2)=[ϕ(S2)].[\hat{M}]\frown(f^{*}\beta_{1}\smile\dots\smile f^{*}\beta_{n-2})=[\phi(S^{2})].

By naturality of the cup product and the cap product, and using the fact that ff is of degree 1, we have

[(fϕ)(S2)]\displaystyle[(f\phi)_{*}(S^{2})] =f[ϕ(S2)]\displaystyle=f_{*}[\phi(S^{2})]
=f([M^](fβ1fβn2))\displaystyle=f_{*}\Big{(}[\hat{M}]\frown(f^{*}\beta_{1}\smile\dots\smile f^{*}\beta_{n-2})\Big{)}
=f([M^]f(β1βn2))\displaystyle=f_{*}\Big{(}[\hat{M}]\frown f^{*}(\beta_{1}\smile\dots\smile\beta_{n-2})\Big{)}
=f[M^](β1βn2)\displaystyle=f_{*}[\hat{M}]\frown(\beta_{1}\smile\dots\smile\beta_{n-2})
=[M](β1βn2),\displaystyle=[M]\frown(\beta_{1}\smile\dots\smile\beta_{n-2}),

which means the class [M](β1βn2)[M]\frown(\beta_{1}\smile\dots\smile\beta_{n-2}) is spherical, contradicting our assumptions. This contradiction shows that [M^](fβ1fβn2)H2(M^;)[\hat{M}]\frown(f^{*}\beta_{1}\smile\dots\smile f^{*}\beta_{n-2})\in H_{2}(\hat{M};\mathbb{Z}) is also non-spherical. Thus M^\hat{M} is an SYS manifold as desired. \blacksquare

Unlike the case in the previous lemma, if a closed orientable manifold XX admits a map ff of degree d>1d>1 to an SYS manifold, then XX is not necessarily SYS [Gro18, Section 5, Example 3]. What we have instead is the following.

Lemma 4.3.

Suppose MnM^{n} is a connected SYS manifold with β1,β2,,βn2\beta_{1},\beta_{2},\dots,\beta_{n-2} in H1(M;)H^{1}(M;\mathbb{Z}) such that [M](β1β2βn2)H2(M;)[M]\frown(\beta_{1}\smile\beta_{2}\smile\dots\smile\beta_{n-2})\in H_{2}(M;\mathbb{Z}) is non-spherical and such that the Poincaré dual of β1\beta_{1} is represented by a closed connected embedded orientable hypersurface Σ\Sigma. Let M^\hat{M} be the dd-cyclic cover of MM obtained by cutting and pasting along Σ\Sigma. Then M^\hat{M} is also an SYS manifold.

Proof.

Notice that Σ\Sigma is homological nontrivial, hence non-separating. Let p:M^Mp:\hat{M}\to M be the covering map. Let Σ0\Sigma_{0} be one copy of Σ\Sigma in M^\hat{M}, which is also non-separating. Let β^1H1(M^;)\hat{\beta}_{1}\in H^{1}(\hat{M};\mathbb{Z}) be the Poincaré dual of Σ\Sigma. Using naturality of the cup product and the cap product and the assumptions [Σ0]=[M^]β^1[\Sigma_{0}]=[\hat{M}]\frown\hat{\beta}_{1}, [Σ]=[M]β1[\Sigma]=[M]\frown\beta_{1}, we have

p([M^](β^1pβ2pβn2))\displaystyle p_{*}\Big{(}[\hat{M}]\frown(\hat{\beta}_{1}\smile p^{*}\beta_{2}\smile\dots\smile p^{*}\beta_{n-2})\Big{)}
=p(([M^]β^1)p(β2βn2))\displaystyle=p_{*}\Big{(}([\hat{M}]\frown\hat{\beta}_{1})\frown p^{*}(\beta_{2}\smile\dots\smile\beta_{n-2})\Big{)}
=p([Σ0]p(β2βn2))\displaystyle=p_{*}\Big{(}[\Sigma_{0}]\frown p^{*}(\beta_{2}\smile\dots\smile\beta_{n-2})\Big{)}
=p[Σ0](β2βn2))\displaystyle=p_{*}[\Sigma_{0}]\smile(\beta_{2}\smile\dots\smile\beta_{n-2})\Big{)}
=[Σ](β2βn2)\displaystyle=[\Sigma]\frown(\beta_{2}\smile\dots\smile\beta_{n-2})
=([M]β1)(β2βn2)\displaystyle=([M]\frown\beta_{1})\frown(\beta_{2}\smile\dots\smile\beta_{n-2})
=[M](β1β2βn2).\displaystyle=[M]\frown(\beta_{1}\smile\beta_{2}\smile\dots\smile\beta_{n-2}).

Since [M](β1β2βn2)H2(M;)[M]\frown(\beta_{1}\smile\beta_{2}\smile\dots\smile\beta_{n-2})\in H_{2}(M;\mathbb{Z}) is non-spherical, this means the class [M^](β^1pβ2pβn2)H2(M^;)[\hat{M}]\frown(\hat{\beta}_{1}\smile p^{*}\beta_{2}\smile\dots\smile p^{*}\beta_{n-2})\in H_{2}(\hat{M};\mathbb{Z}) is non-spherical as well. Thus M^\hat{M} is an SYS manifold as desired. \blacksquare

Lemma 4.4.

Let MnM^{n} be an SYS manifold with nonzero cohomology classes β1,,βn2\beta_{1},\dots,\beta_{n-2} in H1(M;)H^{1}(M;\mathbb{Z}) such that the homology class [M](β1βn2)H2(M;)[M]\frown(\beta_{1}\smile\dots\smile\beta_{n-2})\in H_{2}(M;\mathbb{Z}) is non-spherical. Let Σn1\Sigma^{n-1} be a closed embedded orientable hypersurface representing the Poincaré dual of β1\beta_{1}. Then Σ\Sigma is an SYS manifold.

Proof.

Consider the embedding f:ΣMf:\Sigma\to M. Using naturality of cup product and cap product and the assumption f[Σ]=[M]β1f_{*}[\Sigma]=[M]\frown\beta_{1}, we have

f([Σ](fβ2fβn2))\displaystyle f_{*}\Big{(}[\Sigma]\frown(f^{*}\beta_{2}\smile\dots\smile f^{*}\beta_{n-2})\Big{)}
=f([Σ])(β2βn2)\displaystyle=f_{*}([\Sigma])\frown(\beta_{2}\smile\dots\smile\beta_{n-2})
=([M]β1)(β2βn2)\displaystyle=([M]\frown\beta_{1})\frown(\beta_{2}\smile\dots\smile\beta_{n-2})
=[M](β1β2βn2),\displaystyle=[M]\frown(\beta_{1}\smile\beta_{2}\smile\dots\smile\beta_{n-2}),

so the class [Σ](fβ2fβn2)H2(Σ)[\Sigma]\frown(f^{*}\beta_{2}\smile\dots\smile f^{*}\beta_{n-2})\in H_{2}(\Sigma) is non-spherical as well. Thus Σ\Sigma is an SYS manifold as desired. \blacksquare

We are now ready to give a proof of Theorem 1.3.

Proof of Theorem 1.3.

Assume MM is an SYS manifold, XX is any closed nn-manifold, and M#XM\#X admits a complete metric of positive scalar curvature. By taking a connected component we can assume MM is connected.

