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Article

Chen Inequalities for Spacelike Submanifolds in Statistical Manifolds of Type Para-Kähler Space Forms

1
Department of Applied Mathematics, Bucharest University of Economic Studies, 6 Piaţa Romană, 010374 Bucharest, Romania
2
Romanian Academy, Costin C. Kiriţescu National Institute of Economic Research—Centre of Mountain Economy (CE-MONT), 13 Calea 13 Septembrie, 030508 Bucharest, Romania
3
Department of Mathematics, University of Hasselt, BE 3590 Diepenbeek, Belgium
4
Department of Teacher Education, Thomas More University College, 2290 Vorselaar, Belgium
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Submission received: 28 December 2021 / Revised: 17 January 2022 / Accepted: 18 January 2022 / Published: 21 January 2022
(This article belongs to the Special Issue Analytic and Geometric Inequalities: Theory and Applications)

Abstract

:
In this paper, we prove some inequalities between intrinsic and extrinsic curvature invariants, namely involving the Chen first invariant and the mean curvature of totally real and holomorphic spacelike submanifolds in statistical manifolds of type para-Kähler space forms. Furthermore, we investigate the equality cases of these inequalities. As illustrations of the applications of the above inequalities, we consider a few examples.

1. Introduction

A fundamental challenge in submanifold theory is to obtain simple relationships between the main intrinsic and extrinsic invariants of submanifolds [1]. There is an increased interest to provide answers of this open problem establishing some types of geometric inequalities (see, e.g., [2,3,4,5,6]).
The study of Chen invariants started in 1993, when Chen investigated basic inequalities for submanifolds in real space forms, now called the Chen inequalities [7]. An insightful and comprehensive study on Chen inequalities can be discovered in [2]. Recently, illustrations of some selected research works on Chen invariants are revealed in [8,9,10]. Actual solutions of the above problem are focused on inequalities for submanifolds in a statistical manifold, concept introduced by Amari [11] in 1985 in the context of information geometry. The statistical manifolds also have applications in physics, machine learning, statistics, etc. Recently, Chen et al. established a Chen first inequality for statistical submanifolds in Hessian manifolds of constant Hessian curvature [12]. Moreover, Aytimur et al. studied Chen inequalities for statistical submanifolds of Kähler-like statistical manifolds [13].
The para-complex numbers (hyperbolic numbers) are introduced by Graves in 1845 [14] in the form z = x + y j , where x and y are real numbers, j 2 = 1 and j 1 . Later, the para-Kähler geometry is concerned with the study of para-Kähler structures. The notion of para-Kähler manifold, first called stratified space by Rashevskij [15], is clearly defined in 1949 by Ruse [16] and Rozenfeld [17]. This geometry has applications in areas of mathematics, mechanics, physics [18], and general theory of relativity [19]. Mihai et al. investigated skew-symmetric vector fields on C R -submanifolds of para-Kähler manifolds [20]. Recently, the concept of Codazzi–para-Kähler structure was introduced by Fei and Zhang in [21] in order to represent the interaction of Codazzi couplings with para-Kähler geometry. Very recently, Vîlcu studied statistical manifolds endowed with almost product structures and para-Kähler-like statistical submersions [22]. Moreover, Chen et al. established Casorati inequalities for totally real spacelike submanifolds in statistical manifolds of type para-Kähler space forms [23].
The topic of totally real and Lagrangian submanifolds of Kähler manifolds has been studied extensively (see, e.g., [24,25,26,27]). However, just a few results are devoted to the context of para-Kähler manifolds. Chen established optimal Chen inequalities for Lagrangian submanifolds of the flat para-Kähler manifold ( E 2 n , g , P ) [28]. Furthermore, the Lagrangian H-umbilical submanifolds of para-Kähler manifolds are explored in [29,30].
In this paper, we prove some inequalities between intrinsic and extrinsic curvature invariants, namely involving the Chen first invariant and the mean curvature of totally real and holomorphic spacelike submanifolds in statistical manifolds of type para-Kähler space forms. In this respect, we use a calculus of optimization theory. In addition, the case of equalities is demonstrated and some examples are revealed.

