We use the tangential component ψT of an immersion of a compact hypersurface of the Euclidean space Em+1 in finding two characterizations of a sphere. In first characterization, we use ψT as a geodesic vector field (vector field with all its trajectories geodesics) and in the second characterization, we use ψT to annihilate the de-Rham Laplace operator on the hypersurface.
Citation: Sharief Deshmukh, Mohammed Guediri. Characterizations of Euclidean spheres[J]. AIMS Mathematics, 2021, 6(7): 7733-7740. doi: 10.3934/math.2021449
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We use the tangential component ψT of an immersion of a compact hypersurface of the Euclidean space Em+1 in finding two characterizations of a sphere. In first characterization, we use ψT as a geodesic vector field (vector field with all its trajectories geodesics) and in the second characterization, we use ψT to annihilate the de-Rham Laplace operator on the hypersurface.
Geometry of hypersurfaces of a Riemannian manifold is one of the important branches of differential geometry. In that, one of important questions is characterizing spheres among compact hypersurfaces of a Euclidean space [1,3,4,5,6,7,8]. On a Riemannian manifold (M,g), the Ricci operator S is defined using Ricci tensor Ric, namely Ric(X,Y)=g(SX,Y), X∈X(M), where X(M) is the Lie algebra of smooth vector fields on M. Similarly, the rough Laplace operator on the Riemannian manifold (M,g), Δ: X(M)→X(M) is defined by
ΔX=m∑i=1(∇ei∇eiX−∇∇eieiX), X∈X(M), | (1.1) |
where ∇ is the Riemannian connection and {e1,...,em} is a local orthonormal frame on M, m=dimM. Rough Laplace operator is used in finding characterizations of spheres as well as of Euclidean spaces [11,12]. Recall that de-Rham Laplace operator ◻: X(M)→X(M) on a Riemannian manifold (M,g) is defined by ([10], p83)
◻=S+Δ | (1.2) |
and is used to characterize a Killing vector field on a compact Riemannian manifold. Recall that a vector field u on a Riemannian manifold (M,g) is said to be a geodesic vector field [9] if
∇uu=0. | (1.3) |
Let M be an orientable immersed hypersurface of the Euclidean space and ψ:M→Em+1 be the immersion. We denote the unit normal to the hypersurface M by ξ and support function of the hypersurface by σ defined by σ=⟨ψ,ξ⟩, where ⟨,⟩ is the Euclidean metric on Em+1. Then treating ψ as position vector field of the hypersurface M, we have ψ=ψT+σξ.
Consider the sphere Sm(c) of constant curvature c as hypersurface of the Euclidean space Em+1 with unit normal ξ and shape operator A=−√cI. Now, consider the embedding ψ:Sm(c)→Em+1. Then it follows that the tangential component ψT for the sphere Sm(c) satisfies ◻ψT=0 as well as ψT is a geodesic vector field. These raise two questions: (i) Under what condition on a compact hypersurface M of a Euclidean space Em+1 with immersion ψ:M→Em+1 such that ψT is a geodesic vector field, M is isometric to a sphere? (ii) Under what conditions on a compact hypersurface M of a Euclidean space Em+1 with immersion ψ:M→Em+1 such that ψT satisfying ◻ψT=0, M is isometric to a sphere? In this paper, we answer these questions, for first question by showing that under the condition Ric(ψT,ψT)≥m−1m(div ψT)2 the hypersurface is isometric to a sphere, where as for the second question, it requires the condition |σα|≤1, where α is the mean curvature (Theorem 3.1 and Theorem 3.2).
Let M be an orientable immersed hypersurface of of the Euclidean space Em+1 with immersion ψ:M→Em+1 with unit normal ξ and shape operator A. Then we have the following Gauss-Weingarten formulae
DXY=∇XY+g(AX,Y)ξ, DXξ=−AX , X,Y∈X(M), | (2.1) |
where D, ∇ are Riemannian connections on Em+1, M respectively, g is the induced metric on M and X(M) is the Lie algebra of smooth vector fields on M. The curvature tensor field R and the Ricci curvature Ric of the hypersurface are given by
R(X,Y)Z=g(AY,Z)AX−g(AX,X)AY, X,Y,Z∈X(M) | (2.2) |
and
Ric(X,Y)=mαg(AX,Y)−g(AX,AY), X,Y∈X(M), | (2.3) |
where, α=1mTr.A is the mean curvature of the hypersurface [2]. Using Eq (2.3), we see that the Ricci operator S of the hypersurface M is given by
S(X)=mαAX−A2X, X∈X(M) | (2.4) |
Also, as the Euclidean space Em+1 is space of constant curvature, the Codazzi equation for the hypersurface M is
(∇A)(X,Y)=(∇A)(Y,X), X,Y∈X(M), | (2.5) |
where (∇A)(X,Y)=∇XAY−A(∇XY). Using Eq (2.5) and symmetry of the shape operator A, the gradient grad α of the mean curvature α is given by
grad α=1mm∑i=1(∇A)(ei,ei), | (2.6) |
where {e1,...en} is a local orthonormal frame on M.
