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      Nonpropagation of massive mode on AdS2 in topologically massive gravity

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          Abstract

          Making use of Achucarro-Ortiz (AO) type of dimensional reduction, we study the topologically massive gravity with a negative cosmological constant on AdS2 spacetimes. For a constant dilaton, this two-dimensional model also admits three AdS2 vacuum solutions, which are related to two AdS3 and warped AdS3 backgrounds with an identification upon uplifting three dimensions. We carry out the perturbation analysis around these backgrounds to find what is a physically propagating field. However, it turns out that there is no propagating massive mode on AdS2 background, in contrast to the Kaluza-Klein (KK) type of dimensional reduction. We note that two dimensionally reduced actions are different and thus, the non-equivalence of their on-shell amplitudes is obtained.

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          Massive Gravity in Three Dimensions

          A particular higher-derivative extension of the Einstein-Hilbert action in three spacetime dimensions is shown to be equivalent at the linearized level to the (unitary) Pauli-Fierz action for a massive spin-2 field. A more general model, which also includes `topologically-massive' gravity as a special case, propagates the two spin 2 helicity states with different masses. We discuss the extension to massive \({\cal N}\)-extended supergravity, and we present a `cosmological' extension that admits an anti-de Sitter vacuum.
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            Three-dimensional Chern-Simons black holes

            We construct black hole solutions to three-dimensional Einstein-Maxwell theory with both gravitational and electromagnetic Chern-Simons terms. These intrinsically rotating solutions are geodesically complete, and causally regular within a certain parameter range. Their mass, angular momentum and entropy are found to satisfy the first law of black hole thermodynamics. These Chern-Simons black holes admit a four-parameter local isometry algebra, which generically is \(sl(2,R)\times R\), and may be generated from the corresponding vacua by local coordinate transformations.
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              Relating black holes in two and three dimensions

              , (2010)
              The three dimensional black hole solutions of Ba\~nados, Teitelboim and Zanelli (BTZ) are dimensionally reduced in various different ways. Solutions are obtained to the Jackiw-Teitelboim theory of two dimensional gravity for spinless BTZ black holes, and to a simple extension with a non-zero dilaton potential for black holes of fixed spin. Similar reductions are given for charged black holes. The resulting two dimensional solutions are themselves black holes, and are appropriate for investigating exact ``S-wave'' scattering in the BTZ metrics. Using a different dimensional reduction to the string inspired model of two dimensional gravity, the BTZ solutions are related to the familiar two dimensional black hole and the linear dilaton vacuum.
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                Author and article information

                Journal
                27 January 2009
                2010-04-23
                Article
                10.1140/epjc/s10052-010-1333-3
                0901.4390
                1c3bb978-6958-4ccd-a3b2-460fecd87972

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                Eur.Phys.J.C67:533-541,2010
                19 pages, version to appear in EPJC
                hep-th gr-qc

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