Ming LI Jiazu ZHOU
The kinematic formulas are the most beautiful and also useful formulas in integral geometry.At the beginning of his classical paper[4]Chern said:“One of the basic problems in integral geometry is to find explicit formulas for the integrals of geometric quantities over the kinematic density in terms of known integral invariants.”
For instance,Chern proved in[3]the fundamental kinematic formula in then-dimensional Euclidean space En.LetD0andD1be two domains with smooth boundaries∂D0and∂D1,respectively,in En.If we denote byGthe group of rigid motions of Enwith density dg,and byOn−1the volume of the unit sphereSn−1in En,then the fundamental kinematic formula is
whereχ(·)denotes the Euler characteristic,σ(·)the volume andtheithtotal mean curvature.
In[4],Chern gave the integral formulas of the quantities which appear in Weyl’s formula for the volume of tubes.LetM0andM1be two closed smooth submanifolds of dimensionpandqrespectively in En,and then
where the quantitiesμeappear in Weyl’s formula for the volume of tubes(see[14]),0≤e≤p+q−nandeis even.The coefficientsciare constants depending onn,p,qande.
These formulas can also be found in books[11–12].
In his paper[18],Zhou obtained the kinematic formulas for mean curvature power integrals in then-dimensional Euclidean space,which are the generalization of the formulas of the 3-dimensional case in[1,16]and are of the extrinsic type.LetSi(i=0,1)be two closed smooth hypersurfaces in En.Denote byHthe mean curvature ofandThen(see[18])
wherecpqklnare constants depending on the indices,is a kind of total curvature ofThis is a remarkable work in which the moving frame method is effectively used and a successful application of the kinematic formulas is given.
The novel approach to study the containment problem and geometric inequalities by using kinematic formulas has been systematically developed.For the recent developments,interested readers can refer to[8–10,15–23].We also recommend the books[11–12]for the classical results of integral geometry and its applications.
In fact,integral geometry can be set up within the framework of the theory of homogeneous spaces.
LetGbe a unimodular Lie group with kinematic density dgandHa closed subgroup ofG.LetMandNbe two compact submanifolds in the homogeneous spaceG/H,Mfixed andgNthe image ofNunder a motiong∈G.LetI(M∩gN)denote some kind of global geometric invariants ofM∩gNwhich may be volume,curvature integral,etc.Then the goal of the kinematic formulas related to the invariantI(M∩gN)is to evaluate the following integral
by the known integral invariants ofMandN.
Howard proved in[7]a theorem of kinematic formulas in arbitrary homogeneous spaces.It indicates the computability of kinematic formulas with which the related invariants are of the following type
wherehis the second fundamental form ofinG/H,Pis an invariant polynomial in the components ofhwith value,anddσ(x)is the volume element.
This theorem is general and implicit.However,it still requires concrete calculation to obtain explicit formulas,particularly when the kinematic formula is of the extrinsic type.
We prefer the formulas in the Euclidean case.First,because they are important from the point of view of their applications,and second,because they lead to more computable results.
In this paper,we give another kind of explicit kinematic formulas about two closed orientable hypersurfaces in En,n≥3.The manifolds that appear are assumed to be smooth.
We will denote the group of rigid motions of EnbyG.The isotropic subgroup ofGis denoted byG0.IndeedG0is the special orthogonal groupSO(n).The groupsGandG0are unimodular with canonical densities dgand dg0respectively.Let dσbe the Lebesgue measure of En,and then we haveMoreover,the total volume ofG0denoted byJnis finite and given by
whereOi−1is the volume of thei−1 dimensional unit sphere in Eiwith the value
Our motivation comes from the following formulas in[6,12–13].For example,letMbe a closed hypersurface in En,and then
In this formula,the integerisatis fies 0≤i≤n−2,Lis a random oriented hyperplane,and dLis the canonical invariant measure atdenotes themean curvature integral ofwhich is considered as a hypersurface inL.Similarly,for the sake of simplicity.
Taking an arbitrary orientable closed hypersurface in place ofL,we obtain the following kinematic formula.It is not of Howard’s type.
