Quantum-Enhanced Advanced LIGO Detectors in the Era of Gravitational-Wave Astronomy
Massachusetts Institute of Technology · Australian National University · +35 more institutions
Abstract
The Laser Interferometer Gravitational Wave Observatory (LIGO) has been directly detecting gravitational waves from compact binary mergers since 2015. We report on the first use of squeezed vacuum states in the direct measurement of gravitational waves with the Advanced LIGO H1 and L1 detectors. This achievement is the culmination of decades of research to implement squeezed states in gravitational-wave detectors. During the ongoing O3 observation run, squeezed states are improving the sensitivity of the LIGO interferometers to signals above 50 Hz by up to 3 dB, thereby increasing the expected detection rate by 40% (H1) and 50% (L1).
Citation impact
- FWCI
- 47.62
- Percentile
- 100%
- References
- 44
Authors
201- MTM. TseCorresponding
Massachusetts Institute of Technology
- HYHaocun Yu
Massachusetts Institute of Technology
- NKN. Kijbunchoo
Australian National University, ARC Centre of Excellence for Gravitational Wave Discovery
- AFA. Fernandez-Galiana
Massachusetts Institute of Technology
- PDP. Dupej
University of Glasgow
Topics & keywords
- LIGO
- Gravitational wave
- Physics
- Gravitational-wave astronomy
- Interferometry
- Gravitational-wave observatory
- Astronomical interferometer
- Observatory
Funding
- NSNational Science FoundationAwards: 0757058, 0823459, PHY-0757058, 1122374, PHY-0823459, CE170100004
- MIMassachusetts Institute of TechnologyAwards: PHY-0757058, 1122374
- CICalifornia Institute of Technology
- SAScience and Technology Facilities CouncilAwards: ST/S00243X/1, ST/S000305/1, ST/S000550/1, ST/S002464/1, 2142081, ST/N00003X/1, 1802894, ST/N000072/1
- ARAustralian Research CouncilAwards: LE170100217, No. CE170100004, CE170100004, 1122374