Speaker
Description
This study investigates the alignment of theoretical and observational Cosmic Microwave Back-
ground (CMB) power spectra, focusing on the high-dissipative regime of the most reliable effective
theory of inflation. Using marginalized posterior distributions, we analyze parameter spaces con-
strained by our model and compare them to observational data from the Planck 2018 results. The
diagonal plots of marginalized distributions reveal the most probable values for each parameter, pro-
viding insights into the model’s consistency with empirical evidence. We parametrized the model
with an accelerated cosmology solution instead of a specific potential for the model. A comparative
analysis of the theoretical power spectrum (f = 0.186 CT = 100) and Planck 2018 data highlights a
close match, particularly at the first acoustic peak ℓ ≈ 220 and subsequent higher-order peaks. These
results emphasize the robustness of the proposed model and its potential for accurately describing
the early universe’s dynamics.
