EUROPEAN JOURNAL OF PURE AND APPLIED MATHEMATICS Vol. 1, No. 2, 2008, (21-31) ISSN 1307-5543 – www.ejpam.com Some results on K-contact and Trans-Sasakian Manifolds Bagewadi Channabasappa1,∗, Basavarajappa N.S2, Prakasha D.G 1, and Venkatesha1 1 Department of Mathematics and Computer Science, Kuvempu University, Jnana Sahyadri-577 451, Shimoga, Karnataka, INDIA. 2 Department of Mathematics, SBM Jain College of Engineering, 562 112, Jakkasandra BAN- GALORE. Abstract. We obtain results on the vanishing of divergence of Pseudo projective curvature tensor P̃ with respect to semi-symmetric metric connection on k-contact and trans-Sasakian manifolds. AMS subject classifications: 53D15,53B15. Key words: k-contact manifold, Trans-Sasakian manifold, Pseudo projective curvature tensor, η-Einstein manifold. 1. Introduction In 1924, Friedman and Schouten [11] introduced the notion of semi-symmetric lin- ear connection on a differentiable manifold. Then in 1932, Hayden [14] introduced the idea of metric connection with a torsion on a Riemannain manifold. A systematic study of semi-symmetric metric connection on a Riemannain manifold has been given by Yano [18] in 1970 and later studied by K.S.Amur and S.S.Pujar [1], C.S.Bagewadi [2], U.C.De et al [10], Sharafuddin and Hussain [16] and others. The authors U.C.De [10] and C.S.Bagewadi et al [ [3, 12]] have obtained results on the conservativeness of Pro- jective, Pseudo projective, Conformal, Concircular, Quasi conformal curvature tensors on k-contact, Kenmotsu and trans-sasakian manifolds. In this paper we extend the conservativeness of Pseudo projective curvature tensor to k-contact and trans-Sasakian manifolds admitting semi-symmetric metric connection. After preliminaries in section 2, we study in section 3 the Pseudo projective curvature tensor with respect to semi-symmetric metric connection on k-contact manifold. In the section 4 we study some properties regarding Pseudo projective curvature tensor with respect to this connection on trans-Sasakian manifold under the condition φ(gradα) = (n− 2)gradβ and obtained some interesting results. ∗Corresponding author. Email addresses: prof bagewadi@yahoo.co.in (Bagewadi Channabasappa), nsb sbmjce@yahoo.co.in (Basavarajappa N.S) http://www.ejpam.com 21 c© 2007 EJPAM All rights reserved. Bagewadi C.S. et al. / Eur. J. Pure Appl. Math, 1 (2008), (21-31) 22 2. Preliminaries Let Mn be an almost contact metric manifold [9] with an almost contact metric struc- ture (φ, ξ, η, g), that is, φ is a (1, 1) tensor field, ξ is a vector field; η is a 1-form and g is a compatible Riemannian metric such that φ2 = −I + η ⊗ ξ, η(ξ) = 1, φ(ξ) = 0, η.