Geometrical Destabilisation of Ultra-Light Axions in String Inflation
High Energy Physics - Theory
2019-06-05 v1 Cosmology and Nongalactic Astrophysics
Abstract
We perform a detailed analytical and numerical analysis of the multi-field evolution of Fibre Inflation and show that, regardless of the microscopic realisation of the model, the mass-squared of one of the two ultra-light axions becomes always negative during inflation. This implies that the corresponding isocurvature perturbations experience a potential geometrical destabilisation which seems to bring the system away from the perturbative regime. Therefore we conclude that a full understanding of the inflationary evolution of Fibre Inflation can be achieved only via a non-perturbative analysis where the backreaction of tachyonic isocurvature perturbations is properly taken into account.
Keywords
Cite
@article{arxiv.1903.01497,
title = {Geometrical Destabilisation of Ultra-Light Axions in String Inflation},
author = {Michele Cicoli and Veronica Guidetti and Francisco G. Pedro},
journal= {arXiv preprint arXiv:1903.01497},
year = {2019}
}
Comments
22 pages + bibliography, 9 figures