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Strongly scale-dependent polyspectra from curvaton self-interactions

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arxiv 1108.2708 v2 pith:BDMU7ZY4 submitted 2011-08-12 astro-ph.CO hep-th

classification astro-ph.COhep-th
keywords curvatonself-interactionsmodelmodelsparametersspectraladditionalbehaviour
verification ladder T0 review T1 audit T2 compute T3 formal
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We study the scale dependence of the non-linearity parameters f_NL and g_NL in curvaton models with self-interactions. We show that the spectral indices n_fNL=d ln|f_NL|/(d ln k) and n_gNL=d ln |g_NL|/(d ln k) can take values much greater than the slow--roll parameters and the spectral index of the power spectrum. This means that the scale--dependence of the bi and trispectrum could be easily observable in this scenario with Planck, which would lead to tight additional constraints on the model. Inspite of the highly non-trivial behaviour of f_NL and g_NL in the curvaton models with self-interactions, we find that the model can be falsified if g_NL(k) is also observed.

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Cited by 2 Pith papers

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

  1. Memoirs of the curvaton: non-perturbative non-Gaussianity and supermassive primordial black holes

    astro-ph.CO 2026-06 unverdicted novelty 6.0 of 10

    Curvaton self-interactions in non-quadratic potentials produce a local non-Gaussian map that enables supermassive primordial black hole formation at peak amplitudes of order 10^{-5} while remaining consistent with μ-d...

  2. Curvaton distribution from stochastic inflation

    astro-ph.CO 2024-11 conditional novelty 5.0 of 10

    Closed-form probability distributions for the curvature perturbation are derived for four exactly solvable curvaton potentials, and the mass-decay-rate parameter space is split into regions by the probability of produ...

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