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Ghosts & Matter Couplings in Massive (bi-&multi-)Gravity

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arxiv 1409.3834 v2 pith:EQVOVYQU submitted 2014-09-12 hep-th astro-ph.COgr-qc

Ghosts & Matter Couplings in Massive (bi-&multi-)Gravity

classification hep-th astro-ph.COgr-qc
keywords couplingghostscalemattercouplingscut-offgravityimplies
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Recently, several works have investigated the coupling to matter in ghost-free massive (bi-&multi-)gravity and a new effective coupling to matter has been proposed. In this note we clarify some confusion on the existence and the implications of a ghost above the strong coupling scale. We confirm that the standard constraint which is otherwise typically present in this type of theories disappears on generic backgrounds as soon as this new coupling is considered. This implies the re-emergence of the Boulware-Deser ghost. Nevertheless the absence of ghost in the decoupling limit implies that the cut-off scale (if identified with the scale at which the ghost enters) is higher than the strong coupling scale. Therefore there is a valid interesting region of applicability for these couplings at scales below the cut-off.

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    A status review arguing that ghost-free massive gravity remains a theoretically consistent and phenomenologically viable infrared modification of General Relativity, with open UV questions.