Theorem 1.1Let S0and S1be two closed oriented hypersurfaces in the n-dimensional Euclidean spaceEn.For any integer i satisfying0≤i≤n−2,we have an asymmetric kinematic formula
where the coefficientsc(p,i,n)depend only on p,i and n with value
Note that the formula(1.3)can be viewed as a limiting case of(1.4).
Remark 1.1By direct observation,ifiis even,then(1.4)is just a special case of(1.1)for the hypersurfaces.
But the situation is different ifiis odd.The simplest case isi=1.Sinceis actually the volumeσ(·),we have the following result.
Corollary 1.1Let S0and S1be two closed oriented hypersurfaces in the n-dimensional Euclidean spaceEn.Then
More speci fically,foris the total geodesic curvature of the curve,denoted asThen the above formula is
The formula(1.5)gives exactly an integral representation of the total mean curvature based on any given closed hypersurface.
In the papers[3–4],Chern associated each given Riemannian manifold certain fiber bundle with canonical densities.These concepts and the moving frame method have been proved to be effective in integral geometry.We would like to follow this way in this paper.
We agree in this section on the following indix ranges:
LetMbe anm-dimensional submanifold in an orientedn-dimensional Riemannian manifoldNwith Riemannian metricandthe identity map.
First of all,we mention the local structure ofM(see[5]).LocallyMcan be attached to a Darboux framee1,···,em,em+1,···,en,which is a smooth orthonormal frame field and satis fies thate1,···,emis tangent toM.In the rest of this article,when we mention frames tangent to an oriented manifold,it is always assumed that the orientation of the frames has been chosen to be compatible with the orientation of the given manifold.So here the orientation ofe1,···,emande1,···,em,em+1,···,enis the same as that ofMandNrespectively.
Letrespectively be the canonical forms and the Levi-Civita connection forms on the orthogonal groupSO(n)principle bundleSO(N)under arbitrary extension of the given Darboux frame.These forms can be pulled back onMby the Darboux frame.The images are still denoted by
Let∇be the Levi-Civita connection on the tangent bundleTN,and then we have
and
From the above equation,we obtain
The quantitiesare the components of the second fundamental form ofM.
We review the de finition of the mean curvature integrals of a hypersurfaces as follows.Letm=n−1,and thenMis an oriented hypersurface inN,which has a chosen orientation.Theithmean curvature is related to the following characteristic polynomial oforfor simplicity in the hypersurface cases.Let
and then theithmean curvature is de fined as
and theithtotal mean curvature,if it exists,is denoted by
In this paper,we writeinstead ofto emphasize that the calculation is done inN,sinceMmay be simultaneously a submanifold of other ambient spaces.Notationis used for the same purpose.
For a fixed nonnegative integerk,we de fine a spaceEkassociated withMby the set
is a fiber bundle with the base spaceMand the fiberEkis called the tangentk-bundle ofMhere.In fact,Ekis an orientable differentiable manifold of dimensionAt any point where(x;e1,···,ek)∈Ek,one extends(x;e1,···,ek)to be a Darboux framee1,···,enbesidex,and then de fines the following form:
whereis the volume element ofM,and the restriction ofon the fibers is indeed the density ofSO(m)/SO(m−k).It is proved in[3],that Θ is independent of the choice of extension and is well de fined onEk.It gives rise to a density ofEk.
LetS0andS1be two closed oriented hypersurfaces in then-dimensional Euclidean space En.The tangent(n−2)-bundles ofS0andS1are denoted byEn−2,0andEn−2,1,respectively.
For eachg∈Gsuch thatis the tangent(n−2)-bundle ofwith density Φg.Then Φg∧dgis a density of the setD={(X,Y,g)∈
For any point(x;e1,···,en−2)ofwe complement it into an orthonormal framesuch thatis orthogonal toS0and also into an orthonormal framesuch thatis orthogonal togS1.Letθ∈(0,π)be the angle betweenand,and then the following differential formula(see[3–4,11–12])is well known for the density ofD:
where Θ0and Θ1are the densities ofEn−2,0andEn−2,1,respectively.Indeed the right side of(3.1)is a density of
Observe that the subset ofDisfor fixedg∈G,and the left side of(1.4)writes as
By(3.1),we see that the above integration is
We turn our attention to the computation of.The problem is to givea representation by the curvatures ofS0andgS1atwhen the motiongis fixed.
