Bi-slant submanifolds of an S manifold

Aykut Akgün (Technical Sciences Vocational High School, Adiyaman Universitesi, Adiyaman, Turkey)
Mehmet Gülbahar (Mathematics, Harran Universitesi, Sanliurfa, Turkey)

Arab Journal of Mathematical Sciences

ISSN: 1319-5166

Article publication date: 17 September 2021

Issue publication date: 23 January 2024

809

Abstract

Purpose

Bi-slant submanifolds of S-manifolds are introduced, and some examples of these submanifolds are presented.

Design/methodology/approach

Some properties of Di-geodesic and Di-umbilical bi-slant submanifolds are examined.

Findings

The Riemannian curvature invariants of these submanifolds are computed, and some results are discussed with the help of these invariants.

Originality/value

The topic is original, and the manuscript has not been submitted to any other journal.

Keywords

Citation

Akgün, A. and Gülbahar, M. (2024), "Bi-slant submanifolds of an S manifold", Arab Journal of Mathematical Sciences, Vol. 30 No. 1, pp. 16-29. https://doi.org/10.1108/AJMS-04-2021-0073

Publisher

:

Emerald Publishing Limited

Copyright © 2021, Aykut Akgün and Mehmet Gülbahar

License

Published in Arab Journal of Mathematical Sciences. Published by Emerald Publishing Limited. This article is published under the Creative Commons Attribution (CC BY 4.0) licence. Anyone may reproduce, distribute, translate and create derivative works of this article (for both commercial and non-commercial purposes), subject to full attribution to the original publication and authors. The full terms of this licence may be seen at http://creativecommons.org/licences/by/4.0/legalcode


1. Introduction

Slant submanifolds were firstly introduced by B. Y. Chen as a generalization of invariant and anti-invariant submanifolds of Kaehler manifolds and initial computations, results and examples of these kinds of submanifolds were presented in his book [1]. A submanifold M of an almost Hermitian manifold involving an almost complex structure J is called a slant submanifold if the angle between JXp and Xp is independent of choosing of point p ∈ M and every non-zero tangent vector Xp. Later, the concept of slant submanifolds has been drawing attentions of many geometers and these submanifolds have been studying in various space forms admitting complex, contact and product structures [2–6] etc.

From the definition of slant submanifolds, the concept of slanting can be carried to distributions in the tangent bundle on a Riemannian manifold. A smooth distribution D is called as a slant distribution if the angle between JD and D is constant. By using slant distributions, bi-slant submanifolds of almost Hermitian manifolds were defined by A. Carriazo [7, 8].

A submanifold M of an almost Hermitian manifold is called a bi-slant submanifold if there exist two orthogonal slant distributions, D1 and D2, on tangent bundle TM of M with slant angles θ1 and θ2, respectively, such that one writes

(1.1)TM=D1D2.

Here, ⊕ denotes the orthogonal direct sum.

In the literature, there exist very interesting works on bi-slant submanifolds of various spaces [9–14]. An important aspect of slant submanifolds is that they can be considered as a generalization of semi-slant, hemi-slant and CR submanifolds. In fact, a bi-slant submanifold becomes.

  1. a semi-slant submanifold if and only if θ1 = 0 (or θ2 = 0),

  2. a hemi-slant submanifold if and only if θ1=π2 (or θ2=π2),

  3. a CR-submanifold if and only if θ1 = 0 and θ2=π2.

One of the important points about bi-slant submanifolds is deal to the relations between bi-slant submanifolds and slant submanifolds. Although slant submanifolds may seem like a special case of bi-slant submanifolds at first glance, this information is not correct in general. It should be noted that a bi-slant submanifold may not be a slant submanifold even if θ1 = θ2. Another point to note that one cannot know the angle between JD1 and D2 for any bi-slant submanifolds. Furthermore, any invariant submanifold does not have to be a bi-slant submanifold even if θ1 = θ2 = 0.