φ = 0, (2.1) g(φX, φY ) = g(X,Y )− η(X)η(Y ), (2.2) g(X,φY ) = −g(φX, Y ), g(X, ξ) = η(X), (2.3) for all X,Y ∈ TM . If Mn is a k-contact Riemannian manifold, then besides (2.1), (2.2) and (2.9 ) the following relations hold [15]: ∇Xξ = −φX, (2.4) (∇Xη)(Y ) = −g(φX, Y ), (2.5) S(X, ξ) = (n− 1)η(X), (2.6) η(R(X,Y )Z) = g(Y,Z)η(X)− g(X,Z)η(Y ), (2.7) for any vector fields X, Y , where R and S denote respectively the curvature tensor of type (1, 3) and the Ricci tensor of type (0, 2). An almost contact metric structure (φ, ξ, η, g) in M is called trans-Sasakian structure [14] if (M × R, J,G) belongs to the class w4 [ [8], [13]] where J is the almost complex structure on M ×R defined by J(X,λd/dt) = (φX − λξ, η(X)d/dt) for all vector fields X on M and smooth functions λ on M ×R and G is the product metric on M ×R. This may be expressed by the condition [8] (∇Xφ)Y = α(g(X,Y )ξ − η(Y )X) + β(g(φX, Y )ξ − η(Y )φX) (2.8) for some smooth functions functions α and β on M , and we say that the trans-Sasakian structure is of type (α, β). Let M be a n-dimensional trans-Sasakian manifold. From (2.8)it is easy to see that ∇Xξ = −αφX + β(X − η(X)ξ), (2.9) (∇Xη)Y = −αg(φX, Y ) + βg(φX, φY ). (2.10) In a n-dimensional trans-Sasakian manifold, we have R(ξ,X)ξ = (α2 − β2 − ξβ)(η(X)ξ −X), (2.11) 2αβ + ξα = 0, (2.12) S(X, ξ) = ((n− 1)(α2 − β2)− ξβ)η(X)− (n− 2)Xβ − (φX)α. (2.13) If in a n-dimensional trans Sasakian manifold of type(α, β), we have [4] φ(gradα) = (n− 2)gradβ, (2.14) Bagewadi C.S. et al. / Eur. J. Pure Appl. Math, 1 (2008), (21-31) 23 then (2.11) and (2.13) reduces to R(ξ,X)ξ = (α2 − β2)(η(X)ξ −X), (2.15) S(X, ξ) = (n− 1)(α2 − β2)η(X). (2.16) In this paper we study trans Sasakian manifold under the condition (2.14). Let (Mn, g) be an n-dimensional Riemannian manifold of class C∞ with metric tensor g and let ∇ be the Levi-Civita connection on Mn. A linear connection ∇̃ on (Mn, g) is said to be semi symmetric [16] if the torsion tensor T of the connection ∇̃ satisfies T (X,Y ) = π(Y )X − π(X)Y, (2.17) where π is a 1-form on Mn with ρ as associated vector field, i.e., π(X) = g(X, ρ) for any differentiable vector field X on Mn. A semi-symmetric connection ∇̃ is called semi-symmetric metric connection [5] if it further satisfies ∇̃g = 0. In an almost contact manifold semi-symmetric metric connection is defined by identi- fying the 1-form π of (2.17) with the contact-form η, i.e., by setting [16] T (X,Y ) = η(Y )X − η(X)Y (2.18) with ξ as associated vector field. i.e., g(X, ξ) = η(X). The relation between the