TY  - JOUR
AU  - Olmo, G. J.
AU  - Rubiera-Garcia, D.
AU  - Sanchez-Puente, A.
PY  - 2016
DA  - 2016//
TI  - Impact of curvature divergences on physical observers in a wormhole space-time with horizons
T2  - Class. Quantum Gravity
JO  - Classical and Quantum Gravity
SP  - 115007
EP  - 12pp
VL  - 33
IS  - 11
PB  - Iop Publishing Ltd
KW  - Singularities
KW  - black holes
KW  - metric-affine geometry
AB  - 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-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.
SN  - 0264-9381
UR  - http://arxiv.org/abs/1602.01798
UR  - https://doi.org/10.1088/0264-9381/33/11/115007
DO  - 10.1088/0264-9381/33/11/115007
LA  - English
N1  - WOS:000377442000010
ID  - Olmo_etal2016
ER  -