On the other hand, one of the most fundamental problems in submanifold theory is to establish main relations between the extrinsic and intrinsic curvature invariants for submanifolds. In this respect, B. Y. Chen [15] established an inequality involving Ricci curvature and the squared mean curvature known as the Chen-Ricci inequality in the literature. Later, this inequality has been investigated for submanifolds of ambient spaces cf [16–20].

Considering the facts mentioned above, we investigate bi-slant submanifolds of metric f-manifolds and S-manifolds in this paper. We give some examples and investigate to totally geodesic and totally umbilical submanifolds of bi-slant submanifolds. Furthermore, we compute the curvature tensors and examine the Chen-Ricci inequality and its results on these submanifolds.

2. Preliminaries

Let (M̃,g̃) be an m-dimensional Riemannian manifold with a Riemannian metric g̃ and {e1, …, em} be an orthonormal basis for TpM̃ at a point pM̃. The Ricci curvature Ric̃ is defined by

(2.1)Ric̃X,Y=j=1mg̃R̃(ej,X)Y,ej
for any X,YTM̃. For a fixed i1,,m, we have
(2.2)Ric̃ei,eiRic̃ei=jimK̃(ei,ej).

Here, K̃(ei,ej) denotes the sectional curvature of the plane section spanned by ei and ej in TM̃.

Let Πk be a k-plane subsection of TpM̃ and X be a unit vector in Πk. We choose an orthonormal basis {e1, …, ek} of Πk such that e1 = X. Then, the Ricci curvature Ric̃Πk of Πk at X is defined by

(2.3)Ric̃Πk(X)=K̃12+K̃13++K̃(e1,ek).

Here, Ric̃Πk(X) is called as k-Ricci curvature of X [15]. Thus for each fixed ei, i1,,k we get

(2.4)Ric̃Πk(ei)=jikK̃(ei,ej).

Let (M, g) be an n-dimensional submanifold of an m-dimensional Riemannian manifold (M̃,g̃) with the induced metric g from g̃. The Gauss and Weingarten formulas are given by

̃XY=XY+hX,Yand̃XN=ANX+XN
for all X, Y ∈ TM and N ∈ TM. Here, ̃, ∇ and ∇ are, respectively, the Riemannian, induced Riemannian and induced normal connections in M̃, M and the normal bundle TM of M and h is the second fundamental form related to the shape operator A by
(2.5)g̃hX,Y,N=gANX,Y.

The mean curvature vector H is given by H=1ntrace(h). The submanifold M is called totally geodesic in M̃ if h = 0 and minimal if H = 0. If hX,Y=gX,YH for all X, Y ∈ TM, then M is called totally umbilical [21].

Let R and R̃ denote the Riemannian curvature tensor fields of M and M̃ respectively. The well-known equation of Gauss is given by

(2.6)gR(X,Y)Z,W=g̃R̃(X,Y)Z,W+g̃h(X,W),h(Y,Z)g̃h(X,Z),h(Y,W)
for all X, Y, Z, W ∈ TM.

Now, we shall recall the Chen-Ricci inequality in the following:

Theorem 2.1.

[[22], Theorem 6.1] Let M be an n-dimensional submanifold of a Riemannian manifold. Then, the following statements are true.

  1. For any unit vector field X ∈ TM, it follows that

(2.7) RicX14n2H2+Ric̃(TpM)X,
where Ric̃(TpM)X is the n-Ricci curvature of the tangent space TpM of X at p ∈ M with respect to the ambient manifold M̃.
  1. The equality case of (2.7 is satisfied by for a unit vector field X ∈ TpM if and only if

(2.8) hX,Y=0,forallYTpMorthogonaltoX,2hX,X=nHp.
  1. The equality case of (2.7) holds for all unit tangent vector X ∈ TpM if and only if either p is a totally geodesic point or n = 2 and p is a totally umbilical point.

