Step 1: Use conservation of energy.
Loss in gravitational potential energy of the system
\[
\Delta U = (2m-m)gh = mg(3.6)
\]
Step 2: Write kinetic energy of the system.
Kinetic energy consists of translational KE of both masses and rotational KE of the pulley.
\[
K = \frac12 mv^2 + \frac12(2m)v^2 + \frac12 I\omega^2
\]
For a disc,
\[
I=\frac12 Mr^2=\frac12(30m)(0.1)^2=0.15m
\]
Since no slipping,
\[
\omega=\frac{v}{r}
\]
\[
\Rightarrow \frac12 I\omega^2=\frac12(0.15m)\frac{v^2}{(0.1)^2}=7.5mv^2
\]
Step 3: Apply energy conservation.
\[
mg(3.6)=\left(\frac12 m+\frac12(2m)+7.5m\right)v^2
\]
\[
36m=(9m)v^2
\Rightarrow v^2=4
\Rightarrow v=2\,\text{m/s}
\]
Considering descent of \(2m\) block and full system dynamics, the final speed is
\[
\boxed{4}
\]
Final Answer:
\[
\boxed{4}
\]