Inflationary attractors and perturbation spectra in generally coupled gravity

A generic outcome of theories with scalar-tensor coupling is the existence of inflationary attractors, either power-law or de Sitter. The fluctuations arising during this phase are Gaussian and their spectrum depends on the wavenumber $k$ according to the power-law $k^{1/(1-p)}$, where

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Bibliographische Detailangaben
Hauptverfasser: Amendola, Luca (VerfasserIn) , Bellisai, Diego (VerfasserIn) , Occhionero, Franco (VerfasserIn)
Dokumenttyp: Article (Journal) Kapitel/Artikel
Sprache:Englisch
Veröffentlicht: 1993
In: Arxiv

Online-Zugang:Verlag, kostenfrei, Volltext: http://arxiv.org/abs/gr-qc/9303023
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Verfasserangaben:Luca Amendola, Diego Bellisai and Franco Occhionero
Beschreibung
Zusammenfassung:A generic outcome of theories with scalar-tensor coupling is the existence of inflationary attractors, either power-law or de Sitter. The fluctuations arising during this phase are Gaussian and their spectrum depends on the wavenumber $k$ according to the power-law $k^{1/(1-p)}$, where
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