pith. sign in

arxiv: 1805.11298 · v1 · pith:JSGJBXJNnew · submitted 2018-05-29 · 🌌 astro-ph.CO

Single-Field Consistency relation and δ N-Formalism

classification 🌌 astro-ph.CO
keywords effectformalismbispectrumconsistencydeltalimitperturbationrelation
0
0 comments X p. Extension
pith:JSGJBXJN Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{JSGJBXJN}

Prints a linked pith:JSGJBXJN badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

According to the equivalence principal, the long wavelength perturbations must not have any dynamical effect on the short scale physics up to ${\cal O} (k_L^2/k_s^2)$. Their effect can be always absorbed to a coordinate transformation locally. So any physical effect of such a perturbation appears only on scales larger than the scale of the perturbation. The bispectrum in the squeezed limit of the curvature perturbation in single-field slow-roll inflation is a good example, where the long wavelength effect is encoded in the spectral index through Maldacena's consistency relation. This implies that one should be able to derive the bispectrum in the squeezed limit without resorting to the in-in formalism in which one computes perturbative corrections field-theoretically. In this short paper, we show that the $\delta N$ formalism as it is, or more generically the separate universe approach, when applied carefully can indeed lead to the correct result for the bispectrum in the squeezed limit. Hence despite the common belief that the $\delta N$ formalism is incapable of recovering the consistency relation within itself, it is in fact self-contained and consistent.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.