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Propagating degrees of freedom on maximally-symmetric backgrounds in $f(R)$ theories of gravity
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abstract
In the context of $f(R)$ gravity, as well as other extended theories of gravity, the correct counting of globally well-defined dynamical modes has recently drawn a vivid interest. In this communication we present a consistent approach shedding light on such issues for both so-called degenerate and non-degenerate $f(R)$ models embedded in maximally-symmetric backgrounds. We find that the linearised spectrum of degenerate models on these backgrounds is empty, lacking both the graviton and scalaron modes which appear in generic non-degenerate models. Our work generalises previous results in the literature applicable only to the specific (degenerate) model $f(R)=\alpha R^2$; in fact, we find that the same pathologies discovered therein emerge for all choices of $f(R)$ belonging to the wide class of degenerate models.
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Cited by 1 Pith paper
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Close Hyperbolic Encounters In f(R) Gravity
In f(R) gravity, close hyperbolic black-hole encounters emit a scalar gravitational-wave mode whose promised detectability is not supported by the paper's own amplitude formulas.
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