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.
Cicoli M., Guidetti V., Pedro F.G. (2019). Geometrical destabilisation of ultra-light axions in string inflation. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2019(5), 046-046 [10.1088/1475-7516/2019/05/046].
Geometrical destabilisation of ultra-light axions in string inflation
Cicoli M.Supervision
;Guidetti V.Membro del Collaboration Group
;Pedro F. G.Membro del Collaboration Group
2019
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.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.