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J. Math. Pures Appl. 99 (2013) 330–342

www.elsevier.com/locate/matpur

Geometric and differentiable rigidity of submanifolds in spheres

Hongwei Xu, Fei Huang, Entao Zhao

Center of Mathematical Sciences, Zhejiang University, Hangzhou, 310027, China Received 31 March 2012

Available online 12 October 2012

Abstract

In this paper, we investigate rigidity of geometric and differentiable structures of complete submanifolds via an extrinsic geo- metrical quantityτ (x)defined by the second fundamental form. We verify a geometric rigidity theorem for complete submanifolds with parallel mean curvature in a unit sphereSn+p. Inspired by the rigidity theorem, we prove a differentiable sphere theorem for complete submanifolds inSn+p. Moreover, we obtain a differentiable pinching theorem for complete submanifolds in aδ(>14)- pinched Riemannian manifold.

©2012 Elsevier Masson SAS. All rights reserved.

Résumé

Dans cet article, on étudie la rigidité de structures géométriques et différentiable de sous-variétés complètes via une quantité géométrique extrinsèqueτ (x)définie par sa deuxième forme fondamentale. On démonte un théorème de rigidité géométrique pour les sous-variétés complètes à courbure moyenne parallèle dans une sphère unitéSn+p. Inspiré par le théorème de rigidité, on établit un théorème de sphère différentiable pour les sous-variétés complètes dansSn+p. On obtient aussi un théorème de pincement différentiable pour les sous-variétés complètes dans une variété riemannienneδ(>14)-pincée.

©2012 Elsevier Masson SAS. All rights reserved.

MSC:53C20; 53C24; 53C40

Keywords:Complete submanifolds; Geometric and differentiable structures; Rigidity theorem; Ricci flow; Stable currents

1. Introduction

The study of relations between geometric invariants and the structures of the geometry and topology of a manifold is a longstanding subject in global differential geometry (see[2,5,8,24]). In 1930’s, Hopf conjectured that a compact, simply connected Riemannian manifold whose sectional curvatures are close to 1 is homeomorphic to a sphere. This conjecture is known as the curvature pinching problem, which was first taken up by Rauch[23]. In 1960’s, making use of the comparison technique, Berger[1]and Klingenberg[16]proved that a compact, simply connected manifold M whose sectional curvatures all lie in the interval (1/4,1]is homeomorphic to the sphereSn. Since the complex projective spaceCPm(m2)has sectional curvatures in the interval[1/4,1], the pinching constant 1/4 is optimal

* Corresponding author.

E-mail addresses:[email protected](H. Xu),[email protected](F. Huang),[email protected](E. Zhao).

0021-7824/$ – see front matter ©2012 Elsevier Masson SAS. All rights reserved.

http://dx.doi.org/10.1016/j.matpur.2012.09.003

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for even dimensional cases. Later, Micallef and Moore [20]obtained a topological sphere theorem for pointwise 1/4-pinched manifolds via the technique of minimal surfaces. Meanwhile, the geometry of compact Kähler manifolds admitting negatively 1/4-pinched Riemannian metric was investigated by Yau and Zheng[34]. In 2008, Böhm and Wilking [3] proved that a compact Riemannian manifold with 2-positive curvature operator is diffeomorphic to a spherical space form. Recently, Brendle and Schoen[6] proved a remarkable differentiable pinching theorem for pointwise 1/4-pinched Riemannian manifolds by developing Hamilton’s Ricci flow theory[15]. Furthermore, they gave a classification of weakly pointwise 1/4-pinched Riemannian manifolds[7]. More recently, Brendle[4]obtained the celebrated convergence result for the Ricci flow.

Theorem 1.1.Let(M, g0)be a compact Riemannian manifold of dimensionn4. Assume that

R1313+λ2R1414+R2323+λ2R2424−2λR1234>0, (1) for all orthonormal four frames{e1, e2, e3, e4}and allλ∈ [−1,1]. Then the normalized Ricci flow with initial met- ricg0

∂tg(t)= −2Ricg(t)+2

nrg(t)g(t),

exists for all time and converges to a metric with positive constant sectional curvature ast→ +∞. Hererg(t)denotes the mean value of the scalar curvature ofg(t).

