Generating ekpyrotic curvature perturbations before the big bang

Jean-Luc Lehners, Paul McFadden, Neil Turok, and Paul J. Steinhardt
Phys. Rev. D 76, 103501 – Published 1 November 2007

Abstract

We analyze a general mechanism for producing a nearly scale-invariant spectrum of cosmological curvature perturbations during a contracting phase preceding a big bang, which can be entirely described using 4D effective field theory. The mechanism, based on first producing entropic perturbations and then converting them to curvature perturbations, can be naturally incorporated in cyclic and ekpyrotic models in which the big bang is modeled as a brane collision, as well as other types of cosmological models with a pre-big bang phase. We show that the correct perturbation amplitude can be obtained and that the spectral tilt ns tends to range from slightly blue to red, with 0.97<ns<1.02 for the simplest models, a range compatible with current observations but shifted by a few percent towards the blue compared to the prediction of the simplest, large-field inflationary models.

  • Received 8 June 2007

DOI:https://doi.org/10.1103/PhysRevD.76.103501

©2007 American Physical Society

Authors & Affiliations

Jean-Luc Lehners1,*, Paul McFadden2,†, Neil Turok1,‡, and Paul J. Steinhardt3,4,§

  • 1DAMTP, CMS, Wilberforce Road, CB3 0WA, Cambridge, United Kingdom
  • 2ITFA, Valckenierstraat 65, 1018XE Amsterdam, The Netherlands
  • 3Joseph Henry Laboratories, Princeton University, Princeton, New Jersey 08544, USA
  • 4Princeton Center for Theoretical Physics, Jadwin Hall, Princeton University, Princeton, New Jersey 08544, USA

  • *j.lehners@damtp.cam.ac.uk
  • mcfadden@science.uva.nl
  • n.g.turok@damtp.cam.ac.uk
  • §steinh@princeton.edu

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Issue

Vol. 76, Iss. 10 — 15 November 2007

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