Quantum-noise reduction schemes for future advanced gravitational-wave detectors
- Document #:
- LIGO-T1300633-v1
- Document type:
- T - Technical notes
Other Versions:
- Abstract:
- Future advanced gravitational-wave detectors, such as Advanced LIGO, Advanced VIRGO, and KAGRA will be limited by noise due to quantum fluctuations in the light, around the most sensitive detection band ~ 100Hz. There are two different approaches for improving the sensitivity: squeezing or canceling the noise by properly designing the input or output optics of the detector, and increasing the response to the gravitational-wave signal by modifying the test mass dynamics. In this project we take advantage of frequency-dependence of the optical spring to effectively reduce inertia of the test mass with multiple optical springs.
- Files in Document:
- Other Files:
- Final report (final_report.pdf, file is not accessible)
- Progress report 1 (pr_1.pdf, file is not accessible)
- Progress report 2 (pr_2.pdf, file is not accessible)
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