R^2,1中线性Weingarten曲面的Baecklund变换

本文对三维Minkowski空间R^2，1中具有性质K-2mH m^2-ι^2=0或H=constant的类时曲面定义了一个Darboux线汇，同时得到了相应的Baecklund变换。     

应用高斯公式应注意的一个问题

在利用高斯公式计算第二类曲面积分时 ,若曲面为非封闭曲面 ,此时添加辅助曲面时 ,要特别注意 ,要保证在封闭曲面及内部满足高斯公式的条件 ,稍有不慎就会得出错误的结果 .如下面这个例子 :例　算曲面积分 I = Σxdydz ydzdx zdxdy(x2 y2 z2 ) 3/2 ,其中Σ为曲面 1 -z5 =(x -2 ) 21 6 (y -1 ) 29(z≥ 0 )的上侧 .解　令 P =x(x2 y2 z2 ) 3/2 ,Q =y(x2 y2 z2 ) 3/2 ,R =z(x2 y2 z2 ) 3/2设Σ1是 xoy平面上由 (x -2 ) 21 6 (y -1 ) 29≤ 1所围部分的下侧 ,Ω是Σ与Σ1所围闭域 .∵ P x =-2 x2 y2 z2(x2 y2 z2…     

R~(2,1)中线性Weingarten曲面的Bcklund变换(英文)

本文对三维Minkowski空间R~(2,1)中具有性质K-2mH+m~2-l~2=0或H=constant的类时曲面定义了一个Darboux线汇,同时得到了相应的Bcklund变换。     

正平均曲率的一个注记

设Ω是R~n(n≥2)中的单连通有界开集,其边界骪Ω是无限可微的封闭超曲面。设H(S)是Ω的平均曲率(n=2,H(s)是曲率)。假定s∈Ω,H(s)>0。记 则我们证明 ii)H_0/H_1≤(1-1/n)~2|Ω|/|Ω|~2 integral from n=Ω to (ds)/(H(s))~2, iii)|Ω|≤(1-1/n)integral from n=Ω to (ds)/H(s), 我们有如下未解决问题:是否成立不等式     

高斯公式应用小议

在利用高斯公式计算曲面积分时 ,许多学生往往忽视了对定理条件的考察。比如 :同济四版《高等数学》下册总习题十的第 3 ( 4)题就是一例。例 1 :计算 ∑xdydz +ydzdx +zdxdy( x2 +y2 +z2 ) 3 ,其中 ∑:1 -z5=( x -2 ) 21 6+( y -1 ) 29( z≥ 0 )上侧。多数学生在利用高斯公式求解时 ,做法如下 :解 :令 P =x( x2 +y2 +z2 ) 3 ,Q =y( x2 +y2 +z2 ) 3 ,R =zx2 +y2 +z2 ) 3 ,补 ∑1:z =0 ( x -2 ) 21 6+( y -1 ) 29≤ 1 下侧。于是由高斯公式得 : ∑+ ∑ 1Pdydz +Qdzdx +Rdxdy = Ω P x+ Q y+ R z dv Ω0 dv =0 ,其中Ω为由 ∑ +∑1所围区…     

R2,1中类时Weingarten曲面的Bcklund变换

本文利用平行变换,得到3维Minkowski空间R2,1中的K-2mH+m2-l2=0(H2>K,0≤m相似文献   

一类具有任意次数的参数多项式极小曲面

极小曲面是在几何造型设计中有着重要应用的一类特殊曲面.本文从几何造型的视角提出一类次数任意的参数多项式极小曲面.所提出的极小曲面具有显式的参数表示,并具有一些重要的几何性质,如对称性、包含直线和自交性.根据几何性质,本文将该参数多项式极小曲面划分为4类:n=4k+1,n=4k+2,n=4k+3,n=4+4,其中n是极小曲面的次数,k是正整数.本文给出与之相对应的共轭极小曲面的显式参数形式,并实现其等距变形.     

关于仿射极小平移超曲面

本文属于仿射微分几何。在3-维欧氏空间 E~3中,F.Scherk 定理告诉我们,极小平移曲面必需是平面或 Scherk 曲面az=1n(cos ax/cos ay),a=constant。在一般(n+1)维仿射空间 A~(n+1)中,仿射极小平移超曲面是什么曲面?本文得到了这种曲面共有两类的结果(见定理1)。当 n=2时,这就是引文[3]中的结果(见定理2)。     

CPn中的弱等焦Hopf超曲面

本文研究了 CPn中的弱等焦Hopf超曲面的分类,弱等焦超曲面首先是由滕楚莲与Thorbergsson在[13]中引入的.设M是CPn中的弱等焦Hopf超曲面,则M的不同焦半径的个数是2,4或6;并且当g=2或4时,M在CPn中是等参的;当g=6时,n=8,(M-)=π-1(M)与S7中的等参超曲面不Lie等价,此处π:S7→CP3是Hopf纤维化.     

