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Calculations for cosmic axion detectionCalculations are presented, using properly nomalized couplings and masses for Dine-Fischler-Srednicki axions, of power rates and signal temperatures for axion-photon conversion in microwave cavities. The importance of the galactic-halo axion line shape is emphasized. Spin-coupled detection as an alternative to magnetic-field-coupled detection is mentioned.
Document ID
19860028136
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1103/PhysRevLett.55.1797
Authors
Krauss, L. (Harvard University Cambridge, MA, United States)
Moody, J. (Harvard Univ. Cambridge, MA, United States)
Wilczek, F. (California, University Santa Barbara, United States)
Morris, D. E. (California, University Berkeley, United States)
Date Acquired
August 12, 2013
Publication Date
October 21, 1985
Publication Information
Publication: Physical Review Letters
Volume: 55
ISSN: 0031-9007
Subject Category
Space Radiation
Accession Number
86A12874
Funding Number(s)
CONTRACT_GRANT: NSF PHY-82-15492
CONTRACT_GRANT: DE-AC03-76SF-0098
CONTRACT_GRANT: NSF PHY-82-17853
Distribution Limits
Public
Copyright
Other

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