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Gamma rays and energetic particles from primordial black holesThe standard model of quarks and leptons is used to discuss the signatures of black-hole evaporations. A firm bound on the primordial black hole abundance is obtained from MeV data. It is argued that the MeV bound can be improved by exploiting the new generation of TeV and PeV telescopes.
Document ID
19920028972
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Halzen, F.
(Wisconsin Univ. Madison, WI, United States)
Zas, E.
(Wisconsin, University Madison, United States)
Macgibbon, J. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Weekes, T. C.
(Whipple Observatory Amado, AZ, United States)
Date Acquired
August 15, 2013
Publication Date
October 31, 1991
Publication Information
Publication: Nature
Volume: 353
ISSN: 0028-0836
Subject Category
Space Radiation
Accession Number
92A11596
Distribution Limits
Public
Copyright
Other

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