English

A New delta N Formalism for Multi-Component Inflation

Astrophysics 2009-10-09 v2

Abstract

The delta N formula that relates the final curvature perturbation on comoving slices to the inflaton perturbation on flat slices after horizon crossing is a powerful and intuitive tool to compute the curvature perturbation spectrum from inflation. However, it is customarily assumed further that the conventional slow-roll condition is satisfied, and satisfied by all components, during horizon crossing. In this paper, we develop a new delta N formalism for multi-component inflation that can be applied in the most general situations. This allows us to generalize the idea of general slow-roll inflation to the multi-component case, in particular only applying the general slow-roll condition to the relevant component. We compute the power spectrum of the curvature perturbation in multi-component general slow-roll inflation, and find that under quite general conditions it is invertible.

Keywords

Cite

@article{arxiv.astro-ph/0506262,
  title  = {A New delta N Formalism for Multi-Component Inflation},
  author = {Hyun-Chul Lee and Misao Sasaki and Ewan D. Stewart and Takahiro Tanaka and Shuichiro Yokoyama},
  journal= {arXiv preprint arXiv:astro-ph/0506262},
  year   = {2009}
}

Comments

24 pages, no figure

R2 v1 2026-07-22T08:52:59.075Z