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  Gravitational waves

Schutz, B. F. (1994). Gravitational waves. Nuclear Physics B - Proceedings Supplements, 35, 44-53. doi:10.1016/0920-5632(94)90217-8.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-7446-0 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-7449-A
Genre: Journal Article

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Schutz, Bernard F.1, 2, Author              
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, escidoc:24013              
2External Organizations, Department of Physics and Astronomy, University of Wales College of Cardiff, P.O. Box 913, Cardiff CF2 3YB, United Kingdom, escidoc:persistent22              

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 Abstract: In the last few years there have been a number of significant developments in research towards the detection of gravitational radiation from astronomical objects. The construction of 3 large-scale (3- or 4-km) interferometric detectors has been funded; new high-sensitivity bars are under construction; there is a serious proposal using two interferometers has been used to put the data from the first coincidence observation using two interferometers has been used to put upper limits on gravitational wave bursts; and new theoretical studies of the relativistic two-body problem have shown that observations of the coalescences of two neutron stars or black holes from binary orbits can provide detailed information about the stars' masses and spins –– but only if we can solve the two-body problem better than we have done so far. These developments are reviewed here.

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 Dates: 2002-09-191994
 Publication Status: Published in print
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 Rev. Method: Peer
 Identifiers: DOI: 10.1016/0920-5632(94)90217-8
eDoc: 60217
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Title: Nuclear Physics B - Proceedings Supplements
Source Genre: Journal
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Pages: - Volume / Issue: 35 Sequence Number: - Start / End Page: 44 - 53 Identifier: ISSN: 0920-5632