For a quantum mechanically Gaussian shaped, electrically charged, massive particle, we compute th... more 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–Nordstrom space-time when the charge-to-mass ratio \(0 1\). 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.
For a quantum mechanically Gaussian shaped, electrically charged, massive particle, we compute th... more 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–Nordstrom space-time when the charge-to-mass ratio \(0 1\). 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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Papers by Octavian Micu