Constructing a counterexample to the black hole complementarity

Details Constructing a counterexample to the black hole complementarity Constructing a counterexample to the black hole complementarity

2008-02-12

arxiv.org/abs/0802.1625v3

Phys.Rev.D78:104008,2008

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, 5 figures

Scientific paper

10.1103/PhysRevD.78.104008

We propose a regular black hole whose inside generates a de Sitter space and then is finally frustrated into a singularity. It is a modified model which was suggested originally by Frolov, Markov, and Mukhanov. In our model, we could adjust a regular black hole so that its period before going into the extreme state is much longer than the information retention time. During this period an observer could exist who observes the information of the Hawking radiation, falls freely into the regular center of the black hole, and finally meets the free-falling information again. The existence of such an observer implies that the complementary view may not be consistent with a regular black hole, and therefore, is not appropriate as a generic principle of black hole physics.

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