Classical and quantum geometry of moduli spaces in three-dimensional gravity
J. E. Nelson, R. F. Picken
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.
Create a lesson
Related papers
High-order compact ALE gas-kinetic scheme on three-dimensional unstructured meshes
Yibo Wang, Xing Ji, Liang Pan
Multiplicity and parity in Hirota's N-soliton conditions: the bilinear families L\,(Dx3+Λ)2n+1
Shi Zhenhua
An exact unstable mode of self-similar Yang--Mills solutionsin 5+1 dimensions
Piotr Bizoń
Lorentz-Invariant Measure for Path Integrals in the Future Cone
Vladimir V. Belokurov, Vsevolod V. Chistiakov, Klavdiia A. Lursmanashvili et al.
An Excursion into Grassmannian Spectra
Dmitri Bykov, Viacheslav Krivorol
Eigenstates on O-algebras with an application to ladder operators
Fabio Bagarello, Hiroshi Inoue, Salvatore Triolo