3. Metric f-manifolds and their submanifolds

A Riemannian manifold (M̃,g̃) is called as a metric f-manifold if there exists an f structure f,ξ1,,ξs,η1,,ηs consisting of a tensor field f of type 1,1, structure vector fields ξ1, …, ξs and 1-forms η1, …, ηs such that this structure satisfies [23].

(3.1)f2=I+α=1sηαξα,ηα(ξα)=1,fξ=0,ηαf=0
for any α ∈{1, …, s} and
(3.2)g̃(X,Y)=g̃(fX,fY)+α=1sηα(X)ηα(Y).
for any X,YTM̃. We note that the first and one of the remaining relations of (3.1) imply the other two relations.

The condition for an f structure being normal is equivalent to vanishing of the torsion tensor such that we have

f,f+2α=1sdηαξα,
where f,f is the Nijenhuis tensor of f, given by
f,fX,Y=fX,fYffX,YfX,fY+f2X,Y.

Let F denotes the fundamental 2-form which is defined by

(3.3)F(X,Y)=g̃(X,fY)
for any X,YTM̃. An f metric structure f,ξα,ϕα,g̃ becomes an S manifold if F = ; and the f structure is normal. For an S manifold, it is known that the following relation holds for any XTM̃ and α ∈{1, …, s}
(3.4)̃Xξα=fX.

Now, suppose that L to be a distribution spanned by the structure vector fields ξ1, …, ξs of an S manifold and D be its complementary orthogonal distribution. In this case, we can write

(3.5)TM=DL.

Hence, it is clear that if XL then ηα(X) = 0 for any α = {1, …, s} and if XD then fX = 0.

Let Π be a plane section spanned by X and fX for any XD. Then this plane is called an f section of D and the sectional curvature of such a plane is called as f sectional curvature. An S manifold whose all of f sectional curvatures are a constant value c is said to be an S space form. The Riemann curvature tensor of an S space form of constant f sectional curvature c is given by

(3.6)g̃R̃(X,Y)Z,W)=c4g(fX,fW)g(fY,fZ)g(fX,fZ)g(fY,fW)+g(X,fW)g(Y,fZ)g(X,fZ)g(Y,fW)2g(X,fY)g(Z,fW)
for all X,Y,Z,WTM̃ [24].

Next, let M be a submanifold of a metric f manifold. For any X ∈ TM, we put

(3.7)fX=TX+NX,
where TX is the tangential part and NX is the normal part of fX respectively. In a similar way, for any vector field normal to M, we put
(3.8)fV=tV+nV,
where tV and nV are the tangential and normal parts of fV respectively.

From (3.2), (3.3) and (3.7), it is easy to see that

(3.9)g(TX,Y)=g(X,TY)
for any X, Y ∈ TM.

A submanifold M is said to be an invariant submanifold (resp. anti-invariant) if T = 0 (resp. N = 0) [25]. For each non-zero vector field X in TM, if the angle between fX and TX is independent of the choice of p ∈ M and X then M is called a slant submanifold. Note that M is a slant submanifold if and only if there exists a constant λ ∈ [0, 1] satisfying

(3.10)T2=λI+λα=1sηαξα,
where I denotes the identity map [26].

4. Bi-slant submanifolds

Let M be a submanifold of an S manifold and ξ1, …, ξs to be tangent to M. A smooth distribution D on M is called a slant distribution if the angle between X and fX is constant for each non-zero vector X in Dp and for each p ∈ M.

Next, we suppose that P is the projection to TM onto D. In a similar way to (3.10) it can be also proved that D is a slant distribution if and only if there exists a constant λ ∈ [0, 1] satisfying

(4.1)(PT)2=λI+λα=1sηαξα.
Definition 4.1.

For a submanifold M of an S manifold M̃ we say that M is a bi-slant submanifold of M̃ if there exist there orthogonal distributions D1, D2 and L such that

  1. TM=D1D2L.

  2. For any i ∈{1, 2}, Di is a slant distribution with slant angle θi.

Now we shall give some examples of bi-slant submanifolds of S manifolds.

