Abstract
For a quantum mechanically Gaussian shaped, electrically charged, massive particle, we compute the Horizon Wave-function(s) in order to study (a) the existence of the inner Cauchy horizon of the corresponding Reissner–Nordström space-time when the charge-to-mass ratio \(0<\alpha <1\) and (b) the survival of a naked singularity when the charge-to-mass ratio \(\alpha >1\). Our results suggest that any semiclassical instability one expects near the inner horizon may not occur in quantum black holes, with a mass around the Planck scale, and that no states with charge-to-mass ratio greater than a critical value (of the order of \(\sqrt{2}\)) should exist.
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Acknowledgements
We would like to thank D. Stojkovic for his contribution to the work reported here. R.C. was supported in part by the INFN grant FLAG. O.M. was supported in part by research grant UEFISCDI project PN-II-RU-TE-2011-3-0184.
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Casadio, R., Micu, O. (2018). A Quantum Cosmic Conjecture. In: Nicolini, P., Kaminski, M., Mureika, J., Bleicher, M. (eds) 2nd Karl Schwarzschild Meeting on Gravitational Physics. Springer Proceedings in Physics, vol 208. Springer, Cham. https://doi.org/10.1007/978-3-319-94256-8_14
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DOI: https://doi.org/10.1007/978-3-319-94256-8_14
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