Research article

Characterizations of Euclidean spheres

  • Received: 22 March 2021 Accepted: 10 May 2021 Published: 14 May 2021
  • MSC : 53C20, 53A30

  • 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), XX(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=mi=1(eieiXeieiX)XX(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:MEm+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:MEm+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:MEm+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)m1m(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:MEm+1 with unit normal ξ and shape operator A. Then we have the following Gauss-Weingarten formulae

    DXY=XY+g(AX,Y)ξDXξ=AX , X,YX(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)AXg(AX,X)AYX,Y,ZX(M) (2.2)

    and

    Ric(X,Y)=mαg(AX,Y)g(AX,AY)X,YX(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)=mαAXA2XXX(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,YX(M) (2.5)

    where (A)(X,Y)=XAYA(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=1mmi=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:MEm+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+σAXgrad σ=AψTXX(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:MR 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 hXX(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)2Hh2). (2.10)

    On the other hand, given a Riemannian manifold (M,g) and a vector field XX(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,ZX(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:MEm+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:MEm+1 be an immersion of a compact simply connected hypersurface with ψT a non-trivial geodesic vector field, m2. Then the Ricci curvature satisfies

    Ric(ψT,ψT)m1m(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)m1m(div ψT)2. (3.1)

    Then, using Eqs (1.3) and (2.7), we have σAψT=ψT. Taking covariant derivative with respect to XX(M) in this equation and using Eq (2.7), we get

    X(σ)AψT+σ(A)(X,ψT)+σA(X+σAX)=XσAX

    that is

    σ(A)(X,ψT)=X(σ)AψTX2σAXσ2A2XXX(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)m2mσασ2A2

    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)=AψT2m2mσασ2A2. (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))=m2mσασ2A2.

    Integrating the above equation while using Minkowski's formula (2.9), we have

    M(Ric(ψT,ψT)+m(m1)m2σ2α2+σ2A2)=0

    that is,

    M(Ric(ψT,ψT)m(m1)(σ2α21))=Mσ2(mα2A2). (3.4)

    Now, we use div ψT=m(1+σα) and Eq (2.9), to arrive at

    M(div ψT)2=m2M(1+2σα+σ2α2)=m2M(σ2α21)

    and inserting the above equation in Eq (3.4), we have

    M(Ric(ψT,ψT)m1m(div ψT)2)=Mσ2(mα2A2). (3.5)

    Using inequality (3.1) in Eq (3.5), we get

    Mσ2(mα2A2)0

    and above inequality in view of the Schwart's inequality A2mα2 implies

    σ2(mα2A2)=0.

    If σ=0, then by Minkowski's formula (2.9), we get a contradiction. Thus, we have A2=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

    mi=1(A)(ei,ei)=grad α

    Using Eq (2.6), we get (m1)grad α=0 and with restriction on dimension m, we conclude α is a constant. Moreover, this constant α0 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:MEm+1 be an immersion of a compact simply connected hypersurface with ψT=0, m2. 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)2AψT2+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)+m2m2σ2α2)=0. (3.9)

    Define a smooth function h on the hypersurface M, by h=12ψ2, 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)2Hh2)=M(1m(Δh)2Hh2+m1m(Δh)2)

    Inserting Δh=m(1+σα) in the last term of the right hand side of above equation, we have

    M(1m(Δh)2Hh2)=M(Ric(ψT,ψT)m(m1)(1+σα)2)

    and using Eq (2.9), we get

    2M(1m(Δh)2Hh2)=M(2Ric(ψT,ψT)2m(m1)(σ2α21)). (3.11)

    Combining Eqs (3.9) and (3.11), we arrive at

    2M(1m(Δh)2Hh2)=m(m2)M(1σ2α2).

    Using Schwarz' inequality Hh21m(Δh)2 and inequality (3.6) with m2, in above equation, we conclude the equality Hh2=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(AαI)=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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