Kinetic Axion from non-minimally coupled PQ Field

26 Sept 2024, 15:20
16m
Seminar room 4a

Seminar room 4a

Cosmology & Astroparticle Physics Parallel Thursday Cosmo 3

Speaker

Riccardo Natale (DESY)

Description

Axion Kinetic Misalignment can be generated by higher-order operators that explicitly break the PQ symmetry at very high energies. This results in a kick in the angular direction of the PQ field, causing a delay in the onset of axion oscillations. For the higher-order operator to be relevant, the PQ radial mode must reach very high values. We explore the possibility that a non-minimally coupled PQ field, with a $\xi R|\Phi|^2$ term, combined with a stiff era, can generate the exact initial conditions for a Kinetic Misalignment Mechanism.

Primary authors

Riccardo Natale (DESY) Enrico Morgante (U. Trieste & INFN)

Presentation materials