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Calibrating the system dynamics of LISA Pathfinder

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Title: Calibrating the system dynamics of LISA Pathfinder
Authors: 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
Gibert, F
Giardini, D
Giusteri, R
Grimani, C
Grzymisch, J
Harrison, I
Heinzel, G
Hewitson, M
Hollington, D
Hoyland, D
Hueller, M
Inchauspe, H
Jennrich, O
Jetzer, P
Karnesis, N
Kaune, B
Korsakova, N
Killow, CJ
Lobo, JA
Lloro, I
Liu, L
Lopez-Zaragoza, JP
Maarschalkerweerd, R
Mance, D
Meshksar, N
Martin, V
Martin-Polo, L
Martino, J
Martin-Porqueras, F
Mateos, I
McNamara, PW
Mendes, J
Mendes, L
Nofrarias, M
Paczkowski, S
Perreur-Lloyd, M
Petiteau, A
Pivato, P
Plagnol, E
Ramos-Castro, J
Reiche, J
Robertson, D
Rivas, F
Russano, G
Slutsky, J
Sopuerta, CF
Sumner, T
Texier, D
Thorpe, J
Vetrugno, D
Vitale, S
Wanner, G
Ward, H
Wass, P
Weber, WJ
Wissel, L
Wittchen, A
Zweifel, P
Item Type: Journal Article
Abstract: LISA Pathfinder (LPF) was a European Space Agency mission with the aim to test key technologies for future space-borne gravitational-wave observatories like LISA. The main scientific goal of LPF was to demonstrate measurements of differential acceleration between free-falling test masses at the sub-femto-g level, and to understand the residual acceleration in terms of a physical model of stray forces, and displacement readout noise. A key step toward reaching the LPF goals was the correct calibration of the dynamics of LPF, which was a three-body system composed by two test-masses enclosed in a single spacecraft, and subject to control laws for system stability. In this work, we report on the calibration procedures adopted to calculate the residual differential stray force per unit mass acting on the two test-masses in their nominal positions. The physical parameters of the adopted dynamical model are presented, together with their role on LPF performance. The analysis and results of these experiments show that the dynamics of the system was accurately modeled and the dynamical parameters were stationary throughout the mission. Finally, the impact and importance of calibrating system dynamics for future space-based gravitational wave observatories is discussed.
Issue Date: 15-Jun-2018
Date of Acceptance: 26-Apr-2018
URI: http://hdl.handle.net/10044/1/61649
DOI: https://dx.doi.org/10.1103/PhysRevD.97.122002
ISSN: 2470-0010
Publisher: American Physical Society
Journal / Book Title: Physical Review D
Volume: 97
Issue: 12
Copyright Statement: © 2018 American Physical Society.
Keywords: Science & Technology
Physical Sciences
Astronomy & Astrophysics
Physics, Particles & Fields
Physics
INTERFEROMETRY
MISSION
Publication Status: Published
Article Number: 122002
Online Publication Date: 2018-06-12
Appears in Collections:Physics
High Energy Physics



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