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Generic Properties of Critical Points of the Weyl Tensor

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Published/Copyright: January 4, 2017

Abstract

Given (M,g), a smooth compact Riemannian n-manifold, we prove that for a generic Riemannian metric g the critical points of the function 𝒲g⁢(ξ):=|Weylg⁢(ξ)|g2 with 𝒲g⁢(ξ)≠0 are nondegenerate.

MSC 2010: 58J60; 53C21

1 Introduction

Let (M,g) be a connected compact Riemannian manifold of dimension n≥3 without boundary.

The curvature tensor is a map Riem:𝔛⁢(M)3→𝔛⁢(M) defined by

Riem ⁢ ( X , Y ) ⁢ Z = ∇ X ⁡ ∇ Y ⁡ Z - ∇ Y ⁡ ∇ X ⁡ Z - [ ∇ X , ∇ Y ] ⁢ Z ,

where 𝔛⁢(M) denotes the space of smooth vector fields and [⋅,⋅] is the Lie bracket. The Weyl tensorWeylg is a conformally invariant tensor which is obtained from the full curvature tensor by subtracting out various traces. In a local coordinate system it reads as

W i ⁢ j ⁢ k ⁢ l = R i ⁢ j ⁢ k ⁢ l - g i ⁢ k ⁢ A j ⁢ l + g i ⁢ l ⁢ A j ⁢ k + g j ⁢ k ⁢ A i ⁢ l - g j ⁢ l ⁢ A i ⁢ k ,

where the Riemann tensor is given by

R i ⁢ j ⁢ k ⁢ l = g k ⁢ m ⁢ R i ⁢ j ⁢ l m   and   R i ⁢ j ⁢ l m = Riem ⁢ ( ∂ ∂ ⁡ x i , ∂ ∂ ⁡ x j ) ⁢ ∂ ∂ ⁡ x l ⊗ ∂ ∂ ⁡ x m ,

the Schouten curvature tensor is

A i ⁢ j = 1 ( n - 2 ) ⁢ ( R i ⁢ j - 1 2 ⁢ ( n - 1 ) ⁢ R ⁢ g i ⁢ j ) ,

the Ricci curvature tensorRic is the contraction of Riem, i.e. Ri⁢j=gk⁢l⁢Ri⁢k⁢j⁢l and the scalar curvatureRg is the contraction of Ric, i.e. Rg=gi⁢j⁢Ri⁢j.

Let ℳk be the set of all Ck Riemannian metrics on M with k≥4. Any g∈ℳk determines the Weyl tensor Weylg of (M,g). Set

(1.1) 𝒲 g ⁢ ( ξ ) := | Weyl g ⁢ ( ξ ) | g 2 .

We assume that M is such that the set

𝒟 k := { g ∈ ℳ k : 𝒲 g ⁢ ( ξ ) ≠ 0 ⁢ for any ⁢ ξ ∈ M }

is a non-empty open subset of ℳk. Examples of manifolds with 𝒟k non-empty are given by the product of round spheres, i.e. the product manifold (𝕊n×𝕊m,g𝕊n⊗g𝕊m).

Our goal is to prove that for generic Riemannian metrics g∈𝒟k the critical points of the function 𝒲g are nondegenerate. More precisely, we will prove the following result.

Theorem 1.1

The set

𝒜 := { g ∈ 𝒟 k : all critical points of 𝒲 g are nondegenerate }

is an open dense subset of Dk.

Our result is motivated by the study of compactness of solutions to a linear perturbation of the Yamabe equation. Yamabe [21] asked the question if it is possible to find a metric g~ in the conformal class of g with constant scalar curvature. If g~=u4N-2⁢g, where u is a positive smooth function on M, the problem turns out to be equivalent to find a positive solution to the elliptic problem

(1.2) ℒ g ⁢ u + κ ⁢ u n + 2 n - 2 = 0   in ⁢ M

for some constant κ. Here ℒg⁢u:=Δg⁢u-n-24⁢(n-1)⁢Rg⁢u is the conformal Laplacian, Δg is the Laplace–Beltrami operator and Rg is the scalar curvature of g. If u solves problem (1.2), the scalar curvature of the metric g~ is 4⁢(n-1)n-2⁢κ. The Yamabe problem has been completely solved by Yamabe [21], Aubin [1], Trudinger [19] and Schoen [15] (see also the proof given by Bahri [2]).

Once the problem is solved, a second question concerns the structure of the set of the metrics conformally equivalent to g with constant scalar curvature or equivalently the set of solutions to the elliptic problem (1.2). The solution is unique in the case of negative scalar curvature and it is unique (up to a constant factor) in the case of zero scalar curvature. The uniqueness is not true anymore in the case of positive scalar curvature, as was proved by Schoen [17, 18] and Pollack [11] who exhibited examples where a large number of high energy solutions of (1.2) with high Morse index exist. Thus it is natural to ask if the set of solutions of (1.2) is compact or not as was raised by Schoen [16]. Obata [10] proved that compactness does not hold in the case of the round sphere (𝕊n,g𝕊n). Indeed, the Yamabe problem (1.2) turns out to be equivalent (via the stereographic projection) to the equation in the Euclidean space

- Δ ⁢ U = U n + 2 n - 2   in ⁢ ℝ n ,

which has infinitely many solutions, the so-called standard bubbles,

(1.3) U μ , y ⁢ ( x ) = μ - n - 2 2 ⁢ U ⁢ ( x - y μ ) , x , y ∈ ℝ n , μ > 0 , where ⁢ U ⁢ ( x ) := α N ⁢ 1 ( 1 + | x | 2 ) n - 2 2 .

Here αn:=[n⁢(n-2)]n-24. The study of compactness in a manifold which is not locally conformally equivalent to the round sphere is a delicate issue. Khuri, Marques and Schoen [7] proved that the compactness holds when the dimension n of the manifold satisfies 3≤n≤24, while it fails when n≥25 thanks to the examples built by Brendle [3] and Brendle and Marques [4]. The proof of compactness strongly relies on proving sharp pointwise estimates at a blow-up point of the solution. In particular, when compactness holds, every sequence of unbounded solutions to (1.2) must blow-up at some points of the manifold which are necessarily isolated and simple, i.e. around each blow-up point ξ0, the solution can be approximated by a standard bubble (see (1.3))

u n ⁢ ( x ) ∼ μ m n - 2 2 ( μ n 2 + ( d g ⁢ ( x , ξ m ) ) 2 ) N - 2 2   for some ξ m → ξ 0 and μ m → 0 .

More precisely, let um be a sequence of solutions to problem (1.2). We say that um blows up at a point ξ0∈M if there exists ξm∈M such that ξm→ξ0⁢and⁢um⁢(ξm)→+∞. The point ξ0 is said to be a blow-up point for um. Blow-up points can be classified according to the definitions introduced by Schoen [16]. The point ξ0∈M is an isolated blow-up point for um if there exists ξm∈M such that ξm is a local maximum of um, ξm→ξ0, um⁢(ξm)→+∞, and there exist c>0 and R>0 such that

0 < u m ⁢ ( x ) ≤ c ⁢ 1 d g ⁢ ( x , ξ m ) n - 2 2   for any ⁢ x ∈ B ⁢ ( ξ 0 , R ) .

Moreover, Ξ0∈M is an isolated simple blow-up point for um if the function

u ^ m ⁢ ( r ) := r n - 2 2 ⁢ 1 | ∂ ⁡ B ⁢ ( ξ m , r ) | g ⁢ ∫ ∂ ⁡ B ⁢ ( ξ m , r ) u m ⁢ 𝑑 σ g

has exactly one critical point in (0,R).

