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Published July 29, 1968 | Version public
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Gravitational radiation damping

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Abstract

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).

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©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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CaltechAUTHORS:THOprl68

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2006-08-08
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