LehmerDH数在模p剩余系的分布

设 p≥ 3为素数 ,集合A ={a|1≤a 相似文献   

公式H_n=lnn+C+ε_n及在级数中的运用

证明公式Hn =lnn+C+εn,并在级数收敛性判别中运用     

关联数列的数表问题

近年来“数表问题”如一颗璀璨的“明珠”，频频出现在国际、国内的数学联赛、中、高考试卷上，它与数列知识联手，凑出一曲曲优美的“乐章”，所谓“数表”就是满足一定条件的数，按一定规律排成一个表，这类问题题型灵活、解法巧妙、规律性强、学生乐见，低、中、高档题均可出现，故成为很多出题专家们的“新宠”，下面就关联数列的数表问题进行分类探究．用以抛砖引玉，期望读者从中受益，进而得出解决此类问题的一般方法。     

精心设计问题培养学生能力

记忆特征告诉我们，要加强对某一件事的记忆，加深对某一问题的理解，“错误”与“教训”是最为深刻的．数学教学何尝不是如此．例如，为了加深学生对等差数列的前n项和公式的理解和应用，在教学中可设计如下两个问题：     

基于Hamaker假设的黏着接触弹性模型

为研究微纳米系统中的黏着接触问题，基于Hamaker假设和Lennard-Jones势能定律，通过积分方法得到了球体与平面间的黏着力，同时结合经典弹性理论建立了一种新型的球体与平面黏着接触的弹性模型，该模型可以同时得到平面轮廓随间距的变形过程及黏着力和平面变形量随间距的变化规律，当球体半径较大时，所建模型与基于Derjaguin近似的黏着模型给出的结果基本一致，随着球体半径的逐渐减小，两种模型的差异逐渐增大，这是由于Derjaguin近似的误差随球体半径的减小而增大引起的，因此，当球体的半径趋近纳米级时，基于Hamaker假设的黏着接触模型可以给出更加准确的结果。     

一类积分不等式的推广

对一些基本的积分不等式进行了推广，给出了含有n个无关变元的更广泛的非线性积分不等式．利用所得的不等式讨论了某些非线性积分方程解的有界性．     

BOUNDEDNESS OF MAXIMAL SINGULAR INTEGRALS

The authors study the singular integrals under the Hormander condition and the measure not satisfying the doubling condition. At first, if the corresponding singular integral is bounded from L2 to itself, it is proved that the maximal singular integral is bounded from L∞to RBMO except that it is infinite μ-a.e. on Rd. A sufficient condition and a necessary condition such that the maximal singular integral is bounded from L2 to itself are also obtained. There is a small gap between the two conditions.     

The Iyengar Type Inequalities with Exact Estimations and the Chebyshev Central Algorithms of Integrals

In this paper, both low order and high order extensions of the Iyengar type inequality are obtained. Such extensions are the best possible in the same sense as that of the Iyengar inequality. hzrthermore, the Chebyshev central algorithms of integrals for some function classes and some related problems are also considered and investigated.     

Rotational Deformation of Neutron Stars

The rotational deformations of two kinds of neutron stars are calculated by using Hartle‘s slow-rotation formulism. The results show that only the faster rotating neutron star gives an obvious deformation. For the slow rotating neutron star with a period larger than hundreds of millisecond, the rotating deformation is very weak.     

半线性波动方程的自相似解

研究了具有非线性项|u|~αu的半线性波动方程的Cauclly问题,利用仿积分解及交换子估计等技术,证明了当α为一般的实数且满足一定的限制时,Cauchy问题自相似解的存在性。本文的结果回答了Planchon在其工作中所遗留的问题。