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Large non-Gaussianities in the Effective Field Theory Approach to Single-Field Inflation: the Trispectrum

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arxiv 1006.5411 v1 pith:XNFKJDOL submitted 2010-06-28 astro-ph.CO gr-qchep-phhep-th

Large non-Gaussianities in the Effective Field Theory Approach to Single-Field Inflation: the Trispectrum

classification astro-ph.CO gr-qchep-phhep-th
keywords theorytrispectrumgeneraleffectivefieldinflationinteractionslarge
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We perform the analysis of the trispectrum of curvature perturbations generated by the interactions characterizing a general theory of single-field inflation obtained by effective field theory methods. We find that curvature-generated interaction terms, which can in general give an important contribution to the amplitude of the four-point function, show some new distinctive features in the form of their trispectrum shape-function. These interesting interactions are invariant under some recently proposed symmetries of the general theory and, as shown explicitly, do allow for a large value of the trispectrum.

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  1. Trispectrum in Extended USR Model with Transition to SR

    astro-ph.CO 2025-09 conditional novelty 6.0

    In the two-phase USR-SR inflation model, g_NL = 25 h^3 / (3 (h-6)^3) and tau_NL = 9 h^4 / (h-6)^4, confirmed by both delta-N and in-in formalisms.