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Runnings in the curvaton

Kobayashi T.
•
Takahashi T.
2012
  • journal article

Periodico
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Abstract
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 f NL becomes strongly scale-dependent. From the point of view of the f NL 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 f NL 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 f NL can be large enough to be probed with future CMB experiments. © 2012 IOP Publishing Ltd and Sissa Medialab srl.
DOI
10.1088/1475-7516/2012/06/004
WOS
WOS:000306003500004
Archivio
http://hdl.handle.net/20.500.11767/124829
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-84863475127
https://arxiv.org/abs/1203.3011
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Soggetti
  • cosmological perturba...

  • non-gaussianity

  • physics of the early ...

  • power spectrum

  • Settore FIS/02 - Fisi...

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