Constructing a counterexample to the black hole complementarity

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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.
Publisher
AMER PHYSICAL SOC
Issue Date
2008
Language
English
Article Type
Article
Keywords

FALSE-VACUUM BUBBLES; QUANTUM INFORMATION; GRAVITATIONAL-FIELD; HAWKING RADIATION; DOMAIN-WALLS; UNIVERSE; ENTROPY; CREATION; HORIZON; WORLDS

Citation

PHYSICAL REVIEW D, v.78, no.10

ISSN
1550-7998
DOI
10.1103/PhysRevD.78.104008
URI
http://hdl.handle.net/10203/87130
Appears in Collection
RIMS Journal Papers
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