Let ψT be the tangential component of the immersion ψ:M→Em+1 and σ=⟨ψ,ξ⟩ be the support function of the hypersurface M. Then, we have ψ=ψT+σξ and using Eq (2.1), we get
∇XψT=X+σAX, grad σ=−AψT, X∈X(M). | (2.7) |
Using above equation, we have
div ψT=m(1+σα). | (2.8) |
Thus, for a compact hypersurface M of the Euclidean space Em, on integrating the above equation, we have the following Minkowski's formula
∫M(1+σα)=0. | (2.9) |
On a compact Riemannian manifold (M,g), the Laplace operator Δ acting on a smooth function h:M→R is defined by Δh=div (grad h) and the Hessian operator Hh for the smooth function h is a symmetric operator defined by
Hh(X)=∇Xgrad h, X∈X(M). |
On a compact Riemannian manifold (M,g), we have the following formula known as Bochner's formula
∫MRic(grad h,grad h)=∫M((Δh)2−‖Hh‖2). | (2.10) |
On the other hand, given a Riemannian manifold (M,g) and a vector field X∈X(M), , we let θX denote the dual one form of X (that is, defined by θX(Y)=g(X,Y)) and AX be the (1,1)-tensor (viewed as an endomorphism) defined by
AX(Y)=∇YX |
Write as usual
LXg(Y,Z)+dθX(Y,Z)=2g(AX(Y),Z), |
for all Y,Z∈X(M).
Let B and ϕ be the symmetric and anti-symmetric parts of AX. In other words, we have
LXg(Y,Z)=2g(B(Y),Z)dθX(Y,Z)=2g(ϕ(Y),Z) |
Now, formula ∇XψT=X+σAX in Eq (2.7) is nothing but AψT=I+σA. It follows that B=I+σA and ϕ=0, and this implies that ψT is gradient.
Let M be an orientable compact immersed hypersurface of the Euclidean space Em+1 with immersion ψ:M→Em+1 and unit normal ξ, shape operator A. In this section, we answer the questions raised in the introduction and find two new characterizations of the Euclidean spheres.
Theorem 1. Let ψ:M→Em+1 be an immersion of a compact simply connected hypersurface with ψT a non-trivial geodesic vector field, m≥2. Then the Ricci curvature satisfies
Ric(ψT,ψT)≥m−1m(divψT)2, |
if and only if, the mean curvature α is a constant, ψT is a non-homothetic conformal vector field, and M is\ isometric to the sphere Sm(α2).
Proof. Suppose ψT is a geodesic vector field and the Ricci curvature of the hypersurface M satisfies
Ric(ψT,ψT)≥m−1m(div ψT)2. | (3.1) |
Then, using Eqs (1.3) and (2.7), we have σAψT=−ψT. Taking covariant derivative with respect to X∈X(M) in this equation and using Eq (2.7), we get
X(σ)AψT+σ(∇A)(X,ψT)+σA(X+σAX)=−X−σAX, |
that is
σ(∇A)(X,ψT)=−X(σ)AψT−X−2σAX−σ2A2X, X∈X(M). |
Now, for a local orthonormal frame {e1,...,em} on M, choosing X=ei in above equation and taking the inner product with ei in above equation and summing the resulting equation, we conclude
mσψT(α)=−g(AψT,grad σ)−m−2mσα−σ2‖A‖2, |
where we used symmetry of the shape operator A and Eq (2.6). Now, using Eq (2.7) in above equation, we have
mσψT(α)=‖AψT‖2−m−2mσα−σ2‖A‖2. | (3.2) |
Note that div (α(σψT))=σψT(α)+αdiv (σψT) and using Eqs (2.7), (2.8), we get
σψT(α)=div (α(σψT))+αg(AψT,ψT)−mσα(1+σα). | (3.3) |
Inserting the above equation in Eq (3.2) and using Eq (2.3), we conclude
Ric(ψT,ψT)−m2σα(1+σα)+div (α(σψT))=−m−2mσα−σ2‖A‖2. |
Integrating the above equation while using Minkowski's formula (2.9), we have
∫M(Ric(ψT,ψT)+m(m−1)−m2σ2α2+σ2‖A‖2)=0, |
that is,
∫M(Ric(ψT,ψT)−m(m−1)(σ2α2−1))=∫Mσ2(mα2−‖A‖2). | (3.4) |
Now, we use div ψT=m(1+σα) and Eq (2.9), to arrive at
∫M(div ψT)2=m2∫M(1+2σα+σ2α2)=m2∫M(σ2α2−1) |
and inserting the above equation in Eq (3.4), we have
∫M(Ric(ψT,ψT)−m−1m(div ψT)2)=∫Mσ2(mα2−‖A‖2). | (3.5) |
Using inequality (3.1) in Eq (3.5), we get
∫Mσ2(mα2−‖A‖2)≥0 |
and above inequality in view of the Schwart's inequality ‖A‖2≥mα2 implies
σ2(mα2−‖A‖2)=0. |
If σ=0, then by Minkowski's formula (2.9), we get a contradiction. Thus, we have ‖A‖2=mα2 and this equality holds, if and only if, A=αI. In other words, M is shown to be totally umbilical. Moreover, using A=αI, we have
(∇A)(X,Y)=X(α)Y, |
and we get
m∑i=1(∇A)(ei,ei)=grad α. |
Using Eq (2.6), we get (m−1)grad α=0 and with restriction on dimension m, we conclude α is a constant. Moreover, this constant α≠0 due to the fact that the Euclidean space does not have a compact minimal hypersurface. Inserting A=αI in Eq (2.2), we see that the simply connected hypersurface M has constant curvature α2 and M being compact, it is complete. Hence, M is complete simply connected hypersurface of constant positive curvature α2 and is therefore isometric to the sphere Sm(α2). Since B=(1+σα)I, we get LψTg=2(1+σα)g. In other words, ψT is a conformal vector field which is non-homothetic, given that the function 1+σα is not constant as ψT is supposed to be non-trivial. The converse is trivial as ψT for the natural embedding ψ: Sm(α2)→Em+1 has ψT=0, which satisfies the hypothesis of the Theorem.
