http://arxiv.org/abs/2004.10778
In this letter we shall provide a formal derivation of the inflationary slow-roll indices for $F(R)$ gravity from the power spectrum without the condition $\dot{\epsilon}_1=0$, frequently used in the literature, where $\epsilon_1=-\frac{\dot{H}}{H^2}$ is the first slow-roll index. We shall employ Karamata’s theorem for regularly varying functions, and as we show, we shall derive the same expressions for the scalar and tensor spectral index of $F(R)$ gravity, also appearing in the current literature, without the misleading and rather strong condition $\dot{\epsilon}_1=0$. The only conditions that are needed are the slow-roll assumption, and the smallness of the slow-roll indices and of their derivatives during inflation.
V. Oikonomou
Fri, 24 Apr 20
16/63
Comments: EPL Accepted