Semiclassical black holes with large N rescaling and information loss problem
We consider semiclassical black holes and related rescalings with N massless fields. For a given semiclassical solution of an N = 1 universe, we can find other solution of a large N universe by the rescaling. After the rescaling, any curvature quantity takes a sufficiently small value without changing its causal structure. Via the rescaling, we argue that black hole complementarity for semiclassical black holes cannot provide a fundamental resolution of the information loss problem, and the violation of black hole complementarity requires sufficiently reasonable amounts of N. Such N might be realized from some string inspired models. Finally, we claim that any fundamental resolution of the information loss problem should resolve the problem of the singularity. ; Korean government (MOEHRD) (KRF-313-2007-C00164 / KRF-341-2007-C00010); Korea government (MEST) through Center for Quantum Spacetime (CQUeST) of Sogang University (2005-0049409)