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scalar curvature in a de Sitter space

Shu Shichang and Liu Sanyang

Abstract

In this paper, we investigaten-dimensional complete space-like submanifolds Mn with constant normalized scalar curvatureR in a de Sitter spaceSpn+p(c).

Suppose that the normalized mean curvature vector field is parallel. We prove that if the norm square khk2 of the second fundamental form of Mn satisfies nR¯≤ khk2 min{α(n,R), β(n,¯ R)}, then¯ Mn is a totally umbilical submani- fold; orn= 3 andM3is a hyperbolic cylinderH1(c−λ2)×S2(c−µ2) inS14(c), where ¯R=c−R≥0, α(n,R) and¯ β(n,R) are constants only depend on¯ nand R.¯

Mathematics Subject Classification: 53C42,53A10.

Key words:space-like submanifolds, de Sitter space, totally umbilical manifolds, hyperbolic cylinder.

1. Introduction

A de Sitter spaceSn+pp (c) is an (n+p)-dimensional connected complete pseudo- Riemannian manifold of index pwith constant curvaturec >0. Goddard [7] conjec- tured that a complete space-like hypersurface in Sn+11 (c) with constant mean cur- vature H must be totally umbilical. Akutagawa [2] and Ramanathan [11] proved independently that the conjecture is true ifH2≤cwhenn= 2 andn2H2<4(n−1)c whenn≥3. Cheng [4] generalized this result to complete space-like submanifolds in Spn+p(c) with parallel mean curvature vector. For the study of space-like hypersur- faces with constant scalar curvature in a de Sitter space, Zheng ([15], [16]) proved that the compact space-like hypersurfaceMn in a de Sitter space S1n+1(c) with constant scalar curvature is totally umbilical if k(M)>0 and R < c, wherek(M) and R are the sectional curvature and the normalized scalar curvature ofMn. Later, Cheng and Ishikawa [5] showed that if the conditionK(M)>0 is deleted, then Zheng’s result in [15], [16] is also true. Recently, Liu [8] proved the following theorem

Theorem 1. Let Mn be an n-dimensional (n3) complete space-like hypersurface with constant normalized scalar curvatureRin an(n+ 1)-dimensional de Sitter space S1n+1 and denote R¯ = 1−R. If the norm square khk2 of the second fundamental

Balkan Journal of Geometry and Its Applications, Vol.9, No.2, 2004, pp. 82-91.

c

°Balkan Society of Geometers, Geometry Balkan Press 2004.

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form of Mn satisfies nR¯ supkhk2 ≤D(n,R), then either (i)¯ supkhk2 =nR¯ and Mn is totally umbilical; or (ii) supkhk2=D(n,R)¯ andMn is a hyperbolic cylinder H1(1−coth2r)×Sn−1(1−tanh2r), where

D(n,R) =¯ n

(n2)(nR¯2)[n(n1) ¯R24(n1) ¯R+n].

On the other hand, it is natural and very important to study n-dimensional sub- manifolds with constant scalar curvature and higher codimension in a de Sitter space Spn+p(c). But there are few results about it. In this paper, we shall prove the following Theorem 2. Let Mn be ann-dimensional (n3) complete space-like submanifold with constant normalized scalar curvatureRin an(n+p)-dimensional de Sitter space Spn+p(c). Suppose that the normalized mean curvature vector field is parallel andR¯= c−R 0. If the norm square khk2 of the second fundamental form ofMn satisfies nR¯ ≤ khk2min{α(n,R), β(n,¯ R)},¯ then Mn is a totally umbilical submanifold; or n= 3 andM3 is a hyperbolic cylinderH1(c−λ2)×S2(c−µ2)inS14(c), where α(n,R) =¯ n

n−2

(n1)(n2)2R¯2+ [nc(n1) ¯R]2

(n2)2R¯+ 2[nc(n1) ¯R] , β(n,R) =¯ n

n−2[nc−(n−1) ¯R].

