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Telescope search for a 3-eV to 8-eV axionAxions of mass 3-8 eV should have a cosmological abundance of about 50/cu cm and reside in rich clusters of galaxies. Their decays to two photons will produce a line at a wavelength of about 3100-8300 A. This effort has searched unsuccessfully for such a feature in the tergalactic light of three rich clusters, closing this 'window', and leaving open only the window from 10 to the -6th to 0.001 eV. This implies that if the axion exists, it likely comprises the dark matter. The present flux limits are of relevance to other relics whose decays produce monoenergetic photons.
Document ID
19910044091
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Bershady, Matthew A.
(Chicago, University IL, United States)
Ressell, M. Ted
(Chicago Univ. Chicago, IL, United States)
Turner, Michael S.
(NASAFermilab Astrophysics Center Batavia; Chicago, University, IL, United States)
Date Acquired
August 14, 2013
Publication Date
March 18, 1991
Publication Information
Publication: Physical Review Letters
Volume: 66
ISSN: 0031-9007
Subject Category
Astrophysics
Accession Number
91A28714
Funding Number(s)
CONTRACT_GRANT: NAGW-1340
Distribution Limits
Public
Copyright
Other

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