Notes on a quantum gravitational collaps

Details Notes on a quantum gravitational collaps Notes on a quantum gravitational collaps

2000-12-30

arxiv.org/abs/gr-qc/0101004v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

The Ninth Marcel Grossmann Meeting

Scientific paper

Everybody knows what the classical black holes are. In short, this is a spacetime region beyond the so-called event horizon. The notion of the event horizon is mathematically well defined. The situation with a definition of quantum black hole is not so clear. The problem is that the classical event horizon can be defined only globally, i.e. in order to be sure we have a black hole we would need an infinite time interval. But, in classical physics we have trajectories off all the particles and equations of motion for all the fields and can, in principle, construct some ideal models for the gravitational collapse and study the black hole formation under different conditions.

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