The purpose of the present article is to investigate the geometry and topology from the viewpoint of submanifolds.

After the pioneering rigidity theorem for closed minimal submanifolds in a unit sphere due to Simons[26], Lawson [17]and Chern, do Carmo and Kobayashi[12]obtained a classification ofn-dimensional closed minimal submanifolds inSn+p whose squared norm of the second fundamental form satisfiesSn/(2−1/p). Further discussions on the rigidity theorems have been carried out by many other authors (see[21,22,33], etc.). In 1990, Xu[29]proved a rigidity theorem for compact submanifolds with parallel mean curvature in a sphere.

Theorem 1.2.LetMbe ann-dimensional oriented compact submanifold with parallel mean curvature in an(n+p)- dimensional unit sphereSn+p. Denote byHandSthe mean curvature and squared norm of the second fundamental form, respectively. IfSC(n, p, H ),thenMis either a totally umbilic sphereSn(1

1+H2), a Clifford hypersurface in an(n+1)-sphere, or the Veronese surface inS4(1

1+H2). Here the constantC(n, p, H )is defined by

C(n, p, H )=

⎧⎪

⎪⎪

⎪⎪

⎪⎩

α(n, H ), forp=1, orp=2andH=0,

n 2p1

, forp2andH=0,

min{α(n, H ),n+nH2

2p11

+nH2}, forp3andH=0, α(n, H )=n+ n3

2(n−1)H2n(n−2) 2(n−1)

n2H4+4(n−1)H2.

Later, the above pinching constantC(n, p, H )was improved, by Li and Li[19]forH =0 and by Xu[30]for H=0, to

C(n, p, H )=

α(n, H ), forp=1, orp=2 andH=0, min{α(n, H ),13(2n+5nH2)}, otherwise.

The special case of Theorem1.2forp=1 was also studied by Cheng and Nakagawa[11]independently.

On the other hand, Lawson and Simons[18]proved a topological sphere theorem for closed submanifolds in a unit sphere by using the non-existence for stable currents on compact submanifolds in a sphere. Shiohama and Xu[25]

improved Lawson–Simons’ result and proved a topological sphere theorem for complete submanifolds in a simply connected space form with nonnegative constant curvature. Recently, Xu and Zhao[32]and Xu and Gu[31]obtained some differentiable sphere theorems for complete submanifolds.

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LetMnbe ann-dimensional Riemannian submanifold in an (n+p)-dimensional Riemannian manifoldNn+p. Set U M=

xMUxM, whereUxM= {uTxM: u =1}andTxMis the tangent space atxM. In 1986, Gauchman [13]proved that ifMis ann-dimensional closed minimal submanifold inSn+p, and ifσ (u)13 for any unit vector uU M, whereσ (u)= h(u, u) 2andhis the second fundamental form ofM, then eitherσ (u)≡0 orσ (u)13. Xu, Fang and Xiang[28]generalized this rigidity result to the case whereMis ann-dimensional closed submanifold with parallel mean curvature inSn+p. In[32], Xu and Zhao proved the following theorem.

Theorem 1.3. LetM be an n-dimensional complete submanifold in an (n+p)-dimensional unit sphere Sn+p. If σ (u) <13 for alluU M, thenMis diffeomorphic to the standard unitn-sphereSn.

Puttingβ(u, v)= h(u, u)h(v, v) 2foru, vUxM, we define τ (x)= max

u,vUxM, uvβ(u, v).

Note that if h(u, u) 2< cfor anyuUxM, wherecis some positive constant, thenβ(u, v) <4cfor anyu, vUxM. This impliesτ (x) <4c.

In this paper, we first obtain the following geometric rigidity theorem.

Theorem A. Let M be an n-dimensional complete submanifold with parallel mean curvature in an (n+p)- dimensional unit sphereSn+p.

(1) Whenp=1, orp=2andH=0, ifMis compact andτ (x)4for allxM,then eitherτ (x)≡0andMis the totally umbilical sphereSn(1

1+H2), orτ (x)≡4.

