ON M-Projectively Flat LP-Sasakian Manifolds

In the present paper, we study the nature of LP-Sasakian manifolds admitting the M-projective curvature tensor. It is examined whether this manifold satisfies the condition W(X, Y ).R = 0. Moreover, it is proved that, in the M-projectively flat LP-Sasakian manifolds, the conditions R(X, Y ).R = 0 an...

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Автори: Zengin, F. Ö., Зенгін, F. О.
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Мова:Англійська
Опубліковано: Institute of Mathematics, NAS of Ukraine 2013
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Ukrains’kyi Matematychnyi Zhurnal
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author Zengin, F. Ö.
Зенгін, F. О.
author_facet Zengin, F. Ö.
Зенгін, F. О.
author_sort Zengin, F. Ö.
baseUrl_str https://umj.imath.kiev.ua/index.php/umj/oai
collection OJS
datestamp_date 2020-03-18T19:25:49Z
description In the present paper, we study the nature of LP-Sasakian manifolds admitting the M-projective curvature tensor. It is examined whether this manifold satisfies the condition W(X, Y ).R = 0. Moreover, it is proved that, in the M-projectively flat LP-Sasakian manifolds, the conditions R(X, Y ).R = 0 and R(X, Y ).S = 0 are satisfied. In the last part of the paper, an M-projectively flat space-time is introduced, and some properties of this space are obtained.
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fulltext UDC 517.91 F. Ö. Zengin (Istanbul Techn. Univ., Turkey) ON M -PROJECTIVELY FLAT LP-SASAKIAN MANIFOLDS ПРО M -ПРОЕКТИВНО ПЛОСКI LP-МНОГОВИДИ САСАКЯНА The object of the present paper is to study the nature of LP-Sasakian manifolds admitting the M -projective curvature tensor. It is examined whether this manifold satisfies the condition W (X,Y ).R = 0. Moreover, it is proved that, in the M -projectively flat LP-Sasakian manifolds, the conditions R(X,Y ).R = 0 and R(X,Y ).S = 0 are satisfied. In the last part of our paper, M -projectively flat space-time is introduced and some properties of this space are obtained. Вивчається природа многовидiв Сасакяна, що допускають M -проективний тензор кривизни. Перевiрено, чи задо- вольняє цей многовид умовуW (X,Y ).R = 0. Бiльш того, доведено, що умовиR(X,Y ).R = 0 таR(X,Y ).S = 0 ви- конуються для M -проективно плоских LP-многовидiв Сасакяна. В останнiй частинi роботи введено M -проективно плоский простiр-час та встановлено деякi властивостi цього простору. 1. Introduction. A Riemannian manifold (M, g) is called a Sasakian manifold if there exists a Killing vector field ξ of unit length on M so that tensor field Φ of type (1,1), defined by Φ(X) = = −∇Xξ, satisfies the condition (∇XΦ)(Y ) = g(X,Y )ξ − g(ξ, Y )X for any pair of vector fields X and Y on M. This is a curvature condition which can be easily expressed in terms the Riemann curvature tensor as R(X, ξ)Y = g(ξ, Y )X − g(X,Y )ξ. Equivalently, the Riemannian cone defined by (C(M), ḡ,Ω) = (R+XM, dr2 + r2g, d(r2η)) is Kähler with the Kähler form Ω = d(r2η), where