We present an overview of quantum noise in gravitational wave interferometers. Current gravi-tational wave detectors are modified variants of a Michelson interferometer and the quantum noise limits are strongly influenced by the optical configuration of the interferometer. We describe recent developments in the treatment of quantum noise in the complex interferometers of present-day and future gravitational-wave detectors and explore prospects for beating the standard quantum limit by use of both injected and ponderomotive squeezing in future interferometers. PACS numbers: 04.80.Nn, 95.55.Ym, 42.50.Dv,03.65.Bz, 03.65.Ta I
Quantum noise limits the sensitivity of interferometric measurements. It is generally admitted that ...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
International audienceThe current generation of gravitational wave laser interferometer detectors op...
We present an overview of quantum noise in gravitational wave interferometers. Gravitational wave de...
The fast progress in improving the sensitivity of the gravitational-wave detectors, we all have witn...
Interferometric gravitational wave detectors (such as advanced LIGO) employ high-power solid-state l...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
It has long been thought that the sensitivity of laser interferometric gravitational-wave detectors ...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
Quantum noise limits the sensitivity of interferometric measurements. It is generally admitted that ...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
International audienceThe current generation of gravitational wave laser interferometer detectors op...
We present an overview of quantum noise in gravitational wave interferometers. Gravitational wave de...
The fast progress in improving the sensitivity of the gravitational-wave detectors, we all have witn...
Interferometric gravitational wave detectors (such as advanced LIGO) employ high-power solid-state l...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
It has long been thought that the sensitivity of laser interferometric gravitational-wave detectors ...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
Quantum noise limits the sensitivity of interferometric measurements. It is generally admitted that ...
Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitiv...
International audienceThe current generation of gravitational wave laser interferometer detectors op...