Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light
- Autores
- Aasi, J.; Abadie, J.; Abbott, P.; Abbott, R.; Abbott, T. D.; Kozameh, Carlos Nicolas; Winkelmann, L.; Winkler, W.; Wip, C. C.; Wittel, H.; Woan, G.; Wooley, R.; Worden, J.; Yablon, J.; Yakushin, I.; Yamamoto, H.; Yancey, C. C.; Yang, H.; Yeaton Massey, D.; Yoshida, S.; Yum, H.; Zanolin, M.; Zhang, F.; Zhang, L.; Zhao, C.; Zhu, H.; Zhu, X. J.; Zotov, N.; Zucker, M. E.; Zweizig, J.
- Año de publicación
- 2013
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Nearly a century after Einstein first predicted the existence of gravitational waves, a global network of Earth-based gravitational wave observatories1,2,3,4 is seeking to directly detect this faint radiation using precision laser interferometry. Photon shot noise, due to the quantum nature of light, imposes a fundamental limit on the attometre-level sensitivity of the kilometre-scale Michelson interferometers deployed for this task. Here, we inject squeezed states to improve the performance of one of the detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) beyond the quantum noise limit, most notably in the frequency region down to 150 Hz, critically important for several astrophysical sources, with no deterioration of performance observed at any frequency. With the injection of squeezed states, this LIGO detector demonstrated the best broadband sensitivity to gravitational waves ever achieved, with important implications for observing the gravitational-wave Universe with unprecedented sensitivity
Fil: Aasi, J.. California Institute of Technology; Estados Unidos
Fil: Abadie, J.. California Institute of Technology; Estados Unidos
Fil: Abbott, P.. California Institute of Technology; Estados Unidos
Fil: Abbott, R.. California Institute of Technology; Estados Unidos
Fil: Abbott, T. D.. State University of Louisiana; Estados Unidos
Fil: Kozameh, Carlos Nicolas. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Winkelmann, L.. Max Planck Institut f¨ur Gravitationsphysik; Alemania. Leibniz Universit¨at Hannover; Alemania
Fil: Winkler, W.. Max Planck Institut f¨ur Gravitationsphysik; Alemania. Leibniz Universit¨at Hannover; Alemania
Fil: Wip, C. C.. Massachusetts Institute of Technology; Estados Unidos
Fil: Wittel, H.. Max Planck Institut f¨ur Gravitationsphysik; Alemania. Leibniz Universit¨at Hannover; Alemania
Fil: Woan, G.. University of Glasgow; Reino Unido
Fil: Wooley, R.. Livingston Observatory; Estados Unidos
Fil: Worden, J.. Hanford Observatory; Estados Unidos
Fil: Yablon, J.. Northwestern University; Estados Unidos
Fil: Yakushin, I.. Livingston Observatory; Estados Unidos
Fil: Yamamoto, H.. California Institute of Technology; Estados Unidos
Fil: Yancey, C. C.. University of Maryland; Estados Unidos
Fil: Yang, H.. Caltech-CaRT; Estados Unidos
Fil: Yeaton Massey, D.. California Institute of Technology; Estados Unidos
Fil: Yoshida, S.. Southeastern Louisiana University; Estados Unidos
Fil: Yum, H.. Northwestern University; Estados Unidos
Fil: Zanolin, M.. Embry-Riddle Aeronautical University; Estados Unidos
Fil: Zhang, F.. Massachusetts Institute of Technology; Estados Unidos
Fil: Zhang, L.. California Institute of Technology; Estados Unidos
Fil: Zhao, C.. University of Western Australia; Australia
Fil: Zhu, H.. State University of Pennsylvania; Estados Unidos
Fil: Zhu, X. J.. University of Western Australia; Australia
Fil: Zotov, N.. Louisiana Tech University; Estados Unidos
Fil: Zucker, M. E.. Massachusetts Institute of Technology; Estados Unidos
Fil: Zweizig, J.. California Institute of Technology; Estados Unidos - Materia
-
Gravitational Waves
Ligo
Detection
Sensitivity - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/29326
Ver los metadatos del registro completo
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Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of lightAasi, J.Abadie, J.Abbott, P.Abbott, R.Abbott, T. D.Kozameh, Carlos NicolasWinkelmann, L.Winkler, W.Wip, C. C.Wittel, H.Woan, G.Wooley, R.Worden, J.Yablon, J.Yakushin, I.Yamamoto, H.Yancey, C. C.Yang, H.Yeaton Massey, D.Yoshida, S.Yum, H.Zanolin, M.Zhang, F.Zhang, L.Zhao, C.Zhu, H.Zhu, X. J.Zotov, N.Zucker, M. E.Zweizig, J.Gravitational WavesLigoDetectionSensitivityhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Nearly a century after Einstein first predicted the existence of gravitational waves, a global network of Earth-based gravitational wave observatories1,2,3,4 is seeking to directly detect this faint radiation using precision laser interferometry. Photon shot noise, due to the quantum nature of light, imposes a fundamental limit on the attometre-level sensitivity of the kilometre-scale Michelson interferometers deployed for this task. Here, we inject squeezed states to improve the performance of one of the detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) beyond the quantum noise limit, most notably in the frequency region down to 150 Hz, critically important for several astrophysical sources, with no deterioration of performance observed at any frequency. With the injection of squeezed states, this LIGO detector demonstrated the best broadband sensitivity to gravitational waves ever achieved, with important implications for observing the gravitational-wave Universe with unprecedented sensitivityFil: Aasi, J.. California Institute of Technology; Estados UnidosFil: Abadie, J.. California Institute of Technology; Estados UnidosFil: Abbott, P.. California Institute of Technology; Estados UnidosFil: Abbott, R.. California Institute of Technology; Estados UnidosFil: Abbott, T. D.. State University of Louisiana; Estados UnidosFil: Kozameh, Carlos Nicolas. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Winkelmann, L.. Max Planck Institut f¨ur Gravitationsphysik; Alemania. Leibniz Universit¨at Hannover; AlemaniaFil: Winkler, W.. Max Planck Institut f¨ur Gravitationsphysik; Alemania. Leibniz Universit¨at Hannover; AlemaniaFil: Wip, C. C.. Massachusetts Institute of Technology; Estados UnidosFil: Wittel, H.. Max Planck Institut f¨ur Gravitationsphysik; Alemania. Leibniz Universit¨at Hannover; AlemaniaFil: Woan, G.. University of Glasgow; Reino UnidoFil: Wooley, R.. Livingston Observatory; Estados UnidosFil: Worden, J.. Hanford Observatory; Estados UnidosFil: Yablon, J.. Northwestern University; Estados UnidosFil: Yakushin, I.. Livingston Observatory; Estados UnidosFil: Yamamoto, H.. California Institute of Technology; Estados UnidosFil: Yancey, C. C.. University of Maryland; Estados UnidosFil: Yang, H.. Caltech-CaRT; Estados UnidosFil: Yeaton Massey, D.. California Institute of Technology; Estados UnidosFil: Yoshida, S.. Southeastern Louisiana University; Estados UnidosFil: Yum, H.. Northwestern University; Estados UnidosFil: Zanolin, M.. Embry-Riddle Aeronautical University; Estados UnidosFil: Zhang, F.. Massachusetts Institute of Technology; Estados UnidosFil: Zhang, L.. California Institute of Technology; Estados UnidosFil: Zhao, C.. University of Western Australia; AustraliaFil: Zhu, H.. State University of Pennsylvania; Estados UnidosFil: Zhu, X. J.. University of Western Australia; AustraliaFil: Zotov, N.. Louisiana Tech University; Estados UnidosFil: Zucker, M. E.. Massachusetts Institute of Technology; Estados UnidosFil: Zweizig, J.. California Institute of Technology; Estados UnidosNature Publishing Group2013-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/29326Aasi, J.; Abadie, J.; Abbott, P.; Abbott, R.; Abbott, T. D.; et al.; Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light; Nature Publishing Group; Nature Photonics; 7; 10-2013; 613-6191749-4885CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1038/nphoton.2013.177info:eu-repo/semantics/altIdentifier/url/https://www.nature.com/articles/nphoton.2013.177info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:33:47Zoai:ri.conicet.gov.ar:11336/29326instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:33:47.882CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light |
| title |
Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light |
| spellingShingle |
Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light Aasi, J. Gravitational Waves Ligo Detection Sensitivity |
| title_short |
Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light |
| title_full |
Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light |
| title_fullStr |
Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light |
| title_full_unstemmed |
Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light |
| title_sort |
Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light |
| dc.creator.none.fl_str_mv |
Aasi, J. Abadie, J. Abbott, P. Abbott, R. Abbott, T. D. Kozameh, Carlos Nicolas Winkelmann, L. Winkler, W. Wip, C. C. Wittel, H. Woan, G. Wooley, R. Worden, J. Yablon, J. Yakushin, I. Yamamoto, H. Yancey, C. C. Yang, H. Yeaton Massey, D. Yoshida, S. Yum, H. Zanolin, M. Zhang, F. Zhang, L. Zhao, C. Zhu, H. Zhu, X. J. Zotov, N. Zucker, M. E. Zweizig, J. |
| author |
Aasi, J. |
| author_facet |
Aasi, J. Abadie, J. Abbott, P. Abbott, R. Abbott, T. D. Kozameh, Carlos Nicolas Winkelmann, L. Winkler, W. Wip, C. C. Wittel, H. Woan, G. Wooley, R. Worden, J. Yablon, J. Yakushin, I. Yamamoto, H. Yancey, C. C. Yang, H. Yeaton Massey, D. Yoshida, S. Yum, H. Zanolin, M. Zhang, F. Zhang, L. Zhao, C. Zhu, H. Zhu, X. J. Zotov, N. Zucker, M. E. Zweizig, J. |
| author_role |
author |
| author2 |
Abadie, J. Abbott, P. Abbott, R. Abbott, T. D. Kozameh, Carlos Nicolas Winkelmann, L. Winkler, W. Wip, C. C. Wittel, H. Woan, G. Wooley, R. Worden, J. Yablon, J. Yakushin, I. Yamamoto, H. Yancey, C. C. Yang, H. Yeaton Massey, D. Yoshida, S. Yum, H. Zanolin, M. Zhang, F. Zhang, L. Zhao, C. Zhu, H. Zhu, X. J. Zotov, N. Zucker, M. E. Zweizig, J. |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
Gravitational Waves Ligo Detection Sensitivity |
| topic |
