Deutsch
 
Hilfe Datenschutzhinweis Impressum
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT
  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.

Item is

Dateien

einblenden: Dateien
ausblenden: Dateien
:
schutz_61248.pdf (Verlagsversion), 2MB
Name:
schutz_61248.pdf
Beschreibung:
-
OA-Status:
Sichtbarkeit:
Öffentlich
MIME-Typ / Prüfsumme:
application/pdf
Technische Metadaten:
Copyright Datum:
-
Copyright Info:
-
Lizenz:
-

Externe Referenzen

einblenden:

Urheber

einblenden:
ausblenden:
 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, ou_24013              
2External Organizations, Department of Applied Mathematics and Astronomy, University College, Cardiff, Wales, U.K., ou_persistent22              
3External Organizations, Department of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, Scotland, ou_persistent22              
4External Organizations, Rutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 0QX, U.K., ou_persistent22              
5External Organizations, California Institute of Technology, Pasadena, California, U.S.A, ou_persistent22              

Inhalt

einblenden:
ausblenden:
Schlagwörter: -
 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.

Details

einblenden:
ausblenden:
Sprache(n):
 Datum: 1987
 Publikationsstatus: Erschienen
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: Expertenbegutachtung
 Identifikatoren: DOI: 10.1016/0083-6656(87)90012-2
eDoc: 61248
 Art des Abschluß: -

Veranstaltung

einblenden:

Entscheidung

einblenden:

Projektinformation

einblenden:

Quelle 1

einblenden:
ausblenden:
Titel: Vistas in Astronomy
Genre der Quelle: Zeitschrift
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: -
Seiten: - Band / Heft: 30 (2) Artikelnummer: - Start- / Endseite: 109 - 134 Identifikator: ISSN: 0083-6656