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On primordial trispectrum from exchanging scalar modes in general multiple field inflationary models

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arxiv 1009.1311 v2 pith:WFLS43FB submitted 2010-09-07 hep-th astro-ph.CO

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keywords primordialtrispectrummodelsexchanginggeneralizedmodesmulti-fieldscalar
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We make an complementary investigation of the primordial trispectrum from exchanging intermediate scalar modes in multi-field inflation models with generalized kinetic terms. Together with the calculation of irreducible contributions to the primordial trispectrum in Ref.[103], we give the full leading-order primordial trispectrum in generalized multi-field models.

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  1. Trispectrum in Extended USR Model with Transition to SR

    astro-ph.CO 2025-09 conditional novelty 6.0 of 10

    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.

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