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Massive Black Holes and the Laser Interferometer Space Antenna (LISA)The goals of the USA mission include both astrophysical investigations and fundamental physics tests. The main astrophysical questions concern the space density, growth, mass function, and surroundings of massive black holes. Thus the crucial issue for the USA mission is the likelihood of observing signals from such sources. Four possible sources of this kind are discussed briefly in this paper. It appears plausible, or even likely. that one or more of these types of sources can be detected and studied by LISA.
Document ID
19990066627
Acquisition Source
Headquarters
Document Type
Reprint (Version printed in journal)
Authors
Blender, Peter L.
(Colorado Univ. Boulder, CO United States)
Hils, Dieter
(Colorado Univ. Boulder, CO United States)
Stebbins, Robin T.
(Colorado Univ. Boulder, CO United States)
Date Acquired
August 19, 2013
Publication Date
January 1, 1998
Publication Information
Publication: Eighteenth Texas Symposium on Relativistic Astrophysics and Cosmology
Publisher: World Scientific Publishing Co. Pte. Ltd.
ISBN: 9810234872
Subject Category
Astrophysics
Report/Patent Number
LC-98-16902
Meeting Information
Meeting: Relativistic Astrophysics and Cosmology
Location: Chicago, IL
Country: United States
Start Date: December 15, 1996
End Date: December 20, 1996
Sponsors: Fermi National Accelerator Lab., Department of Energy, NASA Headquarters, National Science Foundation, Chicago Univ.
Funding Number(s)
CONTRACT_GRANT: NAGw-4772
CONTRACT_GRANT: NAGw-4865
Distribution Limits
Public
Copyright
Other

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