Frequency-Dependent Squeezed Vacuum Source for Broadband Quantum Noise Reduction in Advanced Gravitational-Wave Detectors-Reference-Cited by-同舟云学术

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Frequency-Dependent Squeezed Vacuum Source for Broadband Quantum Noise Reduction in Advanced Gravitational-Wave Detectors

Published:2020-04-28 Issue:17 Volume:124 Page:
ISSN:0031-9007
Container-title:Physical Review Letters
language:en
Short-container-title:Phys. Rev. Lett.

Author:

Zhao Yuhang^ORCID,Aritomi Naoki,Capocasa Eleonora^ORCID,Leonardi Matteo,Eisenmann Marc,Guo Yuefan,Polini Eleonora^ORCID,Tomura Akihiro,Arai Koji,Aso Yoichi^ORCID,Huang Yao-Chin,Lee Ray-Kuang^ORCID,Lück Harald^ORCID,Miyakawa Osamu,Prat Pierre,Shoda Ayaka^ORCID,Tacca Matteo,Takahashi Ryutaro^ORCID,Vahlbruch Henning,Vardaro Marco,Wu Chien-Ming^ORCID,Barsuglia Matteo,Flaminio Raffaele

Funder

National Astronomical Observatory of Japan

Japan Society for the Promotion of Science

Horizon 2020 Framework Programme

Japan Science and Technology Agency

Advanced Technology Center

Publisher

American Physical Society (APS)

Subject

General Physics and Astronomy

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.124.171101/fulltext

Reference28 articles.

1. Observation of Gravitational Waves from a Binary Black Hole Merger

2. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

3. GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

4. Advanced LIGO

5. Advanced Virgo: a second-generation interferometric gravitational wave detector

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