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Asymptotic symmetries in 3d gravity with torsion

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arxiv gr-qc/0301051 v1 pith:QL2BIS7Q submitted 2003-01-15 gr-qc hep-th

Asymptotic symmetries in 3d gravity with torsion

classification gr-qc hep-th
keywords asymptoticgravitysymmetriestorsionalgebraanti-deasymptoticallycanonical
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We study the nature of asymptotic symmetries in topological 3d gravity with torsion. After introducing the concept of asymptotically anti-de Sitter configuration, we find that the canonical realization of the asymptotic symmetry is characterized by the Virasoro algebra with classical central charge, the value of which is the same as in general relativity: c=3l/2G.

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  1. Non-Relativistic Chern-Simons Supergravity with Torsion

    hep-th 2026-04 unverdicted novelty 7.0

    A parameterized family of non-relativistic supergravity theories with torsion is obtained in three dimensions from the semigroup expansion of an N=2 supersymmetric Mielke-Baekler algebra.