Mathematics Subject Classification (2020). 53C42; 35J60; 53C21.
Introduction
Let M M M be a hypersurface in the ( n + 1 ) (n+1) ( n + 1 ) -dimensional Euclidean space R n + 1 \mathbb{R}^{n+1} R n + 1 . Let κ ( X ) \kappa(X) κ ( X ) , H ( X ) H(X) H ( X ) , and ν ( X ) \nu(X) ν ( X ) denote the principal curvatures, mean curvature, and unit outward normal vector of M M M at X X X , respectively. Define the ( 0 , 2 ) (0,2) ( 0 , 2 ) -tensor
η i j = H g i j − h i j , \eta_{ij}=Hg_{ij}-h_{ij}, η ij = H g ij − h ij ,
where g i j g_{ij} g ij and h i j h_{ij} h ij are the coefficients of the first and second fundamental forms. The tensor η \eta η is the first Newton transformation of h h h with respect to g g g . If λ ( η ) = ( λ 1 , … , λ n ) \lambda(\eta)=(\lambda_1,\ldots,\lambda_n) λ ( η ) = ( λ 1 , … , λ n ) denotes the eigenvalues of η \eta η , then
λ i = H − κ i = ∑ j ≠ i κ j , i = 1 , … , n . \lambda_i=H-\kappa_i=\sum_{j\ne i}\kappa_j,\qquad i=1,\ldots,n. λ i = H − κ i = j = i ∑ κ j , i = 1 , … , n .
The classical prescribed curvature equation
σ k ( κ ( X ) ) = f ( X , ν ( X ) ) \sigma_k(\kappa(X))=f(X,\nu(X)) σ k ( κ ( X )) = f ( X , ν ( X ))
plays a fundamental role in fully nonlinear elliptic equations and geometric analysis. The cases k = 1 k=1 k = 1 , k = 2 k=2 k = 2 , and k = n k=n k = n correspond, up to the usual normalization, to the prescribed mean, scalar, and Gauss curvature equations. The classical theory of fully nonlinear Hessian equations and prescribed curvature problems on star-shaped hypersurfaces can be found in [1 , 2 ] . In a different but closely related direction, Chu and Jiao [3 ] studied the Hessian-type curvature equation
σ k ( λ ( η ) ) = f ( X , ν ( X ) ) \sigma_k(\lambda(\eta))=f(X,\nu(X)) σ k ( λ ( η )) = f ( X , ν ( X ))
for star-shaped hypersurfaces. They established a global curvature estimate under the natural condition λ ( η ) ∈ Γ k \lambda(\eta)\in\Gamma_k λ ( η ) ∈ Γ k and applied it to the corresponding prescribed curvature problem. Their proof combines a maximum-principle test function with a partial curvature estimate that provides the good third-order terms needed to control the derivatives of the right-hand side. Related global curvature estimates for convex hypersurfaces and prescribed curvature measure problems were established in [6 , 5 ] . The evolution of star-shaped hypersurfaces by symmetric functions of their principal curvatures was also studied in [15 ] .
Sum Hessian equations constitute another natural class of fully nonlinear equations. In Euclidean domains the model equation is
σ k ( D 2 u ) + α σ k − 1 ( D 2 u ) = f ( x , u , D u ) , α > 0. \sigma_k(D^2u)+\alpha\sigma_{k-1}(D^2u)=f(x,u,Du),\qquad\alpha>0. σ k ( D 2 u ) + α σ k − 1 ( D 2 u ) = f ( x , u , D u ) , α > 0.
The operator is a linear combination of two neighboring Hessian operators of different degrees and is therefore nonhomogeneous. Li, Ren, and Wang [9 ] identified the natural admissible region
Γ k − 1 ∩ { λ : σ k ( λ ) + α σ k − 1 ( λ ) > 0 } \Gamma_{k-1}\cap\{\lambda:\sigma_k(\lambda)+\alpha\sigma_{k-1}(\lambda)>0\} Γ k − 1 ∩ { λ : σ k ( λ ) + α σ k − 1 ( λ ) > 0 }
and studied curvature estimates for related linear combinations of elementary symmetric functions on convex hypersurfaces. Liu and Ren [12 ] obtained Pogorelov-type C 2 C^2 C 2 estimates for the standard sum Hessian equation. Liang, Yan, and Zhu [11 ] subsequently developed Pogorelov estimates and rigidity results for ( k − 1 ) (k-1) ( k − 1 ) -convex solutions under an additional semi-convexity assumption, stressing that the loss of homogeneity prevents a direct transfer of several arguments from the pure k k k -Hessian equation. Further developments include the Pogorelov estimates of Li and Ren [10 ] and the interior estimate of Ren and Sun [13 ] for a two-sum Hessian equation with a nonnegative variable coefficient α ( x ) ≥ 0 \alpha(x)\geq0 α ( x ) ≥ 0 satisfying the structural condition D 2 α = β I D^2\alpha=\beta I D 2 α = β I , under the additional assumption Δ u > 0 \Delta u>0 Δ u > 0 .
Of particular relevance to the present problem is the work of Ren and Wang [14 ] , who considered
σ k ( μ ) + α σ k − 1 ( μ ) = f ( x , u , D u ) , μ i = ∑ j ≠ i λ j ( D 2 u ) , \sigma_k(\mu)+\alpha\sigma_{k-1}(\mu)=f(x,u,Du),\qquad\mu_i=\sum_{j\ne i}\lambda_j(D^2u), σ k ( μ ) + α σ k − 1 ( μ ) = f ( x , u , D u ) , μ i = j = i ∑ λ j ( D 2 u ) ,
so that μ \mu μ is the spectrum of ( Δ u ) I − D 2 u (\Delta u)I-D^2u ( Δ u ) I − D 2 u . They established interior C 2 C^2 C 2 and Pogorelov-type estimates for 0 < k < n 0<k<n 0 < k < n , while the endpoint k = n k=n k = n requires a weaker estimate. This is algebraically the closest Euclidean-domain analogue of our operator. The geometric setting here is different: η = H g − h \eta=Hg-h η = H g − h is defined by the second fundamental form of a closed hypersurface, and the goal is a global curvature estimate rather than an interior Hessian estimate.
There are also recent geometric works on sum curvature equations formulated directly in the principal curvatures. For example, Yang and Lu [16 ] study complete hypersurfaces of constant sum Hessian curvature in hyperbolic space, with curvature function σ n − 1 ( κ ) + α σ n ( κ ) \sigma_{n-1}(\kappa)+\alpha\sigma_n(\kappa) σ n − 1 ( κ ) + α σ n ( κ ) . These problems, as well as the convex-hypersurface results of Li, Ren, and Wang [9 ] , are structurally distinct from applying the sum Hessian operator to the eigenvalues of the first Newton transformation H g − h Hg-h H g − h .
Motivated by the above developments and by the geometric framework of Chu and Jiao, we study the prescribed sum Hessian curvature equation associated with η \eta η . Fix a constant α > 0 \alpha>0 α > 0 . For 1 ≤ j ≤ n 1\le j\le n 1 ≤ j ≤ n , set
S j , α ( λ ) = σ j ( λ ) + α σ j − 1 ( λ ) , σ 0 ≡ 1. S_{j,\alpha}(\lambda)=\sigma_j(\lambda)+\alpha\sigma_{j-1}(\lambda),\qquad\sigma_0\equiv1. S j , α ( λ ) = σ j ( λ ) + α σ j − 1 ( λ ) , σ 0 ≡ 1.
Our equation is
S k , α ( λ ( η ) ) = σ k ( λ ( η ) ) + α σ k − 1 ( λ ( η ) ) = f ( X , ν ( X ) ) , X ∈ M . (1) S_{k,\alpha}(\lambda(\eta))=\sigma_k(\lambda(\eta))+\alpha\sigma_{k-1}(\lambda(\eta))=f(X,\nu(X)),\qquad X\in M. \tag*{(1)} S k , α ( λ ( η )) = σ k ( λ ( η )) + α σ k − 1 ( λ ( η )) = f ( X , ν ( X )) , X ∈ M . (1)
The natural admissible region is
Γ ~ k , α : = Γ k − 1 ∩ { λ ∈ R n : S k , α ( λ ) > 0 } , \widetilde{\Gamma}_{k,\alpha}:=\Gamma_{k-1}\cap\{\lambda\in\mathbb{R}^n:S_{k,\alpha}(\lambda)>0\}, Γ k , α := Γ k − 1 ∩ { λ ∈ R n : S k , α ( λ ) > 0 } ,
where
Γ j = { λ ∈ R n : σ 1 ( λ ) > 0 , … , σ j ( λ ) > 0 } . \Gamma_j=\{\lambda\in\mathbb{R}^n:\sigma_1(\lambda)>0,\ldots,\sigma_j(\lambda)>0\}. Γ j = { λ ∈ R n : σ 1 ( λ ) > 0 , … , σ j ( λ ) > 0 } .
A C 2 C^2 C 2 hypersurface is called ( η , k , α ) (\eta,k,\alpha) ( η , k , α ) -admissible if λ ( η ) ∈ Γ ~ k , α \lambda(\eta)\in\widetilde{\Gamma}_{k,\alpha} λ ( η ) ∈ Γ k , α everywhere on M M M .
The key structural observation is obtained by introducing the augmented vector
λ ^ = ( λ 1 , … , λ n , α ) ∈ R n + 1 . \widehat{\lambda}=(\lambda_1,\ldots,\lambda_n,\alpha)\in\mathbb{R}^{n+1}. λ = ( λ 1 , … , λ n , α ) ∈ R n + 1 .
Then
S j , α ( λ ) = σ j ( λ ^ ) . S_{j,\alpha}(\lambda)=\sigma_j(\widehat{\lambda}). S j , α ( λ ) = σ j ( λ ) .
Thus the nonhomogeneous sum Hessian operator is the restriction of the standard Hessian operator in one higher dimension to the affine hyperplane whose last coordinate equals α \alpha α . This recovers ellipticity and concavity from σ k 1 / k \sigma_k^{1/k} σ k 1/ k in one higher dimension. On the other hand, the loss of homogeneity changes the Euler identity and produces an additional lower-order term in the maximum-principle calculation. The main analytical task is to absorb this term using the partial curvature estimate.
To the best of our knowledge, a global curvature estimate and a corresponding prescribed-curvature existence theorem for (1) on closed star-shaped hypersurfaces under the natural ( η , k , α ) (\eta,k,\alpha) ( η , k , α ) -admissibility condition have not previously been established. Our first main result is the following.
Theorem 1.1. Let 2 ≤ k ≤ n − 1 2\le k\le n-1 2 ≤ k ≤ n − 1 and let α > 0 \alpha>0 α > 0 . Let M M M be a closed, star-shaped, ( η , k , α ) (\eta,k,\alpha) ( η , k , α ) -admissible hypersurface in R n + 1 \mathbb{R}^{n+1} R n + 1 satisfying (1), where f > 0 f>0 f > 0 and f ∈ C 2 ( U ) f\in C^2(\mathcal{U}) f ∈ C 2 ( U ) for an open neighborhood U \mathcal{U} U of the unit normal bundle of M M M in R n + 1 × S n \mathbb{R}^{n+1}\times\mathbb{S}^n R n + 1 × S n . Then
max X ∈ M max 1 ≤ i ≤ n ∣ κ i ( X ) ∣ ≤ C , \max_{X\in M}\max_{1\le i\le n}|\kappa_i(X)|\le C, X ∈ M max 1 ≤ i ≤ n max ∣ κ i ( X ) ∣ ≤ C , where
C = C ( n , k , α , ∥ M ∥ C 1 , inf f , ∥ f ∥ C 2 ) . C=C\left(n,k,\alpha,\|M\|_{C^1},\inf f,\|f\|_{C^2}\right). C = C ( n , k , α , ∥ M ∥ C 1 , inf f , ∥ f ∥ C 2 ) .
The restriction k ≤ n − 1 k \le n-1 k ≤ n − 1 enters in the partial curvature estimate in § 3 ; the endpoint k = n k=n k = n requires a different argument and is not treated here. The proof follows the maximum-principle strategy of Chu and Jiao, but the lower-order α σ k − 1 \alpha\sigma_{k-1} α σ k − 1 term changes the Euler identity and gives rise to an additional quantity R α R_\alpha R α . The principal new point in the estimate is to control this term without strengthening the natural admissibility condition.
We also prove an existence result. Put
Φ α ( r ) : = ( n k ) ( n − 1 ) k r k + α ( n k − 1 ) ( n − 1 ) k − 1 r k − 1 . (2) \Phi_\alpha(r) := \binom{n}{k}\frac{(n-1)^k}{r^k}+\alpha\binom{n}{k-1}\frac{(n-1)^{k-1}}{r^{k-1}}. \tag*{(2)} Φ α ( r ) := ( k n ) r k ( n − 1 ) k + α ( k − 1 n ) r k − 1 ( n − 1 ) k − 1 . (2)
This is the value of the left-hand side of (1) on the sphere of radius r r r . Since the sum Hessian operator is not homogeneous, the spherical barriers used for the pure k k k -Hessian case acquire the second term in (2) .
Theorem 1.2. Let 2 ≤ k ≤ n − 1 2 \le k \le n-1 2 ≤ k ≤ n − 1 , α > 0 \alpha> 0 α > 0 , and 0 < r 1 < 1 < r 2 0 < r_1 < 1 < r_2 0 < r 1 < 1 < r 2 . Let
f ∈ C 2 ( ( B ‾ r 2 ∖ B r 1 ) × S n ) f \in C^2\left((\overline{B}_{r_2}\setminus B_{r_1})\times\mathbb{S}^n\right) f ∈ C 2 ( ( B r 2 ∖ B r 1 ) × S n ) be positive and assume
f ( X , X ∣ X ∣ ) ≥ Φ α ( r 1 ) , ∣ X ∣ = r 1 , f ( X , X ∣ X ∣ ) ≤ Φ α ( r 2 ) , ∣ X ∣ = r 2 . (3) \begin{aligned}
f\left(X,\frac{X}{|X|}\right)&\ge\Phi_\alpha(r_1), \quad|X|=r_1,\\
f\left(X,\frac{X}{|X|}\right)&\le\Phi_\alpha(r_2), \quad|X|=r_2. \tag*{(3)}
\end{aligned} f ( X , ∣ X ∣ X ) f ( X , ∣ X ∣ X ) ≥ Φ α ( r 1 ) , ∣ X ∣ = r 1 , ≤ Φ α ( r 2 ) , ∣ X ∣ = r 2 . (3) Assume moreover that for every fixed x , ν ∈ S n x,\nu\in\mathbb{S}^n x , ν ∈ S n ,
∂ ∂ ρ [ ρ k f ( ρ x , ν ) ] ≤ 0 , r 1 ≤ ρ ≤ r 2 . (4) \frac{\partial}{\partial\rho}\left[\rho^k f(\rho x,\nu)\right]\le0,\quad r_1\le\rho\le r_2. \tag*{(4)} ∂ ρ ∂ [ ρ k f ( ρ x , ν ) ] ≤ 0 , r 1 ≤ ρ ≤ r 2 . (4) Then, for every 0 < β < 1 0<\beta<1 0 < β < 1 , equation (1) admits a unique C 3 , β C^{3,\beta} C 3 , β star-shaped ( η , k , α ) (\eta,k,\alpha) ( η , k , α ) -admissible solution satisfying r 1 ≤ ∣ X ∣ ≤ r 2 r_1\le|X|\le r_2 r 1 ≤ ∣ X ∣ ≤ r 2 .
When α = 0 \alpha=0 α = 0 , equation (1) formally reduces to the Hessian-type curvature equation of Chu and Jiao. For α > 0 \alpha>0 α > 0 , both the global curvature estimate and the existence argument must account for the nonhomogeneous lower-order Hessian term. In particular, the curvature estimate requires a separate control of R α R_\alpha R α , while the continuity method uses the modified spherical value (2).
The paper is organized as follows. § 2 records the structural properties of the sum Hessian operator. § 3 proves the global curvature estimate. § 4 establishes the a priori estimates and completes the existence and uniqueness proof by the continuity method.
