أعرض تسجيلة المادة بشكل مبسط
| dc.creator |
Rowan Sheila |
|
| dc.creator |
Hough Jim |
|
| dc.date |
2000 |
|
| dc.date.accessioned |
2013-06-01T11:41:50Z |
|
| dc.date.available |
2013-06-01T11:41:50Z |
|
| dc.date.issued |
2013-06-01 |
|
| dc.identifier |
http://www.livingreviews.org/lrr-2000-3 |
|
| dc.identifier |
http://www.doaj.org/doaj?func=openurl&genre=article&issn=14338351&date=2000&volume=3&issue=&spage=3 |
|
| dc.identifier.uri |
http://koha.mediu.edu.my:8181/jspui/handle/123456789/8627 |
|
| dc.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. |
|
| dc.publisher |
Max-Planck Institute for Gravitational Physics |
|
| dc.source |
Living Reviews in Relativity |
|
| dc.subject |
Gravitational Waves |
|
| dc.title |
Gravitational Wave Detection by Interferometry (Ground and Space) |
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أعرض تسجيلة المادة بشكل مبسط