η is the dual 1-form of ξ. The 4-tuple s = (ξ, η,Φ, g) is commonly called a Sasakian structure on M and ξ is its characteristic or Reeb vector field. Sasakian geometry is a special kind of contact metric geometry such that the structure transverse to the Reeb vector field ξ is Kähler and invariant under the flow of ξ. On the analogy of Sasakian manifolds, in 1989 Matsumoto [1, 2], introduced the notion of LP-Sasakian manifolds. Again the same notion is introduced by Mihai and Rosca [3] and obtained many interesting results. LP-Sasakian manifolds are also studied by De et al. [4], Shaikh et al. [5 – 8], Taleshian and Asghari [9], Venkatesha and Bagewadi [10] and many others. The M -projective curvature tensor of a Riemannian manifold M defined by Pokhariyal and Mishra [11] is in the following form: W (X,Y )Z = R(X,Y )Z − 1 2(n− 1) ( S(Y,Z)X − S(X,Z)Y + g(Y, Z)QX − g(X,Z)QY ) , (1.1) where R(X,Y )Z and S(X,Y ) are the curvature tensor and the Ricci tensor of M, respectively and Q is the Ricci operator defined by S(X,Y ) = g(QX,Y ). Some properties of this tensor in Sasakian and Kähler manifolds have been studied before [12, 13]. In 2010, Chaubey and Ojha [14] investigated the M -projective curvature tensor of a Kenmotsu manifold. The object of the present paper is to study LP-Sasakian manifolds admitting M -projective curva- ture tensor. The paper is organized as follows. Section 2 is concerned with some preliminaries about LP-Sasakian manifolds. Section 3 deals with LP-Sasakian manifolds withM -projective curvature ten- sor. Section 4 is devoted to M -projectively flat LP-Sasakian manifolds. In Section 5, M -projectively flat LP-Sasakian spacetimes are introduced. c© F. Ö. ZENGİN, 2013 1560 ISSN 1027-3190. Укр. мат. журн., 2013, т. 65, № 11 ON M -PROJECTIVELY FLAT LP-SASAKIAN MANIFOLDS 1561 2. Preliminaries. An n-dimensional differentiable manifold M is called an LP-Sasakian man- ifold [1, 2] if it admits a (1, 1) tensor field ϕ, a contravariant vector field ξ, a 1-form η and a Lorentzian metric g which satisfy: ϕ2 = I + η ⊗ ξ, (2.1) η(ξ) = −1, (2.2) g(ϕX,ϕY ) = g(X,Y ) + η(X)η(Y ), (2.3) ∇Xξ = ϕX, g(X, ξ) = η(X), (2.4) (∇Xϕ)Y = g(X,Y )ξ + 2η(X)η(Y )ξ, (2.5) where ∇ denotes the operator of the covariant differentiation with respect to the Lorentzian metric g. It can be easily seen that in an LP-Sasakian manifold, the following relations hold: ϕξ = 0, η(ϕX) = 0, rankϕ = n− 1. Again if we put Ω(X,Y ) = g(X,ϕY ) for any vector fields X and Y, then Ω(X,Y ) is symmetric (0, 2) tensor field [1]. Also since the 1-form η is closed in an LP-Sasakian manifold, we have [1, 4] (∇Xη)(Y ) = Ω(X,Y ), Ω(X, ξ) = 0 for any vector fields X and Y. Also, in an LP-Sasakian manifold, the following conditions hold [2, 4]: g(R(X,Y )Z, ξ) = η(R(X,Y )Z) = g(Y,Z)η(X)− g(X,Z)η(Y ), (2.6) R(ξ,X)Y = g(X,Y )ξ − η(Y )X, (2.7) R(X,Y )ξ = η(Y )X − η(X)Y, (2.8) R(ξ,X)ξ = X + η(X)ξ, (2.9) S(X, ξ) = (n− 1)η(X), (2.10) S(ϕX,ϕY ) = S(X,Y ) + (n− 1)η(X)η(Y ) (2.11) for any vector fields X, Y, Z where R(X,Y )Z is the