Mutated Hilltop Inflation in the Era of Present and Future CMB Experiments

TL;DR

This paper evaluates mutated hilltop inflation models against current and future CMB observational data, demonstrating their consistency with existing constraints and potential detectability in upcoming experiments.

Contribution

It provides a comprehensive confrontation of mutated hilltop inflation predictions with recent observational data and forecasts their testability with future CMB experiments.

Findings

Mutated hilltop inflation aligns well with Planck-2018 and BICEP/Keck-2018 data.

The model can probe tensor-to-scalar ratio down to ~10^{-4}.

Predictions remain consistent with upcoming CMB experiments like LiteBIRD and Simons Observatory.

Abstract

In this article we confront both large-field and small-field sectors of mutated hilltop inflation model with the recent observational results. We begin with confrontation of predictions from mutated hilltop inflation with the joint analysis of Planck-2018 and BICEP/Keck-2018 data. Subsequently, we extend our analysis by incorporating the ACT-DR6 data in combination with Planck-2018, BICEP/Keck-2018, and DESI-Y1 observations. In both cases, the predictions of mutated hilltop inflation show good consistency with the observational constraints. We have also forecasted the constraints on mutated hilltop inflation model from upcoming CMB experiments, LiteBIRD and Simons Observatory along with their combinations. Here also we find that the prediction from mutated hilltop inflation are in tune with those upcoming CMB experiments. The small-field sector of mutated hilltop inflation, in principle, can probe up to $r\sim \mathcal{O}(10^{-4})$, resulting in a tensor amplitude consistent with current bounds and potentially detectable by next-generation CMB missions. However, accommodating the high observational value of the scalar spectral index may demand relatively higher e-foldings in mutated hilltop inflation. A key appealing feature of the mutated hilltop inflation model turns out to be its ability to remain consistent with a potential non-detection of primordial gravitational waves by LiteBIRD and/or Simons Observatory.