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Restoring General Relativity in massive bi-gravity theory

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arxiv 1307.3640 v3 pith:IKRMQI7B submitted 2013-07-13 gr-qc hep-th

classification gr-qchep-th
keywords generalrelativitysolutiontheoryvainshteinbi-gravitydistancesequation
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We study static spherically symmetric solutions of massive bi-gravity theory, free from the Boulware-Deser ghost. We show the recovery of General Relativity via the Vainshtein mechanism, in the weak limit of the physical metric. We find a single polynomial equation determining the behavior of the solution for distances smaller than the inverse graviton mass. This equation is generically of the seventh order, while for a specific choice of the parameters of the theory it can be reduced to lower orders. The solution is analytic in different regimes: for distances below the Vainshtein radius (where General Relativity is recovered), and in the opposite regime, beyond the Vainshtein radius, where the solution approaches the flat metric.

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  1. Pleba\'nski-Demia\'nski solutions in bigravity and Kerr-Schild double copy relations using an effective metric

    gr-qc 2024-12 conditional novelty 5.0 of 10

    A double Kerr-Schild ansatz in bigravity yields Plebanski-Demianski-type solutions whose double, single, and zeroth copy fields satisfy Maxwell and Klein-Gordon equations in Plebanski coordinates.

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