2. Preliminaries

A statistical manifold is a semi-Riemannian manifold ( M ¯ , g ¯ ), endowed with a pair of torsion-free affine connections ( ¯ , ¯ * ) which satisfy the formula:
X g ¯ ( Y , Z ) = g ¯ ( ¯ X Y , Z ) + g ¯ ( Y , ¯ X * Z ) ,
for any X, Y, Z Γ ( T M ¯ ) , where Γ ( T M ¯ ) is the set of smooth tangent vector fields on M ¯ . Denote by ( M ¯ , g ¯ , ¯ ) a statistical manifold [31]. The connections ¯ and ¯ * are called conjugate (dual) connections. An obvious property of these dual connections is ¯ = ( ¯ * ) * . The pair ( ¯ , g ¯ ) is named statistical structure.
It follows that ( M ¯ , g ¯ , ¯ * ) is also a statistical manifold. Denote by ¯ 0 the Levi–Civita connection of M ¯ defined by ¯ 0 = ¯ + ¯ * 2 [32].
Suppose M is an m-dimensional submanifold of a 2 n -dimensional statistical manifold ( M ¯ , g ¯ , ¯ ) with g the induced metric on M, and ∇ the induced connection on M. Then ( M , g , ) is likewise a statistical manifold.
The formulas of Gauss [31] are represented by the expressions:
¯ X Y = X Y + h ( X , Y ) , ¯ X * Y = X * Y + h * ( X , Y ) ,
for any X , Y Γ ( T M ) , where the bilinear and symmetric ( 0 , 2 ) -tensors h and h * are called the imbedding curvature tensor of M in M ¯ with respect to ¯ and ¯ * , respectively.
Denote by R and R ¯ the ( 0 , 4 ) -curvature tensors for the connections ∇ and ¯ , respectively.
Then, for the vector fields X , Y , Z , and W tangent to M, the equation of Gauss on the connection ¯ is given by [32]:
g ¯ ( R ¯ ( X , Y ) Z , W ) = g ( R ( X , Y ) Z , W ) + g ¯ ( h ( X , Z ) , h * ( Y , W ) ) g ¯ ( h * ( X , W ) , h ( Y , Z ) ) .
Similarly, let R * and R ¯ * be the ( 0 , 4 ) -curvature tensors for the connections * and ¯ * , respectively.
Hence, the equation of Gauss on the connection ¯ * becomes [32]:
g ¯ ( R ¯ * ( X , Y ) Z , W ) = g ( R * ( X , Y ) Z , W ) + g ¯ ( h * ( X , Z ) , h ( Y , W ) ) g ¯ ( h ( X , W ) , h * ( Y , Z ) ) ,
for any vector fields X , Y , Z , and W tangent to M.
Denote by S the statistical curvature tensor field on the statistical manifold ( M , g , ) defined by [31]:
S ( X , Y ) Z = 1 2 { R ( X , Y ) Z + R * ( X , Y ) Z } ,
for any X , Y , Z Γ ( T M ) . Clearly, S is skew-symmetric. Thus S is a Riemann-curvature-like-tensor [33].
For a non-degenerate two-dimensional subspace π of the tangent space T x M , at a point x M , the sectional curvature of ( M , , g ) [31] is given by:
K ( π ) = K ( X Y ) = g ( S ( X , Y ) Y , X ) g ( X , X ) g ( Y , Y ) g 2 ( X , Y ) ,
where { X , Y } is a basis of π .
Denote by K 0 the sectional curvature of the Levi–Civita connection 0 on M.
The scalar curvature  τ of ( M , , g ) at a point x M is defined by the expression:
τ ( x ) = 1 i < j m K ( e i e j ) = 1 i < j m g ( S ( e i , e j ) e j , e i ) ,
where { e 1 , , e m } is an orthonormal frame at x.
Denote by τ 0 the scalar curvature of the Levi–Civita connection 0 on M.
Let { e 1 , , e m } and { e m + 1 , , e 2 n } be orthonormal bases of the tangent space T x M and T x M , respectively, at a point x M . Then, the mean curvature vector fields of M for ¯ and ¯ * are defined by, respectively:
H = 1 m i = 1 m h i i , H * = 1 m i = 1 m h i i * .
