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Schwinger-Keldysh mechanism in extended quasi single field inflation

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arxiv 1901.01905 v1 pith:WUM53IMK submitted 2019-01-07 gr-qc astro-ph.COhep-th

Schwinger-Keldysh mechanism in extended quasi single field inflation

classification gr-qc astro-ph.COhep-th
keywords inflationmechanismschwinger-keldyshfieldfieldssemi-heavyamplitudesanalysis
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study an extension of quasi-single field model of inflation containing multiple semi-heavy isocurvaton fields using the Schwinger-Keldysh mechanism. We calculate the amplitudes and the shapes of the bispectrum and the trispectrum. We show that the diagrammatic approach associated with the Schwinger-Keldysh mechanism simplifies the analysis considerably compared to standard in-in formalism. This method is helpful to study the spectroscopy of masses and couplings of light and semi-heavy fields during inflation.

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Cited by 1 Pith paper

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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.