Scale dependence of local fNL

We consider possible scale-dependence of the non-linearity parameter fNL in local and quasi-local models of non-Gaussian primordial density perturbations. In the simplest model where the primordial perturbations are a quadratic local function of a single Gaussian field then fNL is scale-independent...

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Bibliographic Details
Main Authors: Byrnes, Christian (Author) , Gerstenlauer, Mischa (Author) , Nurmi, Sami (Author) , Tasinato, Gianmassimo (Author) , Wands, D. (Author)
Format: Article (Journal)
Language:English
Published: 26 February 2010
In: Journal of cosmology and astroparticle physics
Year: 2010, Issue: 2, Pages: 1-24
ISSN:1475-7516
DOI:10.1088/1475-7516/2010/02/034
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1088/1475-7516/2010/02/034
Verlag, lizenzpflichtig, Volltext: https://dx.doi.org/10.1088/1475-7516/2010/02/034
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Author Notes:Christian T. Byrnes, Sami Nurmi, Gianmassimo Tasinato and David Wands
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Summary:We consider possible scale-dependence of the non-linearity parameter fNL in local and quasi-local models of non-Gaussian primordial density perturbations. In the simplest model where the primordial perturbations are a quadratic local function of a single Gaussian field then fNL is scale-independent by construction. However scale-dependence can arise due to either a local function of more than one Gaussian field, or due to non-linear evolution of modes after horizon-exit during inflation. We show that the scale dependence of fNL is typically first order in slow-roll. For some models this may be observable with experiments such as Planck provided that fNL is close to the current observational bounds.
Item Description:Gesehen am 23.03.2023
Im Titel ist "NL" nach f tiefgestellt
Physical Description:Online Resource
ISSN:1475-7516
DOI:10.1088/1475-7516/2010/02/034