多元函数积分学的物理意义在解题中的应用

本文用高等数学知识和物理知识相结合 ,利用多元函数积分学的物理意义解决一类题目 ,显得相当简便。例 1　设 D是以点 O( 0 ,0 )、A( 1 ,2 )和 B( 2 ,1 )为顶点的三角形区域 ,求 Dxdxdy.解　直线 OA,OB和 AB的方程分别为y =2 x,y =12 x和 y =3 -x Dxdxdy = D1xdxdxy + D2xdxdy =∫10xdx∫2 xx/2dy +∫21xdx∫3- xx/2dy =32 .　　本题若用形心公式则更为简便 :由形心公式 x= Dxdσ Ddσ得 , Dxdσ=x. Ddσ.形心横坐标为 :x=0 +1 +23 =1 ,此三角形的面积为 32 ,所以 Dxdxdy =32 .此法具有通用性 ,对于规则的形体都适用。例 2…     

The stability of a minimal surface in a pseudo-Euclidean space

We prove that any piece of a space-like minimal surface of the form z=z(x, y), in the pseudo-Euclidean space E^3,1 with line element dx²+dy²–dz² has the greatest area among close space-like surfaces with the same boundary. For time-like surfaces the following assertion is proved. Let V² be a time-like minimal surface in E^3,1. Then for any domain on V², there exists a smooth variation in the class of time-like surfaces with fixed boundary that increases the area, and there exists a smooth variation in the same class of surfaces that decreases the area.Translated from Ukrainskii Geometricheskii Sbornik, No. 33, pp. 41–45, 1990.     

COMPLETE EXTREMAL SURFACES OF MIXED TYPE IN 3-DIMENSIONAL MINKOWSKI SPACE

ＣＯＭＰＬＥＴＥＥＸＴＲＥＭＡＬＳＵＲＦＡＣＥＳＯＦＭＩＸＥＤＴＹＰＥＩＮ３－ＤＩＭＥＮＳＩＯＮＡＬＭＩＮＫＯＷＳＫＩＳＰＡＣＥ￥ＧＵＣＨＡＯＨＡＯ（ＩｎｓｔｉｔｕｔｅｏｆＭａｔｈｅｍａｔｉｃｓ，ＦｕｄａｎＵｎｉｖｅｒｓｉｔｙ，Ｓｈａｎｇｈａｉ２００...     

Surfaces with zero mean curvature vector in neutral 4-manifolds

Space-like surfaces and time-like surfaces with zero mean curvature vector in oriented neutral 4-manifolds are isotropic and compatible with the orientations of the spaces if and only if their lifts to the space-like and the time-like twistor spaces respectively are horizontal. In neutral Kähler surfaces and paraKähler surfaces, complex curves and paracomplex curves respectively are such surfaces and characterized by one additional condition. In neutral 4-dimensional space forms, the holomorphic quartic differentials defined on such surfaces vanish. There exist time-like surfaces with zero mean curvature vector and zero holomorphic quartic differential which are not compatible with the orientations of the spaces and the conformal Gauss maps of time-like surfaces of Willmore type and their analogues give such surfaces.     

Space-like loxodromes on rotational surfaces in Minkowski 3-space

We find all space-like loxodromes on rotational surfaces which have space-like meridians or time-like meridians, respectively by using a relevant Lorentzian angle in Minkowski 3-space. To understand loxodromes better, we draw some pictures of them via Mathematica computer program.     

INFINITESIMAL DEFORMATIONS OF TIME-LIKE SURFACES IN MINKOWSKI 3-SPACE

In this paper, infinitesimal deformations of time-like surfaces are investigated in Minkowski 3-space R^2,1. It is shown that some given deformations of the time-like surface can be described by 2 1 dimensional integrable systems. Moreover spectral parameters are introduced, and it is proved that deformation families are soliton surfaces‘ families.     

关于三维Minkowski空间中直线汇的一些注记

本文研究了三维Minkowski空间中直线汇的一些性质,特别是关于类时线汇的性质．讨论了线汇基本元素的存在性,并证明了关于三维Minkowski空间中类时线汇的配分参数的一个结果,推广了苏步青1927年的—个成果．     

Time-like Linear Weingarten Surfaces in Lorentzian Space Forms

In this paper we study Backlund transformations of time-like linear Weingarten surfaces with negative discriminant in Lorentzian space forms.     

B(A)CKLUND TRANSFORMATION ON SURFACES WITH CONSTANT MEAN CURVATURE IN R2'1

In this paper,the authors obtain the Backlund transformation on time-like surfaces with constant mean curvature in R2,1.Using this transformation,families of surfaces with constant mean curvature from known ones can be constructed.     

Asymptotic behavior of classical solutions of reducible quasilinear hyperbolic systems with characteristic boundaries

In this paper, we investigate the asymptotic behavior of classical solutions of reducible quasilinear hyperbolic systems with characteristic boundaries. Under some suitable assumptions, we prove that the solution approaches a combination of Lipschitz continuous and piecewise C¹ traveling wave solution. As an application, we apply the result to the equation for time-like extremal surfaces in the Minkowski space-time R1+(1+n).