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arXiv:1801.03000v1 [math.DG] 09 Jan 2018

Some Properties of Kenmotsu Manifolds Admitting

a Semi-symmetric Non-metric Connection

S. K. Chaubey

Section of Mathematics, Department of IT, Shinas college of technology,

Shinas, P.O. Box 77, Postal Code 324, Sultanate of Oman.

Email: sk2222_{-}math@yahoo.co.in

A. C. Pandey

Department of Mathematics, Bramanand P. G. College, Kanpur208004-208004, U. P., India.

Email: acpbnd7373@gmail.com

N. V. C. Shukla

Department of Mathematics and Astronomy, Lucknow University -226007, U.P., India.

Email: nvcshukla7272@gmail.com

Subject Classification: 53C1553C15, 53B0553B05, 53C2553C25.

Keywords: Kenmotsu manifold, semi-symmetric non-metric connection, generalized recurrent manifold, generalized Ricci-recurrent manifold, weakly symmetric manifold, weakly Ricci-symmetric manifold.

Abstract

The aim of this paper is to study generalized recurrent, generalized Ricci-recurrent, weakly symmetric and weakly Ricci-symmetric Kenmotsu manifolds with respect to the semi-symmetric non-metric connection.

1 Introduction

Let (Mn,g)(M_{n},g) be a Riemannian manifold of dimension nn. A linear connection \nabla in (Mn,g)(M_{n},g), whose torsion tensor TT of type (1,2)(1,2) is defined as

T(X,Y)=XYYX[X,Y],T(X,Y)=\nabla_{X}Y-\nabla_{Y}X-[X,Y], (1)

for arbitrary vector fields XX and YY, is said to be torsion free or symmetric if TT vanishes, otherwise it is non-symmetric. If the connection \nabla satisfy g=0\nabla{g}=0 in (Mn,g)(M_{n},g), then it is called metric connection otherwise it is non-metric. Friedmann and Schouten [1] introduced the notion of semi-symmetric linear connection on a differentiable manifold. Hayden [2] introduced the idea of semi-symmetric linear connection with non-zero torsion tensor on a Riemannian manifold. The idea of semi-symmetric metric connection on Riemannian manifold was introduced by Yano [3]. He proved that a Riemannian manifold with respect to the semi-symmetric metric connection has vanishing curvature tensor if and only if it is conformally flat. This result was generalize for vanishing Ricci tensor of the semi-symmetric metric connection by T. Imai ([4], [6]). Various properties of such connection have studied in ([41], [42]) and by many other geometers. Agashe and Chafle [13] defined and studied a semi-symmetric non-metric connection in a Riemannian manifold. This was further developed by Agashe and Chafle [14], De and Kamilya [17], Pandey and Ojha [15], Chaturvedi and Pandey [19] and others. Sengupta, De and Binh [22], De and Sengupta [16] defined new type of semi-symmetric non-metric connections on a Riemannian manifold and studied some geometrical properties with respect to such connections. In this connection, the properties of non-metric connections have studied in ([37], [24], [23], [38], [39]) and many others. In 20082008, Tripathi introduced the generalized form of a new connection in Riemannian manifold [36]. Chaubey [20, 21] defined semi-symmetric non-metric connections on an almost contact metric manifold and studied its different geometrical properties. Some properties of such connections have been noticed in ([25], [26], [27], [28], [43]) and others.
In 1972, K. Kenmotsu [18] introduced a class of contact Riemann manifold known as Kenmotsu Manifold. He studied that if a Kenmotsu manifold satisfies the condition R(X,Y)Z = 0, then the manifold is of negative curvature -1, where R is the Riemannian curvature tensor of type (1,3) and R(X,Y)Z is derivative of tensor algebra at each point of the tangent space. Several properties of Kenmotsu Manifold have been studied by Sinha and Srivastav [7], De [8], De and Pathak [9], Chaubey et al. ([10], [11], [12]) and many others. Ozgur [32] studied generalised recurrent Kenmotsu manifold and proved that if M be a generalised recurrent Kenmotsu manifold and generalised Ricci Recurrent Kenmotsu manifold then β=α\beta=\alpha holds on M. Sular studies the generalised recurrent and generalised Ricci recurrent Kenmotsu manifolds with respect to semi symmetric metric connection and proved that β=2α\beta=2\alpha where α\alpha and β\beta are smooth functions and M is generalised recurrent and generalised Ricci recurrent Kenmotsu manifold admitting a semi-symmetric connection [35]. In the present paper, we studied the properties of semi-symmetric non-metric connection in Kenmotsu manifolds.
The present paper is organized as follows. Section 22 is preliminaries in which basic concepts of Kenmotsu manifolds are given. Section 33 deals with the brief account of semi-symmetric non-metric connection. In section 44, we define a generalized recurrent Kenmotsu manifolds with respect to the semi-symmetric non-metric connection and studied its some properties. Section 55 is concerned with the weakly symmetric Kenmotsu manifolds with respect to the semi-symmetric non-metric connection.

