Mode analysis of cosmological perturbations with the $E$-model $\alpha$-attractor inflaton potentials

Abstract

We have carried out detailed $k$-mode analysis of single-inflaton slow-roll inflationary perturbations including quantum fluctuations by setting up non-linear coupled differential equations of inflaton field ($\varphi$), its perturbation ($\delta \varphi$) and the metric perturbation (the Bardeen potential, ${\Phi }_B$), and calculated the number of e-folds ($N$), scalar spectral index ($n_s$), tensor spectral index ($n_h$), scalar power spectrum (${\Delta }_s$), tensor power spectrum (${\Delta }_h$), tensor-to-scalar ratio ($r$) and the Hubble parameter ($H$) for different $k$ values at the horizon crossing. In these calculations we have employed the $E$-model $\alpha$-attractor potentials which are found to display slow-roll behaviour. The values of $n_s$ and $r$ obtained by us are consistent with those given by the well-known universal $\alpha$-attractor formulae. We got $n_s=0.956908$ and $r=0.005571$ at $k=10^6$ Planck unit for the value of the potential parameter $n=1$. These can be compared with the Planck-2018 data viz., $n_s=0.9649\pm 0.0042$ at $68\%$ CL, $r<0.064$ at $95\%$ CL and ACT-2020 data viz., $n_s=0.9691\pm 0.0041$ at $68\%$ CL.

12 figures, 14 pages