EUROPEAN JOURNAL OF PURE AND APPLIED MATHEMATICS Vol. 11, No. 3, 2018, 671-681 ISSN 1307-5543 – www.ejpam.com Published by New York Business Global Locally Conformal Almost Cosymplectic Manifold of Φ-holomorphic Sectional Conharmonic Curvature Tensor Habeeb M. Abood1, Farah Hassan J. Al-Hussaini1,∗ 1 Department of Mathematics, College of Education for Pure Sciences, University of Basrah, Basrah, Iraq Abstract. The aim of the present paper is to study the geometry of locally conformal almost cosymplectic manifold of Φ-holomorphic sectional conharmonic curvature tensor. In particular, the necessary and sufficient conditions that locally conformal almost cosymplectic manifold is a manifold of point constant Φ-holomorphic sectional conharmonic curvature tensor have been found. The relation between the mentioned manifold and the Einstein manifold is determined. 2010 Mathematics Subject Classifications: 53C55, 53B35 Key Words and Phrases: Locally conformal almost cosymplectic manifold, conharmonic cur- vature tensor, Φ-holomorphic sectional conharmonic curvature tensor, Einstein manifold. 1. Introduction Sectional curvature provides a lot of information with regard to substance geometry of Riemannian manifolds. Manifolds with constant sectional curvature are a great source of study. Morever, contact geometry plays important roles in Physics, optics, differential equations and phase spaces of a dynamical system. This stimulated the researchers to work in the domain of constancy holomorphic sectional curvatures of locally conformal almost cosymplectic manifold which is a motivating class of almost contact metric manifold.. The study of constant holomorphic sectional curvature of almost Hermitian manifolds was started by Tanno [19] in 1973. He obtained an algebraic characterization for an almost Hermitian manifold to constringe to a space of constant holomorphic sectional curvature, which he later extended for Sasakian manifold. In 1988, Kim [7] studied total spaces of constant Φ-holomorphic sectional curvature and in 1989, he studied [8] total spaces with flat contact Bochner curvature tensor for fibred Sasakian spaces with conformal fibres. In 1993, Takano [18] discuss fibred Sasakian spaces of constant Φ-holomorphic sectional ∗Corresponding author. DOI: https://doi.org/10.29020/nybg.ejpam.v11i3.3261 Email addresses: iraqsafwan2006@gmail.com (H. M. Abood), farahalhussaini14@yahoo.com (F. H. J. Al-Hussaini) http://www.ejpam.com 671 c© 2018 EJPAM All rights reserved. H. M. Abood, F. H. J. Al-Hussaini / Eur. J. Pure Appl. Math, 11 (3) (2018), 671-681 672 and at the same time Nagaich [14] showed a generalized Tanno’s results for indefinite almost Hermitian manifold. In 2009, Rani et al. [17] considered similar condition of [19] to another distinct class of almost contact manifold known as (ε)-Sasakian manifold. In 2012, Kirichenko and Kharitonova [12] studied the constancy of Φ-holomorphic sectional curvature of normal locally conformal almost cosymplectic Manifold. 