Theorem 2. Let ψ:M→Em+1 be an immersion of a compact simply connected hypersurface with ◻ψT=0, m≥2. Then the mean curvature α and support function σ satisfies
|σα|≤1, |
if and only if, the mean curvature α is a constant, ψT is a parallel vector field (i.e., the covariant derivative of ψT vanishes), and M is isometric to the sphere Sm(α2).
Proof. Let M be a compact simply connected hypersurface of the Euclidean space Em+1 with ◻ψT=0, and
|σα|≤1. | (3.6) |
We use Eqs (2.6) and (2.7) in computing ΔψT, where Δ is rough Laplace operator, and obtain
ΔψT=A(grad σ)+mσgrad α. |
Using Eq (2.7), we get
ΔψT=−A2(ψT)+mσgrad α. | (3.7) |
Also, in view of Eq (2.4), we have
S(ψT)=mαA(ψT)−A2(ψT). | (3.8) |
Now, using Eqs (1.2), (3.7) and (3.8), we conclude
◻ψT=−2A2(ψT)+mαA(ψT)+mσgrad α |
and taking the inner product in above equation with ψT and using ◻ψT=0, we arrive at
mαg(AψT,ψT)−2g(AψT,AψT)+mσψT(α)=0. |
Using Eq (3.3), we conclude
2mαg(AψT,ψT)−2‖AψT‖2+mdiv (α(σψT))−m2σα(1+σα)=0 |
and in view of Eq (2.3), we get
2Ric(ψT,ψT)+mdiv (α(σψT))−m2σα(1+σα)=0. |
Integrating the above equation, while using Eq (2.9), we get
∫M(2Ric(ψT,ψT)+m2−m2σ2α2)=0. | (3.9) |
Define a smooth function h on the hypersurface M, by h=12‖ψ‖2, which has gradient grad h=ψT and Δh=m(1+σα). Also using Eq (2.7), the Hessian Hh is given by
Hh=I+σA. | (3.10) |
Thus, using Bochner's formula (2.10), we have
∫MRic(ψT,ψT)=∫M((Δh)2−‖Hh‖2)=∫M(1m(Δh)2−‖Hh‖2+m−1m(Δh)2). |
Inserting Δh=m(1+σα) in the last term of the right hand side of above equation, we have
∫M(1m(Δh)2−‖Hh‖2)=∫M(Ric(ψT,ψT)−m(m−1)(1+σα)2) |
and using Eq (2.9), we get
2∫M(1m(Δh)2−‖Hh‖2)=∫M(2Ric(ψT,ψT)−2m(m−1)(σ2α2−1)). | (3.11) |
Combining Eqs (3.9) and (3.11), we arrive at
2∫M(1m(Δh)2−‖Hh‖2)=m(m−2)∫M(1−σ2α2). |
Using Schwarz' inequality ‖Hh‖2≥1m(Δh)2 and inequality (3.6) with m≥2, in above equation, we conclude the equality ‖Hh‖2=1m(Δh)2 and this equality holds, if and only if
Hh=ΔhmI. |
Now, using Eq (3.10) and Δh=m(1+σα) in above equation, we get
σ(A−αI)=0. |
If σ=0, we get a contradiction by Eq (2.9). Thus, we get A=αI and following the proof of Theorem 3.1, we get M is isometric to the sphere Sn(α2). We also deduce that LψTg=2(1+σα)g, with both σ and α constants. It follows that 1+σα=0, since otherwise ψT becomes a homothetic vector field and consequently M is isometric to the Euclidean space, a contradiction. Thus, ∇X=AψT=0, that is ψT is parallel. The converse is trivial as on Sm(α2) as hypersurface of the Euclidean space Em+1, we have ψT=0 and σ=−1α, and |σα|=1.
This work was supported by NSTIP strategic technologies program number (13-MAT874-02) in the Kingdom of Saudi Arabia.
The authors declare that there is no conflict of interest.
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