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Primordial non-gaussianities in single field inflation

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arxiv astro-ph/0503692 v2 pith:V2SAF47J submitted 2005-03-31 astro-ph gr-qchep-th

classification astro-phgr-qchep-th
keywords fieldfunctionscalarspeedthree-pointinflationparametersprimordial
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We calculate the three-point function for primordial scalar fluctuations in a single field inflationary scenario where the scalar field Lagrangian is a completely general function of the field and its first derivative. We obtain an explicit expression for the three-point correlation function in a self-consistent approximation scheme where the expansion rate varies slowly, analogous to the slow-roll limit in standard, single-field inflation. The three-point function can be written in terms of the familiar slow-roll parameters and three new parameters which measure the non-trivial kinetic structure of the scalar field, the departure of the sound speed from the speed of light, and the rate of change of the sound speed.

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Cited by 4 Pith papers

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

  1. Stochastic scalar-tensor inflation and beyond

    gr-qc 2026-06 unverdicted novelty 7.0 of 10

    Extends the stochastic inflation formalism to a wide class of scalar-tensor theories by mapping EFT of dark energy coefficients to stochastic equations of motion.

  2. Non-Gaussianity in SMICA

    astro-ph.CO 2025-11 unverdicted novelty 7.0 of 10

    New SMICA formalism and binned bispectrum estimator jointly recover power spectra, spectral parameters, foreground 3-point correlators, and primordial non-Gaussianity constraints from multi-frequency polarization maps...

  3. Inflationary trispectrum of gauge fields from scalar and tensor exchanges

    hep-th 2025-09 conditional novelty 6.0 of 10

    The inflationary trispectrum of gauge fields from scalar and tensor exchanges is derived analytically, yielding beta^zeta_nl = (b^zeta_nl)^2 in the counter-collinear limit and growing flattened-limit signals.

  4. Stochastic Homology of Gaussian vs. non-Gaussian Random Fields: Graphs towards Betti Numbers and Persistence Diagrams

    astro-ph.CO 2019-08 conditional novelty 5.0 of 10

    The paper introduces a Morse-graph formalism that yields approximate, one-parameter-fitted formulas for expected Betti numbers of 2D Gaussian random fields and shows these homology statistics are sensitive to local no...

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