Classical and quantum geometry of moduli spaces in three-dimensional gravity
J. E. Nelson, R. F. Picken

TL;DR
This paper explores the classical and quantum geometric structures of the phase space in 3D Einstein gravity with a torus topology and negative cosmological constant, using holonomy matrices and their quantization.
Contribution
It introduces a novel approach to quantize the phase space of 3D gravity via holonomy matrices satisfying q-commutation relations, extending classical geometric brackets.
Findings
Quantization leads to non-commuting holonomy matrices.
The Goldman bracket is quantized in this framework.
Provides a geometric interpretation of quantum moduli space.
Abstract
We describe some results concerning the phase space of 3-dimensional Einstein gravity when space is a torus and with negative cosmological constant. The approach uses the holonomy matrices of flat SL(2,R) connections on the torus to parametrise the geometry. After quantization, these matrices acquire non-commuting entries, in such a way that they satisfy q-commutation relations and exhibit interesting geometrical properties. In particular they lead to a quantization of the Goldman bracket.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Advanced Operator Algebra Research
