1. Introduction
Nearly Kähler geometry arises as a natural generalization of Kähler geometry and has garnered significant attention due to its deep connections with differential geometry, complex geometry, and theoretical physics. Among the most remarkable examples of such structures is the 6-dimensional unit sphere
, which serves as a canonical example of a strictly nearly Kähler manifold that is not Kähler. The nearly Kähler structure on
originates from its immersion in
, viewed as a space of purely imaginary Cayley numbers (octonions). This endows
with a natural almost complex structure
J, defined through the vector cross product in
, such that the condition
holds for every vector field
X on
. The metric
g is the standard round metric induced by the Euclidean metric on
.
The geometric significance of
as a nearly Kähler manifold lies in the fact that, while its almost complex structure
J is not integrable (hence,
is not a complex manifold), it still satisfies certain symmetries and curvature properties that resemble those of Kähler manifolds. These properties make
an ideal setting for studying submanifolds with interesting geometric behavior, particularly those that interact in subtle ways with the ambient nearly Kähler structure [
1].
Gray’s seminal work [
2] showed that there exist no complex hypersurfaces in
, which distinguishes the geometry of
from classical Kähler manifolds [
3,
4]. This nonexistence result paved the way for studying alternative classes of submanifolds such as totally real submanifolds, CR-submanifolds, and almost contact hypersurfaces [
5]. In particular, CR-submanifolds of
have been studied extensively in the literature [
6,
7], where 4-dimensional CR-submanifolds were shown to exhibit rich geometry influenced by the ambient nearly Kähler structure. Furthermore, totally real submanifolds of dimensions 2 and 3 have been analyzed in depth in several works [
8,
9,
10,
11], where the absence of complex directions plays a central role in determining their curvature and topological properties. For further classification and information on the properties of such totally real submanifolds, we refer the reader to [
12,
13,
14].
While much attention has been paid to CR and totally real submanifolds, hypersurfaces of
have emerged as an equally important class, especially due to their intrinsic and extrinsic geometric characteristics. Hypersurfaces of
naturally inherit an almost contact metric structure induced by the nearly Kähler structure of the ambient space. Several authors have contributed to the study of such hypersurfaces [
6,
15,
16,
17], focusing on their curvature properties, the behavior of the characteristic vector field
, and conditions for minimality and contact geometry. A one-parameter family of totally umbilical hypersurfaces in
is also discussed in [
16,
18,
19].
Two-dimensional submanifolds in
have also been studied, notably by Berndt et al. [
20], who analyzed almost complex curves and showed that their intrinsic geometry shares similarities with that of Hopf hypersurfaces. These curves serve as lower-dimensional analogs of more complex structures and provide important insight into the role of
J-invariant subspaces. Additional contributions to this subject are found in [
21,
22,
23], where the authors explored properties of almost complex and minimal surfaces within this framework. In particular, ref. [
22] links the study of such surfaces to the affine Toda field model.
More recently, Deshmukh and collaborators have investigated hypersurfaces in nearly Kähler manifolds under various curvature constraints. In [
15], Deshmukh characterized Hopf hypersurfaces of
by examining the behavior of the characteristic vector field and imposing suitable geometric conditions. In [
17], Deshmukh and Al-Dayel extended this study by introducing nearly Sasakian and nearly cosymplectic structures on hypersurfaces of
, thereby enriching the class of admissible geometric structures and providing a broader context for understanding submanifolds of nearly Kähler spaces.
Moreover, hypersurfaces in other nearly Kähler settings, such as
, have been considered. In [
24], the authors investigated contact and minimal hypersurfaces with conformal vector fields in such product manifolds. These studies not only deepen our understanding of the interaction between curvature and topology, but also motivate the search for new examples and classifications of hypersurfaces in
with distinctive geometric features.
In light of the above developments, the aim of the present paper is to further explore the geometry of hypersurfaces in the nearly Kähler 6-sphere . In particular, we are interested in understanding how certain curvature conditions, expressed via the behavior of functions such as where and , can influence the global geometry of the hypersurface. We demonstrate, under suitable conditions on , that the hypersurface M of must be a standard sphere. These results contribute to the broader effort of classifying hypersurfaces in nearly Kähler manifolds and understanding their intrinsic and extrinsic geometries in the context of almost contact metric structures.
2. Some Basic Results
Let
be the nearly Kähler 6-sphere endowed with a nearly Kähler structure
, where
J is the almost complex structure and
is the associated almost Hermitian metric on
. Then the identities
hold for all
, where
denotes the Riemannian connection on
with respect to
g, and
is a tensor of the type
and has the properties given below:
Lemma 1 ([
15])
. For any , the tensor G satisfies- (a)
;
- (b)
;
- (c)
;
- (d)
;
- (e)
.
Let be an immersed hypersurface of the nearly Kähler manifold . We denote the covariant derivatives on M, , and as ∇, , and D, respectively. Let N and denote the unit vector fields normal to M and . Since , it follows that . We define the unit vector field as .
Let
be the 1-form dual to
, that is,
, for all
, so that
. Define the operator
as
the tangential component of
. Then,
and hence,
and
.
Now define and for any .
For an orientable hypersurface
M of
, the Gauss and Weingarten formulas are given by
for all
, where
A is the shape operator of
M. The Gauss and Codazzi equations for hypersurfaces are [
25]
where
.
