Frequency-Dependent Squeezed Vacuum Source for the Advanced Virgo Gravitational-Wave Detector

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

Autoren

  • Virgo Collaboration
  • H. Vahlbruch
  • H. Lück
  • K. Danzmann

Organisationseinheiten

Externe Organisationen

  • Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
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Details

OriginalspracheEnglisch
Aufsatznummer041403
FachzeitschriftPhysical review letters
Jahrgang131
Ausgabenummer4
PublikationsstatusVeröffentlicht - 25 Juli 2023

Abstract

In this Letter, we present the design and performance of the frequency-dependent squeezed vacuum source that will be used for the broadband quantum noise reduction of the Advanced Virgo Plus gravitational-wave detector in the upcoming observation run. The frequency-dependent squeezed field is generated by a phase rotation of a frequency-independent squeezed state through a 285 m long, high-finesse, near-detuned optical resonator. With about 8.5 dB of generated squeezing, up to 5.6 dB of quantum noise suppression has been measured at high frequency while close to the filter cavity resonance frequency, the intracavity losses limit this value to about 2 dB. Frequency-dependent squeezing is produced with a rotation frequency stability of about 6 Hz rms, which is maintained over the long term. The achieved results fulfill the frequency dependent squeezed vacuum source requirements for Advanced Virgo Plus. With the current squeezing source, considering also the estimated squeezing degradation induced by the interferometer, we expect a reduction of the quantum shot noise and radiation pressure noise of up to 4.5 dB and 2 dB, respectively.

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Frequency-Dependent Squeezed Vacuum Source for the Advanced Virgo Gravitational-Wave Detector. / Virgo Collaboration; Vahlbruch, H.; Lück, H. et al.
in: Physical review letters, Jahrgang 131, Nr. 4, 041403, 25.07.2023.

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

Virgo Collaboration, Vahlbruch H, Lück H, Danzmann K. Frequency-Dependent Squeezed Vacuum Source for the Advanced Virgo Gravitational-Wave Detector. Physical review letters. 2023 Jul 25;131(4):041403. doi: 10.1103/physrevlett.131.041403
Virgo Collaboration ; Vahlbruch, H. ; Lück, H. et al. / Frequency-Dependent Squeezed Vacuum Source for the Advanced Virgo Gravitational-Wave Detector. in: Physical review letters. 2023 ; Jahrgang 131, Nr. 4.
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@article{13ce2a6ffa14407a9d3b6c7943527570,
title = "Frequency-Dependent Squeezed Vacuum Source for the Advanced Virgo Gravitational-Wave Detector",
abstract = "In this Letter, we present the design and performance of the frequency-dependent squeezed vacuum source that will be used for the broadband quantum noise reduction of the Advanced Virgo Plus gravitational-wave detector in the upcoming observation run. The frequency-dependent squeezed field is generated by a phase rotation of a frequency-independent squeezed state through a 285 m long, high-finesse, near-detuned optical resonator. With about 8.5 dB of generated squeezing, up to 5.6 dB of quantum noise suppression has been measured at high frequency while close to the filter cavity resonance frequency, the intracavity losses limit this value to about 2 dB. Frequency-dependent squeezing is produced with a rotation frequency stability of about 6 Hz rms, which is maintained over the long term. The achieved results fulfill the frequency dependent squeezed vacuum source requirements for Advanced Virgo Plus. With the current squeezing source, considering also the estimated squeezing degradation induced by the interferometer, we expect a reduction of the quantum shot noise and radiation pressure noise of up to 4.5 dB and 2 dB, respectively.",
author = "{The Virgo Collaboration} and F. Acernese and M. Agathos and A. Ain and S. Albanesi and C. All{\'e}n{\'e} and A. Allocca and A. Amato and C. Amra and M. Andia and T. Andrade and N. Andres and M. Andr{\'e}s-Carcasona and T. Andri{\'c} and S. Ansoldi and S. Antier and T. Apostolatos and E. Z. Appavuravther and M. Ar{\`e}ne and N. Arnaud and M. Assiduo and Melo, {S. Assis de Souza} and P. Astone and F. Aubin and S. Babak and F. Badaracco and S. Bagnasco and J. Baird and T. Baka and G. Ballardin and G. Baltus and B. Banerjee and P. Barneo and F. Barone and M. Barsuglia and D. Barta and A. Basti and M. Bawaj and M. Bazzan and F. Beirnaert and M. Bejger and V. Benedetto and M. Berbel and S. Bernuzzi and D. Bersanetti and A. Bertolini and U. Bhardwaj and S. Danilishin and H. Vahlbruch and H. L{\"u}ck and K. Danzmann",
note = "Funding Information: The authors gratefully acknowledge the support of the Max Planck Society, Leibniz Universit{\"a}t Hannover and Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) through project Grant No. VA 1031/1-1 and Germany{\textquoteright}s Excellence Strategy—EXC-2123 QuantumFrontiers—390837967 for the construction, installation, and operation of the squeezed light source. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS), and the Netherlands Organization for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as from the Spanish Agencia Estatal de Investigaci{\'o}n, the Consellera d{\textquoteright}Innovaci{\'o}, Universitats, Ci{\`e}ncia i Societat Digital de la Generalitat Valenciana and the CERCA Programme Generalitat de Catalunya, Spain, the National Science Centre of Poland, the European Commission, the Hungarian Scientific Research Fund (OTKA), the French Lyon Institute of Origins (LIO), the Belgian Fonds de la Recherche Scientifique (FRS-FNRS), Actions de Recherche Concert{\'e}es (ARC), Fonds Wetenschappelijk Onderzoek—Vlaanderen (FWO), Belgium, {\'E}cole Polytechnique, Japan Society for the Promotion of Science (Grant-in-Aid for Scientific Research No. 21H04476) and the Institute for Cosmic Ray Research (ICRR) and the LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001).",
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month = jul,
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language = "English",
volume = "131",
journal = "Physical review letters",
issn = "1079-7114",
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Download

TY - JOUR

T1 - Frequency-Dependent Squeezed Vacuum Source for the Advanced Virgo Gravitational-Wave Detector

AU - The Virgo Collaboration

AU - Acernese, F.