(2) Whenp3, orp=2andH=0, ifτ (x)43 for allxM,then eitherτ (x)≡0andMis the totally umbilical sphereSn(1

1+H2), orτ (x)43.

Corollary 1.4.(See[13,28].) LetMbe ann-dimensional complete submanifold with parallel mean curvature in an (n+p)-dimensional unit sphereSn+p.

(1) Whenp=1, orp=2andH=0, ifMis compact andσ (u)1for alluU M,then eitherσ (u)≡0andMis the totally umbilical sphereSn(1

1+H2), ormaxuU Mσ (u)=1.

(2) Whenp3, orp=2andH=0, ifσ (u)13for alluU M,then eitherσ (u)≡0andMis the totally umbilical sphereSn(1

1+H2), orσ (u)13.

Then we prove the following differentiable rigidity theorem, which is a generalization of Theorem1.3.

Theorem B. Let M be an n-dimensional complete submanifold in an (n+p)-dimensional unit sphereSn+p. If τ (x) <43for allxM, thenMis diffeomorphic to the standard unitn-sphereSn.

Remark 1.5.Examples3.5and3.6in Section3show that our pinching constants in Theorems A and B are sharp.

If the ambient space is a general Riemannian manifold, we obtained the following differentiable pinching theorem.

Theorem C. Let M be an n-dimensional complete submanifold in an (n+p)-dimensional pointwise δ(>1/4)- pinched Riemannian manifold Nn+p. Denote by K(x, π )the sectional curvature ofN for 2-plane πTxN and pointxN. SetKmax(x):=maxπTxNK(x, π )forxM. Ifτ (x) <169Kmax(x)(δ14)for allxM,thenMis diffeomorphic to a space form. In particular, ifMis simply connected, thenMis diffeomorphic to the standard unit n-sphereSnor the Euclidean spaceRn.

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Our paper is organized as follows. In Section2, we introduce some basic equations in the geometry of submanifolds and give a lower bound for the sectional curvature of the submanifold in terms of the extrinsic quantityτ (x). We prove two rigidity theorems for submanifolds of spheres in Section3. Then we give the proof of Theorem A. In Section4, Theorems B and C are proved by using convergence results for the Ricci flow of Hamilton[15]and Brendle[4], and the non-existence theorem for stable currents due to Lawson and Simons[18]. Moreover, we present a differentiable pinching theorem for even dimensional submanifolds in pinched Riemannian manifolds.

2. Preliminaries

LetMbe ann-dimensional Riemannian manifold isometrically immersed in an (n+p)-dimensional Riemannian manifoldNn+p. We shall make use of the following convention on the range of indices:

1A, B, C, . . .n+p, 1i, j, k, . . .n, n+1α, β, γ , . . .n+p.

Choose a local orthonormal frame field{eA}onNn+p such thatei’s are tangent toM. Let{ωA}be the dual frame field of{eA}and{ωAB}the connection 1-forms ofNn+p. Restricting these forms toM, we have

ωαi=

j

hαijωj, hαij =hαj i,

h=

α,i,j

hαijωiωjeα, ξ=1

n α,i

hαiieα,

Rij kl=Kij kl+

α

hαikhαj lhαilhαj k

, (2)

Rαβkl=Kαβkl+

i

hαikhβilhαilhβik

, (3)

whereh,ξ,Rij kl,Rαβklare the second fundamental form, the mean curvature vector, the Riemannian curvature tensor and the normal curvature tensor ofM, andKABCD is the Riemannian curvature tensor ofN, respectively. We set

H= ξ , Hα= hαij

n×n.

Denote the first and second covariant derivatives ofhαij byhαij kandhαij kl, respectively. Then we have

k

hαij kωk=dhαij+

k

hαkjωik+

k

hαikωj k+

β

hβijωαβ,

k

hαij klωl=dhαij k+

l

hαlj kωil+

l

hαilkωj l+

l

hαij lωkl+

β

hβij kωαβ.