2 Preliminaries

An nn-dimensional Riemannian manifold (Mn,g)(M_{n},g) of class CC^{\infty} with a 11-form η\eta, the associated vector field ξ\xi and a (1,1)(1,1) tensor field ϕ\phi satisfying

ϕ2X+X=η(X)ξ,{\phi}^{2}{X}+X={\eta(X)}{\xi}, (2)
ϕξ=0,η(ϕX)=0,η(ξ)=1,{\phi}{\xi}=0,\hskip 14.22636pt{\eta({\phi{X}})}=0,\hskip 14.22636pt{\eta(\xi)}=1, (3)

for arbitrary vector field XX, is called an almost contact manifold. This system (ϕ,ξ,η)({\phi},{\xi},{\eta}) is called an almost contact structure to MnM_{n} [5]. If the associated Riemannian metric gg in MnM_{n} satisfy

g(ϕX,ϕY)=g(X,Y)η(X)η(Y),g({\phi}X,{\phi}Y)=g(X,Y)-{\eta}(X){\eta}(Y), (4)

for arbitrary vector fields XX, YY in MnM_{n}, then (Mn,g)(M_{n},g) is said to be an almost contact metric manifold. Putting ξ{\xi} for XX in (4) and using (3), we obtain

g(ξ,Y)=η(Y).g({\xi},Y)={\eta}(Y). (5)

Also,

φ(X,Y)=defg(ϕX,Y)\varphi(X,Y){\stackrel{{\scriptstyle\mathrm{def}}}{{=}}}g({\phi}X,Y) (6)

gives

φ(X,Y)+φ(Y,X)=0.\varphi(X,Y)+\varphi(Y,X)=0. (7)

where φ=dη\varphi=d\eta is 2-form.
If moreover

(DXϕ)(Y)=g(ϕX,Y)ξη(Y)ϕX,(D_{X}{\phi})(Y)=g({\phi{X}},Y){\xi}-{\eta({Y})}{\phi{X}}, (8)
DXξ=Xη(X)ξ,D_{X}{\xi}=X-{\eta({X})}{\xi}, (9)

hold in (Mn,g)(M_{n},g), where DD being the Levi-Civita connection of the Riemannian metric gg, then (Mn,g)(M_{n},g) is called a Kenmotsu manifold [18]. Also the following relations hold in a Kenmotsu manifold

K(X,Y)ξ=η(X)Yη(Y)X,K(X,Y){\xi}=\eta({X})Y-\eta{(Y)}X, (10)
K(ξ,X)Y=η(Y)Xg(X,Y)ξ,K({\xi},X)Y=\eta(Y){X}-g(X,Y){\xi}, (11)
S(X,ξ)=(n1)η(X),S(X,{\xi})=-(n-1){\eta(X)}, (12)
(DXη)(Y)=g(X,Y)η(X)η(Y)(D_{X}{\eta})(Y)=g(X,Y)-{\eta(X)}{\eta(Y)} (13)

for arbitrary vector fields XX and YY, where KK and SS denote the Riemannian curvature and Ricci tensors of the connection DD respectively.

3 Semi-symmetric non-metric connection

A linear connection \nabla on (Mn,g)(M_{n},g) is said to be a semi-symmetric non-metric connection if the torsion tensor TT of the connection \nabla and the Riemannian metric gg satisfy the following conditions:

T(X,Y)=2φ(X,Y)ξ,T(X,Y)=2\varphi(X,Y)\xi, (14)
(Xg)(Y,Z)=η(Y)φ(X,Z)η(Z)φ(X,Y),(\nabla_{X}g)(Y,Z)=-\eta(Y)\varphi(X,Z)-\eta(Z)\varphi(X,Y), (15)

for arbitrary vector fields XX, YY and ZZ, where η\eta is 11-form on (Mn,g)(M_{n},g) with ξ\xi as associated vector field. If DD denotes the Levi-Civita connection, then the semi-symmetric non-metric connection [21, 26] \nabla on (Mn,g)(M_{n},g) is defined as

XY=DXY+g(ϕX,Y)ξ,\nabla_{X}Y=D_{X}Y+g(\phi{X},Y)\xi, (16)

for arbitrary vector fields XX and YY.

