An approach toward a self-consistent treatment, at a semiclassical level, of black hole evaporation is presented. The different backreaction effects of massless scalar and vector fields are discussed. On this basis a new evolution scheme for evaporating black holes is suggested in which the evaporation comes to an end before all mass is radiated away.
Balbinot R., Barletta A. (1989). The backreaction and the evolution of quantum black holes. CLASSICAL AND QUANTUM GRAVITY, 6(2), 195-202 [10.1088/0264-9381/6/2/013].
The backreaction and the evolution of quantum black holes
Balbinot R.;Barletta A.
1989
Abstract
An approach toward a self-consistent treatment, at a semiclassical level, of black hole evaporation is presented. The different backreaction effects of massless scalar and vector fields are discussed. On this basis a new evolution scheme for evaporating black holes is suggested in which the evaporation comes to an end before all mass is radiated away.File in questo prodotto:
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