Deformed Density Matrix and Quantum Entropy of the Black Hole
arXiv:gr-qc/0603068 · doi:10.3390/e8010031
Abstract
In the present work the approach - density matrix deformation - earlier developed by the author to study a quantum theory of the Early Universe (Planck's scales) is applied to study a quantum theory of black holes. On this basis the author investigates the information paradox problem, entropy of the black hole remainders after evaporation, and consistency with the holographic principle. The possibility for application of the proposed approach to the calculation of quantum entropy of a black hole is considered.
17 pages, Latex, new reference
References in corpus (11)
- Black holes and information theory
- Do black holes radiate?
- Light-sheets and Bekenstein's bound
- Deformed Density Matrix and Generalized Uncertainty Relation in Thermodynamics
- Non-Unitary and Unitary Transitions in Generalized Quantum Mechanics, New Small Parameter and Information Problem Solving
- Quantum Mechanics at Planck's scale and Density Matrix
- Flat space physics from holography
- Quantum Mechanics of the Early Universe and its Limiting Transition
- Pure States, Mixed States and Hawking Problem in Generalized Quantum Mechanics
- The Universe as a Nonuniform Lattice in Finite-Volume Hypercube. I.Fundamental Definitions and Particular Features
- The Density Matrix Deformation in Physics of the Early Universe and Some of its Implications
Cited by in corpus (5)
- Entropy In The Present And Early Universe: New Small Parameters And Dark Energy Problem
- Quantum Theory at Planck Scale, Limiting Values, Deformed Gravity and Dark Energy Problem
- Deformed Quantum Field Theory, Thermodynamics at Low and High Energies, and Gravity. I
- The Black Hole Quantum Entropy and Its Minimal Value
- Probable Entropic Nature of Gravity in Ultraviolet and Infrared Limits, Part I. An Ultraviolet Case