Tilt-to-length coupling in LISA Pathfinder: Long-term stability

M. Armano; H. Audley; J. Baird; P. Binetruy; M. Born; D. Bortoluzzi; E. Castelli; A. Cavalleri; A. Cesarini; A. M. Cruise; K. Danzmann; M. De Deus Silva; I. Diepholz; G. Dixon; R. Dolesi; L. Ferraioli; V. Ferroni; E. D. Fitzsimons; M. Freschi; L. Gesa; D. Giardini; F. Gibert; R. Giusteri; C. Grimani; J. Grzymisch; I. Harrison; M. S. Hartig; G. Heinzel; M. Hewitson; D. Hollington; D. Hoyland; M. Hueller; H. Inchauspé; O. Jennrich; P. Jetzer; U. Johann; B. Johlander; N. Karnesis; B. Kaune; C. J. Killow; N. Korsakova; J. A. Lobo; J. P. López-Zaragoza; R. Maarschalkerweerd; D. Mance; V. Martín; L. Martin-Polo; F. Martin-Porqueras; J. Martino; P. W. McNamara; J. Mendes; L. Mendes; N. Meshksar; M. Nofrarias; S. Paczkowski; M. Perreur-Lloyd; A. Petiteau; E. Plagnol; J. Ramos-Castro; J. Reiche; F. Rivas; D. I. Robertson; G. Russano; J. Sanjuan; J. Slutsky; C. F. Sopuerta; T. Sumner; D. Texier; J. I. Thorpe; D. Vetrugno; S. Vitale; G. Wanner; H. Ward; P. J. Wass; W. J. Weber; L. Wissel; A. Wittchen; P. Zweifel

doi:10.48550/arXiv.2407.05852

Tilt-to-length coupling in LISA Pathfinder: Long-term stability

M. Armano
, H. Audley
, J. Baird
, P. Binetruy
, M. Born
, D. Bortoluzzi
, E. Castelli
, A. Cavalleri
, A. Cesarini
, A. M. Cruise
, K. Danzmann
, M. De Deus Silva
, I. Diepholz
, G. Dixon
, R. Dolesi
, L. Ferraioli
, V. Ferroni
, E. D. Fitzsimons
, M. Freschi
, L. Gesa

D. Giardini, F. Gibert, R. Giusteri, C. Grimani, J. Grzymisch, I. Harrison, M. S. Hartig^*, G. Heinzel, M. Hewitson, D. Hollington, D. Hoyland, M. Hueller, H. Inchauspé, O. Jennrich, P. Jetzer, U. Johann, B. Johlander, N. Karnesis, B. Kaune, C. J. Killow, N. Korsakova, J. A. Lobo, J. P. López-Zaragoza, R. Maarschalkerweerd, D. Mance, V. Martín, L. Martin-Polo, F. Martin-Porqueras, J. Martino, P. W. McNamara, J. Mendes, L. Mendes, N. Meshksar, M. Nofrarias, S. Paczkowski, M. Perreur-Lloyd, A. Petiteau, E. Plagnol, J. Ramos-Castro, J. Reiche, F. Rivas, D. I. Robertson^*, G. Russano, J. Sanjuan, J. Slutsky, C. F. Sopuerta, T. Sumner, D. Texier, J. I. Thorpe, D. Vetrugno, S. Vitale, G. Wanner^*, H. Ward, P. J. Wass, W. J. Weber, L. Wissel, A. Wittchen, P. Zweifel

^*Korrespondierende*r Autor*in für diese Arbeit

Institut für Gravitationsphysik

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

Abstract

The tilt-to-length coupling during the LISA Pathfinder mission has been numerically and analytically modeled for particular time spans. In this work, we investigate the long-term stability of the coupling coefficients of this noise. We show that they drifted slowly (by 1 μm/rad and 6×10-6 in 100 days) and were strongly correlated to temperature changes within the satellite (8 μm/rad/K and 30×10-6/K). Based on analytical tilt-to-length coupling models, we attribute the temperature-driven coupling changes to rotations of the test masses and small distortions in the optical setup. Particularly, our findings lead to the conclusion that LISA Pathfinder's optical baseplate was bent during the cooldown experiment, which started in late 2016 and lasted several months.

