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Phys. Rev. D 67, 121301(R) (2003) [5 pages]

Inflationary models inducing non-Gaussian metric fluctuations

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Francis Bernardeau
Service de Physique Théorique, CEA/DSM/SPhT, Unité de recherche associée au CNRS, CEA/Saclay 91191 Gif-sur-Yvette cédex, France

Jean-Philippe Uzan
Laboratoire de Physique Théorique, CNRS-UMR 8627, Bât. 210, Université Paris XI, F-91405 Orsay Cedex, France
Institut d’Astrophysique de Paris, GReCO, CNRS-FRE 2435, 98 bis, Bd Arago, 75014 Paris, France

Received 17 September 2002; published 4 June 2003

We construct explicit models of multifield inflation in which the primordial metric fluctuations do not necessarily obey Gaussian statistics. These models are realizations of mechanisms in which non-Gaussianity is first generated by a light scalar field and then transferred into curvature fluctuations. The probability distribution functions of the metric perturbation at the end of inflation are computed. This provides a guideline for designing strategies to search for non-Gaussian signals in future CMB and large scale structure surveys.

© 2003 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.67.121301
DOI:
10.1103/PhysRevD.67.121301
PACS:
98.80.Cq