The gravitational field of three-dimensional galaxies
The gravitational field of three-dimensional galaxies
复制标题
三维星系的引力场
DOI：
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发表时间：
1973
期刊：
影响因子：
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通讯作者：
M. Clutton
中科院分区：
文献类型：
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作者：
M. Clutton
计算引力场的最简单方法是使用一组双正交的质量势函数对。利用超球多项式，导出了一组适用于三维质量分布的函数。讨论了计算引力场的算法，试图最大化计算效率。
The simplest method of calculating gravitational fields is to use a set of biorthogonal pairs of mass-potential functions. A suitable set of functions for three dimensional mass distributions is derived which uses ultraspherical polynomials. Algorithms for computing the gravitational field are discussed which attempt to maximise computational efficiency.