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Axion String Constraints

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Battye, R. A., Shellard, E. P. S.·1994·Physical Review Letters

Abstract

We study the production of cosmological axions in the standard scenario in which a global string network forms at the Peccei-Quinn phase transition. We make detailed calculations of the axions produced by string loops, comparing these with estimates of other contributions from long strings and domain walls. We delineate key uncertainties in string network evolution, the chief of which is the magnitude of radiative backreaction. We conclude that axions produced by these topological contributions provide the significant cosmological constraint on the symmetry breaking scale ${f}_{a}$ and the axion mass ${m}_{a}$.

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Metadata

Authors
Battye, R. A., & Shellard, E. P. S.
Venue
Physical Review Letters
Published
1994-11-28
Volume
73
Issue
22
Pages
2954-2957
ISSN
0031-9007 (ISSN-L)
OpenAlex
W2041523692
Cited by
160
References
0
FWCI
6.80
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Axion String Constraints. https://app.cochat.ai/papers/10.1103/physrevlett.73.2954
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Battye, R. A., & Shellard, E. P. S. (1994). Axion String Constraints. Physical Review Letters. https://doi.org/10.1103/physrevlett.73.2954

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