Inspired by this question a normal extension would be to ask:
What is the minimum potential energy required (to behave as a turning point) for an elastic collision between $2$ point particles $A$ and $B$ with velocity $v_A^{\mu}$ and $v_B^{\mu}$ in a relativistic classical mechanics? (Assume number of particles are conserved)
I suspect the action should be of the form:
$$ S = -\underbrace{m_A \int d^4 x \delta^3(q^i_A(\tau_A) - x^i)}_{\text{Action of particle A}} -\underbrace{m_B \int d^4 x \delta^3(q_B^i(\tau_B) - x^i)}_{\text{Action of particle B}} - \underbrace{V_0 \int \delta^3 (x^i- q^i_c)d^4 x}_{\text{Potential behaving as turning point}} $$
where $m_k$ is the mass of the $k$'th particle, $q_k^i$ is $i$'th component of the $k$'th particle, $V_0$ is a constant, $\tau$ is the proper time and $q_c$ is the intersections of the geodesics $A$ and $B$.
P.S: Do check the question on why a naive application of Total energy $\geq$ Potential Energy will not suffice.