1111.4332 (Ovidiu Cristinel Stoica)
Ovidiu Cristinel Stoica
An analytic extension of the Reissner-Nordstrom solution at and beyond the
singularity is presented. The extension is obtained by using new coordinates,
in which the determinant of the metric tends to 0 when approaching r=0. The
metric is still singular in the new coordinates, but its components become
finite and smooth. Using this extension is shown that the charged and
non-rotating black hole singularities are compatible with the global
hyperbolicity and with the conservation of the initial value data. Geometric
models for electrically charged particles are obtained.
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http://arxiv.org/abs/1111.4332
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