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.
2019
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].
Cicoli M.; Guidetti V.; Pedro F.G.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/695704
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