Preliminaries
We first recall some basic definitions and properties of the elementary symmetric functions. For 1 ≤ k ≤ n 1\le k\le n 1 ≤ k ≤ n , the k k k -th elementary symmetric function is defined by
σ k ( λ ) = ∑ 1 ≤ i 1 < ⋯ < i k ≤ n λ i 1 ⋯ λ i k , \sigma_k(\lambda)=\sum_{1\le i_1<\cdots<i_k\le n}\lambda_{i_1}\cdots\lambda_{i_k}, σ k ( λ ) = 1 ≤ i 1 < ⋯ < i k ≤ n ∑ λ i 1 ⋯ λ i k ,
for λ = ( λ 1 , λ 2 , … , λ n ) ∈ R n \lambda=(\lambda_1,\lambda_2,\ldots,\lambda_n)\in\mathbb{R}^n λ = ( λ 1 , λ 2 , … , λ n ) ∈ R n . For convenience, we further set
σ 0 ( λ ) = 1 , σ k ( λ ) = 0 for k > n or k < 0. \sigma_0(\lambda)=1,\qquad\sigma_k(\lambda)=0\quad\text{for }k>n\text{ or }k<0. σ 0 ( λ ) = 1 , σ k ( λ ) = 0 for k > n or k < 0.
We next record the structural properties of the Hessian sum operator.
Lemma 2.1. Let α > 0 \alpha> 0 α > 0 and let λ ^ = ( λ , α ) ∈ R n + 1 \widehat{\lambda} = (\lambda,\alpha) \in\mathbb{R}^{n+1} λ = ( λ , α ) ∈ R n + 1 . Then
S j , α ( λ ) = σ j ( λ ^ ) , 1 ≤ j ≤ n . S_{j,\alpha}(\lambda) = \sigma_j(\widehat{\lambda}), \qquad1 \le j \le n. S j , α ( λ ) = σ j ( λ ) , 1 ≤ j ≤ n . Moreover,
λ ∈ Γ ~ k , α ⟺ λ ^ ∈ Γ k n + 1 . \lambda\in\widetilde{\Gamma}_{k,\alpha} \Longleftrightarrow\widehat{\lambda} \in\Gamma_k^{n+1}. λ ∈ Γ k , α ⟺ λ ∈ Γ k n + 1 . Consequently, Γ ~ k , α \widetilde{\Gamma}_{k,\alpha} Γ k , α is open and convex, and
G ( λ ) : = S k , α ( λ ) 1 / k G(\lambda) := S_{k,\alpha}(\lambda)^{1/k} G ( λ ) := S k , α ( λ ) 1/ k is elliptic and concave on Γ ~ k , α \widetilde{\Gamma}_{k,\alpha} Γ k , α .
Proof. The identity
σ j ( λ 1 , … , λ n , α ) = σ j ( λ ) + α σ j − 1 ( λ ) \sigma_j(\lambda_1,\ldots,\lambda_n,\alpha) = \sigma_j(\lambda) + \alpha\sigma_{j-1}(\lambda) σ j ( λ 1 , … , λ n , α ) = σ j ( λ ) + α σ j − 1 ( λ )
is immediate from the definition of the elementary symmetric functions. If λ ∈ Γ ~ k , α \lambda\in\widetilde{\Gamma}_{k,\alpha} λ ∈ Γ k , α , then for 1 ≤ j ≤ k − 1 1 \le j \le k-1 1 ≤ j ≤ k − 1 ,
σ j ( λ ^ ) = σ j ( λ ) + α σ j − 1 ( λ ) > 0 , \sigma_j(\widehat{\lambda}) = \sigma_j(\lambda) + \alpha\sigma_{j-1}(\lambda) > 0, σ j ( λ ) = σ j ( λ ) + α σ j − 1 ( λ ) > 0 ,
and σ k ( λ ^ ) = S k , α ( λ ) > 0 \sigma_k(\widehat{\lambda}) = S_{k,\alpha}(\lambda) > 0 σ k ( λ ) = S k , α ( λ ) > 0 . Hence λ ^ ∈ Γ k n + 1 \widehat{\lambda} \in\Gamma_k^{n+1} λ ∈ Γ k n + 1 . Conversely, if λ ^ ∈ Γ k n + 1 \widehat{\lambda} \in\Gamma_k^{n+1} λ ∈ Γ k n + 1 , then for 1 ≤ j ≤ k − 1 1 \le j \le k-1 1 ≤ j ≤ k − 1 the standard ellipticity of σ j + 1 \sigma_{j+1} σ j + 1 on Γ j + 1 \Gamma_{j+1} Γ j + 1 gives
σ j ( λ ) = ∂ σ j + 1 ( λ ^ ) ∂ λ ^ n + 1 > 0. \sigma_j(\lambda) = \frac{\partial\sigma_{j+1}(\widehat{\lambda})}{\partial\widehat{\lambda}_{n+1}} > 0. σ j ( λ ) = ∂ λ n + 1 ∂ σ j + 1 ( λ ) > 0.
Thus λ ∈ Γ k − 1 \lambda\in\Gamma_{k-1} λ ∈ Γ k − 1 , while S k , α ( λ ) = σ k ( λ ^ ) > 0 S_{k,\alpha}(\lambda) = \sigma_k(\widehat{\lambda}) > 0 S k , α ( λ ) = σ k ( λ ) > 0 . The convexity statement follows by intersecting the convex cone Γ k n + 1 \Gamma_k^{n+1} Γ k n + 1 with the affine hyperplane λ ^ n + 1 = α \widehat{\lambda}_{n+1} = \alpha λ n + 1 = α . Finally, G ( λ ) = σ k ( λ ^ ) 1 / k G(\lambda) = \sigma_k(\widehat{\lambda})^{1/k} G ( λ ) = σ k ( λ ) 1/ k , so ellipticity and concavity follow from the corresponding standard properties of σ k 1 / k \sigma_k^{1/k} σ k 1/ k on Γ k \Gamma_k Γ k [1 ] .
For later use, if λ \lambda λ is diagonal, write
S k i i = ∂ S k , α ∂ λ i , G i i = ∂ G ∂ λ i . S_k^{ii} = \frac{\partial S_{k,\alpha}}{\partial\lambda_i}, \qquad G^{ii} = \frac{\partial G}{\partial\lambda_i}. S k ii = ∂ λ i ∂ S k , α , G ii = ∂ λ i ∂ G .
Then
S k i i = σ k − 1 ( λ ∣ i ) + α σ k − 2 ( λ ∣ i ) , S_k^{ii} = \sigma_{k-1}(\lambda|i) + \alpha\sigma_{k-2}(\lambda|i), S k ii = σ k − 1 ( λ ∣ i ) + α σ k − 2 ( λ ∣ i ) ,
∑ i S k i i = ( n − k + 1 ) σ k − 1 ( λ ) + α ( n − k + 2 ) σ k − 2 ( λ ) (5) \sum_i S_k^{ii} = (n-k+1)\sigma_{k-1}(\lambda) + \alpha(n-k+2)\sigma_{k-2}(\lambda) \tag*{(5)} i ∑ S k ii = ( n − k + 1 ) σ k − 1 ( λ ) + α ( n − k + 2 ) σ k − 2 ( λ ) (5)
and
∑ i λ i S k i i = k S k , α ( λ ) − α σ k − 1 ( λ ) . \sum_i \lambda_i S_k^{ii} = kS_{k,\alpha}(\lambda) - \alpha\sigma_{k-1}(\lambda). i ∑ λ i S k ii = k S k , α ( λ ) − α σ k − 1 ( λ ) .
Thus, on a solution of (1) , if
f ~ = f 1 / k , R α : = α k f 1 / k − 1 σ k − 1 ( λ ) (6) \widetilde{f} = f^{1/k}, \qquad R_\alpha:= \frac{\alpha}{k}f^{1/k-1}\sigma_{k-1}(\lambda) \tag*{(6)} f = f 1/ k , R α := k α f 1/ k − 1 σ k − 1 ( λ ) (6)
then
∑ i G i i λ i = f ~ − R α . \sum_i G^{ii}\lambda_i = \widetilde{f} - R_\alpha. i ∑ G ii λ i = f − R α .
For F ( κ ) = G ( η ( κ ) ) F(\kappa)=G(\eta(\kappa)) F ( κ ) = G ( η ( κ )) , at a fixed point, choose a local orthonormal frame such that g i j = δ i j g_{ij}=\delta_{ij} g ij = δ ij , h i j = κ i δ i j h_{ij}=\kappa_i\delta_{ij} h ij = κ i δ ij , then
F i i = ∂ F ∂ κ i = ∑ p ≠ i G p p . (7) F^{ii}=\frac{\partial F}{\partial\kappa_i}=\sum_{p\ne i}G^{pp}. \tag*{(7)} F ii = ∂ κ i ∂ F = p = i ∑ G pp . (7)
Consequently,
∑ i F i i h i i = ∑ i G i i η i i = f ~ − R α . (8) \sum_i F^{ii}h_{ii}=\sum_i G^{ii}\eta_{ii}=\widetilde f-R_\alpha. \tag*{(8)} i ∑ F ii h ii = i ∑ G ii η ii = f − R α . (8)
Lemma 2.2. For λ ∈ Γ ~ k , α \lambda\in\widetilde{\Gamma}_{k,\alpha} λ ∈ Γ k , α ,
∑ i F i i ≥ c n , k > 0 , (9) \sum_i F^{ii}\ge c_{n,k}>0, \tag*{(9)} i ∑ F ii ≥ c n , k > 0 , (9) and
0 ≤ R α ≤ α ( n − 1 ) ( n − k + 1 ) ∑ i F i i . (10) 0\le R_\alpha\le\frac{\alpha}{(n-1)(n-k+1)}\sum_i F^{ii}. \tag*{(10)} 0 ≤ R α ≤ ( n − 1 ) ( n − k + 1 ) α i ∑ F ii . (10)
Proof. By (7) and (5) ,
∑ i F i i = ( n − 1 ) ∑ i G i i = n − 1 k f 1 / k − 1 [ ( n − k + 1 ) σ k − 1 ( λ ) + α ( n − k + 2 ) σ k − 2 ( λ ) ] ≥ ( n − 1 ) ( n − k + 1 ) k f 1 / k − 1 σ k − 1 ( λ ^ ) . \begin{aligned}
\sum_i F^{ii}&=(n-1)\sum_i G^{ii}\\
&=\frac{n-1}{k}f^{1/k-1}\left[(n-k+1)\sigma_{k-1}(\lambda)+\alpha(n-k+2)\sigma_{k-2}(\lambda)\right]\\
&\ge\frac{(n-1)(n-k+1)}{k}f^{1/k-1}\sigma_{k-1}(\widehat{\lambda}).
\end{aligned} i ∑ F ii = ( n − 1 ) i ∑ G ii = k n − 1 f 1/ k − 1 [ ( n − k + 1 ) σ k − 1 ( λ ) + α ( n − k + 2 ) σ k − 2 ( λ ) ] ≥ k ( n − 1 ) ( n − k + 1 ) f 1/ k − 1 σ k − 1 ( λ ) .
Since λ ^ ∈ Γ k n + 1 \widehat{\lambda}\in\Gamma_k^{n+1} λ ∈ Γ k n + 1 , the Newton–Maclaurin inequality gives
σ k − 1 ( λ ^ ) ≥ c n , k f ( k − 1 ) / k , \sigma_{k-1}(\widehat{\lambda})\ge c_{n,k}f^{(k-1)/k}, σ k − 1 ( λ ) ≥ c n , k f ( k − 1 ) / k ,
which proves (9). Formula (10) follows immediately by comparing (6) with the displayed formula for ∑ i F i i \sum_i F^{ii} ∑ i F ii . □
We now recall the standard geometric formulas for star-shaped radial graphs that will be used in the sequel.
Let M M M be the radial graph of a positive function ρ \rho ρ on S n \mathbb{S}^n S n ,
X ( x ) = ρ ( x ) x , x ∈ S n . X(x)=\rho(x)x,\qquad x\in\mathbb{S}^n. X ( x ) = ρ ( x ) x , x ∈ S n .
If g ^ \widehat g g and ∇ \nabla ∇ denote the standard metric and covariant derivative on S n \mathbb{S}^n S n , then
g i j = ρ 2 g ^ i j + ρ i ρ j , h i j = ρ 2 g ^ i j + 2 ρ i ρ j − ρ ρ i j ρ 2 + ∣ ∇ ρ ∣ 2 . (11) g_{ij}=\rho^2\widehat g_{ij}+\rho_i\rho_j,\qquad
h_{ij}=\frac{\rho^2\widehat g_{ij}+2\rho_i\rho_j-\rho\rho_{ij}}{\sqrt{\rho^2+|\nabla\rho|^2}}. \tag*{(11)} g ij = ρ 2 g ij + ρ i ρ j , h ij = ρ 2 + ∣∇ ρ ∣ 2 ρ 2 g ij + 2 ρ i ρ j − ρ ρ ij . (11)
and
ν = ρ x − ∇ ρ ρ 2 + ∣ ∇ ρ ∣ 2 . \nu=\frac{\rho x-\nabla\rho}{\sqrt{\rho^2+|\nabla\rho|^2}}. ν = ρ 2 + ∣∇ ρ ∣ 2 ρ x − ∇ ρ .
In particular, with
u = ⟨ X , ν ⟩ , u=\langle X,\nu\rangle, u = ⟨ X , ν ⟩ ,
we have
u = ρ 2 ρ 2 + ∣ ∇ ρ ∣ 2 . (12) u=\frac{\rho^2}{\sqrt{\rho^2+|\nabla\rho|^2}}. \tag*{(12)} u = ρ 2 + ∣∇ ρ ∣ 2 ρ 2 . (12)
Fix X 0 ∈ M X_0 \in M X 0 ∈ M and let { e 1 , … , e n } \{e_1,\ldots,e_n\} { e 1 , … , e n } be a local orthonormal frame near X 0 X_0 X 0 . With the sign convention used throughout the paper,
X i j = − h i j ν , ν i = h i j e j (13) \begin{aligned}
X_{ij} &= -h_{ij}\nu,\\
\nu_i &= h_{ij}e_j \tag*{(13)}
\end{aligned} X ij ν i = − h ij ν , = h ij e j (13)
h i j k = h i k j , R i j k l = h i k h j l − h i l h j k . (14) \begin{aligned}
h_{ijk} &= h_{ikj},\\
R_{ijkl} &= h_{ik}h_{jl}-h_{il}h_{jk}. \tag*{(14)}
\end{aligned} h ij k R ij k l = h ik j , = h ik h j l − h i l h j k . (14)
We shall also use
h i j k l = h k l i j + ( h m j h i l − h m l h i j ) h m k + ( h m j h k l − h m l h k j ) h m i . (15) h_{ijkl}=h_{klij}+(h_{mj}h_{il}-h_{ml}h_{ij})h_{mk}+(h_{mj}h_{kl}-h_{ml}h_{kj})h_{mi}. \tag*{(15)} h ij k l = h k l ij + ( h mj h i l − h m l h ij ) h mk + ( h mj h k l − h m l h k j ) h mi . (15)
Curvature estimate
We prove Theorem 1.1. Since λ ( η ) ∈ Γ k − 1 ⊂ Γ 1 \lambda(\eta)\in\Gamma_{k-1}\subset\Gamma_1 λ ( η ) ∈ Γ k − 1 ⊂ Γ 1 ,
0 < σ 1 ( λ ( η ) ) = ( n − 1 ) H , 0<\sigma_1(\lambda(\eta))=(n-1)H, 0 < σ 1 ( λ ( η )) = ( n − 1 ) H ,
so H > 0 H>0 H > 0 . It is therefore enough to obtain a uniform upper bound for the largest principal curvature κ max \kappa_{\max} κ m a x .
By (12) there is a constant C C C , depending only on the C 1 C^1 C 1 geometry of the radial graph, such that
C − 1 ≤ u ≤ C . (16) C^{-1}\leq u\leq C. \tag*{(16)} C − 1 ≤ u ≤ C . (16)
Set
a = 1 2 inf M u > 0. a=\frac{1}{2}\inf_M u>0. a = 2 1 M inf u > 0.