curvature tensor and S(X,Y ) is the Ricci tensor. ISSN 1027-3190. Укр. мат. журн., 2013, т. 65, № 11 1562 F. Ö. ZENGİN 3. LP-Sasakian manifold satisfying W (X,Y ).S = 0. Let us consider an LP-Sasakian mani- fold (M, g) satisfying the condition W (X,Y ).S = 0. (3.1) Now, we have S(W (ξ,X)Y,Z) + S(Y,W (ξ,X)Z) = 0. (3.2) From (1.1), (2.7) and (2.10), we get W (ξ,X)Y = 1 2 g(X,Y )ξ − 1 2 η(Y )X − 1 2(n− 1) S(X,Y )ξ + 1 2(n− 1) η(Y )QX. (3.3) By using (2.10) and (3.3), (3.2) takes the form 1 2 (n− 1)g(X,Y )η(Z) + 1 2 (n− 1)g(X,Z)η(Y )− S(X,Z)η(Y )− −S(X,Y )η(Z) + 1 2(n− 1) S(QX,Z)η(Y ) + 1 2(n− 1) S(QX,Y )η(Z) = 0. (3.4) Let λ be the eigenvalue of the endomorphism Q corresponding to an eigenvector X. Then QX = λX. (3.5) By using (3.5) in (3.4), we obtain 1 2 (n− 1)g(X,Y )η(Z) + 1 2 (n− 1)g(X,Z)η(Y )− S(X,Z)η(Y )− −S(X,Y )η(Z) + λ 2(n− 1) S(X,Z)η(Y ) + λ 2(n− 1) S(X,Y )η(Z) = 0. (3.6) Remembering that g(QX,Y ) = S(X,Y ) and using (3.6), we have g(QX,Y ) = g(λX, Y ) = λg(X,Y ) = S(X,Y ). (3.7) Thus, from (3.6) and (3.7), taking Z = ξ in (3.6) and using (2.2), it can be easily seen that( λ2 2(n− 1) − λ+ n− 1 2 ) (g(X,Y )− η(X)η(Y )) = 0. (3.8) Finally, taking Y = ξ in (3.8) and using the properties (2.2) and (2.4)2, we obtain( λ2 2(n− 1) − λ+ n− 1 2 ) η(X) = 0. (3.9) In this case, as η(X) 6= 0, we have from (3.9) λ2 − 2(n− 1)λ+ (n− 1)2 = 0. (3.10) From (3.10), it follows that the non-zero eigenvalues of the endomorphism Q are congruent such as (n− 1). Thus we can state the following theorem. ISSN 1027-3190. Укр. мат. журн., 2013, т. 65, № 11 ON M -PROJECTIVELY FLAT LP-SASAKIAN MANIFOLDS 1563 Theorem 3.1. If an n-dimensional (n ≥ 3) LP-Sasakian manifold admitting M -projective cur- vature tensor and with non-zero Ricci tensor S satisfies W (X,Y ).S = 0, then the non-zero eigenvalues of the symmetric endomorphism Q of the tangent space corresponding to S are congruent such as (n− 1). 4. M -projectively flat LP-sasakian manifolds. Let us consider that M be an M -projectively flat LP-Sasakian manifold. Thus, we have W (X,Y )Z = 0 for all vector fields X, Y, Z. Then, we get from (1.1) R(X,Y )Z = 1 2(n− 1) ( S(Y, Z)X − S(X,Z)Y + g(Y,Z)QX − g(X,Z)QY ) . (4.1) Taking Z = ξ in (4.1) and using the relations (2.4), (2.8) and (2.10), we find η(Y )X − η(X)Y = 1 n− 1 [ η(Y )QX − η(X)QY ] . (4.2) Again taking Y = ξ in (4.2) and applying (2.2), (4.2) reduces to QX = (n− 1)X. (4.3) Hence in view of (2.7), (4.1) and (4.3), we get S(X,Y )ξ = (n− 1)g(X,Y )ξ. (4.4) Taking the inner product of both sides (4.4) with ξ and using (2.2), we have S(X,Y ) = (n− 1)g(X,Y ). (4.5) Next, we have the following theorem. Theorem 4.1. Let M be an n-dimensional M -projectively flat LP-Sasakian manifold. Then M is an Einstein manifold and the Ricci tensor of M is in the form S(X,Y ) = (n− 1)g(X,Y ). In this case, by the use of (4.3) and (4.5) in (4.1), we obtain R(X,Y )Z = g(Y, Z)X − g(X,Z)Y. (4.6) According to Karcher [15], a Lorentzian manifold is called infinitesimally spatially isotropic relative to a unit timelike vector