Attractor models in scalar–tensor theories of inflation
Abstract
In this work, we study the cosmological attractor models of inflation in connection with certain scalar–tensor theories of gravity, e.g. f(R) gravity and Brans–Dicke theory. For some particular choices of the functional degrees of freedom in these theories, one obtains Starobinsky-like predictions in the (ns−r) observable plane. We have demonstrated that these choices in the Lagrangian density of certain f(R) and Brans–Dicke theories fulfil the condition of the cosmological attractors. That explains why known predictions of f(R) and Brans–Dicke theories in certain cases appear to be the predictions of the much discussed attractor theories. In addition, we did an analysis showing how the predictions of an attractor model are preserved with respect to the variation in the functional freedom of the theory.
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