On the set D = { κ max > 0 } D=\{\kappa_{\max}>0\} D = { κ m a x > 0 } consider
Q = log κ max − log ( u − a ) + A 2 ∣ X ∣ 2 , Q=\log\kappa_{\max}-\log(u-a)+\frac{A}{2}|X|^2, Q = log κ m a x − log ( u − a ) + 2 A ∣ X ∣ 2 ,
where A > 1 A>1 A > 1 will be fixed later. The function Q Q Q tends to − ∞ -\infty − ∞ at ∂ D \partial D ∂ D and hence attains its maximum at some X 0 ∈ D X_0\in D X 0 ∈ D . Choose a local orthonormal frame near X 0 X_0 X 0 such that
h i j = δ i j h i i , h 11 ≥ h 22 ≥ ⋯ ≥ h n n h_{ij}=\delta_{ij}h_{ii},\qquad h_{11}\geq h_{22}\geq\cdots\geq h_{nn} h ij = δ ij h ii , h 11 ≥ h 22 ≥ ⋯ ≥ h nn
at X 0 X_0 X 0 . Then
η 11 ≤ η 22 ≤ ⋯ ≤ η n n . \eta_{11}\leq\eta_{22}\leq\cdots\leq\eta_{nn}. η 11 ≤ η 22 ≤ ⋯ ≤ η nn .
If κ max ( X 0 ) \kappa_{\max}(X_0) κ m a x ( X 0 ) has multiplicity, we use the standard Calabi perturbation of the second fundamental form so that the largest eigenvalue becomes simple at X 0 X_0 X 0 . The perturbation may be chosen arbitrarily small; all estimates below are uniform in the perturbation parameter, and we let that parameter tend to zero at the end. Thus, without loss of generality for the maximum-principle calculation, we may work with the smooth eigenvalue branch h 11 h_{11} h 11 near X 0 X_0 X 0 and set
Q ^ = log h 11 − log ( u − a ) + A 2 ∣ X ∣ 2 . \widehat{Q}=\log h_{11}-\log(u-a)+\frac{A}{2}|X|^2. Q = log h 11 − log ( u − a ) + 2 A ∣ X ∣ 2 .
It has a local maximum at X 0 X_0 X 0 . From now on all computations are at X 0 X_0 X 0 .
Since G G G is symmetric, elliptic, and concave, the ordering above gives
G 11 ≥ G 22 ≥ ⋯ ≥ G n n , F 11 ≤ F 22 ≤ ⋯ ≤ F n n . G^{11} \ge G^{22} \ge\cdots\ge G^{nn}, \qquad F^{11} \le F^{22} \le\cdots\le F^{nn}. G 11 ≥ G 22 ≥ ⋯ ≥ G nn , F 11 ≤ F 22 ≤ ⋯ ≤ F nn .
The first- and second-derivative conditions are
0 = Q ^ i = h 11 i h 11 − u i u − a + A ⟨ X , e i ⟩ , (17) 0 = \widehat{Q}_i = \frac{h_{11i}}{h_{11}} - \frac{u_i}{u-a} + A\langle X,e_i\rangle, \tag*{(17)} 0 = Q i = h 11 h 11 i − u − a u i + A ⟨ X , e i ⟩ , (17)
and
0 ≥ F i i Q ^ i i = F i i ( log h 11 ) i i − F i i ( log ( u − a ) ) i i + A 2 F i i ( ∣ X ∣ 2 ) i i . (18) 0 \ge F^{ii}\widehat{Q}_{ii} = F^{ii}(\log h_{11})_{ii} - F^{ii}(\log(u-a))_{ii} + \frac{A}{2}F^{ii}(|X|^2)_{ii}. \tag*{(18)} 0 ≥ F ii Q ii = F ii ( log h 11 ) ii − F ii ( log ( u − a ) ) ii + 2 A F ii ( ∣ X ∣ 2 ) ii . (18)
Lemma 3.1. At X 0 X_0 X 0 , if h 11 ≥ 1 h_{11} \ge1 h 11 ≥ 1 , then
0 ≥ − 2 h 11 ∑ i ≥ 2 G 1 i , 1 i h 11 i 2 − F i i h 11 i 2 h 11 2 + a u − a F i i h i i 2 + F i i u i 2 ( u − a ) 2 − ( C + R α ) h 11 + A ∑ i F i i − C A . (19) \begin{aligned}
0 \ge{}&-\frac{2}{h_{11}}\sum_{i\ge2}G^{1i,1i}h_{11i}^{2}
-\frac{F^{ii}h_{11i}^{2}}{h_{11}^{2}}
+\frac{a}{u-a}F^{ii}h_{ii}^{2}
+\frac{F^{ii}u_i^{2}}{(u-a)^{2}}\\
&-(C+R_\alpha)h_{11}+A\sum_iF^{ii}-CA. \tag*{(19)}
\end{aligned} 0 ≥ − h 11 2 i ≥ 2 ∑ G 1 i , 1 i h 11 i 2 − h 11 2 F ii h 11 i 2 + u − a a F ii h ii 2 + ( u − a ) 2 F ii u i 2 − ( C + R α ) h 11 + A i ∑ F ii − C A . (19)
Proof. From (13), (8),
A 2 F i i ( ∣ X ∣ 2 ) i i = A ∑ i F i i ( 1 − h i i u ) = A ∑ i F i i − A u f ~ + A u R α . (20) \begin{aligned}
\frac{A}{2}F^{ii}(|X|^2)_{ii}
=A\sum_iF^{ii}(1-h_{ii}u) \\
&=A\sum_iF^{ii}-Au\widetilde f+AuR_\alpha. \tag*{(20)}
\end{aligned} 2 A F ii ( ∣ X ∣ 2 ) ii = A i ∑ F ii ( 1 − h ii u ) = A i ∑ F ii − A u f + A u R α . (20)
Moreover, by (13)–(14),
u i = h i i ⟨ X , e i ⟩ , u i i = ∑ k h i i k ⟨ X , e k ⟩ − u h i i 2 + h i i . (21) u_i=h_{ii}\langle X,e_i\rangle,\qquad
u_{ii}=\sum_k h_{iik}\langle X,e_k\rangle-uh_{ii}^{2}+h_{ii}. \tag*{(21)} u i = h ii ⟨ X , e i ⟩ , u ii = k ∑ h iik ⟨ X , e k ⟩ − u h ii 2 + h ii . (21)
Thus
− F i i ( log ( u − a ) ) i i = − 1 u − a ∑ k F i i h i i k ⟨ X , e k ⟩ + u u − a F i i h i i 2 -F^{ii}(\log(u-a))_{ii}
=-\frac{1}{u-a}\sum_kF^{ii}h_{iik}\langle X,e_k\rangle
+\frac{u}{u-a}F^{ii}h_{ii}^{2} − F ii ( log ( u − a ) ) ii = − u − a 1 k ∑ F ii h iik ⟨ X , e k ⟩ + u − a u F ii h ii 2
− f ~ − R α u − a + F i i u i 2 ( u − a ) 2 . (22) -\frac{\widetilde f-R_\alpha}{u-a}
+\frac{F^{ii}u_i^{2}}{(u-a)^{2}}. \tag*{(22)} − u − a f − R α + ( u − a ) 2 F ii u i 2 . (22)
Since η i i , k = H k − h i i , k \eta_{ii,k}=H_k-h_{ii,k} η ii , k = H k − h ii , k and (7) holds,
F i i h i i , k = G i i η i i , k . F^{ii}h_{ii,k}=G^{ii}\eta_{ii,k}. F ii h ii , k = G ii η ii , k .
Differentiating G ( η ) = f ~ G(\eta)=\widetilde f G ( η ) = f in the direction e k e_k e k gives
G i i η i i , k = f ~ k . G^{ii}\eta_{ii,k}=\widetilde f_k. G ii η ii , k = f k .
At the diagonal point X 0 X_0 X 0 , ν k = h k k e k \nu_k=h_{kk}e_k ν k = h k k e k , and the chain rule for f ~ = f ~ ( X , ν ) \widetilde f=\widetilde f(X,\nu) f = f ( X , ν ) therefore yields
f ~ k = ( d X f ~ ) ( e k ) + h k k ( d ν f ~ ) ( e k ) . \widetilde f_k=(d_X\widetilde f)(e_k)+h_{kk}(d_\nu\widetilde f)(e_k). f k = ( d X f ) ( e k ) + h k k ( d ν f ) ( e k ) .
On the other hand,
∑ i F i i h i i , k = ∑ i ∑ p ≠ i G p p h i i , k = ∑ p G p p ( H k − h p p , k ) = ∑ p G p p η p p , k . \sum_iF^{ii}h_{ii,k}
=\sum_i\sum_{p\ne i}G^{pp}h_{ii,k}
=\sum_pG^{pp}(H_k-h_{pp,k})
=\sum_pG^{pp}\eta_{pp,k}. i ∑ F ii h ii , k = i ∑ p = i ∑ G pp h ii , k = p ∑ G pp ( H k − h pp , k ) = p ∑ G pp η pp , k .
Hence
F i i h i i , k = ( d X f ~ ) ( e k ) + h k k ( d ν f ~ ) ( e k ) . (23) F^{ii}h_{ii,k}=(d_X\widetilde{f})(e_k)+h_{kk}(d_\nu\widetilde{f})(e_k). \tag*{(23)} F ii h ii , k = ( d X f ) ( e k ) + h k k ( d ν f ) ( e k ) . (23)
Indeed, by (23),
− 1 u − a ∑ k F i i h i i , k ⟨ X , e k ⟩ = − 1 u − a ∑ k h k k ( d ν f ~ ) ( e k ) ⟨ X , e k ⟩ − 1 u − a ( d X f ~ ) ( X T ) , -\frac{1}{u-a}\sum_k F^{ii}h_{ii,k}\langle X,e_k\rangle
=-\frac{1}{u-a}\sum_k h_{kk}(d_\nu\widetilde{f})(e_k)\langle X,e_k\rangle
-\frac{1}{u-a}(d_X\widetilde{f})(X^T), − u − a 1 k ∑ F ii h ii , k ⟨ X , e k ⟩ = − u − a 1 k ∑ h k k ( d ν f ) ( e k ) ⟨ X , e k ⟩ − u − a 1 ( d X f ) ( X T ) ,
where X T = ∑ k ⟨ X , e k ⟩ e k X^T=\sum_k\langle X,e_k\rangle e_k X T = ∑ k ⟨ X , e k ⟩ e k . Moreover, ∣ X T ∣ ≤ ∣ X ∣ ≤ C |X^T|\leq|X|\leq C ∣ X T ∣ ≤ ∣ X ∣ ≤ C , u − a ≥ a > 0 u-a\geq a>0 u − a ≥ a > 0 , and ∣ d X f ~ ∣ ≤ C |d_X\widetilde{f}|\leq C ∣ d X f ∣ ≤ C , because d X f ~ = 1 k f 1 / k − 1 d X f d_X\widetilde{f}=\frac{1}{k}f^{1/k-1}d_Xf d X f = k 1 f 1/ k − 1 d X f , inf f > 0 \inf f>0 inf f > 0 , and ∥ f ∥ C 1 ≤ C \|f\|_{C^1}\leq C ∥ f ∥ C 1 ≤ C . Hence
− 1 u − a ∑ k F i i h i i , k ⟨ X , e k ⟩ ≥ − 1 u − a ∑ k h k k ( d ν f ~ ) ( e k ) ⟨ X , e k ⟩ − C . -\frac{1}{u-a}\sum_k F^{ii}h_{ii,k}\langle X,e_k\rangle
\geq-\frac{1}{u-a}\sum_k h_{kk}(d_\nu\widetilde{f})(e_k)\langle X,e_k\rangle-C. − u − a 1 k ∑ F ii h ii , k ⟨ X , e k ⟩ ≥ − u − a 1 k ∑ h k k ( d ν f ) ( e k ) ⟨ X , e k ⟩ − C .
Using (8), we therefore obtain
− F i i ( log ( u − a ) ) i i ≥ − 1 u − a ∑ k h k k ( d ν f ~ ) ( e k ) ⟨ X , e k ⟩ + u u − a F i i h i i 2 + R α u − a + F i i u i 2 ( u − a ) 2 − C . (24) -F^{ii}(\log(u-a))_{ii}
\geq-\frac{1}{u-a}\sum_k h_{kk}(d_\nu\widetilde{f})(e_k)\langle X,e_k\rangle
+\frac{u}{u-a}F^{ii}h_{ii}^{2}
+\frac{R_\alpha}{u-a}
+\frac{F^{ii}u_i^2}{(u-a)^2}-C. \tag*{(24)} − F ii ( log ( u − a ) ) ii ≥ − u − a 1 k ∑ h k k ( d ν f ) ( e k ) ⟨ X , e k ⟩ + u − a u F ii h ii 2 + u − a R α + ( u − a ) 2 F ii u i 2 − C . (24)
For the first term in (18),
F i i ( log h 11 ) i i = F i i h 11 i i h 11 − F i i h 11 i 2 h 11 2 . (25) F^{ii}(\log h_{11})_{ii}
=\frac{F^{ii}h_{11ii}}{h_{11}}-\frac{F^{ii}h_{11i}^{2}}{h_{11}^{2}}. \tag*{(25)} F ii ( log h 11 ) ii = h 11 F ii h 11 ii − h 11 2 F ii h 11 i 2 . (25)
The commutation identity (15) and (8) yield
F i i h 11 i i = F i i h i i 11 − F i i h i i 2 h 11 + ( f ~ − R α ) h 11 2 . (26) F^{ii}h_{11ii}=F^{ii}h_{ii11}-F^{ii}h_{ii}^{2}h_{11}+(\widetilde{f}-R_\alpha)h_{11}^{2}. \tag*{(26)} F ii h 11 ii = F ii h ii 11 − F ii h ii 2 h 11 + ( f − R α ) h 11 2 . (26)
Differentiating G ( η ) = f ~ G(\eta)=\widetilde{f} G ( η ) = f twice in the e 1 e_1 e 1 direction gives
F i i h i i 11 = − G i j , k l η i j , 1 η k l , 1 + f ~ 11 . F^{ii}h_{ii11}=-G^{ij,kl}\eta_{ij,1}\eta_{kl,1}+\widetilde{f}_{11}. F ii h ii 11 = − G ij , k l η ij , 1 η k l , 1 + f 11 .