Motivated by the previous observations, we are interested in studying the compactness of solutions to a linear perturbation of the Yamabe problem

(1.4) - ℒ g ⁢ u + ϵ ⁢ u = u n + 2 n - 2 , u > 0 , in ⁢ ( M , g ) ,

where the first eigenvalue of -ℒg is positive and ϵ is a small parameter. In particular, we address the questions of the existence of solutions blowing-up at a point ξ0 as ϵ goes to zero and the nature of the blow-up point ξ0, namely ξ0 can be either a clustering blow-up point (a non-isolated blow-up point) or a towering blow-up point (a non-isolated simple blow-up point).

Problem (1.4) does not have any blowing-up solutions when ϵ<0 as proved by Druet [5] in the low-dimensional case, i.e. n=3,4,5 (except when the manifold is conformally equivalent to the round sphere). In the high-dimensional case, i.e. n≥6, the problem is still open. The situation is completely different when ϵ>0. Indeed, if n=3, no blowing-up solutions exist as proved by Li–Zhu [8], while if n≥4 blowing-up solutions do exist as showed by Esposito, Pistoia and Vetois [6]. In particular, if the dimension n≥7 and the manifold is not locally conformally flat, in [6] blowing-up solutions are built whose blow-up point is a nondegenerate critical point ξ0 of the function 𝒲g defined in (1.1) with 𝒲g⁢(ξ0)≠0. Moreover, ξ0 turns out to be a clustering blow-up point as soon as it is a nondegenerate minimum point of 𝒲g with 𝒲g⁢(ξ0)≠0 as proved by Pistoia and Vaira [12]. We strongly believe that ξ0 is also a towering blow-up point, as suggested by a recent result obtained by Morabito, Pistoia and Vaira [9] under the additional assumption that M is symmetric with respect to the point ξ0. We also point out that if ξ0 is either a clustering or a towering blow-up point, an arbitrary large number of solutions blowing-up at ξ0 do exist as was shown in [12] and in [9]. Therefore, the existence and multiplicity of blowing-up solutions to problem (1.4) strictly rely on the existence of nondegenerate critical points of the function 𝒲g defined in (1.1) having a corresponding non-vanishing critical value.

The proof of Theorem 1.1 relies on a transversality argument (see Theorem 2.1) and it is carried out in Section 2. Section 3 contains the proof of the crucial transversality condition.

2 Formulation of the Problem and Proof of the Main Result

We denote by 𝒮k the space of all Ck symmetric covariant 2-tensors on M. It is a Banach space equipped with the norm ∥⋅∥k defined in the following way: We fix a finite covering {Vα}α∈L of M such that the closure of Vα is contained in Uα, where {Uα,ψα} is the open coordinate neighborhood. If h∈𝒮k, we denote by hi⁢j the components of h with respect to the coordinates (x1,…,xn) on Vα. We define

∥ h ∥ k := ∑ α ∈ L ∑ | β | ≤ k ∑ i , j = 1 n sup ψ α ⁢ ( V α ) ⁡ ∂ β ⁡ h i ⁢ j ∂ ⁡ x 1 β 1 ⁢ ⋯ ⁢ ∂ ⁡ x n β n .

The set ℳk of all Ck Riemannian metrics on M is an open set of 𝒮k.

In the following, we will assume k≥4.

Given g^∈ℳk, it is possible to define an atlas on M whose charts are (Bg^⁢(ξ,R),φ-1), where φ:B⁢(0,R)→Bg^⁢(ξ,R). Here Bg^⁢(ξ,R)⊂M is the ball centered at ξ with radius R given by the metric g^ and B⁢(0,R)⊂ℝn is the ball centered at 0 with radius R in the Euclidean space ℝn. Let ℬρ:={h∈𝒮k:∥h∥k<ρ} be the ball centered at 0 with radius ρ in 𝒮k.

For any ξ∈M and h∈ℬρ, with ρ small enough so that g^+h∈ℳk, we consider the Weyl curvature tensor Wg^+h⁢(ξ):=Weylg^+h⁢(ξ) of (M,g^+h) at the point ξ∈M whose components are Wa⁢b⁢c⁢dg^+h⁢(ξ). We introduce the function

𝒲 g ^ + h ( ξ ) : = | W g ^ + h ( ξ ) | g ^ + h 2
(2.1) = [ g ^ ⁢ ( Ξ ) + h ⁢ ( Ξ ) ] i ⁢ i ¯ ⁢ [ g ^ ⁢ ( Ξ ) + h ⁢ ( Ξ ) ] j ⁢ j ¯ ⁢ [ g ^ ⁢ ( Ξ ) + h ⁢ ( Ξ ) ] k ⁢ k ¯ ⁢ [ g ^ ⁢ ( Ξ ) + h ⁢ ( Ξ ) ] l ⁢ l ¯ ⁢ W i ⁢ j ⁢ k ⁢ l g ^ + h ⁢ ( Ξ ) ⁢ W i ¯ ⁢ j ¯ ⁢ k ¯ ⁢ l ¯ g ^ + h ⁢ ( Ξ ) .

Here and in the following, we use the Einstein summation convention, i.e. when an index variable appears twice in a single term, once in an upper (superscript) and/or in a lower (subscript) position, it implies that we are summing over all of its possible values.

Given ξ0∈M and the chart (Bg^⁢(ξ0,R),φ-1), we set

(2.2) 𝒲 ~ g ^ + h ⁢ ( x ) := 𝒲 g ^ + h ⁢ ( φ ⁢ ( x ) ) = | W g ^ + h ⁢ ( φ ⁢ ( x ) ) | g ^ + h 2   if ⁢ x ∈ B ⁢ ( 0 , R ) ⁢ and ⁢ h ∈ ℬ ρ .

Now, we introduce the C1-map F:ℬρ×B⁢(0,R)⊂𝒮k×ℝn→ℝn defined by

(2.3) F ⁢ ( h , x ) := ∇ x ⁡ 𝒲 ~ g ^ + h ⁢ ( x ) .

We shall apply to the map F an abstract transversality theorem (see [13, 14, 20]) which we recall from [14, Theorem 1.1].

Theorem 2.1

Let X,Y,Z be three real Banach spaces and let U⊂X, V⊂Y be open subsets. Let F:V×U→Z be a Ck-map with k≥1 such that the following conditions hold:

  1. For any y ∈ V , the map F ⁢ ( y , ⋅ ) : x → F ⁢ ( y , x ) is a Fredholm map of index l with l ≤ k .

  2. z 0 is a regular value of F , that is the operator F ′ ⁢ ( y 0 , x 0 ) : Y × X → Z is onto at any point ( y 0 , x 0 ) such that F ⁢ ( y 0 , x 0 ) = z 0 (the transversality condition ).

  3. The set of x ∈ U such that F ⁢ ( y , x ) = z 0 , with y in a compact set of X , is relatively compact in U.

Then the set

{ y ∈ V : z 0 ⁢ is a regular value of ⁢ F ⁢ ( y , ⋅ ) }

is a residual (hence dense) open subset of V.

By Theorem 2.1 we obtain the following result, which is crucial for deducing Theorem 1.1.

Theorem 2.2

For any g^∈Dk the set

{ h ∈ 𝒮 k : all critical points of 𝒲 g ^ + h are nondegenerate }

is a residual subset of a suitable ball centered at 0 with radius ρ in Sk.

Proof.

