Lorentz-Minkowski空间中的乘积空间R~k×H~(n-k)

本文的主要结果是:Lorentz-Minkowski空间中介于两个同心伪圆柱面之间的完备、类空、常平均曲率超曲面必为伪圆柱面,即乘积空间R~k×H~(n-k)．对于常高阶平均曲率的情况,如果截曲率有下界,那么介于两个同心伪球面之间的完备类空超曲面必为伪球面．     

Lorentz-Minkowski空间中的乘积空间R~k×H~(n-k)

本文的主要结果是:Lorentz-Minkowski空间中介于两个同心伪圆柱面之间的完备、类空、常平均曲率超曲面必为伪圆柱面,即乘积空间R~k×H~(n-k)．对于常高阶平均曲率的情况,如果截曲率有下界,那么介于两个同心伪球面之间的完备类空超曲面必为伪球面．     

一类极小曲面的不存在性

本文考虑三维 Euclid 空间 R~3中拓扑型为球面的有限全曲率完备嵌入极小曲面.通过对伪嵌入极小曲面的研究,证明了一类嵌入极小曲面的不存在性,并明确了伪嵌入与嵌入极小曲面的差异.     

四维球面上的稳定超曲面

我们研究四维球面中的1-极小稳定完备非紧超曲面.得到在适当限制平均曲率与高斯曲率的情况下,四维球面中不存在具有多项式体积增长的1-极小稳定完备非紧超曲面.这些结果部分证实了外围空间是四维球面时Alencar等人提出的猜测.     

一类具有平行平均曲率和有限全曲率的完备子流形

本文把Berard P.,do Carmo M.,Santos W.在1998年所得的结果,分别推广到局部对称的Cartan-Hadamard流形中具有常平均曲率和有限全曲率的完备超曲面,以及球面上具有平行平均曲率和有限全曲率的完备子流形.     

纯量曲率和平均曲率成线性关系的完备超曲面

本文首先讨论纯量曲率R和平均曲率H满足R=kH,k=Const。的完备曲面帮超曲面。证得:R~3中这样的曲面是球面、柱面或平面;R~(n 1)中这样的超曲面当它是凸的且R有上界时是超球面、超平面或广义圆柱面;R~(2 p)(p≥1)中这样的曲面在一定附加条件下是包括球面和平面在内的四种曲面,最后讨论类似的子流形。这些结果改进或推广了[5,6,7]的结果。     

关于R~4内的常数量曲率的完备超曲面

本文证明了下述的主要结果:设 M 为 R~4中的完备常中曲率超曲面,且数量曲率为常数,如果 M 不是常主曲率超曲面,则一定有R<0.     

复射影空间中具有常数量曲率的实超曲面

将球面上常数量曲率超曲面推广到复射影空间中,得到此类实超曲面的某些积分不等式.     

圆球面为边的常F-平均曲率类空超曲面

设F(t)是上伪球面H_+~n上时轴旋转不变且满足凸条件的光滑函数.本文证得:Lorentz空间L~(n+1)中,以圆球面S~(n-1)(R)为边界且有非零常F-平均曲率的紧致类空超曲面必为Wulff帽.     

关于Weingarten超曲面的一个存在性定理

本文研究伪黎曼空间型中一类特殊的Weingarten超曲面的存在性问题.通过引入伪黎曼空间型中旋转超曲面的概念,并给出其主曲率计算公式.得到伪黎曼空间型中旋转型Weingarten超曲面的存在性定理.推广并统一了相关结果.     

-1=1?

推证 :- 1 =i2 =( i4) 12 =1 .显然结论错误 ,但究竟错在哪里呢 ?诡辩揭密 :关于复数指数幂运算律 ,详见人教版原高二代数教材 P1 91有 :　　　　 ( zm) n =zmn,　　　　 zm . zn =zm+ n,　　　　 zmzn =zm-n,其中 m、n∈ N.实质上 ,m,n∈ Z也成立 .可见 ,i2 ≠ ( i4) 12 ,即 - 1≠ 1 .-1=1?!712000$陕西省咸阳市天王中学@曹万宏     

ℒ1 subspaces ofl 1

It is proved that every subspace ofl ₁ which is an Λ_{1, λ} space with λ close enough to 1 is isomorphic tol ₁.     

On almost 1-1 extensions

We show that a broad class of extensions of measure preserving systems in the context of ergodic theory can be realized by topological models for which the extension is “almost one-one”.     

BestL 1-approximations of classesW 1 r by Splines fromW 1 r

We obtain the exact values of the bestL ₁-approximations of the classesW ₁ ^r of periodic functions by periodic polynomial splines of degreer and defect 1 with equidistant knots that belong to the classW ₁ ^r .Translated from Ukrainskii Matematicheskii Zhurnal, Vol. 46, No. 10, pp. 1410–1413, October, 1994.     

Non-linear oscillations of a satellite at 1:1:1 resonance

The motion of a satellite about its centre of mass in a central Newtonian gravitational field is investigated. The satellite is considered to be a dynamically symmetrical rigid body. It is assumed that the ratio of the polar and equatorial principal central moments of inertia of the satellite is 4/3, or close to this. The orbit of the centre of mass is elliptic, and the orbit eccentricity is assumed to be small. In the limit case, when the orbit of the centre of mass is circular, a steady motion exists (corresponding to relative equilibrium of the satellite in the orbital system of coordinates) in which the axis of dynamic symmetry is directed along the velocity vector of the centre of mass of the satellite; here, the frequencies of the small linear oscillations of the axis of symmetry are equal or close to one another. But in an elliptic orbit of small eccentricity, multiple 1:1:1 resonance occurs in this case, as the oscillation frequencies mentioned are equal or close to the frequency of motion of the centre of mass of the satellite in orbit. The non-linear problem of the existence, bifurcations and stability of periodic motions of the satellite with a period equal to the rotation period of its centre of mass in orbit is investigated.     

关于Goormaghtigh方程(x~3-1)/(x-1)=(y~n-1)/(y-1)

本文证明了：Ｇｏｏｒｍａｇｈｔｉｇｈ方程适合的例外解（ｘ，ｙ，ｎ），满足以及