The following sections are included:External force problems in three dimensionsLaws of motion in non-Cartesian basesIsotropic and anisotropic oscillatorsKepler problemRutherford scattering and the discovery of the atomic nucleusSystems with velocity-dependent forcesProblems#External force problems in three ...
In all applications considered in the previous chapters of this monograph, it was assumed that the particle was in a field of a finite number of ZRPs. Now we shall consider an infinite number of...doi:10.1007/978-1-4684-5451-2_6Yu. N. Demkov...
From a consistent expression for the quadriforce describing the interaction between a colored particle and gauge fields, we investigate the relativistic motion of a particle with isospin interacting with a BPS monopole and with a Julia–Zee dyon. The analysis of such systems reveals the existence ...
A new boundary-integral algorithm for the motion of a particle between two parallel plane walls in Poiseuille flow at low Reynolds number was developed to study the translational and rotational velocities for a broad range of particle sizes and depths in the channel. Instead of the free-space Gr...
theSU(2)magnetic fieldThe motion of a particle in the instanton fieldSummary Preliminaries The equations of motion according to Wong The equations of motion according to Drechsler and Rosenblum The motion of a particle in theSU(2)magnetic field The motion of a particle in the instanton field ...
The method is based on the introduction of a fictitious attracting center with a ... VA Shefer - 《Astronomy Reports》 被引量: 21发表: 1998年 A strongly interacting dynamic particle swarm optimization method A novel dynamic interacting particle swarm optimization algorithm (DYN-PSO) is proposed....
Astrophysical plasma is often an extremely tenuous hot gas of charged particles, without net charge on average. If there are very few encounters between particles, we need only to consider the responses of a particle to the force fields in which it moves
Thus the inertial law of Galileo postulates the invariance of the dynamic equations with respect to the Galilean transformations [1.11]. Accordingly, it can be interpreted as a principle of relativity, which implies that in any inertial frame: 1. Time is the same. 2. Mass of a particle is...
Classical correlations of defects in lattices with geometrical frustration in the motion of a particle 来自 国家科技图书文献中心 喜欢 0 阅读量: 25 作者:F Pollmann,JJ Betouras,E Runge 摘要: DOI: http://dx.doi.org/10.1103/PhysRevB.73.174417 关键词: Lattice theory and statistics Theories and ...
a particle moving on the plane, the equation of motion is XOY 。The equation of motion is x=3t+5, y=1/2t2+3t-4(SI)(1) The position vectors at time t = 1s and time t = 2s are obtained, and the position shifts of these prime points in 1 second are calculated; (2) Calculate...