2. Preliminaries In this section, we will focus our efforts on the study of almost contact metric manifold. In particular, we dedicate our study on the construction of the class of locally conformal almost cosymplectic manifold in the G-adjoined structure space. Definition 2.1. [1] Let M be 2n + 1 dimensional smooth manifold , η be differential 1- form called a contact form, ξ be vector field called a characteristic, Φ be an endomorphism of the module of the vector fields X(M) called a structure endomorphisim, then the triple (η, ξ,Φ) is called an almost contact structure if the following conditions hold (i) η(ξ) = 1 ; (ii) Φ(ξ) = 0 ; (iii) η ◦ Φ = 0 ; (iv) Φ2 = −id+ η ⊗ ξ. Morover, if there is a Riemannian metric g = 〈., .〉 on M such that 〈ΦX,ΦY 〉 = 〈X,Y 〉 − η(X)η(Y ), X, Y ∈ X(M), then the tetrad of tensors (η, ξ,Φ, g) is called an almost contact metric structure. In this case the manifold M equipped with this structure is called an almost contact metric manifold. Definition 2.2. [9] Let (M, η,Φ, g) be almost contat metric manifold (AC-manifold). In the module X(M) we can determine two complementary projections m, `, where m = η⊗ξ and ` = −Φ2; thus X(M) = L⊕ ℵ, where L =ImΦ = kerη and ℵ =Imm = kerΦ, where ` and m are the projections onto the submodules L and ℵ respectively. Definition 2.3. [9] In the complexification module Lc of the module L define two endo- morphisms σ and σ̄ as σ = 1 2(id − √ −1Φ) and σ̄ = −1 2(id + √ −1Φ). We can define two projections by the forms: Π = σ ◦ ` = −1 2 (Φ2 − √ −1Φ) and Π̄ = σ̄ ◦ ` = 1 2 (Φ2 + √ −1Φ), where σ ◦Φ = Φ ◦ σ = iσ and σ̄ ◦Φ = Φ ◦ σ̄ = −iσ̄. Therefore, If we denote ImΠ = D √ −1 Φ and ImΠ̄ = D− √ −1 Φ , then Xc(M) = D √ −1 Φ ⊕D− √ −1 Φ ⊕D0 Φ, where D √ −1 Φ , D− √ −1 Φ and D0 Φ are proper submodules. H. M. Abood, F. H. J. Al-Hussaini / Eur. J. Pure Appl. Math, 11 (3) (2018), 671-681 673 Definition 2.4. [11] At each point p ∈ M2n+1, there is a frame in T cp (M) of the form (p, ε0, ε1, ..., εn, ε1̂, ..., εn̂), where εa = √ 2σp(ep), εâ = √ 2σ̄(ep), â = a+n, ε0 = ξp, the mappings σp : Lp −→ D √ −1 Φ , σ̄p : Lp −→ D− √ −1 Φ are isomorphism and anti-isomorphism respectively, and ea are orthonormal bases of Lp. The frame (p, ε0, ε1, ..., εn, ε1̂, ..., εn̂) is called an A-frame. Lemma 2.1. [13] The matrices components of tensors Φp and gp in A-frame have the following froms respectively: (Φi j) =  0 0 0 0 √ −1In o 0 0 − √ −1In  , (gij) =  1 0 0 0 0 −In 0 In 0  , where In is the identity matrix of order n. It is well known, that the set of such frames defines an G-structure on M with structure group 1×U(n), represented by matrix of the form  1 0 0 0 A 0 0 0 A  , where A ∈ U(n). This structure is called an G-adjoined