Stokes问题在各向异性网格下的Bernadi-Raugel有限元逼近

在各向异性网格下,得到了Stokes问题著名的Bernadi-Raugel混合有限元格式的超逼近性质,而且通过构造插值后处理算子得到了关于速度的超收敛结果.     

$(f,g)$-反演的一些应用

我们给出了马欣荣的关于$(f, g)$-反演的三种应用. 在$(f, g)$-演中通过取具体的函数和序列, 我们推出了一些关于超几何级数与调和数的恒等式. 然后我们给出了一些关于$q$-超几何项的反演关系. 最后, 我们将$(f, g)$-反演和$q$-微分算子结合, 得到了一些$q$-级数恒等式.     

Stokes型积分-微分方程Q_2-P_1元的超收敛分析

本文研究Q2-P1混合元对Stokes型积分-微分方程的有限元方法.利用积分恒等式技巧给出了关于流体速度u和压力p的误差估计,特别是在压力p的误差中去掉了影响解的稳定性的1因子t-2,改善了以往文献的结果.同时,通过构造适当的插值后处理算子得到了整体超收敛结果.     

分数阶超Yang族及其超哈密顿结构

通过应用分数阶超迹恒等式以及建立在李超代数上的广义零曲率方程,得到分数阶超Yang族和它的分数阶超哈密顿结构.应用该方法还可以得到其他分数阶超方程族.     

关于超Euler图的一个猜想的注记

本文研究了Catlin的关于超Euler图的一个猜想,借助于收缩方法,得到了该猜想的两个充分条件.     

局部对称黎曼流形中的超曲面

研究了局部对称黎曼流形中具有常平均曲率超曲面的几何性质,得到了关于其第二基本形式模长平方的拼挤定理.     

抛物问题各向异性有限元的超收敛分析

本文研究具有各向异性特征的双二次元对二阶抛物方程的逼近.通过积分恒等式和插值后处理技术,在各向异性网格下得到了相应的超逼近和超收敛结果.     

带随机移民的超布朗运动占位时的大偏差

本文考虑了带随机移民的超布朗运动占位时过程,其移民速度由另外一超布朗运动的轨道所决定.在维数d≥7时,得到它的大偏差原理.     

带随机移民的超布朗运动占位时的大偏差

本文考虑了带随机移民的超布朗运动占位时过程,其移民速度由另外一超布朗运动的轨道所决定在维数d≥7时,得到它的大偏差原理.     

半线性抛物方程各向异性最低阶R-T混合元超收敛分析

利用各向异性判别定理验证了最低阶数R-T混合元具有各向异性特征.利用积分恒等式技巧,得到了R-T元对半线性抛物方程的超逼近性质.通过构造新的插值后处理格式,导出了超收敛结果及后验误差估计.     

扩散速度与组元的质量守恒方程

在混合物流动中,某组元i的质量迁移速度(绝对速度)等于对流速度(牵连速度)与扩散速度(相对速度)之和.扩散速度——以及扩散系数——依对流速度取法之不同而不同.在湍流中,组元i的质量迁移速度是(?)(质量加权的时间平均速度).扩散速度((?)-a)是由湍流扩散速度(?)和分子扩散速度v_1-a所组成((?)是组元i的时平均速度,a是某种取法的对流速度).因此,湍流扩散速度与对流速度的取法无关.组元i的质量守恒方程,其右端的扩散须依其左端对流速度取法之不同而不同.在湍流情况下,它可能没有扩散项,或只有湍流扩散项,或既有湍流扩散项又有分子扩散项,如果我们取(?),或(?),或任何其它速度作为对流速度的话.在层流中会遇到只有分子扩散项而无湍流扩散项的例子.分子扩散总是依赖于对流速度的选取.与混合气体情况不同,在二相流中.分子扩散项的重要性相当于、或甚至超过湍流扩散项.     

Fully-developed free-convective flow of micropolar and viscous fluids in a vertical channel

The problem of fully-developed laminar free-convection flow in a vertical channel is studied analytically with one region filled with micropolar fluid and the other region with a viscous fluid. Using the boundary and interface conditions proposed by previous investigators, analytical expressions for linear velocity, micro-rotation velocity and temperature have been obtained. Numerical results are presented graphically for the distribution of velocity, micro-rotation velocity and temperature fields for varying physical parameters such as the ratio of Grashof number to Reynolds number, viscosity ratio, width ratio, conductivity ratio and micropolar fluid material parameter. It is found that the effect of the micropolar fluid material parameter suppress the velocity whereas it enhances the micro-rotation velocity. The effect of the ratio of Grashof number to Reynolds number is found to enhance both the linear velocity and the micro-rotation velocity. The effects of the width ratio and the conductivity ratio are found to enhance the temperature distribution.     

