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• W2034201851 abstract "We provide a general formalism to calculate the infrared correlators of multiple interacting scalar fields in the de Sitter space by means of the stochastic approach. These scalar fields are treated as test fields, and hence our result is applicable to the models such as the curvaton scenario where the fields that yield initially isocurvature modes do not contribute to the cosmic energy density during inflationary expansion. The stochastic formalism combined with the argument of conformal invariance of the correlators reflecting the de Sitter isometries allows us to fix the form and amplitude of the three-point functions completely and partially for the four-point functions in terms of calculable quantities. It turns out that the naive scaling argument employed in the previous literature does not necessarily hold, and we derive the necessary and sufficient condition for the correlator to obey the naive scaling. We also find that correlation functions can, in principle, exhibit more complicated structure than argued in the literature." @default.
• W2034201851 created "2016-06-24" @default.
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• W2034201851 date "2012-12-10" @default.
• W2034201851 modified "2023-10-17" @default.
• W2034201851 title "Consequences of a stochastic approach to the conformal invariance of inflationary correlators" @default.
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• W2034201851 doi "https://doi.org/10.1103/physrevd.86.123514" @default.
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