Galaxies 2013, 1(2), 96-106; doi:10.3390/galaxies1020096

Conformally Coupled Inflation

Received: 29 June 2013; in revised form: 19 July 2013 / Accepted: 19 July 2013 / Published: 30 July 2013
(This article belongs to the Special Issue Cosmology with Fluid Components)
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Abstract: A massive scalar field in a curved spacetime can propagate along the light cone, a causal pathology, which can, in principle, be eliminated only if the scalar couples conformally to the Ricci curvature of spacetime. This property mandates conformal coupling for the field driving inflation in the early universe. During slow-roll inflation, this coupling can cause super-acceleration and, as a signature, a blue spectrum of primordial gravitational waves.
Keywords: inflation; non-minimal coupling; early universe
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MDPI and ACS Style

Faraoni, V. Conformally Coupled Inflation. Galaxies 2013, 1, 96-106.

AMA Style

Faraoni V. Conformally Coupled Inflation. Galaxies. 2013; 1(2):96-106.

Chicago/Turabian Style

Faraoni, Valerio. 2013. "Conformally Coupled Inflation." Galaxies 1, no. 2: 96-106.

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