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Regularization of the Reissner-Nordström black hole

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Abstract.

An inner de Sitter region is glued smoothly and consistently with an outer Reissner-Nordström (RN) spacetime on a spherical thin shell. Mass and charge of the outer RN spacetime are defined by the de Sitter and shell parameters. The radius of the shell plays the role of a cut-off which, by virtue of the regular de Sitter interior removes the singularity at r = 0. The topology of the inner de Sitter region with the radius of the thin shell becomes compact. For stability the perturbed shell is shown to satisfy a modified polytropic equation of state which has vanishing mass and pressure on the unperturbed shell as dictated by the junction conditions.

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Authors and Affiliations

  1. Department of Physics, Faculty of Arts and Sciences, Eastern Mediterranean University, via Mersin 10, Famagusta, North Cyprus, Turkey

    S. Habib Mazharimousavi & M. Halilsoy

Authors
  1. S. Habib Mazharimousavi
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  2. M. Halilsoy
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Correspondence to S. Habib Mazharimousavi.

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Habib Mazharimousavi, S., Halilsoy, M. Regularization of the Reissner-Nordström black hole. Eur. Phys. J. Plus 133, 386 (2018). https://doi.org/10.1140/epjp/i2018-12194-7

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  • DOI: https://doi.org/10.1140/epjp/i2018-12194-7

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