QND measurements for future gravitational-wave detectors
arXiv:0910.0319 · doi:10.1007/s10714-010-1060-y
Abstract
Second-generation interferometric gravitational-wave detectors will be operating at the Standard Quantum Limit, a sensitivity limitation set by the trade off between measurement accuracy and quantum back action, which is governed by the Heisenberg Uncertainty Principle. We review several schemes that allows the quantum noise of interferometers to surpass the Standard Quantum Limit significantly over a broad frequency band. Such schemes may be an important component of the design of third-generation detectors.
22 pages, 6 figures, 1 table; In version 2, more tutorial information on quantum noise in GW interferometer and several new items into Reference list were added
References in corpus (5)
- Triple Michelson Interferometer for a Third-Generation Gravitational Wave Detector
- Beating quantum limits in optomechanical sensor by cavity detuning
- Local readout enhancement for detuned signal-recycling interferometers
- Quantum variational measurement in the next generation gravitational-wave detectors
- Geometry-Driven Shift in the Tomonaga-Luttinger Exponent of Deformed Cylinders
Cited by in corpus (25)
- Gravitational Radiation Detection with Laser Interferometry
- Quantum Measurement Theory in Gravitational-Wave Detectors
- Force sensing based on coherent quantum noise cancellation in a hybrid optomechanical cavity with squeezed-vacuum injection
- Realistic Filter Cavities for Advanced Gravitational Wave Detectors
- Advanced quantum techniques for future gravitational-wave detectors
- Quantum back-action in measurements of zero-point mechanical oscillations
- Coherent Cancellation of Backaction Noise in optomechanical Force Measurements
- Quantum correlations of light due to a room temperature mechanical oscillator for force metrology
- Trajectories without quantum uncertainties
- Quantum Limits of Interferometer Topologies for Gravitational Radiation Detection
- Ultra-precision quantum sensing and measurement based on nonlinear hybrid optomechanical systems containing ultracold atoms or atomic Bose-Einstein condensate
- Negative optical inertia for enhancing the sensitivity of future gravitational-wave detectors
- Quantum noise of non-ideal Sagnac speed meter interferometer with asymmetries
- Laser interferometry with translucent and absorbing mechanical oscillators
- Realistic polarizing Sagnac topology with DC readout for the Einstein Telescope
- A Broadband Signal Recycling Scheme for Approaching the Quantum Limit from Optical Losses
- A two-carrier scheme: evading the 3dB quantum penalty of heterodyne readout in gravitational-wave detectors
- Effects of static and dynamic higher-order optical modes in balanced homodyne readout for future gravitational waves detectors
- All-optical coherent quantum-noise cancellation in cascaded optomechanical systems
- Quantum noise cancellation in asymmetric speed meters with balanced homodyne readout
- Study of acceleration measurement in gravitational wave detection
- Trade-off between quantum and thermal fluctuations in mirror coatings yields improved sensitivity of gravitational-wave interferometers
- Quantum noise in the mirror-field system: A field theoretic approach
- Pass-through Mach-Zehnder topologies for macroscopic quantum measurements
- Quantum Non-demolition Measurements in the Relativistic Dirac Oscillator