AHMET YILDIZ, UDAY CHAND DE and ERHAN ATA
Communicated by the former editorial board
The object of the present paper is to introduce a new concept called generalized η-Einstein manifold in a Lorentzian Para-Sasakian manifold. Some geometric properties have been studied. Finally an example has been constructed to prove the existance of a generalizedη-Einstein Lorentzian Para-Sasakian manifold.
AMS 2010 Subject Classification: 53B20, 53B25, 53B50.
Key words: Lorentzian Para-Sasakian manifolds,η-Einstein manifold, general- izedη-Einstein Lorentzian Para-Sasakian manifold.
1. INTRODUCTION
A Lorentzian Para-Sasakian manifold Mn is said to be an η-Einstein manifold if the following condition
(1.1) S(X, Y) =ag(X, Y) +bη(X)η(Y), holds on Mn,wherea, b are smooth functions.
A Lorentzian Para-Sasakian manifold Mn is said to be a generalized η- Einstein manifold if the following condition
(1.2) S(X, Y) =ag(X, Y) +bη(X)η(Y) +cΩ(X, Y),
holds on M, where a, b, c are smooth functions and Ω(X, Y) = g(φX, Y). If c= 0 then the manifold reduces to anη-Einstein manifold.
In the present paper we have studied generalized η-Einstein manifold in a Lorentzian Para-Sasakian manifold. The paper is organized as follows: After Preliminaries in Section 3 we study some geometric properties of generalizedη- Einstein Lorentzian Para-Sasakian manifolds and conformally flat generalized η-Einstein Lorentzian Para-Sasakian manifolds. In the last section we construct an example of a generalized η-Einstein Lorentzian Para-Sasakian manifold.
MATH. REPORTS16(66),1(2014), 61–67
2.PRELIMINARIES
In [1], K. Matsumoto introduced the notion of Lorentzian Para-Sasakian (brieflyLP-Sasakian) manifold. In [2], the authors defined the same notion in- dependently and they obtained many results about this type manifold (see also [3] and [8]). Several authors have studied Lorentzian para-Sasakian manifolds such as [4, 7, 9] and many others.
LetMnbe ann-dimensional differentiable manifold equipped with a triple (φ, ξ, η),whereφis a (1,1)-tensor field,ξ is a vector field,η is a 1-form onMn such that
(2.1) η(ξ) =−1,
(2.2) φ2 =I+η⊗ξ,
which implies
(2.3) i) φξ = 0, ii) η(φ) = 0, iii) rank(φ) =n−1.
Then Mn admits a Lorentzian metric g, such that (2.4) g(φX, φY) =g(X, Y) +η(X)η(Y),
and Mn is said to admit a Lorentzian almost paracontact structure (φ,ξ,η,g).
In this case, we have
(2.5) g(X, ξ) =η(X), ∇Xξ=φX,
Ω(X, Y) =g(X, φY) =g(φX, Y) = Ω(Y, X).
In (2.1) and (2.2) if we replaceξby−ξ, then the triple (φ,ξ,η) is an almost paracontact structure onMndefined by Sato [5]. The Lorentzian metric given by (2.5) stands analogous to the almost paracontact Riemannian metric for any almost paracontact manifold (see [5, 6]).
A Lorentzian almost paracontact manifold Mn equipped with the struc- ture (φ,ξ,η,g) is called Lorentzian paracontact manifold [1] if
Ω(X, Y) = 1
2((∇Xη)Y + (∇Yη)X).
A Lorentzian almost paracontact manifold Mn equipped with the struc- ture (φ,ξ,η,g) is calledLorentzian para-Sasakian manifold (brieflyLP-Sasakian manifold) [1] if
(∇Xφ)Y =g(φX, φY)ξ+η(Y)φ2X.
In aLP-Sasakian manifold the 1-formη is closed. Also in [1], it is proved that if an n-dimensional Lorentzian manifold (Mn, g) admits a timelike unit vector field ξ such that the 1-form η associated to ξ is closed and satisfies
(∇X∇Yη)W =g(X, Y)η(W) +g(X, W)η(Y) + 2η(X)η(Y)η(W),
thenMn admits anLP-Sasakian structure.
