Advanced quantum techniques for future gravitational-wave detectors
Quantum fluctuation of light limits the sensitivity of advanced laser interferometric gravitational-wave detectors. It is one of the principal obstacles on the way towards the next-generation gravitational-wave observatories. The envisioned significant improvement of the detector sensitivity require...
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| Veröffentlicht in: | Living Reviews in Relativity 2019-04, Vol.22 (1), p.1-89, Article 2 |
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| creator | Danilishin, Stefan L. Khalili, Farid Ya Miao, Haixing |
| description | Quantum fluctuation of light limits the sensitivity of advanced laser interferometric gravitational-wave detectors. It is one of the principal obstacles on the way towards the next-generation gravitational-wave observatories. The envisioned significant improvement of the detector sensitivity requires using quantum non-demolition measurement and back-action evasion techniques, which allow us to circumvent the sensitivity limit imposed by the Heisenberg uncertainty principle. In our previous review article (Danilishin and Khalili in Living Rev Relativ 15:5,
2012
), we laid down the basic principles of quantum measurement theory and provided the framework for analysing the quantum noise of interferometers. The scope of this paper is to review novel techniques for quantum noise suppression proposed in the recent years and put them in the same framework. Our delineation of interferometry schemes and topologies is intended as an aid in the process of selecting the design for the next-generation gravitational-wave observatories. |
| doi_str_mv | 10.1007/s41114-019-0018-y |
| format | Article |
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2012
), we laid down the basic principles of quantum measurement theory and provided the framework for analysing the quantum noise of interferometers. The scope of this paper is to review novel techniques for quantum noise suppression proposed in the recent years and put them in the same framework. Our delineation of interferometry schemes and topologies is intended as an aid in the process of selecting the design for the next-generation gravitational-wave observatories.</description><identifier>ISSN: 2367-3613</identifier><identifier>EISSN: 1433-8351</identifier><identifier>DOI: 10.1007/s41114-019-0018-y</identifier><language>eng</language><publisher>Cham: Springer International Publishing</publisher><subject>Astrophysics and Astroparticles ; Classical and Quantum Gravitation ; Cosmology ; Demolition ; Detection equipment ; Gravitational waves ; Observatories ; Physics ; Physics and Astronomy ; Relativity Theory ; Review Article</subject><ispartof>Living Reviews in Relativity, 2019-04, Vol.22 (1), p.1-89, Article 2</ispartof><rights>The Author(s) 2019</rights><rights>COPYRIGHT 2019 Springer</rights><rights>Living Reviews in Relativity is a copyright of Springer, (2019). All Rights Reserved. © 2019. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c432t-be62f67d6c7c6122294de24cb7f908d5916045095def491e66246c465b5056713</citedby><cites>FETCH-LOGICAL-c432t-be62f67d6c7c6122294de24cb7f908d5916045095def491e66246c465b5056713</cites><orcidid>0000-0001-7758-7493</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s41114-019-0018-y$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://doi.org/10.1007/s41114-019-0018-y$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>314,777,781,861,27905,27906,41101,42170,51557</link.rule.ids></links><search><creatorcontrib>Danilishin, Stefan L.</creatorcontrib><creatorcontrib>Khalili, Farid Ya</creatorcontrib><creatorcontrib>Miao, Haixing</creatorcontrib><title>Advanced quantum techniques for future gravitational-wave detectors</title><title>Living Reviews in Relativity</title><addtitle>Living Rev Relativ</addtitle><description>Quantum fluctuation of light limits the sensitivity of advanced laser interferometric gravitational-wave detectors. It is one of the principal obstacles on the way towards the next-generation gravitational-wave observatories. The envisioned significant improvement of the detector sensitivity requires using quantum non-demolition measurement and back-action evasion techniques, which allow us to circumvent the sensitivity limit imposed by the Heisenberg uncertainty principle. In our previous review article (Danilishin and Khalili in Living Rev Relativ 15:5,
2012
), we laid down the basic principles of quantum measurement theory and provided the framework for analysing the quantum noise of interferometers. The scope of this paper is to review novel techniques for quantum noise suppression proposed in the recent years and put them in the same framework. 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2012
), we laid down the basic principles of quantum measurement theory and provided the framework for analysing the quantum noise of interferometers. The scope of this paper is to review novel techniques for quantum noise suppression proposed in the recent years and put them in the same framework. Our delineation of interferometry schemes and topologies is intended as an aid in the process of selecting the design for the next-generation gravitational-wave observatories.</abstract><cop>Cham</cop><pub>Springer International Publishing</pub><doi>10.1007/s41114-019-0018-y</doi><tpages>89</tpages><orcidid>https://orcid.org/0000-0001-7758-7493</orcidid><oa>free_for_read</oa></addata></record> |
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| subjects | Astrophysics and Astroparticles Classical and Quantum Gravitation Cosmology Demolition Detection equipment Gravitational waves Observatories Physics Physics and Astronomy Relativity Theory Review Article |
| title | Advanced quantum techniques for future gravitational-wave detectors |
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