AU - Agathos, M.

AU - Ain, A.

AU - Albanesi, S.

AU - Alléné, C.

AU - Allocca, A.

AU - Amato, A.

AU - Amra, C.

AU - Andia, M.

AU - Andrade, T.

AU - Andres, N.

AU - Andrés-Carcasona, M.

AU - Andrić, T.

AU - Ansoldi, S.

AU - Antier, S.

AU - Apostolatos, T.

AU - Appavuravther, E. Z.

AU - Arène, M.

AU - Arnaud, N.

AU - Assiduo, M.

AU - Melo, S. Assis de Souza

AU - Astone, P.

AU - Aubin, F.

AU - Babak, S.

AU - Badaracco, F.

AU - Bagnasco, S.

AU - Baird, J.

AU - Baka, T.

AU - Ballardin, G.

AU - Baltus, G.

AU - Banerjee, B.

AU - Barneo, P.

AU - Barone, F.

AU - Barsuglia, M.

AU - Barta, D.

AU - Basti, A.

AU - Bawaj, M.

AU - Bazzan, M.

AU - Beirnaert, F.

AU - Bejger, M.

AU - Benedetto, V.

AU - Berbel, M.

AU - Bernuzzi, S.

AU - Bersanetti, D.

AU - Bertolini, A.

AU - Bhardwaj, U.

AU - Danilishin, S.

AU - Vahlbruch, H.

AU - Lück, H.

AU - Danzmann, K.

N1 - Funding Information: The authors gratefully acknowledge the support of the Max Planck Society, Leibniz Universität Hannover and Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) through project Grant No. VA 1031/1-1 and Germany’s Excellence Strategy—EXC-2123 QuantumFrontiers—390837967 for the construction, installation, and operation of the squeezed light source. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS), and the Netherlands Organization for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as from the Spanish Agencia Estatal de Investigación, the Consellera d’Innovació, Universitats, Ciència i Societat Digital de la Generalitat Valenciana and the CERCA Programme Generalitat de Catalunya, Spain, the National Science Centre of Poland, the European Commission, the Hungarian Scientific Research Fund (OTKA), the French Lyon Institute of Origins (LIO), the Belgian Fonds de la Recherche Scientifique (FRS-FNRS), Actions de Recherche Concertées (ARC), Fonds Wetenschappelijk Onderzoek—Vlaanderen (FWO), Belgium, École Polytechnique, Japan Society for the Promotion of Science (Grant-in-Aid for Scientific Research No. 21H04476) and the Institute for Cosmic Ray Research (ICRR) and the LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001).

PY - 2023/7/25

Y1 - 2023/7/25

N2 - In this Letter, we present the design and performance of the frequency-dependent squeezed vacuum source that will be used for the broadband quantum noise reduction of the Advanced Virgo Plus gravitational-wave detector in the upcoming observation run. The frequency-dependent squeezed field is generated by a phase rotation of a frequency-independent squeezed state through a 285 m long, high-finesse, near-detuned optical resonator. With about 8.5 dB of generated squeezing, up to 5.6 dB of quantum noise suppression has been measured at high frequency while close to the filter cavity resonance frequency, the intracavity losses limit this value to about 2 dB. Frequency-dependent squeezing is produced with a rotation frequency stability of about 6 Hz rms, which is maintained over the long term. The achieved results fulfill the frequency dependent squeezed vacuum source requirements for Advanced Virgo Plus. With the current squeezing source, considering also the estimated squeezing degradation induced by the interferometer, we expect a reduction of the quantum shot noise and radiation pressure noise of up to 4.5 dB and 2 dB, respectively.

AB - In this Letter, we present the design and performance of the frequency-dependent squeezed vacuum source that will be used for the broadband quantum noise reduction of the Advanced Virgo Plus gravitational-wave detector in the upcoming observation run. The frequency-dependent squeezed field is generated by a phase rotation of a frequency-independent squeezed state through a 285 m long, high-finesse, near-detuned optical resonator. With about 8.5 dB of generated squeezing, up to 5.6 dB of quantum noise suppression has been measured at high frequency while close to the filter cavity resonance frequency, the intracavity losses limit this value to about 2 dB. Frequency-dependent squeezing is produced with a rotation frequency stability of about 6 Hz rms, which is maintained over the long term. The achieved results fulfill the frequency dependent squeezed vacuum source requirements for Advanced Virgo Plus. With the current squeezing source, considering also the estimated squeezing degradation induced by the interferometer, we expect a reduction of the quantum shot noise and radiation pressure noise of up to 4.5 dB and 2 dB, respectively.

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U2 - 10.1103/physrevlett.131.041403

DO - 10.1103/physrevlett.131.041403

M3 - Article

VL - 131

JO - Physical review letters

JF - Physical review letters

SN - 1079-7114

IS - 4

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