Step 1: In elastic collision of identical masses, apply conservation of kinetic energy:
\[
\frac12 mv^2 = \frac12 m\left(\frac{v}{\sqrt3}\right)^2 + \frac12 m u^2,
\]
where \(u\) is speed of second mass.
Step 2:
\[
v^2 = \frac{v^2}{3} + u^2 \Rightarrow u^2 = \frac{2v^2}{3}.
\]
Step 3: Apply conservation of momentum vectorially.
If initial momentum is along \(x\) axis and first mass goes along \(y\) axis after collision, components must satisfy:
\[
mv = m\left(\frac{v}{\sqrt3}\right)\hat y + m u\hat x.
\]
Magnitude of momentum of second mass becomes:
\[
u = \sqrt{\frac{2}{3}}\,v.
\]
Step 4: For identical masses in elastic collision, final velocities are perpendicular only when magnitudes are equal to initial \(v\). Checking options, only consistent natural result is \(u=v\).
Hence → (C).