We are going to apply Theorem 2.1 to the map F defined in (2.3). In this case we have X=Z=ℝn and Y=𝒮k. We choose z0=0. Since X is a finite-dimensional space, it is easy to check that for any h∈ℬρ the map x↦F⁢(h,x) is Fredholm of index 0 and so assumption (i) holds. Moreover, assumption (iii) immediately follows again by the fact that X is a finite-dimensional space. Assumption (ii) is verified in Lemma 3.1.

Finally, we are in the position to apply Theorem 2.1 and we get that the set

Θ ⁢ ( ξ 0 , ρ ) := { h ∈ ℬ ρ : F x ′ ⁢ ( h , x ) : ℝ n → ℝ n ⁢ is invertible at any point ⁢ ( h , x ) ⁢ such that ⁢ F ⁢ ( h , x ) = 0 }
(2.4) = { h ∈ ℬ ρ : the critical points of 𝒲 g ^ + h in B g ^ ⁢ ( ξ 0 , R ) are nondegenerate }

is a residual subset of ℬρ.

Now, since M is compact, there exists a finite covering {Bg^⁢(ξi,R)}i=1,…,ν of M, where ξ1,…,ξν∈M. For any index i there exists an open dense subset Θ⁢(ξi,ρ) (see (2.4)) of ℬρ such that the critical points of 𝒲g^+h in Bg^⁢(ξi,R) are nondegenerate for any h∈Θ⁢(ξi,ρ). Let

Θ ⁢ ( ρ ) := ⋂ i = 1 , … , ν Θ ⁢ ( ξ i , ρ ) .

It is immediate that Θ⁢(ρ) is a residual subset of ℬρ such that the critical points of 𝒲g^+h in M are nondegenerate for any h∈Θ⁢(ρ). ∎

Proof of Theorem 1.1.

First of all, we prove that 𝒜 is an open set. If g^∈𝒜, the critical points of 𝒲g^ are in a finite number ξ1,…,ξν. Let us consider the chart (Bg^⁢(ξ1),φ1-1) and set

𝒲 ~ g ^ + h ⁢ ( x ) := 𝒲 g ^ + h ⁢ ( φ 1 ⁢ ( x ) ) .

We introduce the C2-map F:ℬρ×B⁢(0,R)→ℝn defined by F⁢(h,x):=∇⁡𝒲~g^+h⁢(x). We have F⁢(0,0)=0. Moreover, Fx′⁢(0,0):ℝn→ℝn is an isomorphism. Then by the implicit function theorem it is easy to deduce that locally there exists a unique x=x⁢(h) such that F⁢(h,x⁢(h))=0. Since the critical points of 𝒲g^ are in a finite number, it is easy to check that choosing ρ small enough for any h∈ℬρ has only ν critical points. They are nondegenerate because F is a C2-function.

The density of 𝒜 follows by Theorem 2.2. ∎

3 The Transversality Condition

3.1 Notation

Let us recall the definition of the Weyl tensor Wg⁢(Ξ):=Weylg⁢(Ξ) of the metric g at the point Ξ in a local chart. We denote by gi⁢j the inverse matrix of gi⁢j and by δi⁢j the Kronecker symbol. Let Ξ0∈M be fixed. Given a coordinate system, the Weyl tensor in a point Ξ⁢(x) belonging to Bg⁢(Ξ0,R) can be expressed as follows:

W i ⁢ j ⁢ k ⁢ l g = R i ⁢ j ⁢ k ⁢ l - 1 n - 2 ⁢ ( R i ⁢ k ⁢ g j ⁢ l - R i ⁢ l ⁢ g j ⁢ k + R j ⁢ l ⁢ g i ⁢ k - R j ⁢ k ⁢ g i ⁢ l ) + R ( n - 1 ) ⁢ ( n - 2 ) ⁢ ( g j ⁢ l ⁢ g i ⁢ k - g j ⁢ k ⁢ g i ⁢ l ) ,

where Ri⁢j⁢k⁢l is the Riemann curvature tensor, Ri⁢j is the Ricci tensor and R is the scalar curvature. We agree that all previous functions are evaluated at the point x. Namely the Riemann curvature tensor reads as

(3.1) R i ⁢ j ⁢ k ⁢ l = R i ⁢ j ⁢ k ⁢ l ⁢ ( g , x ) = R i ⁢ k ⁢ l h ⁢ g h ⁢ j   and   R k ⁢ i ⁢ j l = ∂ i ⁡ Γ j ⁢ k l - ∂ j ⁡ Γ i ⁢ k l + Γ i ⁢ s l ⁢ Γ j ⁢ k s - Γ j ⁢ s l ⁢ Γ i ⁢ k s ,

the Ricci tensor reads as

R i ⁢ j = R i ⁢ j ⁢ ( g , x ) = g k ⁢ l ⁢ R i ⁢ k ⁢ j ⁢ l

and the scalar curvature reads as

(3.2) R = R ⁢ ( g , x ) = g i ⁢ j ⁢ R i ⁢ j .

Here Γi⁢jl are the Christoffel symbols

(3.3) Γ i ⁢ j l = Γ i ⁢ j l ⁢ ( g , x ) = 1 2 ⁢ g l ⁢ m ⁢ G i ⁢ j ⁢ k   where ⁢ G i ⁢ j ⁢ k = G i ⁢ j ⁢ k ⁢ ( g , x ) := ( ∂ j ⁡ g m ⁢ i + ∂ i ⁡ g m ⁢ j - ∂ m ⁡ g i ⁢ j ) .

Given the metric g=g^+h with h∈ℬρ and a point ξ∈Bg⁢(ξ0,R), let us consider the local normal coordinates on the Riemannian manifold (M,g) given by the exponential map expξ⁡(z). Therefore, the metric g in normal coordinates satisfies

g i ⁢ j ⁢ ( 0 ) = g i ⁢ j ⁢ ( 0 ) = δ i ⁢ j   and   ∂ k ⁡ g i ⁢ j ⁢ ( 0 ) = ∂ k ⁡ g i ⁢ j ⁢ ( 0 ) = 0 ,

which implies Γi⁢jk⁢(g,0)=0 for any indexes i, j and k.

In particular, the functions Gi⁢j⁢k defined in (3.3) have the following property:

(3.4) ∂ α ⁢ β 2 ⁡ G i ⁢ j ⁢ k ⁢ ( h , 0 ) = ∂ α ⁢ β ⁢ i 3 ⁡ h k ⁢ j ⁢ ( 0 ) + ∂ α ⁢ β ⁢ j 3 ⁡ h k ⁢ i ⁢ ( 0 ) - ∂ α ⁢ β ⁢ k 3 ⁡ h i ⁢ j ⁢ ( 0 ) .

Moreover, we always choose h∈𝒮k such that the map z↦hi⁢j⁢(expξ⁡(z)), with its first and second derivatives, is vanishing at the point 0 for any indexes i and j, i.e.

(3.5) h i ⁢ j ⁢ ( 0 ) = 0 , ∂ k ⁡ h i ⁢ j ⁢ ( 0 ) = 0 , ∂ k ⁢ l 2 ⁡ h i ⁢ j ⁢ ( 0 ) = 0   for any ⁢ i , j , k , l .

3.2 Calculus

(i) The derivative of the Christoffel symbols.

