arXiv · 1403.4186
Solving the Tension between High-Scale Inflation and Axion Isocurvature Perturbations
Abstract
The BICEP2 experiment determined the Hubble parameter during inflation to be about $10^{14}$ GeV. Such high inflation scale is in tension with the QCD axion dark matter if the Peccei-Quinn (PQ) symmetry remains broken during and after inflation, because too large axion isocurvature perturbations would be generated. The axion isocurvature perturbations can be suppressed if the axion acquires a sufficiently heavy mass during inflation. We show that this is realized if the PQ symmetry is explicitly broken down to a discrete symmetry and if the breaking is enhanced during inflation. We also show that, even when the PQ symmetry becomes spontaneously broken after inflation, such a temporarily enhanced PQ symmetry breaking relaxes the constraint on the axion decay constant.
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Tetsutaro Higaki, Kwang Sik Jeong, Fuminobu Takahashi. 2014-08-19. Solving the Tension between High-Scale Inflation and Axion Isocurvature Perturbations. https://doi.org/10.1016/j.physletb.2014.05.014
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