The curvature tensor RR of the semi-symmetric non-metric connection [26] \nabla is defined as

R(X,Y)Z\displaystyle R(X,Y)Z =\displaystyle= K(X,Y)Z+g(ϕY,Z)DXξg(ϕX,Z)DYξ\displaystyle K(X,Y)Z+g(\phi{Y},Z)D_{X}\xi-g(\phi{X},Z)D_{Y}\xi (17)
+g((DXϕ)(Y)(DYϕ)(X),Z)ξ.\displaystyle+g\left((D_{X}\phi)(Y)-(D_{Y}\phi)(X),Z\right)\xi.

From (3), (5), (8) and (9), it follows that

R(X,Y)Z=K(X,Y)Z+g(ϕY,Z)Xg(ϕX,Z)Y+2η(Z)g(ϕX,Y)ξR(X,Y)Z=K(X,Y)Z+g(\phi{Y},Z)X-g(\phi{X},Z)Y+2\eta(Z)g(\phi{X},Y)\xi (18)

which give

S~(Y,Z)=S(Y,Z)+(n1)g(ϕY,Z)\tilde{S}(Y,Z)=S(Y,Z)+(n-1)g(\phi{Y},Z) (19)

and

r~=r.\tilde{r}=r. (20)

Here S~\tilde{S} and r~\tilde{r} denote the Ricci tensor and scalar curvature with respect to the semi-symmetric non-metric connection \nabla and rr is the scalar curvature with respect to the Levi-Civita connection DD. From (20) we leads the following corollary:

Corollary 1

Let MnM_{n} be an nn-dimensional Kenmotsu manifold equipped with a semi-symmetric non-metric connection \nabla, then the scalar curvature with respect to semi-symmetric non-metric connection is equal to scalar curvature with respect to Levi-Civita connection.

Replacing ZZ by ξ\xi in (18) and (19) and then using (3) and (5), we get

R(X,Y)ξ=K(X,Y)ξ+2g(ϕX,Y)ξR(X,Y)\xi=K(X,Y)\xi+2g(\phi{X},Y)\xi (21)

and

S~(Y,ξ)=S(Y,ξ).\tilde{S}(Y,\xi)=S(Y,\xi). (22)

4 Generalized Recurrent Kenmotsu Manifolds

Definition 1

A non-flat nn-dimensional differentiable manifold MnM_{n}, (n>3)(n>3), is called generalized recurrent manifold [29] if its curvature tensor KK satisfies the condition

(DXK)(Y,Z)W=A(X)K(Y,Z)W+B(X)[g(Z,W)Yg(Y,W)Z],(D_{X}K)(Y,Z)W=A(X)K(Y,Z)W+B(X)\left[g(Z,W)Y-g(Y,W)Z\right], (23)

where AA and B0B\neq{0} are 11-forms defined as

A(X)=g(X,ρ1),B(X)=g(X,ρ2),A(X)=g(X,\rho_{1}),{\hskip 10.5pt}B(X)=g(X,\rho_{2}), (24)

for arbitrary vector fields XX, YY, ZZ and WW. Here ρ1\rho_{1} and ρ2\rho_{2} are the vector fields associated with the 11-forms AA and BB respectively.

Definition 2

A non-flat nn-dimensional differentiable manifold MnM_{n}, (n>3)(n>3), is called generalized Ricci-recurrent [29] if its Ricci tensor SS satisfies the condition

(DXS)(Y,Z)=A(X)S(Y,Z)+(n1)B(X)g(Y,Z),(D_{X}S)(Y,Z)=A(X)S(Y,Z)+(n-1)B(X)g(Y,Z), (25)

for arbitrary vector fields XX, YY and ZZ, where AA and BB are defined as in (24).

In the similar fashion, we defined the following definitions :

Definition 3

A non-flat nn-dimensional differentiable manifold MnM_{n}, (n>3)(n>3), is called generalized recurrent with respect to the semi-symmetric non-metric connection \nabla if its curvature tensor RR satisfies the condition

(XR)(Y,Z)W=A(X)R(Y,Z)W+B(X)[g(Z,W)Yg(Y,W)Z],(\nabla_{X}R)(Y,Z)W=A(X)R(Y,Z)W+B(X)\left[g(Z,W)Y-g(Y,W)Z\right], (26)

for arbitrary vector fields XX, YY, ZZ and WW.

