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The LISA Pathfinder Mission

Authors :
Ivan Lloro
G. Russano
Gerhard Heinzel
C. García Marirrodriga
J. Reiche
Matteo Benedetti
S. Madden
J. Bogenstahl
Víctor S. Martín
M. Caleno
H. B. Tu
P. Prat
Peter Zweifel
M. Hueller
Ph. Jetzer
E. Mitchell
N. Dumbar
Heather Audley
D. Wealthy
José F. F. Mendes
X. Llamas
H. Ward
J. A. Romera Perez
M. Cruise
C. Trenkel
Stefano Vitale
A. Grynagier
Ignacio Mateos
Karsten Danzmann
Eric Plagnol
M. Diaz-Aguilo
Oliver Jennrich
Daniele Bortoluzzi
W. J. Weber
Paul McNamara
T. J. Sumner
Christian J. Killow
Domenico Giardini
Martin Hewitson
A. Lobo
Walter Fichter
Daniel Hollington
Valerio Ferroni
G. Dixton
Carlos F. Sopuerta
Miquel Nofrarías
Antonella Cavalleri
Felipe Guzman
D. Hoyland
Davor Mance
David Robertson
G. Congedo
Luigi Ferraioli
N. Korsakova
Michael Perreur-Lloyd
Ewan Fitzsimons
Ingo Diepholz
Alexander Schleicher
D. Texier
N. Brandt
A.M. Taylor
F. De Marchi
Rita Dolesi
Daniele Nicolodi
Gudrun Wanner
Juan Ramos-Castro
Ferran Gibert
R. Gerndt
Tobias Ziegler
Michele Armano
F. Antonucci
M. Freschi
Catia Grimani
S. Wen
J. Huesler
B. Johlander
Ian Harrison
S. Waschke
Peter Wass
N. Karnesis
Pierre Binétruy
Lluis Gesa
G. Auger
R. Maarschalkerweerd
H. Rozemeijer
D. Shaul
J. Fauste
Source :
ASP Conference Series Volumes, ResearcherID, INSPIRE-HEP, Web of Science
Publication Year :
2013

Abstract

LISA Pathfinder (formerly known as SMART-2) is an European Space Agency mission designed to pave the way for the joint ESA/NASA Laser Interferometer Space Antenna (LISA) mission by testing in flight the critical technologies required for space-borne gravitational wave detection; it will put two test masses in a near-perfect gravitational free-fall and control and measure their motion with unprecedented accuracy. This is achieved through technology comprising inertial sensors, high precision laser metrology, drag-free control, and an ultra precise micro-Newton propulsion system. LISA Pathfinder (LPF) essentially mimics one arm of spaceborne gravitational wave detectors by shrinking the million kilometre scale armlengths down to a few tens of centimetres, giving up the sensitivity to gravitational waves, but keeping the measurement technology. The scientific objective of the LISA Pathfinder mission consists then of the first in-flight test of low frequency gravitational wave detection metrology. In this paper I will give a brief overview of the mission, focusing on scientific and technical goals.

Details

Database :
OpenAIRE
Journal :
ASP Conference Series Volumes, ResearcherID, INSPIRE-HEP, Web of Science
Accession number :
edsair.doi.dedup.....1a2a28ed8089fd46392ee9fe6309c36c