field U if its Riemann curvature tensor R satisfies the relation R(X,Y )Z = δ [ g(Y, Z)X − g(X,Z)Y ] for all X,Y, Z ∈ U⊥ and R(X,U)U = γX for X ∈ U⊥ where δ, γ are real valued functions on the manifold. Hence, we can obtain the following theorem. Theorem 4.2. An n-dimensional M -projectively flat LP-Sasakian manifold is infinitesimally spatially isotropic relative to the unit timelike vector field ξ. Theorem 4.3. Let M be an n-dimensional M -projectively flat LP-Sasakian manifold. Then M is semisymmetric, i.e., the condition R(X,Y ).R = 0 holds. ISSN 1027-3190. Укр. мат. журн., 2013, т. 65, № 11 1564 F. Ö. ZENGİN Proof. Let M be an n-dimensional M -projectively flat LP-Sasakian manifold. Thus, we can write R(X,Y ).R = R(X,Y )R(Z,U)V −R(R(X,Y )Z,U)V− −R(Z,R(X,Y )U)V −R(Z,U)R(X,Y )V (4.7) for all vector fields X, Y, Z, U, V on M. So from (4.6), we get R(R(X,Y )Z,U)V = g(U, V )g(Y, Z)X − g(Y,Z)g(X,V )U− −g(X,Z)g(U, V )Y + g(X,Z)g(Y, V )U. (4.8) Again, we obtain R(Z,R(X,Y )U)V = g(U, Y )g(X,V )Z − g(U, Y )g(Z, V )X− −g(U,X)g(Y, V )Z + g(X,U)g(Z, V )Y (4.9) and finally R(Z,U)R(X,Y )V = g(U,X)g(Y, V )Z − g(X,Z)g(Y, V )U− −g(X,V )g(U, Y )Z + g(X,V )g(Z, Y )U. (4.10) So from (4.7) – (4.10), one can easily get R(X,Y ).R = 0. Theorem4.3 is proof is proved. Corollary 4.1. Let M be an n-dimensional M -projectively flat LP-Sasakian manifold. Then M is Ricci semisymmetric, i.e., the condition R(X,Y ).S = 0 holds. Proof. Let M be an n-dimensional M -projectively flat LP-Sasakian manifold. Since a semisym- metric manifold is also Ricci semisymmetric, [16], from Theorem 4.2, the proof is clear. 5. M -projectively flat LP-Sasakian spacetimes. In this section, we consider that M is an M -projectively flat LP-Sasakian spacetime (M4, g) satisfying the Einstein’s equations with a cosmo- logical constant. Further let ξ be the unit time-like velocity vector of the fluid. It is known that the Einstein’s equations with a cosmological constant can be written as [17] S(X,Y )− r 2 g(X,Y ) + λg(X,Y ) = kT (X,Y ) (5.1) for all vector fields X and Y. Here, S(X,Y ) and T (X,Y ) denote the Ricci tensor and the energy- momentum tensor, respectively. In addition, λ is the cosmological constant and k is the non-zero gravitational constant. Hence by use of (4.5), (5.1) forms into T (X,Y ) = ( λ− 3 k ) g(X,Y ). (5.2) Thus, we have the following theorem. ISSN 1027-3190. Укр. мат. журн., 2013, т. 65, № 11 ON M -PROJECTIVELY FLAT LP-SASAKIAN MANIFOLDS 1565 Theorem 5.1. Let M4 be an M -projectively flat LP-Sasakian spacetime satisfying the Einstein’s equations with a cosmological constant. Then the energy momentum tensor of this space is found as in (5.2). In a perfect fluid spacetime, the energy momentum tensor is in the form T (X,Y ) = (σ + p)u(X)u(Y ) + pg(X,Y ), (5.3) where σ is the energy density, p is the isotropic pressure and u(X) is a non-zero 1-form such that g(X,V ) = u(X) for all X, V being the velocity vector field of the flow, that is, g(V, V ) = −1. Also, σ + p 6= 0. With the help of (5.2) and (5.3), we