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Ghost-Free Derivative Interactions for a Massive Graviton

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arxiv 1305.7227 v4 pith:B6GMZ72P submitted 2013-05-30 hep-th gr-qc

Ghost-Free Derivative Interactions for a Massive Graviton

classification hep-th gr-qc
keywords termstheoryconstructdrgteinstein-hilbertfreeghost-freegraviton
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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If the kinetic interactions of a Lorentz-invariant massive graviton are Einstein-Hilbert, then the only possible potential terms free from the Boulware-Deser ghost are those of de Rham, Gabadadze and Tolley (dRGT). We point out there are other possibilities if the kinetic terms are not required to be Einstein-Hilbert. We construct pseudo-linear ghost-free potentials, terms that derive in a natural way from the linear theory. The simplicity of this approach allows us to construct diffeomorphism non-invariant higher-derivative interaction terms that do not introduce ghosts. We conjecture that these terms should have counterparts in the full dRGT theory. These terms would introduce new free parameters into the theory and may change some of the conclusions heretofore drawn.

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  1. Massive Gravity @ 15

    hep-th 2026-07 unverdicted

    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.