Resonant sideband extraction is a new optical configuration for laser-interferometric gravitational wave detectors with Fabry-Perot cavities in the arms. It reduces the thermal load on the beam splitter and the coupling mirrors of the cavities and also allows one to adapt the frequency response of the detector to a variety of requirements. We report the first experimental demonstration using a table-top setup at a detuned operating point. An increase of sensitivity by 6 dB was observed for artificial signals at frequencies above the arm cavity bandwidth, and the overall transfer function agreed well with theoretical predictions
Thermal lensing limits the performance of advanced interferometric gravitational wave detectors that...
Large-scale gravitational-wave detectors currently under construction such as the LIGO detectors use...
We report on our prototype experiment that uses a 4-m detuned resonant sideband extraction interfero...
Resonant sideband extraction is a new optical configuration for laser-interferometric gravitational ...
We present an experimental demonstration of a locking and control scheme for an interferometer using...
As a future plan, an advanced gravitational-wave detector will employ an optical configuration of re...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
We introduce a new Fabry-Perot based interferometric gravitational wave detector that, compared with...
We present a new optical control scheme for a laser interferometric gravitational wave detector that...
Next generation gravitational wave antennas employ resonant sideband extraction (RSE) interferometer...
In anticipation of an upgrade of the LIGO detector to an advanced configuration in 2004, a tabletop ...
The 4m Resonant Sideband Extraction (RSE) interferometer is a planned prototype of the LCGT interfer...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
Diffraction gratings have been proposed as core elements in future laser-interferometric gravitation...
The 4m Resonant Sideband Extraction (RSE) interferometer is a planned prototype of the LCGT interfer...
Thermal lensing limits the performance of advanced interferometric gravitational wave detectors that...
Large-scale gravitational-wave detectors currently under construction such as the LIGO detectors use...
We report on our prototype experiment that uses a 4-m detuned resonant sideband extraction interfero...
Resonant sideband extraction is a new optical configuration for laser-interferometric gravitational ...
We present an experimental demonstration of a locking and control scheme for an interferometer using...
As a future plan, an advanced gravitational-wave detector will employ an optical configuration of re...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
We introduce a new Fabry-Perot based interferometric gravitational wave detector that, compared with...
We present a new optical control scheme for a laser interferometric gravitational wave detector that...
Next generation gravitational wave antennas employ resonant sideband extraction (RSE) interferometer...
In anticipation of an upgrade of the LIGO detector to an advanced configuration in 2004, a tabletop ...
The 4m Resonant Sideband Extraction (RSE) interferometer is a planned prototype of the LCGT interfer...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
Diffraction gratings have been proposed as core elements in future laser-interferometric gravitation...
The 4m Resonant Sideband Extraction (RSE) interferometer is a planned prototype of the LCGT interfer...
Thermal lensing limits the performance of advanced interferometric gravitational wave detectors that...
Large-scale gravitational-wave detectors currently under construction such as the LIGO detectors use...
We report on our prototype experiment that uses a 4-m detuned resonant sideband extraction interfero...