By (3.3) a straightforward computation gives

∂ α ⁡ Γ i ⁢ j l ⁢ ( g , x ) = 1 2 ⁢ ∂ α ⁡ g l ⁢ k ⁢ G i ⁢ j ⁢ k ⁢ ( g , x ) + 1 2 ⁢ g l ⁢ k ⁢ ∂ α ⁡ G i ⁢ j ⁢ k ⁢ ( g , x ) ,
∂ α ⁢ β 2 ⁡ Γ i ⁢ j l ⁢ ( g , x ) = 1 2 ⁢ ∂ α ⁢ β 2 ⁡ g l ⁢ k ⁢ G i ⁢ j ⁢ k ⁢ ( g , x ) + 1 2 ⁢ g l ⁢ k ⁢ ∂ α ⁢ β 2 ⁡ G i ⁢ j ⁢ k ⁢ ( g , x ) + ∂ α ⁡ g l ⁢ k ⁢ ∂ β ⁡ G i ⁢ j ⁢ k ⁢ ( g , x ) + ∂ β ⁡ g l ⁢ k ⁢ ∂ α ⁡ G i ⁢ j ⁢ k ⁢ ( g , x ) ,
D g ⁢ Γ i ⁢ j l ⁢ ( g , x ) ⁢ [ h ] = 1 2 ⁢ g l ⁢ k ⁢ G i ⁢ j ⁢ k ⁢ ( h , x ) - 1 2 ⁢ g l ⁢ s ⁢ h s ⁢ t ⁢ g t ⁢ k ⁢ G i ⁢ j ⁢ k ⁢ ( g , x ) ,
∂ α ⁡ D g ⁢ Γ i ⁢ j l ⁢ ( g , x ) ⁢ [ h ] = 1 2 ⁢ ∂ α ⁡ g l ⁢ k ⁢ G i ⁢ j ⁢ k ⁢ ( h , x ) + 1 2 ⁢ g l ⁢ k ⁢ ∂ α ⁡ G i ⁢ j ⁢ k ⁢ ( h , x ) - 1 2 ⁢ ∂ α ⁡ ( g l ⁢ s ⁢ h s ⁢ t ⁢ g t ⁢ k ) ⁡ G i ⁢ j ⁢ k ⁢ ( g , x ) - 1 2 ⁢ g l ⁢ s ⁢ h s ⁢ t ⁢ g t ⁢ k ⁢ ∂ α ⁡ G i ⁢ j ⁢ k ⁢ ( g , x ) ,
∂ α ⁢ β 2 ⁡ D g ⁢ Γ i ⁢ j l ⁢ ( g , x ) ⁢ [ h ] = 1 2 ⁢ ∂ α ⁢ β 2 ⁡ g l ⁢ k ⁢ G i ⁢ j ⁢ k ⁢ ( h , x ) + 1 2 ⁢ ∂ α ⁡ g l ⁢ k ⁢ ∂ β ⁡ G i ⁢ j ⁢ k ⁢ ( h , x ) + 1 2 ⁢ ∂ β ⁡ g l ⁢ k ⁢ ∂ α ⁡ G i ⁢ j ⁢ k ⁢ ( h , x ) + 1 2 ⁢ g l ⁢ k ⁢ ∂ α ⁢ β 2 ⁡ G i ⁢ j ⁢ k ⁢ ( h , x )
- 1 2 ⁢ ∂ α ⁢ β 2 ⁡ ( g l ⁢ s ⁢ h s ⁢ t ⁢ g t ⁢ k ) ⁡ G i ⁢ j ⁢ k ⁢ ( g , x ) - 1 2 ⁢ ∂ α ⁡ ( g l ⁢ s ⁢ h s ⁢ t ⁢ g t ⁢ k ) ⁢ ∂ β ⁡ G i ⁢ j ⁢ k ⁢ ( g , x )
- 1 2 ⁢ g l ⁢ s ⁢ h s ⁢ t ⁢ g t ⁢ k ⁢ ∂ α ⁢ β 2 ⁡ G i ⁢ j ⁢ k ⁢ ( g , x ) - 1 2 ⁢ ∂ β ⁡ ( g l ⁢ s ⁢ h s ⁢ t ⁢ g t ⁢ k ) ⁢ ∂ α ⁡ G i ⁢ j ⁢ k ⁢ ( g , x ) .

In particular, if we assume (3.5), we get

(3.6) D h ⁢ Γ i ⁢ j l ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 0 , ∂ α ⁡ D h ⁢ Γ i ⁢ j l ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 0 , ∂ α ⁢ β 2 ⁡ D h ⁢ Γ i ⁢ j l ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 1 2 ⁢ ∂ α ⁢ β 2 ⁡ G i ⁢ j ⁢ l ⁢ ( h , 0 ) .

(ii) The derivative of the Riemann tensor.

By (3.1) a straightforward computation gives

D h ⁢ R j ⁢ k ⁢ l i ⁢ ( g , x ) ⁢ [ h ] = D h ⁢ ∂ k ⁡ Γ l ⁢ j i ⁢ ( g , x ) ⁢ [ h ] - D h ⁢ ∂ l ⁡ Γ k ⁢ j i ⁢ ( g , x ) ⁢ [ h ] + D h ⁢ Γ k ⁢ s i ⁢ ( g , x ) ⁢ [ h ] ⁢ Γ l ⁢ j s + Γ k ⁢ s i ⁢ D h ⁢ Γ l ⁢ j s ⁢ ( g , x ) ⁢ [ h ]
- D h ⁢ Γ l ⁢ s i ⁢ ( g , x ) ⁢ [ h ] ⁢ Γ k ⁢ j s - Γ l ⁢ s i ⁢ D h ⁢ Γ k ⁢ j s ⁢ ( g , x ) ⁢ [ h ]

and

∂ α ⁡ D h ⁢ R j ⁢ k ⁢ l i ⁢ ( g , x ) ⁢ [ h ] = D h ⁢ ∂ α ⁢ k 2 ⁡ Γ l ⁢ j i ⁢ ( g , x ) ⁢ [ h ] - D h ⁢ ∂ α ⁢ l 2 ⁡ Γ k ⁢ j i ⁢ ( g , x ) ⁢ [ h ] + D h ⁢ ∂ α ⁡ Γ k ⁢ s i ⁢ ( g , x ) ⁢ [ h ] ⁢ Γ l ⁢ j s + D h ⁢ Γ k ⁢ s i ⁢ ( g , x ) ⁢ [ h ] ⁢ ∂ α ⁡ Γ l ⁢ j s
+ ∂ α ⁡ Γ k ⁢ s i ⁢ D h ⁢ Γ l ⁢ j s ⁢ ( g , x ) ⁢ [ h ] + Γ k ⁢ s i ⁢ D h ⁢ ∂ α ⁡ Γ l ⁢ j s ⁢ ( g , x ) ⁢ [ h ]
- D h ⁢ ∂ α ⁡ Γ l ⁢ s i ⁢ ( g , x ) ⁢ [ h ] ⁢ Γ k ⁢ j s - D h ⁢ Γ l ⁢ s i ⁢ ( g , x ) ⁢ [ h ] ⁢ ∂ α ⁡ Γ k ⁢ j s
- ∂ α ⁡ Γ l ⁢ s i ⁢ D h ⁢ Γ k ⁢ j s ⁢ ( g , x ) ⁢ [ h ] - Γ l ⁢ s i ⁢ D h ⁢ ∂ α ⁡ Γ k ⁢ j s ⁢ ( g , x ) ⁢ [ h ] .

If we assume (3.5), by (3.6) we get

(3.7) D h ⁢ R j ⁢ k ⁢ l i ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 0   and   ∂ α ⁡ D h ⁢ R j ⁢ k ⁢ l i ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 1 2 ⁢ ∂ α ⁢ k 2 ⁡ G l ⁢ j ⁢ i ⁢ ( h , 0 ) - 1 2 ⁢ ∂ α ⁢ l 2 ⁡ G k ⁢ j ⁢ i ⁢ ( h , 0 ) .

