Abstract
After giving a pedagogical review we clarify that the stochastic approach to inflation is generically reliable only at zeroth order in the (geometrical) slow-roll parameter $\epsilon_1$ if and only if $\epsilon_2^2\ll 6/\epsilon_1$, with the notable exception of slow-roll. This is due to the failure of the stochastic $\Delta N$ formalism in its standard formulation. However, by keeping the formalism in its regime of validity, we showed that, in ultra-slow-roll, the stochastic approach to inflation reproduces the power spectrum calculated from the linear theory approach.
| Original language | English |
|---|---|
| Journal | Journal of Cosmology and Astroparticle Physics |
| DOIs | |
| Publication status | Published - 29 Mar 2019 |
Bibliographical note
v3: typo in the appendix corrected. Results unchanged. Published version in JCAPKeywords
- gr-qc
- astro-ph.CO
- hep-ph
- hep-th
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