Lan Boon Leong
School of Engineering, Monash University, 46150 Petaling Jaya, Selangor, Malaysia.
Chaos. 2006 Sep;16(3):033107. doi: 10.1063/1.2218379.
The dynamics of a periodically delta-kicked Hamiltonian system moving at low speed (i.e., at speed much less than the speed of light) is studied numerically. In particular, the trajectory of the system predicted by Newtonian mechanics is compared with the trajectory predicted by special relativistic mechanics for the same parameters and initial conditions. We find that the Newtonian trajectory, although close to the relativistic trajectory for some time, eventually disagrees completely with the relativistic trajectory, regardless of the nature (chaotic, nonchaotic) of each trajectory. However, the agreement breaks down very fast if either the Newtonian or relativistic trajectory is chaotic, but very much slower if both the Newtonian and relativistic trajectories are nonchaotic. In the former chaotic case, the difference between the Newtonian and relativistic values for both position and momentum grows, on average, exponentially. In the latter nonchaotic case, the difference grows much slower, for example, linearly on average.
对低速(即速度远小于光速)运动的周期性δ驱动哈密顿系统的动力学进行了数值研究。具体而言,将牛顿力学预测的系统轨迹与在相同参数和初始条件下狭义相对论力学预测的轨迹进行了比较。我们发现,牛顿轨迹尽管在一段时间内接近相对论轨迹,但最终与相对论轨迹完全不一致,无论每条轨迹的性质(混沌、非混沌)如何。然而,如果牛顿轨迹或相对论轨迹是混沌的,这种一致性很快就会瓦解,但如果牛顿轨迹和相对论轨迹都是非混沌的,瓦解速度则要慢得多。在前一种混沌情况下,位置和动量的牛顿值与相对论值之间的差异平均呈指数增长。在后一种非混沌情况下,差异增长要慢得多,例如平均呈线性增长。