Horizon quantization and thermodynamics of the 2+1 black hole
Michele Maggiore

TL;DR
This paper applies a horizon quantization method to the 2+1 dimensional black hole, demonstrating it accurately predicts thermodynamic properties and deriving the horizon wave function's Schrödinger equation.
Contribution
It extends a previously proposed 4D horizon quantization approach to 2+1 dimensions, using string dynamics to describe horizon behavior.
Findings
Correctly reproduces the black hole's temperature and entropy
Derives the Schrödinger equation for the horizon wave function
Validates the quantization method in lower-dimensional black holes
Abstract
We test on the 2+1 dimensional black hole the quantization method that we have previously proposed in four dimensions. While in the latter case the horizon dynamics is described, at the effective level, by the action of a relativistic membrane, in the 2+1 case it is described by a string. We show that this approach reproduces the correct value of the temperature and entropy of the 2+1 dimensional black hole, and we write down the Schroedinger equation satisfied by the horizon wave function.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
