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We show that axion emission from neutron stars is the dominant energy-loss mechanism for a range of values of the Peccei-Quinn symmetry-breaking scale (F) not excluded by previous constraints. This gives the possibility of obtaining a better bound on F from measurements of surface temperature of neutron stars.
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Naoki Iwamoto (Mon,) studied this question.
synapsesocial.com/papers/6a203c6761bb8c494db5d82d — DOI: https://doi.org/10.1103/physrevlett.53.1198
Naoki Iwamoto
Wave Life Sciences (United States)
Physical Review Letters
University of California, Santa Barbara
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