Nucleated black holes in de Sitter space evaporate via standard Hawking radiation back to the empty vacuum, rendering nucleation a temporary fluctuation.
Trace anomaly of a conformally invariant quantum field in curved spacetime
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Backreaction in semiclassical scalar QED in 1+1D avoids instabilities and produces over-screening at high external charges.
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The Fate of Nucleated Black Holes in de Sitter Quantum Gravity
Nucleated black holes in de Sitter space evaporate via standard Hawking radiation back to the empty vacuum, rendering nucleation a temporary fluctuation.