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Article

Quarter-Symmetric Non-Metric Connection of Non-Integrable Distributions

School of Mathematics Science, Mudanjiang Normal University, Mudanjiang 157011, China
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Symmetry 2024, 16(7), 848; https://doi.org/10.3390/sym16070848
Submission received: 3 June 2024 / Revised: 30 June 2024 / Accepted: 3 July 2024 / Published: 5 July 2024
(This article belongs to the Section Mathematics)

Abstract

:
In this paper, we focus on non-integrable distributions with a quarter-symmetric non-metric connection (QSNMC) in generalized Riemannian manifold. First, by studying a quarter-symmetric connection on the generalized Riemannian manifold, we obtain the condition that the connection is non-metric. Then, the Gauss, Codazzi and Ricci equations are proved for non-integrable distributions with respect to a quarter-symmetric non-metric connection in generalized Riemannian manifold. Furthermore, we deduce Chen’s inequalities for non-integrable distributions of real space forms with a quarter-symmetric non-metric connection in generalized Riemannian manifold as applications. After that, we give some examples of non-integrable distributions in Riemannian manifold with quarter-symmetric non-metric connection.

1. Introduction

In 1924, Friedmann and Schouten introduced the concept of semi-symmetric connection [1], while in 1932, Hayden defined metric connections with torsion tensor [2]. Wang Yong discussed non-integrable distribution in a Riemannian manifold with a semi-symmetric metric connection and a semi-symmetric non-metric connection in [3]. And, he deduced the Gauss, Codazzi and Ricci equations for a non-integrable distribution corresponding to a semi-symmetric metric connection and a semi-symmetric non-metric connection. A linear connection ∇ is said to be semi-symmetric on an n-dimensional Riamannian manifold ( M n , g ), if its torsion tensor T, defined by T ( X , Y ) = X Y Y X [ X , Y ] , ( X , Y Γ ( M ) ), is of the form T ( X , Y ) = ω ( Y ) X ω ( X ) Y , where ω is a 1-form. If we change X to AX, then the connection is called a quarter-symmetric connection when A is a (1,1)-tensor field [4].
At first, the idea of quarter-symmetric linear connections in differentiable manifold was introduced by Golab in 1975 [5]. Recently, more and more scholars pay attention to the quarter-symmetric connection on various manifolds. For example, in 2008, Sular, Özgür and De investigated the curvature tensor and the Ricci tensor of a Kenmotsu manifold with respect to the quarter-symmetric metric connection [6]. In 2010, De and Mondal studied a quarter-symmetric metric connection on a three-dimensional quasi-Sasakian manifold. They deduced the relation between the Riemannian connection and the quarter-symmetric metric connection on a three-dimensional quasi-Sasakian manifold. And, they investigated the curvature tensor, the Ricci tensor, scalar curvature and the first Bianchi identity of a three-dimensional quasi-Sasakian manifold with respect to the quarter-symmetric metric connection [7]. In 2012, Mondal and De studied the above with a quarter-symmetric non-metric connection on a P-Sasakian manifold again [8]. In 2019, He and Zhao studied submanifolds of an almost contact metric manifold admitting a quarter-symmetric non-metric connection. And, they proved the induced connection on a submanifold is also quarter-symmetric non-metric connection. Furthermore, they obtain the Gauss, Cadazzi and Ricci equations for submanifolds with respect to the quarter-symmetric non-metric connection, and show some applications of these equations [9]. Furthermore, Yang Yuchen and Wang Yong studied non-integrable distributions with a quarter-symmetric metric connection and a quarter-symmetric non-metric connection in Riemannian manifold in [10]. In 2019, Wang Yong obtained Chen’s inequalities for submanifolds of complex space forms and Sasakian space forms with quarter-symmetric connections [11]. In 2020, Chen’s inequalities for submanifolds in ( κ , μ ) -contact space form with two kinds of generalized semi-symmetric non-metric connections were obtained by Wang Yong [12]. In 2021, He, Zhang and Zhao, in [13], derived a first Chen-type inequality for a statistical submanifold of a statistical manifold M of a constant curvature, such that M admits a non-integrable distribution on M with a constant rank. In the same year, Al-Khaldi, Aquib, Aslam et al. obtained improved Chen–Ricci inequalities for submanifolds of generalized space forms with quarter-symmetric metric connection, with the help of which they completely characterized the Lagrangian submanifold in generalized complex space form and a Legendrian submanifold in a generalized Sasakian space form [14]. Respectively, Li, Khatri, Singh et al. obtained Chen’s inequalities for submanifolds of generalized Sasakian-space-form, admitting a quarter-symmetric connection in [15]. However, the problems related to quarter-symmetric non-metric connections on non-integrable distributions remain to be solved. Some new results will be presented in this paper and the system work of non-integrable distribution will be further improved.
In Section 2, we introduce some basic concepts about a quarter-symmetric connection on the generalized Riemannian manifold. And, we explain the conditions for becoming a non-metric connection. In Section 3, by assigning coefficients a and b, the Gauss formula and the Weingarten formula are established, and the Gauss, Codazzi and Ricci equations for non integrable distributions with respect to a quarter-symmetric non-metric connection are obtained. In Section 4, we prove Chen’s inequalities, in this case as applications. Finally, in Section 5, some examples based on non-integrable distributions in a Riemannian manifold with quarter-symmetric non-metric connections are presented.

