BLACK HOLE THERMODYNAMICS FOR PRODUCING HORIZON OSCILLATIONS
Journal Title: Aerospace Research in Bulgaria - Year 2016, Vol 28, Issue
Abstract
We present a scenario for addressing the information loss problem in black holes which preserves the unitarity of the S-matrix. Our approach is based on quantizing the curvature singularity using classical non-commutative geometry. Also we take advantage of the developments in unification of quantum mechanics and gravity to provide a two-dimensional holographic description of the event horizon. Hence we discretize the holographic screen (horizon) into individual pixels, Planck area in size, each carrying a degree of freedom. We provide a generic phenomenon which arises naturally from black hole perturbation theory to produce a remnant-free final stage evolution and omit the necessity of introducing an additional membrane, as it has been proposed by Susskind. A stronger version of the Page’s argument regarding the no-cloning theorem is considered.
Authors and Affiliations
Alexander Yosifov, Lachezar Filipov
Keywords
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