The advanced LIGO input optics
The advanced LIGO gravitational wave detectors are nearing their design sensitivity and should begin taking meaningful astrophysical data in the fall of 2015. These resonant optical interferometers will have unprecedented sensitivity to the strains caused by passing gravitational waves. The input op...
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| Veröffentlicht in: | Review of scientific instruments 2016-01, Vol.87 (1), p.014502-014502 |
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| creator | Mueller, Chris L. Arain, Muzammil A. Ciani, Giacomo DeRosa, Ryan. T. Effler, Anamaria Feldbaum, David Frolov, Valery V. Fulda, Paul Gleason, Joseph Heintze, Matthew Kawabe, Keita King, Eleanor J. Kokeyama, Keiko Korth, William Z. Martin, Rodica M. Mullavey, Adam Peold, Jan Quetschke, Volker Reitze, David H. Tanner, David B. Vorvick, Cheryl Williams, Luke F. Mueller, Guido |
| description | The advanced LIGO gravitational wave detectors are nearing their design sensitivity and should begin taking meaningful astrophysical data in the fall of 2015. These resonant optical interferometers will have unprecedented sensitivity to the strains caused by passing gravitational waves. The input optics play a significant part in allowing these devices to reach such sensitivities. Residing between the pre-stabilized laser and the main interferometer, the input optics subsystem is tasked with preparing the laser beam for interferometry at the sub-attometer level while operating at continuous wave input power levels ranging from 100 mW to 150 W. These extreme operating conditions required every major component to be custom designed. These designs draw heavily on the experience and understanding gained during the operation of Initial LIGO and Enhanced LIGO. In this article, we report on how the components of the input optics were designed to meet their stringent requirements and present measurements showing how well they have lived up to their design. |
| doi_str_mv | 10.1063/1.4936974 |
| format | Article |
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These resonant optical interferometers will have unprecedented sensitivity to the strains caused by passing gravitational waves. The input optics play a significant part in allowing these devices to reach such sensitivities. Residing between the pre-stabilized laser and the main interferometer, the input optics subsystem is tasked with preparing the laser beam for interferometry at the sub-attometer level while operating at continuous wave input power levels ranging from 100 mW to 150 W. These extreme operating conditions required every major component to be custom designed. These designs draw heavily on the experience and understanding gained during the operation of Initial LIGO and Enhanced LIGO. 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| ispartof | Review of scientific instruments, 2016-01, Vol.87 (1), p.014502-014502 |
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| source | AIP Journals Complete; Alma/SFX Local Collection |
| subjects | ASTROPHYSICS BEAMS Continuous radiation Customization DESIGN Extreme environments Gravitation GRAVITATIONAL WAVE DETECTORS GRAVITATIONAL WAVES INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY INTERFEROMETERS INTERFEROMETRY Laser beams LASERS OPTICS PETROLEUM RESIDUES Scientific apparatus & instruments SENSITIVITY |
| title | The advanced LIGO input optics |
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