Analytical solutions of laminar swirl decay in a straight pipe

In this work, the laminar swirl flow in a straight pipe is revisited and solved analytically by using prescribed axial flow velocity profiles. Based on two axial velocity profiles, namely a slug flow and a developed parabolic velocity profiles, the swirl velocity equation is solved by the separation of variable technique for a rather general inlet swirl velocity distribution, which includes a forced vortex in the core and a free vortex near the wall. The solutions are expressed by the Bessel function for the slug flow and by the generalized Laguerre function for the developed parabolic velocity. Numerical examples are calculated and plotted for different combinations of influential parameters. The effects of the Reynolds number, the pipe axial distance, and the inlet swirl profiles on the swirl velocity distribution and the swirl decay are analyzed. The current results offer analytical equations to estimate the decay rate and the outlet swirl intensity and velocity distribution for the design of swirl flow devices.     

Unsteady flow past a flat plate with suction

A solution is given for the transient response for laminar boundary layer flow past a flat plate to a step-function change in suction velocity. An arbitrary but constant suction velocity normal to the plate is allowed prior to step-change. Using the Laplace transform technique the solutions for the unsteady velocity profile and shear stress are obtained and are graphically sketched when the suction velocity doubles in the stepchange. The results show clear evidence of boundary-layer contraction when suction velocity is increased.     

Optimum velocity for a person moving under rain

The total rain received by a moving body has previously been modelled by defining a wetness function. Several cases such as one-dimensional motion of an inclined plane, two-dimensional motion of an inclined plane, motion with time-varying velocity, inclined rain for an inclined plane, rain on a cylindrical surface and three-dimensional motion of a convex body were treated in detail. One of the major conclusions was that for a fixed distance, assuming vertical rain, the body should travel as fast as possible since the total wetness decreases with increasing velocity. The wetness function was shown to decrease asymptotically to a constant value as the velocity increases and in the high-speed range, increasing the velocity does not decrease the wetness substantially. One might think that the excess amount of energy required for a higher speed does not compensate for the small fraction of decrease in wetness. In this work, criteria are developed for a critical speed (optimum speed), for which the wetness is small enough for a reasonable energy consumption. Three cases are investigated: (1) vertical rain; (2) rain inclined towards the body; (3) rain inclined away from the body. In the first two cases, there is no absolute minimum for the wetness function and the optimum velocity is determined by special criteria. The third case is somewhat different, however, and if the inclination angle is higher than a critical value, an absolute minimum for wetness is obtained and the optimum velocity for this case is defined to be the velocity corresponding to this absolute minimum. Therefore the definition of optimum velocity is qualitatively different from the first two cases.     

On MHD flow along an infinite flat wall with constant suction

Exact solutions of the Navier-Stokes equations are derived by a Laplace-transform technique for two-dimensional, incompressible flow of an electrically conducting fluid past an infinite porous plate under the action of a transverse magnetic field subject to the conditions: (i) the magnetic Prandtl number P_m is unity, and (ii) the Alfven velocity is less than the suction velocity. It is assumed that the flow is independent of the distance parallel to the plate and that the velocity component normal to the plate is constant. General formulae are derived for the velocity distribution and the magnetic field in terms of the given external velocity. The skin-friction is obtained and some special cases are considered.     

Flocking dynamics for a multiagent system involving task strategy

Collective behavior sometimes requires forming a particular formation or reaching a certain velocity to accomplish a specific task, such as bird migration. In this paper, we investigate the collective migration model, which consists of two parts: Cucker–Smale type interaction and target velocity. Each agent has a strategy to allocate limited energy to group interaction and velocity tracking. In this case, if the system achieves monocluster flocking then the final velocity is equal to target velocity. When the strategy is invariant, we show that 1/2 is a critical threshold which is consistent with the classical Cucker–Smale model. When the strategy is time varying, we provide a time-varying strategy named threshold strategy to ensure that for any initial state the system achieves monocluster flocking and the final velocity reaches target velocity. In addition, the case of multiple target velocities is considered. According to the theory of bicluster flocking, we obtain a sufficient framework to guarantee that the system achieves bicluster flocking and two groups would reach their target velocities, respectively.     

A model for the corona of a spherical star cluster

A general model for the outer layers of steady spherical star systems is considered. The corona is assumed to be formed by stars flying out of the system along ballistic orbits. Expressions for density runs and velocity dispersions are found. Models of three kinds are studied, namely, systems with isotropic velocity distribution, spheres with purely radial orbits, and models with ellipsoidal velocity distribution. The following isotropic distribution functions were considered as examples: the truncated Maxwellian distribution, King’s model, and the spherical analogue of Perek’s model. The truncated Maxwellian distribution of radial velocities is an example of a radial orbit system. The truncated Schwarzschildian velocity distribution and generalized polytropes introduced by Kuzmin and Veltmann are examples of models with ellipsoidal velocity distribution. Density asymptotics are found for all models provided that the self-gravitation of coronas is neglected.