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Tidal radiationThe general theory of tides is developed within the framework of Einstein's theory of gravitation. It is based on the concept of Fermi frame and the associated notion of tidal frame along an open curve in spacetime. Following the previous work of the author an approximate scheme for the evaluation of tidal gravitational radiation is presented which is valid for weak gravitational fields. The emission of gravitational radiation from a body in the field of a black hole is discussed, and for some cases of astrophysical interest estimates are given for the contributions of radiation due to center-of-mass motion, purely tidal deformation, and the interference between the center of mass and tidal motions.
Document ID
19770062405
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Mashhoon, B.
(Maryland, University College Park, Md.; Utah, University, Salt Lake City, Utah, United States)
Date Acquired
August 9, 2013
Publication Date
September 1, 1977
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
77A45257
Funding Number(s)
CONTRACT_GRANT: NSF GP-43708X
CONTRACT_GRANT: NGR-21-002-010
CONTRACT_GRANT: NSF PHY-74-16311-A02
Distribution Limits
Public
Copyright
Other

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