English

Bayesian evidence of the post-Planck curvaton

Cosmology and Nongalactic Astrophysics 2015-08-05 v2 High Energy Physics - Theory

Abstract

We perform a Bayesian model comparison for scenarios within the quadratic curvaton model, determining the degree to which both are disfavoured with respect to the Λ\LambdaCDM concordance model and single-field quadratic inflation, using the recent \emph{Planck} data release. Despite having three additional model parameters, the simplest curvaton scenario is not disfavoured relative to single-field quadratic inflation, and it becomes favoured against this single-field model when we include the joint BICEP/Keck/\emph{Planck} analysis. In all cases we assume an instantaneous inflaton decay and no surviving isocurvature perturbations. Despite the success of \emph{Planck} reaching its forecast measurement accuracy, we show that the current constraints on local non-Gaussianity are insufficiently precise to have any significant impact on the evidence ratios so far. We also determine the precision σ(fNL)\sigma(f_{\mathrm{NL}}) required by future measurements assuming a fiducial value of fNL=5/4f_{\mathrm{NL}}=-5/4 or 10.810.8 to no longer disfavour the curvaton against the Λ\LambdaCDM parametrisation, and we discuss the effect that the predicted increase in precision from future measurements on fNLf_{\mathrm{NL}} may have. We show that our results are not very sensitive to our choice of priors.

Keywords

Cite

@article{arxiv.1502.06951,
  title  = {Bayesian evidence of the post-Planck curvaton},
  author = {Robert J. Hardwick and Christian T. Byrnes},
  journal= {arXiv preprint arXiv:1502.06951},
  year   = {2015}
}

Comments

14 pages, 1 figure, 5 tables, Version 2

R2 v1 2026-06-22T08:37:00.094Z