On weakly symmetric Kenmotsu manifolds



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On weakly symmetric Kenmotsu manifolds C ihan Özgür Abstract. We consider weakly symmetric and weakly Ricci-symmetric Kenmotsu manifolds. We show that there exist no weakly symmetric and weakly Ricci-symmetric Kenmotsu manifolds unless α+σ+γ and ρ+µ+υ are everywhere zero, respectively. M.S.C. 2000: 53C21, 53D15. Key words: Kenmotsu manifold, weakly symmetric manifold, weakly Ricci-symmetric manifold. 1 Introduction The notions of weakly symmetric and weakly Ricci-symmetric manifolds were introduced by L. Tamássy and T. Q. Binh in [8] and [9]. A non-flat n-dimensional differentiable manifold (M, g), n > 3, is called pseudosymmetric if there exists a 1-form α on M such that ( X R)(Y, Z, V ) = 2α(X)R(Y, Z)V + α(y )R(X, Z)V +α(z)r(y, X)V + α(v )R(Y, Z)X + g(r(y, Z)V, X)A, where X, Y, Z, V χ(m) are arbitrary vector fields and α is a 1-form on M. A χ(m) is the vector field corresponding through g to the 1-form α which is given by g(x, A) = α(x) (see [2]). A non-flat n-dimensional differentiable manifold (M, g), n > 3, is called weakly symmetric (see [8] and [9]) if there exist 1-forms α, β, γ and σ such that the condition (1.1) ( X R)(Y, Z, V ) = α(x)r(y, Z)V + β(y )R(X, Z)V +γ(z)r(y, X)V + σ(v )R(Y, Z)X + g(r(y, Z)V, X)P holds for all vector fields X, Y, Z, V χ(m). A weakly symmetric manifold (M, g) is pseudosymmetric if β = γ = σ = 1 2α and P = A, locally symmetric if α = β = γ = σ = 0 and P = 0. A weakly symmetric manifold is said to be proper if at least one of the 1-forms α, β, γ and σ is not zero or P 0. A non-flat n-dimensional differentiable manifold (M, g), n > 3, is called weakly Ricci-symmetric (see [8] and [9]) if there exist 1-forms ρ, µ, υ such that the condition (1.2) ( X S)(Y, Z) = ρ(x)s(y, Z) + µ(y )S(X, Z) + υ(z)s(x, Y ), Differential Geometry - Dynamical Systems, Vol.8, 2006, pp. 204-209. c Balkan Society of Geometers, Geometry Balkan Press 2006.

On weakly symmetric Kenmotsu manifolds 205 holds for all vector fields X, Y, Z χ(m). If ρ = µ = υ then M is called pseudo Ricci-symmetric (see [3]). If M is weakly symmetric, from (1.1), we have (1.3) ( X S)(Z, V ) = α(x)s(z, V ) + β(r(x, Z)V ) + γ(z)s(x, V ) +σ(v )S(X, Z) + p(r(x, V )Z), where p is defined by p(x) = g(x, P ) for all X χ(m) (see [9]). In [9], it was considered weakly symmetric and weakly Ricci-symmetric Einstein and Sasakian manifolds. In [5] and [7], the authors studied weakly symmetric and weakly Ricci-symmetric K-contact manifolds and Lorentzian para-sasakian manifolds, respectively. In this study, we consider weakly symmetric and weakly Ricci symmetric Kenmotsu manifolds. 2 Preliminaries Let (M, ϕ, ξ, η, g) be an n-dimensional almost contact metric manifold, where ϕ is a (1,1) tensor field, ξ is the structure vector field, η is a 1-form and g is the Riemannian metric. It is well-known that (ϕ, ξ, η, g) satisfy (2.1) η(ξ) = 1, ϕξ = 0, (2.2) η(x) = g(x, ξ), ϕ 2 X = X + η(x)ξ, (2.3) η(ϕx) = 0, g(ϕx, ϕy ) = g(x, Y ) η(x)η(y ), for any vector fields X, Y on M (see [1]). If moreover (2.4) ( X ϕ)y = g(x, ϕy )ξ η(y )ϕx, (2.5) X ξ = X η(x)ξ, where denotes the Riemannian connection of g, then (M, ϕ, ξ, η, g) is called a Kenmotsu manifold. In a Kenmotsu manifold (see [6]), the following relations hold (2.6) ( X η)y = g(x, Y ) η(x)η(y ), (2.7) R(ξ, X)Y = η(y )X g(x, Y )ξ, (2.8) S(X, ξ) = (1 n)η(x), for any vector fields X, Y where R is the Riemannian curvature tensor and S is the Ricci tensor.