Originalsprache	Englisch
Aufsatznummer	063005
Seitenumfang	14
Fachzeitschrift	Physical Review D
Jahrgang	110
Ausgabenummer	6
DOIs	https://doi.org/10.48550/arXiv.2407.05852 https://doi.org/10.1103/PhysRevD.110.063005
Publikationsstatus	Veröffentlicht - 3 Sept. 2024

ASJC Scopus Sachgebiete

Kern- und Hochenergiephysik

Zugriff auf Dokument

10.48550/arXiv.2407.05852Lizenz: CC BY 4.0
10.1103/PhysRevD.110.063005Lizenz: CC BY 4.0

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QuantumFrontiers: Exzellenzcluster 2123/1: Licht und Materie an der Quantengrenze
Schmidt, P. O. (Projektleiter*in (Principal Investigator)), Ospelkaus-Schwarzer, S. (Projektleiter*in (Principal Investigator)), Chichkov, B. (Projektleiter*in (Principal Investigator)), Danzmann, K. (Projektleiter*in (Principal Investigator)), Ertmer, W. (Projektleiter*in (Principal Investigator)), Hammerer, K. J. (Projektleiter*in (Principal Investigator)), Haug, R. (Projektleiter*in (Principal Investigator)), Heinzel, G. (Projektleiter*in (Principal Investigator)), Heurs, M. (Projektleiter*in (Principal Investigator)), Klempt, C. (Projektleiter*in (Principal Investigator)), Kroker, S. (Projektleiter*in (Principal Investigator)), Lisdat, C. (Projektleiter*in (Principal Investigator)), Mehlstäubler, T. (Projektleiter*in (Principal Investigator)), Müller, J. (Projektleiter*in (Principal Investigator)), Ospelkaus, C. (Projektleiter*in (Principal Investigator)), Rasel, E. M. (Projektleiter*in (Principal Investigator)), Recher, P. (Projektleiter*in (Principal Investigator)), Santos, L. S. (Projektleiter*in (Principal Investigator)), Schilling, M. (Projektleiter*in (Principal Investigator)), Schlickum, U. (Projektleiter*in (Principal Investigator)), Schumacher, H. W. (Projektleiter*in (Principal Investigator)), Surzhykov, A. (Projektleiter*in (Principal Investigator)), Waag, A. (Projektleiter*in (Principal Investigator)), Werner, R. (Projektleiter*in (Principal Investigator)) & Willke, B. (Projektleiter*in (Principal Investigator))
1 Jan. 2019 → 31 Dez. 2025
Projekt: Forschung

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Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., De Deus Silva, M., Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Freschi, M., ... Zweifel, P. (2024). Tilt-to-length coupling in LISA Pathfinder: Long-term stability. Physical Review D, 110(6), Artikel 063005. https://doi.org/10.48550/arXiv.2407.05852, https://doi.org/10.1103/PhysRevD.110.063005

@article{9cf30765b57e457ca36f1dcb2911e995,

title = "Tilt-to-length coupling in LISA Pathfinder: Long-term stability",

abstract = "The tilt-to-length coupling during the LISA Pathfinder mission has been numerically and analytically modeled for particular time spans. In this work, we investigate the long-term stability of the coupling coefficients of this noise. We show that they drifted slowly (by 1 μm/rad and 6×10-6 in 100 days) and were strongly correlated to temperature changes within the satellite (8 μm/rad/K and 30×10-6/K). Based on analytical tilt-to-length coupling models, we attribute the temperature-driven coupling changes to rotations of the test masses and small distortions in the optical setup. Particularly, our findings lead to the conclusion that LISA Pathfinder's optical baseplate was bent during the cooldown experiment, which started in late 2016 and lasted several months.",

