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. ColletteS. 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

(Astro)-Particles Physics

Research output: Contribution to Journal › Article › Academic › peer-review

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.

Original language	English
Article number	215008
Pages (from-to)	1-24
Number of pages	24
Journal	Classical and Quantum Gravity
Volume	39
Issue number	21
Early online date	26 Sept 2022
DOIs	https://doi.org/10.1088/1361-6382/ac8fdb
Publication status	Published - 3 Nov 2022

Bibliographical note

Funding

ETpathfinder is a cryogenic research and development laboratory with team members from twenty research institutions and is funded by a consortium of financial partners 21

Funders	Funder number
Flamish Government
Ministerie van Economische Zaken
Ministerie van Onderwijs, Cultuur en Wetenschap
Interreg Vlaanderen-Nederland

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

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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), 1-24. Article 215008. https://doi.org/10.1088/1361-6382/ac8fdb

@article{ddc33804f56e433ca62d5f07b271b260,

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.",

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 H.J. Bulten 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 J.-S. Hennig and M. Hennig and T. Hertog and S. Hild and H.-D. Hoffmann and G. Hoft and M. Hopman and D. Hoyland and G.A. Iandolo 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 A.N. Koushik and M. Kraan and {van de Kraats}, M. and S.L. Kranzhoff and P. Kuijer and K.A. Kukkadapu and K. Lam and N. Letendre and P. Li and R. Limburg and F. Linde and J.-P. Locquet 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 P.M. Recaman and {van Remortel}, N. and L. Rolland and {de Roo}, L. and E. Roose and J.C. Rosier 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 C.H. Vermeer 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 = "{\textcopyright} 2022 The Author(s). Published by IOP Publishing Ltd",

year = "2022",

month = nov,

day = "3",

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

language = "English",

volume = "39",

pages = "1--24",

journal = "Classical and Quantum Gravity",

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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, 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, J-S, Hennig, M, Hertog, T, Hild, S, Hoffmann, H-D, 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, J-P, 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, vol. 39, no. 21, 215008, pp. 1-24. https://doi.org/10.1088/1361-6382/ac8fdb

TY - JOUR

T1 - ETpathfinder: 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.

UR - http://www.scopus.com/inward/record.url?scp=85139189769&partnerID=8YFLogxK

U2 - 10.1088/1361-6382/ac8fdb

DO - 10.1088/1361-6382/ac8fdb

M3 - Article

SN - 0264-9381

VL - 39

SP - 1

EP - 24

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 21

M1 - 215008

ER -

ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors

Abstract

Bibliographical note

Funding

UN SDGs

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