λandµare the two distinct principal curvatures of M3 such that one has the multi- plicity 1 and the other the multiplicity 2.

2 Preliminaries

Let Spn+p(c) be an (n+p)-dimensional de Sitter space with indexp. Let Mn be ann-dimensional connected space-like submanifold immersed inSpn+p(c). We choose a local field of semi-Riemannian orthonormal frames e1,· · ·, en+p in Spn+p(c) such that at each point of Mn, e1,· · ·, en span the tangent space of Mn and form an orthonormal frame there. We use the following convention on the range of indices:

1≤A, B, C,· · · ≤n+p; 1≤i, j, k,· · · ≤n;n+1≤α, β, γ,· · · ≤n+p. Letω1,· · ·, ωn+p

be its dual frame field so that the semi-Riemannian metric of Spn+p(c) is given by d¯s2 = P

i

ωi2P

α ω2α = P

A

εAω2A, where εi = 1 and εα = −1. Then the structure equations ofSpn+p(c) are given by

A=X

B

εBωAB∧ωB, ωAB+ωBA= 0, (1)

AB=X

C

εCωAC∧ωCB1 2

X

C,D

KABCDωC∧ωD, (2)

KABCD=AεBACδBD−δADδBC).

(3)

Restrict these form toMn. Then we have

ωα= 0, n+ 1≤α≤n+p.

(4)

From Cartan’s Lemma we have

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ωαi=X

j

hαijωj, hαij =hαji. (5)

The connection forms ofMn are characterized by the structure equations i =

Xn

j=1

ωij∧ωj, ωij+ωji= 0, (6)

ij =X

k

ωik∧ωkj1 2

X

k,l

Rijklωk∧ωl, (7)

Rijkl=c(δikδjl−δilδjk)X

α

(hαikhαjl−hαilhαjk), (8)

whereRijkl are the components of the curvature tensor ofMn. Denote byhthe second fundamental form ofMn. Then

h=X

i,j,α

hαijωi⊗ωj⊗eα. (9)

Denote by ξ, H and khk2 the mean curvature vector field, the mean curvature and the norm square of the second fundamental form ofMn. Then they are defined by

ξ= 1 n

X

α

(X

i

hαii)eα, H =kξk= 1 n

sX

α

(X

i

hαii)2, khk2=X

i,j,α

(hαij)2. (10)

Moreover, the normal curvature tensor{Rαβkl}, the Ricci curvature tensor{Rik}and the scalar curvaturen(n−1)R are expressed as

Rαβkl=X

m

(hαkmhβml−hαlmhβmk), (11)

Rik= (n1)cδik−nX

α

(X

l

hαll)hαik+X

α,j

hαijhαjk, (12)

n(n−1)(R−c) =khk2−n2H2, (13)

whereR is the normalized scalar curvature.

Define the first and the second covariant derivatives of {hαij}, say{hαijk} and{hαijkl}

by X

k

hαijkωk =dhαij+X

k

hαkjωkj+X

k

hαikωkj+X

β

hβijωβα, (14)

X

l

hαijklωl=dhαijk+X

m

hαmjkωmi+X

m

hαimkωmj+X

m

hαijmωmk+X

β

hβijkωβα.

We obtain the Codazzi equation by straightforward computations hαijk =hαikj.

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It follows that the Ricci identities hold

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hαijkl−hαijlk=X

m

hαmjRmjkl+X

m

hαimRmjkl+X

β

hβijRβαkl. (16)

The Laplacian of hαij is defined by ∆hαij = P

k

hαijkk. From (16) we obtain for any α, n+ 1≤α≤n+p,

∆hαij=X

k

hαkkij+X

k,m

hαkmRmijk+X

k,m

hαimRmkjk+X

k,β

hβikRβαjk. (17)

