A Numerical Convolution Representation of Potential for a Disk Surface Density in 3D

الملخص EN

This study presents a numerical convolution representation of a potential induced from a disk of surface density, which has often been investigated in the center region of galaxies.

The advantage of this representation is to release the softening length for the N-body method and artificial boundary conditions for the spectral methods.

With the help of fast Fourier transform, the computational complexity is only O(M2(log2M)), where M is the number of zones in one dimension.

Numerical results show an almost second order of accuracy on a Cartesian coordinate system.

A comparison study also demonstrates that this method can calculate the potential for disk surface density based on the uniform grids.