Example 4.2.

Let E8+s denotes the Euclidean (8 + s) space with Cartesian coordinates (x1, x2, x3, x4, y1, y2, y3, y4, z1, …, zs). An S structure on E8+s is usually given by the following equations:

ηα=12dzαi=14yidxi,ξα=2zα,g=α=1sηαηα+18i=14dxi+dxi+dyi+dyi,fi=14Xixi+Yiyi+α=1sZαzα=i=14YixiXiyi+α=1sYiyizα.

Consider a (4 + s)-dimensional submanifold M of E8+s given by the following equation:

x(u,v,w,m,t1,t2,,ts)=(ucosθ1,usinθ1,wcosθ2,wsinθ2,v,0,m,0,t1,t2,,ts)
for any θ0,Π2. Then we obtain a basis of TM as follows:
e1=u+α=1scosθ1vtα=cosθ1x1+α=1sy1zα+sinθ1x1+α=1sy2zα,e2=v=y1,e3=w+α=1scosθ2mtα=cosθ2x3+α=1sy3zα+sinθ2x3+α=1sy4zα,e4=m,e4+α=tα=2zα=ξα,foranyα=1,2,,s.

Suppose that D1=Span{e1,e2}, D2=Span{e3,e4} and L=Span{e4+1,,e4+s}. Then we see that M is a bi-slant submanifold with angle (θ1, θ2). Moreover, the vector fields

e5+s=sinθ1x1+α=1sy1zα+cosθ1x1+α=1sy2zα,e6+s=y2,e7+s=sinθ2x3+α=1sy3zα+cosθ2x4+α=1sy4zα,e8+s=y4
form a basis of the normal space TM. Also, it can be shown that both bases are orthonormal.
Example 4.3.

Consider the Euclidean 8-space E8+s with the usual S structure given in Example 4.2. For any constant k,

x(u,v,w,m,t1,,ts)=2ekucosucosv,ekusinucosv,ekucosusinv,ekusinusinv,ekucoswcosm,ekusinwcosm,ekucoswsinm,ekusinwsinm,t1,,ts
defines a (4 + s)-dimensional bi-slant submanifold M with the bi-slant angles (θ1, θ2) such that
θ1=arccosk2k2+1
and
θ2=arccoskk2+1.

Further examples could be given.

Let Pi: TMDi be projections. Then we can write any vector field X in TM by these projections

(4.2)X=P1X+P2X+α=13ηα(X)ξα
and
(4.3)φX=TX+NX=P1TX+P2TX+α=13ηα(X)ξα+NX.

Following the proof way of equation (3.8) in Ref. [10] and using the above facts, we get the following theorem:

Theorem 4.4.

Let M be a (2n + 2m + s)-dimensional bi-slant submanifold of M̃. Then there exists an orthonormal frame field {e1, …, e2n, e2n+1, …, e2n+2m, ξ1, …, ξs} on TM where D1=Span{e1, …, e2n}, D2=Span{e2n+1,,e2n+2m},

L=Span{ξ1, …, ξs} such that the following conditions hold:

Te1=cosθ1e2+P2Te1,Te2=cosθ1e1+P2Te2,Te2n=cosθ1e2n1+P2Te2n
and
Te2n+1=cosθ2e2n+2+P1Te2n+1,Te2n+2=cosθ2e2n+1+P1Te2n+2,Te2n+2m=cosθ2e2n+2m1+P1Te2n+2m.

Considering (4.1) and Theorem 4.4, we obtain the following lemmas immediately:

Lemma 4.5.

Let M be a bi-slant submanifold of M̃. we can write

(4.4) g(TPiX,TPiY)=cos2θig(PiX,PiY)α=13ηα(TPiX)ηα(TPiY)
for any X, Y ∈ TM.

