Abstract
Consistency conditions for nonminimally coupled f(R) theories have been derived by requiring the absence of tachyons and instabilities in the scalar fluctuations. This note confirms these results and clarifies a subtlety regarding different definitions of sound speeds.
Notes
The propagation of the two fields in the action (2) could actually be deduced by just treating the two scalars as test fields and expanding around a flat space, and it is easy to see that only the field \(\psi \) has a nontrivial sound speed, stemming from the nonlinear dependence on its kinetic term. In Ref. [3] we however used the full machinery of the cosmological perturbation theory, perturbing both fields and the metric, to arrive at the results that indeed, at the relevant limit, are compatible with the simplest guess one would base on the ample previous literature on scalar fields in cosmology.
One can though check that in practice this does not make a difference for the results as the parameter constraints derived from the two definitions would coincide for all the four explicit example classes of models considered in Ref. [3].
References
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Appendix
Appendix
In this appendix we rederive the action (2) from action (1), again using, as a cross-check, a somewhat different method from [3]. There we kept the matter Lagrangian \(\hat{\mathcal {L}}\) general and applied a Legendre transformation method for both the R and the \(\mathcal {\hat{L}}\). Here we specify \(\mathcal {\hat{L}}=\hat{X}\) and apply a straightforward generalisation of a well-known procedure that recasts a minimally coupled f(R) gravity into a scalar-tensor theory.
So we begin with action (1) where \(\mathcal {\hat{L}}=\hat{X}\). Introducing a field \(\alpha \) and a Lagrange multiplier \(\varphi \) that sets \(\alpha =R\) we can write the action equivalently as
We then vary the action with respect to \(\alpha \), and solve it from its own equation of motion
and it is then legitimate to plug the solution back into the action, to obtain
Under a conformal rescaling \(g_{\mu \nu }=\Omega ^2 g_{\mu \nu }\), the relevant quantities transform as
Performing the rescaling with the conformal factor
we obtain:
We have then recovered the same relation between actions (1) and (2) as was obtained in [3].
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Koivisto, T.S., Tamanini, N. A note on viability of nonminimally coupled f(R) theory. Gen Relativ Gravit 48, 97 (2016). https://doi.org/10.1007/s10714-016-2087-5
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DOI: https://doi.org/10.1007/s10714-016-2087-5