$\left(k = \frac{1}{4\pi\epsilon_0} \text{ and } r_0 = k \frac{Z e^2}{m v_0^2}\right)$
The interaction between the $\alpha$ particle and the nucleus is governed by the Coulomb force. This force is a central force, meaning it always acts along the line connecting the two particles. A key consequence of a central force is the conservation of angular momentum.
Let $m$ be the mass of the $\alpha$ particle.
$ L_i = m v_0 b $
$ L_f = m v_m r_m $
Since angular momentum is conserved during the scattering process:
$ L_i = L_f $
Substituting the expressions for $L_i$ and $L_f$:
$ m v_0 b = m v_m r_m $
Dividing both sides by the mass $m$ gives:
$ v_0 b = v_m r_m $
This relationship holds true based on the conservation of angular momentum. Therefore, the option stating $v_0 b = v_m r_m$ is correct.
The other options involve considerations of energy conservation and approximations under specific conditions, such as when the impact parameter is much smaller than the characteristic length scale $r_0$.
Consider the potential $U(r)$ defined as $$U(r) = -U_0 \frac{e^{- \alpha r}}{r}$$ where $ \alpha$ and $U_0$ are real constants of appropriate dimensions. According to the first Born approximation, the elastic scattering amplitude calculated with $U(r)$ for a (wave-vector) momentum transfer $q$ and $ \alpha \to 0$, is proportional to
(Useful integral: $ \int_0^{ \infty} \sin(qr)e^{- \alpha r} dr = \frac{q}{ \alpha^2+q^2}$)