Lemma 4.6.

Any totally geodesic or totally umbilical bi-slant submanifold of an S manifold is an invariant submanifold.

Proof. From (3.4) and (3.7), we have for any X in TM and α ∈{1, …, s}

̃Xξα=TX+NX
which shows that
hX,ξα=NX.

Hence, if M is totally geodesic or then it is clear that N = 0 which shows that the submanifold is invariant.

From Theorem 4.6, we see that the study of totally geodesic or totally umbilical bi-slant submanifolds of an S manifold reduces to the study of invariant submanifolds. Therefore, we shall investigate to the concepts of Di geodesic or Di totally umbilical bi-slant submanifolds of an S manifold throughout this study.

Now, let us consider any two vector fields X and Y in TM such that we write

(4.5)X=P1X+P2X+α=1sη(X)ξαandY=P1Y+P2Y+α=1sη(Y)ξα.

If M is Di geodesic, then we have h(PiX, PiY) = 0. Using this fact we see that the submanifold is totally Di geodesic if and only if

(4.6)h(X,Y)=h(PiX,PjY)+h(PjX,PiY)+h(PjX,PjY)+α=1sηα(X)h(Y,ξα)+ηα(Y)h(X,ξα).

If M is totally Di umbilical if and only if

(4.7)h(X,Y)=h(PiX,PjY)+h(PjX,PiY)+h(PjX,PjY)+α=1sηα(X)h(Y,ξα)+ηα(Y)h(X,ξα)+g(fX,fY)
for ij ∈{1, 2}.
Theorem 4.7.

Let M be (2n + 2m + s)-dimensional (θ1, θ2) bi-slant submanifold of an S manifold. If M is Di-geodesic then we have the following relations:

  1. For any XiDi, we have NXi = 0.

  2. For any ij ∈{1, 2}, we have

(4.8) PiTPjT=sin2θiI.

Proof. From (3.4) and (3.7), the proof of the statement (1) is straightforward.

Now we prove the statement (2), Since M is Di-geodesic, we put

(4.9)fPiX=TPiX=PiTPiX+PjTPiX
for any X ∈ TM. Using Lemma 4.5, we get
g̃(fPiX,fPiX)=cos2θig(PiX,PiX)+g(PjTPiX,PjTPiX),
which implies that
g(PjTPiX,PjTPiX)=sin2θig(PiX,PiX).

Hence we obtain

g(PiTPjTPiX,PiX)=sin2θig(PiX,PiX),
which shows the proof of statement (2).
Theorem 4.8.

Let M be a (θ1, θ2) bi-slant submanifold of M̃. For any θ[0,π2], M is θ-slant if and only if the following relations hold:

(4.10) P2TP1TP1+P2TP2TP1=0,
(4.11) P1TP1TP2+P1TP2TP2=0,
(4.12) P1TP2TP1=cos2θ1cos2θP1,
(4.13) P2TP1TP2=cos2θ2cos2θP2.

Proof. Suppose that M is θ-slant and D=D1D2. Then we write

(4.14) T(TX)=TP1TX+P2TX.
for any XD. Using (3.10), (4.1) and (4.14), we have
(4.15) T(TX)=cos2θ1P1X+P1TP1TP2X+P2TP1TP1X+P2TP1TP2X+P1TP2TP1X+P1TP2TP2X+P2TP2TP1Xcos2θ2P2X.

Considering tangential parts of D1 and D2 in (4.15), the proof is straightforward.

The converse can be obtained directly.

Theorem 4.9.

Let M be a Di-geodesic (θ1, θ2) bi-slant submanifold. If M is θ-slant for any θ[0,π2], then θ1 = θ2 and there exists the following equation for i ∈{1, 2}.

(4.16) cos2θ=cos2θi.

Proof. From (4.7), (4.12) and (4.13) we get

(4.17) sin2θi=cos2θicos2θ,
which implies (4.16). Since equation (4.16) satisfies for all i ∈{1, 2}, we obtain that θ1 = θ2.□

Remark 4.10.

