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certain conditions

Cihan ¨ Ozg¨ur and Sibel Sular

Abstract.This paper deals withN(k)-quasi Einstein manifolds satisfying the conditionsR(ξ, X)·C= 0 andR(ξ, XCe= 0, whereCandCedenote the Weyl conformal curvature tensor and the quasi-conformal curvature tensor, respectively.

M.S.C. 2000: 53C25.

Key words:k-nullity distribution, quasi Einstein manifold,N(k)-quasi Einstein man- ifold, Weyl conformal curvature tensor, quasi-conformal curvature tensor.

1 Introduction

The notion of a quasi-Einstein manifold was introduced by M. C. Chaki in [2]. A non-flat n-dimensional Riemannian manifold (M, g) is said to be a quasi Einstein manifoldif its Ricci tensorS satisfies

(1.1) S(X, Y) =ag(X, Y) +(X)η(Y), X, Y ∈T M

for some smooth functionsaandb6= 0, whereη is a nonzero 1-form such that (1.2) g(X, ξ) =η(X), g(ξ, ξ) =η(ξ) = 1

for the associated vector fieldξ. The 1-formη is called the associated 1-form and the unit vector fieldξis called the generator of the manifold. If b= 0 then the manifold is reduced to an Einstein manifold. If the generatorξbelongs tok-nullity distribution N(k) then the quasi Einstein manifold is called as an N(k)-quasi Einstein manifold [6]. In [6], it was proved that a conformally flat quasi-Einstein manifold isN(k)-quasi Einstein. Consequently, it was shown that a 3-dimensional quasi-Einstein manifold is an N(k)-quasi-Einstein manifold. The derivation conditions R(ξ, X)·R = 0 and R(ξ, X)·S= 0 were also studied in [6], whereRandSdenote the curvature and Ricci tensor, respectively. In [4], the derivation conditionsZ(ξ, X)· Z= 0,Z(ξ, X)·R= 0 andR(ξ, X)· Z = 0 onN(k)-quasi Einstein manifolds were studied, where Z is the concircular curvature tensor. Moreover, in [4], for anN(k)-quasi Einstein manifold,

Balkan Journal of Geometry and Its Applications, Vol.13, No.2, 2008, pp. 74-79.

c

°Balkan Society of Geometers, Geometry Balkan Press 2008.

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it was proved thatk=n−1a+b. In this study, we considerN(k)-quasi Einstein manifolds satisfying the conditionsR(ξ, X)·C= 0 andR(ξ, X)·Ce= 0. The paper is organized as follows: In Section 2, we give the definitions of Weyl conformal curvature tensor and quasi-conformal curvature tensor. In Section 3, we give a brief introduction about N(k)-quasi Einstein manifolds. In Section 4, we prove that for an n≥4 dimensional N(k)-quasi Einstein manifold, the conditionR(ξ, X)·C= 0 orR(ξ, X)·Ce= 0 holds on the manifold if and only if eithera=−bor the manifold is conformally flat.

2 Preliminaries

Let (Mn, g) be a Riemannian manifold. We denote byC and Ce theWeyl conformal curvature tensor[7] and thequasi-conformal curvature tensor[8] of (Mn, g) which are defined by

C(X, Y)Z = R(X, Y)Z 1

n−2{S(Y, Z)X−S(X, Z)Y +g(Y, Z)QX−g(X, Z)QY}

(2.1)

+ r

(n1)(n2){g(Y, Z)X−g(X, Z)Y} and

C(X, Ye )Z = λR(X, Y)Z+µ{S(Y, Z)X−S(X, Z)Y +g(Y, Z)QX−g(X, Z)QY}

(2.2)

−r n[ λ

n−1+ 2µ]{g(Y, Z)X−g(X, Z)Y},

respectively, where λ and µ are arbitrary constants, which are not simultaneously zero. HereQis the Ricci operator defined by

S(X, Y) =g(QX, Y).

Ifλ= 1 and µ=n−21 then the quasi-conformal curvature tensor is reduced to the Weyl conformal curvature tensor. For ann≥4 dimensional Riemannian manifold if C= 0 then the manifold is said to be conformally flat [7], ifCe = 0 then it is called asquasi-conformally flat [8].R·C andR·Ce are defined by

(2.3) (R(U, X)·C)(Y, Z, W) =R(U, X)C(Y, Z)W −C(R(U, X)Y, Z)W

−C(Y, R(U, X)Z)W−C(Y, Z)R(U, X)W.

and

(2.4) (R(U, X)·C)(Y, Z, We ) =R(U, X)C(Y, Z)We −C(R(U, X)Y, Z)We

−C(Y, R(U, X)Z)We −C(Y, Z)R(U, Xe )W,

respectively, for all vector fieldsU, X, Y, Z, W where R(U, X) acts onC andCe as a derivation [3].