semi-symmetric metric connection ∇̃ and the Levi-Civita connection ∇ of (Mn, g) has been obtained by K.Yano [18], which is given by ∇̃XY = ∇XY + η(Y )X − g(X,Y )ξ, (2.19) where η(Y ) = g(Y, ξ). Further, a relation between the curvature tensor R and R̃ of type (1, 3) of the connec- tions ∇ and ∇̃ respectively is given by [18]. R̃(X,Y )Z = R(X,Y )Z −K(Y,Z)X +K(X,Z)Y − g(Y, Z)FX + g(X,Z)FY. (2.20) where K is a tensor field of type (0, 2) defined by K(Y, Z) = g(FY,Z) = (∇Y η)(Z)− η(Y )η(Z) + 1 2 η(ξ)g(Y,Z), (2.21) for any vector fields X and Y . From (2.20), it follows that S̃(Y,Z) = S(Y, Z)− (n− 2)K(Y,Z)− a.g(Y, Z) (2.22) where S̃ denotes the Ricci tensor with respect to ∇̃ and a = Tr.K. Differentiating (2.22) covariantly with respect to X, we obtain [6] (∇̃X S̃)(Y,Z) = (∇XS)(Y,Z)− (n− 2)(∇XK)(Y, Z)− η(Y )S(X,Z)− η(Z)S(X,Y ) +(n− 2)η(Y )K(X,Z) + (n− 2)η(Z)K(Y,X) + g(X,Y )S(ξ, Z) +g(X,Z)S(Y, ξ)− (n− 2)g(X,Z)K(Y, ξ)− (n− 2)g(X,Y )K(Z, ξ)(2.23) Bagewadi C.S. et al. / Eur. J. Pure Appl. Math, 1 (2008), (21-31) 24 Now let ei be an orthogonal basis of the tangent space at each point of the manifold Mn for i = 1, 2, ...., n. Putting Y = Z = ei in (2.23 ) and then taking summation over the index i, we get ∇̃X r̃ = ∇Xr − (n− 2)(∇Xa) (2.24) Further, since ξ is a killing vector in k-contact manifold. S, α, r, and a are invariant under it, i.e., LξS = 0, Lξr = 0 (2.25) LξK = 0, Lξa = 0 (2.26) We recall some definitions which are used in later section, A Riemannian manifold is said to be η-Einstein manifold if the Ricci tensor S is of the form S(X,Y ) = λg(X,Y ) + µη(X)η(Y ) where λ, µ are the associated functions on the manifold. A Riemannian manifold is said to be cyclic-Ricci tensor, if the Ricci tensor S satisfies the condition (∇XS)(Y, Z) + (∇Y S)(Z,X) + (∇ZS)(X,Y ) = 0 3. k-contact Manifold Admitting a Semi-symmetric Metric Connection With Div.P̃ = 0 The pseudo projective curvature tensor on a Riemannian manifold is given by ( [7], [17]) P̃ (X,Y )Z = aR(X,Y )Z + b(S(Y,Z)X − S(X,Z)Y ] r n [ a n− 1 + b ] [g(Y,Z)X − g(X,Z)Y ]. (3.1) In this section we prove the following: If a k-contact manifold Mn (n > 2) admits a semi- symmetric metric connection and if the Pseudo projective curvature tensor with respect to this connection is conservative, then the manifold is η-Einstein; the scalar curvature of such a manifold is given by (3.14). Proof. : Let us suppose that in a k-contact ManifoldMn with respect to semi-symmetric metric connection Div.C = 0 where Div denotes the divergence. Differentiate (3.1) covariantly and then contracting we get Div.P̃ . By virtue of