Published September 1972 | Version public
Journal Article

Gravitational-Wave Astronomy

Abstract

The "windows" of observational astronomy have become broader. They now include, along with photons from many decades of the electromagnetic spectrum, extraterrestrial "artifacts" of other sorts: cosmic rays, meteorites, particles from the solar wind, samples of the lunar surface, and neutrinos. With gravitational-wave astronomy, we are on the threshold-or just beyond the threshold-of adding another window; it is a particularly important window because it will allow us to observe phenomena that cannot be studied adequately by other means: gravitational collapse, the interiors of supernovae, black holes, short-period binaries, and perhaps new details of pulsar structure. There is the further possibility that gravitational-wave astronomy will reveal entirely new phenomena-or familiar phenomena in unfamiliar guise-in trying to explain the observations of Joseph Weber.

Additional Information

© 1972 Annual Reviews. For valuable discussions we thank many colleagues, particularly V. B. Braginskii and G. J. Dick. For assistance with the literature search we thank M. Ko and L. Will. The survey of literature for this review was concluded in December 1971. Supported in part by the National Science Foundation (GP-28027, GP-27304) and the National Aeronautics and Space Administration Caltech/JPL contract NAS 7-100 (188-41-54-02-01), and grant NGR 05-002-256. Fannie and John Hertz Foundation Fellow.

Additional details

Identifiers

Eprint ID
71256
Resolver ID
CaltechAUTHORS:20161019-084347968

Funding

NSF
GP-28027
NSF
GP-27304
NASA
NAS 7-100
NASA
188-41-54-02-01
NASA
NGR 05-002-256
Fannie and John Hertz Foundation

Dates

Created
2016-10-19
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Updated
2021-11-11
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