Black Holes, Information, and Hilbert Space for Quantum Gravity
Yasunori Nomura, Jaime Varela, and Sean J. Weinberg

TL;DR
This paper presents a quantum gravity framework for black hole formation and evaporation that preserves information, depends on the reference frame, and reconciles quantum mechanics with classical observations, including the firewall phenomenon.
Contribution
It introduces a unitary, frame-dependent description of black holes in quantum gravity that maintains information and unifies different observational perspectives.
Findings
Black hole states can be superpositions of different geometries.
Information is encoded in phases of superposed states.
Firewall phenomena require fine-tuned initial states.
Abstract
A coarse-grained description for the formation and evaporation of a black hole is given within the framework of a unitary theory of quantum gravity preserving locality, without dropping the information that manifests as macroscopic properties of the state at late times. The resulting picture depends strongly on the reference frame one chooses to describe the process. In one description based on a reference frame in which the reference point stays outside the black hole horizon for sufficiently long time, a late black hole state becomes a superposition of black holes in different locations and with different spins, even if the back hole is formed from collapsing matter that had a well-defined classical configuration with no angular momentum. The information about the initial state is partly encoded in relative coefficients---especially phases---of the terms representing macroscopically…
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Taxonomy
TopicsCosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories · Black Holes and Theoretical Physics
