Speaker
Silvia Pla Garcia
(TUM)
Description
This project explores the effects of renormalization on the amplitude of the inflationary spectra at scales measurable in the cosmic microwave background.
Via a gauge-invariant analysis, it is explained why the standard prediction for the spectra on superhorizon scales is a late-time attractor while they are UV finite at all times. This result is independent of the equation of state after inflation, showing that the standard prediction is fully robust.
Primary authors
Silvia Pla Garcia
(TUM)
Dr
Ben Stefanek
(IFIC)