2. Quarter-Symmetric Non-Metric Connection (QSNMC)

In this section, we will give some important information that will be used in this paper. The pair ( M , G = g + F ) is defined a generalized Riemannian manifold, where M denotes a differentiable manifold (dim M = m ) and G denotes a non-symmetric (0,2) tensor [16]. For its non-symmetry, the tensor G (i.e., the generalized Riemannian metric) can be expressed as
G ( X , Y ) = g ( X , Y ) + F ( X , Y ) ,
where g represents its symmetric part and F represents its skew-symmetric part. Specifically, g ( X , Y ) is defined as
g ( X , Y ) = 1 2 ( G ( X , Y ) + G ( Y , X ) ) ,
while F ( X , Y ) is defined as
F ( X , Y ) = 1 2 ( G ( X , Y ) G ( Y , X ) ) .
Suppose that the symmetric part g is a non-degenerate part with arbitrary characteristics. Furthermore, there exists a relationship between the symmetric part g and the skew-symmetric part F given by
F ( X , Y ) = g ( A X , Y ) ,
where A denotes the (1,1) tensor field associated with skew-symmetric tensor F. So, the quarter-symmetric connection on the generalized Riemannian manifold is determined by the torsion tensor, given in the following form:
X Q Y = X Y + a ω ( Y ) A X + b ω ( X ) A Y ,
whose torsion tensor given with
T Q ( X , Y ) = ( a b ) ( ω ( Y ) A X ω ( X ) A Y ) ,
where a and b denotes different real numbers (i.e., a , b R , a b ) and ω denotes a 1-form associated with vector field P, i.e., ω ( X ) = g ( X , P ) .
If the linear connection Q preserves the generalized Riemannian metric G, it is referred to as a generalized metric (G-metric) connection. The preservation of G implies that both its symmetric part g and its skew-symmetric part F are preserved by Q , i.e.,
Q G = 0 Q g = Q F = 0 Q g = Q A = 0 .
The connection Q is called a non-metric connection if it does not preserve the symmetric metric g, Q g 0 ; otherwise, it is considered metric.
In the following article, we will only focus on the quarter-symmetric non-metric connection in generalized Riemannian manifold ( M , G = g + F ) .

