Evolution to a smooth universe in an ekpyrotic contracting phase with w>1

David Garfinkle, Woei Chet Lim, Frans Pretorius, and Paul J. Steinhardt
Phys. Rev. D 78, 083537 – Published 27 October 2008

Abstract

A period of slow contraction with equation of state w>1, known as an ekpyrotic phase, has been shown to flatten and smooth the universe if it begins the phase with small perturbations. In this paper, we explore how robust and powerful the ekpyrotic smoothing mechanism is by beginning with highly inhomogeneous and anisotropic initial conditions and numerically solving for the subsequent evolution of the universe. Our studies, based on a universe with gravity plus a scalar field with a negative exponential potential, show that some regions become homogeneous and isotropic while others exhibit inhomogeneous and anisotropic behavior in which the scalar field behaves like a fluid with w=1. We find that the ekpyrotic smoothing mechanism is robust in the sense that the ratio of the proper volume of the smooth to nonsmooth region grows exponentially fast along time slices of constant mean curvature.

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  • Received 6 August 2008

DOI:https://doi.org/10.1103/PhysRevD.78.083537

©2008 American Physical Society

Authors & Affiliations

David Garfinkle1,*, Woei Chet Lim2,†, Frans Pretorius2,‡, and Paul J. Steinhardt2,3,§

  • 1Department of Physics, Oakland University, Rochester, Michigan 48309, USA
  • 2Joseph Henry Laboratories, Princeton University, Princeton, New Jersey 08544, USA
  • 3Princeton Center for Theoretical Science, Princeton University, Princeton, New Jersey 08544, USA

  • *garfinkl@oakland.edu
  • wlim@princeton.edu
  • fpretori@princeton.edu
  • §steinh@princeton.edu

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Vol. 78, Iss. 8 — 15 October 2008

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