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Non-linear isocurvature perturbations and non-Gaussianities

David Langlois1, Filippo Vernizzi2 and David Wands3

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We study non-linear primordial adiabatic and isocurvature perturbations and their non-Gaussianity. After giving a general formulation in the context of an extended δN formalism, we analyse in detail two illustrative examples. The first is a mixed curvaton–inflaton scenario in which fluctuations of both the inflaton and a curvaton (a light isocurvature field during inflation) contribute to the primordial density perturbation. The second example is that of double inflation involving two decoupled massive scalar fields during inflation. In the mixed curvaton–inflaton scenario we find that the bispectrum of primordial isocurvature perturbations may be large and comparable to the bispectrum of adiabatic curvature perturbations.


Keywords

cosmological perturbation theory

inflation

physics of the early universe

 

E-print Number: 0809.4646

Cited: by |

Refers: to

PACS

98.80.Cq Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)

98.70.Vc Background radiations

Subjects

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 12 (December 2008)

Received 4 October 2008, accepted for publication 4 November 2008

Published 2 December 2008



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