3. The Gauss, Codazzi and Ricci Equations for Non-Integrable Distribution with QSNMC

Let ( M , G = g + F ) be a m-dimensional smooth generalized Riemannian manifold, and ∇ be the Levi-Civita connection of g. We denote Γ ( M ) as the C ( M ) -module of vector fields on M and define X Y as the covariant derivative of Y with respect to X when X , Y Γ ( M ) . Let D T M be a non-integrable distribution, i.e., a subbundle of the tangent bundle T M with constant rank n, and there exist X D , Y D Γ ( D ) , such that [ X D , Y D ] is not in Γ ( D ) , where Γ ( D ) is the space of sections of D. The distribution D inherits a metric tensor field g D from the original g in M. Let D T M be the orthogonal distribution to D, which inherits a metric tensor field g D from the g, and then g = g D g D . Let π D : T M D , π D : T M D be the projections. For X D , Y D Γ ( D ) , we define X D D Y D = π D ( X D Y D ) and [ X D , Y D ] D = π D ( [ X D , Y D ] ) and [ X D , Y D ] D = π D ( [ X D , Y D ] ) . When X D , Y D Γ ( D ) and f C ( M )
f X D D Y D = f X D D Y D , X D D ( f Y D ) = X D ( f ) Y D + f X D D Y D ,
T ( X D , Y D ) = X D D Y D Y D D X D [ X D , Y D ] = [ X D , Y D ] D ,
and
X D Y D = X D D Y D + B ( X D , Y D ) , B ( X D , Y D ) = π D X D Y D .
We note that B ( X D , Y D ) B ( Y D , X D ) .
We define the connection (1) with coefficients a = b = 1 2 on M as a new quarter-symmetric non-metric connection [16], i.e.,
X Q Y = X Y + 1 2 ω ( Y ) A X 1 2 ω ( X ) A Y ,
whose torsion tensor given with
T Q ( X , Y ) = ω ( Y ) A X ω ( X ) A Y ,
and which satisfies
( X Q g ) ( Y , Z ) = 1 2 ( ω ( Y ) F ( X , Z ) + ω ( Z ) F ( X , Y ) ) .
For X D , Y D Γ ( D ) ,
X D Q Y D =   Q X D D Y D + B Q ( X D , Y D ) ,   Q X D D Y D = π D X D Q Y D , B Q ( X D , Y D ) = π D X D Q Y D .
We call the B ( X D , Y D ) as the second fundamental form with respect to the quarter-symmetric non-metric connection. By (4), (5) and (8), we have
  Q X D D Y D = X D D Y D + 1 2 ω ( Y D ) A X D 1 2 ω ( X D ) A Y D , B Q ( X D , Y D ) = B ( X D , Y D ) .
By (3) and (9), we have
  Q T D ( X D , Y D ) = [ X D , Y D ] D + ω ( Y D ) A X D ω ( X D ) A Y D .
Similarly to the case D = T M , we have the following.
Theorem 1. 
There exists a unique linear connection   Q D : Γ ( D ) × Γ ( D ) Γ ( D ) on D, which satisfies   Q T D ( X D , Y D ) = [ X D , Y D ] D + ω ( Y D ) A X D ω ( X D ) A Y D .
Let E 1 , . . . , E n be the orthonormal basis on D. We define the mean curvature vector associated with Q on D by H Q = 1 n i = 1 n B Q ( E i , E i ) Γ ( D ) . By (9), then H Q = H , where H = 1 n i = 1 n B ( E i , E i ) Γ ( D ) . If H Q = 0 , we say that D is minimal with respect to the quarter-symmetric non-metric connection Q . If γ ˙ Q γ ˙ = 0 , we say the curve γ is Q -geodesic. If every Q -geodesic with initial condition in D is contained in D, we say that D is totally geodesic with respect to the quarter-symmetric non-metric connection Q .
Let h ( X , Y ) = 1 2 [ B ( X , Y ) + B ( Y , X ) ] and h Q ( X , Y ) = 1 2 [ B Q ( X , Y ) + B Q ( Y , X ) ] . If h = H g D (respectively, h Q = H Q g D ), we say that D is umbilical with respect to ∇ (respectively, Q ). We have the following.
Proposition 1. 
D is minimal (respectively, umbilical) with respect toif and only if D is minimal (respectively, umbilical) with respect to Q .
Let ξ Γ ( D ) and X D Γ ( D ) , then by (5), we have
X D Q ξ = X D ξ + 1 2 ω ( ξ ) A X D 1 2 ω ( X D ) A ξ .
Let A ξ : Γ ( D ) Γ ( D ) be the shape operator with respect to ∇, defined by
g D ( A ξ X D , Y D ) = g D ( B ( X D , Y D ) , ξ ) .
Let L X D ξ = π D X D ξ , then X D ξ = π D X D ξ + L X D ξ , so
π D X D ξ = A ξ X D , X D ξ = A ξ X D + L X D ξ ,
which we call the Weingarten formula with respect to ∇ and L X D ξ : Γ ( D ) × Γ ( D ) Γ ( D ) is a metric connection on D along Γ ( D ) .
Let A ξ Q = ( A ξ 1 2 ω ( ξ ) A ) I and   Q L X D ξ = ( L X D ξ 1 2 ω ( X D ) A ) I ; then, by (11) and (13), we obtain the Weingarten formula with respect to Q .
X D Q ξ = A ξ Q X D + Q L X D ξ ,
Given X , Y , Z Γ ( T M ) , the curvature tensor R with respect to ∇ is defined by
R Q ( X , Y ) Z = X Q Y Z Y X Z [ X , Y ] Z .
Given X D , Y D , Z D Γ ( D ) , the curvature tensor R D on D with respect to D is defined by
  Q R D ( X D , Y D ) Z D =   Q X D D   Q Y D D Z D Q Y D D   Q X D Z D Q [ X D , Y D ] D D Z D π D [ [ X D , Y D ] D , Z D ] .
In (16),   Q R D is a tensor field by adding the extra term π D [ [ X D , Y D ] D , Z D ] . Given X D , Y D , Z D , W D Γ ( D ) , the Riemannian curvature tensors R Q ,   Q R D are defined by
R Q ( X D , Y D , Z D , W D ) = g ( R Q ( X D , Y D ) Z D , W D ) ,   Q R D ( X D , Y D , Z D , W D ) = g ( Q R D ( X D , Y D ) Z D , W D ) .
Theorem 2. 
Given X D , Y D , Z D , W D Γ ( D ) , we have the Gauss equation for D with respect to Q in the following.
