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Gravitational radiation damping

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
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/PhysRevLett.21.320DOIUNSPECIFIED
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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