In the case of the mean curvature vectorξ6= 0, we know thaten+1=ξ/His a normal vector field defined globally onMn. We definekµk2and kτk2by

kµk2=X

i,j

(hn+1ij −Hδij)2, kτk2= X

α>n+1

X

i,j

(hαij)2, (18)

respectively. Thenkµk2andkτk2are functions defined onMn globally, which do not depend on the choice of the orthonormal frame{e1,· · ·, en}. And we have

khk2=nH2+kµk2+kτk2. (19)

From the definition of the mean curvature vector ξ, we know nH = P

i

hn+1ii and P

i

hαii= 0 forn+ 2≤α≤n+ponMn. From (13),(18) and (19), we have

∆(n2H2) = ∆khk2= ∆(trHn+12 ) + ∆kτk2. (20)

Hence, from (8),(11) and (17) and by a direct calculation we conclude

1

2∆(trHn+12 ) = P

i,j,k

(hn+1ijk )2+P

i,j

hn+1ij ∆hn+1ij

= P

i,j,k

(hn+1ijk )2+P

i,j

hn+1ij (nH)ij+nctrHn+12 −n2H2c

−nHtr(Hn+13 ) + [tr(Hn+12 )]2+ P

β>n+1

[tr(Hn+1Hβ)]2, (21)

1

2∆kτk2 = P

i,j,k,α>n+1

(hαijk)2+ P

i,j,α>n+1

hαij∆hαij

= P

i,j,k,α>n+1

(hαijk)2+nckτk2−nH P

α>n+1

tr(Hα2Hn+1)

+ P

α>n+1[tr(Hn+1Hα)]2+ P

α,β>n+1

[tr(HαHβ)]2, (22)

whereHαdenote the matrix (hαij) for allα.

We need the following Lemmas.

Lemma 1( [3]). Let i}ni=1 be a set of real numbers satisfying P

i

µi = 0 and P

i

µ2i =β2, whereβ≥0. Then

|X

i

µ3i| ≤ n−2 pn(n−1)β3, (23)

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and the equalities hold if and only if at least n−1 of the µi’s are equal with each other.

Lemma 2 ([10], [13])). LetMn be a complete Riemannian manifold whose Ricci curvature is bounded from below. IfF is a C2-function bounded from above on Mn, then for any ε >0, there is a pointx∈Mn such that

supF−ε < F(x),k∇Fk(x)< ε,∆F(x)< ε.

(24)

Lemma 3( [12]). Let A, B be symmetric n×n matrices satisfyingAB =BA and trA=trB= 0. Then

|trA2B| ≤ n−2

pn(n−1)(trA2)(trB2)1/2. (25)

3 Proof of Theorem 2

For a C2-functionf defined on Mn, we defined its gradient and Hessian (fij) by the following formulas

df =X

i

fiωi, X

j

fijωj=dfi+X

j

fjωji. (26)

LetT =P

i,j

Tijωi⊗ωj be a symmetric tensor onMn defined by Tij=nHδij−hn+1ij .

(27)

Following Cheng-Yau [6], we introduce an operator2associated toT acting onf by 2f =X

i,j

Tijfij =X

i,j

(nHδij−hn+1ij )fij. (28)

By a simple calculation and from (20), we obtain 2(nH) = P

i,j

(nHδij−hn+1ij )(nH)ij

= 12∆(n2H2)− kgrad(nH)k2P

i,j

hn+1ij (nH)ij

= 12∆(trHn+12 ) +12∆kτk2− kgrad(nH)k2P

i,j

hn+1ij (nH)ij. (29)

We choose a local orthonormal frame field{e1,· · ·, en}such thathn+1ij =λiδij. Since P

i

i−H) = 0, then X

i

i−H)2=X

i

λ2i −nH2= trHn+12 −nH2=kµk2. Then by Lemma 1

−nHtr(Hn+13 ) = −nHP

i

λ3i

= −3nH2kµk2−n2H4−nHP

i

i−H)3

≥ −3nH2kµk2−n2H4−√n(n−2)

n(n−1)Hkµk3. (30)

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From (21),(30) andtrHn+12 =kµk2+nH2,we have

1

2∆(trHn+12 ) P

i,j,k

(hn+1ijk )2+P

i,j

hn+1ij (nH)ij

+kµk2{kµk2−√n(n−2)

n(n−1)Hkµk+nc−nH2}

P

i,j,k

(hn+1ijk )2+P

i,j

hn+1ij (nH)ij

+kµk2{nc−nH2−√n(n−2)

n(n−1)Hkµk}.