We next make the estimate for f ~ 11 \widetilde{f}_{11} f 11 explicit. Extend f f f smoothly in the normal variable to a neighborhood of S n \mathbb{S}^{n} S n ; all derivatives of this extension are controlled by the given C 2 C^2 C 2 norm. At X 0 X_0 X 0 the frame is geodesic and h h h is diagonal. Applying the chain rule twice to f ~ ( X , ν ) \widetilde{f}(X,\nu) f ( X , ν ) produces a term
∑ k h k 11 ( d ν f ~ ) ( e k ) \sum_k h_{k11}(d_\nu\widetilde{f})(e_k) k ∑ h k 11 ( d ν f ) ( e k )
from the tangential part of ν 11 \nu_{11} ν 11 . Every remaining term contains either a bounded first or second derivative of f f f , or at most two factors of h 1 j h_{1j} h 1 j . Since h 1 j = 0 h_{1j}=0 h 1 j = 0 for j ≠ 1 j\neq1 j = 1 at X 0 X_0 X 0 , those remaining terms are bounded below by − C ( 1 + h 11 2 ) -C(1+h_{11}^{2}) − C ( 1 + h 11 2 ) . Thus
F i i h i i 11 ≥ − G i j , k l η i j , 1 η k l , 1 + ∑ k h k 11 ( d ν f ~ ) ( e k ) − C h 11 2 − C . (27) F^{ii}h_{ii11}\geq-G^{ij,kl}\eta_{ij,1}\eta_{kl,1}+\sum_k h_{k11}(d_\nu\widetilde{f})(e_k)-Ch_{11}^{2}-C. \tag*{(27)} F ii h ii 11 ≥ − G ij , k l η ij , 1 η k l , 1 + k ∑ h k 11 ( d ν f ) ( e k ) − C h 11 2 − C . (27)
For completeness, at a diagonal matrix the standard second-derivative formula for a symmetric spectral function gives
G i j , k l ξ i j ξ k l = ∑ p , q G p p , q q ξ p p ξ q q + 2 ∑ p < q G p p − G q q η p p − η q q ξ p q 2 . G^{ij,kl}\xi_{ij}\xi_{kl}=\sum_{p,q}G^{pp,qq}\xi_{pp}\xi_{qq}+2\sum_{p<q}\frac{G^{pp}-G^{qq}}{\eta_{pp}-\eta_{qq}}\xi_{pq}^{2}. G ij , k l ξ ij ξ k l = p , q ∑ G pp , q q ξ pp ξ q q + 2 p < q ∑ η pp − η q q G pp − G q q ξ pq 2 .
with the quotient understood by continuity when two eigenvalues coincide. Concavity makes the whole quadratic form nonpositive and, since η 11 ≤ η i i \eta_{11}\leq\eta_{ii} η 11 ≤ η ii and G 11 ≥ G i i G^{11}\geq G^{ii} G 11 ≥ G ii , one has G 1 i , i 1 ≤ 0 G^{1i,i1}\leq0 G 1 i , i 1 ≤ 0 . Keeping only the off-diagonal terms involving index 1, and using
η 1 i , 1 = − h 1 i , 1 = − h 11 i \eta_{1i,1}=-h_{1i,1}=-h_{11i} η 1 i , 1 = − h 1 i , 1 = − h 11 i
by Codazzi, we obtain
− G i j , k l η i j , 1 η k l , 1 ≥ − 2 ∑ i ≥ 2 G 1 i , i 1 h 11 i 2 . (28) -G^{ij,kl}\eta_{ij,1}\eta_{kl,1}\geq-2\sum_{i\geq2}G^{1i,i1}h_{11i}^{2}. \tag*{(28)} − G ij , k l η ij , 1 η k l , 1 ≥ − 2 i ≥ 2 ∑ G 1 i , i 1 h 11 i 2 . (28)
Substituting (27) –(28) into (26) and then (25) gives
F i i ( log h 11 ) i i ≥ − 2 h 11 ∑ i ≥ 2 G 1 i , i 1 h 11 i 2 − F i i h 11 i 2 h 11 2 − F i i h i i 2 + 1 h 11 ∑ k h k 11 ( d ν f ~ ) ( e k ) − ( C + R α ) h 11 . (29) F^{ii}(\log h_{11})_{ii}\geq-\frac{2}{h_{11}}\sum_{i\geq2}G^{1i,i1}h_{11i}^{2}-\frac{F^{ii}h_{11i}^{2}}{h_{11}^{2}}-F^{ii}h_{ii}^{2}
+\frac{1}{h_{11}}\sum_k h_{k11}(d_\nu\widetilde f)(e_k)-(C+R_\alpha)h_{11}. \tag*{(29)} F ii ( log h 11 ) ii ≥ − h 11 2 i ≥ 2 ∑ G 1 i , i 1 h 11 i 2 − h 11 2 F ii h 11 i 2 − F ii h ii 2 + h 11 1 k ∑ h k 11 ( d ν f ) ( e k ) − ( C + R α ) h 11 . (29)
The two d ν f ~ d_\nu\widetilde f d ν f terms in (24) and (29) actually cancel up to the harmless A A A -term. Indeed, Codazzi gives h k 11 = h 11 k h_{k11}=h_{11k} h k 11 = h 11 k , while (17) and u k = h k k ⟨ X , e k ⟩ u_k=h_{kk}\langle X,e_k\rangle u k = h k k ⟨ X , e k ⟩ give
h k 11 h 11 = h k k ⟨ X , e k ⟩ u − a − A ⟨ X , e k ⟩ . \frac{h_{k11}}{h_{11}}=\frac{h_{kk}\langle X,e_k\rangle}{u-a}-A\langle X,e_k\rangle. h 11 h k 11 = u − a h k k ⟨ X , e k ⟩ − A ⟨ X , e k ⟩ .
Hence
1 h 11 ∑ k h k 11 ( d ν f ~ ) ( e k ) − 1 u − a ∑ k h k k ( d ν f ~ ) ( e k ) ⟨ X , e k ⟩ = − A ∑ k ⟨ X , e k ⟩ ( d ν f ~ ) ( e k ) ≥ − C A , \frac{1}{h_{11}}\sum_k h_{k11}(d_\nu\widetilde f)(e_k)-\frac{1}{u-a}\sum_k h_{kk}(d_\nu\widetilde f)(e_k)\langle X,e_k\rangle
=-A\sum_k\langle X,e_k\rangle(d_\nu\widetilde f)(e_k)\geq-CA, h 11 1 k ∑ h k 11 ( d ν f ) ( e k ) − u − a 1 k ∑ h k k ( d ν f ) ( e k ) ⟨ X , e k ⟩ = − A k ∑ ⟨ X , e k ⟩ ( d ν f ) ( e k ) ≥ − C A ,
where the last inequality uses the C 1 C^{1} C 1 bound for f f f and the C 0 C^{0} C 0 bound for ∣ X ∣ |X| ∣ X ∣ . Combining (20) , (24) , and (29) in (18) , and discarding the nonnegative terms R α / ( u − a ) R_\alpha/(u-a) R α / ( u − a ) and A u R α AuR_\alpha A u R α , proves (19) . □
We next absorb the unfavorable term in (19) .
Lemma 3.2. If h 11 h_{11} h 11 and A A A are sufficiently large, depending only on the data in Theorem 1.1 , then
( C + R α ) h 11 ≤ a 2 ( u − a ) ∑ i F i i h i i 2 + A 2 ∑ i F i i . (30) (C+R_\alpha)h_{11}\leq\frac{a}{2(u-a)}\sum_i F^{ii}h_{ii}^{2}+\frac{A}{2}\sum_i F^{ii}. \tag*{(30)} ( C + R α ) h 11 ≤ 2 ( u − a ) a i ∑ F ii h ii 2 + 2 A i ∑ F ii . (30)
Proof. Fix a small number δ > 0 \delta>0 δ > 0 .
Case 1. Suppose ∣ h i i ∣ ≤ δ h 11 |h_{ii}|\leq\delta h_{11} ∣ h ii ∣ ≤ δ h 11 for every i ≥ 2 i\geq2 i ≥ 2 . Then
∣ η 11 ∣ ≤ ( n − 1 ) δ h 11 |\eta_{11}|\leq(n-1)\delta h_{11} ∣ η 11 ∣ ≤ ( n − 1 ) δ h 11
and
[ 1 − ( n − 2 ) δ ] h 11 ≤ η 22 ≤ ⋯ ≤ η n n ≤ [ 1 + ( n − 2 ) δ ] h 11 . (31) [1-(n-2)\delta]h_{11}\leq\eta_{22}\leq\cdots\leq\eta_{nn}\leq[1+(n-2)\delta]h_{11}. \tag*{(31)} [ 1 − ( n − 2 ) δ ] h 11 ≤ η 22 ≤ ⋯ ≤ η nn ≤ [ 1 + ( n − 2 ) δ ] h 11 . (31)
Introduce the normalized eigenvalues μ i = η i i / h 11 \mu_i=\eta_{ii}/h_{11} μ i = η ii / h 11 . By (31) , under the present assumption,
∣ μ 1 ∣ ≤ ( n − 1 ) δ , 1 − ( n − 2 ) δ ≤ μ i ≤ 1 + ( n − 2 ) δ ( i ≥ 2 ) . |\mu_1|\leq(n-1)\delta,\qquad1-(n-2)\delta\leq\mu_i\leq1+(n-2)\delta\quad(i\geq2). ∣ μ 1 ∣ ≤ ( n − 1 ) δ , 1 − ( n − 2 ) δ ≤ μ i ≤ 1 + ( n − 2 ) δ ( i ≥ 2 ) .
Thus μ \mu μ lies in a fixed small neighborhood of ( 0 , 1 , … , 1 ) (0,1,\ldots,1) ( 0 , 1 , … , 1 ) . Since
σ k − 1 ( 0 , 1 , … , 1 ) = ( n − 1 k − 1 ) > 0 , σ k − 2 ( 0 , 1 , … , 1 ) = ( n − 1 k − 2 ) > 0 , \sigma_{k-1}(0,1,\ldots,1)=\binom{n-1}{k-1}>0,\qquad\sigma_{k-2}(0,1,\ldots,1)=\binom{n-1}{k-2}>0, σ k − 1 ( 0 , 1 , … , 1 ) = ( k − 1 n − 1 ) > 0 , σ k − 2 ( 0 , 1 , … , 1 ) = ( k − 2 n − 1 ) > 0 ,
continuity gives, after fixing δ > 0 \delta>0 δ > 0 sufficiently small,
σ k − 1 ( η ) = h 11 k − 1 σ k − 1 ( μ ) ≥ c h 11 k − 1 , σ k − 2 ( η ) = h 11 k − 2 σ k − 2 ( μ ) ≥ c h 11 k − 2 . \sigma_{k-1}(\eta)=h_{11}^{k-1}\sigma_{k-1}(\mu)\geq ch_{11}^{k-1},\qquad\sigma_{k-2}(\eta)=h_{11}^{k-2}\sigma_{k-2}(\mu)\geq ch_{11}^{k-2}. σ k − 1 ( η ) = h 11 k − 1 σ k − 1 ( μ ) ≥ c h 11 k − 1 , σ k − 2 ( η ) = h 11 k − 2 σ k − 2 ( μ ) ≥ c h 11 k − 2 .
Using the exact trace formula from Lemma 2.2,
∑ i F i i = n − 1 k f 1 / k − 1 [ ( n − k + 1 ) σ k − 1 ( η ) + α ( n − k + 2 ) σ k − 2 ( η ) ] . \sum_i F^{ii}=\frac{n-1}{k}f^{1/k-1}\left[(n-k+1)\sigma_{k-1}(\eta)+\alpha(n-k+2)\sigma_{k-2}(\eta)\right]. i ∑ F ii = k n − 1 f 1/ k − 1 [ ( n − k + 1 ) σ k − 1 ( η ) + α ( n − k + 2 ) σ k − 2 ( η ) ] .
and the positive upper and lower bounds for f f f , we obtain
∑ i F i i ≥ c h 11 k − 1 . \sum_i F^{ii}\geq ch_{11}^{k-1}. i ∑ F ii ≥ c h 11 k − 1 .
Since k ≥ 2 k\geq2 k ≥ 2 and h 11 ≥ 1 h_{11}\geq1 h 11 ≥ 1 , h 11 k − 1 ≥ h 11 h_{11}^{k-1}\geq h_{11} h 11 k − 1 ≥ h 11 . We may therefore fix A A A large enough, depending only on the data, so that
C h 11 ≤ A 2 ∑ i F i i . Ch_{11}\leq\frac{A}{2}\sum_i F^{ii}. C h 11 ≤ 2 A i ∑ F ii .
It remains to estimate R α h 11 R_\alpha h_{11} R α h 11 . In terms of the normalized vector μ \mu μ , as δ → 0 \delta\to0 δ → 0 one has
μ → ( 0 , 1 , … , 1 ) . \mu\to(0,1,\ldots,1). μ → ( 0 , 1 , … , 1 ) .
Because k ≤ n − 1 k\leq n-1 k ≤ n − 1 , for every j ≥ 2 j\geq2 j ≥ 2 ,
σ k − 1 ( ( 0 , 1 , … , 1 ) ∣ j ) = ( n − 2 k − 1 ) > 0 , \sigma_{k-1}((0,1,\ldots,1)|j)=\binom{n-2}{k-1}>0, σ k − 1 (( 0 , 1 , … , 1 ) ∣ j ) = ( k − 1 n − 2 ) > 0 ,
and
σ k − 2 ( ( 0 , 1 , … , 1 ) ∣ j ) = ( n − 2 k − 2 ) > 0. \sigma_{k-2}((0,1,\ldots,1)|j)=\binom{n-2}{k-2}>0. σ k − 2 (( 0 , 1 , … , 1 ) ∣ j ) = ( k − 2 n − 2 ) > 0.
For j ≥ 2 j\geq2 j ≥ 2 ,
G j j = 1 k f 1 / k − 1 [ σ k − 1 ( η ∣ j ) + α σ k − 2 ( η ∣ j ) ] . G^{jj}=\frac{1}{k}f^{1/k-1}\left[\sigma_{k-1}(\eta|j)+\alpha\sigma_{k-2}(\eta|j)\right]. G j j = k 1 f 1/ k − 1 [ σ k − 1 ( η ∣ j ) + α σ k − 2 ( η ∣ j ) ] .
The two displayed limiting values above are strictly positive, so, after decreasing the already fixed δ \delta δ if necessary,
σ k − 1 ( η ∣ j ) ≥ c h 11 k − 1 , σ k − 2 ( η ∣ j ) ≥ c h 11 k − 2 , j ≥ 2. \sigma_{k-1}(\eta|j)\geq ch_{11}^{k-1},\qquad\sigma_{k-2}(\eta|j)\geq ch_{11}^{k-2},\qquad j\geq2. σ k − 1 ( η ∣ j ) ≥ c h 11 k − 1 , σ k − 2 ( η ∣ j ) ≥ c h 11 k − 2 , j ≥ 2.
Hence
G j j ≥ c f 1 / k − 1 ( h 11 k − 1 + α h 11 k − 2 ) , j ≥ 2. G^{jj}\geq cf^{1/k-1}\left(h_{11}^{k-1}+\alpha h_{11}^{k-2}\right),\qquad j\geq2. G j j ≥ c f 1/ k − 1 ( h 11 k − 1 + α h 11 k − 2 ) , j ≥ 2.
On the other hand, all components of μ \mu μ are uniformly bounded, so the same formula for G i i G^{ii} G ii gives
∑ i G i i ≤ C f 1 / k − 1 ( h 11 k − 1 + α h 11 k − 2 ) . \sum_i G^{ii} \leq C f^{1/k-1}\left(h_{11}^{k-1}+\alpha h_{11}^{k-2}\right). i ∑ G ii ≤ C f 1/ k − 1 ( h 11 k − 1 + α h 11 k − 2 ) .
Since ∑ i F i i = ( n − 1 ) ∑ i G i i \sum_i F^{ii}=(n-1)\sum_i G^{ii} ∑ i F ii = ( n − 1 ) ∑ i G ii , it follows that
F 11 = ∑ j ≠ 1 G j j ≥ c ∑ i F i i . F^{11}=\sum_{j\ne1}G^{jj}\geq c\sum_i F^{ii}. F 11 = j = 1 ∑ G j j ≥ c i ∑ F ii .
It follows that
∑ i F i i h i i 2 ≥ F 11 h 11 2 ≥ c h 11 2 ∑ i F i i . (32) \sum_i F^{ii}h_{ii}^2\geq F^{11}h_{11}^2\geq ch_{11}^2\sum_i F^{ii}. \tag*{(32)} i ∑ F ii h ii 2 ≥ F 11 h 11 2 ≥ c h 11 2 i ∑ F ii . (32)
By (10), R α ≤ C ∑ i F i i R_\alpha\leq C\sum_i F^{ii} R α ≤ C ∑ i F ii , while (32) gives
∑ i F i i ≤ C h 11 2 ∑ i F i i h i i 2 . \sum_i F^{ii}\leq\frac{C}{h_{11}^2}\sum_i F^{ii}h_{ii}^2. i ∑ F ii ≤ h 11 2 C i ∑ F ii h ii 2 .
Consequently
R α h 11 ≤ C h 11 ∑ i F i i h i i 2 . R_\alpha h_{11}\leq\frac{C}{h_{11}}\sum_i F^{ii}h_{ii}^2. R α h 11 ≤ h 11 C i ∑ F ii h ii 2 .
Because a > 0 a>0 a > 0 and u u u is uniformly bounded above and below by (16), the coefficient a / [ 4 ( u − a ) ] a/[4(u-a)] a / [ 4 ( u − a )] has a fixed positive lower bound. Thus, for sufficiently large h 11 h_{11} h 11 ,
R α h 11 ≤ a 4 ( u − a ) ∑ i F i i h i i 2 . R_\alpha h_{11}\leq\frac{a}{4(u-a)}\sum_i F^{ii}h_{ii}^2. R α h 11 ≤ 4 ( u − a ) a i ∑ F ii h ii 2 .
This proves (30) in Case 1.
