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Consistent massive graviton on arbitrary backgrounds

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arxiv 1410.8302 v2 pith:62W65RJ6 submitted 2014-10-30 hep-th gr-qc

classification hep-thgr-qc
keywords metricgravitonmassivearbitrarybackgroundconstraintscovariantdrgt
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We obtain the fully covariant linearized field equations for the metric perturbation in the de Rham-Gabadadze-Tolley (dRGT) ghost free massive gravities. For a subset of these theories, we show that the non dynamical metric that appears in the dRGT setup can be completely eliminated leading to the theory of a massive graviton moving in a single metric. This has a mass term which contains non trivial contributions of the space-time curvature. We show further how 5 covariant constraints can be obtained including one which leads to the tracelessness of the graviton on flat space-time and removes the Boulware-Deser ghost. The 5 constraints are obtained for a background metric which is arbitrary, i.e. which does not have to obey the background field equations.

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  1. Perturbations of black holes in mass-varying massive gravity

    gr-qc 2026-07 conditional novelty 5.0 of 10

    In mass-varying massive gravity, the beta=alpha^2 branch of constant-scalar Schwarzschild-(A)dS solutions has delta X=0, so tensor perturbations obey the GR equations while scalar stability depends on potential parameters.

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