Published October 15, 2006 | Version v1
Journal article

Second-order gauge-invariant perturbations during inflation

  • 1. Dipartimento di Fisica, Universita degli Studi di Bologna and INFN, via Irnerio 46, I-40126 Bologna (Italy)
  • 2. INAF/IASF-BO, Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna Istituto Nazionale di Astrofisica Via Gobetti 101, I-40129 Bologna (Italy) and INAF/OAB, Osservatorio Astronomico di Bologna Istituto Nazionale di Astrofisica Via Ranzani 1, I-40127 Bologna (Italy) and INFN, Sezione di Bologna, Via Irnerio 46, I-40126 Bologna (Italy)

Description

The evolution of gauge invariant second-order scalar perturbations in a general single field inflationary scenario are presented. Different second-order gauge-invariant expressions for the curvature are considered. We evaluate perturbatively one of these second order curvature fluctuations and a second-order gauge-invariant scalar field fluctuation during the slow-roll stage of a massive chaotic inflationary scenario, taking into account the deviation from a pure de Sitter evolution and considering only the contribution of super-Hubble perturbations in mode-mode coupling. The spectra resulting from their contribution to the second order quantum correlation function are nearly scale-invariant, with additional logarithmic corrections with respect to the first order spectrum. For all scales of interest the amplitude of these spectra depends on the total number of e-folds. We find, on comparing first and second order perturbation results, an upper limit to the total number of e-folds beyond which the two orders are comparable

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
74
Journal Issue
8
Journal Page Range
p. 083522-083522.13
ISSN
0556-2821
CODEN
PRVDAQ

Optional Information

Notes
(c) 2006 The American Physical Society