@Article{Olmo_etal2016, author="Olmo, G. J. and Rubiera-Garcia, D. and Sanchez-Puente, A.", title="Impact of curvature divergences on physical observers in a wormhole space-time with horizons", journal="Classical and Quantum Gravity", year="2016", publisher="Iop Publishing Ltd", volume="33", number="11", pages="115007--12pp", optkeywords="Singularities; black holes; metric-affine geometry", abstract="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{\textquoteright}s electrodynamics and, roughly speaking, consists of two Reissner-Nordstrom (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.", optnote="WOS:000377442000010", optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=2728), last updated on Thu, 07 Jul 2016 11:45:05 +0000", issn="0264-9381", doi="10.1088/0264-9381/33/11/115007", opturl="http://arxiv.org/abs/1602.01798", opturl="https://doi.org/10.1088/0264-9381/33/11/115007", archivePrefix="arXiv", eprint="1602.01798", language="English" }