Loss in long-storage-time optical cavities
arXiv:1310.1820 · doi:10.1364/OE.21.030114
Abstract
Long-storage-time Fabry-Perot cavities are a core component of many precision measurement experiments. Optical loss in such cavities is a critical parameter in determining their performance; however, it is very difficult to determine a priori from independent characterisation of the individual cavity mirrors. Here, we summarise three techniques for directly measuring this loss in situ and apply them to a high-finesse, near-concentric, 2 m system. Through small modifications of the cavity's length, we explore optical loss as a function of beam spot size over the 1-3 mm range. In this regime we find that optical loss is relatively constant at around 10 ppm per mirror and shows greater dependence on the positions of the beam spots on the cavity optics than on their size. These results have immediate consequences for the application of squeezed light to advanced gravitational-wave interferometers.
References in corpus (2)
Cited by in corpus (30)
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- A Cryogenic Silicon Interferometer for Gravitational-wave Detection
- A Gravitational Wave Detector with Cosmological Reach
- Frequency-Dependent Squeezing for Advanced LIGO
- Prospects for doubling the range of Advanced LIGO
- Proposal for Gravitational-Wave Detection Beyond the Standard Quantum Limit via EPR Entanglement
- Audio-band frequency-dependent squeezing
- Review of the Advanced LIGO gravitational wave observatories leading to observing run four
- Searching for Axion Dark Matter with Birefringent Cavities
- Decoherence and degradation of squeezed states in quantum filter cavities
- Advanced quantum techniques for future gravitational-wave detectors
- Narrowing the filter cavity bandwidth via optomechanical interaction
- Design of a speed meter interferometer proof-of-principle experiment
- Laser Frequency Noise in Next Generation Gravitational-Wave Detectors
- The next detectors for gravitational wave astronomy
- Measurement of optical losses in a high-finesse 300 m filter cavity for broadband quantum noise reduction in gravitational-wave detectors
- Molecular adsorbed layer formation on cooled mirrors and its impacts on cryogenic gravitational wave telescopes
- An arm length stabilization system for KAGRA and future gravitational-wave detectors
- First results from the Axion Dark-Matter Birefringent Cavity (ADBC) experiment
- Implications of the Quantum Noise Target for the Einstein Telescope Infrastructure Design
- A phase-sensitive optomechanical amplifier for quantum noise reduction in laser interferometers
- Characterization of optical systems for the ALPS II experiment
- Direct approach to realising quantum filters for high-precision measurements
- A back-linked Fabry-Perot interferometer for space-borne gravitational wave observations
- Improving the stability of frequency dependent squeezing with bichromatic control of filter cavity length, alignment and incident beam pointing
- Scattering Loss in Precision Metrology due to Mirror Roughness
- Performance of multiple filter-cavity schemes for frequency-dependent squeezing in gravitational-wave detectors
- Any Light Particle Search II - Status Overview
- Design of a tabletop interferometer with quantum amplification
- Application of optomechanical frequency conversion on gravitational wave detection