Definition 4

A non-flat nn-dimensional differentiable manifold MnM_{n}, (n>3)(n>3), is called generalized Ricci-recurrent with respect to the semi-symmetric non-metric connection \nabla if its Ricci tensor S~\tilde{S} satisfies the condition

(XS~)(Y,Z)=A(X)S~(Y,Z)+(n1)B(X)g(Y,Z),(\nabla_{X}\tilde{S})(Y,Z)=A(X)\tilde{S}(Y,Z)+(n-1)B(X)g(Y,Z), (27)

for arbitrary vector fields XX, YY, ZZ, where AA and BB are defined as in (24). Now we consider the generalized recurrent and generalized Ricci-recurrent Kenmotsu manifolds admitting the semi-symmetric non-metric connection \nabla and prove the following theorems:

Theorem 4.1

Let MnM_{n} be an nn-dimensional generalized recurrent Kenmotsu manifold equipped with a semi-symmetric non-metric connection \nabla. Then B=AB=A holds on MnM_{n}.

Proof 1

Replacing YY and WW by ξ\xi in (26) and using (3) and (5), we obtain

(XR)(ξ,Z)ξ=A(X)R(ξ,Z)ξ+B(X)[η(Z)ξZ].(\nabla_{X}R)(\xi,Z)\xi=A(X)R(\xi,Z)\xi+B(X)\left[\eta(Z)\xi-Z\right]. (28)

In consequence of (10) and (21), (28) becomes

(XR)(ξ,Z)ξ=(B(X)A(X))[η(Z)ξZ].(\nabla_{X}R)(\xi,Z)\xi=\left(B(X)-A(X)\right)\left[\eta(Z)\xi-Z\right]. (29)

It can be easily seen that

(XR)(ξ,Z)ξ=XR(ξ,Z)ξR(Xξ,Z)ξR(ξ,XZ)ξR(ξ,Z)Xξ.(\nabla_{X}R)(\xi,Z)\xi=\nabla_{X}R(\xi,Z)\xi-R(\nabla_{X}\xi,Z)\xi-R(\xi,\nabla_{X}Z)\xi-R(\xi,Z)\nabla_{X}\xi. (30)

From (3), (10), (21) and (30), it follows that

(XR)(ξ,Z)ξ=0.(\nabla_{X}R)(\xi,Z)\xi=0. (31)

In view of (29) and (31), we get

(B(X)A(X))[η(Z)ξZ]=0.\left(B(X)-A(X)\right)\left[\eta(Z)\xi-Z\right]=0. (32)

Since Zη(Z)ξZ\neq{\eta(Z)\xi} in general, therefore B=AB=A.

Theorem 4.2

If an nn-dimensional generalized Ricci-recurrent Kenmotsu manifold MnM_{n} admitting a semi-symmetric non-metric connection \nabla, then B=AB=A holds on MnM_{n}.

Proof 2

Replacing ZZ by ξ\xi in (27) and then using (5), (12) and (22), we obtain

(XS~)(Y,ξ)=(n1)η(Y)[B(X)A(X)].(\nabla_{X}\tilde{S})(Y,\xi)=(n-1)\eta(Y)\left[B(X)-A(X)\right]. (33)

It is obvious that

(XS~)(Y,ξ)=XS~(Y,ξ)S~(XY,ξ)S~(Y,Xξ).(\nabla_{X}\tilde{S})(Y,\xi)=\nabla_{X}\tilde{S}(Y,\xi)-\tilde{S}(\nabla_{X}Y,\xi)-\tilde{S}(Y,\nabla_{X}\xi). (34)

In consequence of (3), (5), (12), (13), (16) and (22), (34) becomes

(XS~)(Y,ξ)=(n1)g(X,Y)+2(n1)g(ϕX,Y)S(X,Y).(\nabla_{X}\tilde{S})(Y,\xi)=-(n-1)g(X,Y)+2(n-1)g(\phi{X},Y)-S(X,Y). (35)

From (33) and (35), it follows that

(n1)η(Y)[B(X)A(X)]=(n1)g(X,Y)+2(n1)g(ϕX,Y)S(X,Y).(n-1)\eta(Y)\left[B(X)-A(X)\right]=-(n-1)g(X,Y)+2(n-1)g(\phi{X},Y)-S(X,Y). (36)

Putting Y=ξY=\xi in (36) and using (3), (5) and (12), we obtain B=AB=A.

