Published July 29, 1968
| public
Journal Article
Open
Gravitational radiation damping
- Creators
- Thorne, Kip S.
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).
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.Files
THOprl68.pdf
Files
(718.2 kB)
| Name | Size | Download all |
|---|---|---|
|
md5:e412e28e3e31a8939014092017b4f3c2
|
718.2 kB | Preview Download |
Additional details
- Eprint ID
- 4222
- Resolver ID
- CaltechAUTHORS:THOprl68
- Created
-
2006-08-08Created from EPrint's datestamp field
- Updated
-
2021-11-08Created from EPrint's last_modified field
- Caltech groups
- TAPIR