Numerical Analysis of Galactic Rotation Curves
  In this paper we present the discussion on the salient points of the
computational analysis that are at the basis of the paper \emph{Rotation Curves
of Galaxies by Fourth Order Gravity} \citep{StSc}. In fact in this paper any
galactic component (bulge, disk and Dark matter component) required an onerous
numerical computation since the Gauss theorem is not applicable in the Fourth
Order Gravity. The computational and data analysis have been made with the
software Mathematica$^\circledR$.
