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Trispectrum in Extended USR Model with Transition to SR

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arxiv 2509.09608 v1 pith:YJN7DEKF submitted 2025-09-11 astro-ph.CO gr-qchep-th

Trispectrum in Extended USR Model with Transition to SR

classification astro-ph.CO gr-qchep-th
keywords trispectrumphaseinflationstagetransitionattractorextendedsetup
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the trispectrum in a two-phase USR-SR setup of inflation in which the USR stage is extended in the initial phase of inflation while the second stage of inflation proceeds via a slow-roll phase. A key role is played by the sharpness parameter which controls how quickly the system reaches the final attractor phase after the USR stage. We employ both $\delta N$ and in-in formalisms and calculate trispectrum and the corresponding dimensionless parameters $g_{NL}$ and $\tau_{NL}$. We show that both approaches yield the same results and study the shapes of trispectrum in various configurations. It is shown that the maximum value of trispectrum occurs in the setup with an infinitely sharp transition to the attractor phase while much of trispectrum is washed out in the opposite limit of a mild transition.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Evolution of Linear Perturbations under Time-Dependent Hubble Friction I: SR-USR-SR Inflation

    gr-qc 2026-02 conditional novelty 5.0

    Analytic asymptotics show the dip in the SR-USR-SR curvature power spectrum comes from cancellation between two growing modes, not a constant-versus-growing cancellation.