(31)

LetMn be a compele connected submanifold inSpn+p(c) with nowhere zero mean curvatureH. Suppose that the normalized mean curvature vector ξ/H is parallel in TMnand chooseen+1=ξ/H. Thenωαn+1= 0 for allα. ConsequentlyRαn+1jk= 0.

From (11) we have X

i

hαijhn+1ik =X

i

hαikhn+1ij , (32)

i.e.,

HαHn+1 =Hn+1Hα. (33)

If we setB =Hn+1−HI, then trB = 0. By means of (33) we getHαB =BHα for α > n+ 1.By virtue of Lemma 3

|tr(Hα2B)| ≤ n−2

pn(n−1)trHα2

trB2,(α > n+ 1).

(34) Since

tr(Hα2B) = tr(Hα2Hn+1)−HtrHα2,(α > n+ 1), (35)

trB2= trHn+12 −nH2=kµk2, by (34),(35) we conclude

tr(Hα2Hn+1)(H+ n−2

pn(n−1)kµk)trHα2,(α > n+ 1).

(36)

From (22),(36) we get 1

2∆kτk2 X

i,j,k,α>n+1

(hαijk)2+kτk2{nc−nH2 n(n−2)

pn(n−1)Hkµk}.

(37)

We need the following Lemma 4.

Lemma 4. Let Mn be an n-dimensional space-like submanifold in an (n+p)- dimensional de Sitter spaceSpn+p(c). Suppose that the normalized scalar curvatureR is constant and R≤c. Then

X

i,j,k,α

(hαijk)2≥ kgrad(nH)k2.

Proof. According to (13) andR≤c,khk2≤n2H2 and

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nH∇k(nH) =X

i,j,α

hαijhαijk.

Therefore we get

n2H2kgrad(nH)k2=X

k

(X

i,j,α

hαijhαijk)2≤ khk2 X

i,j,k,α

(hαijk)2. Thus the Lemma 4 is true.

Since we have

kµk2≤ khk2−nH2, (38)

from (29),(31),(37),(38) and Lemma 4 we have

2(nH) (kµk2+kτk2){nc−nH2−√n(n−2)

n(n−1)Hkµk}

(khk2−nH2){nc−nH2−√n(n−2)

n(n−1)Hp

khk2−nH2}.

(39)

Denote ¯R=c−R. By (13) we have

khk2−nH2= n−1

n (khk2−nR).¯ (40)

By (39),(40) we have

2(nH) n−1n (khk2−nR){nc¯ (n1) ¯R−1nkhk2

n−2n p

(khk2+n(n−1) ¯R)(khk2−nR)}.¯ (41)

Sincen≥3, then n1 n−2n . Hence we have 2(nH) n−1

n (khk2−nR)P( ¯¯ R,khk2), (42)

where

P( ¯R,khk2) =nc−(n1) ¯R−n−2n khk2

n−2n p

(khk2+n(n−1) ¯R)(khk2−nR).¯ (43)

(1). If nR¯≤ khk2<min{α(n,R), β(n,¯ R)},then¯

nR¯ supkhk2<min{α(n,R), β(n,¯ R)}.¯ (44)

It is directly checked that supkhk2< α(n,R) is equivalent to¯ [nc(n1) ¯R−n−2n supkhk2]2

>(n−2)n2 2[supkhk2+n(n−1) ¯R](supkhk2−nR).¯ (45)

But it is clear from (44) that (45) is equivalent to nc−(n1) ¯R−n−2n supkhk2

>n−2n p

[supkhk2+n(n−1) ¯R](supkhk2−nR).¯ (46)

Hence we have

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P( ¯R,supkhk2)>0.