author = "M. Armano and H. Audley and J. Baird and P. Binetruy and M. Born and D. Bortoluzzi and E. Castelli and A. Cavalleri and A. Cesarini and Cruise, \{A. M.\} and K. Danzmann and \{De Deus Silva\}, M. and I. Diepholz and G. Dixon and R. Dolesi and L. Ferraioli and V. Ferroni and Fitzsimons, \{E. D.\} and M. Freschi and L. Gesa and D. Giardini and F. Gibert and R. Giusteri and C. Grimani and J. Grzymisch and I. Harrison and Hartig, \{M. S.\} and G. Heinzel and M. Hewitson and D. Hollington and D. Hoyland and M. Hueller and H. Inchausp{\'e} and O. Jennrich and P. Jetzer and U. Johann and B. Johlander and N. Karnesis and B. Kaune and Killow, \{C. J.\} and N. Korsakova and Lobo, \{J. A.\} and L{\'o}pez-Zaragoza, \{J. P.\} and R. Maarschalkerweerd and D. Mance and V. Mart{\'i}n and L. Martin-Polo and F. Martin-Porqueras and J. Martino and McNamara, \{P. W.\} and J. Mendes and L. Mendes and N. Meshksar and M. Nofrarias and S. Paczkowski and M. Perreur-Lloyd and A. Petiteau and E. Plagnol and J. Ramos-Castro and J. Reiche and F. Rivas and Robertson, \{D. I.\} and G. Russano and J. Sanjuan and J. Slutsky and Sopuerta, \{C. F.\} and T. Sumner and D. Texier and Thorpe, \{J. I.\} and D. Vetrugno and S. Vitale and G. Wanner and H. Ward and Wass, \{P. J.\} and Weber, \{W. J.\} and L. Wissel and A. Wittchen and P. Zweifel",

note = "Publisher Copyright: {\textcopyright} 2024 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the {"}https://creativecommons.org/licenses/by/4.0/{"}Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Open access publication funded by the Max Planck Society.",

year = "2024",

month = sep,

day = "3",

doi = "10.48550/arXiv.2407.05852",

language = "English",

volume = "110",

journal = "Physical Review D",

issn = "2470-0010",

publisher = "American Physical Society",

number = "6",

}

Armano, M, Audley, H, Baird, J, Binetruy, P, Born, M, Bortoluzzi, D, Castelli, E, Cavalleri, A, Cesarini, A, Cruise, AM, Danzmann, K, De Deus Silva, M, Diepholz, I, Dixon, G, Dolesi, R, Ferraioli, L, Ferroni, V, Fitzsimons, ED, Freschi, M, Gesa, L, Giardini, D, Gibert, F, Giusteri, R, Grimani, C, Grzymisch, J, Harrison, I, Hartig, MS, Heinzel, G, Hewitson, M, Hollington, D, Hoyland, D, Hueller, M, Inchauspé, H, Jennrich, O, Jetzer, P, Johann, U, Johlander, B, Karnesis, N, Kaune, B, Killow, CJ, Korsakova, N, Lobo, JA, López-Zaragoza, JP, Maarschalkerweerd, R, Mance, D, Martín, V, Martin-Polo, L, Martin-Porqueras, F, Martino, J, McNamara, PW, Mendes, J, Mendes, L, Meshksar, N, Nofrarias, M, Paczkowski, S, Perreur-Lloyd, M, Petiteau, A, Plagnol, E, Ramos-Castro, J, Reiche, J, Rivas, F, Robertson, DI, Russano, G, Sanjuan, J, Slutsky, J, Sopuerta, CF, Sumner, T, Texier, D, Thorpe, JI, Vetrugno, D, Vitale, S, Wanner, G, Ward, H, Wass, PJ, Weber, WJ, Wissel, L, Wittchen, A & Zweifel, P 2024, 'Tilt-to-length coupling in LISA Pathfinder: Long-term stability', Physical Review D, Jg. 110, Nr. 6, 063005. https://doi.org/10.48550/arXiv.2407.05852, https://doi.org/10.1103/PhysRevD.110.063005

TY - JOUR

T1 - Tilt-to-length coupling in LISA Pathfinder

T2 - Long-term stability

AU - Armano, M.

AU - Audley, H.

AU - Baird, J.

AU - Binetruy, P.

AU - Born, M.

AU - Bortoluzzi, D.

AU - Castelli, E.

