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The DSR-deformed relativistic symmetries and the relative locality of 3D quantum gravity (1210.7834v1)

Published 29 Oct 2012 in hep-th and gr-qc

Abstract: Over the last decade there were significant advances in the understanding of quantum gravity coupled to point particles in 3D (2+1-dimensional) spacetime. Most notably it is emerging that the theory can be effectively described as a theory of free particles on a momentum space with anti-deSitter geometry and with noncommutative spacetime coordinates of the type $[x{\mu},x{\nu}]=i \hbar \ell \varepsilon{\mu\nu}_{\phantom{\mu\nu}\rho} x{\rho}$. We here show that the recently proposed relative-locality curved-momentum-space framework is ideally suited for accommodating these structures characteristic of 3D quantum gravity. Through this we obtain an intuitive characterization of the DSR-deformed Poincar\'e symmetries of 3D quantum gravity, and find that the associated relative spacetime locality is of the type producing dual-gravity lensing.

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