Constructing a counterexample to the black hole complementarity

dc.creatorYeom, Dong-han
dc.creatorZoe, Heeseung
dc.date2008-02-12
dc.date2008-11-10
dc.date.accessioned2026-07-07T11:55:59Z
dc.date.available2026-07-07T11:55:59Z
dc.descriptionWe 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.
dc.description8 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/0802.1625
dc.identifierhttp://arxiv.org/abs/0802.1625
dc.identifierPhys.Rev.D78:104008,2008
dc.identifierdoi:10.1103/PhysRevD.78.104008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205432
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleConstructing a counterexample to the black hole complementarity
dc.typetext

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