For the Levi–Civita connection ¯ 0 , we denote by h 0 = h + h * 2 the second fundamental form, and by
H 0 = H + H * 2
the mean curvature vector field of M.
Next, the squared mean curvatures of M for ∇ and * are given by:
H 2 = 1 m 2 α = m + 1 2 n i = 1 m h i i α 2 , H * 2 = 1 m 2 α = m + 1 2 n i = 1 m h i i * α 2 ,
where h i j α = g ( h ( e i , e j ) , e α ) and h i j * α = g ( h * ( e i , e j ) , e α ) , for i , j { 1 , , m } , α { m + 1 , , 2 n } .
A tensor field P ± I of type ( 1 , 1 ) , satisfying P 2 = I , where I is the identity tensor field on M ¯ , is named an almost product structure on M ¯ .
An almost para-Hermitian manifold denoted by ( M ¯ , P , g ¯ ) [2] is a manifold M ¯ equipped with an almost product structure P and a semi-Riemannian metric g ¯ performing:
g ¯ ( P X , P Y ) = g ¯ ( X , Y ) ,
for all vector fields X, Y on M ¯ . Notice that the dimension of ( M ¯ , P , g ¯ ) is even.
If ( M ¯ , P , g ¯ ) satisfies the formula ¯ P = 0 , then it is called a para-Kähler manifold [2], where ¯ is the Levi–Civita connection of M ¯ .
An almost para-Hermitian-like manifold  ( M ¯ , P , g ¯ ) [22] is a semi-Riemannian manifold ( M ¯ , g ¯ ) equipped with an almost product structure P satisfying:
g ¯ ( P X , Y ) + g ¯ ( X , P * Y ) = 0 ,
for all vector fields X, Y on M ¯ , where P * is (1,1)-tensor field on M ¯ .
A para-Kähler-like statistical manifold [22] is defined as an almost para-Hermitian-like manifold ( M ¯ , P , g ¯ ) endowed with a statistical structure ( ¯ , g ¯ ) such that ¯ P = 0 . It follows that the para-Kähler-like statistical manifolds are the generalization case of the para-Kähler manifolds.
A statistical manifold of type para-Kähler space form [22] is defined as a para-Kähler-like statistical manifold ( M ¯ , ¯ , P , g ¯ ) where the curvature tensor R ¯ of the connection ¯ satisfies:
R ¯ ( X , Y ) Z = c 4 { g ¯ ( Y , Z ) X g ¯ ( X , Z ) Y + g ¯ ( P Y , Z ) P X g ¯ ( P X , Z ) P Y + g ¯ ( X , P Y ) P Z g ¯ ( P X , Y ) P Z } ,
for any vector fields X , Y , and Z and a real constant c.
A submanifold M in an almost para-Hermitian (like) manifold ( M ¯ , P , g ¯ ) is called totally real if P maps each tangent space T x M into its corresponding normal space T x M .
A submanifold M in an almost para-Hermitian (like) manifold ( M ¯ , P , g ¯ ) is called holomorphic (or invariant) submanifold if P ( T x M ) = T x M , x M .
We consider the following constrained extremum problem
min x M f ( x ) ,
where M is a submanifold of a (semi)-Riemannian manifold ( M ¯ , g ¯ ) , and f : M ¯ R is a function of differentiability class C 2 .
Theorem 1
([34]). If M is complete and connected, ( g r a d f ) ( x 0 ) T x 0 M for a point x 0 M , and the bilinear form F : T x 0 M × T x 0 M R defined by:
F ( X , Y ) = Hess ( f ) ( X , Y ) + g ¯ ( h ( X , Y ) , grad f ) ,
is positive definite in x 0 , then x 0 is the optimal solution of the problem (10), where h is the second fundamental form of M.
Remark 1
([34]). If the bilinear form F defined by (11) is positive semi-definite on the submanifold M, then the critical points of f | M are global optimal solutions of the problem (10).

