ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors

A. Utina; A. Amato; J. Arends; C. Arina; M. de Baar; M. Baars; P. Baer; N. van Bakel; W. Beaumont; A. Bertolini; M. van Beuzekom; S. Biersteker; A. Binetti; H. J.M. ter Brake; G. Bruno; J. Bryant; H. J. Bulten; L. Busch; P. Cebeci; C. Collette; S. Cooper; R. Cornelissen; P. Cuijpers; M. van Dael; S. Danilishin; D. Diksha; S. van Doesburg; M. Doets; R. Elsinga; V. Erends; J. van Erps; A. Freise; H. Frenaij; R. Garcia; M. Giesberts; S. Grohmann; H. Van Haevermaet; S. Heijnen; J. V. van Heijningen; E. Hennes; J. S. Hennig; M. Hennig; T. Hertog; S. Hild; H. D. Hoffmann; G. Hoft; M. Hopman; D. Hoyland; G. A. Iandolo; C. Ietswaard; R. Jamshidi; P. Jansweijer; A. Jones; P. Jones; N. Knust; G. Koekoek; X. Koroveshi; T. Kortekaas; A. N. Koushik; M. Kraan; M. van de Kraats; S. L. Kranzhoff; P. Kuijer; K. A. Kukkadapu; K. Lam; N. Letendre; P. Li; R. Limburg; F. Linde; J. P. Locquet; P. Loosen; H. Lueck; M. Martínez; A. Masserot; F. Meylahn; M. Molenaar; C. Mow-Lowry; J. Mundet; B. Munneke; L. van Nieuwland; E. Pacaud; D. Pascucci; S. Petit; Z. Van Ranst; G. Raskin; P. M. Recaman; N. van Remortel; L. Rolland; L. de Roo; E. Roose; J. C. Rosier; D. Ryckbosch; K. Schouteden; A. Sevrin; A. Sider; A. Singha; V. Spagnuolo; A. Stahl; J. Steinlechner; S. Steinlechner; B. Swinkels; N. Szilasi; M. Tacca; H. Thienpont; A. Vecchio; H. Verkooijen; C. H. Vermeer; M. Vervaeke; G. Visser; R. Walet; P. Werneke; C. Westhofen; B. Willke; A. Xhahi; T. Zhang

doi:10.1088/1361-6382/ac8fdb

ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors

A. Utina
, A. Amato
, J. Arends
, C. Arina
, M. de Baar
, M. Baars
, P. Baer
, N. van Bakel
, W. Beaumont
, A. Bertolini
, M. van Beuzekom
, S. Biersteker
, A. Binetti
, H. J.M. ter Brake
, G. Bruno
, J. Bryant
, H. J. Bulten
, L. Busch
, P. Cebeci
, C. Collette

S. Cooper, R. Cornelissen, P. Cuijpers, M. van Dael, S. Danilishin, D. Diksha, S. van Doesburg, M. Doets, R. Elsinga, V. Erends, J. van Erps, A. Freise, H. Frenaij, R. Garcia, M. Giesberts, S. Grohmann, H. Van Haevermaet, S. Heijnen, J. V. van Heijningen, E. Hennes, J. S. Hennig, M. Hennig, T. Hertog, S. Hild, H. D. Hoffmann, G. Hoft, M. Hopman, D. Hoyland, G. A. Iandolo, C. Ietswaard, R. Jamshidi, P. Jansweijer, A. Jones, P. Jones, N. Knust, G. Koekoek, X. Koroveshi, T. Kortekaas, A. N. Koushik, M. Kraan, M. van de Kraats, S. L. Kranzhoff, P. Kuijer, K. A. Kukkadapu, K. Lam, N. Letendre, P. Li, R. Limburg, F. Linde, J. P. Locquet, P. Loosen, H. Lueck, M. Martínez, A. Masserot, F. Meylahn, M. Molenaar, C. Mow-Lowry, J. Mundet, B. Munneke, L. van Nieuwland, E. Pacaud, D. Pascucci, S. Petit, Z. Van Ranst, G. Raskin, P. M. Recaman, N. van Remortel, L. Rolland, L. de Roo, E. Roose, J. C. Rosier, D. Ryckbosch, K. Schouteden, A. Sevrin, A. Sider, A. Singha, V. Spagnuolo, A. Stahl, J. Steinlechner, S. Steinlechner, B. Swinkels, N. Szilasi, M. Tacca, H. Thienpont, A. Vecchio, H. Verkooijen, C. H. Vermeer, M. Vervaeke, G. Visser, R. Walet, P. Werneke, C. Westhofen, B. Willke, A. Xhahi, T. Zhang

