Demonstration of length control for a filter cavity with coherent control sidebands
- Creators
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Aritomi, Naoki
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Zhao, Yuhang
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Capocasa, Eleonora
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Leonardi, Matteo
- Eisenmann, Marc
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Page, Michael
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Guo, Yuefan
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Polini, Eleonora
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Tomura, Akihiro
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Arai, Koji
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Aso, Yoichi
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van Beuzekom, Martin
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Huang, Yao-Chin
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Lee, Ray-Kuang
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Lück, Harald
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Miyakawa, Osamu
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Prat, Pierre
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Shoda, Ayaka
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Tacca, Matteo
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Takahashi, Ryutaro
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Vahlbruch, Henning
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Vardaro, Marco
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Wu, Chien-Ming
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Barsuglia, Matteo
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Flaminio, Raffaele
Abstract
For broadband quantum noise reduction of gravitational-wave detectors, a frequency-dependent squeezed vacuum field realized using a filter cavity is the most promising technique and will be implemented in Advanced LIGO and Advanced Virgo in the fourth observing run. To obtain the benefit of frequency-dependent squeezing, the length and alignment of the filter cavity with respect to the squeezed vacuum field must be accurately controlled. To this purpose, a new length and alignment control scheme for a filter cavity, using coherent control sidebands, was suggested [Phys. Rev. D 102, 042003 (2020)]. The coherent control sidebands are already used to control the squeezing angle in squeezed vacuum sources for gravitational-wave detectors. As both the squeezed vacuum field and coherent control sidebands have the same mode-matching conditions and almost the same frequency, the length and alignment of the filter cavity with respect to the squeezed vacuum field can be accurately controlled with this scheme. In this paper, we experimentally demonstrate the new control scheme for a filter cavity with coherent control sidebands. In addition to the conventional filter cavity control with the green field, we succeed in controlling the length of a 300-m filter cavity with coherent control sidebands and reduce the filter cavity length noise (rms) from 6.8 to 2.1 pm.
Additional Information
© 2022 American Physical Society. We thank the Advanced Technology Center (ATC) of NAOJ for its support. This work was supported by the JSPS Grant-in-Aid for Scientific Research (Grants Nos. 15H02095, 18H01235, and 21H04476), the LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), and the EU Horizon 2020 Research and Innovation Program under the Marie Sklodowska-Curie Grant Agreement No. 734303 (NEWS) and 101003460 and GA 101003460 (PROBES). N. A. was supported by the JSPS Grant-in-Aid for Scientific Research (Grant No. 18H01224), the JSPS Grant-in-Aid for Challenging Research (Exploratory) (Grant No. 18K18763), and the JST CREST (Grant No. JPMJCR1873). E. C., M. E., and M. P. were supported by the JSPS Grant-in-Aid for JSPS Fellows (Grants Nos. 18F18024, 20F20803, and 20F20713), respectively. H. L. and H. V. were supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany's Excellence Strategy—EXC 2123 QuantumFrontiers—390837967.Attached Files
Published - PhysRevD.106.102003.pdf
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Additional details
- Eprint ID
- 122204
- Resolver ID
- CaltechAUTHORS:20230710-599244800.17
- Japan Society for the Promotion of Science (JSPS)
- 15H02095
- Japan Society for the Promotion of Science (JSPS)
- 18H01235
- Japan Society for the Promotion of Science (JSPS)
- 21H04476
- Agence Nationale pour la Recherche (ANR)
- ANR-10-LABX-0023
- Agence Nationale pour la Recherche (ANR)
- ANR-18-IDEX-0001
- Marie Curie Fellowship
- 734303
- Marie Curie Fellowship
- 101003460
- Japan Society for the Promotion of Science (JSPS)
- 18H01224
- Japan Society for the Promotion of Science (JSPS)
- 18K18763
- Japan Society for the Promotion of Science (JSPS)
- JPMJCR1873
- Japan Society for the Promotion of Science (JSPS)
- 18F18024
- Japan Society for the Promotion of Science (JSPS)
- 20F20803
- Japan Society for the Promotion of Science (JSPS)
- 20F20713
- Deutsche Forschungsgemeinschaft (DFG)
- EXC 2123 - 390837967
- Created
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2023-08-11Created from EPrint's datestamp field
- Updated
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2023-08-14Created from EPrint's last_modified field
- Caltech groups
- LIGO