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3 N (k)-quasi Einstein manifolds

From (1.1) and (1.2) it follows that

(3.1) S(X, ξ) = (a+b)η(X),

(3.2) r=na+b,

whereris the scalar curvature ofMn.

Thek-nullity distributionN(k) [5] of a Riemannian manifoldMn is defined by N(k) :p→Np(k) ={U ∈TpM |R(X, Y)U =k(g(Y, U)X−g(X, U)Y)}

for allX, Y ∈T Mn, wherek is some smooth function. In a quasi-Einstein manifold Mn if the generatorξbelongs to somek-nullity distributionN(k), then we get (3.3) R(ξ, Y)U =k(g(Y, U)ξ−η(U)Y)

andMn is said to be anN(k)-quasi Einstein manifold[6]. In fact, kis not arbitrary as we see in the following:

Lemma 3.1. [4] In ann-dimensionalN(k)-quasi Einstein manifold it follows that

(3.4) k= a+b

n−1.

4 Main Results

In this section, we give the main results of the paper. At first, we give the following theorem:

Theorem 4.1. Let Mn be an n-dimensional,n≥4,N(k)-quasi Einstein manifold.

ThenMn satisfies the conditionR(ξ, X)·C= 0if and only if eithera=−borM is conformally flat.

Proof.Assume thatMn,(n4), is anN(k)-quasi Einstein manifold and satisfies the conditionR(ξ, X)·C= 0.Then from (2.3) we can write

0 = R(ξ, X)C(Y, Z)W −C(R(ξ, X)Y, Z)W

−C(Y, R(ξ, X)Z)W −C(Y, Z)R(ξ, X)W.

(4.1)

So using (3.3) and (3.4) in (4.1) we find 0 = a+b

n−1{C(Y, Z, W, X)ξ−η(C(Y, Z)W)X

−g(X, Y)C(ξ, Z)W+η(Y)C(X, Z)W

−g(X, Z)C(Y, ξ)W +η(Z)C(Y, X)W

−g(X, W)C(Y, Z)ξ+η(W)C(Y, Z)X}.

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Then eithera+b= 0 or

0 = C(Y, Z, W, X−η(C(Y, Z)W)X

−g(X, Y)C(ξ, Z)W+η(Y)C(X, Z)W

−g(X, Z)C(Y, ξ)W +η(Z)C(Y, X)W (4.2)

−g(X, W)C(Y, Z)ξ+η(W)C(Y, Z)X.

Taking the inner product of (4.2) withξwe get

0 = C(Y, Z, W, X)−η(X)η(C(Y, Z)W)

−g(X, Y)η(C(ξ, Z)W) +η(Y)η(C(X, Z)W)

−g(X, Z)η(C(Y, ξ)W) +η(Z)η(C(Y, X)W) (4.3)

−g(X, W)η(C(Y, Z)ξ) +η(W)η(C(Y, Z)X).

In view of (2.1), (1.1) and (3.3) we have

(4.4) η(C(Y, Z)W) = 0.

So using (4.4) into (4.3) we obtain

(4.5) C(Y, Z, W, X) = 0,

i.e., Mn is conformally flat. The converse statement is trivial. This completes the proof of the theorem.¤

It is known [1] that a quasi-conformally flat manifold is either conformally flat or Einstein.

So we have the following corollary:

Corollary 4.2. If (Mn, g)is a quasi-conformally flat N(k)-quasi Einstein manifold then it is conformally flat.

As a generalization of Theorem 4.1 we have the following theorem:

Theorem 4.3. Let Mn be an N(k)-quasi Einstein manifold. Then the condition R(ξ, X)·Ce = 0holds on Mn if and only if eithera=−b or Mn is conformally flat withλ=µ(2−n).

Proof. Since the manifold satisfies the condition R(ξ, X)·Ce = 0, by the use of (2.4)

0 = R(ξ, Y)C(U, Ve )W −C(R(ξ, Ye )U, V)W

−C(U, R(ξ, Ye )V)W −C(U, Ve )R(ξ, Y)W.

(4.6)

SinceMn isN(k)-quasi Einstein by making use of (3.3) and (3.4) in (4.6) we get 0 = a+b

n−1

nC(U, V, W, Ye )ξ−η(C(U, Ve )W)Y

−g(Y, U)C(ξ, Ve )W+η(U)C(Y, Ve )W

−g(Y, V)C(U, ξ)We +η(V)C(U, Ye )W

−g(Y, W)C(U, Ve )ξ+η(W)C(U, Ve )Yo .

