2+1 gravity on the conformal sphere

@article{Gryb201221GO,
  title={2+1 gravity on the conformal sphere},
  author={Sean Gryb and Flavio Mercati},
  journal={Physical Review D},
  year={2012},
  volume={87},
  pages={064006}
}
We show that there are two equivalent first order descriptions of $2+1$ gravity with a nonzero cosmological constant. One is the well-known spacetime description, and the other is in terms of evolving conformal geometry. The key tool that links these pictures is Cartan geometry, a generalization of Riemannian geometry that allows for geometries locally modeled off arbitrary homogeneous spaces. The two different interpretations suggest two distinct phase space reductions. The spacetime picture… 

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References

SHOWING 1-10 OF 36 REFERENCES

Einstein gravity as a 3D conformally invariant theory

We give an alternative description of the physical content of general relativity that does not require a Lorentz invariant spacetime. Instead, we find that gravity admits a dual description in terms

The physical gravitational degrees of freedom

When constructing general relativity (GR), Einstein required 4D general covariance. In contrast, we derive GR (in the compact, without boundary case) as a theory of evolving three-dimensional

Quantum Gravity in 2+1 Dimensions

1. Why (2+1)-dimensional gravity? 2. Classical general relativity in 2+1 dimensions 3. A field guide to the (2+1)-dimensional spacetimes 4. Geometric structures and Chern-Simons theory 5. Canonical

Conformal field theory, (2 + 1)-dimensional gravity and the BTZ black hole

In three spacetime dimensions, general relativity becomes a topological field theory, whose dynamics can be largely described holographically by a two-dimensional conformal field theory at the

de Sitter gauge invariance and the geometry of the Einstein-Cartan theory

A formulation of general relativity as a gauge theory of the de Sitter group SO(3,2) is used to analyse the geometrical structure of the Einstein-Cartan theory. The SO(3,2) symmetry must be

Quantum Gravity at a Lifshitz Point

We present a candidate quantum field theory of gravity with dynamical critical exponent equal to $z=3$ in the UV. (As in condensed-matter systems, $z$ measures the degree of anisotropy between space

On a partially reduced phase space quantization of general relativity conformally coupled to a scalar field

The purpose of this paper is twofold. On the one hand, after a thorough review of the matter free case, we supplement the derivations in our companion paper on ‘loop quantum gravity without the

The link between general relativity and shape dynamics

We define the concept of a linking theory and show how two equivalent gauge theories possessing different gauge symmetries generically arise from a linking theory. We show that under special