  The impact of curvature divergences on physical observers in a black hole
space-time which, nonetheless, is geodesically complete is investigated. This
space-time is an exact solution of certain extensions of General Relativity
coupled to Maxwell's electrodynamics and, roughly speaking, consists on two
Reissner-Nordstr\"{o}m (or Schwarzschild or Minkowski) geometries connected by
a spherical wormhole near the center. We find that, despite the existence of
infinite tidal forces, causal contact is never lost among the elements making
up the observer. This suggests that curvature divergences may not be as
pathological as traditionally thought.
