Consider an -dimensional asymptotically flat spacetime and a future-directed, affinely parametrized outgoing null generator of an achronal boundary , where is a nested family of smooth compact codimension surfaces approaching a singular boundary set in the past. In the twist-free case and under the null energy condition, the Raychaudhuri equation on the dimensional screen bundle reads, where is the tangent to . This equation linearizes, via the rescaling with the Jacobi-map -volume, to the Sturm-type ODE We develop two purely generator-wise criteria forcing a first zero of : (i) an exact Volterra identity combined with concavity leads to a barrier-weighted integral inequality, and (ii) Sturm comparison and a Prüfer-angle estimate yields failure of disconjugacy whenever on a subinterval. We prove that is equivalent to the existence of a focal (conjugate) point and implies at . Using the standard structure of achronal boundaries, this yields a geodesic-wise obstruction: if every generator that could reach satisfies one of the above conditions in the regular spacetime region, then , and hence is not globally visible. As an application, we illustrate one of these criteria in the Einstein-massless scalar field collapse model of Christodoulou.

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