paper

Conditions for Generating Scale-Invariant Density Perturbations

arXiv:astro-ph/0301395 · doi:10.1103/PhysRevD.69.103505

Abstract

We analyze the general conditions on the equation of state required for quantum fluctuations of a scalar field to produce a scale-invariant spectrum of density perturbations, including models which (in the four dimensional effective description) bounce from a contracting to an expanding phase. We show that there are only two robust cases: (inflation) and (the ekpyrotic/cyclic scenario). All other cases, including the case considered by some authors, require extreme fine-tuning of initial conditions and/or the effective potential. For the ekpyrotic/cyclic () case, we also analyze the small deviations from scale invariance.

6 pages, no figures

Conditions for Generating Scale-Invariant Density Perturbations · wovepaper