Author:
Ahmadi Nahid,Noorbala Mahdiyar,Feyzabadi Niloufar,Eghbalpoor Fatemeh,Ahmadi Zahra
Abstract
Abstract
Transitions between different inflationary slow-roll scenarios are known to provide short
non-slow-roll periods with non-trivial consequences. We consider the effect of quantum diffusion
on the inflationary dynamics in a transition process. Using the stochastic δ𝒩
formalism, we follow the detailed evolution of noises through a sharp transition modeled by the
Starobinsky potential, although some of our results apply to any sharp transition. We find how
the stochastic noise induced by the transition affects the coarse-grained fields. We then
consider the special case that the potential is flat after the transition. It is found that,
during a particular phase of evolution, the noise we obtain cannot drive the inflaton past the
classically unreachable field values; so the boundary crossing is delayed. By deriving the
characteristic function, we also study the tail behavior for the distribution of curvature
perturbations ζ, which we find to decay faster than exp(-3ζ).
Subject
Astronomy and Astrophysics
Cited by
10 articles.
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