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Curvaton model constraints from WMAP

delete2003-11-01
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PRE
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C
Chris Gordon
A
Antony Lewis
DOI:10.1016/j.newar.2003.07.021delete
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摘要

摘要

En 中文
Simple curvaton models can generate a mixture of correlated primordial adiabatic and isocurvature perturbations. Working numerically we use the latest WMAP observations and a variety of other data to constrain the curvaton model. We find that models with an isocurvature contribution are not favored relative to simple purely adiabatic models. However, a significant primordial totally correlated baryon isocurvature perturbation is not ruled out. Certain classes of curvaton model are thereby ruled out, other classes predict enough non-Gaussianity to be detectable by the Planck satellite. (C) 2003 Elsevier B.V. All rights reserved.
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