What is the proof for Bertrand's theorem in celestial mechanics?

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Homework Statement
I don't know how I can find the equation (2.78) and the next equations. It is from Classical Dynamics: A Contemporary Approach: Jorge V.
Relevant Equations
integral equation of energy (central problem)
Scanned textbook page on Bertrand's theorem with equations for the orbit angle, the limits for positive and negative k, and the conclusions k = 2 and k = -1.
 
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Usually you will start from ##\mathcal{L} = \frac{1}{2}\mu v^2 - V## and then write\begin{align*}
\frac{1}{2}\mu v^2 + V &= E \\

\frac{1}{2} \mu (\dot{r}^2 + r^2\dot{\varphi}^2) + V(r) &= E
\end{align*}Also ##\varphi## doesn't appear in the Lagrangian so ##\partial \mathcal{L} / \partial \dot{\varphi} = \mu r^2 \dot{\varphi} := L## is conserved, so you can replace ##\tilde{V}(r) := \frac{1}{2} \mu r^2 \dot{\varphi}^2 + V(r) = \dfrac{L^2}{2\mu r^2} + V(r)##. Further, write ##\dot{r} = \dfrac{dr}{d\varphi} \dot{\varphi} = \dfrac{dr}{d\varphi} \dfrac{L}{\mu r^2}## so that\begin{align*}
\frac{L^2}{2\mu^2 r^4} \left( \dfrac{dr}{d\varphi} \right)^2 + \tilde{V}(r) = E
\end{align*}which is simple to invert to the integral\begin{align*}

\varphi(r) = \sqrt{\frac{L^2}{2\mu}} \int^r \frac{dr}{r^2\sqrt{E - \tilde{V}(r)}}

\end{align*}The classic substitution is now ##u=1/r##, which transforms this into\begin{align*}

\tilde{\varphi}(u) = -\sqrt{\frac{L^2}{2\mu}} \int^{u} \frac{du}{\sqrt{E - \tilde{W}(u)}}

\end{align*}Of course we can also take the integral between the minimum and maximum ##u## of the orbit, and using the scaling ##u = yu_{\mathrm{max}}## given in the image the integral becomes\begin{align*}

\Theta := \varphi(r_{\mathrm{max}}) - \varphi(r_{\mathrm{min}}) = \sqrt{\frac{L^2}{2\mu}} \int_{v_{\mathrm{min}}}^1 \frac{u_{\mathrm{max}} dy}{\sqrt{E - \tilde{U}(y)}}

\end{align*}You should notice that since ##\tilde{V}(r) = \dfrac{L^2}{2\mu r^2} + V(r)##, that ##\tilde{W}(u) = \dfrac{L^2 u^2}{2\mu } + V\left(\dfrac{1}{u} \right)##. If we let ##V(r) = \alpha r^k## then ##\tilde{W}(u) = \dfrac{L^2 u^2}{2\mu } + \alpha u^{-k}##. Finally when we substitute for ##y## we see that\begin{align*}
\tilde{U}(y) = \dfrac{L^2 y^2 u_{\mathrm{max}}^2}{2\mu } + \alpha u_{\mathrm{max}}^{-k} y^{-k} = y^2 u_{\mathrm{max}}^2 \left( \dfrac{L^2 }{2\mu } + \alpha (yu_{\mathrm{max}})^{-(k+2)}\right) = u_{\mathrm{max}}^2 \mathcal{Y}(y)
\end{align*}Furthermore ##u_{\mathrm{max}}^2 \mathcal{Y}(1) = \dfrac{L^2 u_{\mathrm{max}}^2}{2\mu} + \alpha (u_{\mathrm{max}})^{-k} = E## is just the energy evaluated at the minimum radius, hence\begin{align*}
\Theta = \sqrt{\frac{L^2}{2\mu}} \int_{v_{\mathrm{min}}}^1 \frac{dy}{\sqrt{\mathcal{Y}(1) - \mathcal{Y}(y)}}
\end{align*}Although I can't comment on the line at the very end of the proof without seeing "equation (2.77)", hope it's somewhat helpful.
 
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