Published June 15, 2011 | Version v1
Journal article

Generating scale-invariant perturbations from rapidly-evolving equation of state

  • 1. Center for Particle Cosmology, Department of Physics and Astronomy University of Pennsylvania, Philadelphia, Pennsylvania 19104 (United States)
  • 2. Department of Physics and Princeton Center for Theoretical Science Princeton University, Princeton, New Jersey 08544 (United States)

Description

Recently, we introduced an ekpyrotic model based on a single, canonical scalar field that generates nearly scale-invariant curvature fluctuations through a purely ''adiabatic mechanism'' in which the background evolution is a dynamical attractor. Despite the starkly different physical mechanism for generating fluctuations, the two-point function is identical to inflation. In this paper, we further explore this concept, focusing in particular on issues of non-Gaussianity and quantum corrections. We find that the degeneracy with inflation is broken at three-point level: for the simplest case of an exponential potential, the three-point amplitude is strongly scale dependent, resulting in a breakdown of perturbation theory on small scales. However, we show that the perturbative breakdown can be circumvented--and all issues raised in Linde et al. (arXiv:0912.0944) can be addressed--by altering the potential such that power is suppressed on small scales. The resulting range of nearly scale-invariant, Gaussian modes can be as much as 12 e-folds, enough to span the scales probed by microwave background and large-scale structure observations. On smaller scales, the spectrum is not scale invariant but is observationally acceptable.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
83
Journal Issue
12
Journal Page Range
p. 123502-123502.18
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
42094525
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
AMPLITUDES; BREAKDOWN; CORRECTIONS; DISTURBANCES; EQUATIONS OF STATE; EVOLUTION; FLUCTUATIONS; INVARIANCE PRINCIPLES; MICROWAVE RADIATION; PERTURBATION THEORY; SCALAR FIELDS; SPECTRA
Descriptors DEC
ELECTROMAGNETIC RADIATION; EQUATIONS; RADIATIONS; VARIATIONS

Optional Information

Notes
(c) 2011 American Institute of Physics