3. Main Inequalities

Theorem 2.
(i) The Chen first invariant of a holomorphic spacelike submanifold M of dimension m in a statistical manifold of type para-Kähler space form ( M ¯ , ¯ , P , g ¯ ) of dimension 2 n satisfies the inequality:
τ K ( π ) 2 ( τ 0 K 0 ( π ) ) + c 8 1 i < j m { g 2 ( e i , P e j ) + g 2 ( P e i , e j ) + 2 g ( e i , P e i ) g ( e j , P e j ) 4 g ( e i , P e j ) g ( P e i , e j ) } c 8 { g 2 ( e 1 , P e 2 ) + g 2 ( P e 1 , e 2 ) + 2 g ( e 1 , P e 1 ) g ( e 2 , P e 2 ) 4 g ( e 1 , P e 2 ) g ( e 2 , P e 1 ) } + ( m 2 ) ( m + 1 ) c 8 m 2 ( m 2 ) 4 ( m 1 ) ( H 2 + H * 2 ) .
(ii) The Chen first invariant of a totally real spacelike submanifold M of dimension m in a statistical manifold of type para-Kähler space form ( M ¯ , ¯ , P , g ¯ ) of dimension 2 n satisfies the inequality:
τ K ( π ) 2 ( τ 0 K 0 ( π ) ) + ( m 2 ) ( m + 1 ) c 8 m 2 ( m 2 ) 4 ( m 1 ) ( H 2 + H * 2 ) .
Moreover, the equality cases of (12) and (13) hold identically at all points x M if and only if we have:
h 1 j α = h 2 j α = h i j α = 0 , h 1 j * α = h 2 j * α = h i j * α = 0 , h 11 α + h 22 α = h 33 α = = h m m α , h 11 * α + h 22 * α = h 33 * α = = h m m * α ,
for any α { m + 1 , , 2 n } and any i , j { 3 , , m } , i < j .
Proof. 
For x M , consider { e 1 , , e m } and { e m + 1 , , e 2 n } orthonormal bases of T x M and T x M , respectively. Let { e 1 , e 2 } be an orthonormal basis in a plane section π at x, where the sectional curvature of T x M is minimum. The Chen first invariant is defined by the expression:
δ M ( x ) = τ ( x ) K ( π ) .
The sectional curvature K ( π ) of the plane section π is given by:
K ( π ) = 1 2 [ g ( R ( e 1 , e 2 ) e 2 , e 1 ) + g ( R * ( e 1 , e 2 ) e 2 , e 1 ) ] .
From the Formulas (1) and (9), we achieve:
g ( R ( e 1 , e 2 ) e 2 , e 1 ) = c 4 { 1 + g 2 ( e 1 , P e 2 ) + g ( e 2 , P e 2 ) g ( e 1 , P e 1 ) 2 g ( P e 1 , e 2 ) g ( e 1 , P e 2 ) } + α = m + 1 2 n ( h 11 * α h 22 α h 12 * α h 12 α ) .
From the Formulas (2) and (9), we have:
g ( R * ( e 1 , e 2 ) e 2 , e 1 ) = g ( R ( e 1 , e 2 ) e 1 , e 2 ) = c 4 { 1 g 2 ( P e 1 , e 2 ) g ( e 2 , P e 2 ) g ( e 1 , P e 1 ) + 2 g ( P e 1 , e 2 ) g ( e 1 , P e 2 ) } + α = m + 1 2 n ( h 11 α h 22 * α h 12 * α h 12 α ) .
Replacing (15) and (16) in (14), we find:
K ( π ) = c 4 { 1 + g 2 ( e 1 , P e 2 ) 2 + g 2 ( P e 1 , e 2 ) 2 + g ( e 2 , P e 2 ) g ( e 1 , P e 1 ) 2 g ( P e 1 , e 2 ) g ( e 1 , P e 2 ) } + 1 2 α = m + 1 2 n ( h 11 α h 22 * α + h 11 * α h 22 α 2 h 12 α h 12 * α ) .
From 2 h 0 = h + h * , it follows that (17) becomes:
K ( π ) = c 4 { 1 + g 2 ( e 1 , P e 2 ) 2 + g 2 ( P e 1 , e 2 ) 2 + g ( e 2 , P e 2 ) g ( e 1 , P e 1 ) 2 g ( P e 1 , e 2 ) g ( e 1 , P e 2 ) } + 2 α = m + 1 2 n [ h 11 0 α h 22 0 α ( h 12 0 α ) 2 ] 1 2 α = m + 1 2 n { [ h 11 α h 22 α ( h 12 α ) 2 ] + [ h 11 * α h 22 * α ( h 12 * α ) 2 ] } .
On the other hand, the scalar curvature of M, related to the sectional curvature K is given by:
τ = 1 2 1 i < j m [ g ( R ( e i , e j ) e j , e i ) + g ( R * ( e i , e j ) e j , e i ) ] .
From the Formulas (2) and (9), we obtain:
