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• W3105769504 endingPage "115007" @default.
• W3105769504 startingPage "115007" @default.
• W3105769504 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's electrodynamics and, roughly speaking, consists of two Reissner–Nordström (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." @default.
• W3105769504 created "2020-11-23" @default.
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• W3105769504 date "2016-04-28" @default.
• W3105769504 modified "2023-10-14" @default.
• W3105769504 title "Impact of curvature divergences on physical observers in a wormhole space–time with horizons" @default.
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• W3105769504 doi "https://doi.org/10.1088/0264-9381/33/11/115007" @default.
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