Case 2. Suppose h 22 > δ h 11 h_{22}>\delta h_{11} h 22 > δ h 11 or h n n < − δ h 11 h_{nn}<-\delta h_{11} h nn < − δ h 11 . Since G 11 ≥ G i i G^{11}\geq G^{ii} G 11 ≥ G ii and (7) holds, for every i ≥ 2 i\geq2 i ≥ 2 ,
F i i ≥ G 11 ≥ 1 n ∑ j G j j = 1 n ( n − 1 ) ∑ j F j j . (33) F^{ii}\geq G^{11}\geq\frac{1}{n}\sum_jG^{jj}=\frac{1}{n(n-1)}\sum_jF^{jj}. \tag*{(33)} F ii ≥ G 11 ≥ n 1 j ∑ G j j = n ( n − 1 ) 1 j ∑ F j j . (33)
Therefore
∑ i F i i h i i 2 ≥ c δ 2 h 11 2 ∑ i F i i . (34) \sum_i F^{ii}h_{ii}^2\geq c\delta^2h_{11}^2\sum_iF^{ii}. \tag*{(34)} i ∑ F ii h ii 2 ≥ c δ 2 h 11 2 i ∑ F ii . (34)
Indeed, Lemma 2.2 gives ∑ i F i i ≥ c > 0 \sum_iF^{ii}\geq c>0 ∑ i F ii ≥ c > 0 , so
C h 11 ≤ C h 11 ∑ i F i i , R α h 11 ≤ C h 11 ∑ i F i i Ch_{11}\leq Ch_{11}\sum_iF^{ii},\qquad R_\alpha h_{11}\leq Ch_{11}\sum_iF^{ii} C h 11 ≤ C h 11 i ∑ F ii , R α h 11 ≤ C h 11 i ∑ F ii
by (10). In view of (34), the right-hand sides are bounded by
C δ 2 h 11 ∑ i F i i h i i 2 . \frac{C}{\delta^2h_{11}}\sum_iF^{ii}h_{ii}^2. δ 2 h 11 C i ∑ F ii h ii 2 .
For sufficiently large h 11 h_{11} h 11 this is at most a [ 4 ( u − a ) ] − 1 ∑ i F i i h i i 2 a[4(u-a)]^{-1}\sum_iF^{ii}h_{ii}^2 a [ 4 ( u − a ) ] − 1 ∑ i F ii h ii 2 . This proves (30) in Case 2 and finishes the proof. □ \square □
Combining Lemmas 3.1 and 3.2,
0 ≥ − 2 h 11 ∑ i ≥ 2 G 1 i , i 1 h 11 i 2 − F i i h 11 i 2 h 11 2 + a 2 ( u − a ) F i i h i i 2 + F i i u i 2 ( u − a ) 2 + A 2 ∑ i F i i − C A . (35) \begin{aligned}
0 \ge{}& -\frac{2}{h_{11}}\sum_{i\ge2}G^{1i,i1}h_{11i}^{2}-\frac{F^{ii}h_{11i}^{2}}{h_{11}^{2}}+\frac{a}{2(u-a)}F^{ii}h_{ii}^{2}\\
&+\frac{F^{ii}u_i^{2}}{(u-a)^{2}}+\frac{A}{2}\sum_i F^{ii}-CA. \tag*{(35)}
\end{aligned} 0 ≥ − h 11 2 i ≥ 2 ∑ G 1 i , i 1 h 11 i 2 − h 11 2 F ii h 11 i 2 + 2 ( u − a ) a F ii h ii 2 + ( u − a ) 2 F ii u i 2 + 2 A i ∑ F ii − C A . (35)
Lemma 3.3. If h 11 h_{11} h 11 and A A A are sufficiently large, then at X 0 X_0 X 0 ,
∣ h i i ∣ ≤ C A , i ≥ 2. |h_{ii}| \le CA,\qquad i\ge2. ∣ h ii ∣ ≤ C A , i ≥ 2.
Proof. From (17) , for any 0 < ε < 1 0<\varepsilon<1 0 < ε < 1 ,
F i i h 11 i 2 h 11 2 ≤ 1 + ε ( u − a ) 2 F i i u i 2 + C ( 1 + 1 ε ) A 2 F i i ⟨ X , e i ⟩ 2 . \frac{F^{ii}h_{11i}^{2}}{h_{11}^{2}}\le\frac{1+\varepsilon}{(u-a)^{2}}F^{ii}u_i^{2}+C\left(1+\frac{1}{\varepsilon}\right)A^{2}F^{ii}\langle X,e_i\rangle^{2}. h 11 2 F ii h 11 i 2 ≤ ( u − a ) 2 1 + ε F ii u i 2 + C ( 1 + ε 1 ) A 2 F ii ⟨ X , e i ⟩ 2 .
Substitute this into (35) and discard the nonnegative concavity term − 2 h 11 − 1 ∑ i ≥ 2 G 1 i , i 1 h 11 i 2 -2h_{11}^{-1}\sum_{i\ge2}G^{1i,i1}h_{11i}^{2} − 2 h 11 − 1 ∑ i ≥ 2 G 1 i , i 1 h 11 i 2 . Since u i = h i i ⟨ X , e i ⟩ u_i=h_{ii}\langle X,e_i\rangle u i = h ii ⟨ X , e i ⟩ , the excess part of the u i 2 u_i^2 u i 2 term is bounded by
ε ( u − a ) 2 F i i u i 2 ≤ C ε F i i h i i 2 , \frac{\varepsilon}{(u-a)^{2}}F^{ii}u_i^{2}\le C\varepsilon F^{ii}h_{ii}^{2}, ( u − a ) 2 ε F ii u i 2 ≤ C ε F ii h ii 2 ,
where we used ∣ X ∣ ≤ C |X|\le C ∣ X ∣ ≤ C and u − a ≥ a > 0 u-a\ge a>0 u − a ≥ a > 0 . Choose ε > 0 \varepsilon>0 ε > 0 so small that this term is absorbed by one half of the positive quadratic term a [ 2 ( u − a ) ] − 1 F i i h i i 2 a[2(u-a)]^{-1}F^{ii}h_{ii}^{2} a [ 2 ( u − a ) ] − 1 F ii h ii 2 . The remaining A A A -term satisfies
C ( 1 + 1 ε ) A 2 F i i ⟨ X , e i ⟩ 2 ≤ C A 2 ∑ i F i i . C\left(1+\frac{1}{\varepsilon}\right)A^{2}F^{ii}\langle X,e_i\rangle^{2}\le CA^{2}\sum_i F^{ii}. C ( 1 + ε 1 ) A 2 F ii ⟨ X , e i ⟩ 2 ≤ C A 2 i ∑ F ii .
We therefore obtain
0 ≥ c ∑ i F i i h i i 2 − C A 2 ∑ i F i i − C A . (36) 0\ge c\sum_i F^{ii}h_{ii}^{2}-CA^{2}\sum_i F^{ii}-CA. \tag*{(36)} 0 ≥ c i ∑ F ii h ii 2 − C A 2 i ∑ F ii − C A . (36)
Starting from (36) , and using (9) , ∑ i F i i ≥ c 0 > 0 \sum_i F^{ii}\ge c_0>0 ∑ i F ii ≥ c 0 > 0 ; since A ≥ 1 A\ge1 A ≥ 1 , the final term satisfies C A ≤ C A 2 ∑ i F i i CA\le CA^{2}\sum_i F^{ii} C A ≤ C A 2 ∑ i F ii and can be absorbed into the middle term after enlarging its constant. Thus
c ∑ i F i i h i i 2 ≤ C A 2 ∑ i F i i . c\sum_i F^{ii}h_{ii}^{2}\le CA^{2}\sum_i F^{ii}. c i ∑ F ii h ii 2 ≤ C A 2 i ∑ F ii .
For each i ≥ 2 i\ge2 i ≥ 2 , (33) gives F i i ≥ c ∑ j F j j F^{ii}\ge c\sum_j F^{jj} F ii ≥ c ∑ j F j j . Hence
c ( ∑ j F j j ) ∑ i ≥ 2 h i i 2 ≤ C A 2 ∑ j F j j . c\left(\sum_j F^{jj}\right)\sum_{i\ge2}h_{ii}^{2}\le CA^{2}\sum_j F^{jj}. c ( j ∑ F j j ) i ≥ 2 ∑ h ii 2 ≤ C A 2 j ∑ F j j .
Cancelling the positive trace gives
∑ i ≥ 2 h i i 2 ≤ C A 2 , \sum_{i\ge2}h_{ii}^{2}\le CA^{2}, i ≥ 2 ∑ h ii 2 ≤ C A 2 ,
and therefore ∣ h i i ∣ ≤ C A |h_{ii}|\le CA ∣ h ii ∣ ≤ C A for every i ≥ 2 i\ge2 i ≥ 2 .
Proof of Theorem 1.1. If h 11 h_{11} h 11 is bounded by a fixed multiple of A A A , there is nothing to prove. Hence we may assume it is sufficiently large. By Lemma 3.3, after increasing this threshold we may also assume
∣ h i i ∣ ≤ δ h 11 , i ≥ 2 , (37) |h_{ii}| \le\delta h_{11}, \qquad i \ge2, \tag*{(37)} ∣ h ii ∣ ≤ δ h 11 , i ≥ 2 , (37)
where δ > 0 \delta> 0 δ > 0 is fixed sufficiently small.
For the i = 1 i=1 i = 1 derivative, (17) gives
h 111 h 11 = u 1 u − a − A ⟨ X , e 1 ⟩ . \frac{h_{111}}{h_{11}}=\frac{u_1}{u-a}-A\langle X,e_1\rangle. h 11 h 111 = u − a u 1 − A ⟨ X , e 1 ⟩ .
For any ε > 0 \varepsilon> 0 ε > 0 , Cauchy–Schwarz yields
F 11 h 111 2 h 11 2 ≤ ( 1 + ε ) F 11 u 1 2 ( u − a ) 2 + C ε A 2 F 11 ⟨ X , e 1 ⟩ 2 . \frac{F^{11}h_{111}^2}{h_{11}^2}\le(1+\varepsilon)\frac{F^{11}u_1^2}{(u-a)^2}+C_\varepsilon A^2F^{11}\langle X,e_1\rangle^2. h 11 2 F 11 h 111 2 ≤ ( 1 + ε ) ( u − a ) 2 F 11 u 1 2 + C ε A 2 F 11 ⟨ X , e 1 ⟩ 2 .
Since u 1 = h 11 ⟨ X , e 1 ⟩ u_1=h_{11}\langle X,e_1\rangle u 1 = h 11 ⟨ X , e 1 ⟩ , the excess term ε F 11 u 1 2 / ( u − a ) 2 \varepsilon F^{11}u_1^2/(u-a)^2 ε F 11 u 1 2 / ( u − a ) 2 is bounded by C ε F 11 h 11 2 C\varepsilon F^{11}h_{11}^2 C ε F 11 h 11 2 . Choose ε \varepsilon ε sufficiently small; then, once h 11 ≫ A h_{11}\gg A h 11 ≫ A , both this excess and the A 2 F 11 A^2F^{11} A 2 F 11 term are absorbed by a fixed fraction of a ( u − a ) − 1 ∑ i F i i h i i 2 a(u-a)^{-1}\sum_i F^{ii}h_{ii}^2 a ( u − a ) − 1 ∑ i F ii h ii 2 . Thus
F 11 h 111 2 h 11 2 ≤ F 11 u 1 2 ( u − a ) 2 + a 8 ( u − a ) F i i h i i 2 . (38) \frac{F^{11}h_{111}^2}{h_{11}^2}\le\frac{F^{11}u_1^2}{(u-a)^2}+\frac{a}{8(u-a)}F^{ii}h_{ii}^2. \tag*{(38)} h 11 2 F 11 h 111 2 ≤ ( u − a ) 2 F 11 u 1 2 + 8 ( u − a ) a F ii h ii 2 . (38)
For i ≥ 2 i\ge2 i ≥ 2 , the standard second-derivative formula for a symmetric spectral function gives
− G 1 i , i 1 = G 11 − G i i η i i − η 11 = F i i − F 11 h 11 − h i i . -G^{1i,i1}=\frac{G^{11}-G^{ii}}{\eta_{ii}-\eta_{11}}=\frac{F^{ii}-F^{11}}{h_{11}-h_{ii}}. − G 1 i , i 1 = η ii − η 11 G 11 − G ii = h 11 − h ii F ii − F 11 .
Set d i = h 11 − h i i d_i=h_{11}-h_{ii} d i = h 11 − h ii . By (37) ,
( 1 − δ ) h 11 ≤ d i ≤ ( 1 + δ ) h 11 , i ≥ 2. (1-\delta)h_{11}\le d_i\le(1+\delta)h_{11},\qquad i\ge2. ( 1 − δ ) h 11 ≤ d i ≤ ( 1 + δ ) h 11 , i ≥ 2.
The spectral second-derivative formula therefore gives
− 2 h 11 G 1 i , i 1 h 11 i 2 = 2 ( F i i − F 11 ) h 11 d i h 11 i 2 ≥ 2 1 + δ ( F i i − F 11 ) h 11 i 2 h 11 2 . -\frac{2}{h_{11}}G^{1i,i1}h_{11i}^2=\frac{2(F^{ii}-F^{11})}{h_{11}d_i}h_{11i}^2\ge\frac{2}{1+\delta}\frac{(F^{ii}-F^{11})h_{11i}^2}{h_{11}^2}. − h 11 2 G 1 i , i 1 h 11 i 2 = h 11 d i 2 ( F ii − F 11 ) h 11 i 2 ≥ 1 + δ 2 h 11 2 ( F ii − F 11 ) h 11 i 2 .
Since
F i i ≤ 2 1 + δ ( F i i − F 11 ) + 2 1 + δ F 11 , F^{ii}\le\frac{2}{1+\delta}(F^{ii}-F^{11})+\frac{2}{1+\delta}F^{11}, F ii ≤ 1 + δ 2 ( F ii − F 11 ) + 1 + δ 2 F 11 ,
we obtain, after summing over i ≥ 2 i\ge2 i ≥ 2 ,
∑ i ≥ 2 F i i h 11 i 2 h 11 2 ≤ − 2 h 11 ∑ i ≥ 2 G 1 i , i 1 h 11 i 2 + C F 11 ∑ i ≥ 2 h 11 i 2 h 11 2 . \sum_{i\ge2}\frac{F^{ii}h_{11i}^2}{h_{11}^2}\le-\frac{2}{h_{11}}\sum_{i\ge2}G^{1i,i1}h_{11i}^2+CF^{11}\sum_{i\ge2}\frac{h_{11i}^2}{h_{11}^2}. i ≥ 2 ∑ h 11 2 F ii h 11 i 2 ≤ − h 11 2 i ≥ 2 ∑ G 1 i , i 1 h 11 i 2 + C F 11 i ≥ 2 ∑ h 11 2 h 11 i 2 .
For i ≥ 2 i\ge2 i ≥ 2 , (17) , u i = h i i ⟨ X , e i ⟩ u_i=h_{ii}\langle X,e_i\rangle u i = h ii ⟨ X , e i ⟩ , and Lemma 3.3 give
∣ h 11 i h 11 ∣ ≤ ∣ h i i ∣ u − a ∣ ⟨ X , e i ⟩ ∣ + A ∣ ⟨ X , e i ⟩ ∣ ≤ C A ∣ ⟨ X , e i ⟩ ∣ . \left|\frac{h_{11i}}{h_{11}}\right|\le\frac{|h_{ii}|}{u-a}|\langle X,e_i\rangle|+A|\langle X,e_i\rangle|\le CA|\langle X,e_i\rangle|. h 11 h 11 i ≤ u − a ∣ h ii ∣ ∣ ⟨ X , e i ⟩ ∣ + A ∣ ⟨ X , e i ⟩ ∣ ≤ C A ∣ ⟨ X , e i ⟩ ∣.
Hence
F 11 ∑ i ≥ 2 h 11 i 2 h 11 2 ≤ C A 2 F 11 . F^{11}\sum_{i\ge2}\frac{h_{11i}^2}{h_{11}^2}\le CA^2F^{11}. F 11 i ≥ 2 ∑ h 11 2 h 11 i 2 ≤ C A 2 F 11 .