R Q ( X D , Y D , Z D , W D ) =   Q R D ( X D , Y D , Z D , W D ) g ( B ( X D , W D ) , B ( Y D , Z D ) ) + g ( B ( Y D , W D ) , B ( X D , Z D ) ) + g ( Y D , Z D ) ω ( B ( X D , W D ) ) g ( X D , Z D ) ω ( B ( Y D , W D ) ) + 1 2 g ( A X D , W D ) ω ( B ( Y D , Z D ) ) 1 2 g ( A Y D , W D ) ω ( B ( X D , Z D ) ) + g ( B ( Z D , W D ) , [ X D , Y D ] ) + 1 2 ω ( [ X D , Y D ] D ) g ( A Z D , W D ) .
Proof. 
From Equations (8) and (14), we have, for X D , Y D , Z D Γ ( D ) ,
X D Q Y D Q Z D = X D Q ( Q Y D D Z D ) + X D Q ( B Q ( Y D , Z D ) ) =   Q X D D   Q Y D D Z D + B Q ( X D , Q Y D D Z D ) A B Q ( Y D , Z D ) X D + 1 2 ω ( B Q ( Y D , Z D ) ) A X D + Q L X D ( B Q ( Y D , Z D ) ) ,
Y D Q X D Q Z D =   Q Y D D   Q X D D Z D + B Q ( Y D , Q X D D Z D ) A B Q ( X D , Z D ) Y D + 1 2 ω ( B Q ( X D , Z D ) ) A Y D + Q L Y D ( B Q ( X D , Z D ) ) .
By (5) and ∇ with zero torsion, we have, for X , Y Γ ( T M ) ,
X 1 Q X 2 = X 2 Q X 1 + [ X 1 , X 2 ] + ω ( X 2 ) A X 1 ω ( X 1 ) A X 2 .
So, by (14) and (21), we obtain
Q [ X D , Y D ] D Z D = Q Z D ( [ X D , Y D ] D ) + [ [ X D , Y D ] D , Z D ] + ω ( Z D ) A [ X D , Y D ] D ω ( [ X D , Y D ] D ) A Z D = A [ X D , Y D ] D Z D + 1 2 ω ( [ X D , Y D ] D ) A Z D + Q L Z D ( [ X D , Y D ] D ) + [ [ X D , Y D ] D , Z D ] + ω ( Z D ) A [ X D , Y D ] D ω ( [ X D , Y D ] D ) A Z D = A [ X D , Y D ] D Z D + Q L Z D ( [ X D , Y D ] D ) + ω ( Z D ) A [ X D , Y D ] D 1 2 ω ( [ X D , Y D ] D ) A Z D + [ [ X D , Y D ] D , Z D ] .
By Q [ X D , Y D ] Z D = Q [ X D , Y D ] D Z D + Q [ X D , Y D ] D Z D and (12) and (8), we have
[ X D , Y D ] Q Z D =   Q [ X D , Y D ] D D Z D + B Q ( [ X D , Y D ] D , Z D ) A [ X D , Y D ] D Z D + L Z D ( [ X D , Y D ] D ) + ω ( Z D ) A [ X D , Y D ] D 1 2 ω ( [ X D , Y D ] D , A Z D ) + [ [ X D , Y D ] D , Z D ] .
By (15), (16), (19), (20), and (23), we have
R Q ( X D , Y D ) Z D =   Q R D ( X D , Y D ) Z D π D [ [ X D , Y D ] D , Z D ] + B Q ( X D , Q Y D D Z D ) B Q ( Y D , Q X D D Z D ) B Q ( [ X D , Y D ] D , Z D ) A B Q ( Y D , Z D ) X D + A B Q ( X D , Z D ) Y D + Q L X D ( B Q ( Y D , Z D ) ) Q L Y D ( B Q ( X D , Z D ) ) + 1 2 ω ( B Q ( Y D , Z D ) ) A X D 1 2 ω ( B Q ( X D , Z D ) ) A Y D + A [ X D , Y D ] D Z D L Z D ( [ X D , Y D ] D ) ω ( Z D ) A [ X D , Y D ] D + 1 2 ω ( [ X D , Y D ] D ) A Z D .
By (12), (17), and (24) and the second equality in (9), we obtain (18). □
Corollary 1. 
If U = 0, ω = 0 and Q = , we obtain
R ( X D , Y D , Z D , W D ) = R D ( X D , Y D , Z D , W D ) g ( B ( X D , W D ) , B ( Y D , Z D ) ) + g ( B ( Y D , W D ) , B ( X D , Z D ) ) + g ( B ( Z D , W D ) , [ X D , Y D ] ) .
Theorem 3. 
Given X D , Y D , Z D Γ ( D ) , we have the Codazzi equation with respect to Q in the following.
( R Q ( X D , Y D ) Z D ) D = ( Q L X D B Q ) ( Y D , Z D ) ( Q L Y D B Q ) ( X D , Z D ) ω ( X D ) B Q ( ( A Y D ) , Z D ) + ω ( Y D ) B Q ( ( A X D ) , Z D ) π D [ [ X D , Y D ] D , Z D ]   Q L Z D ( [ X D , Y D ] D ) ω ( Z D ) A [ X D , Y D ] D ,
where ( Q L X D B Q ) ( Y D , Z D ) =   Q L X D ( B Q ( Y D , Z D ) ) B Q ( Q X D D Y D , Z D ) B Q ( Y D ,   Q X D D Z D ) .
Proof. 
From (25), we have
( R Q ( X D , Y D ) Z D ) D = π D [ X D , Y D ] D , Z D + B Q ( X D , Q Y D D Z D ) B Q ( Y D , Q X D D Z D ) B Q ( [ X D , Y D ] D , Z D ) + L X D ( B Q ( Y D , Z D ) ) L Y D ( B Q ( X D , Z D ) ) L Z D ( [ X D , Y D ] D ) ω ( Z D ) A [ X D , Y D ] D .
By (21), we have, for X D , Y D Γ ( D ) ,
[ X D , Y D ] D = Q X D D Y D Q Y D D X D ω ( Y D ) A X D + ω ( X D ) A Y D .
By (28) and the definition of ( L X B Q ) ( Y D , Z D ) and (27), we obtain
( R Q ( X D , Y D ) Z D ) D = π D [ [ X D , Y D ] D , Z D ] + B Q ( X D , Q Y D D Z D ) B Q ( Y D , Q X D D Z D ) B Q ( Q X D D Y D Q Y D D X D ω ( Y D ) A X D + ω ( X D ) A Y D , Z D ) + Q L X D ( B Q ( Y D , Z D ) ) Q L Y D ( B Q ( X D , Z D ) ) Q L Z D ( [ X D , Y D ] D ) ω ( Z D ) A [ X D , Y D ] D .
So, (26) holds. □
Corollary 2. 
If U = 0 , then we have
( R ( X D , Y D ) Z D ) D = ( L X D B ) ( Y D , Z D ) ( L Y D B ) ( X D , Z D ) π D [ [ X D , Y D ] D , Z D ] L Z D ( [ X D , Y D ] D ) .
Theorem 4. 
Given X D , Y D Γ ( D ) , ξ Γ ( D ) , we have the Ricci equation for D with respect to Q in the following.
( R Q ( X D , Y D ) ξ ) D = B Q ( X D , A ξ Q Y D ) + B Q ( Y D , A ξ Q X D ) + Q R L ( X D , Y D ) ξ ,
where
  Q R L ( X D , Y D ) ξ = Q L X D   Q L Y D ξ Q L Y D   Q L X D ξ Q L [ X D , Y D ] D ξ π D [ X D , Y D ] Q ξ .
Proof. 
From (8) and (14), we have
X D Q Y D Q ξ = X D Q ( A ξ Q Y D ) + X D Q ( Q L Y D ξ ) = Q X D D ( A ξ Q Y D ) B Q ( X D , A ξ Q Y D ) A   Q L Y D ξ Q X D + Q L X D   Q L Y D ξ ,
Y D Q X D Q ξ = Q Y D D ( A ξ Q X D ) B Q ( Y D , A ξ Q X D ) A   Q L X D ξ Q Y D + Q L Y D   Q L X D ξ ,
[ X D , Y D ] Q ξ = [ X D , Y D ] D Q ξ + [ X D , Y D ] D Q ξ = A ξ Q ( [ X D , Y D ] D ) + Q L [ X D , Y D ] D ξ + π D [ X D , Y D ] D Q ξ + π D [ X D , Y D ] D Q ξ .
From (32)–(35), we obtain (31). □
Corollary 3. 
If U = 0 , then we have
R ( X D , Y D ) ξ D = B ( X D , A ξ Y D ) + B ( Y D , A ξ X D ) + R L ( X D , Y D ) ξ ,
where
R L ( X D , Y D ) ξ = L X D L Y D ξ L Y D L X D ξ L [ X D , Y D ] D ξ π D [ X D , Y D ] ξ .