obtain (λ− 3− kp)g(X,Y ) = k(σ + p)u(X)u(Y ). (5.4) Contraction of (5.4) over X and Y leads to λ = 3− k 4 (σ − 3p). (5.5) If we put X = Y = V in (5.4) then we find λ = 3− kσ. (5.6) Combining the equations (5.5) and (5.6), we get σ + p = 0. (5.7) Hence we have the following theorem. Theorem 5.2. In an M -projectively flat LP-Sasakian spacetime M4 satisfying the Einstein’s field equations with a cosmological term then the matter contents of M4 satisfy the vacuum-like equation of state. If we assume a dust in a perfect fluid, we have σ = 3p. (5.8) By putting (5.8) in (5.7), we get p = 0. Thus, we can state the following theorem. Theorem 5.3. The M -projectively flat LP-Sasakian spacetime admitting a dust for a perfect fluid is filled with radiation. In a relativistic spacetime, the energy-momentum tensor is in the form T (X,Y ) = µu(X)u(Y ). (5.9) From (5.2), (5.9) takes the form (λ− 3)g(X,Y ) = kµu(X)u(Y ). (5.10) ISSN 1027-3190. Укр. мат. журн., 2013, т. 65, № 11 1566 F. Ö. ZENGİN Contraction of (5.10) over X and Y leads to λ = 3− 1 4 kµ. (5.11) And, if we put X = Y = V in (5.10), we get λ = 3− kµ. (5.12) Thus, combining the equations (5.11) and (5.12), we finally get that µ = 0. From this relation and (5.9), we find T (X,Y ) = 0. This means that the spacetime is devoid of the matter. In this case, we can give the following theorem. Theorem 5.4. A relativistic M -projectively flat LP-Sasakian manifold satisfying the Einstein’s field equations with a cosmological term is vacuum. 1. Matsumoto K. On Lorentzian almost paracontact manifolds // Bull. Yamagata Univ. Nat. Sci. – 1989. – 12. – P. 151 – 156. 2. Matsumoto K., Mihai I. On a certain transformation in Lorentzian para-Sasakian manifold // Tensor (N. S). – 1988. – 47. – P. 189 – 197. 3. Mihai I., Rosca R. On Lorentzian para-Sasakian manifolds // Class. Anal. – World Sci. Publ. Singapore, 1992. – P. 155 – 169. 4. De U. C., Matsumoto K., Shaikh A. A. On Lorentzian para-Sasakian manifolds // Rend. Semin. mat. Messina. – 1999. – 3. – P. 149 – 156. 5. Shaikh A. A., Baishya K. K. On φ-symmetric LP-Sasakian manifolds // Yokohama Math. J. – 2005. – 52. – P. 97 – 112. 6. Shaikh A. A., Baishya K. K. Some results on LP-Sasakian manifolds // Bull. Math. Sci. Soc. – 2006. – 49(97). – P. 193 – 205. 7. Shaikh A. A., Baishya K. K., Eyasmin S. On the existence of some types of LP-Sasakian manifolds // Commun. Korean Math. Soc. – 2008. – 23, № 1. – P. 1 – 16. 8. Shaikh A. A., Biswas S. On LP-Sasakian manifolds // Bull. Malaysian Math. Sci. Soc. – 2004. – 27. – P. 17 – 26. 9. Taleshian A., Asghari N. On LP-Sasakian manifolds satisfying certain conditions on the concircular curvature tensor // Different. Geom.-Dynam. Syst. – 2010. – 12. – P. 228 – 232. 10. Venkatesha, Bagewadi C. S. On concircular φ-recurrent LP-Sasakian manifolds // Different. Geom.-Dynam. Syst. – 2008. – 10. – P. 312 – 319. 11. Pokhariyal G. P., Mishra R. S. Curvature tensor and their relativistic significance II // Yokohama Math. J. – 1970. – 18. – P. 105 – 108. 