If h 11 h_{11} h 11 is sufficiently large compared with A A A , this is bounded by a [ 8 ( u − a ) ] − 1 F 11 h 11 2 a[8(u-a)]^{-1}F^{11}h_{11}^{2} a [ 8 ( u − a ) ] − 1 F 11 h 11 2 . We have thus proved
∑ i ≥ 2 F i i h i i 2 h 11 2 ≤ 2 h 11 ∑ i ≥ 2 G i i h 11 i 2 + a 8 ( u − a ) F 11 h 11 2 . (39) \sum_{i\ge2}\frac{F^{ii}h_{ii}^{2}}{h_{11}^{2}}\le\frac{2}{h_{11}}\sum_{i\ge2}G^{ii}h_{11i}^{2}+\frac{a}{8(u-a)}F^{11}h_{11}^{2}. \tag*{(39)} i ≥ 2 ∑ h 11 2 F ii h ii 2 ≤ h 11 2 i ≥ 2 ∑ G ii h 11 i 2 + 8 ( u − a ) a F 11 h 11 2 . (39)
Substituting (38) and (39) into (35) yields
0 ≥ a 4 ( u − a ) ∑ i F i i h i i 2 + A 2 ∑ i F i i − C A . (40) 0\ge\frac{a}{4(u-a)}\sum_i F^{ii}h_{ii}^{2}+\frac{A}{2}\sum_i F^{ii}-CA. \tag*{(40)} 0 ≥ 4 ( u − a ) a i ∑ F ii h ii 2 + 2 A i ∑ F ii − C A . (40)
Dropping the first nonnegative term in (40) gives
A 2 ∑ i F i i ≤ C A . \frac{A}{2}\sum_i F^{ii}\le CA. 2 A i ∑ F ii ≤ C A .
Since A > 0 A>0 A > 0 is fixed, ∑ i F i i ≤ C \sum_i F^{ii}\le C ∑ i F ii ≤ C . Using ∑ i F i i = ( n − 1 ) ∑ i G i i \sum_i F^{ii}=(n-1)\sum_i G^{ii} ∑ i F ii = ( n − 1 ) ∑ i G ii , we obtain
∑ i G i i ≤ C . (41) \sum_i G^{ii}\le C. \tag*{(41)} i ∑ G ii ≤ C . (41)
It remains to obtain a positive lower bound for F 11 F^{11} F 11 . Introduce the augmented vector
η ^ = ( η 11 , … , η n n , α ) ∈ Γ k n + 1 . \hat{\eta}=(\eta_{11},\ldots,\eta_{nn},\alpha)\in\Gamma_k^{n+1}. η ^ = ( η 11 , … , η nn , α ) ∈ Γ k n + 1 .
Let G ^ = σ k ( η ^ ) 1 / k \hat{G}=\sigma_k(\hat{\eta})^{1/k} G ^ = σ k ( η ^ ) 1/ k . For the first n n n coordinates, G ^ i i = G i i \hat{G}^{ii}=G^{ii} G ^ ii = G ii , while
G ^ n + 1 , n + 1 = 1 k F 1 / k − 1 σ k − 1 ( η ) ≤ 1 n − k + 1 ∑ i = 1 n G i i . \hat{G}^{n+1,n+1}=\frac{1}{k}F^{1/k-1}\sigma_{k-1}(\eta)\le\frac{1}{n-k+1}\sum_{i=1}^{n}G^{ii}. G ^ n + 1 , n + 1 = k 1 F 1/ k − 1 σ k − 1 ( η ) ≤ n − k + 1 1 i = 1 ∑ n G ii .
Thus (41) implies
∑ a = 1 n + 1 G ^ a a ≤ C . (42) \sum_{a=1}^{n+1}\hat{G}^{aa}\le C. \tag*{(42)} a = 1 ∑ n + 1 G ^ aa ≤ C . (42)
Indeed, writing N = n + 1 N=n+1 N = n + 1 , the identity
σ k ( η ^ ) 1 / k − 1 σ k − 1 ( η ^ ) = k N − k + 1 ∑ a = 1 N G ^ a a ≤ C \sigma_k(\hat{\eta})^{1/k-1}\sigma_{k-1}(\hat{\eta})=\frac{k}{N-k+1}\sum_{a=1}^{N}\hat{G}^{aa}\le C σ k ( η ^ ) 1/ k − 1 σ k − 1 ( η ^ ) = N − k + 1 k a = 1 ∑ N G ^ aa ≤ C
verifies the hypothesis of part (2) of Lemma 2.2 in Hou–Ma–Wu [7 ] . Applied to η ^ ∈ Γ k N \hat{\eta}\in\Gamma_k^N η ^ ∈ Γ k N , that lemma yields a positive lower bound for the G ^ \hat{G} G ^ -derivative corresponding to the largest component of η ^ \hat{\eta} η ^ . By Lemma 3.3,
η 11 = ∑ j ≥ 2 h j j = O ( A ) , \eta_{11}=\sum_{j\ge2}h_{jj}=O(A), η 11 = j ≥ 2 ∑ h j j = O ( A ) ,
whereas, for i ≥ 2 i\ge2 i ≥ 2 ,
η i i = h 11 + O ( A ) . \eta_{ii}=h_{11}+O(A). η ii = h 11 + O ( A ) .
Hence, if h 11 h_{11} h 11 is sufficiently large, a largest component of η ^ \hat{\eta} η ^ is some η p p \eta_{pp} η pp with p ≥ 2 p\ge2 p ≥ 2 . Consequently,
G p p ≥ c > 0 , G^{pp}\ge c>0, G pp ≥ c > 0 ,
and therefore
F 11 = ∑ p ≠ 1 G p p ≥ c > 0. (43) F^{11}=\sum_{p\ne1}G^{pp}\ge c>0. \tag*{(43)} F 11 = p = 1 ∑ G pp ≥ c > 0. (43)
Using (43) in the first term of (40), and using the uniform bounds for u − a u-a u − a , gives
0 ≥ c F 11 h 11 2 − C A ≥ c h 11 2 − C A . 0\ge cF^{11}h_{11}^{2}-CA\ge ch_{11}^{2}-CA. 0 ≥ c F 11 h 11 2 − C A ≥ c h 11 2 − C A .
Hence h 11 ≤ C h_{11}\le C h 11 ≤ C . Finally, since H > 0 H>0 H > 0 and h 11 ≥ h 22 ≥ ⋯ ≥ h n n h_{11}\ge h_{22}\ge\cdots\ge h_{nn} h 11 ≥ h 22 ≥ ⋯ ≥ h nn ,
0 < H = ∑ i = 1 n h i i ≤ ( n − 1 ) h 11 + h n n , 0<H=\sum_{i=1}^{n}h_{ii}\le(n-1)h_{11}+h_{nn}, 0 < H = i = 1 ∑ n h ii ≤ ( n − 1 ) h 11 + h nn ,
so h n n ≥ − ( n − 1 ) h 11 h_{nn}\ge-(n-1)h_{11} h nn ≥ − ( n − 1 ) h 11 . Thus every principal curvature is bounded in absolute value, and the theorem follows.
A priori estimates and proof of Theorem 1.2
We prove Theorem 1.2 by the continuity method. In order to make the argument transparent, we first establish the C 0 C^{0} C 0 , C 1 C^{1} C 1 , and C 2 C^{2} C 2 estimates separately, and then treat existence and uniqueness in the last two subsections.
Set
A n , k = ( n k ) ( n − 1 ) k , B n , k , α = α ( n k − 1 ) ( n − 1 ) k − 1 . A_{n,k}=\binom{n}{k}(n-1)^{k},\qquad B_{n,k,\alpha}=\alpha\binom{n}{k-1}(n-1)^{k-1}. A n , k = ( k n ) ( n − 1 ) k , B n , k , α = α ( k − 1 n ) ( n − 1 ) k − 1 .
so that
Φ α ( r ) = A n , k r k + B n , k , α r k − 1 . \Phi_{\alpha}(r)=\frac{A_{n,k}}{r^{k}}+\frac{B_{n,k,\alpha}}{r^{k-1}}. Φ α ( r ) = r k A n , k + r k − 1 B n , k , α .
Let
C n , k , α = A n , k + B n , k , α . C_{n,k,\alpha}=A_{n,k}+B_{n,k,\alpha}. C n , k , α = A n , k + B n , k , α .
Choose
0 < ε < 1 r 2 k − 1 0<\varepsilon<\frac{1}{r_{2}^{k}-1} 0 < ε < r 2 k − 1 1
and define
f 0 ( X , ν ) = C n , k , α ( 1 + ε ∣ X ∣ k − ε ) . f_{0}(X,\nu)=C_{n,k,\alpha}\left(\frac{1+\varepsilon}{\lvert X\rvert^{k}}-\varepsilon\right). f 0 ( X , ν ) = C n , k , α ( ∣ X ∣ k 1 + ε − ε ) .
The choice of ε \varepsilon ε gives
1 + ε r 2 k − ε = 1 − ε ( r 2 k − 1 ) r 2 k > 0. \frac{1+\varepsilon}{r_{2}^{k}}-\varepsilon
=\frac{1-\varepsilon(r_{2}^{k}-1)}{r_{2}^{k}}>0. r 2 k 1 + ε − ε = r 2 k 1 − ε ( r 2 k − 1 ) > 0.
Since ρ ↦ ( 1 + ε ) ρ − k − ε \rho\mapsto(1+\varepsilon)\rho^{-k}-\varepsilon ρ ↦ ( 1 + ε ) ρ − k − ε is decreasing, it follows that f 0 > 0 f_{0}>0 f 0 > 0 throughout r 1 ≤ ∣ X ∣ ≤ r 2 r_{1}\le\lvert X\rvert\le r_{2} r 1 ≤ ∣ X ∣ ≤ r 2 . On the unit sphere, λ i ( η ) = n − 1 \lambda_{i}(\eta)=n-1 λ i ( η ) = n − 1 for every i i i , and therefore
S k , α ( λ ( η ) ) = A n , k + B n , k , α = C n , k , α = f 0 . S_{k,\alpha}(\lambda(\eta))=A_{n,k}+B_{n,k,\alpha}=C_{n,k,\alpha}=f_{0}. S k , α ( λ ( η )) = A n , k + B n , k , α = C n , k , α = f 0 .
Thus the unit sphere is a solution of the t = 0 t=0 t = 0 equation. Moreover,
∂ ∂ ρ ( ρ k f 0 ) = − k ε C n , k , α ρ k − 1 < 0. \frac{\partial}{\partial\rho}\left(\rho^{k}f_{0}\right)=-k\varepsilon C_{n,k,\alpha}\rho^{k-1}<0. ∂ ρ ∂ ( ρ k f 0 ) = − k ε C n , k , α ρ k − 1 < 0.
A direct calculation gives
ρ k ( f 0 ( ρ ) − Φ α ( ρ ) ) = B n , k , α ( 1 − ρ ) + ε C n , k , α ( 1 − ρ k ) . \rho^k\left(f_0(\rho)-\Phi_\alpha(\rho)\right)=B_{n,k,\alpha}(1-\rho)+\varepsilon C_{n,k,\alpha}(1-\rho^k). ρ k ( f 0 ( ρ ) − Φ α ( ρ ) ) = B n , k , α ( 1 − ρ ) + ε C n , k , α ( 1 − ρ k ) .
Thus
f 0 ( ρ ) > Φ α ( ρ ) ( ρ < 1 ) , f 0 ( ρ ) < Φ α ( ρ ) ( ρ > 1 ) . f_0(\rho)>\Phi_\alpha(\rho)\quad(\rho<1),\qquad f_0(\rho)<\Phi_\alpha(\rho)\quad(\rho>1). f 0 ( ρ ) > Φ α ( ρ ) ( ρ < 1 ) , f 0 ( ρ ) < Φ α ( ρ ) ( ρ > 1 ) .
For t ∈ [ 0 , 1 ] t\in[0,1] t ∈ [ 0 , 1 ] , define
f t = t f + ( 1 − t ) f 0 . f_t=tf+(1-t)f_0. f t = t f + ( 1 − t ) f 0 .
Because the path is a convex combination, f t f_t f t remains positive. The quantity ∂ ρ ( ρ k f t ) \partial_\rho(\rho^k f_t) ∂ ρ ( ρ k f t ) is the same convex combination of ∂ ρ ( ρ k f ) \partial_\rho(\rho^k f) ∂ ρ ( ρ k f ) and ∂ ρ ( ρ k f 0 ) \partial_\rho(\rho^k f_0) ∂ ρ ( ρ k f 0 ) ; hence (4) holds for every t t t . Likewise, f f f satisfies the barrier inequalities in (3) non-strictly while f 0 f_0 f 0 satisfies them strictly at r 1 r_1 r 1 and r 2 r_2 r 2 . Therefore, for every t < 1 t<1 t < 1 , the two barrier inequalities for f t f_t f t are strict. All constants below are independent of t t t .
C 0 C^0 C 0 estimate
Let M t M_t M t be an admissible star-shaped solution with radial function ρ \rho ρ . At a maximum point of ρ \rho ρ ,
∇ ρ = 0 , ∇ 2 ρ ≤ 0. \nabla\rho=0,\qquad\nabla^2\rho\leq0. ∇ ρ = 0 , ∇ 2 ρ ≤ 0.
By (11) ,
g i j = ρ 2 g ^ i j , h i j = ρ g ^ i j − ρ i j ≥ ρ g ^ i j , g_{ij}=\rho^2\widehat{g}_{ij},\qquad h_{ij}=\rho\widehat{g}_{ij}-\rho_{ij}\geq\rho\widehat{g}_{ij}, g ij = ρ 2 g ij , h ij = ρ g ij − ρ ij ≥ ρ g ij ,
and hence
κ i ≥ 1 ρ , λ i ( η ) ≥ n − 1 ρ . \kappa_i\geq\frac{1}{\rho},\qquad\lambda_i(\eta)\geq\frac{n-1}{\rho}. κ i ≥ ρ 1 , λ i ( η ) ≥ ρ n − 1 .
Since S k , α S_{k,\alpha} S k , α is increasing in each eigenvalue throughout the admissible region, and the admissible region is convex by Lemma 2.1, componentwise comparison along the line segment joining λ ( η ) \lambda(\eta) λ ( η ) to the spherical vector gives
f t ( X , ν ) = S k , α ( λ ( η ) ) ≥ Φ α ( ρ ) . (44) f_t(X,\nu)=S_{k,\alpha}(\lambda(\eta))\geq\Phi_\alpha(\rho). \tag*{(44)} f t ( X , ν ) = S k , α ( λ ( η )) ≥ Φ α ( ρ ) . (44)
At such an extremum ν = x = X / ∣ X ∣ \nu=x=X/|X| ν = x = X /∣ X ∣ . If a solution in the closure of the annular class touched ρ = r 2 \rho=r_2 ρ = r 2 at its maximum, then (44) would give f t ( r 2 x , x ) ≥ Φ α ( r 2 ) f_t(r_2x,x)\geq\Phi_\alpha(r_2) f t ( r 2 x , x ) ≥ Φ α ( r 2 ) , contradicting the strict outer barrier for t < 1 t<1 t < 1 .
At a minimum point of ρ \rho ρ the inequalities reverse:
h i j ≤ ρ g ^ i j , λ i ( η ) ≤ n − 1 ρ , h_{ij}\leq\rho\widehat{g}_{ij},\qquad\lambda_i(\eta)\leq\frac{n-1}{\rho}, h ij ≤ ρ g ij , λ i ( η ) ≤ ρ n − 1 ,
and therefore
f t ( X , ν ) ≤ Φ α ( ρ ) . f_t(X,\nu)\leq\Phi_\alpha(\rho). f t ( X , ν ) ≤ Φ α ( ρ ) .
Again ν = x \nu=x ν = x at the extremum. If ρ = r 1 \rho=r_1 ρ = r 1 at the minimum, this inequality contradicts the strict inner barrier f t ( r 1 x , x ) > Φ α ( r 1 ) f_t(r_1x,x)>\Phi_\alpha(r_1) f t ( r 1 x , x ) > Φ α ( r 1 ) for t < 1 t<1 t < 1 . Consequently,
r 1 < ρ < r 2 ( 0 ≤ t < 1 ) , (45) r_1<\rho<r_2\qquad(0\leq t<1), \tag*{(45)} r 1 < ρ < r 2 ( 0 ≤ t < 1 ) , (45)
with the corresponding non-strict bounds at t = 1 t=1 t = 1 by passage to the limit.
