A conformally invariant weight-six correction to the anomaly-induced effective action leaves a free parameter in the semiclassical stress tensor near a Schwarzschild black hole, producing quantum hair.
Gravitational vacuum condensate stars in the effective theory of gravity
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Semiclassical black hole evaporation in four dimensions produces a thunderbolt singularity signaling breakdown of the effective theory at large distances.
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Conformally Invariant Corrections to the Anomaly-Induced Effective Action and Black Hole Evaporation in Four Dimensions
A conformally invariant weight-six correction to the anomaly-induced effective action leaves a free parameter in the semiclassical stress tensor near a Schwarzschild black hole, producing quantum hair.
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Breakdown of Semiclassical Gravity in Four-Dimensional Black Hole Evaporation
Semiclassical black hole evaporation in four dimensions produces a thunderbolt singularity signaling breakdown of the effective theory at large distances.