Different versions of the Robertson-Walker Metric One form of the Robertson-Walker metric is $$ds^2 = c^2dt^2 - a(t)^2[d\chi^2+ S_k(\chi)^2(d\theta^2 + \sin^2\theta ~d\phi^2)]\tag{1}$$
$$\\$$
Considering curvature, where k = 0 , +1, -1 for flat, positive and negative curvatures respectively, then: $$S_k(\chi) = \begin{cases}R\sin(\chi/R)~~~~~~(k=+1)\\\chi~~~~~~~~~~~~~~~~~~~~~~~(k=0)\\R\sinh(\chi/R)~~~~(k=-1)\end{cases}$$
$$\\$$
But another form of this metric is $$ds^2=c^2dt^2 - a(t)^2\left[\frac{dr^2}{1-kr^2} + r^2(d\theta^2+\sin^2~d\phi^2)\right]\tag{2}$$
$$\\$$
How does one go from $(1)$ to $(2)$? (or vice versa) I get that this is due to a switch of choice of coordinates, from radial to co-moving radial, I think? But how can it be shown that they represent the same metric?
 A: From what I understood in my cosmology course, you simply normalize the metric $(1)$ by taking
\begin{equation}
\chi(r)=\int\frac{1}{\sqrt{1-kr^2}}\ \mathrm{d}r\tag{int}
\end{equation}
This integral has 3 different solutions based on the value of $k$ which is your curvature
\begin{equation}
\chi(r)=\left\{\begin{aligned}
&\frac{1}{\sqrt{k}}\sin^{-1}\left(r\sqrt{k}\right)&k>0\\
&r&k=0\\
&\frac{1}{\sqrt{|k|}}\sinh^{-1}\left(r\sqrt{|k|}\right)&k<0
\end{aligned}\right.\tag{sol}
\end{equation}
Through inversion of $(\mathrm{sol})$ you get your $S_k(\chi)$ function, which gives your $r$
\begin{equation}
r(\chi)=S_k(\chi)=\left\{\begin{aligned}
&\frac{1}{\sqrt{k}}\sin\left(\chi\sqrt{k}\right)&k>0\\
&\chi&k=0\\
&\frac{1}{\sqrt{|k|}}\sinh\left(\chi\sqrt{|k|}\right)&k<0
\end{aligned}\right.\tag{2}
\end{equation}
Now, writing our differential we get
\begin{equation}
\left\{\begin{aligned}
\mathrm{d}\chi^2&=\frac{1}{1-kr^2}\mathrm{d}r^2\\\hfill\\
r^2&\left(\mathrm{d}\theta^2+\sin^2(\theta)\mathrm{d}\phi^2\right)=S_k^2(\chi)\left(\mathrm{d}\theta^2+\sin^2(\theta)\mathrm{d}\phi^2\right)
\end{aligned}\right.
\end{equation}
And there you are, it should be what you are searching for if I got the question correctly