5 Weakly symmetric Kenmotsu manifolds

Definition 5

A non-flat nn-dimensional differentiable manifold MnM_{n}, (n>3)(n>3), is called pseudo symmetric [30] if there is a 11-form AA on MnM_{n} such that

(DXK)(Y,Z)W\displaystyle(D_{X}K)(Y,Z)W =\displaystyle= 2A(X)K(Y,Z)W+A(Y)K(X,Z)W+A(Z)K(Y,X)W\displaystyle 2A(X)K(Y,Z)W+A(Y)K(X,Z)W+A(Z)K(Y,X)W (37)
+A(W)K(Y,Z)X+g(K(Y,Z)W,X)ρ1,\displaystyle+A(W)K(Y,Z)X+g(K(Y,Z)W,X)\rho_{1},

where DD is the Levi-Civita connection and XX, YY, ZZ and WW are arbitrary vector fields on MnM_{n}. The vector field ρ1\rho_{1} associated with the 11-form AA is defined by A(X)=g(X,ρ1)A(X)=g(X,\rho_{1}).

Definition 6

A non-flat nn-dimensional differentiable manifold MnM_{n}, (n>3)(n>3), is called weakly symmetric [33, 34] if there are 11-forms AA, BB, CC and DD on MnM_{n} such that

(DXK)(Y,Z)W\displaystyle(D_{X}K)(Y,Z)W =\displaystyle= A(X)K(Y,Z)W+B(Y)K(X,Z)W+C(Z)K(Y,X)W\displaystyle A(X)K(Y,Z)W+B(Y)K(X,Z)W+C(Z)K(Y,X)W (38)
+D(W)K(Y,Z)X+g(K(Y,Z)W,X)σ,\displaystyle+D(W)K(Y,Z)X+g(K(Y,Z)W,X)\sigma,

where XX, YY, ZZ, WW are arbitrary vector fields on MnM_{n}. The vector field σ\sigma associated with the 11-form pp is defined as p(X)=g(X,σ)p(X)=g(X,\sigma). A weakly symmetric manifold MnM_{n} is said to be pseudo symmetric if B=C=D=AB=C=D=A, σ=ρ1\sigma=\rho_{1} and AA is replaced by 2A2A, locally symmetric if A=B=C=D=0A=B=C=D=0 and σ=0\sigma=0. A weakly symmetric manifold is said to be proper if at least one of the 11-forms AA, BB, CC and DD is non zero or σ0\sigma{\neq}0.

Definition 7

A non-flat nn-dimensional differentiable manifold MnM_{n}, (n>3)(n>3), is called weakly Ricci-symmetric [33, 34] if there are 11-forms α\alpha, β\beta and γ\gamma on MnM_{n} such that

(DXS)(Y,Z)=α(X)S(Y,Z)+β(Y)S(X,Z)+γ(Z)S(X,Y),(D_{X}S)(Y,Z)=\alpha(X)S(Y,Z)+\beta(Y)S(X,Z)+\gamma(Z)S(X,Y), (39)

where XX, YY and ZZ are arbitrary vector fields on MnM_{n}. A weakly Ricci-symmetric manifold MnM_{n} is called pseudo Ricci-symmetric if α=β=γ\alpha=\beta=\gamma. Contracting (38) with respect to YY, we get

(DXS)(Z,W)\displaystyle(D_{X}S)(Z,W) =\displaystyle= A(X)S(Z,W)+B(K(X,Z)W)+C(Z)S(W,X)\displaystyle A(X)S(Z,W)+B(K(X,Z)W)+C(Z)S(W,X) (40)
+D(W)S(X,Z)+p(K(X,W)Z),\displaystyle+D(W)S(X,Z)+p(K(X,W)Z),

where pp is defined as p(X)=g(X,σ)p(X)=g(X,\sigma) for arbitrary vector field XX. The author [40] studied the properties of weakly and weakly Ricci symmetric manifolds with examples.

