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Planck-scale corrections to axion models

Barr, S. M., Seckel, D.·1992·Physical Review D

Abstract

It has been argued that quantum gravitational effects will violate all nonlocal symmetries. Peccei-Quinn symmetries must therefore be an "accidental" or automatic consequence of local gauge symmetry. Moreover, higher-dimensional operators suppressed by powers of ${M}_{\mathrm{Pl}}$ are expected to explicitly violate the Peccei-Quinn symmetry. Unless these operators are of dimension $d\ensuremath{\ge}10$, axion models do not solve the strong $\mathrm{CP}$ problem in a natural fashion. A small gravitationally induced contribution to the axion mass has little if any effect on the density of relic axions. If $d=10,11,or 12$ these operators can solve the axion domain-wall problem, and we describe a simple class of Kim-Shifman-Vainshtein-Zakharov axion models where this occurs. We also study the astrophysics and cosmology of "heavy axions" in models where $5\ensuremath{\le}d\ensuremath{\le}10$.

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Metadata

Authors
Barr, S. M., & Seckel, D.
Venue
Physical Review D
Published
1992-07-15
Volume
46
Issue
2
Pages
539-549
ISSN
0556-2821 (ISSN-L)
OpenAlex
W2138268757
Cited by
434
References
0
FWCI
7.31
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Planck-scale corrections to axion models. https://app.cochat.ai/papers/10.1103/physrevd.46.539
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Barr, S. M., & Seckel, D. (1992). Planck-scale corrections to axion models. Physical Review D. https://doi.org/10.1103/physrevd.46.539

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