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New symmetries in Fierz-Pauli massive gravity

We expose a new symmetry for linear perturbations around a solution of non-linear Fierz-Pauli massive gravity plus a bare cosmological constant. The cosmological constant is chosen such that the background metric is flat while the Stuckelberg fields have a non-trivial profile. Around this background, at linear order the new symmetry reduces the propagating degrees of freedom to those of General Relativity, namely the massless helicity 2 modes only. We discuss the physical consequences and possible applications of these findings.

preprint2012arXivOpen access
Gianmassimo TasinatoKazuya KoyamaGustavo Niz
astro-ph.COhep-phhep-th
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Gianmassimo TasinatoKazuya KoyamaGustavo Niz

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