Topologically massive gravity as a Pais-Uhlenbeck oscillator
arXiv:gr-qc/0608085 · doi:10.1088/0264-9381/23/24/023
Abstract
We give a detailed account of the free field spectrum and the Newtonian limit of the linearized "massive" (Pauli-Fierz), "topologically massive" (Einstein-Hilbert-Chern-Simons) gravity in 2+1 dimensions about a Minkowski spacetime. For a certain ratio of the parameters, the linearized free theory is Jordan-diagonalizable and reduces to a degenerate "Pais-Uhlenbeck" oscillator which, despite being a higher derivative theory, is ghost-free.
9 pages, no figures, RevTEX4; version 2: a new paragraph and a reference added to the Introduction, a new appendix added to review Pais-Uhlenbeck oscillators; accepted for publication in Class. Quant. Grav
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Cited by in corpus (9)
- Massive Higher Derivative Gravity in D-dimensional Anti-de Sitter Spacetimes
- Canonical Structure of Higher Derivative Gravity in 3D
- Hamiltonian formalisms and symmetries of the Pais-Uhlenbeck oscillator
- Imaginary-Scaling versus Indefinite-Metric Quantization of the Pais-Uhlenbeck Oscillator
- Reductions of Topologically Massive Gravity I: Hamiltonian Analysis of The Second Order Degenerate Lagrangians
- Generalized Niederer's transformation for quantum Pais-Uhlenbeck oscillator
- Various disguises of the Pais-Uhlenbeck oscillator
- Reductions of Topologically Massive Gravity II: First Order Realizations of Second Order Lagrangians
- Circularly polarized periodic gravitational wave and the Pais-Uhlenbeck oscillator