Thorne, Kip S. (1968) Gravitational radiation damping. Physical Review Letters, 21 (5). pp. 320-323. ISSN 0031-9007. doi:10.1103/PhysRevLett.21.320. https://resolver.caltech.edu/CaltechAUTHORS:THOprl68
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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).
Item Type: | Article | ||||||
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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. | ||||||
Group: | TAPIR | ||||||
Issue or Number: | 5 | ||||||
DOI: | 10.1103/PhysRevLett.21.320 | ||||||
Record Number: | CaltechAUTHORS:THOprl68 | ||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:THOprl68 | ||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
ID Code: | 4222 | ||||||
Collection: | CaltechAUTHORS | ||||||
Deposited By: | Tony Diaz | ||||||
Deposited On: | 08 Aug 2006 | ||||||
Last Modified: | 08 Nov 2021 20:15 |
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