Massive Gravity in Three Dimensions

Eric A. Bergshoeff, Olaf Hohm, and Paul K. Townsend
Phys. Rev. Lett. 102, 201301 – Published 21 May 2009

Abstract

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 N-extended supergravity, and we present a “cosmological” extension that admits an anti–de Sitter vacuum.

  • Received 21 January 2009

DOI:https://doi.org/10.1103/PhysRevLett.102.201301

©2009 American Physical Society

Authors & Affiliations

Eric A. Bergshoeff and Olaf Hohm

  • Centre for Theoretical Physics, University of Groningen, Nijenborgh 4, 9747 AG Groningen, The Netherlands

Paul K. Townsend

  • Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge, CB3 0WA, United Kingdom

See Also

More on massive 3D gravity

Eric A. Bergshoeff, Olaf Hohm, and Paul K. Townsend
Phys. Rev. D 79, 124042 (2009)

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Issue

Vol. 102, Iss. 20 — 22 May 2009

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