206 C ihan Özgür 3 Weakly symmetric Kenmotsu Manifolds In this chapter, we investigate weakly symmetric and weakly Ricci-symmetric Kenmotsu manifolds. Firstly we have; Theorem 3.1 There is no weakly symmetric Kenmotsu manifold M, n > 3, unless α + σ + γ is everywhere zero. Proof. Assume that M is a weakly symmetric Kenmotsu manifold. By the covariant differentiation of the Ricci tensor S with respect to X we have (3.1) ( X S)(Z, V ) = X S(Z, V ) S( X Z, V ) S(Z, X V ). So replacing V with ξ in (3.1) and using (2.8), (2.5) and (2.2) we obtain (3.2) ( X S)(Z, ξ) = (1 n)g(x, Z) S(X, Z). On the other hand replacing V with ξ in (1.3) and by the use of (2.7), (2.8), (2.1) and (2.2) we get (3.3) ( X S)(Z, ξ) = (1 n)α(x)η(z) + η(x)β(z) η(z)β(x) +(1 n)γ(z)η(x) + σ(ξ)s(x, Z) + g(x, Z)p(ξ) η(z)p(x). Hence, comparing the right hand sides of the equations (3.2) and (3.3) we have (3.4) (1 n)g(x, Z) S(X, Z) = (1 n)α(x)η(z) + η(x)β(z) η(z)β(x) +(1 n)γ(z)η(x) + σ(ξ)s(x, Z) + g(x, Z)p(ξ) η(z)p(x). Therefore putting X = Z = ξ in (3.4) and using (2.8) and (2.1) we get Since n > 3, so we obtain (1 n) (α(ξ) + σ(ξ) + γ(ξ)) = 0. (3.5) α(ξ) + σ(ξ) + γ(ξ) = 0 holds on M. Now we will show that α + σ + γ = 0 holds for all vector fields on M. In (1.3) taking Z = ξ similar to the previous calculations it follows that (3.6) (1 n)g(x, V ) S(X, V ) = (1 n)α(x)η(v ) +g(x, V )β(ξ) η(v )β(x) + γ(ξ)s(x, V ) +(1 n)σ(x)η(x) + η(x)p(v ) η(v )p(x). Putting V = ξ in (3.6) by virtue of (2.1) and (2.8) we get (3.7) 0 = (1 n)α(x) + η(x)β(ξ) β(x) + (1 n)γ(ξ)η(x) +(1 n)σ(ξ)η(x) + η(x)p(ξ) p(x).