structure. Definition 2.5. [1] A skew-symmetric tensor Ω(X,Y ) = g(X,ΦY ) is called a fundamental form of the AC-structure. Definition 2.6. [4] An almost contact metric structure S = (η, ξ,Φ, g) is called an almost cosymplectic structure ( AC∫ -structure) if (i) dη = 0 ; (ii) dΩ = 0 . Definition 2.7. [15] A conformal transformation of an AC-structure S = (η, ξ,Φ, g) on a manifold is the passage from S to an AC-structure S̃ = (η̃, ξ̃, Φ̃, g̃) such that η̃ = e−ση, ξ̃ = eσξ, Φ̃ = Φ, g̃ = e−2σg where σ is the determining function of the conformal transformation. If σ =const, then the conformal transformation is said to be trivial. Definition 2.8. [15] An AC-structure S on a manifold M is said to be locally conformal almost cosymplectic (LCAC∫ -structure) if the restriction of this structure to some neigh- borhood U of an arbitrary point p ∈ M admits a conformal transformation of an almost cosymplectic structure.This transformation is called a locally conformal. A manifold M equipped with an LCAC∫ -structure is called an LCAC∫ -manifold. Lemma 2.2. [6] In the G-adjoined structure space, the collection of the structure equations of LCAC∫ -manifold has the following forms: H. M. Abood, F. H. J. Al-Hussaini / Eur. J. Pure Appl. Math, 11 (3) (2018), 671-681 674 (i) dωa = −ωab ∧ ωb +Bab c ω c ∧ ωb +Babcωb ∧ ωc +Ba bω ∧ ωb +Babω ∧ ωb; (ii) dωa = ωba ∧ ωb +Bc abωc ∧ ωb +Babcω b ∧ ωc +Bb aω ∧ ωb +Babω ∧ ωb; (iii) dω = Cbω ∧ ωb + Cbω ∧ ωb; (iv) dωab = −ωac ∧ωcb +Aacdb ωc∧ωd+Aabcdω c∧ωd+Aacbdω d∧ωc+Aabc0ω∧ωc+Aac0b ω∧ωc; where (i) B[abc] = B[abc] = 0; (ii) B[ab] = B[ab] = 0; (iii) Ba b = Bb a = σ0δ b a; (iv) Cab = Cab = 0; (v) Bab c = 2σ[aδ b] c , Bc ab = 2σ[aδ c b]; (vi) Cb = −σb, Cb = −σb; (vii) Aacdb = 2δ [c b σ a]d − 2δ [d b σ a]c +Bacd b − 2σaδ [d b σ c] − 2σeB ae[dδ c] b + 2σbB abc; (viii) A [acd] b = σeB e[daδ c] b ; (ix) Aac[bd] = −2δ [c [bσ a] d] + 2σ[aδ e] b σ[eδ c d] − 2σ[aδ e] d σ[eδ c b] + 1 2 BaecBebd; (x) Aac0b = −2δ [c b σ a]0 +Dac b − δabσc0 − 2BaecBeb − σaσ0δ c b + 2Bacσb −Baeσeδ c b; (xi) A [ac]0 b = σ [c 0 δ a] b − σdδ [a b B d]c + σ0σ [cδ a] b + 1 2 BdcaBbd; (xii) Ba[bcd] = −Ba[dbσC]; (xiii) Babc0 = −2Da[bc] −Badcσ0; (xiv) σ[cd] = σbB bcd. Here Babc, Babc; B ab, Bab; B a b , Bb a; Cab, Cab; C b, Cb; A acd b , Abacd; A ac bd; Aac0b , Abac0; Babci, Babci; D abi, Dabi and σij are smooth functions in the G-adjoined structure space. The following lemma gives the expression for the nonzero components of Riemannian curvature tensor of LCAC∫ -manifold in the G-adjoined structure space. Lemma 2.3. [6] In the G-adjoined structure space, the components of Riemannian cur- vature tensor of LCAC∫ -manifold have the following forms: (i) Rabcd = 2(Aabcd + 4σ[aδ h] [cBd]hb − σ0Bb[dδ a c]); H. M. Abood, F. H. J. Al-Hussaini / Eur. J. Pure Appl. Math, 11 (3) (2018), 671-681 675 (ii) Ra b̂cd = 2(2δ [b [cσ a] d] + 