Loop Corrections to Cosmological Perturbations in Multi-field Inflationary Models
Xian Gao, Fanrong Xu
TL;DR
This paper analyzes one-loop quantum corrections to the adiabatic power spectrum in two-field DBI inflation, focusing on entropy-adiabatic cross-interactions. Using the in-in formalism, it shows that derivative cross-interactions are enhanced by the slow-roll parameter $\ε$ and a small sound speed $c_s$, potentially yielding large loop corrections. Crucially, the calculated loop contributions are infrared finite, owing to the derivative structure of the leading vertices. The results imply that for $c_s \ll 1$ models, higher-order loops and their impact on primordial non-Gaussianities and late-time observables must be carefully accounted for, and a full treatment of the curvature perturbation $\zeta$ via $\delta N$ formalism is needed for connecting to CMB and LSS data.
Abstract
We investigate one-loop quantum corrections to the power spectrum of adiabatic perturbation from entropy modes/adiabatic mode cross-interactions in multiple DBI inflationary models. We find that due to the non-canonical kinetic term in DBI models, the loop corrections are enhanced by slow-varying parameter $ε$ and small sound speed $c_s$. Thus, in general the loop-corrections in multi-DBI models can be large. Moreover, we find that the loop-corrections from adiabatic/entropy cross-interaction vertices are IR finite.