On weakly symmetric Kenmotsu manifolds 207 Now taking X = ξ in (3.6) we have (3.8) 0 = (1 n)α(ξ)η(v ) +(1 n)γ(ξ)η(v ) + (1 n)σ(v ) + p(v ) η(v )p(ξ). Replacing V with X in (3.8) and summing with (3.7), in view of (3.5), we find (3.9) (1 n)α(x) + η(x)β(ξ) β(x) + (1 n)γ(ξ)η(x) + (1 n)σ(x) = 0. Now putting X = ξ in (3.4) we have (3.10) (1 n)α(ξ)η(z) + β(z) η(z)β(ξ) + (1 n)γ(z) + (1 n)σ(ξ)η(z) = 0. Replacing Z with X in (3.10) and taking the summation with (3.9), we have 0 = (1 n)η(x) [α(ξ) + σ(ξ) + γ(ξ)] +(1 n) [α(x) + σ(x) + γ(x)]. So in view of (3.5) we obtain α(x) + σ(x) + γ(x) for all X on M. This completes the proof of the theorem. Theorem 3.2 There is no weakly Ricci-symmetric Kenmotsu manifold M, n > 3, unless ρ + µ + υ is everywhere zero. Proof. Suppose that M is a weakly Ricci-symmetric Kenmotsu manifold. Replacing Z with ξ in (1.2) and using (2.8) we have (3.11) ( X S)(Y, ξ) = (1 n)ρ(x)η(y ) + (1 n)µ(y )η(x) + υ(ξ)s(x, Y ). So in view of (3.11) and (3.2) we obtain (3.12) (1 n)g(x, Y ) S(X, Y ) = (1 n)ρ(x)η(y ) + (1 n)µ(y )η(x) + υ(ξ)s(x, Y ). Taking X = Y = ξ in (3.12) and by the use of (2.8), (2.1) and (2.2) we get which gives (since n > 3) (1 n) (ρ(ξ) + µ(ξ) + υ(ξ)) = 0, (3.13) ρ(ξ) + µ(ξ) + υ(ξ) = 0. Now putting X = ξ in (3.12) we have (1 n)η(y ) [ρ(ξ) + υ(ξ)] + (1 n)µ(y ) = 0. So by virtue of (3.13) this yields (1 n) [ µ(ξ)η(y ) + µ(y )] = 0,

208 C ihan Özgür which gives us (since n > 3) (3.14) µ(y ) = µ(ξ)η(y ). Similarly taking Y = ξ in (3.12) we also have ρ(x) + η(x) [µ(ξ) + υ(ξ)] = 0, hence applying (3.13) into the last equation we find (3.15) ρ(x) = ρ(ξ)η(x). Since ( ξ S)(ξ, X) = 0, then from (1.2) we obtain η(x) [ρ(ξ) + µ(ξ)] + υ(x) = 0. So by making use of (3.13) the last equation reduces to (3.16) υ(x) = υ(ξ)η(x). Therefore changing Y with X in (3.14) and by the summation of the equations (3.14), (3.15) and (3.16) we obtain ρ(x) + µ(x) + υ(x) = (ρ(ξ) + µ(ξ) + υ(ξ)) η(x) and so in view of (3.13) it follows that ρ(x) + µ(x) + υ(x) = 0, for all X, which implies ρ + µ + υ = 0 on M. Our theorem is thus proved. References [1] D. E. Blair, Contact Manifolds in Riemannian Geometry, Lecture Notes in Mathematics 509, Springer-Verlag, Berlin, 1976. [2] M. C. Chaki, On pseudo symmetric manifolds, An. Stiint. Univ. Al. I. Cuza Iasi Sect. I a Mat. 33 (1987), 1, 53 58. [3] M. C. Chaki, On pseudo Ricci symmetric manifolds, Bulgar. J. Phys. 15, 6 (1988), 526 531. [4] U. C. De and S. Bandyopadhyay, On weakly symmetric spaces, Publ. Math. Debrecen 54 (1999), 377-381. [5] U. C. De, T. Q. Binh and A. A. Shaikh, On weakly symmetric and weakly Ricci-symmetric K-contact manifolds, Acta Mathematica Academiae Paedagogicae Nyíregyháziensis 16 (2000), 65-71. [6] K. Kenmotsu, A class of contact Riemannian manifold, Tohoku Math. Jour. 24 (1972), 93-103.

On weakly symmetric Kenmotsu manifolds 209 [7] C. Özgür, On weak symmetries of Lorentzian para-sasakian manifolds, Radovi Matematicki, 11 (2002/03), 263-270. [8] L. Tamássy and T. Q. Binh, On weakly symmetric and weakly projective symmetric Riemannian manifolds, Coll. Math. Soc. J. Bolyai 56 (1992), 663-670. [9] L. Tamássy and T. Q. Binh, On weak symmetries of Einstein and Sasakian manifolds, Tensor, N. S. 53 (1993), 140-148. Author s address: Cihan Özgür Balikesir University, Department of Mathematics, Faculty of Arts and Sciences, Campus of Çağiş, 10145, Balikesir, Turkey e-mail: cozgur@balikesir.edu.tr