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Axion emission from neutron starsIt is shown 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.
Document ID
19840065188
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1103/PhysRevLett.53.1198
Authors
Iwamoto, N. (California, University Santa Barbara, CA; Washington University, St. Louis, MO, United States)
Date Acquired
August 12, 2013
Publication Date
September 17, 1984
Publication Information
Publication: Physical Review Letters
Volume: 53
ISSN: 0031-9007
Subject Category
Astrophysics
Accession Number
84A47975
Funding Number(s)
CONTRACT_GRANT: NSF PHY-77-27084
CONTRACT_GRANT: NSF DMR-83-04213
Distribution Limits
Public
Copyright
Other

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