pith. sign in

arxiv: 1411.4501 · v2 · pith:KJX6JFFInew · submitted 2014-11-17 · 🌌 astro-ph.CO

Constraining Galileon Inflation

classification 🌌 astro-ph.CO
keywords datagalileonmodelbispectrumanalysisapplybayesianbest
0
0 comments X
read the original abstract

In this short paper, we present constraints on the Galileon inflationary model from the CMB bispectrum. We employ a principal-component analysis of the independent degrees of freedom constrained by data and apply this to the WMAP 9-year data to constrain the free parameters of the model. A simple Bayesian comparison establishes that support for the Galileon model from bispectrum data is at best weak.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

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

  1. Planck 2018 results. X. Constraints on inflation

    astro-ph.CO 2018-07 accept novelty 4.0

    Updated Planck CMB measurements give ns = 0.9649 ± 0.0042, r < 0.056, confirm flatness at 0.4 percent, and show no evidence for scale-dependent features or non-slow-roll dynamics in the inflaton potential.