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.
1989
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].
Balbinot R.; Barletta A.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/873589
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