Let β1,β2,,βn2\beta_{1},\beta_{2},\dots,\beta_{n-2} in H1(M;)H^{1}(M;\mathbb{Z}) be the cohomology classes as in the definition of an SYS manifold. By Lemma 2.1, we can take ΣM\Sigma\subset M to be a closed embedded orientable hypersurface such that [Σ]Hn1(M;)[\Sigma]\in H_{n-1}(M;\mathbb{Z}) is dual to β1\beta_{1}. Then there exists a connected component Σ\Sigma^{\prime} of Σ\Sigma such that if we denote the Poincaré dual of [Σ][\Sigma^{\prime}] by β1H1(M;)\beta^{\prime}_{1}\in H^{1}(M;\mathbb{Z}), then the homology class [M](β1β2βn2)H2(M;)[M]\frown(\beta^{\prime}_{1}\smile\beta_{2}\smile\dots\smile\beta_{n-2})\in H_{2}(M;\mathbb{Z}) is also non-spherical. Then by replacing β1\beta_{1} by β1\beta^{\prime}_{1} and Σ\Sigma by Σ\Sigma^{\prime}, we can take Σ\Sigma to be a connected hypersurface dual to β1\beta_{1}.

Apply Theorem 3.4 with m=n1m=n-1 and a=1a=1. Then mm-intermediate curvature reduces to scalar curvature and we have 𝒞n1=12R\mathcal{C}_{n-1}=\frac{1}{2}R. We obtain a closed connected orientable Riemannian manifold (Y~,g~)(\tilde{Y},\tilde{g}), a smooth function hC(Y)h\in C^{\infty}(Y), and a closed embedded orientable hypersurface Λn1Y~\Lambda^{n-1}\subset\tilde{Y} such that

  1. (i)

    Y~=M#iX~i\tilde{Y}=M^{\prime}\#_{i}\tilde{X}_{i}, where MM^{\prime} is a finite cyclic covering of MM obtained by cutting and pasting along Σ\Sigma and the X~i\tilde{X}_{i}’s are a finite number of closed manifolds.

  2. (ii)

    In a neighborhood of Λ\Lambda, Y~\tilde{Y} has positive scalar curvature.

  3. (iii)

    p[Λ]=[Σ]Hn1(M)p_{*}[\Lambda]=[\Sigma]\in H_{n-1}(M^{\prime}), where p:Y~Mp:\tilde{Y}\to M^{\prime} is the projection map and [Σ][\Sigma] is the homology class represented by any copy of Σ\Sigma in MM^{\prime}.

  4. (iv)

    On Λ\Lambda, we have

    HΛ=h,H_{\Lambda}=h,
    12RY~+h22|DY~h|>0,\frac{1}{2}R_{\tilde{Y}}+h^{2}-2|D_{\tilde{Y}}h|>0,

    and

    𝒬(ψ)=Λ(|DΛψ|2(|IIΛ|2+RicY~(ν,ν)+DY~h,ν)ψ2)𝑑n10\mathcal{Q}(\psi)=\int_{\Lambda}\left(|D_{\Lambda}\psi|^{2}-\big{(}|{\rm II}_{\Lambda}|^{2}+\operatorname{Ric}_{\tilde{Y}}(\nu,\nu)+\langle D_{\tilde{Y}}h,\nu\rangle\big{)}\psi^{2}\right)d\mathcal{H}^{n-1}\geq 0

    for all ψC(Λ)\psi\in C^{\infty}(\Lambda).

Using conditions (i) and (iii) and Lemmas 4.3, 4.2, 4.4, we have that Λ\Lambda is an SYS manifold.

On the other hand, the traced Gaussian equation gives

RY~=RΛ+2RicY~(ν,ν)+|IIΛ|2HΛ2.R_{\tilde{Y}}=R_{\Lambda}+2\operatorname{Ric}_{\tilde{Y}}(\nu,\nu)+|{\rm II}_{\Lambda}|^{2}-H_{\Lambda}^{2}.

Applying this in (iv), we obtain that

Λ|DΛψ|2𝑑n1\displaystyle\int_{\Lambda}|D_{\Lambda}\psi|^{2}d\mathcal{H}^{n-1} Λ(|IIΛ|2+RicY~(ν,ν)+DY~h,ν)ψ2𝑑n1\displaystyle\geq\int_{\Lambda}\big{(}|{\rm II}_{\Lambda}|^{2}+\operatorname{Ric}_{\tilde{Y}}(\nu,\nu)+\langle D_{\tilde{Y}}h,\nu\rangle\big{)}\psi^{2}d\mathcal{H}^{n-1}
=Λ(|IIΛ|2+12(RY~RΛ|IIΛ|2+h2)+DY~h,ν)ψ2𝑑n1\displaystyle=\int_{\Lambda}\big{(}|{\rm II}_{\Lambda}|^{2}+\frac{1}{2}(R_{\tilde{Y}}-R_{\Lambda}-|{\rm II}_{\Lambda}|^{2}+h^{2})+\langle D_{\tilde{Y}}h,\nu\rangle\big{)}\psi^{2}d\mathcal{H}^{n-1}
12Λ(RY~+h22|DY~h|)ψ2𝑑n112ΛRΛψ2𝑑n1,\displaystyle\geq\frac{1}{2}\int_{\Lambda}(R_{\tilde{Y}}+h^{2}-2|D_{\tilde{Y}}h|\big{)}\psi^{2}d\mathcal{H}^{n-1}-\frac{1}{2}\int_{\Lambda}R_{\Lambda}\psi^{2}d\mathcal{H}^{n-1},

so by (ii) and (iv),

Λ(2|DΛψ|2+RΛψ2)𝑑n1Λ(RY~+h22|DY~h|)ψ2𝑑n1>0\int_{\Lambda}(2|D_{\Lambda}\psi|^{2}+R_{\Lambda}\psi^{2})d\mathcal{H}^{n-1}\geq\int_{\Lambda}(R_{\tilde{Y}}+h^{2}-2|D_{\tilde{Y}}h|\big{)}\psi^{2}d\mathcal{H}^{n-1}>0

for all 0ψC(Λ)0\neq\psi\in C^{\infty}(\Lambda).

Since 4n1n224\frac{n-1}{n-2}\geq 2 for n3n\geq 3, this shows the conformal Laplacian L=4n1n2ΔΛ+RΛL=-4\frac{n-1}{n-2}\Delta_{\Lambda}+R_{\Lambda} has positive first eigenvalue. If we let ϕ>0\phi>0 denote the first eigenfunction and gΛg_{\Lambda} denote the induced metric of Λ\Lambda, then (Λ,ϕ4n2gΛ)(\Lambda,\phi^{\frac{4}{n-2}}g_{\Lambda}) has scalar curvature R~=ϕ(n+2)/(n2)Lϕ>0{\tilde{R}}=\phi^{-(n+2)/(n-2)}L\phi>0.

