On the Singularities of Reissner-Nordstr\"{o}m Space-Time

M. Abdel-Megied; Ragab M. Gad

On the Singularities of Reissner-Nordstr\"{o}m Space-Time

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arxiv gr-qc/0402077 v2 pith:C7KFS7D5 submitted 2004-02-17 gr-qc

M. Abdel-Megied , Ragab M. Gad This is my paper · ORCID

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keywords reissner-nordstrsingularityspace-timeblackholesingularitiesbehaviorcharge

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It is shown that if two Reissner-Nordstr\"{o}m space-times, both with the same mass m and charge e, glued together in the singularities, then the light ray in black hole of the first space-time can go continuously through the singularity into black hole of the second. The behavior of tidal forces near the Reissner-Nordstr\"{o}m space-time singularity is examined by considering what happens between two particles falling freely towards the singularity.

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Geodesic deviation in the $q$-metric
gr-qc 2025-01 conditional novelty 5.0 of 10

In the q-metric, tidal stretching and compression of radially falling test particles depend on the deformation parameter q and the polar angle θ, and differ from Schwarzschild near the singularity at r=2m.

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