paper

ACT DR6 Insights on the Inflationary Attractor models and Reheating

arXiv:2505.01517 · doi:10.1103/1kj4-s4ts

Abstract

We investigate the observational constraints on -attractor inflationary models and their post-inflationary reheating dynamics in light of the latest CMB data from ACT DR6 combined with Planck18, BICEP/ 2018, and DESI (P-ACT-LB-BK18). Focusing on both E- and T-type attractor potentials, we analyze how inflationary observables, namely the scalar spectral index and the tensor-to-scalar ratio , are indirectly influenced by reheating parameters such as the reheating temperature , the inflaton EoS , and consequently the inflaton's couplings to SM particles. We incorporate constraints from PGW overproduction via bounds. Additionally, we include theoretical constraints from CW one-loop radiative corrections, as well as inflaton self-resonance, a non-perturbative effect that can occur even in the absence of inflaton-SM interactions and imposes a strong lower limit, particularly significant for . Our analysis shows that E-models allow a broad range of reheating scenarios, including matter-like reheating (), whereas the T-model yields more restrictive results and remains viable only for for all three non-gravitational interaction channels, , , and are considered. For stiffer EoS, an intermediate coupling window survives, bounded from above by CW corrections or observational limits, and from below by the combined PGW and self-resonance constraints. We derive updated bounds on inflaton couplings for both decay and scattering channels and identify parameter regions consistent with successful perturbative reheating. These results establish a robust connection between inflationary dynamics, reheating physics, and particle interactions, and provide concrete targets for upcoming precision CMB observations.

16 pages, 10 figures and 4 tables. Published in PRD