Non-Gaussianities from ekpyrotic collapse with multiple fields

Kazuya Koyama, Shuntaro Mizuno, Filippo Vernizzi, David Wands

Research output: Contribution to journalArticle

84 Citations (Scopus)

Abstract

We compute the non-Gaussianity of the curvature perturbation generated by ekpyrotic collapse with multiple fields. The transition from the multi-field scaling solution to a single-field dominated regime converts initial isocurvature field perturbations to an almost scale invariant comoving curvature perturbation. In the specific model of two fields, 1 and 2, with exponential potentials, -Viexp(-ci i), we calculate the bispectrum of the resulting curvature perturbation. We find that the non-Gaussianity is dominated by non-linear evolution on super-Hubble scales and hence is of the local form. The non-linear parameter of the curvature perturbation is given by fNL = 5c j 2/12, where cj is the exponent of the potential for the field which becomes subdominant at late times. Since c j 2 must be large, in order to generate an almost scale invariant spectrum, the non-Gaussianity is inevitably large. Thus, the model is strongly constrained by observational bounds on the spectral index and non-Gaussianity.

Original languageEnglish
Article number024
JournalJournal of Cosmology and Astroparticle Physics
Issue number11
DOIs
Publication statusPublished - 2007 Nov 1
Externally publishedYes

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perturbation
curvature
exponents
scaling

Keywords

  • Cosmological perturbation theory
  • Cosmology with extra dimensions
  • String theory and cosmology

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Non-Gaussianities from ekpyrotic collapse with multiple fields. / Koyama, Kazuya; Mizuno, Shuntaro; Vernizzi, Filippo; Wands, David.

In: Journal of Cosmology and Astroparticle Physics, No. 11, 024, 01.11.2007.

Research output: Contribution to journalArticle

Koyama, Kazuya ; Mizuno, Shuntaro ; Vernizzi, Filippo ; Wands, David. / Non-Gaussianities from ekpyrotic collapse with multiple fields. In: Journal of Cosmology and Astroparticle Physics. 2007 ; No. 11.
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