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Some next-generation gravitational-wave detectors, such as the AmericanAdvanced LIGO project and the Japanese LCGT project, plan to use power recycledresonant sideband extraction (RSE) interferometers for their interferometer'soptical configuration. A power recycled zero-detuning (PRZD) RSEinterferometer, which is the default design for LCGT, has five main lengthdegrees of freedom that need to be controlled in order to operate agravitational-wave detector. This task is expected to be very challengingbecause of the complexity of optical configuration. A new control scheme for aPRZD RSE interferometer has been developed and tested with a prototypeinterferometer. The PRZD RSE interferometer was successfully locked with thecontrol scheme. It is the first experimental demonstration of a PRZD RSEinterferometer with suspended test masses. The result serves as an importantstep for the operation of LCGT.

classical and quantum gravity

Experimental investigation of a control scheme for a zero-detuning  resonant sideband extraction interferometer for next-generation  gravitational-wave detectors