The backreaction and the evolution of quantum black holes

Details The backreaction and the evolution of quantum black holes The backreaction and the evolution of quantum black holes

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cqgra...6..195b&link_type=abstract

Classical and Quantum Gravity (ISSN 0264-9381), vol. 6, Feb. 1, 1989, p. 195-202.

Statistics

Computation

23

Black Holes (Astronomy), Computational Astrophysics, Evolution (Development), Quantum Theory, Black Body Radiation, Luminosity, Space-Time Functions, Stress Tensors, Vector Spaces

Scientific paper

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.

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