This is a contradiction because by [SY79b], an SYS manifold of dimension 3n73\leq n\leq 7 cannot admit a metric of positive scalar curvature. \blacksquare

5. Proof of Theorem 1.6

5.1. Modified stable weighted slicings

In this subsection, we closely follow Section 3 of [BHJ22]. We modify the construction of stable weighted slicing given there and define the modified stable weighted slicing as follows. The only difference is how we define the top slice Σ1\Sigma_{1}. For a stable weighted slicing, Σ1\Sigma_{1} is a stable minimal hypersurface of Σ0\Sigma_{0}; in comparison, we require Σ1\Sigma_{1} to come from the boundary component of some μ\mu-bubble. In particular, Σ1\Sigma_{1} is the same type of hypersurface that we obtain from Theorem 3.4. Our goal is to show that positive mm-intermediate curvature obstructs the existence of modified stable weighted slicings.

Definition 5.1 (Modified stable weighted slicing of order mm with constant aa).

Suppose 2mn12\leq m\leq n-1 and let (Nn,g)(N^{n},g) be a Riemannian manifold of dimension dimN=n\dim N=n. A modified stable weighted slicing of order mm with constant a>0a>0 consists of a collection of submanifolds Σk\Sigma_{k}, 0km0\leq k\leq m, a smooth function hC(N)h\in C^{\infty}(N), and a collection of positive functions ρkC(Σk)\rho_{k}\in C^{\infty}(\Sigma_{k}) satisfying the following conditions:

  • Σ0=N\Sigma_{0}=N and ρ0=1\rho_{0}=1.

  • For k=1k=1, Σ1\Sigma_{1} is an embedded two-sided hypersurface in Σ0\Sigma_{0} such that

    • the mean curvature satisfies HΣ1=h,H_{\Sigma_{1}}=h,

    • the operator 1=ΔΣ1|IIΣ1|2RicΣ0(ν1,ν1)DΣ0h,ν1\mathcal{L}_{1}=-\Delta_{\Sigma_{1}}-|{\rm II}_{\Sigma_{1}}|^{2}-\operatorname{Ric}_{\Sigma_{0}}(\nu_{1},\nu_{1})-\langle D_{\Sigma_{0}}h,\nu_{1}\rangle is a non-negative operator, where ν1\nu_{1} is a unit normal vector field along Σ1\Sigma_{1},

    • we have (𝒞m)Σ0+aHΣ12|DΣ0h|>0,(\mathcal{C}_{m})_{\Sigma_{0}}+aH_{\Sigma_{1}}^{2}-|D_{\Sigma_{0}}h|>0, on Σ1\Sigma_{1}.

  • For each 2km2\leq k\leq m, Σk\Sigma_{k} is an embedded two-sided hypersurface in Σk1\Sigma_{k-1}. Moreover, Σk\Sigma_{k} is a stable critical point of the ρk1\rho_{k-1}-weighted area

    ρk1nk(Σ)=Σρk1𝑑μ\mathcal{H}^{n-k}_{\rho_{k-1}}(\Sigma)=\int_{\Sigma}\rho_{k-1}\,d\mu

    in the class of hypersurfaces ΣΣk1\Sigma\subset\Sigma_{k-1}.

  • For k=1k=1, v1=ρ1C(Σ1)v_{1}=\rho_{1}\in C^{\infty}(\Sigma_{1}) is a first eigenfunction of 1\mathcal{L}_{1}. For each 2km2\leq k\leq m, the function vk=ρkρk1|ΣkC(Σk)v_{k}=\frac{\rho_{k}}{\rho_{k-1}|_{\Sigma_{k}}}\in C^{\infty}(\Sigma_{k}) is a first eigenfunction of the stability operator associated with the ρk1\rho_{k-1}-weighted area.

Let (Nn,g)(N^{n},g) be a closed Riemannian manifold of dimension nn. Throughout this subsection, we assume that we are given a modified stable weighted slicing of order mm. Then all the calculations in [BHJ22, Section 3] for Σk\Sigma_{k}, 2km2\leq k\leq m carry over, and we record them here.

By the first variation formula for weighted area, Corollary 2.2 in [BHJ22], the mean curvature HΣkH_{\Sigma_{k}} of the slice Σk\Sigma_{k} in the manifold Σk+1\Sigma_{k+1} satisfies for 2km2\leq k\leq m the relation

HΣk=DΣk1logρk1,νk.H_{\Sigma_{k}}=-\langle D_{\Sigma_{k-1}}\log\rho_{k-1},\nu_{k}\rangle.

By the second variation formula for weighted area, Proposition 2.3 in [BHJ22], we obtain for 2km2\leq k\leq m the inequality

0\displaystyle 0\leq Σkρk1(ψΔΣkψψDΣklogρk1,DΣkψ)𝑑μ\displaystyle\int_{\Sigma_{k}}\rho_{k-1}\left(-\psi\Delta_{\Sigma_{k}}\psi-\psi\langle D_{\Sigma_{k}}\log\rho_{k-1},D_{\Sigma_{k}}\psi\rangle\right)\,d\mu
Σkρk1(|IIΣk|2+RicΣk1(νk,νk)(DΣk12logρk1)(νk,νk))ψ2𝑑μ\displaystyle-\int_{\Sigma_{k}}\rho_{k-1}\left(|{\rm II}_{\Sigma_{k}}|^{2}+\operatorname{Ric}_{\Sigma_{k-1}}(\nu_{k},\nu_{k})-(D_{\Sigma_{k-1}}^{2}\log\rho_{k-1})(\nu_{k},\nu_{k})\right)\psi^{2}\,d\mu

for all ψC(Σk)\psi\in C^{\infty}(\Sigma_{k}). By Definition 5.1 we may write ρk=ρk1vk\rho_{k}=\rho_{k-1}\,v_{k}, where vk>0v_{k}>0 is the first eigenfunction of the stability operator for the weighted area functional on Σk\Sigma_{k}. The function vkv_{k} satisfies

λkvk=\displaystyle\lambda_{k}v_{k}= ΔΣkvkDΣklogρk1,DΣkvk(|IIΣk|2+RicΣk1(νk,νk))vk\displaystyle-\Delta_{\Sigma_{k}}v_{k}-\langle D_{\Sigma_{k}}\log\rho_{k-1},D_{\Sigma_{k}}v_{k}\rangle-\left(|{\rm II}_{\Sigma_{k}}|^{2}+\operatorname{Ric}_{\Sigma_{k-1}}(\nu_{k},\nu_{k})\right)v_{k}
+(DΣk12logρk1)(νk,νk)vk,\displaystyle+(D_{\Sigma_{k-1}}^{2}\log\rho_{k-1})(\nu_{k},\nu_{k})v_{k},

where λk0\lambda_{k}\geq 0 denotes the first eigenvalue of the stability operator.

By setting wk=logvkw_{k}=\log v_{k} we record the following equation:

(4) λk=\displaystyle\lambda_{k}= ΔΣkwkDΣklogρk1,DΣkwk(|IIΣk|2+RicΣk1(νk,νk))\displaystyle-\Delta_{\Sigma_{k}}w_{k}-\langle D_{\Sigma_{k}}\log\rho_{k-1},D_{\Sigma_{k}}w_{k}\rangle-\left(|{\rm II}_{\Sigma_{k}}|^{2}+\operatorname{Ric}_{\Sigma_{k-1}}(\nu_{k},\nu_{k})\right)
+(DΣk12logρk1)(νk,νk)|DΣkwk|2.\displaystyle+(D_{\Sigma_{k-1}}^{2}\log\rho_{k-1})(\nu_{k},\nu_{k})-|D_{\Sigma_{k}}w_{k}|^{2}.
Lemma 5.2 (First slicing identity, [BHJ22, Lemma 3.1]).

