Let be a pp–wave type spacetime endowed with the metric , where is any Riemannian manifold and an arbitrary function. We show that the behaviour of at spatial infinity determines the causality of , say: (a) if behaves subquadratically (i.e, essentially for some and large distance to a fixed point) and the spatial part $(M_0, <\cdot,\cdot>_x) M$ is globally hyperbolic, (b) if grows at most quadratically (i.e, $-H(x,u) \leq R_1(u) |x|^{2}|x|M$ is always causal, but there are non-distinguishing examples (and thus, non-strongly causal), even when , for small $\epsilon
0$. Therefore, the classical model , $H(x,u) = \sum_{i,j} h_{ij}(u) x_i x_j (\not\equiv 0)$, which is known to be strongly causal but not globally hyperbolic, lies in the critical quadratic situation with complete . This must be taken into account for realistic applications. In fact, we argue that will be subquadratic (and the spacetime globally hyperbolic) if is asymptotically flat. The relation of these results with the notion of astigmatic conjugacy and the existence of conjugate points is also discussed.

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