AU - Cavalleri, A.

AU - Cesarini, A.

AU - Cruise, A. M.

AU - Danzmann, K.

AU - De Deus Silva, M.

AU - Diepholz, I.

AU - Dixon, G.

AU - Dolesi, R.

AU - Ferraioli, L.

AU - Ferroni, V.

AU - Fitzsimons, E. D.

AU - Freschi, M.

AU - Gesa, L.

AU - Giardini, D.

AU - Gibert, F.

AU - Giusteri, R.

AU - Grimani, C.

AU - Grzymisch, J.

AU - Harrison, I.

AU - Hartig, M. S.

AU - Heinzel, G.

AU - Hewitson, M.

AU - Hollington, D.

AU - Hoyland, D.

AU - Hueller, M.

AU - Inchauspé, H.

AU - Jennrich, O.

AU - Jetzer, P.

AU - Johann, U.

AU - Johlander, B.

AU - Karnesis, N.

AU - Kaune, B.

AU - Killow, C. J.

AU - Korsakova, N.

AU - Lobo, J. A.

AU - López-Zaragoza, J. P.

AU - Maarschalkerweerd, R.

AU - Mance, D.

AU - Martín, V.

AU - Martin-Polo, L.

AU - Martin-Porqueras, F.

AU - Martino, J.

AU - McNamara, P. W.

AU - Mendes, J.

AU - Mendes, L.

AU - Meshksar, N.

AU - Nofrarias, M.

AU - Paczkowski, S.

AU - Perreur-Lloyd, M.

AU - Petiteau, A.

AU - Plagnol, E.

AU - Ramos-Castro, J.

AU - Reiche, J.

AU - Rivas, F.

AU - Robertson, D. I.

AU - Russano, G.

AU - Sanjuan, J.

AU - Slutsky, J.

AU - Sopuerta, C. F.

AU - Sumner, T.

AU - Texier, D.

AU - Thorpe, J. I.

AU - Vetrugno, D.

AU - Vitale, S.

AU - Wanner, G.

AU - Ward, H.

AU - Wass, P. J.

AU - Weber, W. J.

AU - Wissel, L.

AU - Wittchen, A.

AU - Zweifel, P.

N1 - Publisher Copyright: © 2024 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/"Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Open access publication funded by the Max Planck Society.

PY - 2024/9/3

Y1 - 2024/9/3

N2 - The tilt-to-length coupling during the LISA Pathfinder mission has been numerically and analytically modeled for particular time spans. In this work, we investigate the long-term stability of the coupling coefficients of this noise. We show that they drifted slowly (by 1 μm/rad and 6×10-6 in 100 days) and were strongly correlated to temperature changes within the satellite (8 μm/rad/K and 30×10-6/K). Based on analytical tilt-to-length coupling models, we attribute the temperature-driven coupling changes to rotations of the test masses and small distortions in the optical setup. Particularly, our findings lead to the conclusion that LISA Pathfinder's optical baseplate was bent during the cooldown experiment, which started in late 2016 and lasted several months.

AB - The tilt-to-length coupling during the LISA Pathfinder mission has been numerically and analytically modeled for particular time spans. In this work, we investigate the long-term stability of the coupling coefficients of this noise. We show that they drifted slowly (by 1 μm/rad and 6×10-6 in 100 days) and were strongly correlated to temperature changes within the satellite (8 μm/rad/K and 30×10-6/K). Based on analytical tilt-to-length coupling models, we attribute the temperature-driven coupling changes to rotations of the test masses and small distortions in the optical setup. Particularly, our findings lead to the conclusion that LISA Pathfinder's optical baseplate was bent during the cooldown experiment, which started in late 2016 and lasted several months.

UR - https://www.scopus.com/pages/publications/85203598585

U2 - 10.48550/arXiv.2407.05852

DO - 10.48550/arXiv.2407.05852

M3 - Article

AN - SCOPUS:85203598585

SN - 2470-0010

VL - 110

JO - Physical Review D

JF - Physical Review D

IS - 6

M1 - 063005

ER -

Tilt-to-length coupling in LISA Pathfinder: Long-term stability

Abstract

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