We have for 2km2\leq k\leq m the identity

ΔΣklogρk1+(DΣk12logρk1)(νk,νk)=ΔΣk1logρk1+HΣk2.\displaystyle\Delta_{\Sigma_{k}}\log\rho_{k-1}+(D_{\Sigma_{k-1}}^{2}\log\rho_{k-1})(\nu_{k},\nu_{k})=\Delta_{\Sigma_{k-1}}\log\rho_{k-1}+H_{\Sigma_{k}}^{2}.
Lemma 5.3 (Second slicing identity, [BHJ22, Lemma 3.2]).

We have for 2km12\leq k\leq m-1 the identity

ΔΣklogρk=\displaystyle\Delta_{\Sigma_{k}}\log\rho_{k}= ΔΣklogρk1+(DΣk12logρk1)(νk,νk)\displaystyle\Delta_{\Sigma_{k}}\log\rho_{k-1}+(D_{\Sigma_{k-1}}^{2}\log\rho_{k-1})(\nu_{k},\nu_{k})
(λk+|IIΣk|2+RicΣk1(νk,νk)+DΣklogρk,DΣkwk).\displaystyle-\left(\lambda_{k}+|{\rm II}_{\Sigma_{k}}|^{2}+\operatorname{Ric}_{\Sigma_{k-1}}(\nu_{k},\nu_{k})+\langle D_{\Sigma_{k}}\log\rho_{k},D_{\Sigma_{k}}w_{k}\rangle\right).
Lemma 5.4 (Second slicing identity for k=1k=1).

We have the identity

ΔΣ1logρ1=\displaystyle\Delta_{\Sigma_{1}}\log\rho_{1}= (λ1+|IIΣ1|2+RicΣ0(ν1,ν1)+DΣ1logρ1,DΣ1w1DΣ0h,ν1).\displaystyle-\left(\lambda_{1}+|{\rm II}_{\Sigma_{1}}|^{2}+\operatorname{Ric}_{\Sigma_{0}}(\nu_{1},\nu_{1})+\langle D_{\Sigma_{1}}\log\rho_{1},D_{\Sigma_{1}}w_{1}\rangle-\langle D_{\Sigma_{0}}h,\nu_{1}\rangle\right).
Proof.

This is a direct computation using that ρ1\rho_{1} is a first eigenfunction of 1\mathcal{L}_{1} with eigenvalue λ1\lambda_{1} and w1=logρ1w_{1}=\log\rho_{1}. \blacksquare

Lemma 5.5 (Stability inequality on the bottom slice, [BHJ22, Lemma 3.3]).

On the bottom slice Σm\Sigma_{m} we have the inequality

Σmρm11(ΔΣm1logρm1+HΣm2)𝑑μΣmρm11(|IIΣm|2+RicΣm1(νm,νm))𝑑μ.\displaystyle\int_{\Sigma_{m}}\rho_{m-1}^{-1}\left(\Delta_{\Sigma_{m-1}}\log\rho_{m-1}+H_{\Sigma_{m}}^{2}\right)d\mu\geq\int_{\Sigma_{m}}\rho_{m-1}^{-1}\left(|{\rm II}_{\Sigma_{m}}|^{2}+\operatorname{Ric}_{\Sigma_{m-1}}(\nu_{m},\nu_{m})\right)\,d\mu.

Similar to [BHJ22, Lemma 3.4], we have the following:

Lemma 5.6 (Main inequality).

We have the inequality

Σmρm11(Λ++𝒢++DΣ0h,ν1)𝑑μ0,\displaystyle\int_{\Sigma_{m}}\rho_{m-1}^{-1}\left(\Lambda+\mathcal{R}+\mathcal{G}+\mathcal{E}+\langle D_{\Sigma_{0}}h,\nu_{1}\rangle\right)\,d\mu\leq 0,

where the eigenvalue term Λ\Lambda, the intrinsic curvature term \mathcal{R}, the extrinsic curvature term \mathcal{E}, and the gradient term 𝒢\mathcal{G} are given by

Λ\displaystyle\Lambda =k=1m1λk,=k=1mRicΣk1(νk,νk),𝒢=k=1m1DΣklogρk,DΣkwk,\displaystyle=\sum_{k=1}^{m-1}\lambda_{k},\;\mathcal{R}=\sum_{k=1}^{m}\operatorname{Ric}_{\Sigma_{k-1}}(\nu_{k},\nu_{k}),\;\mathcal{G}=\sum_{k=1}^{m-1}\langle D_{\Sigma_{k}}\log\rho_{k},D_{\Sigma_{k}}w_{k}\rangle,
and\displaystyle\;\text{and}\;\;\mathcal{E} =k=1m|IIΣk|2k=2mHΣk2.\displaystyle=\sum_{k=1}^{m}|{\rm II}_{\Sigma_{k}}|^{2}-\sum_{k=2}^{m}H_{\Sigma_{k}}^{2}.
Proof.

If we combine Lemma 5.2, and Lemma 5.3, we obtain for 2km12\leq k\leq m-1 the identity

ΔΣklogρk=ΔΣk1logρk1+HΣk2\displaystyle\Delta_{\Sigma_{k}}\log\rho_{k}=\Delta_{\Sigma_{k-1}}\log\rho_{k-1}+H_{\Sigma_{k}}^{2} (λk+|IIΣk|2+RicΣk1(νk,νk)+DΣklogρk,DΣkwk).\displaystyle-\left(\lambda_{k}+|{\rm II}_{\Sigma_{k}}|^{2}+\operatorname{Ric}_{\Sigma_{k-1}}(\nu_{k},\nu_{k})+\langle D_{\Sigma_{k}}\log\rho_{k},D_{\Sigma_{k}}w_{k}\rangle\right).

Summation of this formula over kk from 22 to m1m-1 and using Lemma 5.4 yields

ΔΣm1logρm1=\displaystyle\Delta_{\Sigma_{m}-1}\log\rho_{m-1}= DΣ0h,ν1+k=2m1HΣk2\displaystyle-\langle D_{\Sigma_{0}}h,\nu_{1}\rangle+\sum_{k=2}^{m-1}H_{\Sigma_{k}}^{2}
k=1m1(λk+|IIΣk|2+RicΣk1(νk,νk)+DΣklogρk,DΣkwk).\displaystyle-\sum_{k=1}^{m-1}\left(\lambda_{k}+|{\rm II}_{\Sigma_{k}}|^{2}+\operatorname{Ric}_{\Sigma_{k-1}}(\nu_{k},\nu_{k})+\langle D_{\Sigma_{k}}\log\rho_{k},D_{\Sigma_{k}}w_{k}\rangle\right).