4. Chen’s Inequalities for Non-Integrable Distributions with QSNMC

In the following, we prove Chen’s inequalities with respect to D and Q . For X , Y Γ ( T M ) , we let
α ( X , Y ) = ( X ω ) ( Y ) 1 4 ω ( A X ) ω ( Y ) + 1 4 ω ( X ) ω ( A Y ) ,
where ( X ω ) ( Y ) = X ( ω ( Y ) ) ω ( X Y ) . We have
R Q ( X , Y , Z , W ) = R ( X , Y , Z , W ) + α ( X , Z ) g ( A Y , W ) α ( Y , Z ) g ( A X , W ) + 1 2 ω ( Z ) g ( ( X A ) Y , W ) 1 2 ω ( Z ) g ( ( Y A ) X , W ) + 1 2 ω ( X ) g ( ( Y A ) Z , W ) 1 2 ω ( Y ) g ( ( X A ) Z , W ) + ( Y W ) ( X ) g ( A Z , W ) ( X W ) ( Y ) g ( A Z , W ) ) + 1 4 ω ( Y ) ω ( Z ) g ( A A X , W ) 1 4 ω ( X ) ω ( Z ) g ( A A Y , W ) .
In M, we can choose a local orthonormal frame E 1 , . . . , E n , E n + 1 , . . . , E m , such that E 1 , . . . , E n are orthonormal frames of D. And, we let λ = j = 1 n α ( E j , E j ) and h i j r = Q h i j r = g ( B ( E i , E j ) , E r ) for 1 i , j n and n + 1 r m .
The squared length of B is B 2 = B Q 2 = i , j = 1 n g ( B ( E i , E j ) , B ( E i , E j ) ) . Let M be an m-dimensional real space form of constant sectional curvature c endowed with a quarter-symmetric non-metric connection Q . The curvature tensor R with respect to the Levi-Civita connection on M is expressed by
R ( X , Y , Z , W ) = c { g ( X , W ) g ( Y , Z ) g ( X , Z ) g ( Y , W ) } .
By (38) and (39), we obtain
R Q ( X , Y , Z , W ) = c { g ( X , W ) g ( Y , Z ) g ( X , Z ) g ( Y , W ) } + α ( X , Z ) g ( A Y , W ) α ( Y , Z ) g ( A X , W ) + 1 2 ω ( Z ) g ( ( X A ) Y , W ) 1 2 ω ( Z ) g ( ( Y A ) X , W ) + 1 2 ω ( X ) g ( ( Y A ) Z , W ) 1 2 ω ( Y ) g ( ( X A ) Z , W ) + ( Y W ) ( X ) g ( A Z , W ) ( X W ) ( Y ) g ( A Z , W ) ) + 1 4 ω ( Y ) ω ( Z ) g ( A A X , W ) 1 4 ω ( X ) ω ( Z ) g ( A A Y , W ) .
Let Π D , be a two-plane section. The sectional curvature of   Q K D ( Π ) with respect to D and   Q D is defined by
  Q K D ( Π ) = 1 2 [ Q R D ( E 1 , E 2 , E 2 , E 1 ) Q R D ( E 1 , E 2 , E 1 , E 2 ) ] ,
where E 1 , E 2 are orthonormal basis of Π and   Q K D ( Π ) is independent of the choice of E 1 , E 2 . For any orthonormal basis E 1 , . . . , E n of D, denote by   Q τ D the scalar curvature of D with respect to   Q D , defined by
  Q τ D = 1 2 1 i , j n   Q R D ( E i , E j , E j , E i ) .
By Theorem 2, we have
R Q ( X D , Y D , Z D , W D ) =   Q R D ( X D , Y D , Z D , W D ) g ( B ( X D , W D ) , B ( Y D , Z D ) ) + g ( B ( Y D , W D ) , B ( X D , Z D ) ) + g ( Y D , Z D ) ω ( B ( X D , W D ) ) g ( X D , Z D ) ω ( B ( Y D , W D ) ) + 1 2 g ( A X D , W D ) ω ( B ( Y D , Z D ) ) 1 2 g ( A Y D , W D ) ω ( B ( X D , Z D ) ) + g ( B ( Z D , W D ) , [ X D , Y D ] ) + 1 2 ω ( [ X D , Y D ] D ) g ( A Z D , W D ) .
Let E 1 , E 2 be the orthonormal basis of Π D , and we have the following definition.