Similarly we define the following definitions:

Definition 8

A non-flat nn-dimensional differentiable manifold MnM_{n}, (n>3)(n>3), is called weakly symmetric with respect to the semi-symmetric non-metric connection \nabla if there are 11-forms AA, BB, CC and DD on MnM_{n} such that

(XR)(Y,Z)W\displaystyle(\nabla_{X}R)(Y,Z)W =\displaystyle= A(X)R(Y,Z)W+B(Y)R(X,Z)W+C(Z)R(Y,X)W\displaystyle A(X)R(Y,Z)W+B(Y)R(X,Z)W+C(Z)R(Y,X)W (41)
+D(W)R(Y,Z)X+g(R(Y,Z)W,X)σ,\displaystyle+D(W)R(Y,Z)X+g(R(Y,Z)W,X)\sigma,

where XX, YY, ZZ, WW are arbitrary vector fields on MnM_{n} and the 11-forms AA, BB, CC, DD and the vector field σ\sigma are defined previously.

Definition 9

A non-flat nn-dimensional differentiable manifold MnM_{n}, (n>3)(n>3), is called weakly Ricci-symmetric with respect to the semi-symmetric non-metric connection \nabla if there are 11-forms α\alpha, β\beta and γ\gamma on MnM_{n} such that

(XS~)(Y,Z)=α(X)S~(Y,Z)+β(Y)S~(X,Z)+γ(Z)S~(X,Y),(\nabla_{X}\tilde{S})(Y,Z)=\alpha(X)\tilde{S}(Y,Z)+\beta(Y)\tilde{S}(X,Z)+\gamma(Z)\tilde{S}(X,Y), (42)

where XX, YY, ZZ are arbitrary vector fields on MnM_{n}.

Contracting (41)with YY, we get

(XS~)(Z,W)\displaystyle(\nabla_{X}\tilde{S})(Z,W) =\displaystyle= A(X)S~(Z,W)+B(R(X,Z)W)+C(Z)S~(W,X)\displaystyle A(X)\tilde{S}(Z,W)+B(R(X,Z)W)+C(Z)\tilde{S}(W,X) (43)
+D(W)S~(X,Z)+p(R(X,W)Z),\displaystyle+D(W)\tilde{S}(X,Z)+p(R(X,W)Z),

where pp is defined as p(X)=g(X,σ)p(X)=g(X,\sigma) for arbitrary vector field XX.

O¨\ddot{O}zgu¨\ddot{u}r [31] considered weakly symmetric and weakly Ricci-symmetric Kenmotsu manifolds and proved the following theorems:

Theorem 5.1

There is no weakly symmetric Kenmotsu manifold MM, (n>3)(n>3), unless A+C+DA+C+D is everywhere zero.

Theorem 5.2

There is no weakly Ricci-symmetric Kenmotsu manifold MM, (n>3)(n>3), unless α+β+γ\alpha+\beta+\gamma is everywhere zero.

Sular [35] considered weakly symmetric and weakly Ricci-symmetric Kenmotsu manifolds with respect to the semi-symmetric metric connection and proved the following results:

Theorem 5.3

There is no weakly symmetric Kenmotsu manifold MM admitting a semi-symmetric metric connection, (n>3)(n>3), unless A+C+DA+C+D is everywhere zero.

Theorem 5.4

There is no weakly Ricci-symmetric Kenmotsu manifold MM admitting a semi-symmetric metric connection, (n>3)(n>3), unless α+β+γ\alpha+\beta+\gamma is everywhere zero.

Now we consider the weakly symmetric and weakly Ricci-symmetric Kenmotsu manifolds admitting the semi-symmetric non-metric connection \nabla and prove the following theorems:

Theorem 5.5

Let MnM_{n}, (n>3)(n>3) be an nn-dimensional weakly symmetric Kenmotsu manifold admitting a semi-symmetric non-metric connection \nabla then there is no MnM_{n}, unless A+C+DA+C+D is everywhere zero.

Proof 3

Replacing WW by ξ\xi in (43) and using (3), (5), (10), (11), (12), (18), (21) and (22) we obtain

(XS~)(Z,ξ)\displaystyle(\nabla_{X}\tilde{S})(Z,\xi) =\displaystyle= (n1)A(X)η(Z)+η(X)B(Z)η(Z)B(X)\displaystyle-(n-1)A(X)\eta(Z)+\eta(X)B(Z)-\eta(Z)B(X) (44)
(n1)C(Z)η(X)+D(ξ)S(X,Z)η(Z)p(X)\displaystyle-(n-1)C(Z)\eta(X)+D(\xi)S(X,Z)-\eta(Z)p(X)
+p(ξ)g(X,Z)+(n1)D(ξ)g(ϕX,Z)p(ξ)g(ϕX,Z).\displaystyle+p(\xi)g(X,Z)+(n-1)D(\xi)g(\phi{X},Z)-p(\xi)g(\phi{X},Z).