(47)

On the other hand, 2(nH) = P

i,j

(nHδij−hn+1ij )(nH)ij =P

i

(nH−hn+1ii )(nH)ii

= nP

i

H(nH)iiP

i

λi(nH)ii(n|H|max−C)∆(nH), (48)

where|H|maxis the maximum of the mean curvatureH andCis the minimum of the principal curvaturesi}ni=1 ofMn.

Now we consider the following smooth function on Mn defined by F =−(f2+ a)−1/2, where a(>0) is a real number andf is a non-negativeC2-function onMn. From the hypothesis of the Theorem 2 and the Gauss equation which implies Ricci curvatureRic≥n−1n24H2, we know that the Ricci curvature is bounded below.

Obviously, F is bounded, so we can apply Lemma 2 toF. For any ε >0, there is a point x∈Mn, such that at which F satisfies the properties (24) in Lemma 2. By a simple and direct calculation, we have

F4F = 3kdFk21

2F4∆f2. (49)

From (24),(49) 1

2F4(x)4f2(x) = 3kdFk2(x)−F(x)4F(x)<2−εF(x).

(50)

Thus, for any convergent sequencem}withεm>0 and limm→∞εm= 0, there exists a point sequence{xm}such that the sequence{F(xm)}converges toF0(we can take a subsequence if necessary) and satisfies (24), hence, limm→∞εm[3εm−F(xm)] = 0.

From the definition of supremum and (24), we have limm→∞F(xm) = F0 = supF and hence the definition ofF gives rise to limm→∞f(xm) =f0= supf.

Now we set f =

nH, so limm→∞(nH)(xm) = sup(nH), thus by (13)

limm→∞khk2(xm) = supkhk. Under the hypothesis of the Theorem 2, by (42), (48) and (50) we have

0 12F4(xm)n−1n [khk2(xm)−nR]P¯ ( ¯R,khk2(xm)) 12F4(xm)2[nH(xm)]

(n|H|max−C)12F4(xm)∆(nH)(xm)

< (n|H|max−C)(3ε2m−εmF(xm)).

(51)

Letm→ ∞in (51). Then we have

[supkhk2−nR]P¯ ( ¯R,supkhk2) = 0.

(52)

By (47), we have supkhk2=nR. From (40) and sup(khk¯ 2−nH2) = 0 we getkhk2= nH2, and soMn is totally umbilical.

(2). If khk2= min{α(n,R), β(n,¯ R)}, then we have¯ khk2=α(n,R); or¯ khk2=β(n,R).¯ (i). Ifkhk2=β(n,R), then¯ khk2≤α(n,R). This is equivalent to¯

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[nc(n1) ¯R−n−2

n khk2]2(n2)2

n2 [khk2+n(n−1) ¯R](khk2−nR).¯ (53)

Hence, we have

0 (n2)2

n2 [khk2+n(n−1) ¯R](khk2−nR)¯ 0,

which meanskhk2=nR. By (40)¯ khk2=nH2, i.e.,M is totally umbilical.

(ii). If khk2=α(n,R), then the equality in (53) holds. Since¯ khk2 ≤β(n,R), we¯ have

nc−(n1) ¯R−n−2

n khk2= n−2 n

q

[khk2+n(n−1) ¯R](khk2−nR),¯ i.e., P( ¯R,khk2) = 0. Since khk2 =α(n,R) =¯ const., from (13) we haveH =const..

Therefore we know that ∆(nH) = 0. By (48) we have2(nH)0. From (42) we get 2(nH) = 0. Thus the equalities in (42),(41),(39),(38) and (23) in Lemma 1 hold. When the equalities in (42),(41) hold, we have n1khk2 = n−2n khk2, i.e., n= 3. When the equality in (38) holds, we havekµk2=khk2−nH2. Hence by (19), we havekτk= 0.