conserva- Bagewadi C.S. et al. / Eur. J. Pure Appl. Math, 1 (2008), (21-31) 25 tiveness of P̃ i.e.,div.P̃ = 0, we obtain (a+ b)[(∇XS)(Y,Z)− (∇Y S)(X,Z)]− [a+ b(n− 2)][(∇XK)(Y,Z)− (∇YK)(X,Z)] = (a− b)[S(Y,Z)η(X)− S(X,Z)η(Y )]− a(n− 1)η(R(X,Y )Z) + a.S(X,Y )η(Z) +a(n−A− 1)[g(Y, Z)η(X)− g(X,Z)η(Y )] + b[g(Y, Z)S(X, ξ)− g(X,Z)S(Y, ξ)](3.2) +(a+ b(n− 2))[K(X,Y )η(Z)−K(X,Z)η(Y ) +K(Y,X)η(Z)−K(Y,Z)η(X)] −b(n− 2)[g(Y, Z)K(X, ξ) + g(X,Z)K(Y, ξ)] + 1 n [ a+ (n− 1) (n− 1) ] [g(Y,Z)∇Xr −g(X,Z)∇Y r] + [ a+ 1 n a+ (n− 1) (n− 1) ] [g(Y,Z)∇XA− g(X,Z)∇YA]. By virtue of (2.1) and (2.4) we obtain from (2.21) that K(X,Y ) = g(X,φY )− η(X)η(Y ) + 1 2 g(X,Y ). (3.3) K(X, ξ) = −1 2 η(X) (3.4) LX = −φX − η(X)ξ + 1 2 X. (3.5) Now putting X = ξ in (3.2), then using (2.1), (2.6),(2.7),(3.3) and (3.4), we get (a+ b)[(∇ξS)(Y,Z)− (∇Y S)(ξ, Z)]− [a+ n(n− 2)][(∇ξK)(Y,Z)− (∇YK)(ξ, Z)] = [a+ n(n− 2)])g(φY,Z) + (a− b)S(Y,Z) + [ a ( A+ 1 2 ) + b(2n− 3) ] g(Y,Z) − [ a ( A+ 1 2 ) + b(n− 2) ] η(Y )η(Z) + 1 n [ a+ (n− 1) (n− 1) ] [g(Y, Z)∇ξr − η(Z)∇Y r](3.6) + [ a+ 1 n a+ (n− 1) (n− 1) ] [g(Y,Z)∇ξA− η(Z)∇YA]. From (2.25) and (2.26), we obtain (∇ξS)(Y,Z) = −S(∇Y ξ, Z)− S(Y,∇Zξ), (∇ξr) = 0, (3.7) (∇ξK)(Y,Z) = −K(∇Y ξ, Z)−K(Y,∇Zξ), (∇ξa) = 0, (3.8) respectively. By using(3.7)and(3.8) in (3.6), we have (a+ b)[−S(∇Y ξ, Z)− S(Y,∇Zξ)− (∇Y S)(ξ, Z)] = [a+ n(n− 2)][−K(∇Y ξ, Z)−K(Y,∇Zξ)− (∇YK)(ξ, Z)] +[a+ n(n− 2)])g(φY,Z) + (a− b)S(Y, Z) + [ a ( A+ 1 2 ) + b(2n− 3) ] g(Y,Z) − [ a ( A+ 1 2 ) + b(n− 2) ] η(Y )η(Z) + 1 n [ a+ (n− 1) (n− 1) ] [g(Y,Z)∇ξr − η(Z)∇Y r](3.9) + [ a+ 1 n a+ (n− 1) (n− 1) ] [g(Y,Z)∇ξA− η(Z)∇YA]. Bagewadi C.S. et al. / Eur. J. Pure Appl. Math, 1 (2008), (21-31) 26 Using (2.4) ,(2.6) and (3.4) in (3.9), we get −(a+ b)S(φY,Z)− (a− b)S(Y,Z) = [ a ( A+ 3 2 ) + b(3n− 5) ] g(Y,Z)− [ a ( A+ 3 2 ) − 2b(n− 2) ] η(Y )η(Z) +[a(n+ 1) + b(3n− 5)]g(φY,Z)− 1 n [ a+ (n− 1) (n− 1) ] η(Z)∇Y r − [ a+ 1 n a+ (n− 1) (n− 1) ] η(Z)∇YA. (3.10) Next, by replacing Z by φZ in above and then using (2.1), we obtain −(a+ b)S(φY, φZ)− (a− b)S(Y, φZ)[ a ( A+ 3 2 ) + b(3n− 5) ] g(Y, φZ) + [a(n+ 1) + b(3n− 5)] g(φY, φZ) (3.11) Interchanging Y and Z in (3.11), we have −(a+ b)S(φY, φZ)− (a− b)S(φY,Z)[ a ( A+ 3 2 ) + b(3n− 5) ] g(φY,Z) + [a(n+ 1) + b(3n− 5)] g(φY, φZ) (3.12) By adding (3.11) with (3.12), and then by using the skew-symmetric property of φ, one can get S(Y,Z) = P1.g(Y, Z) +Q1.