Plugging this into Lemma 5.5 yields the result. \blacksquare

The eigenvalue term Λ\Lambda is non-negative, since it is the sum of the non-negative eigenvalues. To estimate the other terms in the above lemma, fix a point xΣmx\in\Sigma_{m} and consider an orthonormal basis {e1,,en}\{e_{1},\dots,e_{n}\} of TxNT_{x}N with ej=νje_{j}=\nu_{j} for 1jm1\leq j\leq m as above. We define for each 1km1\leq k\leq m the extrinsic curvature terms 𝒱k\mathcal{V}_{k}:

𝒱1=\displaystyle\mathcal{V}_{1}= |IIΣ1|2+p=2mq=p+1n(IIΣ1(ep,ep)IIΣ1(eq,eq)IIΣ1(ep,eq)2),\displaystyle|{\rm II}_{\Sigma_{1}}|^{2}+\sum_{p=2}^{m}\sum_{q=p+1}^{n}\left({\rm II}_{\Sigma_{1}}(e_{p},e_{p}){\rm II}_{\Sigma_{1}}(e_{q},e_{q})-{\rm II}_{\Sigma_{1}}(e_{p},e_{q})^{2}\right),
𝒱k=\displaystyle\mathcal{V}_{k}= |IIΣk|2(1212(k1))HΣk2\displaystyle|{\rm II}_{\Sigma_{k}}|^{2}-\left(\frac{1}{2}-\frac{1}{2(k-1)}\right)H_{\Sigma_{k}}^{2}
+p=k+1mq=p+1n(IIΣk(ep,ep)IIΣk(eq,eq)IIΣk(ep,eq)2)for 2km1,\displaystyle+\sum_{p=k+1}^{m}\sum_{q=p+1}^{n}\left({\rm II}_{\Sigma_{k}}(e_{p},e_{p}){\rm II}_{\Sigma_{k}}(e_{q},e_{q})-{\rm II}_{\Sigma_{k}}(e_{p},e_{q})^{2}\right)\;\text{for}\;2\leq k\leq m-1,
𝒱m=\displaystyle\mathcal{V}_{m}= |IIΣm|2(1212(m1))HΣm2.\displaystyle|{\rm II}_{\Sigma_{m}}|^{2}-\left(\frac{1}{2}-\frac{1}{2(m-1)}\right)H_{\Sigma_{m}}^{2}.

Inspecting the estimate for 𝒢\mathcal{G} and \mathcal{R} in [BHJ22, Lemma 3.7 and 3.8], we see that the same calculations carry over, so we have the following lemma:

Lemma 5.7.

[BHJ22, Lemma 3.10]  
We have the pointwise estimate on Σm\Sigma_{m}:

++𝒢𝒞m(e1,,em)+k=1m𝒱k.\displaystyle\mathcal{R}+\mathcal{E}+\mathcal{G}\geq\mathcal{C}_{m}(e_{1},\dots,e_{m})+\sum_{k=1}^{m}\mathcal{V}_{k}.

Now we need to estimate the extrinsic curvature terms 𝒱k\mathcal{V}_{k}. The estimate on the top slice is what differs from [BHJ22].

Lemma 5.8 (Extrinsic curvature terms on the top slice).

Suppose m2mn+2n2>0m^{2}-mn+2n-2>0 and m2mn+m+n>0m^{2}-mn+m+n>0. Then we have the estimate

𝒱1aHΣ120,\displaystyle\mathcal{V}_{1}\geq aH_{\Sigma_{1}}^{2}\geq 0,

for any 0amin{m2(m1),1nm,m2mn+m+n2(m2mn+2n2)}0\leq a\leq\min\{\frac{m}{2(m-1)},\frac{1}{n-m},\frac{m^{2}-mn+m+n}{2(m^{2}-mn+2n-2)}\}.

Proof.

Consider the quantity 𝒱1aHΣ12\mathcal{V}_{1}-aH_{\Sigma_{1}}^{2} for some aa satisfying

0amin{m2(m1),1nm,m2mn+m+n2(m2mn+2n2)}.0\leq a\leq\min\{\frac{m}{2(m-1)},\frac{1}{n-m},\frac{m^{2}-mn+m+n}{2(m^{2}-mn+2n-2)}\}.

We begin by discarding the off-diagonal terms of the second fundamental form IIΣ1{\rm II}_{\Sigma_{1}}:

𝒱1aHΣ12\displaystyle\mathcal{V}_{1}-aH_{\Sigma_{1}}^{2}
=\displaystyle= |IIΣ1|2+p=2mq=p+1n(IIΣ1(ep,ep)IIΣ1(eq,eq)IIΣ1(ep,eq)2)aHΣ12\displaystyle\,|{\rm II}_{\Sigma_{1}}|^{2}+\sum_{p=2}^{m}\sum_{q=p+1}^{n}\left({\rm II}_{\Sigma_{1}}(e_{p},e_{p}){\rm II}_{\Sigma_{1}}(e_{q},e_{q})-{\rm II}_{\Sigma_{1}}(e_{p},e_{q})^{2}\right)-aH_{\Sigma_{1}}^{2}
\displaystyle\geq p=2nIIΣ1(ep,ep)2+p=2mq=p+1nIIΣ1(ep,ep)IIΣ1(eq,eq)aHΣ12\displaystyle\,\sum_{p=2}^{n}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})^{2}+\sum_{p=2}^{m}\sum_{q=p+1}^{n}{\rm II}_{\Sigma_{1}}(e_{p},e_{p}){\rm II}_{\Sigma_{1}}(e_{q},e_{q})-aH_{\Sigma_{1}}^{2}
=\displaystyle= p=2nIIΣ1(ep,ep)2+p=2mIIΣ1(ep,ep)q=p+1mIIΣ1(eq,eq)+p=2mIIΣ1(ep,ep)q=m+1nIIΣ1(eq,eq)aHΣ12\displaystyle\,\sum_{p=2}^{n}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})^{2}+\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})\sum_{q=p+1}^{m}{\rm II}_{\Sigma_{1}}(e_{q},e_{q})+\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})\sum_{q=m+1}^{n}{\rm II}_{\Sigma_{1}}(e_{q},e_{q})-aH_{\Sigma_{1}}^{2}
=\displaystyle= 12p=2mIIΣ1(ep,ep)2+q=m+1nIIΣ1(eq,eq)2+12(p=2mIIΣ1(ep,ep))2\displaystyle\,\frac{1}{2}\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})^{2}+\sum_{q=m+1}^{n}{\rm II}_{\Sigma_{1}}(e_{q},e_{q})^{2}+\frac{1}{2}\left(\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})\right)^{2}
+p=2mIIΣ1(ep,ep)q=m+1nIIΣ1(eq,eq)a(p=2mIIΣ1(ep,ep)+q=m+1nIIΣ1(eq,eq))2\displaystyle\,+\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})\sum_{q=m+1}^{n}{\rm II}_{\Sigma_{1}}(e_{q},e_{q})-a\left(\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})+\sum_{q=m+1}^{n}{\rm II}_{\Sigma_{1}}(e_{q},e_{q})\right)^{2}
=\displaystyle= 12p=2mIIΣ1(ep,ep)2+q=m+1nIIΣ1(eq,eq)2+(12a)(p=2mIIΣ1(ep,ep))2\displaystyle\,\frac{1}{2}\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})^{2}+\sum_{q=m+1}^{n}{\rm II}_{\Sigma_{1}}(e_{q},e_{q})^{2}+\left(\frac{1}{2}-a\right)\left(\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})\right)^{2}
a(q=m+1nIIΣ1(eq,eq))2+(12a)p=2mIIΣ1(ep,ep)q=m+1nIIΣ1(eq,eq).\displaystyle\,-a\left(\sum_{q=m+1}^{n}{\rm II}_{\Sigma_{1}}(e_{q},e_{q})\right)^{2}+\left(1-2a\right)\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})\sum_{q=m+1}^{n}{\rm II}_{\Sigma_{1}}(e_{q},e_{q}).

