Failure of the stochastic approach to inflation beyond slow-roll

Diego Cruces, Cristiano Germani, T. Prokopec

Research output: Contribution to journalArticleAcademicpeer-review

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 languageEnglish
JournalJournal of Cosmology and Astroparticle Physics
DOIs
Publication statusPublished - 29 Mar 2019

Bibliographical note

v3: typo in the appendix corrected. Results unchanged. Published version in JCAP

Keywords

  • gr-qc
  • astro-ph.CO
  • hep-ph
  • hep-th

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