arXiv · 1604.02332
Singularity transition in a Yukawa-Reissner-Nordstr\"om spacetime
Abstract
A screened charge by a Yukawa potential implies that the corresponding electric field is assimptotically zero far away from a small radius scaling. Considering a screened charge, we have a modified metric of type Yukawa-Reissner-Nordstr\"om spacetime, that assimptotically decays from a Reissner-Nordstr\"om spacetime to a Schwarzschild spacetime. This implies that the singularity is screened by distance reducing from two singularities to one single singularity for a suitable distance. We consider the tetrad fields associated to the Yukawa-Reissner-Nordstr\"om spacetime and show that a linear motion in the proper time lead to suitable estimatives to the Yukawa screening parameter associated to a Schwarzschild radius.
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Thiago Prudencio. 2016-04-03. Singularity transition in a Yukawa-Reissner-Nordstr\"om spacetime. https://arxiv.org/abs/1604.02332
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