Inhomogeneous de Sitter Solution with Scalar Field and Perturbations Spectrum

Abstract

We provide an inhomogeneous solution concerning the dynamics of a real self interacting scalar field minimally coupled to gravity in a region of the configuration space where it performs a slow rolling on a plateau of its potential. During the inhomogeneous de Sitter phase the scalar field dominant term is a function of the spatial coordinates only. This solution specialized nearby the FLRW model allows a classical origin for the inhomogeneous perturbations spectrum.

9 pages, no figures, to appear on Mod.Phys.Lett. A

References in corpus (3)

• Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology
• Quasi-Isotropization of the Inhomogeneous Mixmaster Universe Induced by an Inflationary Process
• On the Quasi-Isotropic Inflationary Solution

Cited by in corpus (1)

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