The Ricci tensor Ric and scalar curvature
S of the hypersurface
M are given by
where
is the mean curvature, and
is the squared norm of the shape operator.
Lemma 2 ([
15])
. For any ,- (a)
;
- (b)
;
- (c)
.
Lemma 3. For any ,
- (a)
;
- (b)
.
Proof. From Equation (1), we compute
which proves part (a).
To prove part (b), we use the Gauss formula:
□
3. The Main Results
In this section, we present the main theoretical contributions of our study concerning hypersurfaces in the nearly Kähler 6-sphere . The results are derived under specific geometric and analytical conditions involving the smooth function , where , and is the characteristic vector field induced by the almost complex structure J and the unit normal N to the hypersurface M. These results provide sufficient conditions under which a compact hypersurface of can be characterized as a standard sphere. In particular, we demonstrate the existence of a smooth function h satisfying a certain Laplacian condition involving , and further establish a rigidity result under curvature constraints. The two main theorems are stated as follows:
Theorem 1. Let M be a compact hypersurface of . For any , there exists a function such thatwhere , and Δ
is the Laplacian operator. Theorem 2. Let M be a compact hypersurface of with positive curvature. Suppose there exists a smooth function such thatwhere s satisfies and on M. Then M is isometric to a standard sphere. To prove these theorems, we require the following technical lemma:
Lemma 4. Let . Then,
- (a)
;
- (b)
;
- (c)
.
Proof.
(a) Using the definition of the divergence and the properties of
with a local orthonormal frame
, we compute
(b) For the second identity,
(c) For the third identity, a more involved computation gives
□
It is also well known that for any vector field
, there exists a decomposition
where
satisfies
and
.
Proof of Theorem 1. Let
be any smooth function. Then
, and from the previous lemma, we have
where
.
Since the divergence of a vector field can be represented as the Laplacian of a potential function plus a divergence-free component, there exist a vector field
and a smooth function
such that
Taking the divergence of both sides gives
Thus, we obtain
which completes the proof. □
Proof of Theorem 2. Let
such that
. Then, according to Bochner’s formula, we have
where
for any
.
This can be rearranged as
Now, suppose the Ricci curvature satisfies the bounds
for constants
. Then,
which implies that
Assume that the condition
holds on
M. Then the integrand is non-negative, and so the entire integral must be zero. Therefore,
From the second equality, we obtain
. Substituting this into the first, we get
i.e., the shape operator is proportional to the identity.
Since M has positive curvature, this implies that the hypersurface is totally umbilical and satisfies for some constant . Thus, M is isometric to the standard sphere for some constant . □
Example 1 (Geodesic Hypersphere as a Hypersurface in the Nearly Kähler ).
Let denote the standard 6-dimensional unit sphere endowed with the nearly Kähler structure , where J is the canonical almost complex structure on . We construct a family of real hypersurfaces in by intersecting it with the hyperplane , where is a fixed real number.
Then is a 5-dimensional submanifold of , sinceand thus, Each is a compact, connected, real hypersurface in , often referred to as a geodesic hypersphere centered at the pole in the -direction.
Further, we notice that is a totally umbilical hypersurface in , and its shape operator A satisfieswhere I is the identity transformation in the tangent space. The mean curvature of is given byIn particular, is minimal if and only if , corresponding to the equatorial hypersphere. The unit normal vector field ν of satisfies . Since , where λ is a constant, the structure vector field ξ is a principal direction. Therefore, is a Hopf hypersurface
in the nearly Kähler [25]. Example 2 (Explicit Example for Theorem 1).
Consider the nearly Kähler 6-sphere , equipped with the standard metric g and the nearly Kähler structure J induced from the octonionic cross product. Define the compact hypersurfacei.e., the equatorial 5-sphere. M is totally geodesic in and inherits a Riemannian metric from . Let us define a smooth function as We now construct a function such that .
On the round sphere , the Laplacian of a coordinate function is well known:We aim to solve Assume, for simplicity, that at each point , the structure vector field is given by a fixed linear combination of the frame vectors:where and (since ξ is a unit vector). Thenand we set Thenprovided satisfies . One such choice is , since is an eigenfunction of the Laplacian on with eigenvalue . So we set the following: Thensince , , and . Hence, the constructed functionis a smooth function on that satisfies the required conditionverifying Theorem 1 concretely. 4. Conclusions and Future Work
In this paper, we have explored the geometry of hypersurfaces in the nearly Kähler 6-sphere , focusing particularly on the behavior of the function , where is the characteristic vector field. By analyzing conditions under which the Laplacian of a related scalar function leads to geometric rigidity, we have shown that certain hypersurfaces must necessarily be standard spheres. These results contribute to the broader understanding of submanifold theory in nearly Kähler geometry and provide new insights into the interplay between curvature, complex structures, and scalar function behavior.
As directions for future research, one could consider extending these results to other classes of almost Hermitian manifolds, particularly those with torsion or weaker integrability conditions. Another promising direction is to study the influence of additional geometric structures, such as conformal or CR-structures, on the rigidity of hypersurfaces. Moreover, examining the behavior of
and related Laplace-type equations under various curve [
26,
27] and curvature constraints may yield further classification results or pave the way to applications in geometric analysis and mathematical physics.