Sinceen+1is parallel on the normal bundleT(Mn) ofMn, using the method of Yau [14], we knowM3 lies in a totally geodesic submanifoldS14(c) ofSp3+p(c). When the equalities in (23) of Lemma1 hold, after renumberation if necessary, we can assume that λ=λ16=λ2 =λ3=µ, i.e.,M3 has two distinct principal curvatures, one with the multiplicity 1 and the other with the multiplicity 2. Therefore by [9] or [1],M3 is a hyperbolic cylinder H1(c−λ2)×S2(c−µ2) inS14(c). This completes the proof of the Theorem 2.

Acknowledgements. The author is very grateful to the referee for a careful reading and very helpful suggestions on the earlier version of the manuscript.

This work is partially supported by the National Natural Science Foundation of China and Natural Science Foundation of Shaanxi province.

References

[1] Abe, N., Koike, N., Yamaguchi,Congrence theorems for proper semi-Riemannian hypersurface in a real space form, Yokohama Math.J. 35 (1987), 123-136.

[2] Akutagawa K.,On space-like hypersurface with constant mean curvature in the de Sitter space, Math. Z. 196 (1987), 13-19.

[3] Alencar H. and do Carmo, M.P.,Hypersurfaces with constant mean curvature in spheres, Proc. Amer. Math. Soc, 120 (1994), 1223-1229.

[4] Cheng Q.M.,Complete space-like submanifolds in a de Sitter space with parallel mean curvature vector, Math. Z. 206 (1991), 333-339.

[5] Cheng, Q.M. and Ishikawa, S.,Space-like hypersurfaces with constant scalar cur- vature, Manuscripta Math. 95 (1998), 499-505.

[6] Cheng, S.Y. and Yau, S.T.,Hypersurfaces with constant scalar curvature, Math.

Ann. 225 (1977), 195-204.

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[7] Goddard, A.J.,Some remarks on the existence of space-like hypersurfaces of con- stant mean curvature, Math. Proc. Combrige Phil. Soc. 82 (1997), 489-495.

[8] Liu X.,Complete space-like hypersurfaces with constant scalar curvature, Manu- scripta Math. 105 (2001), 367-377.

[9] Montiel, S., A characterization of hyperbolic cylinders in the de Sitter space, Tˆohoku Math. J. 48 (1996), 23-31.

[10] Omori,H.,Isometric immersion of Riemmanian manifolds, J. Math. Soc. Japan 19 (1967), 205-214.

[11] Remanathan J., Complete space-like hypersurfaces of constant mean curvature in the de Sitter space, Indiana Univ. Math. J. 36 (1987), 349-359.

[12] Santos, W.,Submanifolds with parallel mean curvature vector in spheres, Tˆohoku Math. J. 46 (1994), 403-415.

[13] Yau S.T.,Harmonic functions on complete Riemannian manifolds, Comm. Pure and Appl. Math. 28 (1975), 201-228.

[14] Yau,S.T.,Submanifolds with constant mean curvature, Amer. J. Math 96 (1974), 346-366.

[15] Zheng,Y., On space-like hypersurfaces in the de Sitter spaces, Annals of Global Analysis and Geometry 13 (1995), 317-321.

[16] Zheng,Y.,Space-like hypersurfaces with constant scalar curvature in the de Sitter space, Diff. Geom. Appl. 6 (1996), 51-54.

Shu Shichang

Department of Applied Mathematics, Xidian University, Xi’an 710071, Shaanxi,P.R.China.

e-mail addresses: [email protected], Current address: Department of Mathematics, Xianyang Teachers’ University,

Xianyang, 712000, Shaanxi, P.R.China Liu Sanyang

Department of Applied Mathematics, Xidian University, Xi’an 710071, Shaanxi, P.R.China.

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