A compact cylindrical Green's function expansion for the solution of potential problems

被引:118
作者
Cohl, HS [1 ]
Tohline, JE [1 ]
机构
[1] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA
关键词
galaxies : formation; galaxies : structure; methods : analytical; stars : formation;
D O I
10.1086/308062
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that an exact expression for the Green's function in cylindrical coordinates is [GRAPHICS] where chi = [R-2 + R'(2) + (z - z')(2)]/(2RR'), and Q(m-1/2) is the half-integer degree Legendre function of the second kind. This expression is significantly more compact and easier to evaluate numerically than the more familiar cylindrical Green's function expression, which involves infinite integrals over products of Bessel functions and exponentials. It also contains far fewer terms in its series expansion-and is therefore more amenable to accurate evaluation-than does the familiar expression for \x - x'\(-1) that is given in terms of spherical harmonics. This compact Green's function expression is well suited for the solution of potential problems in a wide variety of astrophysical contexts because it adapts readily to extremely flattened (or extremely elongated), isolated mass distributions.
引用
收藏
页码:86 / 101
页数:16
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