Gravitational Waves Ligo Detection Sensitivity |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Nearly a century after Einstein first predicted the existence of gravitational waves, a global network of Earth-based gravitational wave observatories1,2,3,4 is seeking to directly detect this faint radiation using precision laser interferometry. Photon shot noise, due to the quantum nature of light, imposes a fundamental limit on the attometre-level sensitivity of the kilometre-scale Michelson interferometers deployed for this task. Here, we inject squeezed states to improve the performance of one of the detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) beyond the quantum noise limit, most notably in the frequency region down to 150 Hz, critically important for several astrophysical sources, with no deterioration of performance observed at any frequency. With the injection of squeezed states, this LIGO detector demonstrated the best broadband sensitivity to gravitational waves ever achieved, with important implications for observing the gravitational-wave Universe with unprecedented sensitivity Fil: Aasi, J.. California Institute of Technology; Estados Unidos Fil: Abadie, J.. California Institute of Technology; Estados Unidos Fil: Abbott, P.. California Institute of Technology; Estados Unidos Fil: Abbott, R.. California Institute of Technology; Estados Unidos Fil: Abbott, T. D.. State University of Louisiana; Estados Unidos Fil: Kozameh, Carlos Nicolas. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Winkelmann, L.. Max Planck Institut f¨ur Gravitationsphysik; Alemania. Leibniz Universit¨at Hannover; Alemania Fil: Winkler, W.. Max Planck Institut f¨ur Gravitationsphysik; Alemania. Leibniz Universit¨at Hannover; Alemania Fil: Wip, C. C.. Massachusetts Institute of Technology; Estados Unidos Fil: Wittel, H.. Max Planck Institut f¨ur Gravitationsphysik; Alemania. Leibniz Universit¨at Hannover; Alemania Fil: Woan, G.. University of Glasgow; Reino Unido Fil: Wooley, R.. Livingston Observatory; Estados Unidos Fil: Worden, J.. Hanford Observatory; Estados Unidos Fil: Yablon, J.. Northwestern University; Estados Unidos Fil: Yakushin, I.. Livingston Observatory; Estados Unidos Fil: Yamamoto, H.. California Institute of Technology; Estados Unidos Fil: Yancey, C. C.. University of Maryland; Estados Unidos Fil: Yang, H.. Caltech-CaRT; Estados Unidos Fil: Yeaton Massey, D.. California Institute of Technology; Estados Unidos Fil: Yoshida, S.. Southeastern Louisiana University; Estados Unidos Fil: Yum, H.. Northwestern University; Estados Unidos Fil: Zanolin, M.. Embry-Riddle Aeronautical University; Estados Unidos Fil: Zhang, F.. Massachusetts Institute of Technology; Estados Unidos Fil: Zhang, L.. California Institute of Technology; Estados Unidos Fil: Zhao, C.. University of Western Australia; Australia Fil: Zhu, H.. State University of Pennsylvania; Estados Unidos Fil: Zhu, X. J.. University of Western Australia; Australia Fil: Zotov, N.. Louisiana Tech University; Estados Unidos Fil: Zucker, M. E.. Massachusetts Institute of Technology; Estados Unidos Fil: Zweizig, J.. California Institute of Technology; Estados Unidos |
| description |
Nearly a century after Einstein first predicted the existence of gravitational waves, a global network of Earth-based gravitational wave observatories1,2,3,4 is seeking to directly detect this faint radiation using precision laser interferometry. Photon shot noise, due to the quantum nature of light, imposes a fundamental limit on the attometre-level sensitivity of the kilometre-scale Michelson interferometers deployed for this task. Here, we inject squeezed states to improve the performance of one of the detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) beyond the quantum noise limit, most notably in the frequency region down to 150 Hz, critically important for several astrophysical sources, with no deterioration of performance observed at any frequency. With the injection of squeezed states, this LIGO detector demonstrated the best broadband sensitivity to gravitational waves ever achieved, with important implications for observing the gravitational-wave Universe with unprecedented sensitivity |
| publishDate |
2013 |
| dc.date.none.fl_str_mv |
2013-10 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/29326 Aasi, J.; Abadie, J.; Abbott, P.; Abbott, R.; Abbott, T. D.; et al.; Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light; Nature Publishing Group; Nature Photonics; 7; 10-2013; 613-619 1749-4885 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/29326 |
| identifier_str_mv |
Aasi, J.; Abadie, J.; Abbott, P.; Abbott, R.; Abbott, T. D.; et al.; Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light; Nature Publishing Group; Nature Photonics; 7; 10-2013; 613-619 1749-4885 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/doi/10.1038/nphoton.2013.177 info:eu-repo/semantics/altIdentifier/url/https://www.nature.com/articles/nphoton.2013.177 |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
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Nature Publishing Group |
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Nature Publishing Group |
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