For simplicity, let A:=p=2mIIΣ1(ep,ep)A:=\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p}) and B:=q=m+1nIIΣ1(eq,eq)B:=\sum_{q=m+1}^{n}{\rm II}_{\Sigma_{1}}(e_{q},e_{q}). By the Cauchy–Schwarz inequality,

p=2mIIΣ1(ep,ep)21m1(p=2mIIΣ1(ep,ep))2=1m1A2\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})^{2}\geq\frac{1}{m-1}\left(\sum_{p=2}^{m}{\rm II}_{\Sigma_{1}}(e_{p},e_{p})\right)^{2}=\frac{1}{m-1}A^{2}

and

q=m+1nIIΣ1(eq,eq)21nm(q=m+1nIIΣ1(eq,eq))2=1nmB2.\sum_{q=m+1}^{n}{\rm II}_{\Sigma_{1}}(e_{q},e_{q})^{2}\geq\frac{1}{n-m}\left(\sum_{q=m+1}^{n}{\rm II}_{\Sigma_{1}}(e_{q},e_{q})\right)^{2}=\frac{1}{n-m}B^{2}.

Thus

𝒱1aHΣ12\displaystyle\mathcal{V}_{1}-aH_{\Sigma_{1}}^{2}\geq (m2(m1)a)A2+(1nma)B2+(12a)AB\displaystyle\left(\frac{m}{2(m-1)}-a\right)A^{2}+\left(\frac{1}{n-m}-a\right)B^{2}+\left(1-2a\right)AB
\displaystyle\geq (2(m2(m1)a)(1nma)(12a))|AB|,\displaystyle\left(2\sqrt{\left(\frac{m}{2(m-1)}-a\right)\left(\frac{1}{n-m}-a\right)}-(1-2a)\right)|AB|,

using the assumptions am2(m1)a\leq\frac{m}{2(m-1)} and a1nma\leq\frac{1}{n-m} and the AM-GM inequality.

Using am2mn+m+n2(m2mn+2n2)a\leq\frac{m^{2}-mn+m+n}{2(m^{2}-mn+2n-2)}, we have

4(m2(m1)a)(1nma)(12a)2\displaystyle 4\left(\frac{m}{2(m-1)}-a\right)\left(\frac{1}{n-m}-a\right)-(1-2a)^{2}
=\displaystyle= m2mn+m+n(m1)(nm)2(m2mn+2n2)(m1)(nm)a\displaystyle\,\frac{m^{2}-mn+m+n}{(m-1)(n-m)}-\frac{2(m^{2}-mn+2n-2)}{(m-1)(n-m)}a
\displaystyle\geq  0,\displaystyle\,0,

so 𝒱1aHΣ120\mathcal{V}_{1}-aH_{\Sigma_{1}}^{2}\geq 0 as desired.

\blacksquare

Again, the estimate for 2km2\leq k\leq m in [BHJ22] carry over, so we have the following two lemmas.

Lemma 5.9 (Extrinsic curvature terms on intermediate slices, [BHJ22, Lemma 3.12]).

We have for 2km12\leq k\leq m-1 the estimate

𝒱km2mn+2n22(m1)(nm)(q=m+1nIIΣk(eq,eq))2.\displaystyle\mathcal{V}_{k}\geq\frac{m^{2}-mn+2n-2}{2(m-1)(n-m)}\left(\sum_{q=m+1}^{n}{\rm II}_{\Sigma_{k}}(e_{q},e_{q})\right)^{2}.
Lemma 5.10 (Extrinsic curvature terms on the bottom slice, [BHJ22, Lemma 3.13]).

We have the estimate

𝒱mm2mn+2n22(nm)(m1)HΣm2.\mathcal{V}_{m}\geq\frac{m^{2}-mn+2n-2}{2(n-m)(m-1)}\,H_{\Sigma_{m}}^{2}.

We record by direct computation the following lemma:

Lemma 5.11 (Algebraic lemma).

Suppose 3n73\leq n\leq 7 and 2mn12\leq m\leq n-1 are integers. We define the quantity ξ(n,m)\xi(n,m)\in\mathbb{R} by the formula

ξ(n,m)=min{m2mn+2n2,m2mn+m+n}.\xi(n,m)=\min\{m^{2}-mn+2n-2,m^{2}-mn+m+n\}.

Then for 3n53\leq n\leq 5, we have ξ(n,m)>0\xi(n,m)>0 for all 2mn12\leq m\leq n-1. For 6n76\leq n\leq 7, we have ξ(n,m)>0\xi(n,m)>0 precisely when n2mn1n-2\leq m\leq n-1.

Remark 5.12.

The quantity m2mn+2n2m^{2}-mn+2n-2 is the same as the one in [BHJ22, Lemma 3.14]. Compared to [BHJ22], we need the extra constraint m2mn+m+n>0m^{2}-mn+m+n>0 coming from Lemma 5.8. This comes from our requirement for the top slice to come from the boundary component of some μ\mu-bubble. Unlike stable minimal hypersurfaces where H=0H=0, in our case we have no a priori bound on the mean curvature of the top slice, so we need extra constraint on the dimensions to control it. In [CKL22], Chu–Kwong–Lee used μ\mu-bubbles on the bottom slice in their proof of the rigidity result, and therefore needed the same constraint m2mn+m+n>0m^{2}-mn+m+n>0. This is why their rigidity result is stated for n5n\leq 5. Xu [Xu23] proved the same estimate on the bottom slice without using μ\mu-bubbles, and thus extended the rigidity result to n=6n=6. In our case, since we need μ\mu-bubbles to reduce the non-compact setting to a compact setting, it is unclear whether we can get rid of the constraint m2mn+m+n>0m^{2}-mn+m+n>0.

Using the above lemmas, we can show that manifolds with positive mm-intermediate curvature do not allow stable weighted slicings of order mm with constant aa.

Theorem 5.13 (mm-intermediate curvature and modified stable weighted slicings).

Assume that m2mn+2n2>0m^{2}-mn+2n-2>0 and m2mn+m+n>0m^{2}-mn+m+n>0. Assume 0<amin{m2(m1),1nm,m2mn+m+n2(m2mn+2n2)}0<a\leq\min\{\frac{m}{2(m-1)},\frac{1}{n-m},\frac{m^{2}-mn+m+n}{2(m^{2}-mn+2n-2)}\}. Suppose the closed Riemannian manifold (Nn,g)(N^{n},g) admits a modified stable weighted slicing

ΣmΣ1Σ0=Nn\Sigma_{m}\subset\dots\subset\Sigma_{1}\subset\Sigma_{0}=N^{n}

of order 2mn12\leq m\leq n-1 with constant aa. Then we must have (𝒞m)N0(\mathcal{C}_{m})_{N}\leq 0 at some point on Σm\Sigma_{m}.

Proof.

Suppose that the Riemannian manifold (Nn,g)(N^{n},g) admits a stable weighted slicing

ΣmΣ1Σ0=Nn\Sigma_{m}\subset\dots\subset\Sigma_{1}\subset\Sigma_{0}=N^{n}

of order 2mn12\leq m\leq n-1 with constant aa, and (𝒞m)N>0(\mathcal{C}_{m})_{N}>0 on Σm\Sigma_{m}.