From (35) and (44), it follows that

(n1)g(X,Z)+2(n1)g(ϕX,Z)S(X,Z)\displaystyle-(n-1)g(X,Z)+2(n-1)g(\phi{X},Z)-S(X,Z)
=(n1)A(X)η(Z)+η(X)B(Z)η(Z)B(X)\displaystyle=-(n-1)A(X)\eta(Z)+\eta(X)B(Z)-\eta(Z)B(X)
(n1)C(Z)η(X)+D(ξ)S(X,Z)η(Z)p(X)\displaystyle-(n-1)C(Z)\eta(X)+D(\xi)S(X,Z)-\eta(Z)p(X)
+p(ξ)g(X,Z)+(n1)D(ξ)g(ϕX,Z)p(ξ)g(ϕX,Z).\displaystyle+p(\xi)g(X,Z)+(n-1)D(\xi)g(\phi{X},Z)-p(\xi)g(\phi{X},Z). (45)

Replacing XX and ZZ by ξ\xi in (3) and using (3), (5) and (12), we get

A(ξ)+C(ξ)+D(ξ)=0.A(\xi)+C(\xi)+D(\xi)=0. (46)

Putting Z=ξZ=\xi in (43) and using (3), (5), (10), (11), (12), (18), (21), we obtain

(XS~)(ξ,W)\displaystyle(\nabla_{X}\tilde{S})(\xi,W) =\displaystyle= (n1)A(X)η(W)+g(X,W)B(ξ)η(W)B(X)+η(X)p(W)\displaystyle-(n-1)A(X)\eta(W)+g(X,W)B(\xi)-\eta(W)B(X)+\eta(X)p(W) (47)
g(ϕX,W)B(ξ)+C(ξ)S(W,X)+(n1)C(ξ)g(ϕW,X)\displaystyle-g(\phi{X},W)B(\xi)+C(\xi)S(W,X)+(n-1)C(\xi)g(\phi{W},X)
(n1)D(W)η(X)η(W)p(X)+2g(ϕX,W)p(ξ).\displaystyle-(n-1)D(W)\eta(X)-\eta(W)p(X)+2g(\phi{X},W)p(\xi).

In consequence of (35) and (47), we have

(n1)g(X,W)+2(n1)g(ϕX,W)S(X,W)\displaystyle-(n-1)g(X,W)+2(n-1)g(\phi{X},W)-S(X,W)
=(n1)A(X)η(W)+g(X,W)B(ξ)η(W)B(X)+η(X)p(W)\displaystyle=-(n-1)A(X)\eta(W)+g(X,W)B(\xi)-\eta(W)B(X)+\eta(X)p(W)
g(ϕX,W)B(ξ)+C(ξ)S(W,X)+(n1)C(ξ)g(ϕW,X)\displaystyle-g(\phi{X},W)B(\xi)+C(\xi)S(W,X)+(n-1)C(\xi)g(\phi{W},X)
(n1)D(W)η(X)η(W)p(X)+2g(ϕX,W)p(ξ).\displaystyle-(n-1)D(W)\eta(X)-\eta(W)p(X)+2g(\phi{X},W)p(\xi). (48)

Putting W=ξW=\xi in (3) and using (3), (5) and (12), we get

η(X)B(ξ)p(X)B(X)(n1)C(ξ)η(X)\displaystyle\eta(X)B(\xi)-p(X)-B(X)-(n-1)C(\xi)\eta(X)
(n1)D(ξ)η(X)+η(X)p(ξ)(n1)A(X)=0.\displaystyle-(n-1)D(\xi)\eta(X)+\eta(X)p(\xi)-(n-1)A(X)=0. (49)

Replacing XX with ξ\xi in (3) and then using (3), (5) and (12), we find

(n1)A(ξ)η(W)(n1)C(ξ)η(W)(n1)D(W)+p(W)η(W)p(ξ)=0.-(n-1)A(\xi)\eta(W)-(n-1)C(\xi)\eta(W)-(n-1)D(W)+p(W)-\eta(W)p(\xi)=0. (50)

Replacing WW by XX in (50), we get

(n1)A(ξ)η(X)(n1)C(ξ)η(X)(n1)D(X)+p(X)η(X)p(ξ)=0.-(n-1)A(\xi)\eta(X)-(n-1)C(\xi)\eta(X)-(n-1)D(X)+p(X)-\eta(X)p(\xi)=0. (51)

