English

Non-minimally Coupled Pseudoscalar Inflaton

Cosmology and Nongalactic Astrophysics 2018-10-17 v2 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

We consider a scenario in which the inflaton ϕ\phi is a pseudoscalar field non-minimally coupled to gravity through a term of the form XRϕ2{\cal X} R \phi^2. The pseudoscalar is also coupled to a U(1)U(1) gauge field (or an ensemble of N{\cal N} gauge fields) through an axial coupling of the form ϕFF~\phi F \tilde{F}. After M. M. Anber and L. Sorbo, Phys. Rev. D 81, 043534 (2010), Ref. [1], it is well known that this axial coupling leads to a production of gauge particles which acts as a friction term in the dynamics of the inflaton, producing a slow-roll regime even in presence of a steep potential. A remarkable result in this scenario, is that the spectrum of the chiral gravitational waves sourced by the scalar-gauge field interplay can be enhanced due to the non-minimal coupling with gravity, leading to measurable signatures, while maintaining agreement with current observational constraints on nsn_s and rr. The inclusion of non-minimal coupling could be helpful to alleviate tensions with non-Gaussianity bounds in models including axial couplings.

Keywords

Cite

@article{arxiv.1803.09743,
  title  = {Non-minimally Coupled Pseudoscalar Inflaton},
  author = {Juan P. Beltrán Almeida and Nicolás Bernal},
  journal= {arXiv preprint arXiv:1803.09743},
  year   = {2018}
}

Comments

Two figures and one appendix added. Several references added. Matches the version accepted for publication in PRD

R2 v1 2026-06-23T01:05:34.447Z