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Inflationary axion cosmology

Turner, Michael S., Wilczek, Frank·1991·Physical Review Letters

Abstract

If Peccei-Quinn (PQ) symmetry is broken after inflation, the initial axion angle is a random variable on cosmological scales; based on this fact, estimates of the relic-axion mass density give too large a value if the axion mass is less than about ${10}^{\mathrm{\ensuremath{-}}6}$ eV. This bound can be evaded if the Universe underwent inflation after PQ symmetry breaking and if the observable Universe happens to be a region where the initial axion angle was atypically small, ${\mathrm{\ensuremath{\theta}}}_{1}$\ensuremath{\lesssim}[${\mathit{m}}_{\mathit{a}}$/(${10}^{\mathrm{\ensuremath{-}}6}$ eV${]}^{0.59}$.] We show consideration of fluctuations induced during inflation severely constrains the latter alternative.

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Metadata

Authors
Turner, M. S., & Wilczek, F.
Venue
Physical Review Letters
Published
1991-01-07
Volume
66
Issue
1
Pages
5-8
ISSN
0031-9007 (ISSN-L)
OpenAlex
W2172058970
Cited by
183
References
0
FWCI
4.59
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Inflationary axion cosmology. https://app.cochat.ai/papers/10.1103/physrevlett.66.5
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Turner, M. S., & Wilczek, F. (1991). Inflationary axion cosmology. Physical Review Letters. https://doi.org/10.1103/physrevlett.66.5

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