Maastricht University
National Institute for Subatomic Physics
Vrije Universiteit Amsterdam
Université catholique de Louvain
Eindhoven University of Technology
Fraunhofer Institute for Laser Technology
University of Antwerp
KU Leuven
University of Twente
University of Birmingham
Karlsruhe Institute of Technology
ULiege-Precision Mechatronics Laboratory
Vrije Universiteit Brussel
ICREA
University of Western Australia
Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
Université Grenoble Alpes
Ghent University
RWTH Aachen University

科研成果: 期刊稿件 › 文章 › 同行评审

21 引用（Scopus）

摘要

The third-generation (3G) of gravitational wave observatories, such as the Einstein Telescope (ET) and Cosmic Explorer, aim for an improvement in sensitivity of at least a factor of ten over a wide frequency range compared to the current advanced detectors. In order to inform the design of the 3G detectors and to develop and qualify their subsystems, dedicated test facilities are required. ETpathfinder prototype uses full interferometer configurations and aims to provide a high sensitivity facility in a similar environment as ET. Along with the interferometry at 1550 nm and silicon test masses, ETpathfinder will focus on cryogenic technologies, lasers and optics at 2090 nm and advanced quantum-noise reduction schemes. This paper analyses the underpinning noise contributions and combines them into full noise budgets of the two initially targeted configurations: (1) operating with 1550 nm laser light and at a temperature of 18 K and (2) operating at 2090 nm wavelength and a temperature of 123 K.

源语言	英语
文章编号	215008
期刊	Classical and Quantum Gravity
卷	39
期	21
DOI	https://doi.org/10.1088/1361-6382/ac8fdb
出版状态	已出版 - 3 11月 2022
已对外发布	是

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10.1088/1361-6382/ac8fdb

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Utina, A., Amato, A., Arends, J., Arina, C., de Baar, M., Baars, M., Baer, P., van Bakel, N., Beaumont, W., Bertolini, A., van Beuzekom, M., Biersteker, S., Binetti, A., ter Brake, H. J. M., Bruno, G., Bryant, J., Bulten, H. J., Busch, L., Cebeci, P., ... Zhang, T. (2022). ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors. Classical and Quantum Gravity, 39(21), 文章 215008. https://doi.org/10.1088/1361-6382/ac8fdb

@article{d9325604672c431cb31f6847e5ae8bdf,

title = "ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors",

abstract = "The third-generation (3G) of gravitational wave observatories, such as the Einstein Telescope (ET) and Cosmic Explorer, aim for an improvement in sensitivity of at least a factor of ten over a wide frequency range compared to the current advanced detectors. In order to inform the design of the 3G detectors and to develop and qualify their subsystems, dedicated test facilities are required. ETpathfinder prototype uses full interferometer configurations and aims to provide a high sensitivity facility in a similar environment as ET. Along with the interferometry at 1550 nm and silicon test masses, ETpathfinder will focus on cryogenic technologies, lasers and optics at 2090 nm and advanced quantum-noise reduction schemes. This paper analyses the underpinning noise contributions and combines them into full noise budgets of the two initially targeted configurations: (1) operating with 1550 nm laser light and at a temperature of 18 K and (2) operating at 2090 nm wavelength and a temperature of 123 K.",

keywords = "Cosmic Explorer, ETpathfinder, Einstein Telescope, Voyager, gravitational-wave detectors, third generation of gravitational-wave detectors",

author = "A. Utina and A. Amato and J. Arends and C. Arina and \{de Baar\}, M. and M. Baars and P. Baer and \{van Bakel\}, N. and W. Beaumont and A. Bertolini and \{van Beuzekom\}, M. and S. Biersteker and A. Binetti and \{ter Brake\}, \{H. J.M.\} and G. Bruno and J. Bryant and Bulten, \{H. J.\} and L. Busch and P. Cebeci and C. Collette and S. Cooper and R. Cornelissen and P. Cuijpers and \{van Dael\}, M. and S. Danilishin and D. Diksha and \{van Doesburg\}, S. and M. Doets and R. Elsinga and V. Erends and \{van Erps\}, J. and A. Freise and H. Frenaij and R. Garcia and M. Giesberts and S. Grohmann and \{Van Haevermaet\}, H. and S. Heijnen and \{van Heijningen\}, \{J. V.\} and E. Hennes and Hennig, \{J. S.\} and M. Hennig and T. Hertog and S. Hild and Hoffmann, \{H. D.\} and G. Hoft and M. Hopman and D. Hoyland and Iandolo, \{G. A.\} and C. Ietswaard and R. Jamshidi and P. Jansweijer and A. Jones and P. Jones and N. Knust and G. Koekoek and X. Koroveshi and T. Kortekaas and Koushik, \{A. N.\} and M. Kraan and \{van de Kraats\}, M. and Kranzhoff, \{S. L.\} and P. Kuijer and Kukkadapu, \{K. A.\} and K. Lam and N. Letendre and P. Li and R. Limburg and F. Linde and Locquet, \{J. P.\} and P. Loosen and H. Lueck and M. Mart{\'i}nez and A. Masserot and F. Meylahn and M. Molenaar and C. Mow-Lowry and J. Mundet and B. Munneke and \{van Nieuwland\}, L. and E. Pacaud and D. Pascucci and S. Petit and \{Van Ranst\}, Z. and G. Raskin and Recaman, \{P. M.\} and \{van Remortel\}, N. and L. Rolland and \{de Roo\}, L. and E. Roose and Rosier, \{J. C.\} and D. Ryckbosch and K. Schouteden and A. Sevrin and A. Sider and A. Singha and V. Spagnuolo and A. Stahl and J. Steinlechner and S. Steinlechner and B. Swinkels and N. Szilasi and M. Tacca and H. Thienpont and A. Vecchio and H. Verkooijen and Vermeer, \{C. H.\} and M. Vervaeke and G. Visser and R. Walet and P. Werneke and C. Westhofen and B. Willke and A. Xhahi and T. Zhang",