12. Ojha R. H. A note on the M -projective curvature tensor // Indian J. Pure and Appl. Math. – 1975. – 8, № 12. – P. 1531 – 1534. 13. Ojha R. H. M -projectively flat Sasakian manifolds // Indian J. Pure and Appl. Math. – 1986. – 17, № 4. – P. 481 – 484. 14. Chaubey S. K., Ojha R. H. On the M -projective curvature tensor of a Kenmotsu manifold // Different. Geom.-Dynam. Syst. – 2010. – 12. – P. 52 – 60. 15. Karcher H. Infinitesimal characterization of Friedman universes // Arch. Math. (Basel). – 1982. – 38. – P. 58 – 64. 16. Deszcz R. On the equivalence of Ricci-semisymmetry and semisymmetry // Dep. Math. Agricultural Univ., Wroclaw. Ser. A. Theory and Methods. – 1998. – Rept № 64. 17. O’Neill B. Semi-Riemannian geometry with applications to relativity // Pure and Appl. Math. – New York: Acad. Press, 1983. – 103. Received 22.08.11, after revision — 19.08.13 ISSN 1027-3190. Укр. мат. журн., 2013, т. 65, № 11
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spelling umjimathkievua-article-25352020-03-18T19:25:49Z ON M-Projectively Flat LP-Sasakian Manifolds Про M-проективно плоскі LP-многовиди Сасакяна Zengin, F. Ö. Зенгін, F. О. In the present paper, we study the nature of LP-Sasakian manifolds admitting the M-projective curvature tensor. It is examined whether this manifold satisfies the condition W(X, Y ).R = 0. Moreover, it is proved that, in the M-projectively flat LP-Sasakian manifolds, the conditions R(X, Y ).R = 0 and R(X, Y ).S = 0 are satisfied. In the last part of the paper, an M-projectively flat space-time is introduced, and some properties of this space are obtained. Вивчається природа многовидів Сасакяна, що допускають M-проективний тензор кривизни. Перевірено, чи задовольняє цей многовид умову W(X, Y ).R = 0. Більш того, доведено, що умови R(X, Y ).R = 0 та R(X, Y ).S = 0 виконуються для M-проективно плоских LP-многовидів Сасакяна. В останній частині роботи введено M-проективно плоский простір-час та встановлено деякі властивості цього простору. Institute of Mathematics, NAS of Ukraine 2013-11-25 Article Article application/pdf https://umj.imath.kiev.ua/index.php/umj/article/view/2535 Ukrains’kyi Matematychnyi Zhurnal; Vol. 65 No. 11 (2013); 1560–1566 Український математичний журнал; Том 65 № 11 (2013); 1560–1566 1027-3190 en https://umj.imath.kiev.ua/index.php/umj/article/view/2535/1830 https://umj.imath.kiev.ua/index.php/umj/article/view/2535/1831 Copyright (c) 2013 Zengin F. Ö.
spellingShingle Zengin, F. Ö.
Зенгін, F. О.
ON M-Projectively Flat LP-Sasakian Manifolds
title ON M-Projectively Flat LP-Sasakian Manifolds
title_alt Про M-проективно плоскі LP-многовиди Сасакяна
title_full ON M-Projectively Flat LP-Sasakian Manifolds
title_fullStr ON M-Projectively Flat LP-Sasakian Manifolds
title_full_unstemmed ON M-Projectively Flat LP-Sasakian Manifolds
title_short ON M-Projectively Flat LP-Sasakian Manifolds
title_sort on m-projectively flat lp-sasakian manifolds
url https://umj.imath.kiev.ua/index.php/umj/article/view/2535
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