Peng Qiu-he, Huang Ke-lian, Huang Jie-hao, Li Xiao-qing, Su Hong-jun
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Integration of Poisson's equation for a disk galaxy of finite thickness
Assuming a density perturbance in the form of an Archimedes spiral and an exponential decrease of matter density along the z-direction, Poisson's equation governing the perturbed gravitational field is solved with Hankel's integral transform and the method of steepest descent. For shortwave perturbances in the plane z=0, a simple analytical expression is given. In our approximation, the form of the perturbed field is determinate and is also an Archimedes spiral.
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