i = 1 n F ( E i , E i ) = μ , tr ( B | Π ) = B ( E 1 , E 1 ) + B ( E 2 , E 2 ) , A D = 1 2 1 i , j n g ( B ( E j , E i ) , [ E j , E i ] ) , Ω Π = 1 2 α ( E 1 , E 2 ) F ( E 2 , E 1 ) + 1 2 α ( E 2 , E 2 ) F ( E 1 , E 1 ) + 1 2 α ( E 1 , E 1 ) F ( E 2 , E 2 ) 1 2 α ( E 2 , E 1 ) F ( E 1 , E 2 ) 1 2 g ( B ( E 1 , E 2 ) B ( E 2 , E 1 ) , [ E 1 , E 2 ] ) , C 1 = 1 4 [ 3 j g ( ω ( E 1 ) ( E j A ) E j ω ( E j ) ( E j A ) E 1 , E 1 ) + 3 i g ( ω ( E i ) ( E 1 A ) E 1 ω ( E 1 ) ( E 1 A ) E i , E i ) + 2 i j n g ( ω ( E i ) ( E j A ) E j ω ( E j ) ( E j A ) E i , E i ) ] , C 2 = 1 2 [ 3 j F ( E j , E 1 ) [ ( E j ω ) ( E 1 ) ( E 1 ω ) ( E j ) ] + 3 i F ( E 1 , E i ) [ ( E 1 ω ) ( E i ) ( E i ω ) ( E 1 ) ] + 2 i j n F ( E j , E i ) [ ( E j ω ) ( E i ) ( E i ω ) ( E j ) ] ] , C 3 = 1 8 [ 3 j ω ( E j ) F ( A E 1 ω ( E j ) A E j ω ( E 1 ) , E 1 ) + 3 i ω ( E 1 ) F ( A E i ω ( E 1 ) A E 1 ω ( E i ) , E i ) + 2 i j n ω ( E j ) F ( A E i ω ( E j ) A E j ω ( E i ) , E i ) ] , C 4 = 1 4 [ 3 j F ( ω ( B ( E 1 , E j ) ) E j ω ( B ( E j , E j ) ) E 1 , E 1 ) + 3 i F ( ω ( B ( E i , E 1 ) ) E 1 ω ( B ( E 1 , E 1 ) ) E i , E i ) + 2 i j n F ( ω ( B ( E i , E j ) ) E j ω ( B ( E j , E j ) ) E i , E i ) , C 5 = 1 4 [ 3 j ω ( [ E 1 , E j ] D ) F ( E j , E 1 ) + 2 i n , 1 j n ω ( [ E i , E j ] D ) F ( E j , E i ) ] 1 4 3 j ω ( [ E 1 , E 2 ] D ) F ( E 1 , E 2 ) .
Then, A D and Ω Π are independent of the choice of the orthonormal basis. Let H Q 2 = g ( H Q , H Q ) . For the distribution D of the real space form M endowed with Q , we establish the following inequality called Chen’s first inequality.
Theorem 5. 
Let T M = D D , d i m D = n 3 , and M is a manifold with a constant sectional curvature c and a connection Q , then
  Q τ D Q K D ( Π ) ( n + 1 ) ( n 2 ) 2 c + 1 2 1 i j n n α ( E i , E j ) F ( E j , E i ) n 1 2 λ μ n ( n 1 ) 2 ω ( H ) + 1 4 g ( t r ( B | Π ) , P ) A D + Ω Π + C 1 + C 2 + C 3 + C 4 + C 5 + n 2 ( n 2 ) 2 ( n 1 ) H 2 + 1 2 | | B | | 2 .
Proof. 
Let E 1 , . . . , E n and E n + 1 , . . . , E m be orthonormal basis of D and D , respectively. Let E 1 , E 2 be the orthonormal basis of Π D . By (40), (41) and (43), we obtain
  Q K D ( Π ) = c Ω Π 1 4 g ( t r ( B | Π ) , P ) + r = n + 1 m [ h 11 r h 22 r h 12 r h 21 r ] + 1 4 g ( ω ( E 1 ) ( E 2 A ) E 2 ω ( E 2 ) ( E 2 A ) E 1 , E 1 + 1 4 g ( ω ( E 2 ) ( E 1 A ) E 1 ω ( E 1 ) ( E 1 A ) E 2 , E 2 + 1 2 F ( E 2 , E 1 ) [ ( E 2 ω ) ( E 1 ) ( E 1 ω ) ( E 2 ) ] + 1 2 F ( E 2 , E 1 ) [ ( E 2 ω ) ( E 1 ) ( E 1 ω ) ( E 2 ) ] + 1 2 F ( E 1 , E 2 ) [ ( E 1 ω ) ( E 2 ) ( E 2 ω ) ( E 1 ) ] + 1 8 ω ( E 2 ) F ( A E 1 ω ( E 2 ) A E 2 ω ( E 1 ) , E 1 ) + 1 8 ω ( E 1 ) F ( A E 2 ω ( E 1 ) A E 1 ω ( E 2 ) , E 2 ) + 1 4 F ( ω ( B ( E 1 , E 2 ) ) E 2 ω ( B ( E 2 , E 2 ) ) E 1 , E 1 ) + 1 4 F ( ω ( B ( E 2 , E 1 ) ) E 1 ω ( B ( E 1 , E 1 ) ) E 2 , E 2 ) + 1 4 ω ( [ E 1 , E 2 ] D ) F [ ( E 1 , E 2 ) F ( E 2 , E 1 ) ] .
Similarly, we obtain
  Q τ D = 1 2 1 i j n   Q R D ( E i , E j , E j , E i ) = n ( n 1 ) 2 c + 1 2 1 i j n n α ( E i , E j ) F ( E j , E i ) n 1 2 λ μ A D + r = n + 1 m 1 i < j n [ h i i r h j j r h i j r h j i r ] n ( n 1 ) 2 ω ( H ) + 1 4 1 i j n g ( ω ( E i ) ( E j A ) E j ω ( E j ) ( E j A ) E i , E 1 + 1 2 1 i j n F ( E j , E i ) [ ( E j ω ) ( E i ) ( E i ω ) ( E j ) ] + 1 8 1 i j n ω ( E j ) F ( A E i ω ( E j ) A E j ω ( E i ) , E i ) + 1 4 1 i j n F ( ω ( B ( E i , E j ) ) E j ω ( B ( E j , E j ) ) E i , E i ) 1 4 1 i j n ω ( [ E i , E j ] D ) F ( E j , E i ) .
So,
