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hep-th2005
Backreaction of the Hawking radiation
G. A. Vilkovisky
Black holes create a vacuum matter charge to protect themselves from the quantum evaporation. A spherically symmetric black hole having initially no matter charges radiates away ab…
hep-th2005
Radiation equations for black holes
G. A. Vilkovisky
It has been shown in the previous paper that the metric in the semiclassical region of the collapse spacetime is expressed purely kinematically through the Bondi charges. Here the…
hep-th2005
Kinematics of evaporating black holes
G. A. Vilkovisky
The correspondence principle and causality divide the spacetime of a macroscopic collapsing mass into three regions: classical, semiclassical, and ultraviolet. The semiclassical re…