By definition the Weyl conformal curvature tensor C is given by [10]
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] (2.6)
+ τ
(n−1)(n−2)[g(Y, Z)X−g(X, Z)Y],
where R, S, Q and τ denotes the curvature tensor of type (1,3), Ricci tensor, Ricci operator and scalar curvature of M respectively.
For dimM > 3, if C = 0, then the manifold is called conformally flat manifold.
3. MAIN RESULTS
In this section, we give main results of the paper. At first we give the following:
Theorem 3.1. ξ is an eigenvector of the Ricci tensorS corresponding to the eigen value a−b.
Proof. In (1.2) puttingY =ξ, and using (2.1), (2.3) i) and Ω(X, ξ) = 0, we get
(3.1) S(X, ξ) = (a−b)η(X),
which means that ξ is an eigenvector of the Ricci tensor S corresponding to the eigen valuea−b.
Now, puttingX=ξin (3.1) and again using (2.1), we haveS(ξ, ξ) =b−a.
Now we can state the following:
Theorem 3.2. The scalar b−ais the Ricci curvature in the direction of the generator ξ.
Theorem 3.3. If the Ricci tensor S of type (0,2) of an LP-Sasakian manifold is non-vanishing and satisfies the relation
S(Y, Z)S(X, W)−S(X, Z)S(Y, W) = ρ[g(Y, Z)g(X, W)−g(X, Z)g(Y, W)]
+g(φX, W)g(Y, Z), (3.2)
where ρ is non-zero scalar, then the manifold is a generalized η-Einstein man- ifold.
Proof. PuttingY =Z =ξ in (3.2), we obtain
S(ξ, ξ)S(X, W)−S(X, ξ)S(ξ, W) = ρ[g(ξ, ξ)g(X, W)−g(X, ξ)g(ξ, W)]
+g(φX, W)g(ξ, ξ), which can be written as
(n−1)S(X, W)−(n−1)2η(X)η(W) = ρ[g(X, W)−η(X)η(W)]
−g(φX, W).
(3.3)
Now, (3.3) can be written as
S(X, W) =αg(X, W) +βη(X)η(W) +γΩ(X, W), whereα =−n−1ρ , β = (n−1)− n−1ρ , γ =−n−11 .
Since S 6= 0, ρ is a non-zero scalar, it follows that α, β, γ are non-zero scalars.
This completes the proof.
Now, we consider conformally flat generalized η-Einstein LP-Sasakian manifolds of dim >3.
If a generalizedη-EinsteinLP-Sasakian manifold is conformally flat, then using (1.2) in (2.6), we get
R(X, Y)Z = [ 2α
n−2+ τ
(n−1)(n−2)][g(X, Z)Y −g(Y, Z)X]
+ β
n−2[g(X, Z)η(Y)ξ−g(Y, Z)η(X)ξ +η(X)η(Z)Y −η(Y)η(Z)X]
(3.4)
+ γ
n−2[g(X, Z)φY −g(Y, Z)φX + Ω(X, Z)Y −Ω(Y, Z)X].
Putting Y =ξ in (3.4), we have R(X, ξ)Z = [ 2α
n−2+ τ
(n−1)(n−2)]g(X, Z)ξ (3.5)
− β
n−2g(X, Z)ξ+ γ
n−2Ω(X, Z)ξ, for all X, Y, Z ∈ξ⊥. Again puttingZ =ξ in (3.5), we have
(3.6) R(X, ξ)ξ= 0,
for all X, Y, Z ∈ξ⊥. Now we give the following:
Theorem 3.4. In a conformally flat generalizedη-Einstein LP-Sasakian manifold, the curvature tensor of type (1,3) satisfies the following properties (3.4), (3.5) and (3.6 ) for allX, Y, Z ∈ξ⊥, the(n−1)-dimensional distribution orthogonal to the distribution ξ.
From (3.6), we can state the following:
Corollary3.5. In a conformally flat generalizedη-EinsteinLP-Sasakian manifold the sectional curvature of the plane determined by X, ξ is zero.