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Then eithera=−b or

0 =C(U, V, W, Ye )ξ−η(C(U, Ve )W)Y

−g(Y, U)C(ξ, Ve )W+η(U)C(Y, Ve )W

−g(Y, V)C(U, ξ)We +η(V)C(U, Ye )W (4.7)

−g(Y, W)C(U, Ve )ξ+η(W)C(U, Ve )Y.

Assume thata6=−b. Taking the inner product of (4.7) withξwe obtain 0 = C(U, V, W, Ye )−η(C(U, Ve )W)η(Y)

−g(Y, U)η(C(ξ, Ve )W) +η(U)η(C(Y, Ve )W)

−g(Y, V)η(C(U, ξ)We ) +η(V)η(C(U, Ye )W) (4.8)

−g(Y, W)η(C(U, Ve )ξ) +η(W)η(C(U, Ve )Y).

On the other hand, from (2.2), (3.3) and (3.1) we have (4.9) η(C(U, Ve )W) = b

n[µ(n2) +λ]{g(V, W)η(U)−g(U, W)η(V)}, for all vector fieldsU, V, W onMn. So putting (4.9) into (4.8) we obtain

C(U, V, W, Ye ) = b

n[µ(n2) +λ]{g(V, W)g(Y, U)−g(Y, V)g(U, W)}. Then using (2.2) we can write

λR(U, V, W, Y) +µ{S(V, W)g(Y, U)

−S(U, W)g(V, Y) +g(V, W)S(Y, U)−g(U, W)S(V, Y)}

−na+b n [ λ

n−1+ 2µ]{g(Y, U)g(V, W)−g(Y, V)g(U, W)}

(4.10)

= b

n[µ(n2) +λ]{g(V, W)g(Y, U)−g(Y, V)g(U, W)}. Contracting (4.10) overY andU we get

[λ+µ(n−2)]{S(V, W)(a+b)g(V, W)}= 0.

SinceMnis not EinsteinS(V, W)6= (a+b)g(V, W) so we obtainλ=µ(2−n). Hence from (4.9)

(4.11) η(C(U, Ve )W) = 0

holds for every vector fieldsU, V, W. So using (4.11) in (4.8) we obtainC(U, V, W, Ye ) = 0. Then by the use of Corollary 4.2, the quasi-conformally flatness gives us the confor- mally flatness of the manifold. Conversely, ifCe= 0 then the conditionR(ξ, XCe= 0 holds trivially. Ifa=−b thenR(ξ, X) = 0 thenR(ξ, X)·Ce= 0. Hence the proof of the theorem is completed.¤

So using Theorem 4.1 and Theorem 4.3 we have the following corollary:

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Corollary 4.4. Let Mn be an N(k)-quasi Einstein manifold. Then the following conditions are equivalent:

i)R(ξ, X)·C= 0 withλ=µ(2−n), ii) R(ξ, X)·Ce= 0,

iii) M is conformally flat with λ=µ(2−n).

References

[1] K. Amur, Y. B. Maralabhavi,On quasi-conformally flat spaces, Tensor (N.S.) 31, 2 (1977), 194-198.

[2] M. C. Chaki and R. K. Maity,On quasi Einstein manifolds, Publ. Math. Debrecen 57, 3-4 (2000), 297-306.

[3] R. Deszcz,On pseudosymmetric spaces, Bull. Soc. Belg. Math., Ser. A. 44 (1992), 1-34.

[4] C. ¨Ozg¨ur and M. M. Tripathi, On the concircular curvature tensor of anN(k)- quasi Einstein manifold, Math. Pannon. 18, 1 (2007), 95-100.

[5] S. Tanno,Ricci curvatures of contact Riemannian manifolds, Tˆohoku Math. J.

40 (1988), 441-448.

[6] M. M. Tripathi and J. S. Kim, On N(k)-quasi Einstein manifolds, Commun.

Korean Math. Soc. 22, 3 (2007), 411-417.

[7] K. Yano and M. Kon,Structures on manifolds, Series in Pure Mathematics, 3.

World Scientific Publishing Co., Singapore, 1984.

[8] K. Yano and S. Sawaki,.Riemannian manifolds admitting a conformal transfor- mation group, J. Differential Geometry 2 (1968), 161-184.

Authors’ address:

Cihan ¨Ozg¨ur and Sibel Sular Department of Mathematics,

Balıkesir University, 10145, Balıkesir, Turkey.

E-mail: [email protected], [email protected]

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