note = "Publisher Copyright: {\textcopyright} 2022 The Author(s). Published by IOP Publishing Ltd.",

year = "2022",

month = nov,

day = "3",

doi = "10.1088/1361-6382/ac8fdb",

language = "英语",

volume = "39",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

publisher = "IOP Publishing Ltd.",

number = "21",

}

Utina, A, Amato, A, Arends, J, Arina, C, de Baar, M, Baars, M, Baer, P, van Bakel, N, Beaumont, W, Bertolini, A, van Beuzekom, M, Biersteker, S, Binetti, A, ter Brake, HJM, Bruno, G, Bryant, J, Bulten, HJ, Busch, L, Cebeci, P, Collette, C, Cooper, S, Cornelissen, R, Cuijpers, P, van Dael, M, Danilishin, S, Diksha, D, van Doesburg, S, Doets, M, Elsinga, R, Erends, V, van Erps, J, Freise, A, Frenaij, H, Garcia, R, Giesberts, M, Grohmann, S, Van Haevermaet, H, Heijnen, S, van Heijningen, JV, Hennes, E, Hennig, JS, Hennig, M, Hertog, T, Hild, S, Hoffmann, HD, Hoft, G, Hopman, M, Hoyland, D, Iandolo, GA, Ietswaard, C, Jamshidi, R, Jansweijer, P, Jones, A, Jones, P, Knust, N, Koekoek, G, Koroveshi, X, Kortekaas, T, Koushik, AN, Kraan, M, van de Kraats, M, Kranzhoff, SL, Kuijer, P, Kukkadapu, KA, Lam, K, Letendre, N, Li, P, Limburg, R, Linde, F, Locquet, JP, Loosen, P, Lueck, H, Martínez, M, Masserot, A, Meylahn, F, Molenaar, M, Mow-Lowry, C, Mundet, J, Munneke, B, van Nieuwland, L, Pacaud, E, Pascucci, D, Petit, S, Van Ranst, Z, Raskin, G, Recaman, PM, van Remortel, N, Rolland, L, de Roo, L, Roose, E, Rosier, JC, Ryckbosch, D, Schouteden, K, Sevrin, A, Sider, A, Singha, A, Spagnuolo, V, Stahl, A, Steinlechner, J, Steinlechner, S, Swinkels, B, Szilasi, N, Tacca, M, Thienpont, H, Vecchio, A, Verkooijen, H, Vermeer, CH, Vervaeke, M, Visser, G, Walet, R, Werneke, P, Westhofen, C, Willke, B, Xhahi, A & Zhang, T 2022, 'ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors', Classical and Quantum Gravity, 卷 39, 号码 21, 215008. https://doi.org/10.1088/1361-6382/ac8fdb

TY - JOUR

T1 - ETpathfinder

T2 - a cryogenic testbed for interferometric gravitational-wave detectors

AU - Utina, A.

AU - Amato, A.

AU - Arends, J.

AU - Arina, C.

AU - de Baar, M.

AU - Baars, M.

AU - Baer, P.

AU - van Bakel, N.

AU - Beaumont, W.

AU - Bertolini, A.

AU - van Beuzekom, M.

AU - Biersteker, S.

AU - Binetti, A.

AU - ter Brake, H. J.M.

AU - Bruno, G.

AU - Bryant, J.

AU - Bulten, H. J.

AU - Busch, L.

AU - Cebeci, P.

AU - Collette, C.

AU - Cooper, S.

AU - Cornelissen, R.

AU - Cuijpers, P.

AU - van Dael, M.

AU - Danilishin, S.

AU - Diksha, D.

AU - van Doesburg, S.

AU - Doets, M.

AU - Elsinga, R.

AU - Erends, V.

AU - van Erps, J.

AU - Freise, A.

