6533b86cfe1ef96bd12c8cb7
RESEARCH PRODUCT
Impact of curvature divergences on physical observers in a wormhole space-time with horizons
Diego Rubiera-garciaGonzalo J. OlmoGonzalo J. OlmoAntonio Sanchez-puentesubject
PhysicsHigh Energy Physics - TheoryPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsGeneral relativitySpace timeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Curvature01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum CosmologyExact solutions in general relativityHigh Energy Physics - Theory (hep-th)Causal contact0103 physical sciencesMinkowski spaceWormhole010306 general physicsSchwarzschild radiusdescription
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.
year | journal | country | edition | language |
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2016-02-04 |