η(Y )η(Z) (3.13) whereP1 = [ − a a+ b (n− 1)− b a+ b (3n− 5) ] and Q1 = [ 2a+ b a+ b (n− 1) + b a+ b (3n− 5) ] . There fore the manifold is η-Einstein. Let ei be an orthogonal basis of the tangent space at each point of the manifold Mn for i = 1, 2, ...., n. Putting Y = Z = ei in (3.13) and then taking summation over the index i, we get r = −(n− 1)(n− 2) (a+ 3b) (a+ b) . (3.14) This proves the theorem. Suppose in k-contact manifold admitting a semi-symmetric metric connection, the Pseudo projective curvature tensor with respect to this connection is conservative. Then the manifold has a cyclic-Ricci tensor with respect to Levi-Civita connection; and moreover the scalar curvature of the manifold is constant if and only if the vector field ξ is harmonic provided (a+ b) 6= 0. Bagewadi C.S. et al. / Eur. J. Pure Appl. Math, 1 (2008), (21-31) 27 Proof. Differentiating (3.13) covariantly with respect to X, we have (∇XS)(Y,Z) = [ 2a+ b a+ b (n− 1) + b a+ b (3n− 5) ] [g(φY,X)η(Z) + g(φX,Z)η(Y )] (3.15) Similarly (∇Y S)(Z,X) = [ 2a+ b a+ b (n− 1) + b a+ b (3n− 5) ] [g(φY,Z)η(X) + g(φX, Y )η(Z)](3.16) (∇ZS)(X,Y ) = [ 2a+ b a+ b (n− 1) + b a+ b (3n− 5) ] [g(φX,Z)η(Y ) + g(φZ, Y )η(X)].(3.17) Adding the equations (3.15), (3.16) and (3.17), then using skew-symmetry of φ, we obtain (∇XS)(Y, Z) + (∇Y S)(Z,X) + (∇ZS)(X,Y ) = 0 (3.18) Thus the manifold has a cyclic-Ricci tensor. Taking an orthonormal frame field and contracting (3.15) over X and Z, we obtain dr(Y ) = [ 2a+ b a+ b (n− 1) + b a+ b (3n− 5) ] ψη(Y ) (3.19) where ψ = Tr.φ. From (3.19), it follows that dr(Y ) = 0 if and only ψ = 0 provided (a+ b) 6= 0. (3.20) 4. Trans-Sasakian Manifold Admitting a Semi-symmetric Metric Connection With Div.P̃ = 0 Here we recall some results which will be used in further. [5]: In a trans-Sasakian manifold under the condition (2.14), we have [(∇ξS)(Y,Z)− (∇Y S)(ξ, Z)] = βS(Y, Z)− (n− 1)(α2 − β2)βg(Y, Z) (4.1) −(n− 1)(α2 − β2)αg(Y, φZ) + αS(Y, φZ). [5]: For trans-Sasakian manifold under the condition (2.14), the following results are Bagewadi C.S. et al. / Eur. J. Pure Appl. Math, 1 (2008), (21-31) 28 true (i) K(Y,Z) = αg(Y, φZ) + ( β + 1 2 ) g(Y, Z)− (β + 1)η(Y )η(Z) (ii) K(Y, ξ) = K(ξ, Y ) = −1 2 η(Y ) (iii) K(∇Y ξ, Z) = −α2[g(Y,Z)− η(Y )η(Z)]− 2αβg(φY,Z) −α 2 g(φY,Z) + β ( β + 1 2 ) [g(Y,Z)− η(Y )η(Z)] (4.2) (iv) K(Y,∇Zξ) = α2[g(Y,Z)− η(Y )η(Z)] + α 2 g(φY,Z) +β ( β + 1 2 ) [g(Y,Z)− η(Y )η(Z)]. [5]: In a trans-Sasakian manifold under the condition (2.14), we have [(∇ξK)(Y,Z)− (∇YK)(ξ, Z)] = αg(Y, φZ)− 2αβg(φY,Z) −[(α2 − β2)− (2β + 1)][g(Y, Z)− η(Y )η(Z)].