dc.contributor.author |
Armstrong, J. |
en_US |
dc.contributor.author |
Estabrook, F. |
en_US |
dc.contributor.author |
Tinto, M. |
en_US |
dc.date.accessioned |
2004-09-23T23:32:39Z |
|
dc.date.available |
2004-09-23T23:32:39Z |
|
dc.date.issued |
1999-03 |
en_US |
dc.identifier.citation |
Astrophysical Journal |
en_US |
dc.identifier.citation |
USA |
en_US |
dc.identifier.clearanceno |
99-0595 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2014/17169 |
|
dc.description.abstract |
Ground-based, equal-arm-length laser interferometers are being built to measure high-frequency astrophysical graviatational waves. Because of the arm-length equality, laser light experiences the same delay in each arm and thus phase or frequency noise from the laser itself precisely cancels at the photodetector. |
en_US |
dc.format.extent |
1202272 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en_US |
|
dc.subject.other |
gravitational wave searches time-delay interferometry laser |
en_US |
dc.title |
Time-Delay Interferometry for Space-based Gravitational Wave Searches |
en_US |