Model of black hole evolution

Abstract

From the postulate that a black hole can be replaced by a boundary on the apparent horizon with suitable boundary conditions, an unconventional scenario for the evolution emerges. Only an insignificant fraction of energy of order $(mG{)}^{-1}$ is radiated out. The outgoing wave carries a very small part of the quantum mechanical information of the collapsed body, the bulk of the information remaining in the final stable black hole geometry.

9 pages, harvmac, 3 figures, minor additions

References in corpus (4)

• On the Origin of the Outgoing Black Hole Modes
• Black Hole Horizons and Complementarity
• Entropy and black hole horizons
• Black holes by analytic continuation

Cited by in corpus (4)

• Analogue Gravity
• The Information Problem in Black Hole Evaporation: Old and Recent Results
• An Implication of "Gravity as the Weakest Force"
• Black holes by analytic continuation