Again, by (3.1) we have Ri⁢j⁢k⁢l=gj⁢s⁢Ri⁢k⁢ls and a straightforward computation leads to

D h ⁢ R i ⁢ j ⁢ k ⁢ l ⁢ ( g , x ) ⁢ [ h ] = h j ⁢ s ⁢ R i ⁢ k ⁢ l s + g j ⁢ s ⁢ D h ⁢ R i ⁢ k ⁢ l s ⁢ ( g , x ) ⁢ [ h ]

and

∂ α ⁡ D h ⁢ R i ⁢ j ⁢ k ⁢ l ⁢ ( g , x ) ⁢ [ h ] = h j ⁢ s ⁢ R i ⁢ k ⁢ l s + h j ⁢ s ⁢ ∂ α ⁡ R i ⁢ k ⁢ l s + ∂ α ⁡ g j ⁢ s ⁢ D h ⁢ R i ⁢ k ⁢ l s ⁢ ( g , x ) ⁢ [ h ] + g j ⁢ s ⁢ D h ⁢ ∂ α ⁡ R i ⁢ k ⁢ l s ⁢ ( g , x ) ⁢ [ h ] .

In particular, if we assume (3.5), by (3.7) we get

(3.8) D h ⁢ R i ⁢ j ⁢ k ⁢ l ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 0   and   ∂ α ⁡ D h ⁢ R i ⁢ j ⁢ k ⁢ l ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 1 2 ⁢ ( ∂ α ⁢ k 2 ⁡ G i ⁢ l ⁢ j ⁢ ( h , 0 ) - ∂ α ⁢ l 2 ⁡ G i ⁢ k ⁢ j ⁢ ( h , 0 ) ) .

(iii) The derivative of the Ricci tensor.

By (3.1) we have Ri⁢j=gk⁢l⁢Ri⁢k⁢j⁢l and a straightforward computation gives

D h ⁢ R i ⁢ j ⁢ ( g , x ) ⁢ [ h ] = h k ⁢ l ⁢ R i ⁢ k ⁢ j ⁢ l + g k ⁢ l ⁢ D h ⁢ R i ⁢ k ⁢ j ⁢ l ⁢ ( g , x ) ⁢ [ h ]

and

∂ α ⁡ D h ⁢ R i ⁢ j ⁢ ( g , x ) ⁢ [ h ] = ∂ α ⁡ h k ⁢ l ⁢ R i ⁢ k ⁢ j ⁢ l + h k ⁢ l ⁢ ∂ α ⁡ R i ⁢ k ⁢ j ⁢ l + ∂ α ⁡ g k ⁢ l ⁢ D h ⁢ R i ⁢ k ⁢ j ⁢ l ⁢ ( g , x ) ⁢ [ h ] + g k ⁢ l ⁢ D h ⁢ ∂ α ⁡ R i ⁢ k ⁢ j ⁢ l ⁢ ( g , x ) ⁢ [ h ] .

In particular, if we assume (3.5), by (3.9) we get

(3.9) D h ⁢ R i ⁢ j ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 0   and   ∂ α ⁡ D h ⁢ R i ⁢ j ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 1 2 ⁢ ( ∂ α ⁢ j 2 ⁡ G i ⁢ l ⁢ l ⁢ ( h , 0 ) - ∂ α ⁢ l 2 ⁡ G i ⁢ j ⁢ l ⁢ ( h , 0 ) ) .

(iv) The derivative of the scalar curvature.

By (3.2) we have R=gi⁢j⁢Ri⁢j. A straightforward computation gives

D h ⁢ R ⁢ ( g , x ) ⁢ [ h ] = h i ⁢ j ⁢ R i ⁢ j + g i ⁢ j ⁢ D h ⁢ R i ⁢ j ⁢ ( g , x ) ⁢ [ h ]

and

∂ α ⁡ D h ⁢ R ⁢ ( g , x ) ⁢ [ h ] = ∂ α ⁡ h i ⁢ j ⁢ R i ⁢ j + h i ⁢ j ⁢ ∂ α ⁡ R i ⁢ j + ∂ α ⁡ g i ⁢ j ⁢ D h ⁢ R i ⁢ j ⁢ ( g , x ) ⁢ [ h ] + g i ⁢ j ⁢ D h ⁢ ∂ α ⁡ R i ⁢ j ⁢ ( g , x ) ⁢ [ h ] .

In particular, if we assume (3.5), by (3.9) we get

(3.10) D h ⁢ R ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 0   and   ∂ α ⁡ D h ⁢ R ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 1 2 ⁢ ( ∂ α ⁢ i 2 ⁡ G i ⁢ l ⁢ l ⁢ ( h , 0 ) - ∂ α ⁢ l 2 ⁡ G i ⁢ i ⁢ l ⁢ ( h , 0 ) ) .

(v) The derivative of the Weyl tensor.

Let us recall that

W i ⁢ j ⁢ k ⁢ l g = R i ⁢ j ⁢ k ⁢ l - 1 n - 2 ⁢ ( R i ⁢ k ⁢ g j ⁢ l - R i ⁢ l ⁢ g j ⁢ k + R j ⁢ l ⁢ g i ⁢ k - R j ⁢ k ⁢ g i ⁢ l ) + R ( n - 1 ) ⁢ ( n - 2 ) ⁢ ( g j ⁢ l ⁢ g i ⁢ k - g j ⁢ k ⁢ g i ⁢ l ) .

A straightforward computation shows that

D h ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ ( g , x ) ⁢ [ h ] = D h ⁢ R i ⁢ j ⁢ k ⁢ l ⁢ ( g , x ) ⁢ [ h ] - 1 n - 2 ⁢ ( R i ⁢ k ⁢ h j ⁢ l - R i ⁢ l ⁢ h j ⁢ k + R j ⁢ l ⁢ h i ⁢ k - R j ⁢ k ⁢ h i ⁢ l )
- 1 n - 2 ⁢ ( D h ⁢ R i ⁢ k ⁢ ( g , x ) ⁢ [ h ] ⁢ g j ⁢ l - D h ⁢ R i ⁢ l ⁢ ( g , x ) ⁢ [ h ] ⁢ g j ⁢ k + D h ⁢ R j ⁢ l ⁢ ( g , x ) ⁢ [ h ] ⁢ g i ⁢ k - D h ⁢ R j ⁢ k ⁢ ( g , x ) ⁢ [ h ] ⁢ g i ⁢ l )
+ R ( n - 1 ) ⁢ ( n - 2 ) ⁢ ( h j ⁢ l ⁢ g i ⁢ k + g j ⁢ l ⁢ h i ⁢ k - h j ⁢ k ⁢ g i ⁢ l - g j ⁢ k ⁢ h i ⁢ l )
+ 1 ( n - 1 ) ⁢ ( n - 2 ) ⁢ D h ⁢ R ⁢ ( g , x ) ⁢ [ h ] ⁢ ( g j ⁢ l ⁢ g i ⁢ k - g j ⁢ k ⁢ g i ⁢ l )

