Gravitational wave detectors with broadband high frequency sensitivity

Gravitational wave astronomy is on a path to increase the sensitivity and bandwidth of their detectors to afford the possibility to study a larger variety of sources and physical processes. The authors present solutions to enhance the sensitivity of a laser interferometric gravitational wave detecto...

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Autores principales:	Michael A. Page, Maxim Goryachev, Haixing Miao, Yanbei Chen, Yiqiu Ma, David Mason, Massimiliano Rossi, Carl D. Blair, Li Ju, David G. Blair, Albert Schliesser, Michael E. Tobar, Chunnong Zhao
Formato:	article
Lenguaje:	EN
Publicado:	Nature Portfolio 2021
Materias:	Astrophysics QB460-466 Physics QC1-999
Acceso en línea:	https://doaj.org/article/f2a2419e386a4421bed5dcd4827bf8fa
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spelling	oai:doaj.org-article:f2a2419e386a4421bed5dcd4827bf8fa2021-12-02T12:11:44ZGravitational wave detectors with broadband high frequency sensitivity10.1038/s42005-021-00526-22399-3650https://doaj.org/article/f2a2419e386a4421bed5dcd4827bf8fa2021-02-01T00:00:00Zhttps://doi.org/10.1038/s42005-021-00526-2https://doaj.org/toc/2399-3650Gravitational wave astronomy is on a path to increase the sensitivity and bandwidth of their detectors to afford the possibility to study a larger variety of sources and physical processes. The authors present solutions to enhance the sensitivity of a laser interferometric gravitational wave detector in the frequency band of 1-5 kHz using optomechanics-based white light signal recycling technologies, overcoming previous limitations of signal recycling.Michael A. PageMaxim GoryachevHaixing MiaoYanbei ChenYiqiu MaDavid MasonMassimiliano RossiCarl D. BlairLi JuDavid G. BlairAlbert SchliesserMichael E. TobarChunnong ZhaoNature PortfolioarticleAstrophysicsQB460-466PhysicsQC1-999ENCommunications Physics, Vol 4, Iss 1, Pp 1-8 (2021)
institution	DOAJ
collection	DOAJ
language	EN
topic	Astrophysics QB460-466 Physics QC1-999
spellingShingle	Astrophysics QB460-466 Physics QC1-999 Michael A. Page Maxim Goryachev Haixing Miao Yanbei Chen Yiqiu Ma David Mason Massimiliano Rossi Carl D. Blair Li Ju David G. Blair Albert Schliesser Michael E. Tobar Chunnong Zhao Gravitational wave detectors with broadband high frequency sensitivity
description	Gravitational wave astronomy is on a path to increase the sensitivity and bandwidth of their detectors to afford the possibility to study a larger variety of sources and physical processes. The authors present solutions to enhance the sensitivity of a laser interferometric gravitational wave detector in the frequency band of 1-5 kHz using optomechanics-based white light signal recycling technologies, overcoming previous limitations of signal recycling.
format	article
author	Michael A. Page Maxim Goryachev Haixing Miao Yanbei Chen Yiqiu Ma David Mason Massimiliano Rossi Carl D. Blair Li Ju David G. Blair Albert Schliesser Michael E. Tobar Chunnong Zhao
author_facet	Michael A. Page Maxim Goryachev Haixing Miao Yanbei Chen Yiqiu Ma David Mason Massimiliano Rossi Carl D. Blair Li Ju David G. Blair Albert Schliesser Michael E. Tobar Chunnong Zhao
author_sort	Michael A. Page
title	Gravitational wave detectors with broadband high frequency sensitivity
title_short	Gravitational wave detectors with broadband high frequency sensitivity
title_full	Gravitational wave detectors with broadband high frequency sensitivity
title_fullStr	Gravitational wave detectors with broadband high frequency sensitivity
title_full_unstemmed	Gravitational wave detectors with broadband high frequency sensitivity
title_sort	gravitational wave detectors with broadband high frequency sensitivity
publisher	Nature Portfolio
publishDate	2021
url	https://doaj.org/article/f2a2419e386a4421bed5dcd4827bf8fa
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Gravitational wave detectors with broadband high frequency sensitivity

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