Charged, radiating black holes, inflation, and cosmic censorship

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Abstract
A Vaidya-Bonner-based model of a charged evaporating black hole is examined during the inflationary phase of the universe. The structure and location of the apparent and event horizons of the black hole are determined. The cosmic censorship conjecture is considered within the framework of this model. It is demonstrated that the formation of supermaximal charged black holes is possible due to the inflationary phase, resulting in primordial naked singularities.

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