Generation of squeezed vacuum state in the millihertz frequency band
arXiv:2408.10607 · doi:10.1038/s41377-024-01606-y
Abstract
The detection of gravitational waves has ushered in a new era of observing the universe. Quantum resource advantages offer significant enhancements to the sensitivity of gravitational wave observatories. While squeezed states for ground-based gravitational wave detection have received marked attention, the generation of squeezed states suitable for mid-to-low-frequency detection has remained unexplored. To address the gap in squeezed state optical fields at ultra-low frequencies, we report on the first direct observation of a squeezed vacuum field until Fourier frequency of 4 millihertz with the quantum noise reduction of up to 8 dB, by the employment of a multiple noise suppression scheme. Our work provides quantum resources for future gravitational wave observatories, facilitating the development of quantum precision measurement.
arXiv comment17 pages,4 figures,1 table and 50 Refs. To be published in Light: Science & Applications
References in corpus (30)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Advanced LIGO
- Laser Interferometer Space Antenna
- Enhancing the sensitivity of the LIGO gravitational wave detector by using squeezed states of light
- Detection of 15 dB Squeezed States of Light and their Application for the Absolute Calibration of Photoelectric Quantum Efficiency
- Observation of squeezed light with 10dB quantum noise reduction
- First Long-Term Application of Squeezed States of Light in a Gravitational-Wave Observatory
- Quantum Enhancement of the Zero-Area Sagnac Interferometer Topology for Gravitational Wave Detection
- Observation of -9 dB quadrature squeezing with improvement of phase stability in homodyne measurement
- Coherent control of vacuum squeezing in the Gravitational-Wave Detection Band
- Squeezing in the audio gravitational wave detection band
- Science with the TianQin observatory: Preliminary results on massive black hole binaries
- Quantum engineering of squeezed states for quantum communication and metrology
- GEO 600 and the GEO-HF upgrade program: successes and challenges
- Balanced Homodyne Detection of Optical Quantum States at Audio-Band Frequencies and Below
- First demonstration of 6 dB quantum noise reduction in a kilometer scale gravitational wave observatory
- Frequency-Dependent Squeezed Vacuum Source for Broadband Quantum Noise Reduction in Advanced Gravitational-Wave Detectors
- Low-Frequency Terrestrial Gravitational-Wave Detectors
- Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO
- Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO
- 13dB Squeezed Vacuum States at 1550nm from 12mW external pump power at 775nm
- Quantum enhanced non-interferometric quantitative phase imaging
- Long-term stable squeezed vacuum state of light for gravitational wave detectors
- A new type of quantum speed meter interferometer: measuring speed to search for intermediate mass black holes
- Quantum expander for gravitational-wave observatories
- Estimation of losses in a 300 m filter cavity and quantum noise reduction in the KAGRA gravitational-wave detector
- The first five years of gravitational-wave astrophysics
- Harmonics-assisted optical phase amplifier
- Twin-beam intensity-difference squeezing below 10 Hz
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- Quantum-enhanced laser phase noise filter
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- On-chip squeezed light in the audio frequency band