1 i < j m g ( R ( e i , e j ) e j , e i ) = m ( m 1 ) c 8 + c 4 1 i < j m [ g 2 ( e i , P e j ) + g ( e i , P e i ) g ( e j , P e j ) 2 g ( P e i , e j ) g ( e i , P e j ) ] + 1 i < j m [ g ( h * ( e i , e i ) , h ( e j , e j ) ) g ( h ( e i , e j ) , h * ( e i , e j ) ) ] .
Similarly, we have:
1 i < j m g ( R * ( e i , e j ) e j , e i ) = 1 i < j m g ( R ( e i , e j ) e i , e j ) = m ( m 1 ) c 8 + c 4 1 i < j m [ g ( e i , P e i ) g ( e j , P e j ) + g 2 ( e j , P e i ) 2 g ( e i , P e j ) g ( e j , P e i ) ] 1 i < j m [ g ( h ( e i , e i ) , h * ( e j , e j ) ) g ( h ( e i , e j ) , h * ( e i , e j ) ) ] .
Replacing (20) and (21) in (19), we find:
τ = m ( m 1 ) c 8 + c 4 1 i < j m { g 2 ( e i , P e j ) 2 + g ( e i , P e i ) g ( e j , P e j ) 2 g ( P e i , e j ) g ( e i , P e j ) + g 2 ( e j , P e i ) 2 } + 1 2 α = m + 1 2 n 1 i < j m ( h i i α h j j * α + h j j α h i i * α 2 h i j α h i j * α ) = m ( m 1 ) c 8 + c 4 1 i < j m { g 2 ( e i , P e j ) 2 + g ( e i , P e i ) g ( e j , P e j ) 2 g ( P e i , e j ) g ( e i , P e j ) + g 2 ( e j , P e i ) 2 } + 1 2 α = m + 1 2 n 1 i < j m [ ( h i i α + h i i * α ) ( h j j α + h j j * α ) h i i α h j j α h i i * α h j j * α ( h i j α + h i j * α ) 2 + ( h i j α ) 2 + ( h i j * α ) 2 ] .
From 2 h 0 = h + h * , the latter equation becomes:
τ = m ( m 1 ) c 8 + c 4 1 i < j m { g 2 ( e i , P e j ) 2 + g ( e i , P e i ) g ( e j , P e j ) 2 g ( P e i , e j ) g ( e i , P e j ) + g 2 ( e j , P e i ) 2 } + 2 α = m + 1 2 n 1 i < j m [ h i i 0 α h j j 0 α ( h i j 0 α ) 2 ] 1 2 α = m + 1 2 n 1 i < j m { [ h i i α h j j α ( h i j α ) 2 ] + [ h i i * α h j j * α ( h i j * α ) 2 ] } .
Subtracting (18) from (22), the invariant δ M can be written:
δ M = τ K ( π ) = ( m + 1 ) ( m 2 ) c 8 + c 4 1 i < j m { g 2 ( e i , P e j ) 2 + g ( e i , P e i ) g ( e j , P e j ) 2 g ( P e i , e j ) g ( e i , P e j ) + g 2 ( e j , P e i ) 2 } + 2 α = m + 1 2 n 1 i < j m [ h i i 0 α h j j 0 α ( h i j 0 α ) 2 ] 1 2 α = m + 1 2 n 1 i < j m { [ h i i α h j j α ( h i j α ) 2 ] + [ h i i * α h j j * α ( h i j * α ) 2 ] } c 4 { g 2 ( e 1 , P e 2 ) 2 + g 2 ( P e 1 , e 2 ) 2 + g ( e 2 , P e 2 ) g ( e 1 , P e 1 ) 2 g ( P e 1 , e 2 ) g ( e 1 , P e 2 ) } 2 α = m + 1 2 n [ h 11 0 α h 22 0 α ( h 12 0 α ) 2 ] + 1 2 α = m + 1 2 n { [ h 11 α h 22 α ( h 12 α ) 2 ] + [ h 11 * α h 22 * α ( h 12 * α ) 2 ] } .
Denote by A the expression:
A = ( m + 1 ) ( m 2 ) c 8 + c 4 1 i < j m { g 2 ( e i , P e j ) 2 + g ( e i , P e i ) g ( e j , P e j ) 2 g ( P e i , e j ) g ( e i , P e j ) + g 2 ( e j , P e i ) 2 } c 4 { g 2 ( e 1 , P e 2 ) 2 + g 2 ( P e 1 , e 2 ) 2 + g ( e 2 , P e 2 ) g ( e 1 , P e 1 ) 2 g ( P e 1 , e 2 ) g ( e 1 , P e 2 ) } + 2 ( τ 0 K 0 ( π ) ) .
Moreover, δ M becomes:
δ M = A 1 2 α = m + 1 2 n { 1 i < j m [ h i i α h j j α ( h i j α ) 2 ] h 11 α h 22 α + ( h 12 α ) 2 } 1 2 α = m + 1 2 n { 1 i < j m [ h i i * α h j j * α ( h i j * α ) 2 ] h 11 * α h 22 * α + ( h 12 * α ) 2 } .
It follows that:
δ M = A 1 2 α = m + 1 2 n { 3 i < j m [ h i i α h j j α ( h i j α ) 2 ] + 3 j m [ h 11 α h j j α ( h 1 j α ) 2 ] + 3 j m [ h 22 α h j j α ( h 2 j α ) 2 ] } 1 2 α = m + 1 2 n { 3 i < j m [ h i i * α h j j * α ( h i j * α ) 2 ] + 3 j m [ h 11 * α h j j * α ( h 1 j * α ) 2 ] + 3 j m [ h 22 * α h j j * α ( h 2 j * α ) 2 ] } A 1 2 α = m + 1 2 n { 3 i < j m h i i α h j j α + 3 j m h 11 α h j j α + 3 j m h 22 α h j j α } 1 2 α = m + 1 2 n { 3 i < j m h i i * α h j j * α + 3 j m h 11 * α h j j * α + 3 j m h 22 * α h j j * α } .
Let q α be a quadratic form defined by q α : R m R for any α { m + 1 , , 2 n } ,
q α ( h 11 α , h 22 α , , h m m α ) = 3 i < j m h i i α h j j α + 3 j m ( h 11 α + h 22 α ) h j j α
We investigate the constrained extremum problem
max q α
with the condition
G : h 11 α + h 22 α + + h m m α = k α ,
where k α is a real constant.
We find the solution of the following system of first order partial derivatives:
q α h 11 α = j = 3 m h j j α = 0 q α h 22 α = j = 3 m h j j α = 0 q α h 33 α = h 11 α + h 22 α + j = 4 m h j j α = 0 q α h m m α = h 11 α + h 22 α + j = 3 m 1 h j j α = 0
for any α { m + 1 , , 2 n } .
The solutions of the above system are:
h 11 α + h 22 α = h 33 α = = h m m α = k α m 1 .
For p V, consider F a 2-form, F : T p V × T p V R defined by:
F ( X , Y ) = Hess ( q α ) ( X , Y ) + h ( X , Y ) , ( grad q α ) ( p ) ,
where h is the second fundamental form of V in R m and · , · is the standard inner product on R m .
The Hessian matrix of q α is given by:
Hess ( q α ) = 0 0 1 1 0 0 1 1 1 1 0 1 1 1 1 0 .
As i = 1 m U i = 0 , for a vector field X T p V , then the hyperplane V is totally geodesic in R m . Moreover, we see:
F ( X , Y ) = 2 1 i < j m U i U j 2 U 1 U 2 = ( i = 1 m U i ) 2 i = 1 m ( U i ) 2 2 U 1 U 2 = ( U 1 + U 2 ) 2 i = 3 m ( U i ) 2 0 .
Using the Remark 1, adapted to our case, the critical point ( h 11 α , , h m m α ) of q α is the global maximum point of the problem. Then we achieve:
q α ( m 2 ) 2 ( m 1 ) ( i = 1 m h i i α ) 2 .
Similarly, we consider q α * be a quadratic form defined by q α * : R m R for any α { m + 1 , , 2 n } ,
q α * ( h 11 * α , h 22 * α , , h m m * α ) = 3 i < j m h i i * α h j j * α + 3 j m ( h 11 * α + h 22 * α ) h j j * α .
We also study the constrained extremum problem
max q α *
with the condition
G * : h 11 * α + h 22 * α + + h m m * α = k * α ,
where k * α is a real constant. Therefore, we find:
q α * ( m 2 ) 2 ( m 1 ) ( i = 1 m h i i * α ) 2 .
Finally, δ M from (26) has the expression:
δ M A 1 2 α = m + 1 2 n ( m 2 ) 2 ( m 1 ) ( i = 1 m h i i α ) 2 1 2 α = m + 1 2 n ( m 2 ) 2 ( m 1 ) ( i = 1 m h i i * α ) 2 .
Moreover, δ M satisfies the inequality:
δ M A m 2 ( m 2 ) 4 ( m 1 ) ( H 2 + H * 2 ) .
Consequently, the inequalities (12) and (13) are obtained.
The equality cases of the inequalities (12) and (13) hold if and only if we have equality sign in (26), (28), and (29). In this respect, we find:
h 1 j α = h 2 j α = h i j α = 0 , h 1 j * α = h 2 j * α = h i j * α = 0 , h 11 α + h 22 α = h 33 α = = h m m α , h 11 * α + h 22 * α = h 33 * α = = h m m * α ,
for any α { m + 1 , , 2 n } and any i , j { 3 , , m } , i < j . □

