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arxiv 1203.3011 v2 pith:OHZAIBJC submitted 2012-03-14 astro-ph.CO hep-phhep-th

Runnings in the Curvaton

classification astro-ph.CO hep-phhep-th
keywords curvatonperturbationscurvatonsdensityrunningslargelinearmodels
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We investigate the scale-dependence, or the runnings, of linear and second order density perturbations generated in various curvaton scenarios. We argue that the second order perturbations, i.e. non-Gaussianity, can strongly depend on the scale, even when the linear perturbations are nearly scale-invariant. We present analytic formulae for the runnings from curvatons with general energy potentials, and clarify the conditions under which fNL becomes strongly scale-dependent. From the point of view of the fNL running, curvaton potentials can be classified into roughly two categories by whether the potential flattens or steepens compared to a quadratic one. As such examples, we study pseudo-Nambu-Goldstone curvatons, and self-interacting curvatons, respectively. The dynamics of non-quadratic curvatons and the behaviors of the resulting density perturbations are clarified by analytical methods. Then we also study models where multiple source can be responsible for density perturbations such as the multi-curvaton, and mixed curvaton and inflaton models where the running of fNL can also be large due to their multi-source nature. We make quantitative analysis for each curvaton scenario and discuss in what cases the scale-dependence, in particular, of fNL can be large enough to be probed with future CMB experiments.

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Cited by 2 Pith papers

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

  1. Blue-tilted Runnings and the JWST Early Galaxy Tension

    astro-ph.CO 2026-05 unverdicted novelty 4.0

    A blue-tilted spectrum with running parameters α_s ≈ 0.2 and β_s ≈ 0.2 resolves the JWST early-galaxy abundance tension at 1σ in a joint CMB analysis.

  2. Blue-tilted Runnings and the JWST Early Galaxy Tension

    astro-ph.CO 2026-05 unverdicted novelty 4.0

    Blue-tilted running spectrum with α_s ≈ 0.02 and β_s ≈ 0.02 resolves JWST early galaxy tension at 1σ in joint CMB analysis.