The Laplacian ofhis defined byhαij=

khαij kk. If the mean curvature vector ofMis parallel in the normal bundle TM, i.e.,Xξ=0 for anyXΓ (T M), following[28,30,33], etc. we have

i

hαiik=0,

i

hαiikl=0, for allk, l, α, (4)

hαij=

k,m

hαkmRmij k+

k,m

hαmiRmkj k+

k,β

hβkiRβαj k, (5)

α

Rαβkl

trHα

=0. (6)

LetU M denote the unit tangent bundle onM andUxM its fiber overxM. ThenU M=

xMUxM, where UxM= {uTxM: u =1},TxMis the tangent space ofMatx. Set

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β(u, v)=h(u, u)−h(v, v)2, foru, vUxM. We define a new extrinsic geometrical invariant ofMby

τ (x)= max

u,vUxM,uvβ(u, v), xM.

Proposition 2.1.LetMbe ann-dimensional submanifold in a Riemannian manifoldNn+p, andxa fixed point inM.

Thenτ (x)=0if and only ifxis a totally umbilical point.

Proof. A pointxMis totally umbilical if and only if for eachα=n+1, . . . , n+p, the eigenvalues of the matrix Hα are equal. Suppose{e1, . . . , en}is an orthonormal basis ofTxMsuch thath(ei, ej), eα =κiαδij. Thenκiα,i= 1, . . . , n, aren eigenvalues ofHα. Ifτ (x)=0, then h(ei, ei)=h(ej, ej). This implies thatκiα = h(ei, ei), eα = h(ej, ej), eα =κjα fori=j. That is to say,Hα has only one eigenvalue with multiplicationn. Note that this holds for arbitraryα=n+1, . . . , n+p. HenceMis totally umbilical atx. The inverse is obvious since thatMis totally umbilical atx is equivalent toh(X, Y )= X, Yξ for anyX, YTxM. 2

The following lemma gives a lower bound for the sectional curvature of a submanifold.

Lemma 2.2. Let M be an n-dimensional submanifold in a Riemannian manifold Nn+p. Denote by K(x, π ) the sectional curvature ofN for 2-plane πTxN and point xN. SetKmin(x):=minπTxNK(x, π ) for xM.

Then the sectional curvature ofMatxMis no less thanKmin(x)τ (x)2 .

Proof. ForxM, letu, vbe two perpendicular unit vectors inUxM. Then by Gauss equation (2) we have R(u, v, u, v)=K(u, v, u, v)+

h(u, u), h(v, v)

−h(u, v)2. (7) Note that

τ (x)h(u, u)h(v, v)2=h(u, u)2+h(v, v)2−2

h(u, u), h(v, v) . Therefore,

h(u, u), h(v, v)

1

4h(u, u)2+h(v, v)2τ (x) +1

2

h(u, u), h(v, v)τ (x)

4 . (8)

On the other hand, we have

h(u, v)=1 2

h u+v

√2 ,u+v

√2

h uv

√2 ,uv

√2

.

Since(u+v)/

2 and(uv)/

2 are two perpendicular unit vectors, we have h(u, v)2=1

4 h

u+v

√2 ,u+v

√2

h uv

√2 ,uv

√2

2τ (x)

4 . (9)

Combining (7), (8) and (9), we complete the proof of the lemma. 2 3. Rigidity of submanifolds with parallel mean curvature

In this section, we investigate the geometric rigidity of submanifolds with parallel mean curvature. Let Mn be ann-dimensional complete submanifold with parallel mean curvature in an(n+p)-dimensional unit sphereSn+p. ThenKABCD=δACδBDδADδBC.

Supposeτ (x0)=0 atx0M. Then there exist two perpendicular unit vectorsu0, v0Ux0Msuch that

u,vUmaxx0M,uv

h(u, u)−h(v, v)2=h(u0, u0)h(v0, v0)2.

