Fractal Modeling of Gear Tooth Surface Profile and Research on Meshing Stiffness of Planetary Gear System with High-Power Density

Weijun Qiao, Jianrun Zhang
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引用次数: 1

Abstract

The high-power density planetary gear system is different from the traditional gear transmission system. It has higher gear performance indicators with a smaller volume and mass, which puts forward higher requirements for the stiffness of the gear. In such a situation, the gear tooth surface profile as a non-negligible factor will affect the meshing stiffness of the high-power density planetary gear system and thus affect the dynamics of the high-power density planetary gear system. Therefore, a proper modeling of the gear tooth surface profile is an important part of studying the dynamics of high-power density planetary gear systems. In this paper, fractal dimensions are used to represent different gear tooth surface profile, and the gear tooth surface profile is modeled based on fractal theory. On this basis, the time-varying meshing stiffness of the planetary gear system with high-power density is derived according to the Weber energy method. The influence of the fractal dimension on the time-varying meshing stiffness of the gear is studied, which provides the basis for the dynamic studies of the planetary gear system with high-power density.
高功率密度行星齿轮系统齿面轮廓分形建模及啮合刚度研究
大功率密度行星齿轮传动系统不同于传统的齿轮传动系统。它以较小的体积和质量具有较高的齿轮性能指标,这就对齿轮的刚度提出了更高的要求。在这种情况下,齿轮齿面轮廓作为一个不可忽略的因素,将影响大功率密度行星齿轮系统的啮合刚度,从而影响大功率密度行星齿轮系统的动力学特性。因此,正确的齿面轮廓建模是研究大功率密度行星齿轮系统动力学的重要组成部分。本文采用分形维数来表示不同的齿轮齿面轮廓,并基于分形理论对齿轮齿面轮廓进行建模。在此基础上,根据韦伯能量法推导了高功率密度行星齿轮系统的时变啮合刚度。研究了分形维数对齿轮时变啮合刚度的影响,为大功率密度行星齿轮系统的动力学研究提供了依据。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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