Combining the estimates for the extrinsic curvature terms, Lemmas 5.8, 5.9 and 5.10, with Lemma 5.7 implies

++𝒢𝒞m(e1,,em)+aHΣ12,\displaystyle\mathcal{R}+\mathcal{E}+\mathcal{G}\geq\mathcal{C}_{m}(e_{1},\dots,e_{m})+aH_{\Sigma_{1}}^{2},

which holds on all points on Σm\Sigma_{m}. By definition of Σ1\Sigma_{1}, the following inequality holds on Σ1\Sigma_{1}:

(𝒞m)Σ0+aHΣ12|DΣ0h,ν1|>0.(\mathcal{C}_{m})_{\Sigma_{0}}+aH_{\Sigma_{1}}^{2}-|\langle D_{\Sigma_{0}}h,\nu_{1}\rangle|>0.

Combining these two inequalities yields that on Σm\Sigma_{m}, we have

++𝒢>DΣ0h,ν1.\displaystyle\mathcal{R}+\mathcal{E}+\mathcal{G}>\langle D_{\Sigma_{0}}h,\nu_{1}\rangle.

This contradicts the main inequality, Lemma 5.6. Therefore we must have (𝒞m)N0(\mathcal{C}_{m})_{N}\leq 0 at some point on Σm\Sigma_{m}. \blacksquare

When m=1m=1, mm-intermediate curvature reduces to Ricci curvature, and we also have a non-existence result.

Theorem 5.14 (Ricci curvature and modified stable weighted slicings).

Suppose the closed Riemannian manifold (Nn,g)(N^{n},g) admits a modified stable weighted slicing

Σ1Σ0=Nn\Sigma_{1}\subset\Sigma_{0}=N^{n}

of order m=1m=1 with constant 1n1\frac{1}{n-1}. Then we must have (𝒞1)N0(\mathcal{C}_{1})_{N}\leq 0 at some point on Σ1\Sigma_{1}.

Proof.

Suppose that (Nn,g)(N^{n},g) admits a stable weighted slicing

Σ1Σ0=Nn\Sigma_{1}\subset\Sigma_{0}=N^{n}

of order m=1m=1 with constant a=1na=\frac{1}{n}, and a metric of positive Ricci curvature. By definition, that means we have a smooth function hC(N)h\in C^{\infty}(N) such that

  • the mean curvature of Σ1\Sigma_{1} satisfies HΣ1=h,H_{\Sigma_{1}}=h,

  • the operator 1=ΔΣ1|IIΣ1|2RicΣ0(ν1,ν1)DΣ0h,ν1\mathcal{L}_{1}=-\Delta_{\Sigma_{1}}-|{\rm II}_{\Sigma_{1}}|^{2}-\operatorname{Ric}_{\Sigma_{0}}(\nu_{1},\nu_{1})-\langle D_{\Sigma_{0}}h,\nu_{1}\rangle is a non-negative operator, where ν1\nu_{1} is a unit normal vector field along Σ1\Sigma_{1},

  • we have (𝒞1)Σ0+1n1HΣ12|DΣ0h,ν1|>0,(\mathcal{C}_{1})_{\Sigma_{0}}+\frac{1}{n-1}H_{\Sigma_{1}}^{2}-|\langle D_{\Sigma_{0}}h,\nu_{1}\rangle|>0, on Σ1\Sigma_{1}.

The second condition means that

Σ1|ϕ|2𝑑Σ1Σ1(|IIΣ1|2+RicΣ0(ν1,ν1)+DΣ0h,ν1)ϕ2𝑑Σ1\int_{\Sigma_{1}}|\nabla\phi|^{2}\,d\Sigma_{1}\geq\int_{\Sigma_{1}}(|{\rm II}_{\Sigma_{1}}|^{2}+\operatorname{Ric}_{\Sigma_{0}}(\nu_{1},\nu_{1})+\langle D_{\Sigma_{0}}h,\nu_{1}\rangle)\phi^{2}\,d\Sigma_{1}

for any ϕC(Σ1)\phi\in C^{\infty}(\Sigma_{1}). Here we set ϕ=1\phi=1, and we get

Σ1|IIΣ1|2+RicΣ0(ν1,ν1)+DΣ0h,ν1dΣ10\int_{\Sigma_{1}}|{\rm II}_{\Sigma_{1}}|^{2}+\operatorname{Ric}_{\Sigma_{0}}(\nu_{1},\nu_{1})+\langle D_{\Sigma_{0}}h,\nu_{1}\rangle\,d\Sigma_{1}\leq 0

On the other hand, by discarding the off-diagonal terms and using the Cauchy-Schwarz inequality, we have that on Σ1\Sigma_{1},

|IIΣ1|2+RicΣ0(ν1,ν1)+DΣ0h,ν1\displaystyle|{\rm II}_{\Sigma_{1}}|^{2}+\operatorname{Ric}_{\Sigma_{0}}(\nu_{1},\nu_{1})+\langle D_{\Sigma_{0}}h,\nu_{1}\rangle 1n1HΣ12+RicΣ0(ν1,ν1)+DΣ0h,ν1\displaystyle\geq\frac{1}{n-1}H_{\Sigma_{1}}^{2}+\operatorname{Ric}_{\Sigma_{0}}(\nu_{1},\nu_{1})+\langle D_{\Sigma_{0}}h,\nu_{1}\rangle
1n1HΣ12+𝒞1|DΣ0h,ν1|\displaystyle\geq\frac{1}{n-1}H_{\Sigma_{1}}^{2}+\mathcal{C}_{1}-|\langle D_{\Sigma_{0}}h,\nu_{1}\rangle|
> 0,\displaystyle>\,0,

which contradicts the integral inequality above.

\blacksquare

5.2. Existence of modified stable weighted slicings

In this section we prove the existence of stable weighted slicings of order mm, thus finishing the proof of Theorem 1.6.

Proof of Theorem 1.6.

Assume either 3n53\leq n\leq 5, 1mn11\leq m\leq n-1 or 6n76\leq n\leq 7, m{1,n2,n1}m\in\{1,n-2,n-1\}. Suppose F:Nn𝕋m×MnmF:N^{n}\rightarrow\mathbb{T}^{m}\times M^{n-m} has degree d0d\neq 0. By taking a connected component we can assume NN is connected.

The projection of FF onto the factors yields maps f0:NMf_{0}:N\rightarrow M and maps f1,,fm:NS1f_{1},\dots,f_{m}:N\rightarrow S^{1}. Let Θ\Theta be a top-dimensional form of the manifold MM normalized such that MΘ=1\int_{M}\Theta=1, and let θ\theta be a one-form on the circle S1S^{1} with S1θ=1\int_{S^{1}}\theta=1. We define the pull-back forms Ω:=f0Θ\Omega:=f_{0}^{*}\,\Theta and ωj:=fjθ\omega_{j}:=f_{j}^{*}\,\theta. By the normalization condition we deduce that Nω1ωmΩ=d\int_{N}\omega_{1}\wedge\dots\wedge\omega_{m}\wedge\Omega=d.

