Non-Gaussianity from the bispectrum in general multiple field inflation

Frederico Arroja*, Shuntaro Mizuno, Kazuya Koyama

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

99 Citations (Scopus)


We study the non-Gaussianity from the bispectrum in multi-field inflation models with a general kinetic term. The models include multi-field K-inflation and multi-field Dirac-Born-Infeld (DBI) inflation as special cases. We find that, in general, the sound speeds for the adiabatic and entropy perturbations are different and they can be smaller than 1. Then the non-Gaussianity can be enhanced. Multi-field DBI inflation is shown to be a special case where both sound speeds are the same due to a special form of the kinetic term(Langlois et al 2008 Preprint0804.3139 [hep-th]). We derive the exact second-and third-order actions including metric perturbations. In the small sound speed limit and at leading order in the slow-roll expansion, we derive the three-point function for the curvature perturbation which depends on both adiabatic and entropy perturbations. The contribution from the entropy perturbations has a different momentum dependence if the sound speeds for the entropy and adiabatic perturbations are different, which provides a possibility to distinguish multi-field models from single-field models. On the other hand, in the multi-field DBI case, the contribution from the entropy perturbations has the same momentum dependence as the pure adiabatic contributions and it only changes the amplitude of the three-point function(Langlois et al 2008 Preprint0804.3139 [hep-th]). This could help to ease the constraints on the DBI-inflation models.

Original languageEnglish
Article number015
JournalJournal of Cosmology and Astroparticle Physics
Issue number8
Publication statusPublished - 2008 Aug 1
Externally publishedYes


  • Cosmological perturbation theory
  • Inflation
  • String theory and cosmology

ASJC Scopus subject areas

  • Astronomy and Astrophysics


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