4. EXAMPLE
We consider a 3-dimensional manifold M = {(x, y, z) ∈ R3}, where (x, y, z) are the standard coordinates of R3. Let {e1, e2, e3} be linearly in- dependent global frame onM given by
e1 =ez ∂
∂x, e2 =ez−ax ∂
∂y, e3 = ∂
∂z, wherea is non-zero constant.
Let g be the Lorentzian metric defined by
g(e1, e3) =g(e1, e2) =g(e2, e3) = 0, g(e1, e1) =g(e2, e2) = 1, g(e3, e3) =−1.
Let η be the 1-form defined by
η(X) =g(X, e3),
for any X∈χ(M) . Let φbe the (1,1) tensor field defined by φe1 =−e1, φe2=−e2, φe3 = 0.
Then, using the linearily of φand g, we have η(e3) =−1, φ2X=X+η(X)e3
and
g(φX, φY) =g(X, Y) +η(X)η(Y),
for any X, Y ∈ χ(M). Thus, for e3 = ξ, (φ, ξ, η, g) defines a Lorentzian paracontact structure on M.
Let∇be the Levi-Civita connection with respect to the Lorentzian metric g and R be the curvature tensor ofg. Then we have
[e1, e2] =−aeze2, [e1, e3] =−e1, [e2, e3] =−e2.
Taking e3 =ξ and using Koszul formula for the Lorentzian metric g, we have
∇e1e1 =−e3, ∇e1e2 = 0, ∇e1e3=−e1
∇e2e1 =aeze2, ∇e2e2=−aeze1−e3, ∇e2e3=−e2
∇e3e1 = 0, ∇e3e2= 0, ∇e3e3= 0.
From the above it can be easily seen that (φ, ξ, η, g) is an LP-Sasakian structure on M . So, M3(φ, ξ, η, g) is an LP-Sasakian manifold. Using the
above relations, we can easily calculate the non-vanishing components of the curvature tensor R as follows:
R(e2, e3)e3 =−e2, R(e1, e3)e3 =−e1, R(e1, e2)e2 = (1−a2e2z)e1 R(e2, e3)e2 =−aeze1−e3, R(e1, e3)e1=−e3, R(e1, e2)e1 =−(1−a2e2z)e2
and the components which can be obtained from these by the symmetry prop- erties. From the above, we can easily calculate the non-vanishing components of the Ricci tensorS as follows:
S(e1, e1) =−a2e2z, S(e2, e2) =−a2e2z, S(e3, e3) =−2.
Since {e1, e2, e3} forms a basis, any vector field X, Y ∈ χ(M) can be written as
X =a1e1+b1e2+c1e3 and
Y =a2e1+b2e2+c2e3, wherea1, a2, b1, b2, c1, c2∈R+.Hence,
g(X, Y) =a1a2+b1b2−c1c2
and
S(X, Y) =−
(a1a2+b1b2)a2e2z+ 2c1c2 . Let Ω(X, Y) be a (0,2) tensor defined by
Ω(X, Y) =g(φX, Y) . Then
Ω(e1, e1) =g(φe1, e1) =g(−e1, e1) =−1 Ω(e2, e2) =g(φe2, e2) =g(−e2, e2) =−1 and
Ω(e3, e3) =g(φe3, e3) =g(0, e3) = 0.
We take the scalars a´,band f respectively as follows:
a´= 1−2a2e2z, b=−(1 + 2a2e2z),
f = 1−a2e2z. Then, we have
S(e1, e1) =a´g(e1, e1) +bη(e1)η(e1) +f Ω(e1, e1), S(e2, e2) =a´g(e2, e2) +bη(e2)η(e2) +f Ω(e2, e2), S(e3, e3) =a´g(e3, e3) +bη(e3)η(e3) +f Ω(e3, e3).
Thus, the manifold under consideration is a generalized η-Einstein LP- Sasakian manifold.
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Received 25 October 2011 Inonu University,
Education Faculty, Malatya 44280, Turkey
a.yildiz@inonu.edu.tr ayildiz44@yahoo.com Calcutta University, Department of Pure Mathematics,
35, Ballygaunge Circular Road, Kolkata 700019, West Bengal, India
uc de@yahoo.com Dumlupınar University, Department of Mathematics,
K¨utahya, Turkey erhan.ata@dumlupinar.edu.tr