Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/8627
Title: Gravitational Wave Detection by Interferometry (Ground and Space)
Keywords: Gravitational Waves
Issue Date: 1-Jun-2013
Publisher: Max-Planck Institute for Gravitational Physics
Description: Significant progress has been made in recent years on the development of gravitational wave detectors. Sources such as coalescing compact binary systems, low-mass X-ray binaries, stellar collapses and pulsars are all possible candidates for detection. The most promising design of gravitational wave detector uses test masses a long distance apart and freely suspended as pendulums on Earth or in drag-free craft in space. The main theme of this review is a discussion of the mechanical and optical principles used in the various long baseline systems being built around the world -- LIGO (USA), VIRGO (Italy/France), TAMA 300 (Japan) and GEO 600 (Germany/UK) -- and in LISA, a proposed space-borne interferometer.
URI: http://koha.mediu.edu.my:8181/jspui/handle/123456789/8627
Other Identifiers: http://www.livingreviews.org/lrr-2000-3
http://www.doaj.org/doaj?func=openurl&genre=article&issn=14338351&date=2000&volume=3&issue=&spage=3
Appears in Collections:Physics and Astronomy

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