pith. sign in

arxiv: 1506.01244 · v2 · pith:R77VFCPDnew · submitted 2015-06-03 · 🌀 gr-qc · astro-ph.CO· hep-th

Non-canonical inflation coupled to matter

classification 🌀 gr-qc astro-ph.COhep-th
keywords mattercoupledinflationconformallycorrectionsnon-relativisticabruptlyadditional
0
0 comments X
read the original abstract

We compute corrections to the inflationary potential due to conformally coupled non-relativistic matter. We find that under certain conditions of the matter coupling, inflation may be interrupted abruptly. We display this in the superconformal Starobinsky model, where matter is conformally coupled to the Einstein frame metric. These corrections may easily stop inflation provided that there is an initial density of non-relativistic matter. Since these additional heavy degrees of freedom generically occur in higher dimension theories, for example as Kaluza-Klein modes, this effect can arise in multiple scenarios.

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. Constraints on non-canonical chaotic inflation from ACT DR6 and BICEP/Keck data

    gr-qc 2026-05 unverdicted novelty 3.0

    MCMC fitting of joint P-ACT-LB-BK18 dataset constrains non-canonical parameter alpha to 8.8, 11.7, and 16.4 (1 sigma) for chaotic inflation potentials with n=1/3, 2/3, 1 respectively.