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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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 |
| Record Number: | CaltechAUTHORS:THOprl68 |
| Persistent URL: | http://resolver.caltech.edu/CaltechAUTHORS:THOprl68 |
| Alternative URL: | http://dx.doi.org/10.1103/PhysRevLett.21.320 |
| 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: | 26 Dec 2012 08:58 |
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