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Choose an orthonormal frame{eA}atx0such that

en+1= h(u0, u0)h(v0, v0)

h(u0, u0)h(v0, v0) , (10)

and the matrix(hnij+1)satisfies

hn11+1· · ·hnnn+1, hnij+1=0 (i=j ). (11) Letu0=

ixiei, v0=

iyiei. Since τ (x0)=

h(u0, u0)h(v0, v0), en+1

2

=

i

xi2y2i hnii+1

2

i

xi2hn11+1

i

y2ihnnn+1 2

=

hn11+1hnnn+12

,

by the definition ofτ, we haveτ (x0)=(hn11+1hnnn+1)2. Thus we can take

e1=u0, en=v0. (12)

From (10), we know thath(e1, e1)h(en, en)is parallel toen+1. Hence

hα11=hαnn, α=n+1. (13)

On the other hand, for anyxM,ei, ejTxM, i=j, let u=ei+ej

√2 , v=eiej

√2 . Sinceu, vare perpendicular, we have

α

hαij2

(x)=1

4h(u, u)−h(v, v)2 (14)

1

4τ (x). (15)

Define a tensor fieldA=(Aij kl)onMby

Aij kl=

α

hαijhαkl.

Under the frame satisfying (10)–(13), we have

τ (x0)=A1111+Annnn−2A11nn. (16) By the definition of Laplacian, we obtainτ (x0)=(1, n)=(A)1111+(A)nnnn−2(A)11nn, and

1

2(A)1111=

α,i

hα11hα11ii+ hα11i2

,

1

2(A)nnnn=

α,i

hαnnhαnnii+ hαnni2

,

(A)11nn=

α,i

hα11hαnnii+hαnnhα11ii+2hα11ihαnni .

Using (13), atx0we have

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1

2(1, n)=

i

hn11+1hnnn+1

hn11ii+1hnnnii+1 +

α,i

hα11ihαnni2

i

hn11+1hnnn+1

hn11ii+1hnnnii+1

. (17)

Substituting (2), (3) and (5) into (17), we have 1

2(1, n)n

hn11+1hnnn+12

−2

hn11+1hnnn+1

i,α

hn11+1hnii+1 hα1i2

+

hnii+1hnnn+1 hαni2 +

hn11+1hnnn+1

i,α

hn11+1hnii+1

hα11hαii+

hnii+1hnnn+1 hαnnhαii

. (18)

Lemma 3.1.LetM be ann-dimensional submanifold with parallel mean curvature in a unit sphereSn+p. Suppose τ (x)=0atxM. Let{eA}be an adapted frame satisfying(10)–(13).

(1) Ifp=1, orp=2andH=0, then 1

2(1, n)n

hn11+1hnnn+12 1−1

4

hn11+1hnnn+12

; (2) Ifp3, orp=2andH=0, then

1

2(1, n)n

hn11+1hnnn+12 1−3

4

hn11+1hnnn+12 .

Proof. (1) Ifp=1, by (10) we see that the second term of the right hand side of (18) vanishes. Ifp=2 andH=0, by (6) we have

α

Rαβkl trHα

=0.

Letα,β ben+1 andn+2, respectively. Then we have R(n+1)(n+2)kl

trHn+1

=0, R(n+2)(n+1)kl

trHn+2

=0.

SinceH=0, trHn+1and trHn+2do not equal to 0 at the same time. Hence R(n+1)(n+2)kl=0

for allk, l=1, . . . , n.By (3) and (11) we have R(n+1)(n+2)kl=

n

i=1

hnik+1hnil+2hnil+1hnik+2

=hnkk+1hnkl+2hnll+1hnlk+2

=hnkl+2

hnkk+1hnll+1

=0.

Particularly,

hn1i+2

hn11+1hnii+1

=0, hnni+2

hnnn+1hnii+1

=0.

