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Ghost-free Massive Gravity with a General Reference Metric

5 Pith papers cite this work. Polarity classification is still indexing.

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abstract

Theories of massive gravity inevitably include an auxiliary reference metric. Generically, they also contain an inconsistency known as the Boulware-Deser ghost. Recently, a family of non-linear massive gravity actions, formulated with a flat reference metric, were proposed and shown to be ghost free at the complete non-linear level. In this paper we consider these non-linear massive gravity actions but now formulated with a general reference metric. We extend the proof of the absence of the Boulware-Deser ghost to this case. The analysis is carried out in the ADM formalism at the complete non-linear level. We show that in these models there always exists a Hamiltonian constraint which, with an associated secondary constraint, eliminates the ghost. This result considerably extends the range of known consistent non-linear massive gravity theories. In addition, these theories can also be used to describe a massive spin-2 field in an arbitrary, fixed gravitational background. We also discuss the positivity of the Hamiltonian.

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Bimetric interactions based on metric congruences

hep-th · 2019-06-27 · unverdicted · novelty 6.0

Bimetric interactions are defined via a congruence matrix, with the square root shown as the unique power series solution and algebraic equivalence to the unconstrained vielbein formulation.

Non-primary square roots in massive gravity

hep-th · 2026-06-26 · unverdicted · novelty 5.0 · 2 refs

Non-primary square roots in massive gravity preserve covariance but lack analytic perturbation theory and risk complex domains.

Gravitational wave propagation in bigravity in the late universe

gr-qc · 2025-07-15 · unverdicted · novelty 5.0

Exact solutions and uniform approximations for GW modes in bigravity in de Sitter yield regime-dependent luminosity distances, a new bound from GW170817, and retained coherence between massless and massive signal components.

Planck 2018 results. VI. Cosmological parameters

astro-ph.CO · 2018-07-17 · accept · novelty 5.0

Final Planck CMB data confirms the flat 6-parameter ΛCDM model with Ω_c h² = 0.120 ± 0.001, Ω_b h² = 0.0224 ± 0.0001, n_s = 0.965 ± 0.004, τ = 0.054 ± 0.007, H_0 = 67.4 ± 0.5 km/s/Mpc, and no strong evidence for extensions.

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  • Planck 2018 results. VI. Cosmological parameters astro-ph.CO · 2018-07-17 · accept · none · ref 162

    Final Planck CMB data confirms the flat 6-parameter ΛCDM model with Ω_c h² = 0.120 ± 0.001, Ω_b h² = 0.0224 ± 0.0001, n_s = 0.965 ± 0.004, τ = 0.054 ± 0.007, H_0 = 67.4 ± 0.5 km/s/Mpc, and no strong evidence for extensions.