A Broadband Signal Recycling Scheme for Approaching the Quantum Limit from Optical Losses
arXiv:2011.04793 · doi:10.3390/galaxies9010003
Abstract
Quantum noise limits the sensitivity of laser interferometric gravitational-wave detectors. Given the state-of-the-art optics, the optical losses define the lower bound of the best possible quantum-limited detector sensitivity. In this work, we come up with a broadband signal recycling scheme which gives potential solution to approaching this lower bound by converting the signal recycling cavity to be a broadband signal amplifier using an active optomechanical filter. We will show the difference and advantage of such a scheme compared with the previous white light cavity scheme using the optomechanical filter in [Phys.Rev.Lett.115.211104 (2015)]. The drawback is that the new scheme is more susceptible to the thermal noise of the mechanical oscillator.
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Cited by in corpus (6)
- Gravitational-Wave Detector for Postmerger Neutron Stars: Beyond the Quantum Loss Limit of the Fabry-Perot-Michelson Interferometer
- Towards observing the neutron star collapse with gravitational wave detectors
- Nondegenerate internal squeezing: an all-optical, loss-resistant quantum technique for gravitational-wave detection
- Enhancing the sensitivity of interferometers with stable phase-insensitive quantum filters
- Enhancing high frequency sensitivity of gravitational wave detectors with sloshing-Sagnac interferometer
- Design of a tabletop interferometer with quantum amplification