So the second term of the right hand side of (18) vanishes either. Hence we have the following estimate from (18):

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1

2(1, n)n

hn11+1hnnn+12

+

hn11+1hnnn+1

i

hn11+1hnii+1

α

hα11hαii+

hnii+1hnnn+1

α

hαnnhαii

n

hn11+1hnnn+12

+

hn11+1hnii+1

×

i

−1 4

hn11+1hnii+1

hn11+1hnnn+12

−1 4

hnii+1hnnn+1

hn11+1hnnn+12

=n

hn11+1hnnn+12 1−1

4

hn11+1hnnn+12

. (19)

In the second inequality we have used the following estimate:

α

hα11hαii

α

1 4

hα11hαii2

=1

4h(e1, e1)h(ei, ei)2

1

4h(e1, e1)h(en, en)2

=1 4

hn11+1hnnn+12

. (20)

(2) Ifp3, orp=2 andH=0, (18) can be rewritten as 1

2(1, n)=n

hn11+1hnnn+12

hn11+1

hnnn+1 n

i=2

hn11+1hnii+1 2

α

hα1i2

α

hα11hαii

+

n1

i=1

hnii+1hnnn+1 2

α

hαni2

α

hαnnhαii

. (21)

Fori=1, by (15) we have

2

α

hα1i2

1

2

hn11+1hnnn+12

.

From this and (20) we obtain

n

i=2

hn11+1hnii+1 2

α

hα1i2

α

hα11hαii

n

i=2

hn11+1hnii+1

×3 4

hn11+1hnnn+12

. (22)

Similarly,

n1

i=1

hnii+1hnnn+1 2

α

hαni2

α

hαnnhαii

n1

i=1

hnii+1hnnn+1

×3 4

hn11+1hnnn+12

. (23)

Substituting (22) and (23) into (21), we get

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1

2(1, n)n

hn11+1hnnn+12

hn11+1hnnn+1

×3 4

hn11+1hnnn+12

n

i=2

hn11+1hnii+1 +

n1

i=1

hnii+1hnnn+1

=n

hn11+1hnnn+12

−3 4

hn11+1hnnn+13

× n

i=1

hn11+1hnii+1 +

n

i=1

hnii+1hnnn+1

=n

hn11+1hnnn+12

−3 4n

hn11+1hnnn+14

=n

hn11+1hnnn+12 1−3

4

hn11+1hnnn+12 . This completes the proof of the lemma. 2

Lemma 3.2.LetMbe ann-dimensional compact submanifold with parallel mean curvature in a unit sphereSn+p. We have

(1) Ifp=1, orp=2andH=0, andτ (x)4for anyxM, thenτ (x)is a constant function onM.

(2) Ifp3, orp=2andH=0, andτ (x)43for anyxM, thenτ (x)is a constant function onM.

Proof. It suffices to show thatτ (x)is a subharmonic function. Fix a pointxM. For the Laplacian of continuous functions, we have the generalized definition

(τ )(x)=Clim

r0

1 r2

B(x,r)

τ

B(x,r)

1−τ (x)

,

whereCis a positive constant andB(x, r)is a geodesic ball centered atxwith radiusr.

Ifτ (x)=0, thenτ (x)0 sinceτ is nonnegative onM.

If τ (x)=0, in a small neighborhood Ox of x within the cut-locus ofx, we denote by u(y), v(y)two vectors tangent toMobtained by parallel transport ofu(x)=e1, v(x)=enalong the unique geodesic joiningxtoy. Define fx(y)= h(u(y), u(y))h(v(y), v(y)) 2. Then

fx(y)|y=x=

A(u, u, u, u)+A(v, v, v, v)−2A(u, u, v, v)

y=x=(1, n).

Sinceτ (x)=fx(x)andτ (y)fx(y), we haveτ (x)fx(x). From Lemma3.1we know that(1, n)0. Hence τ (x)0.

Sincex is arbitrary, we see thatτ (x)is subharmonic, which implies thatτ is a constant function. This completes the proof of Lemma3.2. 2

Theorem 3.3.LetMbe ann-dimensional compact submanifold with parallel mean curvature in a unit sphereSn+p. If p=1, orp=2and H=0, and ifτ (x)4for allxM,then either τ (x)≡0 andM is the totally umbilical sphereSn(1

1+H2), orτ (x)≡4.

Proof. By Lemma3.2,τis a constant function. Whenτ =0, from Lemma2.1we know thatMis the totally umbilical sphereSn(1

1+H2). Whenτ =0, from the definition offx(y)in the proof of Lemma3.2we see thatfx(x)is the maximal value offx. Hence,(1, n)=fx(x)0. By Lemma3.1we have

1

2(1, n)n

hn11+1hnnn+12 1−1

4

hn11+1hnnn+12 .