AU - Frenaij, H.

AU - Garcia, R.

AU - Giesberts, M.

AU - Grohmann, S.

AU - Van Haevermaet, H.

AU - Heijnen, S.

AU - van Heijningen, J. V.

AU - Hennes, E.

AU - Hennig, J. S.

AU - Hennig, M.

AU - Hertog, T.

AU - Hild, S.

AU - Hoffmann, H. D.

AU - Hoft, G.

AU - Hopman, M.

AU - Hoyland, D.

AU - Iandolo, G. A.

AU - Ietswaard, C.

AU - Jamshidi, R.

AU - Jansweijer, P.

AU - Jones, A.

AU - Jones, P.

AU - Knust, N.

AU - Koekoek, G.

AU - Koroveshi, X.

AU - Kortekaas, T.

AU - Koushik, A. N.

AU - Kraan, M.

AU - van de Kraats, M.

AU - Kranzhoff, S. L.

AU - Kuijer, P.

AU - Kukkadapu, K. A.

AU - Lam, K.

AU - Letendre, N.

AU - Li, P.

AU - Limburg, R.

AU - Linde, F.

AU - Locquet, J. P.

AU - Loosen, P.

AU - Lueck, H.

AU - Martínez, M.

AU - Masserot, A.

AU - Meylahn, F.

AU - Molenaar, M.

AU - Mow-Lowry, C.

AU - Mundet, J.

AU - Munneke, B.

AU - van Nieuwland, L.

AU - Pacaud, E.

AU - Pascucci, D.

AU - Petit, S.

AU - Van Ranst, Z.

AU - Raskin, G.

AU - Recaman, P. M.

AU - van Remortel, N.

AU - Rolland, L.

AU - de Roo, L.

AU - Roose, E.

AU - Rosier, J. C.

AU - Ryckbosch, D.

AU - Schouteden, K.

AU - Sevrin, A.

AU - Sider, A.

AU - Singha, A.

AU - Spagnuolo, V.

AU - Stahl, A.

AU - Steinlechner, J.

AU - Steinlechner, S.

AU - Swinkels, B.

AU - Szilasi, N.

AU - Tacca, M.

AU - Thienpont, H.

AU - Vecchio, A.

AU - Verkooijen, H.

AU - Vermeer, C. H.

AU - Vervaeke, M.

AU - Visser, G.

AU - Walet, R.

AU - Werneke, P.

AU - Westhofen, C.

AU - Willke, B.

AU - Xhahi, A.

AU - Zhang, T.

PY - 2022/11/3

Y1 - 2022/11/3

N2 - The third-generation (3G) of gravitational wave observatories, such as the Einstein Telescope (ET) and Cosmic Explorer, aim for an improvement in sensitivity of at least a factor of ten over a wide frequency range compared to the current advanced detectors. In order to inform the design of the 3G detectors and to develop and qualify their subsystems, dedicated test facilities are required. ETpathfinder prototype uses full interferometer configurations and aims to provide a high sensitivity facility in a similar environment as ET. Along with the interferometry at 1550 nm and silicon test masses, ETpathfinder will focus on cryogenic technologies, lasers and optics at 2090 nm and advanced quantum-noise reduction schemes. This paper analyses the underpinning noise contributions and combines them into full noise budgets of the two initially targeted configurations: (1) operating with 1550 nm laser light and at a temperature of 18 K and (2) operating at 2090 nm wavelength and a temperature of 123 K.

AB - The third-generation (3G) of gravitational wave observatories, such as the Einstein Telescope (ET) and Cosmic Explorer, aim for an improvement in sensitivity of at least a factor of ten over a wide frequency range compared to the current advanced detectors. In order to inform the design of the 3G detectors and to develop and qualify their subsystems, dedicated test facilities are required. ETpathfinder prototype uses full interferometer configurations and aims to provide a high sensitivity facility in a similar environment as ET. Along with the interferometry at 1550 nm and silicon test masses, ETpathfinder will focus on cryogenic technologies, lasers and optics at 2090 nm and advanced quantum-noise reduction schemes. This paper analyses the underpinning noise contributions and combines them into full noise budgets of the two initially targeted configurations: (1) operating with 1550 nm laser light and at a temperature of 18 K and (2) operating at 2090 nm wavelength and a temperature of 123 K.

KW - Cosmic Explorer

KW - ETpathfinder

KW - Einstein Telescope

KW - Voyager

KW - gravitational-wave detectors

KW - third generation of gravitational-wave detectors

UR - https://www.scopus.com/pages/publications/85139189769

U2 - 10.1088/1361-6382/ac8fdb

DO - 10.1088/1361-6382/ac8fdb

M3 - 文章

AN - SCOPUS:85139189769

SN - 0264-9381

VL - 39

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 21

M1 - 215008

ER -

ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors

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