Adding (3) and (51) and using (46), we obtain

η(X)B(ξ)(n1)A(X)(n1)D(X)B(X)(n1)C(ξ)η(X)=0.\eta(X)B(\xi)-(n-1)A(X)-(n-1)D(X)-B(X)-(n-1)C(\xi)\eta(X)=0. (52)

Taking X=ξX=\xi in (3) and then using (3), (5) and (12), we find

B(Z)(n1)A(ξ)η(Z)η(Z)B(ξ)(n1)C(Z)(n1)D(ξ)η(Z)=0.B(Z)-(n-1)A(\xi)\eta(Z)-\eta(Z)B(\xi)-(n-1)C(Z)-(n-1)D(\xi)\eta(Z)=0. (53)

Replacing ZZ by XX in (53), we get

B(X)(n1)A(ξ)η(X)η(X)B(ξ)(n1)C(X)(n1)D(ξ)η(X)=0.B(X)-(n-1)A(\xi)\eta(X)-\eta(X)B(\xi)-(n-1)C(X)-(n-1)D(\xi)\eta(X)=0. (54)

Adding (52) and (54) and using (46), we have

A(X)+C(X)+D(X)=0.A(X)+C(X)+D(X)=0. (55)

Hence the statement of the theorem.

Theorem 5.6

Let MnM_{n}, (n>3)(n>3), be an nn-dimensional weakly Ricci-symmetric Kenmotsu manifold admitting a semi-symmetric non-metric connection \nabla then there is no MnM_{n}, unless α+β+γ\alpha+\beta+\gamma is everywhere zero.

Proof 4

Putting Z=ξZ=\xi in (42) and then using (12), (19) and (22), we find

(XS~)(Y,ξ)\displaystyle(\nabla_{X}\tilde{S})(Y,\xi) =\displaystyle= (n1)α(X)η(Y)(n1)β(Y)η(X)\displaystyle-(n-1)\alpha(X)\eta(Y)-(n-1)\beta(Y)\eta(X) (56)
+γ(ξ)S(X,Y)+(n1)γ(ξ)g(ϕX,Y).\displaystyle+\gamma(\xi)S(X,Y)+(n-1)\gamma(\xi)g(\phi{X},Y).

In consequence of (35) and (56), we have

(n1)g(X,Y)+2(n1)g(ϕX,Y)S(X,Y)\displaystyle-(n-1)g(X,Y)+2(n-1)g(\phi{X},Y)-S(X,Y)
=(n1)α(X)η(Y)(n1)β(Y)η(X)\displaystyle=-(n-1)\alpha(X)\eta(Y)-(n-1)\beta(Y)\eta(X)
+γ(ξ)S(X,Y)+(n1)γ(ξ)g(ϕX,Y).\displaystyle+\gamma(\xi)S(X,Y)+(n-1)\gamma(\xi)g(\phi{X},Y). (57)

Taking X=Y=ξX=Y=\xi in (4) and using (3), (5) and (12), we find

α(ξ)+β(ξ)+γ(ξ)=0.\alpha(\xi)+\beta(\xi)+\gamma(\xi)=0. (58)

Replacing XX by ξ\xi in (4) and using (3), (5), (12) and (58), we get

β(Y)=β(ξ)η(Y).\beta(Y)=\beta(\xi)\eta(Y). (59)

Again replacing YY by ξ\xi in (4) and using (3), (5), (12) and (58), we obtain

α(X)=α(ξ)η(X).\alpha(X)=\alpha(\xi)\eta(X). (60)

From (3), (9), (12), (13), (16) and (22), it follows that

(ξS~)(ξ,X)=0.(\nabla_{\xi}\tilde{S})(\xi,X)=0. (61)

In view of (42), above equation becomes

α(ξ)S~(ξ,X)+β(ξ)S~(ξ,X)+γ(X)S~(ξ,ξ)=0.\alpha(\xi)\tilde{S}(\xi,X)+\beta(\xi)\tilde{S}(\xi,X)+\gamma(X)\tilde{S}(\xi,\xi)=0. (62)

With the help of (3), (5), (12) and (22), equation (62) gives

γ(X)=γ(ξ)η(X).\gamma(X)=\gamma(\xi)\eta(X). (63)

Adding (59), (60) and (63) and using (58), we get the statement of the theorem.

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