We have over 12,000 students, from over 100 countries, within one of the safest campuses in the UK


93% of Lancaster students go into work or further study within six months of graduating

Home > Research > Publications & Outputs > Very Large Primordial Non-Gaussianity from mult...
View graph of relations

« Back

Very Large Primordial Non-Gaussianity from multi-field: Application to Massless Preheating

Research output: Contribution to journalJournal article


Article number3
Journal publication date6/04/2006
JournalJournal of Cosmology and Astroparticle Physics
Original languageEnglish


In this paper we derive a generic expression, which is valid for scales larger than Hubble radius and contains only the local terms, for the second order curvature perturbations for more than one field, provided the expansion is sourced by the energy density of a single field. As an application, motivated by our previous paper [1], we apply our formalism to two fields during preheating, where the inflaton oscillations are sourced by $\lambda\phi^4$ potential which is governing the expansion of the Universe. A second field $\sigma$, coupled to the inflaton through $g^2\phi^2\sigma^2$, is excited from the vacuum fluctuations. The excited modes of $\sigma$ amplify the super-Hubble isocurvature perturbations, which seed the second order curvature perturbations to give rise to a significantly large non-Gaussianity. Our results show that within 3 inflaton oscillations for a range of parameters, $1

Bibliographic note

23 pages, JHEP style, references added