2BhabBhdc − δa[cδ b d]σ 2 0); (iii) Ra bcd̂ = Aadbc + 4σ[aδ h] c σ[hδ d b] − 4BdahBchb +BadBbc − δac δdbσ2 0; (iv) Râbcd = 2(2B[c|ab|d] − 2σ[aBb]cd +Ba[cBd]b); (v) Ra0cd = 2(σ0[cδ a d] +BabBbcd − 2σ[aδ h] [cBd]h); (vi) Rabĉ0 = Aac0b + σbB ac − δcbσ0σ a; (vii) Râbc0 = 2Bcab0 + 2Bcabσ0; (viii) Ra0b0 = −δabσ00 − δabσ2 0 −BcbBac − σab − σaσb + 2σ[aδ c] b σc; (ix) Ra 0b̂0 = 2σ0B ab −Dab0 − σab − σaσb + 2Bbacσc. and the other components are conjugate to the above components or can be obtained by the property of symmetry for R or equal to zero. Definition 2.9. [3] A Ricci tensor is a tensor of type (2,0) which is defined by rij = −Rkijk Lemma 2.4. In the G-adjoined structure space, the components of the Ricci tensor of LCAC∫ -manifold are given by the following forms: (i) rab = 2(−2Ac(ab)c − 4(σ[cδ h] [bBc]ha + σ[cδ h] [aBc]hb) + σ0Ba[cδ c b] + σ0Bb[cδ c a] + 2σ0Bab − Dab0 − σab − σaσb + 2Bbahσ h; (ii) râb = −4(δ [a [bσ c] c] − σ[cδ b h]σ [hδ a] c − 1 2 σ[aδ h] b σh + BhcaBhcb + BbchBcha) + (BcbBac − BhbB ah) +Acbac − δabσ00 − 2nσ2 0 − σab − σaσb; (iii) ra0 = −Acac0 − σcBac + nσ0σa + 2(σ0[cδ c a] +BcbBbca − 2σ[cδ h] [cBa]h); (iv) roo = −2n(σ00 + σ2 0)− 2BhcB ch − 2(σcc + σcσc) + 4σ[cδ h] c σh. and the other components can be found by taking the conjugate operator to the above components. Proof. The above components can obtained directly from the Definition 2.10 and Lemma 2.5. Definition 2.10. An LCAC∫ -manifold has Φ-invariant Ricci tensor, if Φ ◦ r = r ◦ Φ. H. M. Abood, F. H. J. Al-Hussaini / Eur. J. Pure Appl. Math, 11 (3) (2018), 671-681 676 Lemma 2.5. An LCAC∫ -manifold has Φ-invariant Ricci tensor if and only if, in the G-adjoined structure space, the following condition râb = rab = 0 holds. We conclude this section by remembering the main concept of our study which is a conharmonic curvature tensor. Definition 2.11. [5] Let M be an AC-manifold of dimension 2n+ 1. A tensor T of type (4, 0) which is invariant under conharmonic transformation and defined by the form: Tijkl = Rijkl − 1 2n− 1 (rilgjk − rjlgik + rjkgil − rikgjl) is called a conharmonic tensor, where Tijkl = −Tjikl = −Tijlk = Tklij . Theorem 2.1. In the G-adjoined structure space, the components of conharmonic curva- ture tensor of LCAC∫ -manifold are given by the following forms: (i) Tabcd = 2(2B[c|ab|d] − 2σ[aBb]cd +Ba[cBd]b); (ii) Tâbcd = 2(Aabcd + 4σ[aδ h] [cBd]hb − σ0Bb[dδ a c])− 1 2n−1(rbcδ a d − rbdδac ); (iii) Tâbcd̂ = Aadbc + 4σ[aδ h] c σ[hδ d b] − 4BdahBchb +BadBbc − δac δdbσ2 0 − 1 2n−1(rdb δ a c + rac δ d b ); (iv) Tâb̂cd = 2(2δ [b [cσ a] d] + 2BhabBhdc − δa[cδ b d]σ 2 0)− 4 2n−1(r [d [aδ c] b]); (v) Tâ0cd = 2(σ0[cδ a d] +BabBbcd − 2σ[aδ h] [cBd]h) + 1 2n−1(r0dδ a c − r0cδ a d); (vi) Tâbĉ0 = Aac0b + σbB ac − δcbσ0σ a − 1 2n−1(ra0δ c b); (vii) Tabc0 = 2Bcab0 + 2Bcabσ0; (viii) Tâ0b0 = −δabσ00 − δabσ2 0 −BcbBac − σab − σaσb + 2σ[aδ c] b