C1 ^{1} 1 estimate
By (12) , it suffices to prove a positive lower bound for the support function u = ⟨ X , ν ⟩ u=\langle X,\nu\rangle u = ⟨ X , ν ⟩ . Consider
w = − log u + γ ( ∣ X ∣ 2 ) , γ ( s ) = L s , w=-\log u+\gamma(|X|^{2}),\qquad\gamma(s)=\frac{L}{s}, w = − log u + γ ( ∣ X ∣ 2 ) , γ ( s ) = s L ,
where L > 1 L>1 L > 1 will be chosen sufficiently large. Suppose that w w w attains its maximum at X 0 X_{0} X 0 . If X 0 X_{0} X 0 is parallel to ν \nu ν , then u = ∣ X ∣ ≥ r 1 u=|X|\ge r_{1} u = ∣ X ∣ ≥ r 1 , and there is nothing to prove. Otherwise X T ≠ 0 X^{T}\ne0 X T = 0 . Choose e 1 = X T / ∣ X T ∣ e_{1}=X^{T}/|X^{T}| e 1 = X T /∣ X T ∣ and complete it to an orthonormal frame. Then
⟨ X , e 1 ⟩ ≠ 0 , ⟨ X , e i ⟩ = 0 ( i ≥ 2 ) . \langle X,e_{1}\rangle\ne0,\qquad\langle X,e_{i}\rangle=0\quad(i\ge2). ⟨ X , e 1 ⟩ = 0 , ⟨ X , e i ⟩ = 0 ( i ≥ 2 ) .
At the maximum point,
0 = w i = − u i u + 2 γ ′ ⟨ X , e i ⟩ . 0=w_{i}=-\frac{u_{i}}{u}+2\gamma'\langle X,e_{i}\rangle. 0 = w i = − u u i + 2 γ ′ ⟨ X , e i ⟩ .
Since u i = h i j ⟨ X , e j ⟩ u_{i}=h_{ij}\langle X,e_{j}\rangle u i = h ij ⟨ X , e j ⟩ and only the e 1 e_{1} e 1 component of X T X^{T} X T is nonzero, we have u i = h i 1 ⟨ X , e 1 ⟩ u_{i}=h_{i1}\langle X,e_{1}\rangle u i = h i 1 ⟨ X , e 1 ⟩ . Thus the i = 1 i=1 i = 1 equation gives h 11 = 2 γ ′ u h_{11}=2\gamma'u h 11 = 2 γ ′ u , whereas the equations with i ≥ 2 i\ge2 i ≥ 2 give h 1 i = 0 h_{1i}=0 h 1 i = 0 . We then rotate e 2 , … , e n e_{2},\ldots,e_{n} e 2 , … , e n to diagonalize the remaining ( n − 1 ) × ( n − 1 ) (n-1)\times(n-1) ( n − 1 ) × ( n − 1 ) block without changing e 1 e_{1} e 1 . Since γ ′ < 0 \gamma'<0 γ ′ < 0 , we have h 11 < 0 h_{11}<0 h 11 < 0 . Because H > 0 H>0 H > 0 , there is an index p ≥ 2 p\ge2 p ≥ 2 such that h p p > 0 h_{pp}>0 h pp > 0 . Hence η p p = H − h p p < H − h 11 = η 11 \eta_{pp}=H-h_{pp}<H-h_{11}=\eta_{11} η pp = H − h pp < H − h 11 = η 11 . For a symmetric concave function, the derivatives are ordered oppositely to the eigenvalues; hence G p p ≥ G 11 G^{pp}\ge G^{11} G pp ≥ G 11 . Since G p p G^{pp} G pp is one of the terms in F 11 = ∑ j ≠ 1 G j j F^{11}=\sum_{j\ne1}G^{jj} F 11 = ∑ j = 1 G j j , we obtain F 11 ≥ G p p ≥ G 11 F^{11}\ge G^{pp}\ge G^{11} F 11 ≥ G pp ≥ G 11 . Consequently ∑ j G j j = G 11 + F 11 ≤ 2 F 11 \sum_{j}G^{jj}=G^{11}+F^{11}\le2F^{11} ∑ j G j j = G 11 + F 11 ≤ 2 F 11 , and therefore
F 11 = ∑ j ≠ 1 G j j ≥ 1 2 ∑ j G j j = 1 2 ( n − 1 ) ∑ i F i i . (46) F^{11}=\sum_{j\ne1}G^{jj}\ge\frac{1}{2}\sum_{j}G^{jj}=\frac{1}{2(n-1)}\sum_{i}F^{ii}. \tag*{(46)} F 11 = j = 1 ∑ G j j ≥ 2 1 j ∑ G j j = 2 ( n − 1 ) 1 i ∑ F ii . (46)
At X 0 X_{0} X 0 ,
w i i = − u i i u + u i 2 u 2 + γ ′ ′ ( ( ∣ X ∣ 2 ) i ) 2 + γ ′ ( ∣ X ∣ 2 ) i i . w_{ii}=-\frac{u_{ii}}{u}+\frac{u_{i}^{2}}{u^{2}}+\gamma''\bigl((|X|^{2})_{i}\bigr)^{2}+\gamma'(|X|^{2})_{ii}. w ii = − u u ii + u 2 u i 2 + γ ′′ ( ( ∣ X ∣ 2 ) i ) 2 + γ ′ ( ∣ X ∣ 2 ) ii .
Because ( ∣ X ∣ 2 ) i = 2 ⟨ X , e i ⟩ (|X|^{2})_{i}=2\langle X,e_{i}\rangle ( ∣ X ∣ 2 ) i = 2 ⟨ X , e i ⟩ and only the i = 1 i=1 i = 1 tangential component is nonzero, the first derivative relation gives
u 1 2 u 2 = 4 γ ′ 2 ⟨ X , e 1 ⟩ 2 , u i = 0 ( i ≥ 2 ) . \frac{u_{1}^{2}}{u^{2}}=4\gamma'^{2}\langle X,e_{1}\rangle^{2},\qquad u_{i}=0\quad(i\ge2). u 2 u 1 2 = 4 γ ′ 2 ⟨ X , e 1 ⟩ 2 , u i = 0 ( i ≥ 2 ) .
Multiplying by F i i F^{ii} F ii and using F i i w i i ≤ 0 F^{ii}w_{ii}\le0 F ii w ii ≤ 0 yields
0 ≥ − F i i u i i u + 4 ( γ ′ 2 + γ ′ ′ ) F 11 ⟨ X , e 1 ⟩ 2 + γ ′ F i i ( ∣ X ∣ 2 ) i i . (47) 0\ge-\frac{F^{ii}u_{ii}}{u}+4(\gamma'^{2}+\gamma'')F^{11}\langle X,e_{1}\rangle^{2}+\gamma'F^{ii}(|X|^{2})_{ii}. \tag*{(47)} 0 ≥ − u F ii u ii + 4 ( γ ′ 2 + γ ′′ ) F 11 ⟨ X , e 1 ⟩ 2 + γ ′ F ii ( ∣ X ∣ 2 ) ii . (47)
By (21) ,
F i i u i i = ∑ k ⟨ X , e k ⟩ F i i h i i , k − u F i i h i i 2 + ∑ i F i i h i i . F^{ii}u_{ii}=\sum_{k}\langle X,e_{k}\rangle F^{ii}h_{ii,k}-uF^{ii}h_{ii}^{2}+\sum_{i}F^{ii}h_{ii}. F ii u ii = k ∑ ⟨ X , e k ⟩ F ii h ii , k − u F ii h ii 2 + i ∑ F ii h ii .
Only k = 1 k=1 k = 1 contributes to the first sum. Using (23) and (8) therefore gives
F i i u i i = ⟨ X , e 1 ⟩ ( d X f ~ ) ( e 1 ) + h 11 ⟨ X , e 1 ⟩ ( d ν f ~ ) ( e 1 ) − u F i i h i i 2 + f ~ − R α . F^{ii}u_{ii}=\langle X,e_{1}\rangle(d_{X}\tilde f)(e_{1})+h_{11}\langle X,e_{1}\rangle(d_{\nu}\tilde f)(e_{1})-uF^{ii}h_{ii}^{2}+\tilde f-R_{\alpha}. F ii u ii = ⟨ X , e 1 ⟩ ( d X f ~ ) ( e 1 ) + h 11 ⟨ X , e 1 ⟩ ( d ν f ~ ) ( e 1 ) − u F ii h ii 2 + f ~ − R α .
Similarly, from ( ∣ X ∣ 2 ) i i = 2 ( 1 − u h i i ) (|X|^{2})_{ii}=2(1-uh_{ii}) ( ∣ X ∣ 2 ) ii = 2 ( 1 − u h ii ) ,
F i i ( ∣ X ∣ 2 ) i i = 2 ∑ i F i i − 2 u ( f ~ − R α ) . F^{ii}(|X|^{2})_{ii}=2\sum_{i}F^{ii}-2u(\tilde f-R_{\alpha}). F ii ( ∣ X ∣ 2 ) ii = 2 i ∑ F ii − 2 u ( f ~ − R α ) .
The radial condition for f t f_t f t is k f t + ( d X f t ) ( X ) ≤ 0 k f_t+(d_Xf_t)(X)\le0 k f t + ( d X f t ) ( X ) ≤ 0 . Since f ~ = f t 1 / k \tilde f=f_t^{1/k} f ~ = f t 1/ k ,
f ~ + ( d X f ~ ) ( X ) = 1 k f t 1 / k − 1 ( k f t + ( d X f t ) ( X ) ) ≤ 0. \tilde f+(d_X\tilde f)(X)=\frac{1}{k}f_t^{1/k-1}\bigl(kf_t+(d_Xf_t)(X)\bigr)\le0. f ~ + ( d X f ~ ) ( X ) = k 1 f t 1/ k − 1 ( k f t + ( d X f t ) ( X ) ) ≤ 0.
Since at X 0 X_0 X 0 ,
X = ⟨ X , e 1 ⟩ e 1 + u ν , X=\langle X,e_1\rangle e_1+u\nu, X = ⟨ X , e 1 ⟩ e 1 + uν ,
the preceding radial inequality gives
− ⟨ X , e 1 ⟩ ( d X f ~ ) ( e 1 ) + f ~ u ≥ ( d X f ~ ) ( ν ) . -\frac{\langle X,e_1\rangle(d_X\tilde f)(e_1)+\tilde f}{u}\ge(d_X\tilde f)(\nu). − u ⟨ X , e 1 ⟩ ( d X f ~ ) ( e 1 ) + f ~ ≥ ( d X f ~ ) ( ν ) .
Also h 11 = 2 γ ′ u h_{11}=2\gamma'u h 11 = 2 γ ′ u , so the normal-derivative contribution satisfies
− h 11 ⟨ X , e 1 ⟩ u ( d ν f ~ ) ( e 1 ) = − 2 γ ′ ⟨ X , e 1 ⟩ ( d ν f ~ ) ( e 1 ) , -\frac{h_{11}\langle X,e_1\rangle}{u}(d_\nu\tilde f)(e_1)=-2\gamma'\langle X,e_1\rangle(d_\nu\tilde f)(e_1), − u h 11 ⟨ X , e 1 ⟩ ( d ν f ~ ) ( e 1 ) = − 2 γ ′ ⟨ X , e 1 ⟩ ( d ν f ~ ) ( e 1 ) ,
which is bounded below by − C ∣ γ ′ ∣ -C|\gamma'| − C ∣ γ ′ ∣ . The terms F i i h i i 2 F^{ii}h_{ii}^2 F ii h ii 2 and R α / u R_\alpha/u R α / u in − F i i u i i / u -F^{ii}u_{ii}/u − F ii u ii / u are nonnegative and may be discarded. Finally,
γ ′ F i i ( ∣ X ∣ 2 ) i i = 2 γ ′ ∑ i F i i − 2 u γ ′ f ~ + 2 u γ ′ R α . \gamma'F^{ii}(|X|^2)_{ii}=2\gamma'\sum_iF^{ii}-2u\gamma'\tilde f+2u\gamma'R_\alpha. γ ′ F ii ( ∣ X ∣ 2 ) ii = 2 γ ′ i ∑ F ii − 2 u γ ′ f ~ + 2 u γ ′ R α .
Since γ ′ < 0 \gamma'<0 γ ′ < 0 , the middle term is nonnegative, whereas (10) bounds the last term below by − C α ∣ γ ′ ∣ ∑ i F i i -C\alpha|\gamma'|\sum_iF^{ii} − C α ∣ γ ′ ∣ ∑ i F ii . The remaining first derivatives of f ~ \tilde f f ~ are uniformly bounded because f t f_t f t has a uniform positive lower bound and a uniform C 1 C^1 C 1 norm. Substituting all these estimates into (47) yields
0 ≥ 4 ( γ ′ 2 + γ ′ ′ ) F 11 ⟨ X , e 1 ⟩ 2 − C ∣ γ ′ ∣ ( 1 + α ) ∑ i F i i − C ( 1 + ∣ γ ′ ∣ ) . (48) 0\ge4(\gamma'^2+\gamma'')F^{11}\langle X,e_1\rangle^2-C|\gamma'|(1+\alpha)\sum_iF^{ii}-C(1+|\gamma'|). \tag*{(48)} 0 ≥ 4 ( γ ′2 + γ ′′ ) F 11 ⟨ X , e 1 ⟩ 2 − C ∣ γ ′ ∣ ( 1 + α ) i ∑ F ii − C ( 1 + ∣ γ ′ ∣ ) . (48)
If
⟨ X , e 1 ⟩ 2 < 1 2 r 1 2 , \langle X,e_1\rangle^2<\frac{1}{2}r_1^2, ⟨ X , e 1 ⟩ 2 < 2 1 r 1 2 ,
then u 2 = ∣ X ∣ 2 − ⟨ X , e 1 ⟩ 2 ≥ r 2 2 / 2 u^2=|X|^2-\langle X,e_1\rangle^2\ge r_2^2/2 u 2 = ∣ X ∣ 2 − ⟨ X , e 1 ⟩ 2 ≥ r 2 2 /2 , and again there is nothing to prove. Otherwise, since s = ∣ X ∣ s=|X| s = ∣ X ∣ lies in the fixed interval [ r 1 , r 2 ] [r_1,r_2] [ r 1 , r 2 ] and γ ( s ) = L / s \gamma(s)=L/s γ ( s ) = L / s ,
γ ′ = − L s 2 , γ ′ ′ = 2 L s 3 , \gamma'=-\frac{L}{s^2},\qquad\gamma''=\frac{2L}{s^3}, γ ′ = − s 2 L , γ ′′ = s 3 2 L ,
so
γ ′ 2 + γ ′ ′ ≥ c L 2 , ∣ γ ′ ∣ ≤ C L . \gamma'^2+\gamma''\ge cL^2,\qquad|\gamma'|\le CL. γ ′2 + γ ′′ ≥ c L 2 , ∣ γ ′ ∣ ≤ C L .
Using (46) and Lemma 2.2, (48) becomes
0 ≥ [ c L 2 − C L ( 1 + α ) ] ∑ i F i i − C ( 1 + L ) . 0\ge[cL^2-CL(1+\alpha)]\sum_iF^{ii}-C(1+L). 0 ≥ [ c L 2 − C L ( 1 + α )] i ∑ F ii − C ( 1 + L ) .
Because ∑ i F i i ≥ c n , k > 0 \sum_iF^{ii}\ge c_{n,k}>0 ∑ i F ii ≥ c n , k > 0 , the right-hand side is positive for L L L sufficiently large, a contradiction. Thus u ≥ c > 0 u\ge c>0 u ≥ c > 0 . Finally, from
u = ρ 2 ρ 2 + ∣ ∇ ρ ∣ 2 u=\frac{\rho^2}{\sqrt{\rho^2+|\nabla\rho|^2}} u = ρ 2 + ∣∇ ρ ∣ 2 ρ 2
and the C 0 C^0 C 0 bounds on ρ \rho ρ ,
∣ ∇ ρ ∣ 2 = ρ 4 u 2 − ρ 2 ≤ C . |\nabla\rho|^2=\frac{\rho^4}{u^2}-\rho^2\le C. ∣∇ ρ ∣ 2 = u 2 ρ 4 − ρ 2 ≤ C .
