English

Non-Gaussianity Consistency Relation for Multi-field Inflation

General Relativity and Quantum Cosmology 2011-07-28 v2 Cosmology and Nongalactic Astrophysics High Energy Physics - Theory

Abstract

While detection of the "local form" bispectrum of primordial perturbations would rule out all single-field inflation models, multi-field models would still be allowed. We show that multi-field models described by the δN\delta N formalism obey an inequality between fNLf_{\rm NL} and one of the local-form {\it trispectrum} amplitudes, τNL\tau_{\rm NL}, such that τNL>12(65fNL)2\tau_{\rm NL}>\frac12(\frac65f_{\rm NL})^2 with a possible logarithmic scale dependence, provided that 2-loop terms are small. Detection of a violation of this inequality would rule out most of multi-field models, challenging inflation as a mechanism for generating the primoridal perturbations.

Keywords

Cite

@article{arxiv.1101.3636,
  title  = {Non-Gaussianity Consistency Relation for Multi-field Inflation},
  author = {Naonori S. Sugiyama and Eiichiro Komatsu and Toshifumi Futamase},
  journal= {arXiv preprint arXiv:1101.3636},
  year   = {2011}
}

Comments

5 pages. Accepted for publication in Physical Review Letters

R2 v1 2026-06-21T17:13:56.184Z