We note that if a (θ1, θ2) bi-slant submanifold is θ-slant, then the angle θ does not have to be equal to θ1 and θ2. For this situation, we refer to Example 4.3 of A. Carriazzo [7] and Example 3.3 of [10].

As a result of Theorem 4.9, we get the following:

Corollary 4.11.

Let M be a Di-geodesic (θ1, θ2) bi-slant submanifold. If M is θ-slant with θ = θ1 = θ2 then M is an invariant submanifold.

Theorem 4.12.

Let M be a (θ1, θ2) bi-slant submanifold. If M is both D1 and D2 geodesic submanifold then θ1+θ2=π2.

Proof. Suppose X is a unit vector field on D such that D=D1D2. Considering the statement of (1) of Theorem 4.7 we put

fX=TP1X+P2TX.
Since M is (θ1, θ2) bi-slant, we write from Theorem 4.4 that
fX=cosθ1P1X+cosθ2P2X.
which implies that cos θ2 =  sin θ1. Therefore, we obtain θ1+θ2=π2 which is the claim of theorem.□

With similar arguments, we have the following theorem.

Theorem 4.13.

Let M be a (θ1, θ2) bi-slant submanifold of an S manifold. Then we have the following statements:

  1. If M is both totally umbilical then it is an invariant submanifold.

  2. If M is D1 and D2 totally umbilical, then θ1+θ2=π2.

As a result od Theorem 4.12 and Theorem 4.13, we obtain the following:

Corollary 4.14.

There do not exist semi-slant and hemi-slant submanifolds of an S manifold which is D1 and D2 geodesic or D1 and D2-totally umbilical.

5. Ricci curvatures of bi-slant submanifolds

In this section, we investigate the Chen-Ricci inequality and its results for bi-slant submanifolds of an S space form.

We need the following lemma for later uses:

Lemma 5.1.

Let M be a (2n + 2m + s)-dimensional (θ1, θ2) bi-slant submanifold of an S-space form and {e1, …, e2n, e2n+1, …, e2n+2m, ξ1, …, ξs} be an orthonormal basis of TM such that D1=Span{e1,,e2n} and D2=Span{e2n+1,,e2n+2m}. Then we have the following equalities:

  1. For any k ∈{1, …, 2n + 2m}, ab ∈{1, …, s} and plane sections Πkℓ = {es, ek}, Πka = Span{ek, ξa} and Πab = Span{ξa, ξb}, we have

(5.1) K̃(Πk)=c4{1+3g(fek,e)2}
and
(5.2) K̃(Πka)=K̃(Πab)=0.
  1. For any i ∈{1, …, 2n} and j ∈{2n + 1, …, 2n + 2m}, we have

(5.3) Ric̃TpM(ei)=c4{(2n+2m1)+3cos2θ1+3P2Tei2}
and
(5.4) Ric̃TpM(ej)=c4{(2n+2m1)+3cos2θ2+3P1Tej2}.

Proof. Putting X = W = ek and Y = Z = e in (3.6) we have

(5.5) g̃R̃(ek,e)e,ek=c4g(fek,fek)g(fe,fe)g(fek,fe)g(fe,fek)+g(ek,fek)g(e,fe)g(ek,fe)g(e,fek)2g(ek,fe)g(e,fek).

From (3.9) and (5.5) we get (5.1). In a similar way, it can be obtained (5.2) which completes the proof of (a). Using (2.2) and (5.1), we obtain (5.3) and (5.4) thus the proof of (b) is straightforward.□

Theorem 5.2.

Let M be a (2n + 2m + s)-dimensional bi-slant submanifold of an S-space form. Then, the following statements are true.

  1. For any unit vector field XD1, it follows that

(5.6) RicX14n2H2+c4{(2n+2m1)+3cos2θ1+P2TX2}.