By Lemma 2.1, we can take ΣM\Sigma\subset M to be a closed embedded orientable hypersurface such that [Σ]Hn1(M;)[\Sigma]\in H_{n-1}(M;\mathbb{Z}) is dual to ω1\omega_{1}. Then there exists a connected component Σ\Sigma^{\prime} of Σ\Sigma such that if we denote the Poincaré dual of [Σ][\Sigma^{\prime}] by ω1H1(M;)\omega^{\prime}_{1}\in H^{1}(M;\mathbb{Z}), then we have Nω1ωmΩ=d\int_{N}\omega^{\prime}_{1}\wedge\dots\wedge\omega_{m}\wedge\Omega=d^{\prime} for some nonzero dd^{\prime}. Then by replacing β1\beta_{1} by β1\beta^{\prime}_{1}, Σ\Sigma by Σ\Sigma^{\prime}, dd by dd^{\prime}, and f1f_{1} by a smooth map representing β1\beta^{\prime}_{1}, we can take Σ\Sigma to be a connected hypersurface dual to β1\beta_{1}.

Suppose the manifold N#XN\#X has positive mm-intermediate curvature. Then we apply Theorem 3.4 with an arbitrary a>0a>0 to be determined later. We obtain a closed orientable Riemannian manifold (Y~,g~)(\tilde{Y},\tilde{g}), a smooth function hC(Y)h\in C^{\infty}(Y), and a closed embedded orientable hypersurface Λ1n1Y~\Lambda_{1}^{n-1}\subset\tilde{Y} such that

  1. (i)

    Y~=N#iX~i\tilde{Y}=N^{\prime}\#_{i}\tilde{X}_{i}, where NN^{\prime} is a finite cyclic covering of NN obtained by cutting and pasting along Σ\Sigma and the X~i\tilde{X}_{i}’s are a finite number of closed manifolds.

  2. (ii)

    In a neighborhood of Λ1\Lambda_{1}, Y~\tilde{Y} has positive mm-intermediate curvature.

  3. (iii)

    p[Λ1]=[Σ]Hn1(N)p_{*}[\Lambda_{1}]=[\Sigma]\in H_{n-1}(N^{\prime}), where p:Y~Np:\tilde{Y}\to N^{\prime} is the projection map and [Σ][\Sigma] is the homology class represented by any copy of Σ\Sigma in NN^{\prime}.

  4. (iv)

    On Λ1\Lambda_{1}, we have

    HΛ1=h,H_{\Lambda_{1}}=h,
    RY~+ah22|DY~h|>0,R_{\tilde{Y}}+ah^{2}-2|D_{\tilde{Y}}h|>0,

    and

    𝒬(ψ)=Λ(|DΛ1ψ|2(|IIΛ1|2+RicY~(ν,ν)+DY~h,ν)ψ2)𝑑n10\mathcal{Q}(\psi)=\int_{\Lambda}\left(|D_{\Lambda_{1}}\psi|^{2}-\big{(}|{\rm II}_{\Lambda_{1}}|^{2}+\operatorname{Ric}_{\tilde{Y}}(\nu,\nu)+\langle D_{\tilde{Y}}h,\nu\rangle\big{)}\psi^{2}\right)d\mathcal{H}^{n-1}\geq 0

    for all ψC(Λ1)\psi\in C^{\infty}(\Lambda_{1}).

Let Λ0=Y~\Lambda_{0}=\tilde{Y}. Then Λ1Λ0=Y~\Lambda_{1}\subset\Lambda_{0}=\tilde{Y} gives a modified stable weighted slicing of order 11 with constant aa. If m=1m=1, we set a=1na=\frac{1}{n}. Then by Theorem 5.14, we must have (𝒞1)Y~0(\mathcal{C}_{1})_{\tilde{Y}}\leq 0 on some point of Σ1\Sigma_{1}, which contradicts condition (ii). This shows N#XN\#X cannot have positive 11-intermediate curvature.

Now assume m2m\geq 2. By condition (i), Y~\tilde{Y} admits a map G:Y~NG:\tilde{Y}\to N with some nonzero degree. By condition (iii) we find that G[Λ1]=[Σ]Hn1(N)G_{*}[\Lambda_{1}]=[\Sigma]\in H_{n-1}(N), so using naturality of the cup and cap products, we obtain

G([Λ1](Gω2GωmGΩ))\displaystyle G_{*}\big{(}[\Lambda_{1}]\frown(G^{*}\omega_{2}\smile\dots\smile G^{*}\omega_{m}\smile G^{*}\Omega)\big{)}
=G([Λ1]G(ω2ωmΩ))\displaystyle=G_{*}\big{(}[\Lambda_{1}]\frown G^{*}(\omega_{2}\smile\dots\smile\omega_{m}\smile\Omega)\big{)}
=G([Λ1]G(ω2ωmΩ))\displaystyle=G_{*}\big{(}[\Lambda_{1}]\frown G^{*}(\omega_{2}\smile\dots\smile\omega_{m}\smile\Omega)\big{)}
=G[Λ1](ω2ωmΩ)\displaystyle=G_{*}[\Lambda_{1}]\frown(\omega_{2}\smile\dots\smile\omega_{m}\smile\Omega)
=[Σ](ω2ωmΩ)\displaystyle=[\Sigma]\frown(\omega_{2}\smile\dots\smile\omega_{m}\smile\Omega)
=([N]ω1)(ω2ωmΩ)\displaystyle=([N]\frown\omega_{1})\frown(\omega_{2}\smile\dots\smile\omega_{m}\smile\Omega)
=[N](ω1ωmΩ)\displaystyle=[N]\frown(\omega_{1}\smile\dots\smile\omega_{m}\smile\Omega)
=d.\displaystyle=d.

This shows

Λ1Gω2GωmGΩ0.\displaystyle\int_{\Lambda_{1}}G^{*}{\omega}_{2}\wedge\dots\wedge G^{*}{\omega}_{m}\wedge G^{*}{\Omega}\neq 0.

Then for 2km2\leq k\leq m, one can inductively construct the slices Λk\Lambda_{k} and the weights ρk\rho_{k}, such that ΛkGωkGωmGΩ0\int_{\Lambda_{k}}G^{*}{\omega}_{k}\wedge\dots\wedge G^{*}{\omega}_{m}\wedge G^{*}{\Omega}\neq 0 holds. For this, we can use the same argument as in [SY17, Proof of Theorem 4.5] or [BHJ22, Proof of Theorem 1.5], where all the details are given.

We thus obtain a modified stable weighted slicing ΛmΛ1Λ0=Y~\Lambda_{m}\subset\dots\subset\Lambda_{1}\subset\Lambda_{0}=\tilde{Y} of order mm with constant aa. By our assumption on nn and mm, we have m2mn+2n2>0m^{2}-mn+2n-2>0 and m2mn+m+n>0m^{2}-mn+m+n>0 by Lemma 5.11. Choose aa so that 0<amin{m2(m1),1nm,m2mn+m+n2(m2mn+2n2)}0<a\leq\min\{\frac{m}{2(m-1)},\frac{1}{n-m},\frac{m^{2}-mn+m+n}{2(m^{2}-mn+2n-2)}\}. Then by Theorem 5.13, we must have (𝒞m)Y~0(\mathcal{C}_{m})_{\tilde{Y}}\leq 0 at some point on ΛmΛ1\Lambda_{m}\subset\Lambda_{1}. This contradicts condition (ii), which shows N#XN\#X cannot have positive mm-intermediate curvature and thereby completes the proof. \blacksquare

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