Published September 17, 1979
| public
Journal Article
Gravitational Wave Detectors
Chicago
Abstract
As outlined in the preceding talk by Dr Thorne, there are many possible sources of gravitational radiation, ranging from the interactions of supermassive black holes to supernova explosions of stars. Detection of such radiation could give information which cannot be obtained otherwise, for example on events occurring in the cores of stellar systems, and could also provide important clues on the existence, nature and behaviour of black holes.
Additional Information
© 1979 Royal Society.Additional details
- Eprint ID
- 63223
- DOI
- 10.1098/rspa.1979.0108
- Resolver ID
- CaltechAUTHORS:20151224-093959427
- Created
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2015-12-24Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field