(4.3) In this section we prove the following: Let in a trans-Sasakian manifoldMn (n > 2) under the condition (2.14) admits a semi-symmetric metric connection the Pseudo projective curvature tensor with respect to this connection is conservative. Then the manifold Mn is η-Einstein with respect to Levi-Civita connection; the scalar curvature of such a manifold is given by (4). Proof. Let us suppose that in a trans-Sasakian Manifold Mn under the condition (2.14)with respect to semi-symmetric metric connection Div.P̃ = 0. Putting X = ξ in (3.2) then using (2.1),(2.3), (2.16) and (4.2(ii)) we get (a+ b)[(∇ξS)(Y, Z)− (∇Y S)(ξ, Z)]− (a+ b(n− 2))[(∇ξK)(Y,Z)− (∇YK)(ξ, Z)] = (a− b)S(Y,Z) + (a+ b(n− 2))αg(Y, φZ)− a(n− 1)η(R(ξ, Y )Z) + [ (a+ b(n− 2)) ( β + 1 2 ) + a(n−A− 1) + b(n− 1)(α2 − β2) + b 2 (n− 2) ] g(Y,Z) − [ a(n−A− 1) + (a+ b(n− 2)) ( β + 1 2 ) + b 2 (n− 2) ] η(Y )η(Z) (4.4) + [ 1 n a+ (n− 1) (n− 1) (n− 2)− a ] [η(Z)∇YA− g(Y,Z)∇ξA] − 1 n [ a+ (n− 1) (n− 1) ] [η(Z)∇Y r − g(Y, Z)∇ξr]. Bagewadi C.S. et al. / Eur. J. Pure Appl. Math, 1 (2008), (21-31) 29 Using (2.15) ,(4.1), (4.2(i)) and (4.3) in above, we get (a+ b)(β − 1)S(Y,Z) + (a+ b)αS(Y, φZ) = −[2α(β + 1)(a+ b(n− 2)) + (a+ b)(n− 1)(α2 − β2)α]g(φY,Z) +P̀ .g(Y,Z) + Q̀.η(Y )η(Z) + [ 1 n a+ (n− 1) (n− 1) (n− 2)− a ] [η(Z)∇YA− g(Y,Z)∇ξA] (4.5) − 1 n [ a+ (n− 1) (n− 1) ] [η(Z)∇Y r − g(Y, Z)∇ξr]. where P̀ = [a(β − 1) + b(β + 1)](n− 1)(α2 − β2) + a(n−A− 1) + b 2 (n− 2) + [a+ b(n− 2)] [ 2 ( β + 1 4 ) − (α2 − β2) ] and Q̀ = [(a− b)(α2 − β2)− b](n− 2)− a ( n−A− 1 2 ) . Next, by replacing Z by φZ in (4.5) and then using (2.1), we obtain −(a+ b)αS(Y,Z)− (a+ b)(β − 1)S(φY,Z) = −[2α(β + 1)[a+ b(n− 2) + (a+ b)(n− 1)(α2 − β2)α]g(Y,Z) −P̀ .g(Y, φZ) + [2α(β + 1)(a+ b(n− 2))]η(Y )η(Z) (4.6) + [ 1 n a+ (n− 1) (n− 1) (n− 2)− a ] g(Y, φZ)∇ξA− 1 n [ a+ (n− 1) (n− 1) ] g(Y, φZ)∇ξr. Interchanging Y and Z in above, we have −(a+ b)αS(Y,Z)− (a+ b)(β − 1)S(Y, φZ) = −[2α(β + 1)[a+ b(n− 2) + (a+ b)(n− 1)(α2 − β2)α]g(Y,Z) −P̀ .g(φY,Z) + [2α(β + 1)(a+ b(n− 2))]η(Y )η(Z) (4.7) + [ 1 n a+ (n− 1) (n− 1) (n− 2)− a ] g(φY,Z)∇ξA− 1 n [ a+ (n− 1) (n− 1) ] g(φY,Z)∇ξr. By adding (4.6) and (4.7), then by using skew-symmetric property of φ, one can obtain S(Y,Z) = P2.g(Y, Z) +Q2.η(Y )η(Z). (4.8) where P2 = [ 2 (β + 1) (a+ b) [a+ b(n− 2)] + (n− 1)(α2 − β2) ] and Q2 = −2 (β + 1) (a+ b) [a+ b(n− 2)]. REFERENCES 30 Therefore the manifold is η-Einstein. Let ei be an orthogonal basis of the tangent space at each point of the manifold Mn for i = 1, 2, ...., n. Putting Y = Z = ei in (4.8) and then taking summation over the index i, we get r = (n− 1) [ 2 (β + 1) (a+ b) [a+ b(n− 2)] + n(α2 − β2) ] . This proves the theorem. 5. Acknowledgment The authors are grateful to the referrers and Eyüp Çetin for their valuable suggestions in the improvement of the paper . 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