Since τ (x)=(hn11+1hnnn+1)24, we obtain from the above inequality thatτ (x)=4. This completes the proof of Theorem3.3. 2

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Theorem 3.4.LetMbe ann-dimensional complete submanifold with parallel mean curvature in a unit sphereSn+p. Ifp3, orp=2 andH=0, and ifτ (x)43 for allxM, then eitherτ (x)≡0 andMis the totally umbilical sphereSn(1

1+H2), orτ (x)43.

Proof. From Lemma2.2, we haveKM13>0. HenceMis a compact submanifold by Myers’ theorem. Whenτ=0, Mis the totally umbilical sphereSn(1

1+H2). Whenτ is a nonzero constant, we have(1, n)0. From Lemma3.1 we have 12(1, n)n(hn11+1hnnn+1)2(134(hn11+1hnnn+1)2). Hence ifτ (x)=(hn11+1hnnn+1)243, we obtain that τ=43. This completes the proof of Theorem3.4. 2

Now we are in a position to give the proof of Theorem A.

Proof of Theorem A. Combing Theorems3.3and3.4, we obtain the assertion of Theorem A. 2

Example 3.5. Let Sq(r) be the q-dimensional sphere of radius r in Rq+1, and let 1k n−1. We embed Sk(1/

2)×Snk(1/

2)inSn+1(1)as follows. Letu∈Sk(1/

2)andv∈Snk(1/

2)be vectors of length 1/√ 2 inRk+1andRnk+1, respectively. We can consider(u, v)as a unit vector inRn+2=Rk+1×Rnk+1. It is easy to see thatSk(1/

2)×Snk(1/

2)is a submanifold inSn+1(1)with constant mean curvature H=

2k−n n

. In particular,Sk(1/

2)×Sk(1/

2)⊂Sn+1(1)is minimal ifn=2k. SinceSn+1(1)⊂Sn+2(1)is totally geodesic, as a submanifold inSn+2(1),Sk(1/

2)×Snk(1/

2)⊂Sn+2(1)is a submanifold with parallel mean curvature vector of normH= |2knn|.

Example 3.6.Denote byRP2,CP2,QP2andCayP2the projective planes over the real numbers, complex numbers, quaternions and octonions, and byψ1:RP2→S4(1),ψ2:CP2→S7(1),ψ3:QP2→S13(1)andψ4:CayP2→ S25(1)the corresponding isometric embeddings. Letψ1 :S2(

3)→S4(1)be the isometric immersion defined by ψ1=ψ1π, whereπ:S2(

3)→RP2is the canonical projection.

Forn2,m0, letSn(1)be the great sphere inSn+m(1)given by Sn(1)=

(x1, . . . , xn+m+1)∈Sn+m(1): xn+2= · · · =xn+m+1=0 , andηn,m:Sn(1)→Sn+m(1)the inclusion. We set

φ1,p=η4,p2ψ1:RP2→S2+p(1), p2, φ2,p=η7,p3ψ2:CP2→S4+p(1), p3, φ3,p=η13,p5ψ3:QP2→S8+p(1), p5, φ4,p=η25,p2ψ4:CayP2→S16+p(1), p9, φ1,p =η4,p2ψ1:S2(

3)→S2+p(1), p2.

Thenφi,p is a minimal isometric embedding andφ1,pis a minimal isometric immersion.

From the proof of Main Theorem 1.6 in[28]we see that, for submanifolds described in Example3.5, there exist u, vUxMat everyxMwhich are perpendicular such thatτ (u, v)=4. Henceτ =4 onM. This implies that the conditionτ 4 of Theorem A(1)is optimal. Similarly, we haveτ43 onφi,p,i=1,2,3,4, andφ1,p described in Example3.6. So the conditionτ (x)43 in Theorem A (2) and Theorem B is optimal in the sense that there exist submanifolds which satisfyτ43 but not isometric or diffeomorphic to a sphere.

Theorem A also improves the rigidity result due to Chen[10].

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