Thorne, Kip S. (1968) Gravitational radiation damping. Physical Review Letters, 21 (5). pp. 320-323. ISSN 0031-9007 http://resolver.caltech.edu/CaltechAUTHORS:THOprl68
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An analysis is presented of the emission of gravitational waves by a star in nonradial pulsation. This analysis, rigorous to first order in the pulsation amplitude and to all orders in G and c, exhibits damping of the pulsation as the waves are emitted (gravitational radiation reaction).
|Additional Information:||©1968 The American Physical Society. Received 7 June 1968. Work supported in part by the National Science Foundation (Grant No. GP-7976 formerly GP-5391 at Caltech, GP 8129 at the University of Chicago), and by the Office of Naval Research [Contract No. Nonr-220(47) at Caltech]. [K.S.T. was an] Alfred P. Sloan Research Fellow during the entire period of this research; John Simon Guggenheim Fellow during part.|
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|Deposited By:||Tony Diaz|
|Deposited On:||08 Aug 2006|
|Last Modified:||26 Dec 2012 08:58|
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