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Lecture notes on Chern-Simons (super-)gravities. Second edition (February 2008)

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arxiv hep-th/0502193 v4 pith:GVTYATFI submitted 2005-02-22 hep-th

classification hep-th
keywords dimensionschern-simonsconnectiongaugetheoriestheoryactionfield
verification ladder T0 review T1 audit T2 compute T3 formal
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This is intended as a broad introduction to Chern-Simons gravity and supergravity. The motivation for these theories lies in the desire to have a gauge invariant system --with a fiber bundle formulation-- in more than three dimensions, which could provide a firm ground for constructing a quantum theory of the gravitational field. The starting point is a gravitational action which generalizes the Einstein theory for dimensions D>4 --Lovelock gravity. It is then shown that in odd dimensions there is a particular choice of the arbitrary parameters of the action that makes the theory gauge invariant under the (anti-)de Sitter or the Poincare groups. The resulting lagrangian is a Chern-Simons form for a connection of the corresponding gauge groups and the vielbein and the spin connection are parts of this connection field. These theories also admit a natural supersymmetric extension for all odd D where the local supersymmetry algebra closes off-shell and without a need for auxiliary fields. No analogous construction is available in even dimensions. A cursory discussion of the unexpected dynamical features of these theories and a number of open problems are also presented.

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Cited by 2 Pith papers

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  1. Holographic $s$- and $p$-wave superconductors from the $4D$ regularization of Einstein-Lovelock theory

    hep-th 2026-06 unverdicted novelty 6.0 of 10

    Higher-order curvature corrections in 4D regularized Lovelock gravity raise the critical temperature of holographic s- and p-wave superconductors for negative coupling α, with the gap frequency also depending on the c...

  2. Gauge Symmetries, Exact Symmetries and Conserved Charges in Minimal Massive Gravity

    hep-th 2025-07 conditional novelty 6.0 of 10

    Minimal Massive Gravity has three gauge symmetries, and a newly constructed transformation generates exact symmetries and a conserved charge in a restricted parameter limit.

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