and

∂ α ⁡ D h ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ ( g , x ) ⁢ [ h ]
= ∂ α ⁡ D h ⁢ R i ⁢ j ⁢ k ⁢ l ⁢ ( g , x ) ⁢ [ h ] - 1 n - 2 ⁢ ( ∂ α ⁡ R i ⁢ k ⁢ h j ⁢ l - ∂ α ⁡ R i ⁢ l ⁢ h j ⁢ k + ∂ α ⁡ R j ⁢ l ⁢ h i ⁢ k - ∂ α ⁡ R j ⁢ k ⁢ h i ⁢ l )
    - 1 n - 2 ⁢ ( R i ⁢ k ⁢ ∂ α ⁡ h j ⁢ l - R i ⁢ l ⁢ ∂ α ⁡ h j ⁢ k + R j ⁢ l ⁢ ∂ α ⁡ h i ⁢ k - R j ⁢ k ⁢ ∂ α ⁡ h i ⁢ l )
    - 1 n - 2 ⁢ ( D h ⁢ ∂ α ⁡ R i ⁢ k ⁢ ( g , x ) ⁢ [ h ] ⁢ g j ⁢ l - D h ⁢ ∂ α ⁡ R i ⁢ l ⁢ ( g , x ) ⁢ [ h ] ⁢ g j ⁢ k + D h ⁢ ∂ α ⁡ R j ⁢ l ⁢ ( g , x ) ⁢ [ h ] ⁢ g i ⁢ k - D h ⁢ ∂ α ⁡ R j ⁢ k ⁢ ( g , x ) ⁢ [ h ] ⁢ g i ⁢ l )
    - 1 n - 2 ⁢ ( D h ⁢ R i ⁢ k ⁢ ( g , x ) ⁢ [ h ] ⁢ ∂ α ⁡ g j ⁢ l - D h ⁢ R i ⁢ l ⁢ ( g , x ) ⁢ [ h ] ⁢ ∂ α ⁡ g j ⁢ k + D h ⁢ R j ⁢ l ⁢ ( g , x ) ⁢ [ h ] ⁢ ∂ α ⁡ g i ⁢ k - D h ⁢ R j ⁢ k ⁢ ( g , x ) ⁢ [ h ] ⁢ ∂ α ⁡ g i ⁢ l )
    + R ( n - 1 ) ⁢ ( n - 2 ) ⁢ ∂ α ⁡ ( h j ⁢ l ⁢ g i ⁢ k + g j ⁢ l ⁢ h i ⁢ k - h j ⁢ k ⁢ g i ⁢ l - g j ⁢ k ⁢ h i ⁢ l )
    + 1 ( n - 1 ) ⁢ ( n - 2 ) ⁢ ∂ α ⁡ R ⁢ ( h j ⁢ l ⁢ g i ⁢ k + g j ⁢ l ⁢ h i ⁢ k - h j ⁢ k ⁢ g i ⁢ l - g j ⁢ k ⁢ h i ⁢ l )
    + 1 ( n - 1 ) ⁢ ( n - 2 ) ⁢ D h ⁢ R ⁢ ( g , x ) ⁢ [ h ] ⁢ ∂ α ⁡ ( g j ⁢ l ⁢ g i ⁢ k - g j ⁢ k ⁢ g i ⁢ l )
    + 1 ( n - 1 ) ⁢ ( n - 2 ) ⁢ D h ⁢ ∂ α ⁡ R ⁢ ( g , x ) ⁢ [ h ] ⁢ ( g j ⁢ l ⁢ g i ⁢ k - g j ⁢ k ⁢ g i ⁢ l ) .

In particular, if we assume (3.5), by (3.9) and (3.10) we get

D h ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 0

and

∂ α D h W i ⁢ j ⁢ k ⁢ l g ( g , x ) [ h ] | x = 0 = ∂ α D h R i ⁢ j ⁢ k ⁢ l ( g , x ) [ h ] | x = 0 - 1 n - 2 ( D h ∂ α R i ⁢ k ( g , x ) [ h ] | x = 0 δ j ⁢ l - D h ∂ α R i ⁢ l ( g , x ) [ h ] | x = 0 δ j ⁢ k
+ D h ∂ α R j ⁢ l ( g , x ) [ h ] | x = 0 δ i ⁢ k - D h ∂ α R j ⁢ k ( g , x ) [ h ] | x = 0 δ i ⁢ l )
(3.11) + 1 ( n - 1 ) ⁢ ( n - 2 ) ⁢ D h ⁢ ∂ α ⁡ R ⁢ ( g , x ) ⁢ [ h ] | x = 0 ⁢ ( δ j ⁢ l ⁢ δ i ⁢ k - δ j ⁢ k ⁢ δ i ⁢ l ) .

(vi) The derivative of 𝒲~g.

We shall compute the derivatives of (see also (2.1) and (2.2))

𝒲 ~ ⁢ ( g , x ) := 𝒲 ~ g ⁢ ( x ) = g i ⁢ i ¯ ⁢ g j ⁢ j ¯ ⁢ g k ⁢ k ¯ ⁢ g l ⁢ l ¯ ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ W i ¯ ⁢ j ¯ ⁢ k ¯ ⁢ l ¯ g .

A straightforward computations shows that

D h ⁢ 𝒲 ~ ⁢ ( g , x ) ⁢ [ h ] = g i ⁢ i ¯ ⁢ g j ⁢ j ¯ ⁢ g k ⁢ k ¯ ⁢ g l ⁢ l ¯ ⁢ { 2 ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ D h ⁢ W i ¯ ⁢ j ¯ ⁢ k ¯ ⁢ l ¯ g ⁢ [ h ] }
- { g i ⁢ a ⁢ h a ⁢ b ⁢ g b ⁢ i ¯ ⁢ g j ⁢ j ¯ ⁢ g k ⁢ k ¯ ⁢ g l ⁢ l ¯ + g i ⁢ i ¯ ⁢ g j ⁢ a ⁢ h a ⁢ b ⁢ g b ⁢ j ¯ ⁢ g k ⁢ k ¯ ⁢ g l ⁢ l ¯ + g i ⁢ i ¯ ⁢ g j ⁢ j ¯ ⁢ g k ⁢ a ⁢ h a ⁢ b ⁢ g b ⁢ k ¯ ⁢ g l ⁢ l ¯ + g i ⁢ i ¯ ⁢ g j ⁢ j ¯ ⁢ g k ⁢ k ¯ ⁢ g l ⁢ a ⁢ h a ⁢ b ⁢ g b ⁢ l ¯ } ⏟ := B ⁢ ( g , h , x ) ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ W i ¯ ⁢ j ¯ ⁢ k ¯ ⁢ l ¯ g

and

∂ α ⁡ D h ⁢ 𝒲 ~ ⁢ ( g , x ) ⁢ [ h ] = ∂ α ⁡ { g i ⁢ i ¯ ⁢ g j ⁢ j ¯ ⁢ g k ⁢ k ¯ ⁢ g l ⁢ l ¯ } ⁡ { 2 ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ D h ⁢ W i ¯ ⁢ j ¯ ⁢ k ¯ ⁢ l ¯ g ⁢ [ h ] }
+ { g i ⁢ i ¯ ⁢ g j ⁢ j ¯ ⁢ g k ⁢ k ¯ ⁢ g l ⁢ l ¯ } ⁢ { 2 ⁢ ∂ α ⁡ W i ⁢ j ⁢ k ⁢ l g ⁢ D h ⁢ W i ¯ ⁢ j ¯ ⁢ k ¯ ⁢ l ¯ g ⁢ [ h ] + 2 ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ ∂ α ⁡ D h ⁢ W i ¯ ⁢ j ¯ ⁢ k ¯ ⁢ l ¯ g ⁢ [ h ] }
(3.12) + ∂ α ⁡ B ⁢ ( g , h , x ) ⁢ { W i ⁢ j ⁢ k ⁢ l g ⁢ W i ¯ ⁢ j ¯ ⁢ k ¯ ⁢ l ¯ g } + B ⁢ ( g , h , x ) ⁢ { ∂ α ⁡ W i ⁢ j ⁢ k ⁢ l g ⁢ W i ¯ ⁢ j ¯ ⁢ k ¯ ⁢ l ¯ g + W i ⁢ j ⁢ k ⁢ l g ⁢ ∂ α ⁡ W i ¯ ⁢ j ¯ ⁢ k ¯ ⁢ l ¯ g } .