  Q τ D Q K D ( Π ) ( n + 1 ) ( n 2 ) 2 c + 1 2 1 i j n n α ( E i , E j ) F ( E j , E i ) n 1 2 λ μ n ( n 1 ) 2 ω ( H ) + 1 4 g ( t r ( B | Π ) , P ) A D + Ω Π + C 1 + C 2 + C 3 + C 4 + C 5 + r = n + 1 m [ ( h 11 r + h 22 r ) 3 j n h j j r + 3 i < j n h i i r h j j r 1 i < j n h i j r h j i r + h 12 r h 21 r ] .
By Lemma 2.4 in [17], we obtain
r = n + 1 m [ ( h 11 r + h 22 r ) 3 j n h j j r + 3 i < j n h i i r h j j r ] n 2 ( n 2 ) 2 ( n 1 ) H 2 .
We note that
r = n + 1 m 1 i < j n h i j r h j i r + h 12 r h 21 r = r = n + 1 m 3 j n h 1 j r h j 1 r 2 i < j n h i j r h j i r r = n + 1 m 3 j n ( h 1 j r ) 2 + ( h j 1 r ) 2 2 + 2 i < j n ( h i j r ) 2 + ( h j i r ) 2 2 r = n + 1 m 3 j n ( h 1 j r ) 2 + ( h j 1 r ) 2 2 + 2 i < j n ( h i j r ) 2 + ( h j i r ) 2 2 + i = 1 n ( h i i r ) 2 2 + ( h 12 r ) 2 + ( h 21 r ) 2 2 = B 2 2 .
By (48)–(50), we obtain (45).
Corollary 4. 
The equality case of (45) holds if and only if D is totally geodesic with respect to Q and h 12 r = h 21 r = 0 .
Proof. 
The equality case of (50) holds if and only if h i i r = 0 , for 1 i n , h 12 r = h 21 r = 0 and h 1 j r = h j 1 r for 3 j n and h k l r = h l k r for 2 k < l n .
The equality case of (49) holds if and only if h 11 r + h 22 r = h i i r for 3 i n . So, Corollary 4 is proven. □
For each unit vector field X D Γ ( D ) , we choose the orthonormal basis E 1 , . . . , E n of D, such that E 1 = X D . We define
  Q Ric D ( X D ) = j = 2 n   Q R D ( X D , E j , E j , X D ) , A D ( X D ) = j = 2 n g ( B ( E j , X D ) , [ E j , X D ] ) , B X D 2 = i = 2 n [ g ( B ( X D , E j ) , B ( X D , E j ) ) + g ( B ( E j , X D ) , B ( E j , X D ) ) ] .
Theorem 6. 
Let T M = D D , dim D = n 2 , and M is a manifold with a constant sectional curvature c and a connection Q , then
  Q Ric D ( X D ) ( n 1 ) c λ F ( X D , X D ) + α ( X D , X D ) F ( X D , X D ) n ω ( H ) + ω ( B ( X D , X D ) ) A D ( X D ) + 1 2 j = 2 n g ( ω ( X D ) ( E j A ) E j ω ( E j ) ( E j A ) X D , X D ) + j = 2 n ( E j ω ) ( X ) F ( E j , X D ) ( X ω ) ( E j ) F ( E j , X D ) + 1 4 j = 2 n ω ( E j ) F ( ω ( E j ) A X D ω ( X ) A E j , X D ) + 1 2 j = 2 n F ( ω ( B ( X D , E j ) ) E j ω ( B ( E j , E j ) ) X D , X D ) . 1 2 j = 2 n ω ( [ X D , E j ] D F ( E j , X D ) ) + n 2 4 H 2 + B X D 2 2 .
Proof. 
By (40), (41) and (43), we have
  Q Ric D ( X D ) ( n 1 ) c λ F ( X D , X D ) + α ( X D , X D ) F ( X D , X D ) n ω ( H ) + ω ( B ( X D , X D ) ) A D ( X D ) + 1 2 j = 2 n g ( ω ( X D ) ( E j A ) E j ω ( E j ) ( E j A ) X D , X D ) + j = 2 n ( E j ω ) ( X D ) F ( E j , X D ) ( X D ω ) ( E j ) F ( E j , X D ) + 1 4 j = 2 n ω ( E j ) F ( ω ( E j ) A X D ω ( X D ) A E j , X D ) + 1 2 j = 2 n F ( ω ( B ( X D , E j ) ) E j ω ( B ( E j , E j ) ) X D , X D ) . 1 2 j = 2 n ω ( [ X D , E j ] D F ( E j , X D ) ) + r = n + 1 m j = 2 n [ h 11 r h j j r h 1 j r h j 1 r ] .
By Lemma 2.5 in [17], we obtain
r = n + 1 n + p j = 2 n h 11 r h j j r n 2 4 H 2 .
We note that
r = n + 1 m j = 2 n h 1 j r h j 1 r r = n + 1 m j = 2 n ( h 1 j r ) 2 + ( h j 1 r ) 2 2 = B X D 2 2 .
By (53)–(55), we obtain (52). □
Corollary 5. 
The equality case of (51) holds if and only if h 1 j r = h j 1 r for 2 j n and h 11 r h 22 r . . . h n n r = 0 .

