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Vacuum polarization in Schwarzschild space-time by anomaly induced effective actions
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Vacuum polarization in Schwarzschild space-time by anomaly induced effective actions
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The characteristic features of $<T_{\mu\nu}>$ in the Boulware, Unruh and Hartle-Hawking states for a conformal massless scalar field propagating in the Schwarzschild space-time are obtained by means of effective actions deduced by the trace anomaly. The actions are made local by the introduction of auxiliary fields and boundary conditions are carefully imposed on them in order to select the different quantum states.
Forward citations
Cited by 4 Pith papers
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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.
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Conformally Invariant Corrections to the Anomaly-Induced Effective Action and Black Hole Evaporation in Four Dimensions
Conformally invariant corrections to the anomaly-induced effective action produce a one-parameter family of quantum hair for Schwarzschild black holes that modifies the near-horizon stress tensor in a static approximation.
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Wald-like entropy and Islands in Dimensionally Reduced Einstein-Hilbert Gravity
Wald-like Noether charge of the DREH plus Polyakov-Liouville action yields the island generalized entropy and unitary Page curves for eternal and quasi-stationary evaporating black holes.
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Hawking radiation from a semi-classical Schwarzschild black hole
Quantum corrections to Schwarzschild black hole evaporation produce a maximum temperature, radiation cessation, an extremal remnant, and logarithmic entropy correction.
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