From now on,the indexesi,j,kare agreed to range from 1 to(n−2),andA,Bfrom 1 to(n−1).
The induced Levi-Civita connection ofgS1is actuallydof Enprojected on the tangent space ofgS1.Hence the curvature ofwith respect togS1is given by
We here denote bythe dual basis with respect to the framee1,···,en−2,and byω1,···,ωnwith respect toe1,···,en.
From the relation
can be represented as
Then
If we attach an orthonormal frame fieldv1,···,vn−1onS0andongS1nearx,the correspondent dual orthonormal frame fields areη1,···,ηn−1andη′1,···,η′n−1,and then there exist orthogonal matricesandsuch that
Now we assume thatandare the principle tangent vectors ofS0andgS1,respectively,and then
whereκAandare the principle curvatures ofS0andgS1atx,respectively.
With the aid of these notions,we reformulate the right side of(3.3)into
The reason of the last equality is that we calculate inandωn−1=ω′n−1=0.
By the linear independence ofωi,we represent the curvature ofas
Following Chern[3],we are going to expand the determinant of(hij)as the polynomial ofandBy the multilinearity of the determinant,one has
whereis the sum of some(n−2)×(n−2)-determinants,and one term in the summation is
while others can be obtained by permuting some upscriptA’s with some upscriptB’s in(3.4),but preserving the orders ofA1A2···AqandB1B2···Bpto themselves.If some elements ofA1A2···AqorB1B2···Bpappear twice,then clearly
By this observation,one has
where
withσandτrunning through the permutation groups of orderqandp,respectively.
The equations(3.5)then imply that
where the summation indexsruns from 1 toq,andtfrom 1 top.So we obtain the following formula about det(hij):
where
and
More generally,we will discuss the coefficients of the characteristic polynomial
It is clear that det(hij)=ψn−2.By a result in linear algebra,theithcoefficient is given by
A similar discussion about det(hij)gives that
where
One notes that the coefficientsatxare only dependent on the relative position ofS0andS1,and they are invariant if the framee1,···,en−2is acted by an element ofO(n−2).
Then the integration(3.2)continues as follows:
The last equality deserves more explanations.Now we are going to discuss the integral ofoverBy fiber integration,we have
One notes that the densitiesandareSO(n−1)invariant respectively.One also remembers thatandare coefficients ofeiandwith respect tovAandrespectively.For any combinations 1≤j1<···<ji≤n−2,there exists a rotation inSO(n−1)by whiche1,···,eiis rotated to the position ofej1,···,eji.So the fiber integral is
On the hypersurfaceS0,for two sets of different indexesA1,···,Aqandthere exists a rotationginSO(n−1),such thatThe same statement is also valid forS1.Let
and then Ω(p,i,n)are independent of the choices ofA1,···,Ai−pandB1,···,Bp.
If we denote theithelementary symmetric polynomial of the elementsas{aA1···aAi},then the integration ofonis
Instead of direct calculation of Ω(p,i,n),we prefer to determine the universal constants c(p,i,n)by takingS0andS1to be hyperspheres,and then evaluate Ω(p,i,n).
The constants will be determined in the last section.We complete the proof of Theorem 1.1.
Letandbe hyperspheres in Enof radii 1 andR(0<R<1)respectively.LetS0be centered at the origin pointO.For a fixed motiong,letybe the distance fromOto the center of
Whenwhich is equivalent tois a hyperspherein a hyperplane of radius
It can be proved that
So we obtain
In this speci fic case,the left side of(1.4)reads
By the polar decomposition of Lebesgue measure dσand using(4.1),the above integration is
Puttingwe reformulate the integration as
By the formula(1.2),the kinematic formula for the hyperspheresS0=Sn−1(1)andS1=Sn−1(R)is proved to be
So the universal coefficients in(1.4)are given by
As a consequence,one has
AcknowledgementsThe first author would like to thank Prof.Huitao Feng for his consistent support and encouragement.The authors would like to thank the referees for their helpful comments and suggestions.
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Chinese Annals of Mathematics,Series B2016年1期