DOE OSTI · 22277839
Supercurvaton
Abstract
We discuss observational consequences of the curvaton scenario, which naturally appears in the context of the simplest model of chaotic inflation in supergravity. The non-gaussianity parameter f{sub NL} in this scenario is very sensitive to the choice of the model parameters; it can be either very small or very large. Under certain conditions, this parameter can take values in the observationally interesting range from O(10) to O(100). We point out that local f{sub NL} can take different values in different parts of the universe. The regions where f{sub NL} is particularly large form a curvaton web resembling a net of thick domain walls, strings, or global monopoles.
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Demozzi, Vittoria, Mukhanov, Viatcheslav, Linde, Andrei. 2011-04-01. Supercurvaton. https://doi.org/10.1088/1475-7516%2F2011%2F04%2F013
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