Hence
∣ ∇ ρ ∣ ≤ C . (49) |\nabla\rho|\le C. \tag*{(49)} ∣∇ ρ ∣ ≤ C . (49)
C2 estimate
The estimates (45) and (49) give uniform upper and lower bounds for ρ \rho ρ and a uniform bound for ∣ ∇ ρ ∣ |\nabla\rho| ∣∇ ρ ∣ . By (11) this controls the first fundamental form, its inverse, the support function, and the C 1 C^1 C 1 geometry entering the constant in Theorem 1.1 . Moreover, since f t = t f + ( 1 − t ) f 0 f_t=tf+(1-t)f_0 f t = t f + ( 1 − t ) f 0 and the annulus r 1 ≤ ∣ X ∣ ≤ r 2 r_1\leq|X|\leq r_2 r 1 ≤ ∣ X ∣ ≤ r 2 is fixed,
inf f t ≥ c > 0 , ∥ f t ∥ C 2 ≤ C \inf f_t\geq c>0,\qquad\|f_t\|_{C^2}\leq C inf f t ≥ c > 0 , ∥ f t ∥ C 2 ≤ C
uniformly for t ∈ [ 0 , 1 ] t\in[0,1] t ∈ [ 0 , 1 ] . Hence all quantities on which the curvature estimate depends are uniform along the path. Theorem 1.1 therefore yields
max M t max 1 ≤ i ≤ n ∣ κ i ∣ ≤ C . \max_{M_t}\max_{1\leq i\leq n}|\kappa_i|\leq C. M t max 1 ≤ i ≤ n max ∣ κ i ∣ ≤ C .
Thus the second fundamental form of M t M_t M t is uniformly bounded.
It remains to translate this geometric curvature bound into a C 2 C^2 C 2 estimate for the radial function. Writing
W = ρ 2 + ∣ ∇ ρ ∣ 2 , W=\sqrt{\rho^2+|\nabla\rho|^2}, W = ρ 2 + ∣∇ ρ ∣ 2 ,
the radial graph formula (11) gives
ρ i j = ρ g ^ i j + 2 ρ ρ i ρ j − W ρ h i j . \rho_{ij}=\rho\widehat{g}_{ij}+\frac{2}{\rho}\rho_i\rho_j-\frac{W}{\rho}h_{ij}. ρ ij = ρ g ij + ρ 2 ρ i ρ j − ρ W h ij .
The C 0 C^0 C 0 and C 1 C^1 C 1 estimates make g g g and g ^ \widehat{g} g uniformly equivalent, so a bound for the second fundamental form with respect to g g g gives a bound for its coordinate components in a g ^ \widehat{g} g -orthonormal frame. The factors W / ρ W/\rho W / ρ and 2 / ρ 2/\rho 2/ ρ in the preceding identity are also uniformly bounded. Hence
∣ ∇ 2 ρ ∣ ≤ C , |\nabla^2\rho|\leq C, ∣ ∇ 2 ρ ∣ ≤ C ,
and therefore
∥ ρ ∥ C 2 ( S n ) ≤ C \|\rho\|_{C^2(S^n)}\leq C ∥ ρ ∥ C 2 ( S n ) ≤ C
uniformly for all admissible solutions along the path.
We also record why this gives uniform ellipticity. The curvature bound makes λ ^ = ( λ ( η ) , α ) \widehat{\lambda}=(\lambda(\eta),\alpha) λ = ( λ ( η ) , α ) uniformly bounded. Moreover σ k ( λ ^ ) = f t ≥ c > 0 \sigma_k(\widehat{\lambda})=f_t\geq c>0 σ k ( λ ) = f t ≥ c > 0 . Since λ ^ ∈ Γ k n + 1 \widehat{\lambda}\in\Gamma_k^{n+1} λ ∈ Γ k n + 1 , Newton–Maclaurin gives positive lower bounds for the lower symmetric functions σ j ( λ ^ ) \sigma_j(\widehat{\lambda}) σ j ( λ ) , 1 ≤ j < k 1\leq j<k 1 ≤ j < k , in terms of the lower bound for σ k \sigma_k σ k . Thus λ ^ \widehat{\lambda} λ stays a positive distance away from ∂ Γ k n + 1 \partial\Gamma_k^{n+1} ∂ Γ k n + 1 and hence in a compact subset of Γ k n + 1 \Gamma_k^{n+1} Γ k n + 1 . The linearized coefficients are therefore bounded above and below uniformly, so the equation is uniformly elliptic along the continuity path.
Existence
Let
I = { t ∈ [ 0 , 1 ] : S k , α ( λ ( η ) ) = f t ( X , ν ) has an admissible star-shaped solution } . \mathcal{I}=\{t\in[0,1]:S_{k,\alpha}(\lambda(\eta))=f_t(X,\nu)\text{ has an admissible star-shaped solution}\}. I = { t ∈ [ 0 , 1 ] : S k , α ( λ ( η )) = f t ( X , ν ) has an admissible star-shaped solution } .
By construction, 0 ∈ I 0\in\mathcal{I} 0 ∈ I , with the unit sphere as the corresponding solution.
We first prove openness. Write ρ = e v \rho=e^v ρ = e v . The principal curvatures have the form
κ i = e − v κ ‾ i ( D v , D 2 v ) , \kappa_i=e^{-v}\overline{\kappa}_i(Dv,D^2v), κ i = e − v κ i ( D v , D 2 v ) ,
and therefore
λ i ( η ) = e − v λ ‾ i ( D v , D 2 v ) . \lambda_i(\eta)=e^{-v}\overline{\lambda}_i(Dv,D^2v). λ i ( η ) = e − v λ i ( D v , D 2 v ) .
After multiplying the equation by e k v e^{kv} e k v , we obtain
σ k ( λ ‾ ) + α e v σ k − 1 ( λ ‾ ) = e k v f t ( e v x , ν ( D v ) ) . \sigma_k(\overline{\lambda})+\alpha e^v\sigma_{k-1}(\overline{\lambda})=e^{kv}f_t(e^v x,\nu(Dv)). σ k ( λ ) + α e v σ k − 1 ( λ ) = e k v f t ( e v x , ν ( D v )) .
Define
P [ v ] : = e k v f t ( e v x , ν ( D v ) ) − σ k ( λ ‾ ) − α e v σ k − 1 ( λ ‾ ) . \mathcal{P}[v]:=e^{kv}f_t(e^v x,\nu(Dv))-\sigma_k(\overline{\lambda})-\alpha e^v\sigma_{k-1}(\overline{\lambda}). P [ v ] := e k v f t ( e v x , ν ( D v )) − σ k ( λ ) − α e v σ k − 1 ( λ ) .
For fixed ( v , D v ) (v,Dv) ( v , D v ) , the radial graph formula shows that the matrix determining the principal curvatures depends affinely on − D 2 v -D^2v − D 2 v through a positive definite change of basis. Since S k , α 1 / k S_{k,\alpha}^{1/k} S k , α 1/ k is elliptic on the admissible set, the above sign convention makes P \mathcal{P} P elliptic with respect to D 2 v D^2v D 2 v . Holding D v Dv D v and D 2 v D^2v D 2 v fixed, we have
P v = e k v ( k f t + ( d X f t ) ( X ) ) − α e v σ k − 1 ( λ ‾ ) = ρ ∂ ∂ ρ ( ρ k f t ) − α e v σ k − 1 ( λ ‾ ) < 0. (50) \begin{aligned}
\mathcal{P}_v&=e^{kv}\bigl(kf_t+(d_Xf_t)(X)\bigr)-\alpha e^v\sigma_{k-1}(\overline{\lambda})\\
&=\rho\frac{\partial}{\partial\rho}(\rho^k f_t)-\alpha e^v\sigma_{k-1}(\overline{\lambda})<0. \tag*{(50)}
\end{aligned} P v = e k v ( k f t + ( d X f t ) ( X ) ) − α e v σ k − 1 ( λ ) = ρ ∂ ρ ∂ ( ρ k f t ) − α e v σ k − 1 ( λ ) < 0. (50)
The strict inequality follows from (4) , α > 0 \alpha>0 α > 0 , and admissibility: positive scaling preserves Γ k − 1 \Gamma_{k-1} Γ k − 1 , so σ k − 1 ( λ ‾ ) > 0 \sigma_{k-1}(\overline{\lambda})>0 σ k − 1 ( λ ) > 0 . At a fixed solution the linearization therefore has the form
L φ = a i j ∇ i j φ + b i ∇ i φ + c φ , ( a i j ) > 0 , c < 0. L\varphi=a^{ij}\nabla_{ij}\varphi+b^i\nabla_i\varphi+c\varphi,\qquad(a^{ij})>0,\qquad c<0. L φ = a ij ∇ ij φ + b i ∇ i φ + c φ , ( a ij ) > 0 , c < 0.
The coefficients are uniformly elliptic at that solution because admissibility is an open condition. If L φ = 0 L\varphi=0 L φ = 0 , the maximum principle applied to the positive maximum and negative minimum of φ \varphi φ gives φ ≡ 0 \varphi\equiv0 φ ≡ 0 ; hence the kernel is trivial. As a second-order elliptic operator on the closed manifold S n S^n S n , L : C 2 , β → C 0 , β L:C^{2,\beta}\to C^{0,\beta} L : C 2 , β → C 0 , β is Fredholm of index zero, so trivial kernel implies surjectivity and therefore invertibility. The implicit function theorem then shows that I \mathcal{I} I is open.
To prove closedness, let t j ∈ I t_j\in\mathcal{I} t j ∈ I and t j → t ∞ t_j\to t_\infty t j → t ∞ , and write the corresponding solutions as ρ j = e v j \rho_j=e^{v_j} ρ j = e v j . The estimates in Subsections 4.1–4.3 give a uniform C 2 C^2 C 2 bound for v j v_j v j and keep the augmented eigenvalues in a fixed compact subset of Γ k n + 1 \Gamma_k^{n+1} Γ k n + 1 . Thus the equations are uniformly elliptic with uniform ellipticity constants. Rewrite the equation in the equivalent form
[ σ k ( λ ‾ ) + α e v σ k − 1 ( λ ‾ ) ] 1 / k = e v f t ( e v x , ν ( D v ) ) 1 / k . \left[\sigma_k(\overline{\lambda})+\alpha e^v\sigma_{k-1}(\overline{\lambda})\right]^{1/k}=e^v f_t(e^v x,\nu(Dv))^{1/k}. [ σ k ( λ ) + α e v σ k − 1 ( λ ) ] 1/ k = e v f t ( e v x , ν ( D v ) ) 1/ k .
For fixed ( x , v , D v ) (x,v,Dv) ( x , v , D v ) , the left-hand side is concave in D 2 v D^2v D 2 v ; it is the restriction of σ k 1 / k \sigma_k^{1/k} σ k 1/ k to the augmented vector ( λ ‾ , α e v ) (\overline{\lambda},\alpha e^v) ( λ , α e v ) , with α e v \alpha e^v α e v fixed, and the curvature matrix is affine in − D 2 v -D^2v − D 2 v after a positive change of basis. The left-hand side is decreasing with respect to D 2 v D^2v D 2 v in the sense of the ordering of symmetric matrices. Thus, with the standard convention that elliptic operators are increasing in D 2 v D^2v D 2 v , we use the equivalent equation Q [ v ] = 0 \mathcal{Q}[v]=0 Q [ v ] = 0 , where
Q [ v ] : = e v f t ( e v x , ν ( D v ) ) 1 / k − [ σ k ( λ ‾ ) + α e v σ k − 1 ( λ ‾ ) ] 1 / k . \mathcal{Q}[v]:=e^v f_t(e^v x,\nu(Dv))^{1/k}-\left[\sigma_k(\overline{\lambda})+\alpha e^v\sigma_{k-1}(\overline{\lambda})\right]^{1/k}. Q [ v ] := e v f t ( e v x , ν ( D v ) ) 1/ k − [ σ k ( λ ) + α e v σ k − 1 ( λ ) ] 1/ k .
The operator Q \mathcal{Q} Q is convex and uniformly elliptic in D 2 v D^2v D 2 v on the uniformly admissible solution family. The Evans–Krylov regularity theory [4 , 8 ] therefore gives
∥ v j ∥ C 2 , θ ( S n ) ≤ C \lVert v_j\rVert_{C^{2,\theta}(S^n)}\le C ∥ v j ∥ C 2 , θ ( S n ) ≤ C
for some $0<\theta<1$. Differentiating the equation gives a uniformly elliptic linear equation for the first derivatives of v j v_j v j whose coefficients are C θ C^\theta C θ ; Schauder estimates then give the C 3 , θ C^{3,\theta} C 3 , θ bound needed for compactness (and, by the assumed C 2 C^2 C 2 regularity of f t f_t f t , the stated C 3 , β C^{3,\beta} C 3 , β regularity for every $\beta<1 after the standard bootstrap on slightly smaller Hölder exponents). Hence a subsequence converges in C 3 , β ′ C^{3,\beta'} C 3 , β ′ for every β ′ < β \beta' < \beta β ′ < β to a solution at t = t ∞ t = t_{\infty} t = t ∞ . The compact containment in the admissible cone shows that admissibility is preserved in the limit. Therefore I \mathcal{I} I is closed, and hence
I = [ 0 , 1 ] , \mathcal{I} = [0,1], I = [ 0 , 1 ] ,
and in particular a solution exists for t = 1 t = 1 t = 1 .
Uniqueness
Let v 1 v_1 v 1 and v 2 v_2 v 2 be two admissible solutions of the equation at t = 1 t = 1 t = 1 . Suppose, toward a contradiction, that w = v 1 − v 2 w = v_1 - v_2 w = v 1 − v 2 has a positive maximum at x 0 x_0 x 0 . Then
D v 1 ( x 0 ) = D v 2 ( x 0 ) , D 2 v 1 ( x 0 ) ≤ D 2 v 2 ( x 0 ) Dv_1(x_0) = Dv_2(x_0), \qquad D^2v_1(x_0) \leq D^2v_2(x_0) D v 1 ( x 0 ) = D v 2 ( x 0 ) , D 2 v 1 ( x 0 ) ≤ D 2 v 2 ( x 0 )
as quadratic forms. Keeping the common gradient and the value v 1 ( x 0 ) v_1(x_0) v 1 ( x 0 ) fixed, ellipticity of P \mathcal{P} P in the Hessian variable gives
P ( v 1 , D v 1 , D 2 v 1 ) ≤ P ( v 1 , D v 2 , D 2 v 2 ) . \mathcal{P}(v_1,Dv_1,D^2v_1) \leq\mathcal{P}(v_1,Dv_2,D^2v_2). P ( v 1 , D v 1 , D 2 v 1 ) ≤ P ( v 1 , D v 2 , D 2 v 2 ) .
Now keep ( D v 2 , D 2 v 2 ) (Dv_2,D^2v_2) ( D v 2 , D 2 v 2 ) fixed. The barred eigenvalues λ ‾ ( D v 2 , D 2 v 2 ) \overline{\lambda}(Dv_2,D^2v_2) λ ( D v 2 , D 2 v 2 ) are independent of the zeroth-order variable v v v and belong to Γ k − 1 \Gamma_{k-1} Γ k − 1 because v 2 v_2 v 2 is admissible. Hence (50) is strictly negative for every v v v between v 2 ( x 0 ) v_2(x_0) v 2 ( x 0 ) and v 1 ( x 0 ) v_1(x_0) v 1 ( x 0 ) . Since v 1 ( x 0 ) > v 2 ( x 0 ) v_1(x_0) > v_2(x_0) v 1 ( x 0 ) > v 2 ( x 0 ) ,
P ( v 1 , D v 2 , D 2 v 2 ) < P ( v 2 , D v 2 , D 2 v 2 ) . \mathcal{P}(v_1,Dv_2,D^2v_2) < \mathcal{P}(v_2,Dv_2,D^2v_2). P ( v 1 , D v 2 , D 2 v 2 ) < P ( v 2 , D v 2 , D 2 v 2 ) .
Both endpoints are solutions, so altogether
0 = P [ v 1 ] ( x 0 ) < P [ v 2 ] ( x 0 ) = 0 , 0 = \mathcal{P}[v_1](x_0) < \mathcal{P}[v_2](x_0) = 0, 0 = P [ v 1 ] ( x 0 ) < P [ v 2 ] ( x 0 ) = 0 ,
a contradiction. Therefore v 1 ≤ v 2 v_1 \leq v_2 v 1 ≤ v 2 . Reversing the roles of the two solutions gives v 2 ≤ v 1 v_2 \leq v_1 v 2 ≤ v 1 , and hence v 1 = v 2 v_1 = v_2 v 1 = v 2 . This proves uniqueness and completes the proof of Theorem 1.2.
Acknowledgments. Peihe Wang is supported by National Natural Science Foundation of Shandong Province(ZR2026MS0039). Hua Zhu is supported by the National Natural Science Foundation of China (Grant Nos. 12501273 and 12661041).