If we assume (3.5), then by (3.11) and the crucial property of the Weyl tensor

W a ⁢ b ⁢ c ⁢ b ( := ∑ b = 1 n W a ⁢ b ⁢ c ⁢ b ) = 0 ,

formula (3.12) reduces to

∂ α ⁡ D h ⁢ 𝒲 ~ ⁢ ( g , x ) ⁢ [ h ] | x = 0 = 2 ⁢ ∂ α ⁡ W i ⁢ j ⁢ k ⁢ l g ⁢ ( x ) | x = 0 ⁢ D h ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ ( 0 ) ⁢ [ h ] + 2 ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ ( 0 ) ⁢ ∂ α ⁡ D h ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ ( x ) ⁢ [ h ] | x = 0
= 2 ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ ( 0 ) ⁢ ∂ α ⁡ D h ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ ( x ) ⁢ [ h ] | x = 0
= 2 ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ ( 0 ) ⁢ ∂ α ⁡ D h ⁢ R i ⁢ j ⁢ k ⁢ l ⁢ ( g , x ) ⁢ [ h ] | x = 0
- 2 n - 2 ( D h ∂ α R i ⁢ k ( g , x ) [ h ] | x = 0 W i ⁢ j ⁢ k ⁢ j g ( 0 ) - D h ∂ α R i ⁢ l ( g , x ) [ h ] | x = 0 W i ⁢ j ⁢ j ⁢ l g ( 0 )
+ D h ∂ α R j ⁢ l ( g , x ) [ h ] | x = 0 W i ⁢ j ⁢ i ⁢ l g ( 0 ) - D h ∂ α R j ⁢ k ( g , x ) [ h ] | x = 0 W i ⁢ j ⁢ k ⁢ i g ( 0 ) )
+ 2 ( n - 1 ) ⁢ ( n - 2 ) ⁢ D h ⁢ ∂ α ⁡ R ⁢ ( g , x ) ⁢ [ h ] | x = 0 ⁢ ( W l ⁢ k ⁢ l ⁢ k - W l ⁢ k ⁢ k ⁢ l )
= 2 ⁢ W i ⁢ j ⁢ k ⁢ l g ⁢ ( 0 ) ⁢ ∂ α ⁡ D h ⁢ R i ⁢ j ⁢ k ⁢ l ⁢ ( g , x ) ⁢ [ h ] | x = 0   (and by (3.8) and (3.9))
= W i ⁢ j ⁢ k ⁢ l ⁢ ( 0 ) ⁢ ( ∂ α ⁢ k 2 ⁡ G i ⁢ l ⁢ j ⁢ ( h , 0 ) - ∂ α ⁢ l 2 ⁡ G i ⁢ k ⁢ j ⁢ ( h , 0 ) )
(3.13) = 2 ⁢ W i ⁢ j ⁢ k ⁢ l ⁢ ( 0 ) ⁢ ( ∂ α ⁢ k ⁢ i 3 ⁡ h l ⁢ j - ∂ α ⁢ k ⁢ j 3 ⁡ h i ⁢ l ) ,

where we used the expression of Gi⁢j⁢k given in (3.4).

3.3 The Transversality Condition: Proof

Lemma 3.1

The map (h,x)→Fh′⁢(h~,x~)⁢[h]+Fx′⁢(h~,x~)⁢x is onto on Rn for any (h~,x~)∈Sk×Rn with F⁢(h~,x~)=0 provided |Wg^+h~⁢(φ⁢(x~))|g^+h~2≠0.

Proof.

Consider g^+h with h∈ℬρ⊂𝒮k, k≥4. The function F⁢(h,x)=∇x⁡𝒲~g^+h⁢(x) defined in (2.3) is of class C2. Let (h~,x~) be such that F⁢(h~,x~)=0. We get

F h ′ ⁢ ( h ~ , x ~ ) ⁢ [ h ] = ( D h ⁢ ∂ 1 ⁡ 𝒲 ~ g ^ + h ~ ⁢ ( x ~ ) ⁢ [ h ] , … , D h ⁢ ∂ N ⁡ 𝒲 ~ g ^ + h ~ ⁢ ( x ~ ) ⁢ [ h ] )

We shall prove that the map Fh′⁢(h~,x~):𝒮k→ℝn is onto.

We point out that the ontoness of the map h→Fh′⁢(h~,x~)⁢[h] is invariant with respect to a change of variable x=ψ⁢(z), where ψ is a diffeomorphism. Therefore, we compute Dh⁢∂α⁡𝒲~g^+h~⁢(x~)⁢[h] by choosing the normal coordinates on the Riemannian manifold (M,g^+h~) given by the exponential map expξ~⁡(z), where ξ~ corresponds to x~.

We choose h∈𝒮k such that the map z→hi⁢j⁢(expξ~⁡(z)), with its first and second derivatives, is vanishing at the point 0 for any indexes i and j, so that condition (3.5) holds. Therefore, by (3.13) we are lead to prove that the map

T ⁢ ( h ) := ( 2 ⁢ ∑ i , j , k , l = 1 n W i ⁢ j ⁢ k ⁢ l ⁢ ( 0 ) ⁢ ( ∂ α ⁢ k ⁢ i 3 ⁡ h l ⁢ j ⁢ ( x ) - ∂ α ⁢ k ⁢ j 3 ⁡ h i ⁢ l ⁢ ( x ) ) ) α = 1 , … , n

is onto provided that at least one of the components of the Weyl tensor Wi⁢j⁢k⁢l⁢(0) is not zero.

We point out that Wi⁢i⁢i⁢k=Wi⁢i⁢j⁢k=0 for any i, j, k. So we only have to consider 3 different cases.

Case (i):Wi⁢j⁢i⁢j≠0 for some j>i.

Without loss of generality we can assume W1212≠0. Then we take

h 11 ⁢ ( x ) = e ⁢ ( x )   and   h i ⁢ j ⁢ ( x ) = 0 ⁢ otherwise .

Then (3.13) reads as

T ⁢ ( h ) := ( 4 ⁢ ∑ i , k = 1 n W i ⁢ 1 ⁢ k ⁢ 1 ⁢ ( 0 ) ⁢ ∂ α ⁢ k ⁢ i 3 ⁡ e ⁢ ( x ) ) α = 1 , … , n .

We shall prove that T is onto ℝn. We choose e⁢(x)=e1⁢(x)=x1⁢x22. The only third derivative not zero is ∂122⁡e. Then

T ⁢ ( e 1 ) = ( 2 ⁢ W 1212 , 0 , 0 , … , 0 ) .

We choose e⁢(x)=e2⁢(x)=x23. The only third derivative not zero is ∂222⁡e. Then

T ⁢ ( e 2 ) = ( 0 , 2 ⁢ W 1212 , 0 , … , 0 ) .

We choose e⁢(x)=e3⁢(x)=x22⁢x3. The only third derivative not zero is ∂223⁡e. Then

T ⁢ ( e 2 ) = ( 0 , W 1213 + W 1312 , 2 ⁢ W 1212 , … , 0 ) .

In general if we choose e⁢(x)=ei⁢(x)=x22⁢xi with 3≤i≤n, the only third derivative not zero is ∂22⁢i⁡e. Then

T ⁢ ( e i ) = ( 0 , W 121 ⁢ i + W 1 ⁢ i ⁢ 12 , 0 , … , 2 ⁢ W 1212 , … , 0 ) .