The equality case of (5.6) holds for all unit tangent vector XD1 if and only if M is D1 totally geodesic.

  1. For any unit vector field XD2, it follows that

(5.7) RicX14n2H2+c4{(2n+2m1)+3cos2θ2+P1TX2}.

The equality case of (5.7) holds for all unit tangent vector XD2 if and only if M is D2 totally geodesic.

  1. The equality cases of both (5.6) and (5.7) satisfy then θ1 + θ2 = 0.

Proof. Putting (5.3) and (5.4) in (2.7), we obtain (5.6) and (5.7) inequalities respectively. Considering the (3) statements of Theorem 2.1 we get M is D1 and D2 geodesic. Using this fact and Theorem 4.12, we have θ1+θ2=π2. This completes the proof of theorem.

Now, we need to following lemma:

Lemma 5.3.

Let M be semi-slant or hemi-slant submanifold of a S manifold. Then we have the following statements:

  1. For any XD1 we have

(5.8) P2TX=0.
  1. For any XD2 we have

(5.9) P1TX=0.

Proof. Suppose that {e1, …, e2n, e2n+1, …, e2n+2m, ξ1, …, ξs} to be an orthonormal frame field on TM where D1=Span{e1,,e2n},

D2=Span{e2n+1,,e2n+2m}L=Span{ξ1,,ξs}. Since M is semi-invariant, we can choose this orthonormal frame field which satisfies

Te1=e2,,Te2n1=e2n,Te2n+1=cosθ2e2n+2,Te2n+2=cosθ2e2n+1,,Te2n+2m=cosθ2e2n+2m1.

Therefore, we have g̃(fX,Y)=0 when XD1 and YD2 which shows the statements of (1) and (2) are also true for semi-slant submanifolds.

In a similar manner, it can be shown that the statements of (i) and (ii) are true for hemi-slant submanifolds.□

Corollary 5.4.

Let M be a (2n + 2m + s)-dimensional semi-slant submanifold of an S space form. Then, the following statements are true.

  1. For any unit vector field XD1, it follows that

(5.10) RicX14n2H2+c4{(2n+2m+2)}.

The equality case of (5.10) holds for all unit tangent vector XD1 if and only if M is D1 totally geodesic point.

  1. For any unit vector field XD2, it follows that

(5.11) RicX14n2H2+c4{(2n+2m1)+3cos2θ2}.

The equality case of (5.11) holds for all unit tangent vector XD2 if and only if M is D2 totally geodesic point.

  1. The equality cases of both (5.10) and (5.11) do not satisfy.

Proof. Under the assumption, using θ1 = 0 and Lemma 5.3 in (5.6) and (5.7) we find (5.10) and (5.11). The equality cases of both (5.10) and (5.11) holds if and only if M is D1 and D2 geodesic. Considering this fact and Corollary 4.14 we get a contraction. Thus the equality cases of both (5.10) and (5.11) do not satisfy.

Following the proof way of Corollary 5.4, we obtain the following corollary:

Corollary 5.5.

Let M be a (2n + 2m + s)-dimensional hemi-slant submanifold of an S space form. Then, the following statements are true.

  1. For any unit vector field XD1, it follows that

(5.12) RicX14n2H2+c4{(2n+2m1)+3cos2θ1}.

The equality case of (5.12) holds for all unit tangent vector XD1 if and only if M is D1 totally geodesic.

  1. For any unit vector field XD2, it follows that

(5.13) RicX14n2H2+c4{(2n+2m1)}.

The equality case of (5.13) holds for all unit tangent vector XD2 if and only if M is a D2 totally geodesic.

  1. The equality cases of both (5.12) and (5.13) do not satisfy.

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Acknowledgements

The authors are thankful to the referees for their valuable comments towards the improvement of the paper.

Corresponding author

Aykut Akgün can be contacted at: muslumakgun@adiyaman.edu.tr

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