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arxiv: gr-qc/0404031 · v1 · submitted 2004-04-07 · 🌀 gr-qc · astro-ph

Inhomogeneous de Sitter Solution with Scalar Field and Perturbations Spectrum

classification 🌀 gr-qc astro-ph
keywords inhomogeneousfieldscalarsolutionperturbationssitterspectrumallows
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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.

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