In anticipation of an upgrade of the LIGO detector to an advanced configuration in 2004, a tabletop prototype of resonant sideband extraction is being designed and constructed at Caltech. We present here two frontally modulated length sensing and control schemes, one in which the signal extraction/recycling mirror is a simple mirror, and one in which it is a Fabry-Perot cavity. Issues regarding the controllability, RF sideband transmission, shot noise, and noise couplings are discussed
Large-scale gravitational-wave detectors currently under construction such as the LIGO detectors use...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
The lock acquisition scheme for the Advanced LIGO optical configuration, which makes use of "resonan...
As a future plan, an advanced gravitational-wave detector will employ an optical configuration of re...
Next generation gravitational wave antennas employ resonant sideband extraction (RSE) interferometer...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
Resonant sideband extraction is a new optical configuration for laser-interferometric gravitational ...
The 4m Resonant Sideband Extraction (RSE) interferometer is a planned prototype of the LCGT interfer...
For a broadband-operated RSE interferometer, a simple and smart length sensing and control scheme wa...
The 4m Resonant Sideband Extraction (RSE) interferometer is a planned prototype of the LCGT interfer...
LCGT plans to use tuned RSE as the optical configuration for its interferometer. A tuned RSE interfe...
We present a new optical control scheme for a laser interferometric gravitational wave detector that...
We introduce a concept that uses detuned arm cavities to increase the shot-noise-limited sensitivity...
We present an experimental demonstration of a locking and control scheme for an interferometer using...
Some next-generation gravitational-wave detectors, such as the American Advanced LIGO project and th...
Large-scale gravitational-wave detectors currently under construction such as the LIGO detectors use...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
The lock acquisition scheme for the Advanced LIGO optical configuration, which makes use of "resonan...
As a future plan, an advanced gravitational-wave detector will employ an optical configuration of re...
Next generation gravitational wave antennas employ resonant sideband extraction (RSE) interferometer...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
Resonant sideband extraction is a new optical configuration for laser-interferometric gravitational ...
The 4m Resonant Sideband Extraction (RSE) interferometer is a planned prototype of the LCGT interfer...
For a broadband-operated RSE interferometer, a simple and smart length sensing and control scheme wa...
The 4m Resonant Sideband Extraction (RSE) interferometer is a planned prototype of the LCGT interfer...
LCGT plans to use tuned RSE as the optical configuration for its interferometer. A tuned RSE interfe...
We present a new optical control scheme for a laser interferometric gravitational wave detector that...
We introduce a concept that uses detuned arm cavities to increase the shot-noise-limited sensitivity...
We present an experimental demonstration of a locking and control scheme for an interferometer using...
Some next-generation gravitational-wave detectors, such as the American Advanced LIGO project and th...
Large-scale gravitational-wave detectors currently under construction such as the LIGO detectors use...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
The lock acquisition scheme for the Advanced LIGO optical configuration, which makes use of "resonan...