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  Gravitational Wave Astronomy - Potential and Possible Realisation

Schutz, B. F., Hough, J., Meers, B. J., Newton, G. P., Robertson, N. A., Ward, H., et al. (1987). Gravitational Wave Astronomy - Potential and Possible Realisation. Vistas in Astronomy, 30(2), 109-134. doi:10.1016/0083-6656(87)90012-2.

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Datensatz-Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-7441-9 Versions-Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-7444-3
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 Urheber:
Schutz, Bernard F.1, 2, Autor              
Hough, Jim3, Autor
Meers, B. J.3, Autor
Newton, G. P.3, Autor
Robertson, N. A.3, Autor
Ward, H.3, Autor
Corbett, I. F.4, Autor
Drever, R. W. P.5, Autor
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, escidoc:24013              
2External Organizations, Department of Applied Mathematics and Astronomy, University College, Cardiff, Wales, U.K., escidoc:persistent22              
3External Organizations, Department of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, Scotland, escidoc:persistent22              
4External Organizations, Rutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 0QX, U.K., escidoc:persistent22              
5External Organizations, California Institute of Technology, Pasadena, California, U.S.A, escidoc:persistent22              

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 Zusammenfassung: Since the pioneering work of Joseph Weber more than a decade ago there has been a continuing effort towards the development of more sensitive gravitational wave detectors. There are a number of interesting astrophysical sources of gravitational waves including coalescing compact binary star systems, stellar collapses and rotating neutron stars, and to detect all of these is likely to require a strain sensitivity better than 10-22 over a bandwidth of a few hundred Hz at frequencies at or below 1kHz. To achieve such sensitivity requires considerable experimental ingenuity; however work in a number of laboratories suggests that such performance should be attainable using laser interferometry between freely suspended masses separated by a distance of the order of a kilometre. This paper includes a review of possible sources and outlines methods of detection currently being developed or planned, with particular emphasis on long baseline laser interferometers.

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 Datum: 1987
 Publikationsstatus: Im Druck publiziert
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 Art der Begutachtung: Expertenbegutachtung
 Identifikatoren: DOI: 10.1016/0083-6656(87)90012-2
eDoc: 61248
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Titel: Vistas in Astronomy
Genre der Quelle: Zeitschrift
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Ort, Verlag, Ausgabe: -
Seiten: - Band / Heft: 30 (2) Artikelnummer: - Start- / Endseite: 109 - 134 Identifikator: ISSN: 0083-6656