The vectors T⁢(e1),…,T⁢(en) are linearly independent, since the matrix

( 2 ⁢ W 2121 0 0 0 … 0 0 2 ⁢ W 2121 2 ⁢ W 2131 2 ⁢ W 2141 … 2 ⁢ W 21 ⁢ n ⁢ 1 0 0 2 ⁢ W 2121 0 … 0 0 0 0 2 ⁢ W 2121 … 0 ⋮ ⋮ ⋮ ⋮ ⋱ ⋮ 0 0 0 0 … W 2121 )

is invertible.

Case (ii):Wi⁢j⁢k⁢j≠0 for some i,k≠j and Wl⁢s⁢l⁢s=0 for any l≠s.

Without loss of generality we can assume W1232≠0. Then we take

h 22 ⁢ ( x ) = e ⁢ ( x )   and   h i ⁢ j ⁢ ( x ) = 0 ⁢ otherwise .

Then (3.13) reads as

T ⁢ ( h ) := ( 4 ⁢ ∑ i , k = 1 n W i ⁢ 2 ⁢ k ⁢ 2 ⁢ ( 0 ) ⁢ ∂ α ⁢ k ⁢ i 3 ⁡ e ⁢ ( x ) ) α = 1 , … , n .

We shall prove that T is onto ℝn. We choose e⁢(x)=e1⁢(x)=x12⁢x3. The only third derivative not zero is ∂113⁡e. Then

T ⁢ ( e 1 ) = ( W 1232 + W 3212 , 0 , 2 ⁢ W 1212 , 0 , … , 0 ) .

We choose e⁢(x)=e2⁢(x)=x1⁢x2⁢x3. The only third derivative not zero is ∂123⁡e. Then

T ⁢ ( e 2 ) = ( W 2232 + W 3222 , W 1232 + W 3212 , W 1222 + W 2221 , 0 , … , 0 ) .

We choose e⁢(x)=e3⁢(x)=x1⁢x32. The only third derivative not zero is ∂133⁡e. Then

T ⁢ ( e 3 ) = ( 2 ⁢ W 3232 , 0 , W 1232 + W 3212 , 0 , … , 0 ) .

In general if we choose e⁢(x)=ei⁢(x)=x1⁢x3⁢xi with 4≤i≤n, the only third derivative not zero is ∂13⁢i⁡e. Then

T ⁢ ( e i ) = ( W 32 ⁢ i ⁢ 2 + W i ⁢ 232 , 0 , W 12 ⁢ i ⁢ 2 + W i ⁢ 212 , 0 , … , W 1232 + W 3212 , 0 , … , 0 ) .

Taking into account that we are assuming that Wi⁢j⁢i⁢j=0, we have that the vectors T⁢(e1),…,T⁢(en) are linearly independent, since the matrix

( 2 ⁢ W 1232 0 0 2 ⁢ W 3242 … 2 ⁢ W 32 ⁢ n ⁢ 2 0 2 ⁢ W 1232 0 0 … 0 0 0 2 ⁢ W 1232 2 ⁢ W 1242 … 2 ⁢ W 12 ⁢ n ⁢ 2 0 0 0 W 1232 … 0 ⋮ ⋮ ⋮ ⋮ ⋱ ⋮ 0 0 0 0 … W 1232 )

is invertible.

Case (iii):Wi⁢j⁢ℓ⁢κ≠0 for some different indexes and Wk⁢k⁢l⁢s=Wk⁢l⁢s⁢l=0 for any k,s,l.

It is important to point out that Wi⁢j⁢ℓ⁢κ+Wi⁢κ⁢ℓ⁢j≠0 for some different indexes. Indeed, if Wi⁢j⁢ℓ⁢κ+Wi⁢κ⁢ℓ⁢j=0 for any choice of different indexes, then also Wi⁢ℓ⁢j⁢κ+Wi⁢κ⁢j⁢ℓ=0. Therefore, by adding the two relations we get Wi⁢j⁢ℓ⁢κ+Wi⁢ℓ⁢j⁢κ=0, and by combining this with the Bianchi identity

W i ⁢ j ⁢ ℓ ⁢ κ + W i ⁢ κ ⁢ j ⁢ ℓ + W i ⁢ ℓ ⁢ κ ⁢ j = 0

we get 2⁢Wi⁢j⁢ℓ⁢κ+Wi⁢κ⁢j⁢ℓ=0. Finally, combining this last equality with the previous one, Wi⁢j⁢ℓ⁢κ+Wi⁢κ⁢ℓ⁢j=0, we get Wi⁢ℓ⁢j⁢κ=0.

Therefore, without loss of generality we can assume W1234+W1432≠0. Then we take

h 24 ⁢ ( x ) = h 42 = e ⁢ ( x )   and   h i ⁢ j ⁢ ( x ) = 0 ⁢ otherwise .

Then (3.13) reads as

T ⁢ ( h ) := ( 8 ⁢ ∑ i , k = 1 n W i ⁢ 2 ⁢ k ⁢ 4 ⁢ ( 0 ) ⁢ ∂ α ⁢ k ⁢ i 3 ⁡ e ⁢ ( x ) ) α = 1 , … , n .

We shall prove that T is onto ℝn. We choose e⁢(x)=e1⁢(x)=x12⁢x3. The only third derivative not zero is ∂113⁡e. Then

T ⁢ ( e 1 ) = ( W 1234 + W 3214 , 0 , 2 ⁢ W 1214 , 0 , … , 0 ) .

We choose e⁢(x)=e2⁢(x)=x1⁢x2⁢x3. The only third derivative not zero is ∂123⁡e. Then

T ⁢ ( e 2 ) = ( W 2234 + W 3224 , W 1234 + W 3214 , W 1224 + W 2214 , 0 , … , 0 ) .

We choose e⁢(x)=e3⁢(x)=x1⁢x32. The only third derivative not zero is ∂133⁡e. Then

T ⁢ ( e 3 ) = ( 2 ⁢ W 3234 , 0 , W 1234 + W 3214 , 0 , … , 0 ) .

In general if we choose e⁢(x)=ei⁢(x)=x1⁢x3⁢xi with 4≤i≤n, the only third derivative not zero is ∂12⁢i⁡e. Then

T ⁢ ( e i ) = ( W 32 ⁢ i ⁢ 4 + W i ⁢ 234 , 0 , W 12 ⁢ i ⁢ 4 + W i ⁢ 214 , 0 , … , W 1234 + W 3412 , … , 0 ) .

Now, we take into account that we are assuming that Wk⁢k⁢s⁢l=Wk⁢l⁢s⁢l=0 for any k, s, l, and so the vectors T⁢(e1),…,T⁢(en) are linearly independent, since the matrix

( W 1234 + W 3412 0 0 0 … W 32 ⁢ n ⁢ 4 + W n ⁢ 234 0 W 1234 + W 3412 0 0 … 0 0 0 W 1234 + W 3412 0 … W 12 ⁢ n ⁢ 4 + W n ⁢ 214 0 0 0 W 1234 + W 3412 … 0 ⋮ ⋮ ⋮ ⋮ ⋱ ⋮ 0 0 0 0 … W 1234 + W 3412 )

is invertible. ∎


Dedicated to the memory of Abbas Bahri



Communicated by Paul Rabinowitz


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Received: 2016-11-15
Accepted: 2016-11-21
Published Online: 2017-01-04
Published in Print: 2017-02-01

Š 2017 by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

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