de.mpg.escidoc.pubman.appbase.FacesBean
Deutsch
 
Hilfe Wegweiser Datenschutzhinweis Impressum Kontakt
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT
  Gravitational wave detection by laser interferometry - on earth and in space

Rüdiger, A., Brillet, A., Danzmann, K., Giazotto, A., & Hough, J. (2001). Gravitational wave detection by laser interferometry - on earth and in space. Comptes Rendus de l'Académie des Sciences Serie IV Physique Astrophysique, 2(9), 1331-1341.

Item is

Basisdaten

einblenden: ausblenden:
Datensatz-Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-56B6-4 Versions-Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-56B7-2
Genre: Zeitschriftenartikel

Dateien

einblenden: Dateien
ausblenden: Dateien
:
3541.pdf (Verlagsversion), 294KB
Beschreibung:
-
Sichtbarkeit:
Öffentlich
MIME-Typ / Prüfsumme:
application/pdf / [MD5]
Technische Metadaten:
Copyright Datum:
-
Copyright Info:
eDoc_access: PUBLIC
Lizenz:
-

Externe Referenzen

einblenden:

Urheber

einblenden:
ausblenden:
 Urheber:
Rüdiger, Albrecht1, Autor              
Brillet, Alain, Autor
Danzmann, Karsten1, Autor              
Giazotto, Adalberto, Autor
Hough, Jim, Autor
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, escidoc:24010              

Inhalt

einblenden:
ausblenden:
Schlagwörter: -
 Zusammenfassung: The space project LISA is approved by ESA as a cornerstone mission in the field of 'fundamental physics', sharing its goal and principle of operation with the groundbased interferometers currently under construction the detection and measurement of gravitational waves by laser interferometry Ground and space detection differ in their frequency ranges, and thus the detectable sources. At low frequencies, ground-based detection is limited by seismic noise, and yet more fundamentally by 'gravity gradient noise', thus covering the range from a few, Hz to a few kHz. On five sites worldwide, detectors of armlengths from 0.3 to 4 km are being built, two of them in Europe (GEO and VIRGO). They will progressively be put in operation between 2001 and 2003. Future improved versions are being planned, with data not until 2008, Le. near the launch of the space project LISA. It is only in space that detection of signals below, say, I Hz is possible, opening a wide window to a different class of interesting sources of gravitational waves. The project LISA consists of three spacecraft in heliocentric orbits, forming a triangle of 5 million km sides

Details

einblenden:
ausblenden:
Sprache(n): eng - Englisch
 Datum: 2001
 Publikationsstatus: Im Druck publiziert
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: -
 Identifikatoren: eDoc: 3541
 Art des Abschluß: -

Veranstaltung

einblenden:

Entscheidung

einblenden:

Projektinformation

einblenden:

Quelle 1

einblenden:
ausblenden:
Titel: Comptes Rendus de l'Académie des Sciences Serie IV Physique Astrophysique
Genre der Quelle: Zeitschrift
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: -
Seiten: - Band / Heft: 2 (9) Artikelnummer: - Start- / Endseite: 1331 - 1341 Identifikator: -