Canonical analysis of cosmological topologically massive gravity at the chiral point
D. Grumiller, R. Jackiw, N. Johansson

TL;DR
This paper performs a canonical analysis of three-dimensional cosmological topologically massive gravity at the chiral point using a Chern-Simons formulation, revealing a local degree of freedom, the topologically massive graviton.
Contribution
It applies Wolfgang Kummer's philosophy to a 3D gravity model and introduces a new Chern-Simons representation for canonical analysis.
Findings
Physical phase space dimension is two per point.
The theory has a local physical degree of freedom, the topologically massive graviton.
The analysis confirms the presence of a propagating mode in the model.
Abstract
Wolfgang Kummer was a pioneer of two-dimensional gravity and a strong advocate of the first order formulation in terms of Cartan variables. In the present work we apply Wolfgang Kummer's philosophy, the `Vienna School approach', to a specific three-dimensional model of gravity, cosmological topologically massive gravity at the chiral point. Exploiting a new Chern-Simons representation we perform a canonical analysis. The dimension of the physical phase space is two per point, and thus the theory exhibits a local physical degree of freedom, the topologically massive graviton.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