σc + 1 2n−1(r00δ a b + rab ); (ix) Tâ0b̂0 = 2σ0B ab −Dab0 − σab − σaσb + 2Bbacσc + 1 2n−1(râb̂). and the other components are conjugate to the above or can be obtained by the property of symmetry for T or equal to zero. Definition 2.12. [16] A Riemannian manifold is called an Einstein manifold, if the Ricci tensor satisfies the equation rij = egij. Definition 2.13. [10] Let M be an AC-manifold, an Φ-holomorphic sectional curvature (ΦHS-curvature) of a manifold M in the direction X ∈ X(M); X 6= 0 is a function H(X) which is defined as: H(X) = 〈R(X,ΦX,X,ΦX, )〉‖X‖−4 H. M. Abood, F. H. J. Al-Hussaini / Eur. J. Pure Appl. Math, 11 (3) (2018), 671-681 677 Definition 2.14. [10] An AC-manifold is called a manifold of point constant ΦHS-curvature if 〈R(X,ΦX,X,ΦX, )〉 = c‖X‖4 where c ∈ C∞(M); for all X ∈ X(M) Lemma 2.6. [10] An AC-manifold is a manifold of point constant ΦHS-curvature c if and only if, on the G-adjoined structure, R (a d) (bc) = c 2 δãdbc where δãdbc = δab δ d c + δac δ d b is the symmetric second-order Kronecker delta. Definition 2.15. Let M be an AC-manifold, an Φ-holomorphic sectional conharmonic curvature (ΦHTS-curvature) of a manifold M in the direction X ∈ X(M); X 6= 0 is a function H(X) which is defined as H(X) = 〈T (X,ΦX,X,ΦX, )〉‖X‖−4 Definition 2.16. An AC-manifold is called a manifold of point constant ΦHST-curvature if 〈T (X,ΦX,X,ΦX, )〉 = c‖X‖4 where c ∈ C∞(M); for all X ∈ X(M). 3. The main results This section is devoted to study the theoretical application of LCAC∫ -manifold of point constant Φ-holomorphic sectional conharmonic curvature. In particular, we found the necessary and sufficient conditions in which the LCAC∫ -manifold of point constant Φ-holomorphic sectional conharmonic curvature is an Eistein manifold. The following theorems gives the necessary and sufficient condition in which an LCAC∫ - manifold is a manifold of point constant ΦHS-curvature. Theorem 3.1. An LCAC∫ -manifold is a manifold of point constant ΦHS-curvature c if and only if, the relation A (ad) (bc) = 1 2 δãdbc (σ2 0 + c)− 4σ[aδ h] c σ[hδ d b] + 4B(da)hBchb−BadBbc holds on the G-adjoined structure space. Proof. According to the components of the Riemannian curvature tensor of LCAC∫ - manifold, it follows that Ra d bc = Aadbc + 4σ[aδh] c σ[hδ d b] − 4BdahBchb +BadBbc − δac δdbσ2 0 Symmetrizing with respect to the pair of upper and lower indices of the tensor Ra d bc , we get R (a d) (bc) = A (ad) (bc) + 4σ[aδh] c σ[hδ d b] − 4B(da)hBchb +BadBbc − 1 2 δãdbc σ 2 0 H. M. Abood, F. H. J. Al-Hussaini / Eur. J. Pure Appl. Math, 11 (3) (2018), 671-681 678 By Lemma 2.6, the constancy condition on the ΦHS-curvature c for a LCAC∫ -manifold, yields A (ad) (bc) = 1 2 δãdbc (σ2 0 + c)− 4σ[aδh] c σ[hδ d b] + 4B(da)hBchb −BadBbc Theorem 3.2. Suppose that M is LCAC∫ -manifold. Then the necessary and suffcient condition in