5. Examples

In this section, two examples, namely the Heisenberg group ( H 3 , g H 3 ) and the three-dimensional unit sphere S 3 of non-integrable distributions in a Riemannian manifold with quarter-symmetric non-metric connections, follow.
Example 1. 
Let ( H 3 , g H 3 ) be the Heisenberg group H 3 endowed with the Riemannian metric g, which has an orthonormal basis X 1 , X 2 , X 3 , satisfy the commutation relations
[ X 1 , X 2 ] = X 3 , [ X 1 , X 3 ] = 0 , [ X 2 , X 3 ] = 0 .
Letbe the Levi-Civita connection on H 3 . By (56) and the Koszul formula, we have
X j X j = 0 , 1 j 3 , X 1 X 2 = 1 2 X 3 , X 2 X 1 = 1 2 X 3 , X 1 X 3 = X 3 X 1 = 1 2 X 2 , X 2 X 3 = X 3 X 2 = 1 2 X 1 .
Consider the distribution D = s p a n { X 1 D , X 2 D } , which is not integrable by (56). The metric of D is induced by the metric on H 3 . Let U = X 1 D + X 2 D + X 3 D . By (57), we have
X i D D X j D = 0 , i , j = 1 , 2 , B ( X 1 D , X 1 D ) = B ( X 2 D , X 2 D ) = 0 , B ( X 1 D , X 2 D ) = 1 2 X 3 D , B ( X 2 D , X 1 D ) = 1 2 X 3 D .
By (9), we obtain
  Q X D D Y D = X D D Y D + 1 2 g ( X 1 D + X 2 D , Y D ) A X D 1 2 g ( X 1 D + X 2 D , X D ) A Y D , B Q ( X D , Y D ) = B ( X D , Y D ) .
And let A X 1 D = X 1 D , A X 2 D = X 2 D , A X 3 D = X 3 D . We have
  Q X 1 D D X 1 D = 0 ,   Q X 1 D D X 2 D = 1 2 X 1 D + 1 2 X 2 D ,   Q X 2 D D X 1 D = 1 2 X 1 D 1 2 X 2 D ,   Q X 2 D D X 2 D = 0 B Q ( X 1 D , X 1 D ) = 0 , B Q ( X 1 D , X 2 D ) = 1 2 X 3 D , B Q ( X 2 D , X 1 D ) = 1 2 X 3 D , B Q ( X 2 D , X 2 D ) = 0 , H Q = 0 .
By (17), (41), (42) and (62), we have
  Q R D ( X 1 D , X 2 D ) X 1 D = 1 4 X 1 D 1 4 X 2 D ,   Q R D ( X 1 D , X 2 D ) X 2 D = 1 4 X 1 D 1 4 X 2 D ,   Q K D ( D ) = 0 ,   Q τ D = 0 .
Example 2. 
Consider the three-dimensional unit sphere S 3 as a Riemannian manifold endowed with the metric induced from R 4 . The tangent space of S 3 at each point has an orthonormal basis e 1 , e 2 , e 3 , which satisfies
[ e 1 , e 2 ] = 2 e 3 , [ e 1 , e 3 ] = 2 e 2 , [ e 2 , e 3 ] = 2 e 1 .
The Levi-Civita connectionof S 3 is given by
e 1 e 2 = e 3 , e 2 e 1 = e 3 , e 1 e 1 = e 2 e 2 = e 3 e 3 = 0 , e 1 e 3 = e 2 , e 3 e 1 = e 2 , e 2 e 3 = e 1 , e 3 e 2 = e 1 .
Let D 1 = s p a n { e 1 D 1 , e 2 D 1 } , by (63), then e i D 1 D 1 e j D 1 = 0 , i , j = 1 , 2 . Let U = e 1 D 1 + e 3 D 1 , A e 1 D 1 = e 1 D 1 , A e 2 D 1 = e 2 D 1 , A e 3 D 1 = e 3 D 1 , then
  Q e 1 D D 1 e 1 D 1 = 0 ,   Q e 1 D D 1 e 2 D 1 = 1 2 e 2 D 1 ,   Q e 2 D 1 D 1 e 1 D 1 = 1 2 e 2 D 1 ,   Q e 2 D 1 D 1 e 2 D 1 = 0 B Q ( e 1 D 1 , e 1 D 1 ) = 0 , B Q ( e 1 D 1 , e 2 D 1 ) = e 3 D 1 , B Q ( e 2 D 1 , e 1 D 1 ) = e 3 D 1 , B Q ( e 2 D 1 , e 2 D 1 ) = 0 , H Q = 0 .   Q R D 1 ( e 1 D 1 , e 2 D 1 ) e 1 D 1 = 4 e 2 D 1 ,   Q R D 1 ( e 1 D 1 , e 2 D 1 ) e 2 D 1 = 4 e 1 D 1 ,   Q K D 1 ( D 1 ) = 4 ,   Q τ D 1 = 4 .

6. Conclusions

This paper proved the Gauss, Codazzi and Ricci equations for non-integrable distributions with respect to a quarter-symmetric non-metric connection. As applications, we deduced Chen’s inequalities for non-integrable distributions of real space forms with a quarter-symmetric metric connection and a quarter-symmetric non-metric connection.
For further work, it would be interesting to research the various affine connection of non-integrable distributions and deal with the applications of the results obtained in the paper. Also, many inequalities of a similar type will be possibly established for different kinds of submanifolds in various ambient manifolds [18].

Author Contributions

All of the authors contributed equally to the writing of this manuscript. These authors contributed to the work equally and should be regarded as co-first authors. All authors have read and agreed to the published version of the manuscript.

Funding

This research was supported by the Project of Science and Technology of Heilongjiang Provincial Education Department (Grant No. 1453ZD019), and the Reform and Development Foundation for Local Colleges and Universities of the Central Government (Grant No. ZYQN2019071).

Data Availability Statement

No data were used to support this study.

Acknowledgments

The authors would like to thank the reviewers for their careful reading and useful comments.

Conflicts of Interest

The authors declare that there are no conflicts of interests in this work.

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Chen, S.; Liu, H. Quarter-Symmetric Non-Metric Connection of Non-Integrable Distributions. Symmetry 2024, 16, 848. https://doi.org/10.3390/sym16070848

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Chen S, Liu H. Quarter-Symmetric Non-Metric Connection of Non-Integrable Distributions. Symmetry. 2024; 16(7):848. https://doi.org/10.3390/sym16070848

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Chen, Shuo, and Haiming Liu. 2024. "Quarter-Symmetric Non-Metric Connection of Non-Integrable Distributions" Symmetry 16, no. 7: 848. https://doi.org/10.3390/sym16070848

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