4. Examples

Example 1.
We point out that any para-Kähler manifold is a para-Kähler-like statistical manifold. Moreover, examples of statistical manifolds of type para-Kähler space forms can be illustrated among para-Kähler space forms. The flat para-Kähler space forms are represented by E n 2 n [35]. Delightful examples of spacelike Lagrangian submanifolds in E n 2 n can be discovered in [28,29]. The para-Kähler space forms of nonzero para-sectional curvature are investigated in [36].
Example 2.
Let R 2 n be a semi-Euclidean space of dimension 2 n , with the coordinates ( x 1 , , x n , y 1 , , y n ) , the flat affine connection ∇ and the pseudo-Riemannian metric g defined by
g = i = 1 n ( d x i 2 α d y i 2 ) ,
where α 0 is a real constant. The almost product structure P on R 2 n is defined by
P ( x i ) = y i , P ( y i ) = x i , i = 1 , , n .
Then ( R 2 n , , P , g ) is a statistical manifold of type para-Kähler space form. Moreover, P * is expressed by
P * ( x i ) = 1 α y i , P * ( y i ) = α x i .
For X an open set of R n , define an isometric immersion u : X R 2 n by
u ( y 1 , , y n ) = ( 0 , , 0 , y 1 , , y n ) .
Then u can be represented as a spacelike Lagrangian submanifold of ( R 2 n , , P , g ) , where the above inequalities are satisfied.

5. Conclusions

In this article, we established new Chen inequalities for totally real and holomorphic spacelike submanifolds in statistical manifolds of type para-Kähler space form. Moreover, we examined the equality cases and we indicated a few examples.

Author Contributions

Conceptualization, S.D. and S.H.; methodology, S.D. and S.H.; software, S.D. and S.H.; validation, S.D. and S.H.; investigation, S.D. and S.H.; visualization, S.D. and S.H. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

Not applicable.

Conflicts of Interest

The authors declare no conflict of interest.

References

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Decu, S.; Haesen, S. Chen Inequalities for Spacelike Submanifolds in Statistical Manifolds of Type Para-Kähler Space Forms. Mathematics 2022, 10, 330. https://0-doi-org.brum.beds.ac.uk/10.3390/math10030330

AMA Style

Decu S, Haesen S. Chen Inequalities for Spacelike Submanifolds in Statistical Manifolds of Type Para-Kähler Space Forms. Mathematics. 2022; 10(3):330. https://0-doi-org.brum.beds.ac.uk/10.3390/math10030330

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Decu, Simona, and Stefan Haesen. 2022. "Chen Inequalities for Spacelike Submanifolds in Statistical Manifolds of Type Para-Kähler Space Forms" Mathematics 10, no. 3: 330. https://0-doi-org.brum.beds.ac.uk/10.3390/math10030330

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