which M is a manifold of point constant ΦHST-curvature C0 is Aadbc = 4BdahBchb +BadBbc − 4σ[aδh] c σ[hδ d b] + δac δ d bσ 2 0 − C0δ a b δ d c − 1 2n− 1 (rdb δ a c + rac δ d b ) Proof. Suppose that M is LCAC∫ -manifold of the point constant ΦHTS-curvature tensor. According to the Definition 2.16, we get 〈T (X,ΦX,X,ΦX, )〉 = C0‖X‖4 In the G-adjoined structure space, we have TijklX i(ΦX)jXk(ΦX)l = C0gijgklX iXjXkX l According to the property (ΦX)a = √ −1Xa, (ΦX)â = − √ −1X â and (ΦX)0 = 0 and then using the properties of conharmonic tensor, we get −4Tâbcd̂ = 4C0δ a b δ d c Hence Aadbc = 4BdahBchb +BadBbc − 4σ[aδh] c σ[hδ d b] + δac δ d bσ 2 0 − C0δ a b δ d c − 1 2n− 1 (rdb δ a c + rac δ d b ) Theorem 3.3. If M is LCAC∫ -manifold of point constant ΦHST-curvature tensor with flat holomorphic sectional curvature tensor and Φ-invariant Ricci tensor. Then M is an Einstein manifold. Proof. Suppose that M is a manifold of point constant ΦHST-curvature tensor. According to Theorem 3.2, we have Aadbc − 4BdahBchb −BadBbc + 4σ[aδh] c σ[hδ d b] + 1 2n− 1 (rdb δ a c + rac δ d b ) = δac δ d bσ 2 0 − C0δ a b δ d c (3.1) Symmetrizing and then antisymmetrizing (3.1) by the indices (a, h) and (a, d) respectively and since M is a manifold with flat holomorphic sectional curvature tensor, then we have 1 2n− 1 (r [d b δ a] c + r[a c δ d] b ) = 1 2 (δdb δ a c − δdc δab )(σ2 0 + C0) (3.2) H. M. Abood, F. H. J. Al-Hussaini / Eur. J. Pure Appl. Math, 11 (3) (2018), 671-681 679 Contracting (3.2) by the indices (d, c), we deduce − (n− 2) 2(2n− 1) (rab + rddδ a b ) = −(n− 1) 2 δab (σ2 0 + C0) (3.3) Symmetrizing and antisymmetrizing (3.3) by the indices (a, d), we obtain rab = eδab where e = (2n− 1)(n− 1) (n− 2) (σ2 0 + C0) Since the Ricci tensor is Φ-invariant Therefore M is Einstein manifold. Theorem 3.4. If M is LCAC∫ -manifold of point constant ΦHST-curvature tensor and Φ- invariant Ricci tensor, then M is an Einstein manifold if and only if Aacbc = BacBbc + c1δ a b . Proof. Suppose that M is a manifold of point constant ΦHST-curvature tensor. According to the Theorem 3.2, we have Aadbc = 4BdahBchb +BadBbc − 4σ[aδh] c σ[hδ d b] + δac δ d bσ 2 0 − C0δ a b δ d c − 1 (2n− 1) (rdb δ a c + rac δ d b )(3.4) Symmetrizing (3.4) by the indices (a, h), we get Aadbc = BadBbc + δac δ d bσ 2 0 − C0δ a b δ d c − 1 (2n− 1) (rdb δ a c + rac δ d b ) (3.5) Contracting (3.5) by the indices (c, d), we deduce Aacbc = BacBbc + (σ2 0 − nC0)δab − 2 (2n− 1) rab (3.6) Since M is an Einstein manifold, it follows that Aacbc = BacBbc + c1δ a b where c1 = σ2 0 − nC0 − 2e (2n−1) Conversely, by substituted Aacbc in equation (3.6), we get rab = eδab According to Φ-invariant of Ricci tensor, it follows that M is Einstein manifold. REFERENCES 680 References [1] D.E. Blair, The theory of quasi-Sasakian structures, J. 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