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• W3105296421 abstract "We compute the fully non-linear cosmic microwave background (CMB) anisotropies on scales larger than the horizon at last scattering in terms of only the curvature perturbation, providing a generalization of the linear Sachs–Wolfe effect at any order in perturbation theory. We show how to compute the n-point connected correlation functions of the large-scale CMB anisotropies for generic primordial seeds provided by standard slow-roll inflation as well as the curvaton and other scenarios for the generation of cosmological perturbations. As an application of our formalism, we compute the three- and four-point connected correlation functions whose detection in future CMB experiments might be used to assess the level of primordial non-Gaussianity, giving the theoretical predictions for the parameters of quadratic and cubic non-linearities fNL and gNL." @default.
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• W3105296421 date "2005-08-23" @default.
• W3105296421 modified "2023-09-25" @default.
• W3105296421 title "Non-Gaussianity of large-scale cosmic microwave background anisotropies beyond perturbation theory" @default.
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• W3105296421 doi "https://doi.org/10.1088/1475-7516/2005/08/010" @default.
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