I'm working through the problems in Chapter 3 of the 3rd edition of Goldstein's Classical Mechanics and I'm stuck on Derivation 4. This problem asks the reader to rewrite the scattering angle
\begin{equation*} \Theta(s) = \pi - 2\int_{r_{m}}^{\infty}{\frac{s\mathrm{d}r}{\displaystyle{r\sqrt{r^{2}\left[1-\frac{V(r)}{E}\right] - s^{2}}}}} \end{equation*}
as
\begin{equation*} \Theta(s) = \pi - 4s\int_{0}^{1}{\frac{\rho\mathrm{d}\rho}{\displaystyle{\sqrt{r_{m}^{2}\left[1-\frac{V(r)}{E}\right]^{2} - s^{2}(1-\rho^{2})}}}} \end{equation*}
(where $r_{m}$, the distance of nearest approach, is such that $V(r_{m})/E = 1$) via a change of variables $r\to \rho(r)$. To attack this problem, I tried writing
\begin{equation*} \frac{\mathrm{d}r}{\displaystyle{r\sqrt{r^{2}\left[1-\frac{V(r)}{E}\right] - s^{2}}}} = \frac{\displaystyle{\frac{r_{m}}{r^{2}}\sqrt{1-\frac{V}{E}}\mathrm{d}r}}{\displaystyle{\sqrt{r_{m}^{2}\left(1-\frac{V}{r}\right)^{2} - \frac{r_{m}^{2}s^{2}}{r^{2}}\left(1-\frac{V}{E}\right)}}} \end{equation*}
which would seem to hint at $\rho$ of a form such that
\begin{equation*} s^{2}(1-\rho^{2}) = \frac{r_{m}^{2}s^{2}}{r^{2}}\left(1-\frac{V}{E}\right) \end{equation*}
or, solving for $\rho^{2}$,
\begin{equation*} \rho^{2} = 1-\frac{r_{m}^{2}}{r^{2}}\left(1-\frac{V}{E}\right). \end{equation*}
Unfortunately, this form of $\rho$ doesn't yield the correct bounds of integration, and I haven't even incorporated the Jacobian term
\begin{equation*} \mathrm{d}\rho = \frac{\mathrm{d}\rho}{\mathrm{d}r}\mathrm{d}r. \end{equation*}
Should I keep working the problem this way, or have I missed something obvious? The physical insight offered by this problem hardly seems worth the effort necessary to solve it (the author suggests its benefit is numerical stability), so I can't help feeling there's an easier way. All the same, I'd love to know what $\rho(r)$ is supposed to be.