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Optimal design of calibration signals in space-borne gravitational wave detectors

Authors :
Miquel Nofrarias
Nikolaos Karnesis
Ferran Gibert
Michele Armano
Heather Audley
Karsten Danzmann
Ingo Diepholz
Rita Dolesi
Luigi Ferraioli
Valerio Ferroni
Martin Hewitson
Mauro Hueller
Henri Inchauspe
Oliver Jennrich
Natalia Korsakova
Paul W. McNamara
Eric Plagnol
James I. Thorpe
Daniele Vetrugno
Stefano Vitale
Peter Wass
William J. Weber
AstroParticule et Cosmologie (APC (UMR_7164))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
AstroParticule et Cosmologie ( APC - UMR 7164 )
Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA )
Source :
Physical Review D, Physical Review D, American Physical Society, 2016, 93 (10), pp.102004. ⟨10.1103/PhysRevD.93.102004⟩, Phys.Rev.D, Phys.Rev.D, 2016, 93 (10), pp.102004. ⟨10.1103/PhysRevD.93.102004⟩, Phys.Rev.D, 2016, 93 (10), pp.102004. 〈10.1103/PhysRevD.93.102004〉
Publication Year :
2016
Publisher :
American Physical Society (APS), 2016.

Abstract

Future space borne gravitational wave detectors will require a precise definition of calibration signals to ensure the achievement of their design sensitivity. The careful design of the test signals plays a key role in the correct understanding and characterisation of these instruments. In that sense, methods achieving optimal experiment designs must be considered as complementary to the parameter estimation methods being used to determine the parameters describing the system. The relevance of experiment design is particularly significant for the LISA Pathfinder mission, which will spend most of its operation time performing experiments to characterise key technologies for future space borne gravitational wave observatories. Here we propose a framework to derive the optimal signals ---in terms of minimum parameter uncertainty--- to be injected to these instruments during its calibration phase. We compare our results with an alternative numerical algorithm which achieves an optimal input signal by iteratively improving an initial guess. We show agreement of both approaches when applied to the LISA Pathfinder case.<br />12 pages, 6 figures

Details

ISSN :
24700029, 24700010, 15507998, and 15502368
Volume :
93
Database :
OpenAIRE
Journal :
Physical Review D
Accession number :
edsair.doi.dedup.....26057b217c52848e2a3ff49e7039dcc3
Full Text :
https://doi.org/10.1103/physrevd.93.102004